Binary_c parameters

The following chapter contains all the parameters that the current version of binary_c can handle, along with their descriptions and other properties.

This information was obtained by the following binary_c build:: binary_c git branch: master binary_c git revision: 6209:20211006:c4a4c332e Built on: Oct 6 2021 08:31:27

Section: stars

Parameter: metallicity
Description: This sets the metallicity of the stars, i.e. the amount (by mass) of matter which is not hydrogen or helium. If you are using the BSE algorithm, this must be 1e-4 <= metallicity <= 0.03. See also nucsyn_metallicity and effective_metallicity.
Parameter input type: Float
Default value: 0.02

Parameter: effective_metallicity
Description: This sets effective metallicity of stars as used in routines like the Schneider wind loss. If not set, or set to DEFAULT_TO_METALLICITY (==-1, the default), this is just the same as metallicity. The main difference between effective_metallicity and metallicity is the range of validity: 0 <= effective_metallicity <= 1, while metallicity’s range of validity is limited by the stellar evolution algorithm (so, for BSE, is 1e-4 <= metallicity <= 0.03).
Parameter input type: Float
Default value: -1
Macros: [‘DEFAULT_TO_METALLICITY = -1’]

Parameter: M_1
Description: The initial mass of star one (in solar units, internally this is star index 0).
Parameter input type: Float
Default value: 0

Parameter: M_2
Description: The initial mass of star two (in solar units, internally this is star index 1).
Parameter input type: Float
Default value: 0

Parameter: M_3
Description: The initial mass of star three (in solar units, internally this is star index 2).
Parameter input type: Float
Default value: 0

Parameter: M_4
Description: The initial mass of star four (in solar units, internally this is star index 3).
Parameter input type: Float
Default value: 0

Parameter: vrot1
Description: The initial equatorial rotational velocity of star one (in km/s, internally this is star index 0). If 0.0, the Hurley et al 2000/2002 prescription is used to set the main-sequence velocity, so for a truly non-rotating star, set to something small (e.g. 0.001). See also vrot2,3,4.
Parameter input type: Float
Default value: 0
Macros: [‘VROT_BSE = 0’, ‘VROT_BREAKUP = -1’, ‘VROT_SYNC = -2’, ‘VROT_NON_ROTATING = -3’]

Parameter: vrot2
Description: The initial equatorial rotational velocity of star two (in km/s, internally this is star index 1). If 0.0, the Hurley et al 2000/2002 prescription is used to set the main-sequence velocity, so for a truly non-rotating star, set to something small (e.g. 0.001). See also vrot1,3,4.
Parameter input type: Float
Default value: 0
Macros: [‘VROT_BSE = 0’, ‘VROT_BREAKUP = -1’, ‘VROT_SYNC = -2’, ‘VROT_NON_ROTATING = -3’]

Parameter: vrot3
Description: The initial equatorial rotational velocity of star three (in km/s, internally this is star index 2). If 0.0, the Hurley et al 2000/2002 prescription is used to set the main-sequence velocity, so for a truly non-rotating star, set to something small (e.g. 0.001). See also vrot1,2,4.
Parameter input type: Float
Default value: 0
Macros: [‘VROT_BSE = 0’, ‘VROT_BREAKUP = -1’, ‘VROT_SYNC = -2’, ‘VROT_NON_ROTATING = -3’]

Parameter: vrot4
Description: The initial equatorial rotational velocity of star four (in km/s, internally this is star index 3). If 0.0, the Hurley et al 2000/2002 prescription is used to set the main-sequence velocity, so for a truly non-rotating star, set to something small (e.g. 0.001). See also vrot1,2,3.
Parameter input type: Float
Default value: 0
Macros: [‘VROT_BSE = 0’, ‘VROT_BREAKUP = -1’, ‘VROT_SYNC = -2’, ‘VROT_NON_ROTATING = -3’]

Parameter: Prot1
Description: The initial equatorial rotational velocity of star one (in km/s, internally this is star index 0). See also Prot2,3,4.
Parameter input type: Float
Default value: 0

Parameter: Prot2
Description: The initial equatorial rotational velocity of star two (in km/s, internally this is star index 1). See also Prot1,3,4.
Parameter input type: Float
Default value: 0

Parameter: Prot3
Description: The initial equatorial rotational period of star three (in days, internally this is star index 2). See also Prot1,2,4.
Parameter input type: Float
Default value: 0

Parameter: Prot4
Description: The initial equatorial rotational period of star four (in days, internally this is star index 3). See also Prot1,2,3.
Parameter input type: Float
Default value: 0

Parameter: inclination1
Description: The initial inclination of star one (in degrees).
Parameter input type: Float
Default value: 0

Parameter: inclination2
Description: The initial inclination of star two (in degrees).
Parameter input type: Float
Default value: 0

Parameter: inclination3
Description: The initial inclination of star three (in degrees).
Parameter input type: Float
Default value: 0

Parameter: inclination4
Description: The initial inclination of star four (in degrees).
Parameter input type: Float
Default value: 0

Parameter: B_1
Description: The initial magnetic field of star one (in Gauss, internally this is star index 0).
Parameter input type: Float
Default value: 0

Parameter: B_2
Description: The initial magnetic field of star two (in Gauss, internally this is star index 1).
Parameter input type: Float
Default value: 0

Parameter: B_3
Description: The initial magnetic field of star three (in Gauss, internally this is star index 2).
Parameter input type: Float
Default value: 0

Parameter: B_4
Description: The initial magnetic field of star four (in Gauss, internally this is star index 3).
Parameter input type: Float
Default value: 0

Parameter: B_inclination1
Description: The initial inclination of the magnetic field of star one (in degrees).
Parameter input type: Float
Default value: 0

Parameter: B_inclination2
Description: The initial inclination of the magnetic field of star two (in degrees).
Parameter input type: Float
Default value: 0

Parameter: B_inclination3
Description: The initial inclination of the magnetic field of star three (in degrees).
Parameter input type: Float
Default value: 0

Parameter: B_inclination4
Description: The initial inclination of the magnetic field of star four (in degrees).
Parameter input type: Float
Default value: 0

Parameter: stellar_type_1
Description: Set the stellar type of star 1 (internal index 0), usually MAIN_SEQUENCE (main sequence). Note that setting the stellar type only works for stars with both age=0 and core_mass=0, i.e. main sequence (hydrogen or helium), white dwarfs, black holes and neutrn stars.
Parameter input type: Integer
Default value: 0
Macros: [‘LOW_MASS_MS = 0’, ‘MS = 1’, ‘HG = 2’, ‘GIANT_BRANCH = 3’, ‘CHeB = 4’, ‘EAGB = 5’, ‘TPAGB = 6’, ‘HeMS = 7’, ‘HeHG = 8’, ‘HeGB = 9’, ‘HeWD = 10’, ‘COWD = 11’, ‘ONeWD = 12’, ‘NS = 13’, ‘BH = 14’, ‘MASSLESS_REMNANT = 15’, ‘LOW_MASS_MAIN_SEQUENCE = 0’, ‘MAIN_SEQUENCE = 1’, ‘HERTZSPRUNG_GAP = 2’, ‘FIRST_GIANT_BRANCH = 3’, ‘CORE_HELIUM_BURNING = 4’, ‘EARLY_ASYMPTOTIC_GIANT_BRANCH = 5’, ‘THERMALLY_PULSING_ASYMPTOTIC_GIANT_BRANCH = 6’, ‘NAKED_MAIN_SEQUENCE_HELIUM_STAR = 7’, ‘NAKED_HELIUM_STAR_HERTZSPRUNG_GAP = 8’, ‘NAKED_HELIUM_STAR_GIANT_BRANCH = 9’, ‘HELIUM_WHITE_DWARF = 10’, ‘CARBON_OXYGEN_WHITE_DWARF = 11’, ‘OXYGEN_NEON_WHITE_DWARF = 12’, ‘NEUTRON_STAR = 13’, ‘BLACK_HOLE = 14’, ‘STAR_WITH_NO_MASS = 15’]

Parameter: stellar_type_2
Description: Set the stellar type of star 2 (internal index 1), usually MAIN_SEQUENCE (main sequence). Note that setting the stellar type only works for stars with both age=0 and core_mass=0, i.e. main sequence (hydrogen or helium), white dwarfs, black holes and neutrn stars.
Parameter input type: Integer
Default value: 0
Macros: [‘LOW_MASS_MS = 0’, ‘MS = 1’, ‘HG = 2’, ‘GIANT_BRANCH = 3’, ‘CHeB = 4’, ‘EAGB = 5’, ‘TPAGB = 6’, ‘HeMS = 7’, ‘HeHG = 8’, ‘HeGB = 9’, ‘HeWD = 10’, ‘COWD = 11’, ‘ONeWD = 12’, ‘NS = 13’, ‘BH = 14’, ‘MASSLESS_REMNANT = 15’, ‘LOW_MASS_MAIN_SEQUENCE = 0’, ‘MAIN_SEQUENCE = 1’, ‘HERTZSPRUNG_GAP = 2’, ‘FIRST_GIANT_BRANCH = 3’, ‘CORE_HELIUM_BURNING = 4’, ‘EARLY_ASYMPTOTIC_GIANT_BRANCH = 5’, ‘THERMALLY_PULSING_ASYMPTOTIC_GIANT_BRANCH = 6’, ‘NAKED_MAIN_SEQUENCE_HELIUM_STAR = 7’, ‘NAKED_HELIUM_STAR_HERTZSPRUNG_GAP = 8’, ‘NAKED_HELIUM_STAR_GIANT_BRANCH = 9’, ‘HELIUM_WHITE_DWARF = 10’, ‘CARBON_OXYGEN_WHITE_DWARF = 11’, ‘OXYGEN_NEON_WHITE_DWARF = 12’, ‘NEUTRON_STAR = 13’, ‘BLACK_HOLE = 14’, ‘STAR_WITH_NO_MASS = 15’]

Parameter: stellar_type_3
Description: Set the stellar type of star 3 (internal index 2), usually MAIN_SEQUENCE (main sequence). Note that setting the stellar type only works for stars with both age=0 and core_mass=0, i.e. main sequence (hydrogen or helium), white dwarfs, black holes and neutrn stars.
Parameter input type: Integer
Default value: 0
Macros: [‘LOW_MASS_MS = 0’, ‘MS = 1’, ‘HG = 2’, ‘GIANT_BRANCH = 3’, ‘CHeB = 4’, ‘EAGB = 5’, ‘TPAGB = 6’, ‘HeMS = 7’, ‘HeHG = 8’, ‘HeGB = 9’, ‘HeWD = 10’, ‘COWD = 11’, ‘ONeWD = 12’, ‘NS = 13’, ‘BH = 14’, ‘MASSLESS_REMNANT = 15’, ‘LOW_MASS_MAIN_SEQUENCE = 0’, ‘MAIN_SEQUENCE = 1’, ‘HERTZSPRUNG_GAP = 2’, ‘FIRST_GIANT_BRANCH = 3’, ‘CORE_HELIUM_BURNING = 4’, ‘EARLY_ASYMPTOTIC_GIANT_BRANCH = 5’, ‘THERMALLY_PULSING_ASYMPTOTIC_GIANT_BRANCH = 6’, ‘NAKED_MAIN_SEQUENCE_HELIUM_STAR = 7’, ‘NAKED_HELIUM_STAR_HERTZSPRUNG_GAP = 8’, ‘NAKED_HELIUM_STAR_GIANT_BRANCH = 9’, ‘HELIUM_WHITE_DWARF = 10’, ‘CARBON_OXYGEN_WHITE_DWARF = 11’, ‘OXYGEN_NEON_WHITE_DWARF = 12’, ‘NEUTRON_STAR = 13’, ‘BLACK_HOLE = 14’, ‘STAR_WITH_NO_MASS = 15’]

Parameter: stellar_type_4
Description: Set the stellar type of star 4 (internal index 3), usually MAIN_SEQUENCE (main sequence). Note that setting the stellar type only works for stars with both age=0 and core_mass=0, i.e. main sequence (hydrogen or helium), white dwarfs, black holes and neutrn stars.
Parameter input type: Integer
Default value: 0
Macros: [‘LOW_MASS_MS = 0’, ‘MS = 1’, ‘HG = 2’, ‘GIANT_BRANCH = 3’, ‘CHeB = 4’, ‘EAGB = 5’, ‘TPAGB = 6’, ‘HeMS = 7’, ‘HeHG = 8’, ‘HeGB = 9’, ‘HeWD = 10’, ‘COWD = 11’, ‘ONeWD = 12’, ‘NS = 13’, ‘BH = 14’, ‘MASSLESS_REMNANT = 15’, ‘LOW_MASS_MAIN_SEQUENCE = 0’, ‘MAIN_SEQUENCE = 1’, ‘HERTZSPRUNG_GAP = 2’, ‘FIRST_GIANT_BRANCH = 3’, ‘CORE_HELIUM_BURNING = 4’, ‘EARLY_ASYMPTOTIC_GIANT_BRANCH = 5’, ‘THERMALLY_PULSING_ASYMPTOTIC_GIANT_BRANCH = 6’, ‘NAKED_MAIN_SEQUENCE_HELIUM_STAR = 7’, ‘NAKED_HELIUM_STAR_HERTZSPRUNG_GAP = 8’, ‘NAKED_HELIUM_STAR_GIANT_BRANCH = 9’, ‘HELIUM_WHITE_DWARF = 10’, ‘CARBON_OXYGEN_WHITE_DWARF = 11’, ‘OXYGEN_NEON_WHITE_DWARF = 12’, ‘NEUTRON_STAR = 13’, ‘BLACK_HOLE = 14’, ‘STAR_WITH_NO_MASS = 15’]

Parameter: max_stellar_type_1
Description: The maximum stellar type of star 1 (internal index 0). Evolution is stopped when the star reaches this stellar type. If this is negative, massless remnants are allowed, and the maximum stellar type is the absolute value.
Parameter input type: Integer
Default value: 16
Macros: [‘LOW_MASS_MS = 0’, ‘MS = 1’, ‘HG = 2’, ‘GIANT_BRANCH = 3’, ‘CHeB = 4’, ‘EAGB = 5’, ‘TPAGB = 6’, ‘HeMS = 7’, ‘HeHG = 8’, ‘HeGB = 9’, ‘HeWD = 10’, ‘COWD = 11’, ‘ONeWD = 12’, ‘NS = 13’, ‘BH = 14’, ‘MASSLESS_REMNANT = 15’, ‘LOW_MASS_MAIN_SEQUENCE = 0’, ‘MAIN_SEQUENCE = 1’, ‘HERTZSPRUNG_GAP = 2’, ‘FIRST_GIANT_BRANCH = 3’, ‘CORE_HELIUM_BURNING = 4’, ‘EARLY_ASYMPTOTIC_GIANT_BRANCH = 5’, ‘THERMALLY_PULSING_ASYMPTOTIC_GIANT_BRANCH = 6’, ‘NAKED_MAIN_SEQUENCE_HELIUM_STAR = 7’, ‘NAKED_HELIUM_STAR_HERTZSPRUNG_GAP = 8’, ‘NAKED_HELIUM_STAR_GIANT_BRANCH = 9’, ‘HELIUM_WHITE_DWARF = 10’, ‘CARBON_OXYGEN_WHITE_DWARF = 11’, ‘OXYGEN_NEON_WHITE_DWARF = 12’, ‘NEUTRON_STAR = 13’, ‘BLACK_HOLE = 14’, ‘STAR_WITH_NO_MASS = 15’]

Parameter: max_stellar_type_2
Description: The maximum stellar type of star 2 (internal index 1). Evolution is stopped when the star reaches this stellar type. If this is negative, massless remnants are allowed, and the maximum stellar type is the absolute value.
Parameter input type: Integer
Default value: 16
Macros: [‘LOW_MASS_MS = 0’, ‘MS = 1’, ‘HG = 2’, ‘GIANT_BRANCH = 3’, ‘CHeB = 4’, ‘EAGB = 5’, ‘TPAGB = 6’, ‘HeMS = 7’, ‘HeHG = 8’, ‘HeGB = 9’, ‘HeWD = 10’, ‘COWD = 11’, ‘ONeWD = 12’, ‘NS = 13’, ‘BH = 14’, ‘MASSLESS_REMNANT = 15’, ‘LOW_MASS_MAIN_SEQUENCE = 0’, ‘MAIN_SEQUENCE = 1’, ‘HERTZSPRUNG_GAP = 2’, ‘FIRST_GIANT_BRANCH = 3’, ‘CORE_HELIUM_BURNING = 4’, ‘EARLY_ASYMPTOTIC_GIANT_BRANCH = 5’, ‘THERMALLY_PULSING_ASYMPTOTIC_GIANT_BRANCH = 6’, ‘NAKED_MAIN_SEQUENCE_HELIUM_STAR = 7’, ‘NAKED_HELIUM_STAR_HERTZSPRUNG_GAP = 8’, ‘NAKED_HELIUM_STAR_GIANT_BRANCH = 9’, ‘HELIUM_WHITE_DWARF = 10’, ‘CARBON_OXYGEN_WHITE_DWARF = 11’, ‘OXYGEN_NEON_WHITE_DWARF = 12’, ‘NEUTRON_STAR = 13’, ‘BLACK_HOLE = 14’, ‘STAR_WITH_NO_MASS = 15’]

