MG14 - Talk detail |
Participant |
Hanauske, Matthias | |||||||
Institution |
Goethe-University - FIAS - Max-von-Laue-Str. 1 - Frankfurt am Main - Hessen - Germany | |||||||
Session |
BN2 |
Accepted |
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Order |
Time |
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Talk |
Oral abstract |
Title |
Structural properties of hypermassive neutron stars | |||||
Coauthors | ||||||||
Abstract |
Based on a large number of numerical-relativity simulations of merging neutron-star binaries, the structural properties of the hypermassive neutron stars (HMNSs) produced in the post-merger phase have been analyzed. The simulations have been performed in full general relativity using the WHISKY code for the general-relativistic hydrodynamic equations. The HMNS properties have been analyzed for a variety of different equation of states and initial neutron star mass values. The evolution of the various properties of the HMNS as it approaches the collapse to a black hole will be discussed. |
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Pdf file |
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