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emptymalei committed Sep 25, 2024
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2 changes: 1 addition & 1 deletion 404.html
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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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2 changes: 1 addition & 1 deletion references/maths/trigonometrics/index.html
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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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2 changes: 1 addition & 1 deletion references/models/harmonic_oscillator/index.html
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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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2 changes: 1 addition & 1 deletion references/models/harmonic_oscillator_chain/index.html
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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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2 changes: 1 addition & 1 deletion references/models/kepler_problem/dynamics/index.html
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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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18 changes: 9 additions & 9 deletions references/models/kepler_problem/model/index.html
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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


Expand Down Expand Up @@ -1799,14 +1799,14 @@ <h2 id="hamilflow.models.kepler_problem.model.Kepler2D" class="doc doc-heading">
<span class="p">)</span> <span class="o">-&gt;</span> <span class="s2">&quot;Self&quot;</span><span class="p">:</span>
<span class="w"> </span><span class="sa">r</span><span class="sd">&quot;&quot;&quot;Alternative initialiser from system and geometry specifications.</span>

<span class="sd"> Given the eccentricity $e$ and the conic section parameter $p$,</span>
<span class="sd"> Given the eccentricity $e$ and the conic section semi-latus rectum $p$,</span>
<span class="sd"> $$l = \pm \sqrt{mp}\,,\quad E = (e^2-1) \left|E_\text{min}\right|\,.$$</span>

<span class="sd"> :param system: the Kepler problem system specification</span>
<span class="sd"> :param geometries: geometric specifications</span>
<span class="sd"> `positive_angular_mom`: whether the angular momentum is positive</span>
<span class="sd"> `ecc`: eccentricity of the conic section</span>
<span class="sd"> `parameter`: parameter of the conic section</span>
<span class="sd"> `parameter`: semi-latus rectum of the conic section</span>
<span class="sd"> &quot;&quot;&quot;</span>
<span class="n">mass</span><span class="p">,</span> <span class="n">alpha</span> <span class="o">=</span> <span class="n">system</span><span class="p">[</span><span class="s2">&quot;mass&quot;</span><span class="p">],</span> <span class="n">system</span><span class="p">[</span><span class="s2">&quot;alpha&quot;</span><span class="p">]</span>
<span class="n">positive_angular_mom</span> <span class="o">=</span> <span class="nb">bool</span><span class="p">(</span><span class="n">geometries</span><span class="p">[</span><span class="s2">&quot;positive_angular_mom&quot;</span><span class="p">])</span>
Expand Down Expand Up @@ -1884,7 +1884,7 @@ <h2 id="hamilflow.models.kepler_problem.model.Kepler2D" class="doc doc-heading">
<span class="c1"># FIXME is it called parameter in English?</span>
<span class="nd">@cached_property</span>
<span class="k">def</span> <span class="nf">parameter</span><span class="p">(</span><span class="bp">self</span><span class="p">)</span> <span class="o">-&gt;</span> <span class="nb">float</span><span class="p">:</span>
<span class="w"> </span><span class="sa">r</span><span class="sd">&quot;&quot;&quot;Conic section parameter of the Kepler problem.</span>
<span class="w"> </span><span class="sa">r</span><span class="sd">&quot;&quot;&quot;Conic section semi-latus rectum of the Kepler problem.</span>

<span class="sd"> $$ p = \frac{l^2}{\alpha m}\,. $$</span>
<span class="sd"> &quot;&quot;&quot;</span>
Expand Down Expand Up @@ -2119,7 +2119,7 @@ <h3 id="hamilflow.models.kepler_problem.model.Kepler2D.parameter" class="doc doc

<div class="doc doc-contents ">

<p>Conic section parameter of the Kepler problem.</p>
<p>Conic section semi-latus rectum of the Kepler problem.</p>
<div class="arithmatex">\[ p = \frac{l^2}{\alpha m}\,. \]</div>
</div>

Expand Down Expand Up @@ -2294,7 +2294,7 @@ <h3 id="hamilflow.models.kepler_problem.model.Kepler2D.from_geometry" class="doc
<div class="doc doc-contents ">

<p>Alternative initialiser from system and geometry specifications.</p>
<p>Given the eccentricity <span class="arithmatex">\(e\)</span> and the conic section parameter <span class="arithmatex">\(p\)</span>,
<p>Given the eccentricity <span class="arithmatex">\(e\)</span> and the conic section semi-latus rectum <span class="arithmatex">\(p\)</span>,
<span class="arithmatex">\(<span class="arithmatex">\(l = \pm \sqrt{mp}\,,\quad E = (e^2-1) \left|E_\text{min}\right|\,.\)</span>\)</span></p>


Expand Down Expand Up @@ -2331,7 +2331,7 @@ <h3 id="hamilflow.models.kepler_problem.model.Kepler2D.from_geometry" class="doc
</td>
<td>
<div class="doc-md-description">
<p>geometric specifications <code>positive_angular_mom</code>: whether the angular momentum is positive <code>ecc</code>: eccentricity of the conic section <code>parameter</code>: parameter of the conic section</p>
<p>geometric specifications <code>positive_angular_mom</code>: whether the angular momentum is positive <code>ecc</code>: eccentricity of the conic section <code>parameter</code>: semi-latus rectum of the conic section</p>
</div>
</td>
<td>
Expand Down Expand Up @@ -2381,14 +2381,14 @@ <h3 id="hamilflow.models.kepler_problem.model.Kepler2D.from_geometry" class="doc
<span class="p">)</span> <span class="o">-&gt;</span> <span class="s2">&quot;Self&quot;</span><span class="p">:</span>
<span class="w"> </span><span class="sa">r</span><span class="sd">&quot;&quot;&quot;Alternative initialiser from system and geometry specifications.</span>

<span class="sd"> Given the eccentricity $e$ and the conic section parameter $p$,</span>
<span class="sd"> Given the eccentricity $e$ and the conic section semi-latus rectum $p$,</span>
<span class="sd"> $$l = \pm \sqrt{mp}\,,\quad E = (e^2-1) \left|E_\text{min}\right|\,.$$</span>

<span class="sd"> :param system: the Kepler problem system specification</span>
<span class="sd"> :param geometries: geometric specifications</span>
<span class="sd"> `positive_angular_mom`: whether the angular momentum is positive</span>
<span class="sd"> `ecc`: eccentricity of the conic section</span>
<span class="sd"> `parameter`: parameter of the conic section</span>
<span class="sd"> `parameter`: semi-latus rectum of the conic section</span>
<span class="sd"> &quot;&quot;&quot;</span>
<span class="n">mass</span><span class="p">,</span> <span class="n">alpha</span> <span class="o">=</span> <span class="n">system</span><span class="p">[</span><span class="s2">&quot;mass&quot;</span><span class="p">],</span> <span class="n">system</span><span class="p">[</span><span class="s2">&quot;alpha&quot;</span><span class="p">]</span>
<span class="n">positive_angular_mom</span> <span class="o">=</span> <span class="nb">bool</span><span class="p">(</span><span class="n">geometries</span><span class="p">[</span><span class="s2">&quot;positive_angular_mom&quot;</span><span class="p">])</span>
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2 changes: 1 addition & 1 deletion references/models/kepler_problem/numerics/index.html
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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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2 changes: 1 addition & 1 deletion references/models/pendulum/index.html
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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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2 changes: 1 addition & 1 deletion tutorials/index.html
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<span class="md-ellipsis">
Motion in a Central Field
Kepler Problem
</span>


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