Parameter: max_stellar_type_3
Description: The maximum stellar type of star 3 (internal index 2). Evolution is stopped when the star reaches this stellar type. If this is negative, massless remnants are allowed, and the maximum stellar type is the absolute value.
Parameter input type: Integer
Default value: 16
Macros: [‘LOW_MASS_MS = 0’, ‘MS = 1’, ‘HG = 2’, ‘GIANT_BRANCH = 3’, ‘CHeB = 4’, ‘EAGB = 5’, ‘TPAGB = 6’, ‘HeMS = 7’, ‘HeHG = 8’, ‘HeGB = 9’, ‘HeWD = 10’, ‘COWD = 11’, ‘ONeWD = 12’, ‘NS = 13’, ‘BH = 14’, ‘MASSLESS_REMNANT = 15’, ‘LOW_MASS_MAIN_SEQUENCE = 0’, ‘MAIN_SEQUENCE = 1’, ‘HERTZSPRUNG_GAP = 2’, ‘FIRST_GIANT_BRANCH = 3’, ‘CORE_HELIUM_BURNING = 4’, ‘EARLY_ASYMPTOTIC_GIANT_BRANCH = 5’, ‘THERMALLY_PULSING_ASYMPTOTIC_GIANT_BRANCH = 6’, ‘NAKED_MAIN_SEQUENCE_HELIUM_STAR = 7’, ‘NAKED_HELIUM_STAR_HERTZSPRUNG_GAP = 8’, ‘NAKED_HELIUM_STAR_GIANT_BRANCH = 9’, ‘HELIUM_WHITE_DWARF = 10’, ‘CARBON_OXYGEN_WHITE_DWARF = 11’, ‘OXYGEN_NEON_WHITE_DWARF = 12’, ‘NEUTRON_STAR = 13’, ‘BLACK_HOLE = 14’, ‘STAR_WITH_NO_MASS = 15’]

Parameter: max_stellar_type_4
Description: The maximum stellar type of star 4 (internal index 3). Evolution is stopped when the star reaches this stellar type. If this is negative, massless remnants are allowed, and the maximum stellar type is the absolute value.
Parameter input type: Integer
Default value: 16
Macros: [‘LOW_MASS_MS = 0’, ‘MS = 1’, ‘HG = 2’, ‘GIANT_BRANCH = 3’, ‘CHeB = 4’, ‘EAGB = 5’, ‘TPAGB = 6’, ‘HeMS = 7’, ‘HeHG = 8’, ‘HeGB = 9’, ‘HeWD = 10’, ‘COWD = 11’, ‘ONeWD = 12’, ‘NS = 13’, ‘BH = 14’, ‘MASSLESS_REMNANT = 15’, ‘LOW_MASS_MAIN_SEQUENCE = 0’, ‘MAIN_SEQUENCE = 1’, ‘HERTZSPRUNG_GAP = 2’, ‘FIRST_GIANT_BRANCH = 3’, ‘CORE_HELIUM_BURNING = 4’, ‘EARLY_ASYMPTOTIC_GIANT_BRANCH = 5’, ‘THERMALLY_PULSING_ASYMPTOTIC_GIANT_BRANCH = 6’, ‘NAKED_MAIN_SEQUENCE_HELIUM_STAR = 7’, ‘NAKED_HELIUM_STAR_HERTZSPRUNG_GAP = 8’, ‘NAKED_HELIUM_STAR_GIANT_BRANCH = 9’, ‘HELIUM_WHITE_DWARF = 10’, ‘CARBON_OXYGEN_WHITE_DWARF = 11’, ‘OXYGEN_NEON_WHITE_DWARF = 12’, ‘NEUTRON_STAR = 13’, ‘BLACK_HOLE = 14’, ‘STAR_WITH_NO_MASS = 15’]

Parameter: probability
Description: The probability is a weighting applied to the star based on, say, the initial mass function. When running a grid of stars to simulate all stars, the summed probability of all the stars should be 1.0.
Parameter input type: Float
Default value: 1

Parameter: phasevol
Description: The system’s phase volume, used by binary_grid.
Parameter input type: Float
Default value: NULL

Parameter: stellar_structure_algorithm
Description: Set the stellar structure algorithm. 0=modified BSE (default), 1=none, 2=external function (must be defined by the calling code), 3=binary_c (not yet implemented).
Parameter input type: Integer
Default value: 0
Macros: [‘STELLAR_STRUCTURE_ALGORITHM_MODIFIED_BSE = 0’, ‘STELLAR_STRUCTURE_ALGORITHM_NONE = 1’, ‘STELLAR_STRUCTURE_ALGORITHM_EXTERNAL_FUNCTION = 2’, ‘STELLAR_STRUCTURE_ALGORITHM_MINT = 3’]

Parameter: solver
Description: The type of solver. Default is the Forward-Euler (0), but could be RK2 (1), RK4 (2) or a predictor-corretor (3).
Parameter input type: Integer
Default value: 0
Macros: [‘SOLVER_FORWARD_EULER = 0’, ‘SOLVER_RK2 = 1’, ‘SOLVER_RK4 = 2’, ‘SOLVER_PREDICTOR_CORRECTOR = 3’]

Parameter: max_evolution_time
Description: Set the maximum age for the stars (Myr).
Parameter input type: Float
Default value: 15000

Parameter: max_model_number
Description: Set the maximum number of models, ignored if 0 (default is 0).
Parameter input type: Integer
Default value: 0

Parameter: monte_carlo_kicks
Description: Turn on Monte-Carlo SN kicks. On (True) by default, and indeed other algorithms are probably broken.
Parameter input type: True|False
Default value: True

Parameter: disable_debug
Description: Disables debug output. Only has an effect when DEBUG is 1, which probably requires a rebuild. Default FALSE.
Parameter input type: True|False
Default value: False

Parameter: timestep_logging
Description: Turn on timestep logging (default is False).
Parameter input type: True|False
Default value: False

Parameter: rejects_in_log
Description: Show timestep rejections in the main log (default is False).
Parameter input type: True|False
Default value: False

Parameter: vandenHeuvel_logging
Description: Turn on van den Heuvel logging (default is False).
Parameter input type: True|False
Default value: False

Parameter: evolution_splitting
Description: If True, turn on splitting of an evolutionary run if splitpoint (e.g. supernova) occurs.
Parameter input type: True|False
Default value: False

Parameter: disable_events
Description: Whether to disable the new events code (defaults to False, so we use events by default)
Parameter input type: True|False
Default value: False

Parameter: evolution_splitting_sn_eccentricity_threshold
Description: Threshold eccentricity above which evolution splitting happens in a system with no SN kick. (0.01)
Parameter input type: Float
Default value: 0.01

Parameter: evolution_splitting_sn_n
Description: Number of runs to split into when a SN occurs.
Parameter input type: Integer
Default value: 10

Parameter: evolution_splitting_maxdepth
Description: Max number of splits in an evolutionary run.
Parameter input type: Integer
Default value: 2

Parameter: equation_of_state_algorithm
Description: Set the equation of state algorithm. 0 = Paczynski.
Parameter input type: Integer
Default value: NULL
Macros: [‘EQUATION_OF_STATE_PACZYNSKI = 0’]

Parameter: opacity_algorithm
Description: Set the opacity algorithm. 0 = Paczynski, 1 = Ferguson/Opal.
Parameter input type: Integer
Default value: NULL
Macros: [‘OPACITY_ALGORITHM_PACZYNSKI = 0’, ‘OPACITY_ALGORITHM_FERGUSON_OPAL = 1’, ‘OPACITY_ALGORITHM_STARS = 2’]

Parameter: wind_mass_loss
Description: Defines the algorithm used for stellar winds. 0 = none, 1 = Hurley et al. (2002), 2 = Schneider (2018).
Parameter input type: Unsigned integer
Default value: 3
Macros: [‘WIND_ALGORITHM_NONE = 0’, ‘WIND_ALGORITHM_HURLEY2002 = 1’, ‘WIND_ALGORITHM_SCHNEIDER2018 = 2’, ‘WIND_ALGORITHM_BINARY_C_2020 = 3’]
Extra: 0

Parameter: gbwind
Description: Wind prescription for first red giant branch stars.  0=Reimers (Hurley et al 2000/2002; choose gb_reimers_eta=0.5 for their mass loss rate), 1=Schroeder+Cuntz 2005 (set gb_reimers_eta=1.0 for their mass loss rate).
Parameter input type: Integer
Default value: 0
Macros: [‘GB_WIND_REIMERS = 0’, ‘GB_WIND_SCHROEDER_CUNTZ_2005 = 1’, ‘GB_WIND_GOLDMAN_ETAL_2017 = 2’, ‘GB_WIND_BEASOR_ETAL_2020 = 3’]

Parameter: postagbwind
Description: Apply special post-(A)GB prescription. Default is POSTAGB_WIND_USE_GIANT which means we just use whatever is prescribed on the giant branch. Other options include: POSTAGB_WIND_NONE = 1 (no wind on the post (A)GB), POSTAGB_WIND_KRTICKA2020 = 2 which uses Krticka, Kubát and Krticková (2020, A&A 635, A173).
Parameter input type: Integer
Default value: 0
Macros: [‘POSTAGB_WIND_GIANT = 0’, ‘POSTAGB_WIND_NONE = 1’, ‘POSTAGB_WIND_KRTICKA2020 = 2’]

Parameter: Teff_postAGB_min
Description: The minimum temperature for which we apply post-(A)GB winds. See also Teff_postAGB_max. (6000 K)
Parameter input type: Float
Default value: 6000

Parameter: Teff_postAGB_max
Description: The maximum temperature for which we apply post-(A)GB winds. See also Teff_postAGB_min. (120000 K)
Parameter input type: Float
Default value: 120000

Parameter: mattsson_Orich_tpagbwind
Description: Experimental: turns on Mattsson’s TPAGB wind when the star is oxygen rich. Requires MATTSSON_MASS_LOSS.
Parameter input type: Integer
Default value: NULL

Parameter: magnetic_braking_factor
Description: Multiplier for the magnetic braking angular momentum loss rate.
Parameter input type: Float
Default value: 1

Parameter: magnetic_braking_gamma
Description: gamma factor in Rappaport style magnetic braking expression.
Parameter input type: Float
Default value: 3

Parameter: magnetic_braking_algorithm
Description: Algorithm for the magnetic braking angular momentum loss rate. 0 = Hurley et al. 2002, 1 = Andronov, Pinnsonneault and Sills 2003, 2 = Barnes and Kim 2010
Parameter input type: Integer
Default value: 0
Macros: [‘MAGNETIC_BRAKING_ALGORITHM_HURLEY_2002 = 0’, ‘MAGNETIC_BRAKING_ALGORITHM_ANDRONOV_2003 = 1’, ‘MAGNETIC_BRAKING_ALGORITHM_BARNES_2010 = 2’, ‘MAGNETIC_BRAKING_ALGORITHM_RAPPAPORT_1983 = 3’]

Parameter: helium_flash_mass_loss
Description: Mass to be lost at the helium flash.
Parameter input type: Float
Default value: 0

Parameter: gb_reimers_eta
Description: First red giant branch wind multiplication factor, cf. eta in Reimers’ mass loss formula. (This multiplies the 4e-13 in Reimers’ formula, or the 8e-14 in Schroeder and Cuntz.)
Parameter input type: Float
Default value: 0.4

Parameter: gbwindfac
Description: Multiplier for the giant branch wind mass loss rate
Parameter input type: Float
Default value: 1

Parameter: tpagbwindfac
Description: Multiplier for the TPAGB wind mass loss rate
Parameter input type: Float
Default value: 1

Parameter: eagbwindfac
Description: Multiplier for the EAGB wind mass loss rate
Parameter input type: Float
Default value: 1

Parameter: nieuwenhuijzen_windfac
Description: Multiplier for the Nieuwenhuijzen & de Jager wind mass loss rate
Parameter input type: Float
Default value: 1

Parameter: tpagbwind
Description: Wind prescription during the TPAGB. 0=Karakas 2002 (a modified Vassiliadis and Wood 1993), 1=Hurley et al 2000/2002 (Vassiliadis and Wood 1993), 2=Reimers, 3=Bloecker, 4=Van Loon,  5=Rob’s C-wind (broken?), 6,7=Vassiliadis and Wood 1993 (Karakas,Hurley variants respectively) when C/O>1, 8=Mattsson, 9 = Goldman et al. (2017), 10 = Beasor et al. (2020).
Parameter input type: Integer
Default value: 0
Macros: [‘TPAGB_WIND_VW93_KARAKAS = 0’, ‘TPAGB_WIND_VW93_ORIG = 1’, ‘TPAGB_WIND_REIMERS = 2’, ‘TPAGB_WIND_BLOECKER = 3’, ‘TPAGB_WIND_VAN_LOON = 4’, ‘TPAGB_WIND_ROB_CWIND = 5’, ‘TPAGB_WIND_VW93_KARAKAS_CARBON_STARS = 6’, ‘TPAGB_WIND_VW93_ORIG_CARBON_STARS = 7’, ‘TPAGB_WIND_MATTSSON = 8’, ‘TPAGB_WIND_GOLDMAN_ETAL_2017 = 9’, ‘TPAGB_WIND_BEASOR_ETAL_2020 = 10’]

Parameter: eagbwind
Description: Wind prescription during the EAGB. 0=BSE (Hurley+2002, based on VW93), 1 = Goldman et al. (2017), 2 = Beasor et al. (2020).
Parameter input type: Integer
Default value: 0
Macros: [‘EAGB_WIND_BSE = 0’, ‘EAGB_WIND_GOLDMAN_ETAL_2017 = 1’, ‘EAGB_WIND_BEASOR_ETAL_2020 = 2’]

Parameter: wind_gas_to_dust_ratio
Description: Gas to dust ratio used in wind calculations (e.g. Goldman et al. 2017). Typically 200 (Milky Way)-500 (Magellanic Clouds). Default is 200, approximately as in MW stars.
Parameter input type: Float
Default value: 200

Parameter: vwind_multiplier
Description: Multiplier for the stellar wind velocity.
Parameter input type: Float
Default value: 1

Parameter: vwind_beta
Description: Beta for stellar wind speed calculations, where vwind=sqrt(beta) * escape velocity. Default 0.125 (from BSE, Hurley et al. 2002).
Parameter input type: Float
Default value: 0.125

Parameter: superwind_mira_switchon
Description: In the Vassiliadis and Wood (1993) AGB wind prescription, the superwind is turned on at a given Mira period, usually 500 days. You can vary when this switch-on happens with this parameter.
Parameter input type: Float
Default value: 500

Parameter: vw93_mira_shift
Description: In the Vassiliadis and Wood (1993) AGB wind prescription, the wind loss rate depends on the Mira period plus this offset. Requires VW93_MIRA_SHIFT.
Parameter input type: Float
Default value: 0

Parameter: vw93_multiplier
Description: In the Vassiliadis and Wood (1993) AGB wind prescription, the wind loss rate is multiplied by this factor. Requires VW93_MULTIPLIER.
Parameter input type: Float
Default value: 1

Parameter: tpagb_reimers_eta
Description: TPAGB Reimers wind multiplication factor, cf. eta in Reimers’ mass loss formula. (This multiplies the 4e-13 in Reimers’ formula, or the 8e-14 in Schroeder and Cuntz.) Note that Reimers is not the default TPAGB wind prescription. See also tpagbwind.
Parameter input type: Float
Default value: 1

Parameter: Tout_Pringle_1992_multiplier
Description: Multiplier for the Tout & Pringle (1992) magnetic wind. (0.0)
Parameter input type: Float
Default value: 0

Parameter: artificial_mass_accretion_rate%d
Description: Constant mass accretion rate for star <n>.
Parameter input type: Float(scanf)
Default value: NULL

Parameter: artificial_mass_accretion_rate_by_stellar_type%d
Description: Constant mass accretion rate for stellar type <n>.
Parameter input type: Float(scanf)
Default value: NULL

Parameter: artificial_angular_momentum_accretion_rate%d
Description: Constant angular momentum accretion for star <n>.
Parameter input type: Float(scanf)
Default value: NULL

Parameter: artificial_orbital_angular_momentum_accretion_rate
Description: Constant angular momentum accretion rate on the orbit.
Parameter input type: Float
Default value: 0

Parameter: artificial_accretion_start_time
Description: Time at which artificial accretion stars. Ignored if <0 (default is -1).
Parameter input type: Float
Default value: -1
Macros: [‘ARTIFICIAL_ACCRETION_IGNORE = -1’]

Parameter: artificial_accretion_end_time
Description: Time at which artificial accretion ends. Ignored if <0 (default is -1).
Parameter input type: Float
Default value: -1
Macros: [‘ARTIFICIAL_ACCRETION_IGNORE = -1’]

Parameter: wr_wind
Description: Massive-star (WR) wind prescription. 0 = Hurley et al 2000/2002, 1=Maeder and Meynet, 2=Nugis and Lamers, 3=John Eldridge’s version of Vink’s early-2000s wind (See Lynnette Dray’s thesis, or John Eldridge’s thesis)
Parameter input type: Integer
Default value: 0
Macros: [‘WR_WIND_BSE = 0’, ‘WR_WIND_MAEDER_MEYNET = 1’, ‘WR_WIND_NUGIS_LAMERS = 2’, ‘WR_WIND_ELDRIDGE = 3’]

Parameter: wr_wind_fac
Description: Massive-star (WR) wind multiplication factor.
Parameter input type: Float
Default value: 1

Parameter: wrwindfac
Description: Massive-star (WR) wind multiplication factor. Synonymous with wr_wind_fac (which you should use instead).
Parameter input type: Float
Default value: 1

