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<section id="module-binarycpython.utils.useful_funcs">
<span id="useful-funcs-module"></span><h1>useful_funcs module<a class="headerlink" href="#module-binarycpython.utils.useful_funcs" title="Permalink to this headline"></a></h1>
<p>Collection of useful functions.</p>
<p>Part of this is copied/inspired by Rob’s binary_stars module</p>
<dl class="simple">
<dt>Functions:</dt><dd><ul class="simple">
<li><p>calc_period_from_sep(m1, m2, sep) calculate the period given the separation.</p></li>
<li><p>calc_sep_from_period(m1, m2, per) does the inverse.</p></li>
<li><p>rzams(m, z) gives you the ZAMS radius of a star</p></li>
<li><p>ZAMS_collision(m1, m2, e, sep, z) returns 1 if stars collide on the ZAMS</p></li>
<li><p>roche_lobe(q): returns roche lobe radius in units of separation</p></li>
<li><p>ragb(m): radius at first thermal pulse</p></li>
<li><p>minimum_period_for_RLOF(M1, M2, metallicity, store_memaddr=-1): function to calculate the minimum period that leads to RLOF on ZAMS</p></li>
<li><p>minimum_separation_for_RLOF(M1, M2, metallicity, store_memaddr=-1): function to calculate the minimum period that leads to RLOF on ZAMS</p></li>
<li><p>maximum_mass_ratio_for_RLOF(M1, orbital_period, store_memaddr=None): Function to calculate the maximum mass ratio that leads to RLOF on ZAMS</p></li>
</ul>
</dd>
<dt>Tasks:</dt><dd><ul class="simple">
<li><p>TODO: check whether these functions are correct</p></li>
</ul>
</dd>
</dl>
<dl class="py function">
<dt class="sig sig-object py" id="binarycpython.utils.useful_funcs.calc_period_from_sep">
<span class="sig-prename descclassname"><span class="pre">binarycpython.utils.useful_funcs.</span></span><span class="sig-name descname"><span class="pre">calc_period_from_sep</span></span><span class="sig-paren">(</span><em class="sig-param"><span class="n"><span class="pre">M1</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">M2</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">sep</span></span></em><span class="sig-paren">)</span><a class="reference internal" href="_modules/binarycpython/utils/useful_funcs.html#calc_period_from_sep"><span class="viewcode-link"><span class="pre">[source]</span></span></a><a class="headerlink" href="#binarycpython.utils.useful_funcs.calc_period_from_sep" title="Permalink to this definition"></a></dt>
<dd><p>calculate period from separation</p>
<dl class="field-list simple">
<dt class="field-odd">Parameters</dt>
<dd class="field-odd"><ul class="simple">
<li><p><strong>M1</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – Primary mass in solar mass</p></li>
<li><p><strong>M2</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – Secondary mass in solar mass</p></li>
<li><p><strong>sep</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – Separation in solar radii</p></li>
</ul>
</dd>
<dt class="field-even">Return type</dt>
<dd class="field-even"><p><code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]</p>
</dd>
<dt class="field-odd">Returns</dt>
<dd class="field-odd"><p>period in days</p>
</dd>
</dl>
</dd></dl>
<dl class="py function">
<dt class="sig sig-object py" id="binarycpython.utils.useful_funcs.calc_sep_from_period">
<span class="sig-prename descclassname"><span class="pre">binarycpython.utils.useful_funcs.</span></span><span class="sig-name descname"><span class="pre">calc_sep_from_period</span></span><span class="sig-paren">(</span><em class="sig-param"><span class="n"><span class="pre">M1</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">M2</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">period</span></span></em><span class="sig-paren">)</span><a class="reference internal" href="_modules/binarycpython/utils/useful_funcs.html#calc_sep_from_period"><span class="viewcode-link"><span class="pre">[source]</span></span></a><a class="headerlink" href="#binarycpython.utils.useful_funcs.calc_sep_from_period" title="Permalink to this definition"></a></dt>
<dd><p>Calculate separation from period.</p>
<dl class="field-list simple">
<dt class="field-odd">Parameters</dt>
<dd class="field-odd"><ul class="simple">
<li><p><strong>M1</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – Primary mass in solar mass</p></li>
