Three-Dimensional General-Relativistic Simulations of Neutron Stars

Details Three-Dimensional General-Relativistic Simulations of Neutron Stars Three-Dimensional General-Relativistic Simulations of Neutron Stars

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confr..91b&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 91-91"

Physics

Scientific paper

In addition to the accurate matter and horizon dynamics of the collapse of rotating stars to black holes, we present the first three-dimensional calculations of the gravitational wave emission in such a process. The initial models are polytropes which are dynamically unstable and near the mass-shedding limit. The waveforms have been extracted using a gauge-invariant approach and reflect the properties of both the initial stellar models and of newly produced black holes.

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