Parameter: BH_prescription
Description: Black hole mass prescrition: relates the mass of a newly formed black hole to its progenitor’s (CO) core mass. BH_HURLEY2002 = 0 = Hurley et al 2000/2002, BH_BELCZYNSKI = 1 = Belczynski (early 2000s), BH_SPERA2015 = Spera+ 2015, BH_FRYER12_DELAYED = 3 = Fryer et al. (2012) delayed prescription, BH_FRYER12_RAPID = 4 = Fryer et al. (2012) rapid prescription, BH_FRYER12_STARTRACK = 5 = Fryer et al. (2012) startrack prescription.
Parameter input type: Integer
Default value: 0
Macros: [‘BH_HURLEY2002 = 0’, ‘BH_BELCZYNSKI = 1’, ‘BH_SPERA2015 = 2’, ‘BH_FRYER12_DELAYED = 3’, ‘BH_FRYER12_RAPID = 4’, ‘BH_FRYER12_STARTRACK = 5’]

Parameter: sn_kick_distribution_II
Description: Set the distribution of speeds applied to kick type II core collapse supernova systems. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 1
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_distribution_ECAP
Description: Set the distribution of speeds applied to the remnants of electron-capture supernovae. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 0
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_distribution_NS_NS
Description: Set the distribution of speeds applied to kick neutron stars and black holes that survive a NS-NS merger. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 0
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_distribution_IBC
Description: Set the distribution of speeds applied to kick newly-born neutron stars and black holes after a type Ib/c core-collapse supernova. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 1
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_distribution_GRB_COLLAPSAR
Description: Set the distribution of speeds applied to kick newly-born neutron stars and black holes after a type Ib/c core-collapse supernova which is also a collapsar. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 1
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_distribution_TZ
Description: Set the distribution of speeds applied to kick newly-born neutron stars and black holes at the death of a Thorne-Zytkow object. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 0
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_distribution_AIC_BH
Description: Set the distribution of speeds applied to kick newly-born neutron stars black holes after accretion induced collapse of a neutron star. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 0
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_distribution_BH_BH
Description: Set the distribution of speeds applied to black holes formed by the merger of two black holes. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 0
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_distribution_BH_NS
Description: Set the distribution of speeds applied to black holes formed by the merger of a neutron star and a black holes. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 0
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_distribution_IA_Hybrid_HeCOWD
Description: Set the distribution of speeds applied to any survivor of a hybrid He-COWD SNIa explosion. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 0
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_distribution_IA_Hybrid_HeCOWD_subluminous
Description: Set the distribution of speeds applied to any survivor of a subluminous hybrid He-COWD SNIa explosion. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Integer
Default value: 0
Macros: [‘KICK_VELOCITY_FIXED = 0’, ‘KICK_VELOCITY_MAXWELLIAN = 1’, ‘KICK_VELOCITY_CUSTOM = 2’]

Parameter: sn_kick_dispersion_II
Description: Set the dispersion of speeds applied to kick type II core collapse supernova systems. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 190

Parameter: sn_kick_dispersion_ECAP
Description: Set the dispersion of speeds applied to the remnants of electron-capture supernovae. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 0

Parameter: sn_kick_dispersion_NS_NS
Description: Set the dispersion of speeds applied to kick neutron stars and black holes that survive a NS-NS merger. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 0

Parameter: sn_kick_dispersion_IBC
Description: Set the dispersion of speeds applied to kick newly-born neutron stars and black holes after a type Ib/c core-collapse supernova. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 190

Parameter: sn_kick_dispersion_GRB_COLLAPSAR
Description: Set the dispersion of speeds applied to kick newly-born neutron stars and black holes after a type Ib/c core-collapse supernova which is also a collapsar. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 190

Parameter: sn_kick_dispersion_TZ
Description: Set the dispersion of speeds applied to kick newly-born neutron stars and black holes at the death of a Thorne-Zytkow object. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 0

Parameter: sn_kick_dispersion_AIC_BH
Description: Set the dispersion of speeds applied to kick newly-born neutron stars black holes after accretion induced collapse of a neutron star. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 0

Parameter: sn_kick_dispersion_BH_BH
Description: Set the dispersion of speeds applied to black holes formed by the merger of two black holes. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 0

Parameter: sn_kick_dispersion_BH_NS
Description: Set the dispersion of speeds applied to black holes formed by the merger of a neutron star and a black holes. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 0

Parameter: sn_kick_dispersion_IA_Hybrid_HeCOWD
Description: Set the dispersion of speeds applied to the survivor of a SNIa explosion of a hybrid He-COWD. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 0

Parameter: sn_kick_dispersion_IA_Hybrid_HeCOWD_subluminous
Description: Set the dispersion of speeds applied to the survivor of a subluminous SNIa explosion of a hybrid He-COWD. 0=fixed, 1=maxwellian (hurley/BSE), 2=custom function (see monte_carlo_kicks.c).
Parameter input type: Float
Default value: 0

Parameter: sn_kick_companion_IA_He
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a Ia He supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_IA_ELD
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a Ia ELD (sub-Mch) supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_IA_CHAND
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a Ia Mch supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_AIC
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when an accretion induced collapse (supernova) occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_ECAP
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when an electron capture supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_IA_He_Coal
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a Ia helium merger supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_IA_CHAND_Coal
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a Ia Mch merger supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_NS_NS
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a neutron-star neutron-star merger. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_GRB_COLLAPSAR
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a GRB Collapsar (rapidly rotating SN Ibc) supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_HeStarIa
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a He-star Ia supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_IBC
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a type Ib/c supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_II
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a type II supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_IIa
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a type IIa supernova occurs. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_WDKICK
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a WD is kicked. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_TZ
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a Thorne-Zytkow object is formed. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_AIC_BH
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a neutron star collapses to a black hole. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_BH_BH
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when two black holes merge. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_BH_NS
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the, kick on the companion when a black hole merges with a neutron star. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_IA_Hybrid_HeCOWD
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the kick on the companion, if it survives, in a hybrid He-COWD type Ia explosion. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: sn_kick_companion_IA_Hybrid_HeCOWD_subluminous
Description: Set the speed (if >=0) of, or the algothim (if <0) used to calculate the kick on the companion, if it survives, in a subluminous hybrid He-COWD type Ia explosion. 0 = none, 1 = Liu+2015, 2 = Wheeler+ 1975.
Parameter input type: Float
Default value: 0
Macros: [‘SN_IMPULSE_NONE = 0’, ‘SN_IMPULSE_LIU2015 = 1’, ‘SN_IMPULSE_WHEELER1975 = 2’]

Parameter: wd_sigma
Description: Set the speed at which white dwarfs are kicked when they form, in km/s. Default is zero (i.e. no kick). Requires WD_KICKS.
Parameter input type: Float
Default value: 0

Parameter: wd_kick_direction
Description: Set the direction of white dwarf kicks. 0 = random, 1 = up, 2 = forward, 3 = backward, 4 = inward, 5 = outward. Requires WD_KICKS.
Parameter input type: Integer
Default value: 0
Macros: [‘KICK_RANDOM = 0’, ‘KICK_STRAIGHT_UP = 1’, ‘KICK_FORWARD = 2’, ‘KICK_BACKWARD = 3’, ‘KICK_INWARD = 4’, ‘KICK_OUTWARD = 5’]

Parameter: wd_kick_when
Description: Decide when to kick a white dwarf. 0=at birth, 1=at first RLOF, 2=at given pulse number (see wd_kick_pulse_number), 3 at every pulse Requires WD_KICKS.
Parameter input type: Integer
Default value: 0
Macros: [‘WD_KICK_END_AGB = 0’, ‘WD_KICK_FIRST_RLOF = 1’, ‘WD_KICK_AT_GIVEN_PULSE = 2’, ‘WD_KICK_AT_EVERY_PULSE = 3’]

Parameter: wd_kick_pulse_number
Description: Apply a kick to a star at a desired pulse number on the TPAGB (i.e. pre-WD). Requires WD_KICKS.
Parameter input type: Integer
Default value: 0

Parameter: minimum_helium_ignition_core_mass
Description: Minimum helium core mass required to ignite helium in the case that the hydrogen envelope is stripped on the giant branch, e.g. to make an sdB or sdO star. Typically 0.4, if 0.0 then the BSE algorithm (based on the total mass) is used.
Parameter input type: Float
Default value: 0

Parameter: minimum_CO_core_mass_for_carbon_ignition
Description: Minimum CO core mass for carbon ignition, assuming Mc,bagb>1.6Msun. Typically around 1.08Msun (Pols+1998).
Parameter input type: Float
Default value: 1.08

Parameter: minimum_CO_core_mass_for_neon_ignition
Description: Minimum CO core mass for neon ignition. Typically around 1.42Msun. Stars that have cores that ignite carbon, but not neon explode in electon-capture supernovae.
Parameter input type: Float
Default value: 1.42

Parameter: minimum_mcbagb_for_nondegenerate_carbon_ignition
Description: Minimum Mc,bagb (core mass at the base of the AGB) for non-degenerate carbon ignition. Typically around 2.25Msun (Pols+1998).
Parameter input type: Float
Default value: 2.25

Parameter: maximum_mcbagb_for_degenerate_carbon_ignition
Description: Maximum Mc,bagb (core mass at the base of the AGB) for degenerate carbon ignition. Typically around 1.6Msun (Pols+1998).
Parameter input type: Float
Default value: 1.6

Parameter: max_neutron_star_mass
Description: Maximum mass of a neutron star before it collapses to a black hole. Typically around 2Msun.
Parameter input type: Float
Default value: 2.2

Parameter: chandrasekhar_mass
Description: The Chandrasekhar mass, usually 1.44Msun
Parameter input type: Float
Default value: 1.38

Parameter: delta_mcmin
Description: A parameter to reduce the minimum core mass for third dredge up to occur on the TPAGB. As used by Izzard and Tout (2004) to increase the amount of dredge up, hence carbon, in Magellanic cloud stars.
Parameter input type: Float
Default value: 0

Parameter: lambda_min
Description: A parameter to increase the efficiency of third dredge up on the TPAGB. The efficiency is lambda * lambda_mult, and setting lambda_min>0 implies that, once Mc>Mcmin (see delta_mcmin) lambda=Max(lambda(fit to Karakas), lambda_min). As used by Izzard and Tout (2004) to increase the amount of dredge up, hence carbon, in Magellanic cloud stars. See also lambda_multiplier.
Parameter input type: Float
Default value: 0

Parameter: lambda_multiplier
Description: A parameter to increase the efficiency of third dredge up on the TPAGB. The efficiency is lambda * lambda_mult, and setting lambda_min>0 implies that, once Mc>Mcmin (see delta_mcmin) lambda=Max(lambda(fit to Karakas), lambda_min). As used by Izzard and Tout (2004) to increase the amount of dredge up, hence carbon, in Magellanic cloud stars.
Parameter input type: Float
Default value: 1

Parameter: minimum_envelope_mass_for_third_dredgeup
Description: The minimum envelope mass for third dredge up on the TPAGB. Early, solar metallicity models by Straniero et al suggested 0.5Msun is typical. However, circumstantial evidence (Izzard et al 2009) as well as newer models by Stancliffe and Karakas suggest that at low metallicity a value nearer zero is more appropriate.
Parameter input type: Float
Default value: 0.5

Parameter: mass_of_pmz
Description: The mass in the partial mixing zone of a TPAGB star, using the Karakas 2012 tables. Ask Carlo Abate for more details, or see the series of papers Abate et al 2012, 2013, 2014. Requires NUCSYN and USE_TABULAR_INTERSHELL_ABUNDANCES_KARAKAS_2012.
Parameter input type: Float
Default value: NULL

Parameter: c13_eff
Description: The “efficiency” of partial mixing in a TPAGB star intershell region, when using the s-process tables of Gallino, Busso, Lugaro et al. as provided by Maria Lugaro for the Izzard et al. 2009 paper. Requires NUCSYN and NUCSYN_S_PROCESS.
Parameter input type: Float
Default value: 1

Parameter: mc13_pocket_multiplier
Description: Multiplies the mass in the partial mixing zone of a TPAGB star, when using the s-process tables of Gallino, Busso, Lugaro et al. as provided by Maria Lugaro for the Izzard et al. 2009 paper. Requires NUCSYN and NUCSYN_S_PROCESS.
Parameter input type: Float
Default value: 1

Parameter: tides_convective_damping
Description: Tidal convective damping algorithm. 0=TIDES_HURLEY2002 Zahn 197x timescales + Hut, as in Hurley et al (2002), 1 = TIDES_ZAHN1989: Zahn 1989 lambdas + Hut.
Parameter input type: Integer
Default value: 0
Macros: [‘TIDES_HURLEY2002 = 0’, ‘TIDES_ZAHN1989 = 1’]

Parameter: E2_prescription
Description: Choose how to calculate the E2 structural parameter (used in tidal timescale calculations). 0=Hurley 1=Izzard (see Siess et al 2013).
Parameter input type: Integer
Default value: 0
Macros: [‘E2_HURLEY_2002 = 0’, ‘E2_IZZARD = 1’, ‘E2_MINT = 2’]

Parameter: dtfac
Description: A parameter to decrease the timestep ONLY during the TPAGB phase.
Parameter input type: Float
Default value: 1

Parameter: hbbtfac
Description: A parameter to modulate the temperature at the base of the hot-bottom burning zone in TPAGB stars. (Works only if NUCSYN is defined)
Parameter input type: Float
Default value: 1

Parameter: wind_multiplier_%d
Description: Wind multiplier for the stellar type specified by the intger %d. By default these are all 1.0.
Parameter input type: Float(scanf)
Default value: NULL

Parameter: wind_type_multiplier_%d
Description: Wind multiplier for different types of wind (MS, GB, AGB, WR, LBV, OTHER), given by the integer %d. By default these are all 1.0.
Parameter input type: Float(scanf)
Default value: NULL

Parameter: pre_main_sequence
Description: Set to True to turn on pre-main sequence evolution. Currently this is not a special stellar type, rather the first (small) fraction of the main sequence has increased radii to match the Railton et al 2014 fits to Tout’s pre-main sequence stars. Requires PRE_MAIN_SEQUENCE. See also pre_main_sequence_fit_lobes.
Parameter input type: True|False
Default value: False

Parameter: pre_main_sequence_fit_lobes
Description: Set to True force a pre-main sequence star into its Roche lobe. This is done by artificially aging it. Requires PRE_MAIN_SEQUENCE
Parameter input type: True|False
Default value: False

Parameter: small_envelope_method
Description: Choose the method used to determine the stellar radius when the envelope mass is very thin. 0 = Hurley et al. (2002), 1 = Miller Bertolami et al. (2016+) for GB and AGB stars only.
Parameter input type: Integer
Default value: 0
Macros: [‘SMALL_ENVELOPE_METHOD_BSE = 0’, ‘SMALL_ENVELOPE_METHOD_MILLER_BERTOLAMI = 1’]

Parameter: timestep_modulator
Description: Multiplier applied to the global timestep. Requires TIMESTEP_MODULATION.
Parameter input type: Float
Default value: 1

Parameter: timestep_multiplier%d
Description: Multiplier applied to timestep limit <n>.
Parameter input type: Float(scanf)
Default value: NULL

Parameter: maximum_timestep
Description: The maximum timestep (MYr).
Parameter input type: Float
Default value: 1e+20

Parameter: zoomfac_multiplier_decrease
Description: When a timestep is rejected, decrease the timestep by this factor (0.5).
Parameter input type: Float
Default value: 0.5

Parameter: zoomfac_multiplier_increase
Description: When a timestep is rejected, zooms, then succeeds, increase the timestep by this factor (1.2).
Parameter input type: Float
Default value: 1.2

Parameter: maximum_timestep_factor
Description: The maximum factor between two subsequent timesteps (1.2).
Parameter input type: Float
Default value: 0

Parameter: maximum_nuclear_burning_timestep
Description: The maximum timestep (MYr) in any nuclear burning phase.
Parameter input type: Float
Default value: 1e+20

Parameter: nova_retention_method
Description: Algorithm used to calculate the amount of mass retained during a nova explosion. 0=use nova_retention_fraction. (other methods pending)
Parameter input type: Integer
Default value: 0
Macros: [‘NOVA_RETENTION_ALGORITHM_CONSTANT = 0’, ‘NOVA_RETENTION_ALGORITHM_CLAEYS2014 = 1’, ‘NOVA_RETENTION_ALGORITHM_HILLMAN2015 = 2’]

Parameter: MINT_metallicity
Description: This sets the metallicity for MINT. It is ignored if set to -1.0, the default, in which case the normal metallicity parameter is used.
Parameter input type: Float
Default value: -1

Parameter: gaia_Teff_binwidth
Description: log10(Effective temperature) bin width used to make Gaia-like HRDs
Parameter input type: Float
Default value: NULL

Parameter: gaia_L_binwidth
Description: log10(luminosity) bin width used to make Gaia-like HRDs
Parameter input type: Float
Default value: NULL

