neutron stars - Universität Heidelberg
neutron stars - Universität Heidelberg
neutron stars - Universität Heidelberg
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Implications for Supernovae – Explosion!<br />
Velocity [km/s]<br />
x 105<br />
1.2<br />
0.8<br />
0.4<br />
0<br />
0.4<br />
0.8<br />
10 1<br />
Radius [km]<br />
(Sagert, Hempel, Pagliara, JSB, Fischer, Mezzacappa, Thielemann, Liebendörfer, 2008)<br />
velocity profile of a supernova for different times (around 250ms)<br />
formation of a core of pure quark matter produces a second shock wave<br />
10 2<br />
10 3<br />
– p.34
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