<html>#2119: The binary neutron star gallery example gives different results with the release candiate.
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<tr><td style='text-align:right'> Reporter:</td><td>Peter Diener</td></tr>
<tr><td style='text-align:right'> Status:</td><td>open</td></tr>
<tr><td style='text-align:right'>Milestone:</td><td>ET_2019_10</td></tr>
<tr><td style='text-align:right'> Version:</td><td>development version</td></tr>
<tr><td style='text-align:right'> Type:</td><td>bug</td></tr>
<tr><td style='text-align:right'> Priority:</td><td>minor</td></tr>
<tr><td style='text-align:right'>Component:</td><td>Other</td></tr>
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<p>Comment (by Roland Haas):</p>
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<p>Running with the new Meudon code and <code>-O3</code> gives waveforms more similar to running with just <code>-O3</code> but rho values closer to <code>-Ofast</code> (but then max(rho) is a pointwise value).</p>
<p><img alt="" src="https://bitbucket.org/repo/8zBLME5/images/1552947736-psi4_Zwicky.png" />
<img alt="" src="https://bitbucket.org/repo/8zBLME5/images/929720229-rho_Optimize.png" />
It looks quite similar to what Peter found using all new code (ie smaller maximum and a deeper dip in rho just after the maximum). </p>
<p></p>
<p>--<br/>
Ticket URL: <a href='https://bitbucket.org/einsteintoolkit/tickets/issues/2119/the-binary-neutron-star-gallery-example'>https://bitbucket.org/einsteintoolkit/tickets/issues/2119/the-binary-neutron-star-gallery-example</a></p>
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