Parameter: gaia_colour_transform_method
Description: Use this to select the method used to transform to Gaia colours from other colour schemes. GAIA_CONVERSION_UBVRI_UNIVARIATE_JORDI2010 = 0 Jordi et al.’s univariate UBVRI fits, GAIA_CONVERSION_UBVRI_BIVARIATE_JORDI2010 = 1 Jordi et al.’s bivariate UBVRI fits, GAIA_CONVERSION_ugriz_UNIVARIATE_JORDI2010 = 2 Jordi et al.’s univariate UBVRI fits, GAIA_CONVERSION_ugriz_BIVARIATE_JORDI2010 = 3 Jordi et al.’s univariate ugriv fits, GAIA_CONVERSION_UBVRI_UNIVARIATE_EVANS2018 = 4 Evans et al. (2018, DR2) fits, GAIA_CONVERSION_ugriz_UNIVARIATE_EVANS2018 = 5 Evans et al. (2018, DR2) fits, GAIA_CONVERSION_UBVRI_RIELLO2020 = 6 Riello et al. (2020, DR3) fits, GAIA_CONVERSION_ugriz_RIELLO2020 = 7 Riello et al. (2020, DR3) fits.
Parameter input type: Integer
Default value: 4
Macros: [‘GAIA_CONVERSION_UBVRI_UNIVARIATE_JORDI2010 = 0’, ‘GAIA_CONVERSION_UBVRI_BIVARIATE_JORDI2010 = 1’, ‘GAIA_CONVERSION_ugriz_UNIVARIATE_JORDI2010 = 2’, ‘GAIA_CONVERSION_ugriz_BIVARIATE_JORDI2010 = 3’, ‘GAIA_CONVERSION_UBVRI_UNIVARIATE_EVANS2018 = 4’, ‘GAIA_CONVERSION_ugriz_UNIVARIATE_EVANS2018 = 5’, ‘GAIA_CONVERSION_UBVRI_RIELLO2020 = 6’, ‘GAIA_CONVERSION_ugriz_RIELLO2020 = 7’]

Parameter: rotationally_enhanced_mass_loss
Description: Set to 1 to enable rotationally enhanced mass loss rate algorithms: 0= none, 1=formula cf. Langer models (=ROTATIONALLY_ENHANCED_MASSLOSS_LANGER_FORMULA), 2=limit accretion rate before wind loss is applied, 3 = both 1 and 2. See also rotationally_enhanced_exponent
Parameter input type: Integer
Default value: 0
Macros: [‘ROTATIONALLY_ENHANCED_MASSLOSS_NONE = 0’, ‘ROTATIONALLY_ENHANCED_MASSLOSS_LANGER_FORMULA = 1’, ‘ROTATIONALLY_ENHANCED_MASSLOSS_ANGMOM = 2’, ‘ROTATIONALLY_ENHANCED_MASSLOSS_LANGER_FORMULA_AND_ANGMOM = 3’]

Parameter: AGB_core_algorithm
Description: Algorithm to use for calculating AGB core masses. 0=Hurley et al. 2002 if no NUCSYN, Karakas 2002 if NUCSYN is defined; 1=Hurley et al. 2002 (overshooting models); 1=Karakas 2002 (non-overshooting models).
Parameter input type: Integer
Default value: 2
Macros: [‘AGB_CORE_ALGORITHM_DEFAULT = 0’, ‘AGB_CORE_ALGORITHM_HURLEY = 1’, ‘AGB_CORE_ALGORITHM_KARAKAS = 2’]

Parameter: AGB_radius_algorithm
Description: Algorithm to use for calculating radii on the TPAGB.
Parameter input type: Integer
Default value: 2
Macros: [‘AGB_RADIUS_ALGORITHM_DEFAULT = 0’, ‘AGB_RADIUS_ALGORITHM_HURLEY = 1’, ‘AGB_RADIUS_ALGORITHM_KARAKAS = 2’]

Parameter: AGB_luminosity_algorithm
Description: Algorithm to use for calculating luminosities on the TPAGB.
Parameter input type: Integer
Default value: 2
Macros: [‘AGB_LUMINOSITY_ALGORITHM_DEFAULT = 0’, ‘AGB_LUMINOSITY_ALGORITHM_HURLEY = 1’, ‘AGB_LUMINOSITY_ALGORITHM_KARAKAS = 2’]

Parameter: AGB_3dup_algorithm
Description: Algorithm to use for calculating third dredge up efficiency on the TPAGB.
Parameter input type: Integer
Default value: 2
Macros: [‘AGB_THIRD_DREDGE_UP_ALGORITHM_DEFAULT = 0’, ‘AGB_THIRD_DREDGE_UP_ALGORITHM_HURLEY = 1’, ‘AGB_THIRD_DREDGE_UP_ALGORITHM_KARAKAS = 2’, ‘AGB_THIRD_DREDGE_UP_ALGORITHM_STANCLIFFE = 3’]

Parameter: overspin_algorithm
Description: Algorithm to determine what we do when a star is rotating at its breakup velocity. OVERSPIN_BSE (0) conservatively transfers the angular momentum back to the orbit. OVERSPIN_MASSLOSS uses the rotationally_enhanced_massloss parameter to lose mass which carries away the angular momentum.
Parameter input type: Integer
Default value: 0
Macros: [‘OVERSPIN_BSE = 0’, ‘OVERSPIN_MASSLOSS = 1’]

Parameter: rotationally_enhanced_exponent
Description: The exponent (power) by which rotationally enhanced mass loss is raised. Requires ROTATIONALLY_ENHANCED_MASS_LOSS. See also rotationally_enhanced_mass_loss.
Parameter input type: Float
Default value: 1

Parameter: batchmode
Description: Set the batchmode control variable. Use only if you know what you are doing!
Parameter input type: Integer
Default value: 3

Parameter: speedtests
Description: If True, turns on speedtests during version information (off by default).
Parameter input type: True|False
Default value: False

Parameter: use_fixed_timestep_%d
Description: Set to True to use fixed timestep <n>, False to turn off. Fixed timesteps are on (this is True) by default.
Parameter input type: Boolean(scanf)
Default value: NULL

Parameter: task%d
Description: Control tasks to be performed by binary_c. By default, these are all TRUE. For more information see binary_c_macros.h, particularly the BINARY_C_TASK_* macros.
Parameter input type: Boolean(scanf)
Default value: NULL

Parameter: orbiting_object
Description: Usage: –orbiting_object mass,spinrate,central_object,period.
Parameter input type: *
Default value: NULL
Extra: 1.0

Parameter: orbiting_objects_log
Description: If True, turn on orbiting-object log.
Parameter input type: True|False
Default value: False

Parameter: orbiting_objects_wind_accretion_multiplier
Description: Multiplier for wind accretion on orbiting objects. Hurley et al 2002 use 1.5, which is the default.
Parameter input type: Float
Default value: 1.5

Parameter: orbiting_objects_close_pc_threshold
Description: How close are orbiting objects allowed to be? Set this to be the absolute percentage difference minimum.
Parameter input type: Float
Default value: 1

Parameter: orbiting_objects_tides_multiplier
Description: Multiplier for tidal torques on orbiting objects.
Parameter input type: Float
Default value: 1

Parameter: evaporate_escaped_orbiting_objects
Description: If True, evaporate orbiting objects that have escaped the system.
Parameter input type: True|False
Default value: False

Parameter: RLOF_transition_objects_escape
Description: If True, objects that escape their Roche lobe are ejected from the system, otherwise they are placed just outside the minimum stable orbit.
Parameter input type: True|False
Default value: False

Parameter: PN_resolve
Description: If True, the timestep will be shortened to resolve better the PN phase (FALSE).
Parameter input type: True|False
Default value: False

Parameter: PN_resolve_minimum_luminosity
Description: The luminosity above which extra time resolution for PNe is applied (see PN_resolve).
Parameter input type: Float
Default value: 31.62

Parameter: PN_resolve_maximum_envelope_mass
Description: The envelope mass below which extra time resolution for PNe is applied (see PN_resolve).
Parameter input type: Float
Default value: 0.1

Parameter: PN_resolve_minimum_effective_temperature
Description: The minimum effective temperature above which extra time resolution for PNe is applied (see PN_resolve).
Parameter input type: Float
Default value: 12500

Parameter: PN_fast_wind
Description: If True, thin-envelope PNe will have fast winds (FALSE).
Parameter input type: True|False
Default value: False

Parameter: PN_fast_wind_dm_GB
Description: The envelope mass below which fast wind used during the GB if PN_fast_wind is TRUE. (See also PN_fast_wind, PN_fast_wind_mdot_GB)
Parameter input type: Float
Default value: 0.01

Parameter: PN_fast_wind_mdot_GB
Description: The envelope mass below which fast wind used during the GB if PN_fast_wind is TRUE. (See also PN_fast_wind, PN_fast_wind_mdot_GB)
Parameter input type: Float
Default value: 1e-06

Parameter: PN_fast_wind_dm_AGB
Description: The envelope mass below which fast wind used during the AGB if PN_fast_wind is TRUE. (See also PN_fast_wind, PN_fast_wind_mdot_AGB)
Parameter input type: Float
Default value: 0.001

Parameter: PN_fast_wind_mdot_AGB
Description: The envelope mass below which fast wind used during the GB if PN_fast_wind is TRUE. (See also PN_fast_wind, PN_fast_wind_mdot_AGB)
Parameter input type: Float
Default value: 1e-06

Parameter: HeWD_HeWD_ignition_mass
Description: HeWD-HeWD mergers above this mass reignite helium. (0.3)
Parameter input type: Float
Default value: 0.3

Parameter: wind_Nieuwenhuijzen_luminosity_lower_limit
Description: Above this luminosity we activate the Nieuwenhuijzen and de Jager wind (4e3 Lsun).
Parameter input type: Float
Default value: 4000

Parameter: wind_LBV_luminosity_lower_limit
Description: Above this luminosity we activate the LBV wind (6e5 Lsun).
Parameter input type: Float
Default value: 600000

Parameter: colour%d
Description: Sets colour %d (0 to NUM_ANSI_COLOURS-1) to the extended ANSI set colour you choose (1-255, 0 means ignore). The colour numbers are defined in src/logging/ansi_colours.h
Parameter input type: Int(scanf)
Default value: NULL

Parameter: apply_Darwin_Radau_correction
Description: Apply Darwin-Radau correction to the moment of inertia to take rotation into account?
Parameter input type: True|False
Default value: False

Parameter: degenerate_core_merger_nucsyn
Description: If TRUE, assume that in a degnerate core merger, energy is generated from nucleosynthesis of the whole core, and that this can disrupt the core. The BSE algorithm (Hurley et al. 2002) assumes this to be TRUE, but binary_c assumes FALSE by default. (FALSE)
Parameter input type: True|False
Default value: False

Parameter: degenerate_core_helium_merger_ignition
Description: If TRUE, assume that when there is a degenerate helium core merger, the star reignites helium. This is required to make R-type carbon stars. (TRUE)
Parameter input type: True|False
Default value: True

Parameter: degenerate_core_merger_dredgeup_fraction
Description: If non-zero, mix this fraction of the degenerate core during a merger.(0.0).
Parameter input type: Float
Default value: 0

Section: binary

Parameter: separation
Description: Set the orbital separation (actually the semi-major axis) of the binary (internal index 0, stellar indices 0 and 1) in solar radii. Note that if the orbital period is given, it is used to calculate the separation. So if you want to set the separation instead, either do not set the orbital period or set the orbital period to zero (0.0).
Parameter input type: Float
Default value: 0

Parameter: separation_triple
Description: Set the orbital separation (actually the semi-major axis) of the triple (internal index 1) in solar radii. Note that if the orbital period is given, it is used to calculate the separation. So if you want to set the separation instead, either do not set the orbital period or set the orbital period to zero (0.0).
Parameter input type: Float
Default value: 0

Parameter: separation_quadruple
Description: Set the orbital separation (actually the semi-major axis) of the quadruple (internal index 2) in solar radii. Note that if the orbital period is given, it is used to calculate the separation. So if you want to set the separation instead, either do not set the orbital period or set the orbital period to zero (0.0).
Parameter input type: Float
Default value: 0

Parameter: orbital_period
Description: Set the initial orbital period of the binary, stars 1 and 2 (internal indices 0 and 1) in days. See also separation.
Parameter input type: Float
Default value: 0

Parameter: orbital_period_triple
Description: Set the initial orbital period of the triple in days. See also separation.
Parameter input type: Float
Default value: 0

Parameter: orbital_period_quadruple
Description: Set the orbital period of the outer binary in a quadrulple (stars 3 and 4, internal indices 2 and 3) in days. See also separation.
Parameter input type: Float
Default value: 0

Parameter: eccentricity
Description: Set the initial eccentricity of the binary orbit (stars 1 and 2, internal indices 0 and 1).
Parameter input type: Float
Default value: 0

Parameter: eccentricity_triple
Description: Set the initial eccentricity of the triple orbit.
Parameter input type: Float
Default value: 0

Parameter: eccentricity_quadruple
Description: Set the initial eccentricity of the outer binary of a quadruple (stars 3 and 4, internal indices 2 and 3).
Parameter input type: Float
Default value: 0

Parameter: incliniation
Description: Set the initial orbital_inclination of the binary relative to zero.
Parameter input type: Float
Default value: 0

Parameter: incliniation_triple
Description: Set the initial orbital_inclination of the triple orbit relative to zero.
Parameter input type: Float
Default value: 0

Parameter: incliniation_quadruple
Description: Set the initial orbital_inclinationy of the quadruple orbit relative to zero.
Parameter input type: Float
Default value: 0

Parameter: orbital_phase
Description: Set the initial orbital phase of the binary orbit.
Parameter input type: Float
Default value: 0

Parameter: orbital_phase_triple
Description: Set the initial orbital phase of the triple orbit.
Parameter input type: Float
Default value: 0

Parameter: orbital_phase_quadruple
Description: Set the initial orbital phase of the quadruple orbit.
Parameter input type: Float
Default value: 0

Parameter: argument_of_periastron
Description: Set the initial argument of periastron of the binary orbit.
Parameter input type: Float
Default value: 0

Parameter: argument_of_periastron_triple
Description: Set the initial argument of periastron of the triple orbit.
Parameter input type: Float
Default value: 0

Parameter: argument_of_periastron_quadruple
Description: Set the initial argument of periastron of the quadruple orbit.
Parameter input type: Float
Default value: 0

Parameter: disc_timestep_factor
Description: Factor that multiplies the natural timestep of a disc.
Parameter input type: Float
Default value: 0.01

Parameter: white_dwarf_cooling_model
Description: White dwarf cooling model, relates age to luminosity. WHITE_DWARF_COOLING_MESTEL = 0 is Mestel’s model, WHITE_DWARF_COOLING_MESTEL_MODIFIED = 1 is Hurley’s modified Mestel model, WHITE_DWARF_COOLING_CARRASCO2014 = 2 is based on Carrasco (2014) tables.
Parameter input type: Integer
Default value: 0
Macros: [‘WHITE_DWARF_COOLING_MESTEL = 0’, ‘WHITE_DWARF_COOLING_MESTEL_MODIFIED = 1’, ‘WHITE_DWARF_COOLING_CARRASCO2014 = 2’]

Parameter: white_dwarf_radius_model
Description: White dwarf radius model, radius to mass (and perhaps age). WHITE_DWARF_RADIUS_NAUENBERG1972 = 0 Nauenberg (1972), WHITE_DWARF_RADIUS_MU = 1 mu-dependent variant, WHITE_DWARF_RADIUS_CARRASCO2014 = 2 is based on Carrasco (2014) tables.
Parameter input type: Integer
Default value: 0
Macros: [‘WHITE_DWARF_RADIUS_NAUENBERG1972 = 0’, ‘WHITE_DWARF_RADIUS_MU = 1’, ‘WHITE_DWARF_RADIUS_CARRASCO2014 = 2’]

Parameter: cbdisc_mass_loss_inner_viscous_accretion_method
Description: Chooses where the mass that is accreted from the inner edge of a circumbinary disc goes, i.e. to which star. 0 = Young and Clarke 2015, 1 = Gerosa et al 2015, 2 = 50:50 (i.e. not dependence on mass).
Parameter input type: Integer
Default value: 0
Macros: [‘CBDISC_MASS_LOSS_INNER_VISCOUS_ACCRETION_METHOD_YOUNG_CLARKE_2015 = 0’, ‘CBDISC_MASS_LOSS_INNER_VISCOUS_ACCRETION_METHOD_GEROSA_2015 = 1’, ‘CBDISC_MASS_LOSS_INNER_VISCOUS_ACCRETION_METHOD_EQUAL = 2’, ‘CBDISC_MASS_LOSS_INNER_VISCOUS_ACCRETION_METHOD_NONE = 3’]

Parameter: cbdisc_inner_edge_stripping
Description: If True, allow inner edge mass stripping.
Parameter input type: True|False
Default value: True

Parameter: cbdisc_end_evolution_after_disc
Description: If True, stop evolution when a disc evaporates.
Parameter input type: True|False
Default value: False

Parameter: cbdisc_no_wind_if_cbdisc
Description: If True, disable stellar winds when there is a circumbinary disc.
Parameter input type: True|False
Default value: False

Parameter: cbdisc_outer_edge_stripping
Description: If True, allow outer edge mass stripping.
Parameter input type: True|False
Default value: True

Parameter: disc_n_monte_carlo_guesses
Description: Number of monte carlo guesses to try in the disc solver if the normal list of guesses fails (0).
Parameter input type: Integer
Default value: 0

Parameter: disc_log
Description: If 1, turn on the disc log. Requires DISC_LOG to be defined on build.
Parameter input type: Integer
Default value: 0
Macros: [‘DISC_LOG_LEVEL_NONE = 0’, ‘DISC_LOG_LEVEL_NORMAL = 1’, ‘DISC_LOG_LEVEL_SUBTIMESTEP = 2’, ‘DISC_LOG_LEVEL_NORMAL_FIRST_DISC_ONLY = -1’, ‘DISC_LOG_LEVEL_SUBTIMESTEP_FIRST_DISC_ONLY = -2’]

