[Commits] [svn:einsteintoolkit] www/about/gallery/ (Rev. 1527)

barry.wardell at gmail.com barry.wardell at gmail.com
Sun Jun 5 17:04:53 CDT 2016


User: barry.wardell
Date: 2016/06/05 05:04 PM

Added:
 /about/gallery/NsNsToHMNS/
  index.php

Modified:
 /about/gallery/
  index.php

Log:
 gallery: Move BNS to a separate page

File Changes:

Directory: /about/gallery/NsNsToHMNS/
=====================================

File [added]: index.php
Delta lines: +30 -0
===================================================================
--- about/gallery/NsNsToHMNS/index.php	                        (rev 0)
+++ about/gallery/NsNsToHMNS/index.php	2016-06-05 22:04:53 UTC (rev 1527)
@@ -0,0 +1,30 @@
+<?php $title="Gallery: Binary, inspiraling neutron stars forming a hypermassive neutron star";
+include_once($_SERVER['DOCUMENT_ROOT'].'/global/header.php');?>
+<script type="text/javascript" src="/global/jwplayer/jwplayer.js"></script>
+
+  <p>This simulation shows how to evolve a pair of neutron stars, reading in
+     initial data provided by the <a href="http://www.lorene.obspm.fr/">LORENE</a> code. The video shows
+     the rest mass density in an equatorial slice of the simulation. The
+     emitted gravitational waves of the inspiral and due to the oscillations in
+     the formed hypermassive neutron star are shown as well. </p>
+  <table>
+   <tr><th>Parameter file</th><td><a href="NsNsToHMNS.par">NsNsToHMNS.par</a></td></tr>
+   <tr><th>Thornlist</th><td><a href="NsNsToHMNS.th">NsNsToHMNS.th</a> (Thorn NSTracker added to release)</td></tr>
+   <tr><th>Initial data file</th><td><a href="G2_I12vs12_D4R33T21_45km.resu.xz">G2_I12vs12_D4R33T21_45km.resu.xz</a> (uncompress using <a href="http://en.wikipedia.org/wiki/XZ_Utils">unxz</a>)</td></tr>
+   <tr><th>Support scripts</th><td><a href="scripts.tar.gz">scripts.tar.gz</a></td></tr>
+   <tr><th>approx. memory</th><td>8.8 GB</td></tr>
+   <tr><th>approx. runtime</th><td>12*48 SU</td></tr>
+  </table>
+  <a href="mp_Psi4_l2_m2_r300.00.asc"><img src="mp_Psi4_l2_m2_r300.00.png" alt="Psi_4^{2,2} at r=300M over time"></a>
+  <div id="NsNsToHMNS_rho">Loading the player...</div>
+  Download movie: <a href="rho.mp4">rho.mp4</a>
+  <script type="text/javascript">
+      jwplayer("NsNsToHMNS_rho").setup({
+          file: "rho.mp4",
+          image: "rho.png",
+          width: 640, height: 480
+      });
+  </script>
+
+
+<?php include_once($_SERVER['DOCUMENT_ROOT'].'/global/footer.php');?>

Directory: /about/gallery/
==========================

File [modified]: index.php
Delta lines: +3 -25
===================================================================
--- about/gallery/index.php	2016-06-05 22:04:49 UTC (rev 1526)
+++ about/gallery/index.php	2016-06-05 22:04:53 UTC (rev 1527)
@@ -22,38 +22,16 @@
 <p>
 <ul>
 <li><a href="tov">Single, stable neutron star</a></li>
+<li><a href="NsNsToHMNS">Binary, inspiraling neutron stars forming a hypermassive neutron star</a></li>
+
 </ul>
 </p>
 
 <!--
  <h4> Single, collapsing neutron star</h4>
 -->
- <h4> Binary, inspiraling neutron stars forming a hypermassive neutron star</h4>
-  <p>This simulation shows how to evolve a pair of neutron stars, reading in
-     initial data provided by the <a href="http://www.lorene.obspm.fr/">LORENE</a> code. The video shows
-     the rest mass density in an equatorial slice of the simulation. The
-     emitted gravitational waves of the inspiral and due to the oscillations in
-     the formed hypermassive neutron star are shown as well. </p>
-  <table>
-   <tr><th>Parameter file</th><td><a href="NsNsToHMNS/NsNsToHMNS.par">NsNsToHMNS.par</a></td></tr>
-   <tr><th>Thornlist</th><td><a href="NsNsToHMNS/NsNsToHMNS.th">NsNsToHMNS.th</a> (Thorn NSTracker added to release)</td></tr>
-   <tr><th>Initial data file</th><td><a href="NsNsToHMNS/G2_I12vs12_D4R33T21_45km.resu.xz">G2_I12vs12_D4R33T21_45km.resu.xz</a> (uncompress using <a href="http://en.wikipedia.org/wiki/XZ_Utils">unxz</a>)</td></tr>
-   <tr><th>Support scripts</th><td><a href="NsNsToHMNS/scripts.tar.gz">scripts.tar.gz</a></td></tr>
-   <tr><th>approx. memory</th><td>8.8 GB</td></tr>
-   <tr><th>approx. runtime</th><td>12*48 SU</td></tr>
-  </table>
-  <a href="NsNsToHMNS/mp_Psi4_l2_m2_r300.00.asc"><img src="NsNsToHMNS/mp_Psi4_l2_m2_r300.00.png" alt="Psi_4^{2,2} at r=300M over time"></a>
-  <div id="NsNsToHMNS_rho">Loading the player...</div>
-  Download movie: <a href="NsNsToHMNS/rho.mp4">rho.mp4</a>
-  <script type="text/javascript">
-      jwplayer("NsNsToHMNS_rho").setup({
-          file: "NsNsToHMNS/rho.mp4",
-          image: "NsNsToHMNS/rho.png",
-          width: 640, height: 480
-      });
-  </script>
 
-  <h4>Poisson equation</h4>
+<h4>Poisson equation</h4>
   
   <p>This example shows how to solve the Poisson equation with a
   generic source term using



More information about the Commits mailing list