User: rhaas Date: 2015/06/17 01:18 AM

Modified: /about/gallery/ index.php

Log: Gallery: use headings to separate individual examples to make them more prominent

File Changes:

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

File [modified]: index.php Delta lines: +5 -17 =================================================================== --- about/gallery/index.php 2015-06-02 13:14:27 UTC (rev 1482) +++ about/gallery/index.php 2015-06-17 06:18:01 UTC (rev 1483) @@ -12,19 +12,13 @@

<h3>Using exclusively the Einstein Toolkit</h3>

-<ul> <!-- - <li> - Single black hole - </li> + <h4> Single black hole</h4> --> <!-- - <li> - Binary black hole inspiral - </li> + <h4> Binary black hole inspiral</h4> --> - <li> - Single, stable neutron star + <h4> Single, stable neutron star</h4> <p>This simulation shows how to evolve a stable, single neutron star. It uses a TOV solution as initial data and follows the initial (numerical) perturbations, writing the maximum density to disk. What can be seen is that the oscillates for a few cycles (only very @@ -41,14 +35,10 @@ <tr><th>approx. runtime</th><td>2.5 SU</td></tr> </table> <a href="tov/rho_max.pdf"><img src="tov/rho_max.png" alt="Maximum density over time"></a> - </li> <!-- - <li> - Single, collapsing neutron star - </li> + <h4> Single, collapsing neutron star</h4> --> - <li> - Binary, inspiraling neutron stars forming a hypermassive neutron star + <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 @@ -72,8 +62,6 @@ width: 640, height: 480 }); </script> - </li> -</ul>

<!-- <h3>Using external but public code</h3>