Parameter: disc_log2d
Description: If 1, turn on the 2d disc log. Requires DISC_LOG to be defined on build.
Parameter input type: Integer
Default value: 0
Macros: [‘DISC_LOG_LEVEL_NONE = 0’, ‘DISC_LOG_LEVEL_NORMAL = 1’, ‘DISC_LOG_LEVEL_SUBTIMESTEP = 2’, ‘DISC_LOG_LEVEL_NORMAL_FIRST_DISC_ONLY = -1’, ‘DISC_LOG_LEVEL_SUBTIMESTEP_FIRST_DISC_ONLY = -2’]

Parameter: disc_log_dt
Description: If non-zero, only allows disc log output every disc_log_dt Myr.
Parameter input type: Float
Default value: 0

Parameter: disc_log_directory
Description: Directory into which disc logging is sent (must exist!).
Parameter input type: String
Default value: /tmp/
Extra: /tmp/

Parameter: post_ce_adaptive_menv
Description: If TRUE, and if post_ce_objects_have_envelopes is TRUE, then the envelope mass of a post-CE star is such that it sits just inside its Roche lobe. If FALSE then a fixed (thin) envelope mass is applied that depends on the stellar type (see macros POST_CE_ENVELOPE_DM_GB, POST_CE_ENVELOPE_DM_EAGB and POST_CE_ENVELOPE_DM_TPAGB).
Parameter input type: True|False
Default value: False

Parameter: post_ce_objects_have_envelopes
Description: If TRUE then post-common-envelope objects have thin envelopes. You need this if you are to have post-CE post-AGB stars. Note that this may be unstable, i.e. you may end up having many CEEs. The mass in the envelope is controlled by post_ce_adaptive_menv. TRUE by default.
Parameter input type: True|False
Default value: False

Parameter: PN_comenv_transition_time
Description: post-common envelope transition time in years (1e2).  This is the time taken to move from CEE ejection to Teff > 30e4 K. Hall et al. (2013) suggest ~100 years.
Parameter input type: Float
Default value: 100

Parameter: minimum_time_between_PNe
Description: The minimum time (Myr) between planetary nebula detections. This prevents multiple, fast common envelopes triggering two PNe (0.1).
Parameter input type: Float
Default value: 0.1

Parameter: PN_Hall_fading_time_algorithm
Description: In stars with low mass (<0.45Msun) cores, you can choose to set the PN fading time to either the minimum (PN_HALL_FADING_TIME_ALGORITHM_MINIMUM) or maximum (PN_HALL_FADING_TIME_ALGORITHM_MAXIMUM) as shown in Fig. 6 of Hall et al. (2013).
Parameter input type: Integer
Default value: 0
Macros: [‘PN_HALL_FADING_TIME_ALGORITHM_MINIMUM = 0’, ‘PN_HALL_FADING_TIME_ALGORITHM_MAXIMUM = 1’]

Parameter: PPN_envelope_mass
Description: Desired pre-planetary nebula (post-AGB) envelope mass.
Parameter input type: Float
Default value: 0.01

Parameter: cbdisc_eccentricity_pumping_method
Description: Select from various eccentricity-pumping methods when there is a circumbinary disc. Requires DISCS. 0 = off.
Parameter input type: Integer
Default value: 1
Macros: [‘CBDISC_ECCENTRICITY_PUMPING_NONE = 0’, ‘CBDISC_ECCENTRICITY_PUMPING_DERMINE = 1’]

Parameter: cbdisc_viscous_photoevaporative_coupling
Description: Set to 1 to turn on viscous-photoevaporative coupling in circumbinary discs. Requires DISCS. 0 = CBDISC_VISCOUS_PHOTOEVAPORATIVE_COUPLING_NONE = off, 1 = CBDISC_VISCOUS_PHOTOEVAPORATIVE_COUPLING_INSTANT instant, 2 = CBDISC_VISCOUS_PHOTOEVAPORATIVE_COUPLING_VISCOUS slow, viscous wind.
Parameter input type: Integer
Default value: 1
Macros: [‘CBDISC_VISCOUS_PHOTOEVAPORATIVE_COUPLING_NONE = 0’, ‘CBDISC_VISCOUS_PHOTOEVAPORATIVE_COUPLING_INSTANT = 1’, ‘CBDISC_VISCOUS_PHOTOEVAPORATIVE_COUPLING_VISCOUS = 2’]

Parameter: cbdisc_inner_edge_stripping_timescale
Description: Defines the timescale for mass loss from by inner edge stripping. 0 = instant, 1 = very long, 2 = viscous at Revap_in, 3 = orbital at Revap_in.
Parameter input type: Integer
Default value: 1
Macros: [‘DISC_STRIPPING_TIMESCALE_INSTANT = 1’, ‘DISC_STRIPPING_TIMESCALE_INFINITE = 2’, ‘DISC_STRIPPING_TIMESCALE_VISCOUS = 3’, ‘DISC_STRIPPING_TIMESCALE_ORBIT = 4’]

Parameter: cbdisc_outer_edge_stripping_timescale
Description: Defines the timescale for mass loss from by outer edge stripping. 0 = instant, 1 = very long, 2 = viscous at Revap_in, 3 = orbital at Revap_out.
Parameter input type: Integer
Default value: 1
Macros: [‘DISC_STRIPPING_TIMESCALE_INSTANT = 1’, ‘DISC_STRIPPING_TIMESCALE_INFINITE = 2’, ‘DISC_STRIPPING_TIMESCALE_VISCOUS = 3’, ‘DISC_STRIPPING_TIMESCALE_ORBIT = 4’]

Parameter: cbdisc_viscous_L2_coupling
Description: Set to 1 to turn on viscous-L2-loss coupling in circumbinary discs. Requires DISCS. 0 = off.
Parameter input type: Integer
Default value: 1

Parameter: gravitational_radiation_model
Description: Model for gravitational radiation from the system. 0=Hurley et al 2002 (Landau and Lifshitz 1951). 1 = as 0 but only when there is no RLOF. 2 = none.
Parameter input type: Integer
Default value: 0
Macros: [‘GRAVITATIONAL_RADIATION_BSE = 0’, ‘GRAVITATIONAL_RADIATION_BSE_WHEN_NO_RLOF = 1’, ‘GRAVITATIONAL_RADIATION_NONE = 2’, ‘GRAVITATIONAL_RADIATION_LANDAU_LIFSHITZ = 3’, ‘GRAVITATIONAL_RADIATION_LANDAU_LIFSHITZ_WHEN_NO_RLOF = 4’]

Parameter: nova_irradiation_multiplier
Description: Multiplier for nova-radiative induced mass loss. (Shara+1986)
Parameter input type: Float
Default value: 0

Parameter: gravitational_radiation_modulator_J
Description: Modulator for gravitational wave radiation angular momentum loss rate (1.0).
Parameter input type: Float
Default value: 1

Parameter: gravitational_radiation_modulator_e
Description: Modulator for gravitational wave radiation eccentricity pumping rate (1.0).
Parameter input type: Float
Default value: 1

Parameter: nova_faml_multiplier
Description: Nova friction-induced angular momentum loss multiplier. (Shara+1986)
Parameter input type: Float
Default value: 0

Parameter: RLOF_angular_momentum_transfer_model
Description: Choose angular momentum transfer model in RLOF. 0=BSE (with discs), 1=conservative
Parameter input type: Integer
Default value: 0
Macros: [‘RLOF_ANGULAR_MOMENTUM_TRANSFER_MODEL_BSE = 0’, ‘RLOF_ANGULAR_MOMENTUM_TRANSFER_MODEL_CONSERVATIVE = 1’]

Parameter: post_SN_orbit_method
Description: Method by which the post-SN orbit is calculated. 0=BSE, 1=Tauris&Taken 1998.
Parameter input type: Integer
Default value: 1
Macros: [‘POST_SN_ORBIT_BSE = 0’, ‘POST_SN_ORBIT_TT98 = 1’]

Parameter: multiplicity
Description: Multiplicity: 1=single star, 2=binary, 3=triple, 4=quadruple.
Parameter input type: Integer
Default value: 0

Parameter: accretion_limit_eddington_steady_multiplier
Description: Steady accretion is limited by the Eddington instability, with limiting rate given by the accretion_limit_eddington_steady_multiplier * the normal (spherically symmetric) Eddington rate. This is known in the trade as the Eddington factor, and anything greater than 1.0 potentially gives you super-Eddington accretion.
Parameter input type: Float
Default value: 1

Parameter: accretion_limit_eddington_LMMS_multiplier
Description: Accretion from a low-mass, convective, main_sequence star is limited by the Eddington instability, with limiting rate given by the accretion_limit_eddington_LMMS_multiplier * the normal (spherically symmetric) Eddington rate. This is known in the trade as the Eddington factor, and anything greater than 1.0 potentially gives you super-Eddington accretion.
Parameter input type: Float
Default value: 1

Parameter: accretion_limit_eddington_WD_to_remnant_multiplier
Description: Accretion from a WD onto a remnant star (e.g. another white dwarf, neutron star or black hole) is limited by the Eddington instability, with limiting rate given by the accretion_limit_eddington_WD_to_remnant_multiplier * the normal (spherically symmetric) Eddington rate. This is known in the trade as the Eddington factor, and anything greater than 1.0 potentially gives you super-Eddington accretion.
Parameter input type: Float
Default value: -1

Parameter: accretion_limit_thermal_multiplier
Description: Mass transfer onto a MS, HG or CHeB star is limited by the accretor’s thermal rate times this multiplier.
Parameter input type: Float
Default value: 1

Parameter: accretion_limit_dynamical_multiplier
Description: Mass transfer is limited by the accretor’s dynamical rate times this multiplier.
Parameter input type: Float
Default value: 1

Parameter: donor_limit_envelope_multiplier
Description: Mass transfer by RLOF is limited by this fraction of the donor’s envelope mass per timestep
Parameter input type: Float
Default value: 0

Parameter: donor_limit_thermal_multiplier
Description: Mass transfer by RLOF is limited by the accretor’s thermal rate times this multiplier.
Parameter input type: Float
Default value: 1

Parameter: donor_limit_dynamical_multiplier
Description: Mass transfer by RLOF is limited by the donor’s dynamical rate times this multiplier.
Parameter input type: Float
Default value: 1

Parameter: Bondi_Hoyle_accretion_factor
Description: Wind accretion rate, as calculated by the Bondi-Hoyle-Littleton formula, multiplcation factor. Hurley et al 2002 use 1.5, which is the default.
Parameter input type: Float
Default value: 1.5

Parameter: tidal_strength_factor
Description: A modulator for the tidal strength. If this factor > 1 then tides are stronger, i.e. tidal timescales are reduced.
Parameter input type: Float
Default value: 1

Parameter: hachisu_qcrit
Description: Critical q=Maccretor/Mdonor above which Hachisu’s disk wind turns on.
Parameter input type: Float
Default value: 1.15
Macros: [‘HACHISU_IGNORE_QCRIT = -1’]

Parameter: hachisu_disk_wind
Description: Set to True to turn on Hachisu’s disk wind when material accretes too fast onto a white dwarf. This helps to make more SNeIa. See also hachisu_qcrit.
Parameter input type: True|False
Default value: False

Parameter: mass_accretion_for_eld
Description: The mass that must be accreted onto a COWD for it to ignite as an edge-lit detonation SNIa.
Parameter input type: Float
Default value: 0.15

Parameter: WDWD_merger_algorithm
Description: Algorithm to be used when merging two white dwarfs. 0 = Hurley et al. (2002), 1 = Perets+ (2019), 2 = Chen+ (2016, todo)
Parameter input type: Integer
Default value: 0
Macros: [‘WDWD_MERGER_ALGORITHM_BSE = 0’, ‘WDWD_MERGER_ALGORITHM_PERETS2019 = 1’, ‘WDWD_MERGER_ALGORITHM_CHEN2016 = 2’]

Parameter: type_Ia_MCh_supernova_algorithm
Description: Algorithm to be used when calculating type Ia yields from Chandrasekhar-mass exploders. 0 = DD7 (Iwamoto 1999), 1 = Seitenzahl 2013 3D hydro yields (you must also set Seitenzahl2013_model)
Parameter input type: Integer
Default value: 0
Macros: [‘TYPE_IA_MCH_SUPERNOVA_ALGORITHM_DD2 = 0’, ‘TYPE_IA_MCH_SUPERNOVA_ALGORITHM_SEITENZAHL2013 = 1’, ‘TYPE_IA_MCH_SUPERNOVA_ALGORITHM_SEITENZAHL2013_AUTOMATIC = 2’]

Parameter: Seitenzahl2013_model
Description: Which of Seitenzahl et al. 2013’s models to use? One of N1,N3,N5,N10,N20,N40,N100L,N100,N100H,N150,N200,N300C,N1600,N1600C,N100_Z0.5,N100_Z0.1,N100_Z0.01 (defaults to N100).
Parameter input type: String
Default value: N100
Extra: N1

Parameter: type_Ia_sub_MCh_supernova_algorithm
Description: Algorithm to be used when calculating type Ia yields from sub-Chandrasekhar-mass exploders. (Currently unused.)
Parameter input type: Integer
Default value: 0
Macros: [‘TYPE_IA_SUB_MCH_SUPERNOVA_ALGORITHM_LIVNE_ARNETT_1995 = 0’]

Parameter: max_HeWD_mass
Description: The maximum mass a HeWD can have before it ignites helium (0.7).
Parameter input type: Float
Default value: 0.7

Parameter: merger_mass_loss_fraction
Description: Fraction of the total mass which is lost when stars merge.
Parameter input type: Float
Default value: 0

Parameter: merger_angular_momentum_factor
Description: When two stars merge the resulting single star retains a fraction of the total system angular momentum (or the critical spin angular momentum, if it is smaller) multiplied by this factor.
Parameter input type: Float
Default value: 1

Parameter: wind_angular_momentum_loss
Description: Prescription for losing angular momentum in a stellar wind. 0=Hurley et al 2002 (‘Tout’) prescription, 1=lw i.e. a factor multiplying the specific orbital angular momentum, 2=lw hybrid for fast winds. Set wind_djorb_fac to the desired factor..
Parameter input type: Integer
Default value: 0
Macros: [‘WIND_ANGMOM_LOSS_BSE = 0’, ‘WIND_ANGMOM_LOSS_LW = 1’, ‘WIND_ANGMOM_LOSS_LW_HYBRID = 2’, ‘WIND_ANGMOM_LOSS_SPHERICALLY_SYMMETRIC = 3’]

Parameter: wind_djorb_fac
Description: Factor multiplying angular momentum loss in a stellar wind when wind_angular_momentum_loss=0 (the Tout/Hurley et al 2002 prescription). See wind_angular_momentum_loss.
Parameter input type: Float
Default value: 1

Parameter: lw
Description: Factor multiplying angular momentum loss in a stellar wind when wind_angular_momentum_loss=1,2 (the ‘lw’ prescription). See wind_angular_momentum_loss.
Parameter input type: Float
Default value: 1

Parameter: VW93_EAGB_wind_speed
Description: Activate this to use Vassiliadis and Wood (1993) wind speed during the EAGB.
Parameter input type: True|False
Default value: False

Parameter: VW93_TPAGB_wind_speed
Description: Activate this to use Vassiliadis and Wood (1993) wind speed during the EAGB.
Parameter input type: True|False
Default value: False

Parameter: use_periastron_Roche_radius
Description: Set this to True to use the Roche lobe radius at periastron, rather than (the default to) assume a circular orbit. This will be useful one day when we treat RLOF in eccentric orbits properly, hopefully.
Parameter input type: True|False
Default value: False

Parameter: qcrit_LMMS
Description: Apply critical q=Mdonor/Maccretor value for low-mass main sequence stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 0.6944
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_MS
Description: Apply critical q=Mdonor/Maccretor value for (non-low mass) main sequence stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 1.6
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_HG
Description: Apply critical q=Mdonor/Maccretor value for Hertzsprung gap stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 4
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_GB
Description: Apply critical q=Mdonor/Maccretor value for first red giant branch stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: -1
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_CHeB
Description: Apply critical q=Mdonor/Maccretor value for core helium burning stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 3
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_EAGB
Description: Apply critical q=Mdonor/Maccretor value for early-AGB stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: -1
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_TPAGB
Description: Apply critical q=Mdonor/Maccretor value for TP-AGB stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: -1
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_HeMS
Description: Apply critical q=Mdonor/Maccretor value for helium main sequence stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 3
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_HeHG
Description: Apply critical q=Mdonor/Maccretor value for helium Hertzsprung gap stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 4
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_HeGB
Description: Apply critical q=Mdonor/Maccretor value for helium red giant stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 0.78125
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_HeWD
Description: Apply critical q=Mdonor/Maccretor value for helium white dwarf stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 3
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_COWD
Description: Apply critical q=Mdonor/Maccretor value for carbon-oxygen white dwarf stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 3
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_ONeWD
Description: Apply critical q=Mdonor/Maccretor value for oxygen-neon white dwarf stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 3
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_NS
Description: Apply critical q=Mdonor/Maccretor value for neutron stars to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 3
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_BH
Description: Apply critical q=Mdonor/Maccretor value for black holes to determine the stability of Roche-lobe overflow for non-degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 3
Macros: [‘QCRIT_BSE = -1’, ‘QCRIT_HJELLMING_WEBBINK = -2’, ‘QCRIT_Q_NO_COMENV = -3’, ‘QCRIT_CHEN_HAN_TABLE = -4’, ‘QCRIT_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GE2015 = -6’, ‘QCRIT_VOS2018 = -7’, ‘QCRIT_TEMMINK2021 = -8’, ‘QCRIT_GB_BSE = -1’, ‘QCRIT_GB_HJELLMING_WEBBINK = -2’, ‘QCRIT_GB_Q_NO_COMENV = -3’, ‘QCRIT_GB_CHEN_HAN_TABLE = -4’, ‘QCRIT_GB_CHEN_HAN_FORMULA = -5’, ‘QCRIT_GB_GE2015 = -6’, ‘QCRIT_GB_VOS2018 = -7’, ‘QCRIT_GB_TEMMINK2021 = -8’]