<li><p><strong>M2</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – Secondary mass in solar mass</p></li>
<li><p><strong>period</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – Period of binary in days</p></li>
</ul>
</dd>
<dt class="field-even">Return type</dt>
<dd class="field-even"><p><code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]</p>
</dd>
<dt class="field-odd">Returns</dt>
<dd class="field-odd"><p>Separation in solar radii</p>
</dd>
</dl>
</dd></dl>
<dl class="py function">
<dt class="sig sig-object py" id="binarycpython.utils.useful_funcs.maximum_mass_ratio_for_RLOF">
<span class="sig-prename descclassname"><span class="pre">binarycpython.utils.useful_funcs.</span></span><span class="sig-name descname"><span class="pre">maximum_mass_ratio_for_RLOF</span></span><span class="sig-paren">(</span><em class="sig-param"><span class="n"><span class="pre">M1</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">orbital_period</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">metallicity</span></span><span class="o"><span class="pre">=</span></span><span class="default_value"><span class="pre">0.02</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">store_memaddr</span></span><span class="o"><span class="pre">=</span></span><span class="default_value"><span class="pre">None</span></span></em><span class="sig-paren">)</span><a class="reference internal" href="_modules/binarycpython/utils/useful_funcs.html#maximum_mass_ratio_for_RLOF"><span class="viewcode-link"><span class="pre">[source]</span></span></a><a class="headerlink" href="#binarycpython.utils.useful_funcs.maximum_mass_ratio_for_RLOF" title="Permalink to this definition"></a></dt>
<dd><p>Wrapper function for _binary_c_bindings.return_maximum_mass_ratio_for_RLOF</p>
<p>Handles the output and returns the maximum mass ratio at which RLOF just does not occur at ZAMS</p>
<dl class="field-list simple">
<dt class="field-odd">Parameters</dt>
<dd class="field-odd"><ul class="simple">
<li><p><strong>M1</strong> – Primary mass in solar mass</p></li>
<li><p><strong>orbital_period</strong> – orbital period in days</p></li>
<li><p><strong>metallicity</strong> – metallicity</p></li>
<li><p><strong>store_memaddr</strong> (<em>optional</em>) – store memory adress</p></li>
</ul>
</dd>
<dt class="field-even">Returns</dt>
<dd class="field-even"><p>maximum mass ratio that just does not cause a RLOF at ZAMS</p>
</dd>
</dl>
</dd></dl>
<dl class="py function">
<dt class="sig sig-object py" id="binarycpython.utils.useful_funcs.minimum_period_for_RLOF">
<span class="sig-prename descclassname"><span class="pre">binarycpython.utils.useful_funcs.</span></span><span class="sig-name descname"><span class="pre">minimum_period_for_RLOF</span></span><span class="sig-paren">(</span><em class="sig-param"><span class="n"><span class="pre">M1</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">M2</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">metallicity</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">store_memaddr</span></span><span class="o"><span class="pre">=</span></span><span class="default_value"><span class="pre">-</span> <span class="pre">1</span></span></em><span class="sig-paren">)</span><a class="reference internal" href="_modules/binarycpython/utils/useful_funcs.html#minimum_period_for_RLOF"><span class="viewcode-link"><span class="pre">[source]</span></span></a><a class="headerlink" href="#binarycpython.utils.useful_funcs.minimum_period_for_RLOF" title="Permalink to this definition"></a></dt>
<dd><p>Wrapper function for _binary_c_bindings.return_minimum_orbit_for_RLOF</p>
<p>Handles the output and returns the minimum orbital period at which RLOF just does not occur at ZAMS</p>
<dl class="field-list simple">
<dt class="field-odd">Parameters</dt>
<dd class="field-odd"><ul class="simple">
<li><p><strong>M1</strong> – Primary mass in solar mass</p></li>
<li><p><strong>M2</strong> – Secondary mass in solar mass</p></li>
<li><p><strong>metallicity</strong> – metallicity</p></li>
<li><p><strong>store_memaddr</strong> (<em>optional</em>) – store memory address</p></li>
</ul>
</dd>
<dt class="field-even">Returns</dt>
<dd class="field-even"><p>minimum orbital_period that just does not cause a RLOF at ZAMS</p>
</dd>
</dl>
</dd></dl>