Parameter: qcrit_degenerate_LMMS
Description: Apply critical q=Mdonor/Maccretor value for (low mass) main sequence stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 1

Parameter: qcrit_degenerate_MS
Description: Apply critical q=Mdonor/Maccretor value for (non-low mass) main sequence stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 1

Parameter: qcrit_degenerate_HG
Description: Apply critical q=Mdonor/Maccretor value for Hertzsprung gap stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 4.7619

Parameter: qcrit_degenerate_GB
Description: Apply critical q=Mdonor/Maccretor value for first red giant branch stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 1.15

Parameter: qcrit_degenerate_CHeB
Description: Apply critical q=Mdonor/Maccretor value for core helium burning stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 3

Parameter: qcrit_degenerate_EAGB
Description: Apply critical q=Mdonor/Maccretor value for early-AGB stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 1.15

Parameter: qcrit_degenerate_TPAGB
Description: Apply critical q=Mdonor/Maccretor value for TP-AGB stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 1.15

Parameter: qcrit_degenerate_HeMS
Description: Apply critical q=Mdonor/Maccretor value for helium main sequence stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 3

Parameter: qcrit_degenerate_HeHG
Description: Apply critical q=Mdonor/Maccretor value for helium Hertzsprung gap stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 4.7619

Parameter: qcrit_degenerate_HeGB
Description: Apply critical q=Mdonor/Maccretor value for helium red giant stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 1.15

Parameter: qcrit_degenerate_HeWD
Description: Apply critical q=Mdonor/Maccretor value for helium white dwarf stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 0.625

Parameter: qcrit_degenerate_COWD
Description: Apply critical q=Mdonor/Maccretor value for carbon-oxygen white dwarf stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 0.625

Parameter: qcrit_degenerate_ONeWD
Description: Apply critical q=Mdonor/Maccretor value for oxygen-neon white dwarf stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 0.625

Parameter: qcrit_degenerate_NS
Description: Apply critical q=Mdonor/Maccretor value for neutron stars to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 0.625

Parameter: qcrit_degenerate_BH
Description: Apply critical q=Mdonor/Maccretor value for black holes to determine the stability of Roche-lobe overflow for degenerate accretors. See also qcrits_*, qcrits_degenerate_*.
Parameter input type: Float
Default value: 0.625

Parameter: mass_for_Hestar_Ia_upper
Description: Only helium stars below this mass can explode as SNIa. Default is zero, i.e. it never happens. See also mass_for_Hestar_Ia_lower.
Parameter input type: Float
Default value: 0

Parameter: mass_for_Hestar_Ia_lower
Description: Only helium stars above this mass can explode as SNIa. Default is zero, i.e. it never happens. See also mass_for_Hestar_Ia_upper.
Parameter input type: Float
Default value: 0

Parameter: alphaCB
Description: Circumbinary disk viscosity parameter, alpha.
Parameter input type: Float
Default value: NULL

Parameter: minimum_donor_menv_for_comenv
Description: Minimum donor envelope mass for common envelope evolution to be triggered (Msun). Default 0.
Parameter input type: Float
Default value: 0

Parameter: comenv_prescription
Description: Use this to choose which common envelope prescription you should use. 0=Hurley et al 2002 (based on the Paczyński energy model) or 1=Nelemans and Tout (angular momentum model). See also alpha_ce, comenv_ms_accretion_mass, comenv_ms_accretion_fraction, comenv_ns_accretion_fraction, comenv_ns_accretion_mass, nelemans_gamma, nelemans_minq, nelemans_max_frac_j_change, nelemans_n_comenvs, lambda_ce, lambda_ionisation.
Parameter input type: Integer
Default value: 0
Macros: [‘COMENV_UNDEF = -1’, ‘COMENV_BSE = 0’, ‘COMENV_NELEMANS_TOUT = 1’, ‘COMENV_NANDEZ2016 = 2’]

Parameter: comenv_prescription%d
Description: Use this to choose which common envelope prescription you should use. 0=Hurley et al 2002 (based on the Paczyński energy model) or 1=Nelemans and Tout (angular momentum model). See also alpha_ce, comenv_ms_accretion_mass, comenv_ms_accretion_fraction, comenv_ns_accretion_fraction, comenv_ns_accretion_mass, nelemans_gamma, nelemans_minq, nelemans_max_frac_j_change, nelemans_n_comenvs, lambda_ce, lambda_ionisation.
Parameter input type: Int(scanf)
Default value: NULL
Macros: [‘COMENV_UNDEF = -1’, ‘COMENV_BSE = 0’, ‘COMENV_NELEMANS_TOUT = 1’, ‘COMENV_NANDEZ2016 = 2’]

Parameter: comenv_ejection_spin_method
Description: When a common envelope is ejected, we need to decide how fast the stars are left spinning. COMENV_EJECTION_SPIN_METHOD_DO_NOTHING (0) is the default, this just leaves the stars/stellar cores spinning with the same spin rate (omega = angular velocity) with which they entered the common envelope phase. COMENV_EJECTION_SPIN_METHOD_SYCHRONIZE instead tidally synchronizes the stars with their new orbital angular velocity.
Parameter input type: Integer
Default value: 0
Macros: [‘COMENV_EJECTION_SPIN_METHOD_DO_NOTHING = 0’, ‘COMENV_EJECTION_SPIN_METHOD_SYNCHRONIZE = 1’]

Parameter: comenv_merger_spin_method
Description: When a common envelope binary merges, we need to decide how fast the resulting single star is left spinning. COMENV_MERGER_SPIN_METHOD_SPECIFIC (0) is the default, this preserves angular momentum but limits the specific angular momentum of the merged star to the specific angular momentum of the system at the onset of common envelope evolution. COMENV_MERGER_SPIN_METHOD_CONSERVE_ANGMOM (1) sets the merger’s angular momentum to be that of the system at the onset of common envelope evolution (which means the star may be rotating supercritically). COMENV_MERGER_SPIN_METHOD_CONSERVE_OMEGA (2) sets the spin rate (angular frequency = omega) of the merged star to be that of the orbit just at the onset of common envelope evolution.
Parameter input type: Integer
Default value: 0
Macros: [‘COMENV_MERGER_SPIN_METHOD_SPECIFIC = 0’, ‘COMENV_MERGER_SPIN_METHOD_CONSERVE_ANGMOM = 1’, ‘COMENV_MERGER_SPIN_METHOD_CONSERVE_OMEGA = 2’, ‘COMENV_MERGER_SPIN_METHOD_BREAKUP = 3’]

Parameter: comenv_ms_accretion_mass
Description: Experimental. During common envelope evolution, a main sequence star may accrete some of the envelope’s mass. Requires COMENV_MS_ACCRETION. See also comenv_ms_accretion_fraction.
Parameter input type: Float
Default value: NULL

Parameter: comenv_ms_accretion_fraction
Description: Experimental. During common envelope evolution, a main sequence may accrete a fraction of the envelope’s mass. Requires COMENV_MS_ACCRETION. See also comenv_ms_accretion_mass.
Parameter input type: Float
Default value: NULL

Parameter: comenv_ns_accretion_mass
Description: Experimental. During common envelope evolution, a neutron star may accrete some of the envelope’s mass. Requires COMENV_NS_ACCRETION. See also comenv_ns_accretion_fraction.
Parameter input type: Float
Default value: NULL

Parameter: comenv_ns_accretion_fraction
Description: Experimental. During common envelope evolution, a neutron star may accrete a fraction of the envelope’s mass. Requires COMENV_NS_ACCRETION. See also comenv_ns_accretion_mass.
Parameter input type: Float
Default value: NULL

Parameter: alpha_ce
Description: Common envelope energy formalism parameter. A fraction alpha of the orbital energy is used to eject the envelope. See Hurley et al 2002 for details.
Parameter input type: Float
Default value: 1

Parameter: alpha_ce%d
Description: Common envelope energy formalism parameter. A fraction alpha of the orbital energy is used to eject the envelope. See Hurley et al 2002 for details.
Parameter input type: Float(scanf)
Default value: NULL

Parameter: lambda_ce
Description: Common envelope parameter. The binding energy of the common envelope is G*M*Menv/(lambda*R). Typically this is taken to be 0.5, but if set to -1 binary_c uses the Dewi and Tauris fits instead, -2 uses the formalism of Wang, Jia and Li (2016) and if -3 then a polytropic formalism is used (see also comenv_splitmass).
Parameter input type: Float
Default value: 0.5
Macros: [‘LAMBDA_CE_DEWI_TAURIS = -1’, ‘LAMBDA_CE_WANG_2016 = -2’, ‘LAMBDA_CE_POLYTROPE = -3’, ‘LAMBDA_CE_KLENCKI_2020 = -4’]

Parameter: lambda_ce%d
Description: Common envelope parameter. The binding energy of the common envelope is G*M*Menv/(lambda*R). Typically this is taken to be 0.5, but if set to -1 binary_c uses the Dewi and Tauris fits instead, -2 uses the formalism of Wang, Jia and Li (2016) and if -3 then a polytropic formalism is used (see also comenv_splitmass).
Parameter input type: Float(scanf)
Default value: NULL

Parameter: comenv_splitmass
Description: When lambda_ce=-2, the envelope binding energy, lambda, is calculated using a polytropic formalism. The comenv_splitmass defines the point, in the units of the core mass, above which material is ejected.
Parameter input type: Float
Default value: NULL

Parameter: nelemans_recalc_eccentricity
Description: If True, recalculate the eccentricity after angular momentum is removed.
Parameter input type: True|False
Default value: False

Parameter: comenv_post_eccentricity
Description: Eccentricity remaining after common envelope ejection.
Parameter input type: Float
Default value: 1e-05

Parameter: nelemans_gamma
Description: Set the fraction of the orbital specific angular momentum that is used to eject the common envelope according to the Nelemans and Tout prescription. See also nelemans_minq, nelemans_max_frac_j_change, nelemans_n_comenvs.
Parameter input type: Float
Default value: 1.75

Parameter: nelemans_minq
Description: Only activate the Nelemans and Tout common envelope prescription for q>nelemans_minq. See also nelemans_gamma, nelemans_max_frac_j_change, nelemans_n_comenvs.
Parameter input type: Float
Default value: 0.2

Parameter: nelemans_max_frac_j_change
Description: Maximum fractional angular momentum change in the Nelemans and Tout common envelope prescription. See also nelemans_gamma, nelemans_minq, nelemans_n_comenvs.
Parameter input type: Float
Default value: 1

Parameter: nelemans_n_comenvs
Description: Set the maximum number of common envelope ejections allowed to follow the Nelemans and Tout prescription, after which the standard alpha prescription is used.
Parameter input type: Integer
Default value: 1

Parameter: lambda_ionisation
Description: A fraction lambda_ionisation of the recombination energy in the common envelope goes into ejecting the envelope. This is usually 0.0, but a positive value can make a big difference to the outcome of common envelope evolution.
Parameter input type: Float
Default value: 0.5

Parameter: lambda_ionisation%d
Description: A fraction lambda_ionisation of the recombination energy in the common envelope goes into ejecting the envelope. This is usually 0.0, but a positive value can make a big difference to the outcome of common envelope evolution.
Parameter input type: Float(scanf)
Default value: NULL

Parameter: lambda_enthalpy
Description: A fraction of the enthalpy to be included in the common envelope evolution binding energy. Only used for the Wang 2016 prescription (so far).
Parameter input type: Float
Default value: 0

Parameter: lambda_enthalpy%d
Description: A fraction of the enthalpy to be included in the common envelope evolution binding energy. Only used for the Wang 2016 prescription (so far).
Parameter input type: Float(scanf)
Default value: NULL

Parameter: cbdisc_albedo
Description: Circumbinary-disc albedo. Requires DISCS.
Parameter input type: Float
Default value: 0

Parameter: cbdisc_gamma
Description: Circumbinary disc gamma (equation of state) parameter. Requires DISCS.
Parameter input type: Float
Default value: 1.4

Parameter: cbdisc_alpha
Description: Circumbinary disc alpha (viscosity) parameter. Requires DISCS.
Parameter input type: Float
Default value: 0.001

Parameter: cbdisc_kappa
Description: Circumbinary disc kappa (opacity) parameter. Requires DISCS.
Parameter input type: Float
Default value: 0.01

Parameter: cbdisc_minimum_evaporation_timescale
Description: Circumbinary disc minimum evaporation timescale (years). If (slow, not edge stripped) mass loss would evaporate the disc on a timescale less than this, simply evaporate the disc immediated. Usually set to 1y, ignore if zero. Requires DISCS.
Parameter input type: Float
Default value: 1

Parameter: cbdisc_torquef
Description: Circumbinary disc binary torque multiplier. Requires DISCS.
Parameter input type: Float
Default value: 0.001

Parameter: cbdisc_max_lifetime
Description: Circumbinary disc maximum lifetime (years, ignored if 0). Requires DISCS.
Parameter input type: Float
Default value: 1e+06

Parameter: cbdisc_init_dM
Description: On cbdisc start, reduce mass by a fraction dM if it won’t converge. Requires DISCS.
Parameter input type: Float
Default value: 0.1

Parameter: cbdisc_init_dJdM
Description: On cbdisc start, reduce angular momentum by a fraction dJ/dM*dM if it won’t converge. Requires DISCS.
Parameter input type: Float
Default value: 0.5

Parameter: cbdisc_mass_loss_constant_rate
Description: Circumbinary disc constant mass loss rate (Msun/year). Requires DISCS.
Parameter input type: Float
Default value: 0

Parameter: cbdisc_mass_loss_FUV_multiplier
Description: Circumbinary disc FUV mass loss rate multiplier (no units). Requires DISCS.
Parameter input type: Float
Default value: 1

Parameter: cbdisc_mass_loss_Xray_multiplier
Description: Circumbinary disc X-ray mass loss rate multiplier (no units). Requires DISCS.
Parameter input type: Float
Default value: 1

Parameter: cbdisc_mass_loss_ISM_ram_pressure_multiplier
Description: Circumbinary disc interstellar medium ram pressure stripping mass loss rate multiplier (no units). Requires DISCS.
Parameter input type: Float
Default value: 1

Parameter: cbdisc_mass_loss_ISM_pressure
Description: Circumbinary disc interstellar medium ram pressure in units of Boltzmann constant per Kelvin (I think…). Requires DISCS. Typically 3000.0. See e.g. http://www.astronomy.ohio-state.edu/~pogge/Ast871/Notes/Intro.pdf page 15 or https://arxiv.org/pdf/0902.0820.pdf Fig. 1 (left panel).
Parameter input type: Float
Default value: 3000

Parameter: cbdisc_mass_loss_inner_viscous_multiplier
Description: Circumbinary disc inner edge viscous mass loss rate multiplier (no units). Requires DISCS.
Parameter input type: Float
Default value: 1

Parameter: cbdisc_mass_loss_inner_viscous_angular_momentum_multiplier
Description: Circumbinary disc inner edge viscous angular momentum multiplier (no units). The inner edge angular momentum Requires DISCS.
Parameter input type: Float
Default value: 1

Parameter: cbdisc_resonance_multiplier
Description: Circumbinary disc resonant interaction multiplier, affects eccentricity pumping and angular momentum rates. Requires DISCS.
Parameter input type: Float
Default value: 1

Parameter: cbdisc_resonance_damping
Description: Circumbinary disc resonant interaction damping: should be on (True) to damp the l=1, m=2 resonance when the disc inner edge lies outside the resonance location. Requires DISCS.
Parameter input type: True|False
Default value: True

Parameter: cbdisc_fail_ring_inside_separation
Description: If True, while converging on a structure, circumbinary discs with Rring < the binary separation are immediately failed.
Parameter input type: True|False
Default value: False

Parameter: cbdisc_mass_loss_inner_L2_cross_multiplier
Description: Circumbinary disc inner edge L2-crossing mass loss rate multiplier (no units). Requires DISCS.
Parameter input type: Float
Default value: 1

Parameter: cbdisc_minimum_luminosity
Description: Circumbinary disc minimum luminosity. If the disc becomes dimmer than this, the disc is evaporated instantly. Requires DISCS.
Parameter input type: Float
Default value: 0

Parameter: cbdisc_minimum_mass
Description: Circumbinary disc minimum mass. If the disc becomes less massive than this, the disc is evaporated instantly. Requires DISCS.
Parameter input type: Float
Default value: 1e-06

Parameter: cbdisc_minimum_fRing
Description: Circumbinary disc minimum fRing. If the disc becomes a ring, and fRing = |Rout/Rin-1| < this value (and this value is non-zero), the disc is evaporated instantly. Requires DISCS.
Parameter input type: Float
Default value: 0.2

Parameter: comenv_disc_angmom_fraction
Description: If >0 Fraction of the common envelope’s angular momentum that goes into the circumbinary disc. If -1 then uses the moments of inertia to calculate (deprecated), if -2 use the common envelope’s specific angular momentum, if -3 uses the L2 point at the end of the common envelope to set the angular momentum. Requires DISCS and DISCS_CIRCUMBINARY_FROM_COMENV.
Parameter input type: Float
Default value: 0

Parameter: comenv_disc_mass_fraction
Description: Fraction of the common envelope’s mass that goes into the circumbinary disc. Requires DISCS and DISCS_CIRCUMBINARY_FROM_COMENV.
Parameter input type: Float
Default value: 0

Parameter: wind_disc_angmom_fraction
Description: If >0 Fraction of the wind envelope’s angular momentum that goes into the circumbinary disc. If -1 then uses the L2 point’s specific angular momentum. Requires DISCS and DISCS_CIRCUMBINARY_FROM_WIND.
Parameter input type: Float
Default value: 0

Parameter: wind_disc_mass_fraction
Description: Fraction of the stellar wind’s mass that goes into the circumbinary disc. Requires DISCS and DISCS_CIRCUMBINARY_FROM_WIND.
Parameter input type: Float
Default value: 0

Parameter: WRLOF_method
Description: Choose whether and how to apply wind-Roche-lobe-overflow. 0=none, 1=q-dependent, 2=quadratic See Abate et al 2013/14 for details. Requires WRLOF_MASS_TRANSFER.
Parameter input type: Integer
Default value: 0
Macros: [‘WRLOF_NONE = 0’, ‘WRLOF_Q_DEPENDENT = 1’, ‘WRLOF_QUADRATIC = 2’]

Parameter: minimum_timestep
Description: The minimum timestep (Myr).
Parameter input type: Float
Default value: 1e-06

Parameter: timestep_solver_factor
Description: Factor applied in timestep_limits, e.g. to prevent X changing too fast by comparing to X/dX/dt, which is usually 1 but can be higher to lengthen timesteps when using an alternative solver.
Parameter input type: Float
Default value: 1

Parameter: RLOF_mdot_factor
Description: Multiplier applied to the mass transfer rate during Roche-lobe overflow. Requires RLOF_MDOT_MODULATION.
Parameter input type: Float
Default value: 1

Parameter: RLOF_f
Description: Factor to enlarge a Roche lobe, nominally because of radiation pressure (see Dermine et al paper). Requires RLOF_RADIATION_CORRECTION.
Parameter input type: Float
Default value: NULL

Parameter: minimum_separation_for_instant_RLOF
Description: If True, instead of evolving the system just report the minimum separation (on the zero-age main sequence) that would lead to instant RLOF. Used by binary_grid. See also minimum_orbital_period_for_instant_RLOF and maximum_mass_ratio_for_instant_RLOF.
Parameter input type: True|False
Default value: False

Parameter: minimum_orbital_period_for_instant_RLOF
Description: If True, instead of evolving the system just report the minimum orbital period (on the zero-age main sequence) that would lead to instant RLOF. Used by binary_grid. See also minimum_separation_for_instant_RLOF and maximum_mass_ratio_for_instant_RLOF.
Parameter input type: True|False
Default value: False

Parameter: maximum_mass_ratio_for_instant_RLOF
Description: If True, instead of evolving the system just report the maximum mass ratio (on the zero-age main sequence) that would lead to instant RLOF, given M1 and orbital period. Used by binary_grid. See also minimum_separation_for_instant_RLOF and minimum_orbital_period_for_instant_RLOF.
Parameter input type: True|False
Default value: False

Parameter: RLOF_method
Description: Use RLOF_method to choose the algorithm you use for Roche-lobe overflow mass loss rate calculations. 0=Hurley et al 2002, 1=Adaptive (for radiative stars) R=RL method, 2=Ritter (probably broken), 3=Claeys etal 2014 variant on Hurley et al 2002.
Parameter input type: Integer
Default value: 0
Macros: [‘RLOF_METHOD_BSE = 0’, ‘RLOF_METHOD_ADAPTIVE = 1’, ‘RLOF_METHOD_RITTER = 2’, ‘RLOF_METHOD_CLAEYS = 3’, ‘RLOF_METHOD_ADAPTIVE2 = 4’]

Parameter: RLOF_interpolation_method
Description: When a star overflows its Roche lobe, it always has R>RL because of the limited time resolution of the simulation. Binary_c then uses an algorithm to get back to when R~RL (within a desired tolerance, set in RLOF_ENTRY_THRESHOLD which is usually 1.02, i.e. overflow of 2%). You can choose algorithm 0, the Hurley et al 2002 method which reverses time (i.e. uses a Newton-like scheme), or 1 to use the binary_c method which rejects a timestep (and hence does no logging on that timestep) and repeats with half the timestep until R~RL. The latter is now the default, because this means there are no negative timesteps which break various other algorithms (e.g. nucleosynthesis).
Parameter input type: Integer
Default value: 0
Macros: [‘RLOF_INTERPOLATION_BINARY_C = 0’, ‘RLOF_INTERPOLATION_BSE = 1’]

Parameter: nova_retention_fraction
Description: The mass accreted during a nova as fraction of mass transferred
Parameter input type: Float
Default value: 0.001

Parameter: beta_reverse_nova
Description: The fraction of mass ejected in a nova explosion which is accreted back onto the companion star. Set to -1 to automatically calculate based on a geometric argument, or 0 or positive to set the value.
Parameter input type: Float
Default value: 0
Macros: [‘BETA_REVERSE_NOVAE_GEOMETRY = -1’]

Parameter: WD_accretion_rate_novae_upper_limit_hydrogen_donor
Description: Upper limit of the stable mass transfer rate onto a white dwarf that leads to novae when the donor is hydrogen rich: above this rate the mass transfer leads to stable burning.
Parameter input type: Float
Default value: -1
Macros: [‘DONOR_RATE_ALGORITHM_CLAEYS2014 = -1’, ‘DONOR_RATE_ALGORITHM_BSE = -2’]

Parameter: WD_accretion_rate_novae_upper_limit_helium_donor
Description: Upper limit of the stable mass transfer rate onto a white dwarf that leads to novae when the donor is helium rich: above this rate the mass transfer leads to stable burning.
Parameter input type: Float
Default value: -1
Macros: [‘DONOR_RATE_ALGORITHM_CLAEYS2014 = -1’, ‘DONOR_RATE_ALGORITHM_BSE = -2’]

Parameter: WD_accretion_rate_novae_upper_limit_other_donor
Description: Upper limit of the stable mass transfer rate onto a white dwarf that leads to novae when the donor is neither hydrogen nor helium rich: above this rate the mass transfer leads to stable burning.
Parameter input type: Float
Default value: -1
Macros: [‘DONOR_RATE_ALGORITHM_CLAEYS2014 = -1’, ‘DONOR_RATE_ALGORITHM_BSE = -2’]

Parameter: WD_accretion_rate_new_giant_envelope_lower_limit_hydrogen_donor
Description: Lower limit of the mass transfer rate onto a white dwarf that leads to a the formation of a new giant envelope with a hydrogen-rich donor. Below this mass transfer leads to stable burning.
Parameter input type: Float
Default value: -1
Macros: [‘DONOR_RATE_ALGORITHM_CLAEYS2014 = -1’, ‘DONOR_RATE_ALGORITHM_BSE = -2’]

Parameter: WD_accretion_rate_new_giant_envelope_lower_limit_helium_donor
Description: Lower limit of the mass transfer rate onto a white dwarf that leads to a the formation of a new giant envelope with a helium-rich donor. Below this mass transfer leads to stable burning.
Parameter input type: Float
Default value: -1
Macros: [‘DONOR_RATE_ALGORITHM_CLAEYS2014 = -1’, ‘DONOR_RATE_ALGORITHM_BSE = -2’]

Parameter: WD_accretion_rate_new_giant_envelope_lower_limit_other_donor
Description: Lower limit of the mass transfer rate onto a white dwarf that leads to a the formation of a new giant envelope when the donor is neither hydrogen nor helium rich. Below this mass transfer leads to stable burning.
Parameter input type: Float
Default value: -1
Macros: [‘DONOR_RATE_ALGORITHM_CLAEYS2014 = -1’, ‘DONOR_RATE_ALGORITHM_BSE = -2’]

Parameter: CRAP_parameter
Description: Tidally enhanced mass loss parameter. See Tout and Eggleton’s paper on the subject. (Was the parameter bb).
Parameter input type: Float
Default value: 0

Parameter: individual_novae
Description: If individual_novae is True, novae are resolved such that each explosion is performed separtaely.
Parameter input type: True|False
Default value: False

Parameter: nova_timestep_accelerator_num
Description: The nova timestep is accelerated if the nova number exceeds nova_timestep_accelerator_num. If zero or negative, acceleration is off. See also nova_timestep_accelerator_index and nova_timestep_accelerator_max. Only used if individual_novae is on.
Parameter input type: Float
Default value: 100

Parameter: nova_timestep_accelerator_index
Description: The index at which the nova timestep is accelerated. A larger value gives longer timesteps. See also nova_timestep_accelerator_num and nova_timestep_accelerator_max. Only used if individual_novae is on.
Parameter input type: Float
Default value: 0.5

Parameter: nova_timestep_accelerator_max
Description: The nova timestep is accelerated by a factor that is capped at nova_timestep_accelerator_max. This parameter is ignored if it is zero or negative. See also nova_timestep_accelerator_num and nova_timestep_accelerator_index. Only used if individual_novae is on.
Parameter input type: Float
Default value: -1

Parameter: nonconservative_angmom_gamma
Description: Mass lost from the system (but NOT from a stellar wind) takes a fraction gamma of the orbital angular momentum with it. Set to -1 to take the specific angular momentum of the donor star. Set to -2 to take super-Eddington, nova and disk-wind angular momenta as if a wind from the accretor.
Parameter input type: Float
Default value: -1
Macros: [‘RLOF_NONCONSERVATIVE_GAMMA_DONOR = -1’, ‘RLOF_NONCONSERVATIVE_GAMMA_ISOTROPIC = -2’]

Parameter: max_stellar_angmom_change
Description: Maxmimum fractional change in stellar angular momentum allowed before a timestep is rejected (0.05).
Parameter input type: Float
Default value: 0.05

Section: nucsyn

Parameter: third_dup
Description: If True, enables third dredge up. Requires NUCSYN and NUCSYN_THIRD_DREDGE_UP.
Parameter input type: True|False
Default value: True

Parameter: third_dup_multiplier
Description: Usage: –third_dup_multiplier <i> <f>. Multiplies the abundance of element <i> by <f> during third dredge up.
Parameter input type: *
Default value: NULL
Extra: 1.0

Parameter: NeNaMgAl
Description: Enables NeNaMgAl reaction network. Requires NUCSYN and NUCSYN_HBB.
Parameter input type: True|False
Default value: True
Extra: Ignore

Parameter: nucsyn_network%d
Description: Usage: –nucsyn_network%d <boolean>. Turn a nuclear network on or off.
Parameter input type: Boolean(scanf)
Default value: NULL

Parameter: nucsyn_network_error%d
Description: Usage: –nucsyn_network_error%d <f>. Threshold error in nuclear network solver for network %d.
Parameter input type: Float(scanf)
Default value: NULL

Parameter: nucreacmult%d
Description: Usage: –nucreacmult%d <f>. Multiply nuclear reaction given by the integer %d (integer) by f (float).
Parameter input type: Float(scanf)
Default value: NULL

Parameter: nucsyn_metallicity
Description: This sets the metallicity of the nucleosynthesis algorithms, i.e. the amount (by mass) of matter which is not hydrogen or helium. Usually you’d just set this with the metallicity parameter, but if you want the nucleosynthesis to be outside the range of the stellar evolution algorithm (e.g. Z=0 or Z=0.04) then you need to use nucsyn_metallicity. That said, it’s also outside the range of some of the nucleosynthesis algorithms as well, so you have been warned!
Parameter input type: Float
Default value: -1
Macros: [‘DEFAULT_TO_METALLICITY = -1’]

Parameter: nucsyn_solver
Description: Choose the solver used in nuclear burning. 0 = KAPS_RENTROP is a Kaps-Rentrop scheme (fast, not great for stiff problems), 1 = LSODA (Adams/BSF switcher), 2 = CVODE library (https://computing.llnl.gov/projects/sundials. Default 0.
Parameter input type: Unsigned integer
Default value: 0
Macros: [‘NUCSYN_SOLVER_KAPS_RENTROP = 0’, ‘NUCSYN_SOLVER_LSODA = 1’, ‘NUCSYN_SOLVER_CVODE = 2’, ‘NUCSYN_SOLVER_NUMBER = 3’, ‘NUCSYN_SOLVER_KAPS_RENTROP = 0’, ‘NUCSYN_SOLVER_LSODA = 1’, ‘NUCSYN_SOLVER_CVODE = 2’, ‘NUCSYN_SOLVER_NUMBER = 3’]
Extra: 0

Parameter: initial_abundance_mix
Description: initial abundance mixture: 0=AG89, 1=Karakas 2002, 2=Lodders 2003, 3=Asplund 2005 (not available?), 4=Garcia Berro, 5=Grevesse Noels 1993
Parameter input type: Unsigned integer
Default value: 0
Macros: [‘NUCSYN_INIT_ABUND_MIX_AG89 = 0’, ‘NUCSYN_INIT_ABUND_MIX_KARAKAS2002 = 1’, ‘NUCSYN_INIT_ABUND_MIX_LODDERS2003 = 2’, ‘NUCSYN_INIT_ABUND_MIX_ASPLUND2005 = 3’, ‘NUCSYN_INIT_ABUND_MIX_GARCIABERRO = 4’, ‘NUCSYN_INIT_ABUND_MIX_GREVESSE_NOELS_1993 = 5’, ‘NUCSYN_INIT_ABUND_MIX_ASPLUND2009 = 6’, ‘NUCSYN_INIT_ABUND_MIX_KOBAYASHI2011_ASPLUND2009 = 7’, ‘NUCSYN_INIT_ABUND_MIX_LODDERS2010 = 8’]
Extra: 0

Parameter: init_abund
Description: Usage: –init_abund <i> <X>. Sets the initial abundance of isotope number <i> to mass fraction <X>.
Parameter input type: *
Default value: NULL
Extra: 0.02

Parameter: init_abund_mult
Description: Usage: –init_abund_mult <i> <f>. Multiplies the initial abundance of isotope number <i> by <f>.
Parameter input type: *
Default value: NULL
Extra: 1.0

Parameter: init_abund_dex
Description: Usage: –init_abund_dex <i> <f>. Changes the initial abundance of isotope number <i> by <f> dex.
Parameter input type: *
Default value: NULL
Extra: 0.0

Parameter: init_abunds_only
Description: If True, outputs only the initial abundances, then exits.
Parameter input type: True|False
Default value: False

Parameter: initial_abunds_only
Description: If True, outputs only the initial abundances, then exits.
Parameter input type: True|False
Default value: False

Parameter: no_thermohaline_mixing
Description: If True, disables thermohaline mixing.
Parameter input type: True|False
Default value: False

Parameter: lithium_GB_post_Heflash
Description: Sets the lithium abundances after the helium flash. Requires NUCSYN and LITHIUM_TABLES.
Parameter input type: Float
Default value: 0

Parameter: lithium_GB_post_1DUP
Description: Sets the lithium abundance after first dredge up. Requires NUCSYN and LITHIUM_TABLES.
Parameter input type: Float
Default value: 0

Parameter: lithium_hbb_multiplier
Description: Multiplies the lithium abundances on the AGB during HBB (based on Karakas/Fishlock et al models).Requires NUCSYN and LITHIUM_TABLES.
Parameter input type: Float
Default value: 1

Parameter: angelou_lithium_decay_function
Description: Functional form which describes Li7 decay. Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Choices are: 0 expoential (see angelou_lithium_decay_time).
Parameter input type: Integer
Default value: NULL
Macros: [‘ANGELOU_LITHIUM_DECAY_FUNCTION_EXPONENTIAL = 0’]

Parameter: angelou_lithium_LMMS_time
Description: Time at which lithium manufacture is triggered in a low-mass (convective) main sequence (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_MS_time
Description: Time at which lithium manufacture is triggered on the main sequence (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_HG_time
Description: Time at which lithium manufacture is triggered on the Hertzsprung gap (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_GB_time
Description: Time at which lithium manufacture is triggered on the giant branch (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_CHeB_time
Description: Time at which lithium manufacture is triggered during core helium burning (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_EAGB_time
Description: Time at which lithium manufacture is triggered on the early AGB (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_TPAGB_time
Description: Time at which lithium manufacture is triggered on the thermally pulsing AGB (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_LMMS_decay_time
Description: Decay time for surface lithium abundance during the low-mass (convective) main sequence (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_MS_decay_time
Description: Decay time for surface lithium abundance on the main sequence (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_HG_decay_time
Description: Decay time for surface lithium abundance on the Hertzsprung gap (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_GB_decay_time
Description: Decay time for surface lithium abundance on the giant branch (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_CHeB_decay_time
Description: Decay time for surface lithium abundance during core helium burning (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_EAGB_decay_time
Description: Decay time for surface lithium abundance on the early AGB (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_TPAGB_decay_time
Description: Decay time for surface lithium abundance on the thermally pulsing AGB (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_LMMS_massfrac
Description: Lithium mass fraction when its manufacture is triggered during the low-mass (convective) main sequence (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_MS_massfrac
Description: Lithium mass fraction when its manufacture is triggered on the main sequence (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_HG_massfrac
Description: Lithium mass fraction when its manufacture is triggered on the Hertzsprung gap (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_GB_massfrac
Description: Lithium mass fraction when its manufacture is triggered on the giant branch (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_CHeB_massfrac
Description: Lithium mass fraction when its manufacture is triggered during core helium burning (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_EAGB_massfrac
Description: Lithium mass fraction when its manufacture is triggered on the early AGB (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_TPAGB_massfrac
Description: Lithium mass fraction when its manufacture is triggered on the thermally pulsing AGB (Myr). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0 (for the start, use 1e-6).
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_vrot_trigger
Description: Equatorial rotational velocity at which lithium manufacture is triggered (km/s). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0.
Parameter input type: Float
Default value: NULL