<dl class="py function">
<dt class="sig sig-object py" id="binarycpython.utils.useful_funcs.minimum_separation_for_RLOF">
<span class="sig-prename descclassname"><span class="pre">binarycpython.utils.useful_funcs.</span></span><span class="sig-name descname"><span class="pre">minimum_separation_for_RLOF</span></span><span class="sig-paren">(</span><em class="sig-param"><span class="n"><span class="pre">M1</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">M2</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">metallicity</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">store_memaddr</span></span><span class="o"><span class="pre">=</span></span><span class="default_value"><span class="pre">-</span> <span class="pre">1</span></span></em><span class="sig-paren">)</span><a class="reference internal" href="_modules/binarycpython/utils/useful_funcs.html#minimum_separation_for_RLOF"><span class="viewcode-link"><span class="pre">[source]</span></span></a><a class="headerlink" href="#binarycpython.utils.useful_funcs.minimum_separation_for_RLOF" title="Permalink to this definition"></a></dt>
<dd><p>Wrapper function for _binary_c_bindings.return_minimum_orbit_for_RLOF</p>
<p>Handles the output and returns the minimum separation at which RLOF just does not occur at ZAMS</p>
<dl class="field-list simple">
<dt class="field-odd">Parameters</dt>
<dd class="field-odd"><ul class="simple">
<li><p><strong>M1</strong> – Primary mass in solar mass</p></li>
<li><p><strong>M2</strong> – Secondary mass in solar mass</p></li>
<li><p><strong>metallicity</strong> – metallicity</p></li>
<li><p><strong>store_memaddr</strong> (<em>optional</em>) – store memory adress</p></li>
</ul>
</dd>
<dt class="field-even">Returns</dt>
<dd class="field-even"><p>minimum separation that just does not cause a RLOF at ZAMS</p>
</dd>
</dl>
</dd></dl>
<dl class="py function">
<dt class="sig sig-object py" id="binarycpython.utils.useful_funcs.ragb">
<span class="sig-prename descclassname"><span class="pre">binarycpython.utils.useful_funcs.</span></span><span class="sig-name descname"><span class="pre">ragb</span></span><span class="sig-paren">(</span><em class="sig-param"><span class="n"><span class="pre">m</span></span></em><span class="sig-paren">)</span><a class="reference internal" href="_modules/binarycpython/utils/useful_funcs.html#ragb"><span class="viewcode-link"><span class="pre">[source]</span></span></a><a class="headerlink" href="#binarycpython.utils.useful_funcs.ragb" title="Permalink to this definition"></a></dt>
<dd><p>Function to calculate radius of a star in units of solar radii at first thermal pulse as a function of mass (Z=0.02 only, but also good for Z=0.0001)</p>
<p>TODO: ask rob about this function. Do we still need this? Can we make something better? (i.e. upon installation of the code run a grid of systems and get the data from there?)</p>
<dl class="field-list simple">
<dt class="field-odd">Parameters</dt>
<dd class="field-odd"><ul class="simple">
<li><p><strong>m</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – mass of star in units of solar mass</p></li>
<li><p><strong>z</strong> – metallicity of star</p></li>
</ul>
</dd>
<dt class="field-even">Return type</dt>
<dd class="field-even"><p><code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]</p>
</dd>
<dt class="field-odd">Returns</dt>
<dd class="field-odd"><p>radius at first thermal pulse in units of solar radii</p>
</dd>
</dl>
</dd></dl>
<dl class="py function">
<dt class="sig sig-object py" id="binarycpython.utils.useful_funcs.roche_lobe">
<span class="sig-prename descclassname"><span class="pre">binarycpython.utils.useful_funcs.</span></span><span class="sig-name descname"><span class="pre">roche_lobe</span></span><span class="sig-paren">(</span><em class="sig-param"><span class="n"><span class="pre">q</span></span></em><span class="sig-paren">)</span><a class="reference internal" href="_modules/binarycpython/utils/useful_funcs.html#roche_lobe"><span class="viewcode-link"><span class="pre">[source]</span></span></a><a class="headerlink" href="#binarycpython.utils.useful_funcs.roche_lobe" title="Permalink to this definition"></a></dt>
<dd><p>A function to evaluate R_L/a(q), Eggleton 1983.</p>
<p># TODO: check the definition of the mass ratio