Parameter: angelou_lithium_vrotfrac_trigger
Description: Fraction of Keplerian (breakup) equatorial rotational velocity at which lithium manufacture is triggered (must be <1, ignored if 0). Requires NUCSYN and NUCSYN_ANGELOU_LITHIUM. Ignored if 0.
Parameter input type: Float
Default value: NULL

Section: output

Parameter: cf_amanda_log
Description: Enable logging to compare to Amanda’s models.
Parameter input type: True|False
Default value: False

Parameter: float_overflow_checks
Description: Turn on to enable floating-point overflow checks at the end of each timestep, if they are available. 0=off, 1=warn (stderr) on failure, 2=exit on failure (0)
Parameter input type: Integer
Default value: 0

Parameter: save_pre_events_stardata
Description: Enable this to save a copy of stardata to stardata->pre_events_stardata just before an event.
Parameter input type: True|False
Default value: False

Parameter: disable_end_logging
Description: Disable the logging that happens at the end of the evolution.
Parameter input type: True|False
Default value: False

Parameter: ensemble
Description: Turn on ensemble calculations and output.
Parameter input type: True|False
Default value: False

Parameter: ensemble_filters_off
Description: Sets all ensemble filters to be off (FALSE) - these can then be enabled one-by-one with –ensemble_filter_[…] TRUE.
Parameter input type: True|False
Default value: False

Parameter: ensemble_filter_%d
Description: Turn on or off ensemble filter <n>. For a list of filters, see ensemble_macros.h.
Parameter input type: Boolean(scanf)
Default value: NULL

Parameter: ensemble_legacy_ensemble
Description: Turn on ensemble legacy population output.
Parameter input type: True|False
Default value: False

Parameter: legacy_yields
Description: Turn on ensemble legacy yield output.
Parameter input type: True|False
Default value: False

Parameter: ensemble_defer
Description: Defer ensemble output.
Parameter input type: True|False
Default value: False

Parameter: ensemble_dt
Description: When doing ensemble calculations, data are stored and/or output every ensemble_dt Myr. See also ensemble, ensemble_logdt, ensemble_startlogtime.
Parameter input type: Float
Default value: 1

Parameter: ensemble_logdt
Description: When doing ensemble calculations, and when logensembletimes is set, the ensemble is stored/output every ensemble_logdt Myr. See also ensemble, ensemble_dt, ensemble_startlogtime.
Parameter input type: Float
Default value: 0.1

Parameter: ensemble_startlogtime
Description: Start log ensemble data storage/calculations/output at ensemble_startlogtime. See also ensemble, ensemble_dt, ensemble_startlogtime.
Parameter input type: Float
Default value: 0.1

Parameter: ensemble_logtimes
Description: When doing ensemble calculations/output, set this to act at log times rather than linear times.
Parameter input type: True|False
Default value: False

Parameter: postagb_legacy_logging
Description: Turn on post-AGB legacy logging.
Parameter input type: True|False
Default value: False

Parameter: disc_legacy_logging
Description: Turn on disc legacy logging.
Parameter input type: True|False
Default value: False

Parameter: EMP_logg_maximum
Description: Maximum logg that EMP stars are allowed to have. See Izzard et al 2009. See also CEMP_cfe_minimum, NEMP_nfe_minimum, EMP_minimum_age.
Parameter input type: Float
Default value: 4

Parameter: EMP_minimum_age
Description: Minimum age that EMP stars are required to have. See Izzard et al 2009. See also CEMP_cfe_minimum, NEMP_nfe_minimum, EMP_logg_maximum.
Parameter input type: Float
Default value: 10

Parameter: EMP_feh_maximum
Description: Maximum [Fe/H] that an EMP stars may have. See Izzard et al 2009. See also CEMP_cfe_minimum, NEMP_nfe_minimum, EMP_logg_maximum, EMP_minimum_age. Default -2.0.
Parameter input type: Float
Default value: -2

Parameter: CEMP_cfe_minimum
Description: Minimum [C/Fe] that CEMP stars are required to have. See Izzard et al 2009. See also NEMP_cfe_minimum, EMP_logg_maximum, EMP_minimum_age. Default 0.7.
Parameter input type: Float
Default value: 0.7

Parameter: NEMP_cfe_minimum
Description: Minimum [N/Fe] that NEMP stars are required to have. See Izzard et al 2009, Pols et al. 2012. See also CEMP_cfe_minimum, EMP_logg_maximum, EMP_minimum_age. Default 1.0.
Parameter input type: Float
Default value: 1

Parameter: thick_disc_start_age
Description: Lookback time for the start of the thick disc star formation, e.g. 13e3 Myr. Units = Myr.
Parameter input type: Float
Default value: NULL

Parameter: thick_disc_end_age
Description: Lookback time for the end of the thick disc star formation, e.g. 4e3 Myr. Units = Myr.
Parameter input type: Float
Default value: NULL

Parameter: thick_disc_logg_min
Description: Minimum logg for thick disc giants to be logged.
Parameter input type: Float
Default value: NULL

Parameter: thick_disc_logg_max
Description: Maximum logg for thick disc giants to be logged.
Parameter input type: Float
Default value: NULL

Parameter: escape_velocity
Description: A parameter used in constructing galactic chemical evolution (GCE) models. If the stellar wind velocity exceeds this value, any chemical yield from the wind is ignored, i.e. assumed lost. (km/s) Requires NUCSYN_GCE_OUTFLOW_CHECKS. Default 1e9 km/s. See also escape_fraction.
Parameter input type: Float
Default value: NULL

Parameter: escape_fraction
Description: A parameter used in constructing galactic chemical evolution (GCE) models. If the stellar wind velocity exceeds this value, any chemical yield from the wind is ignored, i.e. assumed lost. (km/s) Requires NUCSYN_GCE_OUTFLOW_CHECKS. Default 0.0. See also escape_velocity.
Parameter input type: Float
Default value: NULL

Parameter: colour_log
Description: If set to True, thelog is coloured with ANSI colour formatting. Requires FILE_LOG to be defined.
Parameter input type: True|False
Default value: False
Extra:

Parameter: log_filename
Description: Location of the output logging filename. If set to “/dev/null” then there is no logging.
Parameter input type: String
Default value: /tmp/c_log.dat
Extra:

Parameter: log_arrows
Description: Add arrows to the output log to show whether values are increasing or decreasing.
Parameter input type: True|False
Default value: False
Extra:

Parameter: stopfile
Description: File which, when it exists, will stop the current binary_c repeat run.
Parameter input type: String
Default value:
Extra:

Parameter: stardata_dump_filename
Description: Location of the stardata dump file.
Parameter input type: String
Default value:
Extra:

Parameter: stardata_load_filename
Description: Location of the stardata file to load.
Parameter input type: String
Default value:
Extra:

Parameter: api_log_filename_prefix
Description: Location of the output logging filename prefix for the API. If set to “/dev/null” then there is no logging.
Parameter input type: String
Default value:
Extra: 0

Parameter: hrdiag_output
Description: Set to True to output high time-resolution Hertzstrpung-Russell diagram information. Requires HRDIAG.
Parameter input type: True|False
Default value: NULL

Parameter: internal_buffering
Description: Experimental. Set to non-zero values to implement internal buffering prior to output. For use with binary_grid, you shouldn’t really be playing with this.
Parameter input type: Integer
Default value: 2
Macros: [‘INTERNAL_BUFFERING_OFF = 0’, ‘INTERNAL_BUFFERING_PRINT = 1’, ‘INTERNAL_BUFFERING_STORE = 2’]

Parameter: eccentric_RLOF_model
Description: Chooses which model is used to handle eccentric RLOF. Default is RLOF_ECCENTRIC_AS_CIRCULAR, i.e. ignore the eccentricity. Note: requires force_corotation_of_primary_and_orbit to be FALSE.
Parameter input type: Integer
Default value: 0

Parameter: force_circularization_on_RLOF
Description: If True forces circularization of stars and orbit when RLOF starts, this is as in the BSE algorithm. (True)
Parameter input type: True|False
Default value: True

Parameter: wtts_log
Description: If True, enables log file output for WTTS2.
Parameter input type: True|False
Default value: False

Parameter: fabian_imf_log_time
Description: Time at which to output for Fabian Schneider’s IMF project. Requires FABIAN_IMF_LOG
Parameter input type: Float
Default value: NULL
Extra: Ignore

Parameter: fabian_imf_log_timestep
Description: Timestep for Fabian Schneider’s IMF project logging. Requires FABIAN_IMF_LOG
Parameter input type: Float
Default value: NULL
Extra: Ignore

Parameter: version
Description: Display binary_c version and build information. Also performs timing tests.
Parameter input type: *
Default value: NULL
Extra: Ignore

Parameter: dumpversion
Description: Display binary_c version number (short format).
Parameter input type: *
Default value: NULL
Extra: Ignore

Parameter: version_only
Description: Display binary_c version number and build information, but do not perform timing tests or anything that requires stardata to be non-NULL.
Parameter input type: *
Default value: NULL
Extra: Ignore

Parameter: tides_diagnosis_log
Description: Enable logging to test MINT tides. Requires MINT. Choices are: 0 disabled, 1 enable lambda test.
Parameter input type: Integer
Default value: 0
Extra: Ignore

Section: input

Parameter: MINT_dir
Description: Location of MINT algorithm data.
Parameter input type: String
Default value:
Extra:

Parameter: MINT_data_cleanup
Description: Activate checks on incoming data to try to account for problems. Will make data-loading slower, but may fix a few things.
Parameter input type: True|False
Default value: False
Extra:

Parameter: MINT_MS_rejuvenation
Description: Turn on or off (hydrogen) main-sequence rejuvenation.
Parameter input type: True|False
Default value: True
Extra:

Parameter: MINT_remesh
Description: Turn on or off MINT’s remeshing.
Parameter input type: True|False
Default value: True
Extra:

Parameter: MINT_use_ZAMS_profiles
Description: Use chemical profiles at the ZAMS if MINT_use_ZAMS_profiles is TRUE, otherwise set homogeneous abundances. (Default is TRUE, so we use the profiles if they are available.)
Parameter input type: True|False
Default value: True
Extra:

Parameter: MINT_fallback_to_test_data
Description: If TRUE, use the MINT test_data directory as a fallback when data is unavailable. (FALSE)
Parameter input type: True|False
Default value: False
Extra:

Parameter: MINT_disable_grid_load_warnings
Description: Use this to explicitly disable MINT’s warnings when loading a grid with, e.g., missing or too much data.
Parameter input type: True|False
Default value: False
Extra:

Parameter: MINT_Kippenhahn
Description: Turn on or off MINT’s Kippenhahn diagrams. If 0, off, if 1, output star 1 (index 0), if 2 output star 2 (index 1). Default 0.
Parameter input type: Integer
Default value: 0
Extra:

Parameter: MINT_nshells
Description: Set the initial number of shells MINT uses in each star when doing nuclear burning. Note: remeshing can change this. If MINT_nshells is 0, shellular burning and other routines that require shells will not be available. (200)
Parameter input type: Integer
Default value: 200
Extra:

Parameter: MINT_maximum_nshells
Description: Set the maximum number of shells MINT uses in each star when doing nuclear burning. Note that this will be limited to MINT_HARD_MAX_NSHELLS. (1000)
Parameter input type: Integer
Default value: 1000
Extra:

Parameter: MINT_minimum_nshells
Description: Set the minimum number of shells MINT uses in each star when doing nuclear burning. Note that this will be greater than or equal to MINT_HARD_MIN_NSHELLS, which is 0 by default. (0)
Parameter input type: Integer
Default value: 10
Extra:

Parameter: MINT_Kippenhahn_stellar_type
Description: Stellar type selector for Kippenhahn plots. Set to -1 to ignore, otherwise the stellar type number for which Kippenhahn plot data should be output.
Parameter input type: Integer
Default value: -1
Macros: [‘LOW_MASS_MS = 0’, ‘MS = 1’, ‘HG = 2’, ‘GIANT_BRANCH = 3’, ‘CHeB = 4’, ‘EAGB = 5’, ‘TPAGB = 6’, ‘HeMS = 7’, ‘HeHG = 8’, ‘HeGB = 9’, ‘HeWD = 10’, ‘COWD = 11’, ‘ONeWD = 12’, ‘NS = 13’, ‘BH = 14’, ‘MASSLESS_REMNANT = 15’]
Extra:

Parameter: MINT_Kippenhahn_companion_stellar_type
Description: Companion stellar type selector for Kippenhahn plots. Set to -1 to ignore, otherwise the stellar type number for the companion for which Kippenhahn plot data should be output.
Parameter input type: Integer
Default value: -1
Macros: [‘LOW_MASS_MS = 0’, ‘MS = 1’, ‘HG = 2’, ‘GIANT_BRANCH = 3’, ‘CHeB = 4’, ‘EAGB = 5’, ‘TPAGB = 6’, ‘HeMS = 7’, ‘HeHG = 8’, ‘HeGB = 9’, ‘HeWD = 10’, ‘COWD = 11’, ‘ONeWD = 12’, ‘NS = 13’, ‘BH = 14’, ‘MASSLESS_REMNANT = 15’]
Extra:

Parameter: MINT_nuclear_burning
Description: Turn on or off MINT’s nuclear burning algorithm.
Parameter input type: True|False
Default value: False
Extra:

Parameter: MINT_minimum_shell_mass
Description: Minimum shell mass in MINT’s nuclear burning routines.
Parameter input type: Float
Default value: 1e-06
Extra:

Parameter: MINT_maximum_shell_mass
Description: Maximum shell mass in MINT’s nuclear burning routines. :
Parameter input type: Float
Default value: 0.1
Extra:

Section: i/o

Parameter: go
Description: batchmode control command
Extra: Ignore

Parameter: gogo
Description: batchmode control command
Extra: Ignore

Parameter: reset_stars
Description: Reset the star structures. Used in batchmode
Extra: Ignore

Parameter: reset_stars_defaults
Description: Reset the star structures and set defaults. Used in batchmode
Extra: Ignore

Parameter: defaults
Description: Reset all defaults. Used in batchmode
Extra: Ignore

Parameter: echo
Description: Activate batchmode command echoing, i.e. when you enter a command, binary_c repeats the command then executes it.
Extra: Ignore

Parameter: noecho
Description: Deactivate batchmode command echoing. See ‘echo’.
Extra: Ignore

Parameter: noechonow
Description: Deactivate batchmode command echoing. See ‘echo’.
Extra: Ignore

Parameter: bye
Description: Quit binary_c. Used in batchmode.
Extra: Ignore

Parameter: fin
Description: batchmode control command
Extra: Ignore

Parameter: reset_prefs
Description: Reset preferences struct. Used in batchmode
Extra: Ignore

Parameter: status
Description: Output batchmode status information.
Extra: Ignore

Section: algorithms

Parameter: repeat
Description: If > 1, repeats the system as many times as required. Handy if you’re using Monte-Carlo kicks and want to sample the parameter space well. Also, if you are running speed tests this is good to give a statistically more reasonable result. (See e.g. ‘tbse pgo’).
Parameter input type: Integer
Default value: 1

Parameter: random_systems
Description: Experimental. Use this to apply random initial system parameters (masses, separations, etc.). Useful for testing only.
Parameter input type: Integer
Default value: 0

Section: misc

Parameter: random_seed
Description: Random number seed, usually a (possibly negative) integer. Useful for exactly reproducing the evolution of a system which involves a kick (which is a Monte-Carlo, i.e. pseudorandom, process).
Parameter input type: Integer
Default value: 0

Parameter: random_systems_seed
Description: Random number seed for the generation of random systems. See random_systems and random_seed.
Parameter input type: Integer
Default value: 0

Parameter: random_skip
Description: Skip the first <random_seed> random numbers that are generated. Usually this is 0 so they are all used.
Parameter input type: Integer
Default value: 0

Parameter: idum
Description: [NB: deprecated, please use ‘random_seed’ instead.] Random number seed, usually a (possibly negative) integer. Useful for exactly reproducing the evolution of a system which involves a kick (which is a Monte-Carlo, i.e. pseudorandom, process).
Parameter input type: Integer
Default value: 0

Parameter: reverse_time
Description: Make time go backwards. To be considered very experimental!
Parameter input type: True|False
Default value: NULL

Parameter: start_time
Description: Start time for the simulation.
Parameter input type: Float
Default value: 0

Parameter: warmup_cpu
Description: Uses the CPU at maximum power the given number of seconds, prior to running normal stellar evolution.
Parameter input type: *
Default value: NULL
Extra: Ignore

Parameter: help
Description: Display help pages. Usage: –help <help topic>.
Parameter input type: *
Default value: NULL
Extra: Ignore

Parameter: argopts
Description: Display argument options. Usage: –argopts <argument>.
Parameter input type: *
Default value: NULL
Extra: Ignore

Parameter: help_all
Description: Display all help pages.
Parameter input type: *
Default value: NULL
Extra: Ignore

Parameter: list_args
Description: Display list of arguments with their default values. Useful for batchmode.
Parameter input type: *
Default value: NULL
Extra: Ignore