# TODO: check whether the logs are correct</p>
<dl class="field-list simple">
<dt class="field-odd">Parameters</dt>
<dd class="field-odd"><p><strong>q</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – mass ratio of the binary (secondary/primary). If you input: q = mass_accretor/mass_donor, you will get the rochelobe radius of the accretor. And vice versa for the donor.</p>
</dd>
<dt class="field-even">Return type</dt>
<dd class="field-even"><p><code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]</p>
</dd>
<dt class="field-odd">Returns</dt>
<dd class="field-odd"><p>Roche lobe radius in units of the separation</p>
</dd>
</dl>
</dd></dl>
<dl class="py function">
<dt class="sig sig-object py" id="binarycpython.utils.useful_funcs.rzams">
<span class="sig-prename descclassname"><span class="pre">binarycpython.utils.useful_funcs.</span></span><span class="sig-name descname"><span class="pre">rzams</span></span><span class="sig-paren">(</span><em class="sig-param"><span class="n"><span class="pre">m</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">z</span></span></em><span class="sig-paren">)</span><a class="reference internal" href="_modules/binarycpython/utils/useful_funcs.html#rzams"><span class="viewcode-link"><span class="pre">[source]</span></span></a><a class="headerlink" href="#binarycpython.utils.useful_funcs.rzams" title="Permalink to this definition"></a></dt>
<dd><p>Function to determine the radius of a ZAMS star as a function of m and z:</p>
<p>Based on the fits of Tout et al., 1996, MNRAS, 281, 257</p>
<dl class="field-list simple">
<dt class="field-odd">Parameters</dt>
<dd class="field-odd"><ul class="simple">
<li><p><strong>m</strong> – mass of star in solar mass</p></li>
<li><p><strong>z</strong> – metallicity</p></li>
</ul>
</dd>
<dt class="field-even">Returns</dt>
<dd class="field-even"><p>radius of star at ZAMS, in solar radii</p>
</dd>
</dl>
</dd></dl>
<dl class="py function">
<dt class="sig sig-object py" id="binarycpython.utils.useful_funcs.zams_collision">
<span class="sig-prename descclassname"><span class="pre">binarycpython.utils.useful_funcs.</span></span><span class="sig-name descname"><span class="pre">zams_collision</span></span><span class="sig-paren">(</span><em class="sig-param"><span class="n"><span class="pre">m1</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">m2</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">sep</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">e</span></span></em>, <em class="sig-param"><span class="n"><span class="pre">z</span></span></em><span class="sig-paren">)</span><a class="reference internal" href="_modules/binarycpython/utils/useful_funcs.html#zams_collision"><span class="viewcode-link"><span class="pre">[source]</span></span></a><a class="headerlink" href="#binarycpython.utils.useful_funcs.zams_collision" title="Permalink to this definition"></a></dt>
<dd><p>given m1,m2, separation and eccentricity (and metallicity)
determine if two stars collide on the ZAMS</p>
<dl class="field-list simple">
<dt class="field-odd">Parameters</dt>
<dd class="field-odd"><ul class="simple">
<li><p><strong>m1</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – Primary mass in solar mass</p></li>
<li><p><strong>m2</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – Secondary mass in solar mass</p></li>
<li><p><strong>sep</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – separation in solar radii</p></li>
<li><p><strong>e</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – eccentricity</p></li>
<li><p><strong>z</strong> (<code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]) – metallicity</p></li>
</ul>
</dd>
<dt class="field-even">Return type</dt>
<dd class="field-even"><p><code class="xref py py-data docutils literal notranslate"><span class="pre">Union</span></code>[<code class="xref py py-class docutils literal notranslate"><span class="pre">int</span></code>, <code class="xref py py-class docutils literal notranslate"><span class="pre">float</span></code>]</p>
</dd>
<dt class="field-odd">Returns</dt>
<dd class="field-odd"><p>integer boolean whether the binary stars will collide at pericenter</p>
</dd>
</dl>
</dd></dl>
</section>
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