Gravitational waves from core-collapse supernova using CHIMERA

Details Gravitational waves from core-collapse supernova using CHIMERA Gravitational waves from core-collapse supernova using CHIMERA

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aps..apr.e8007y&link_type=abstract

American Physical Society, 2008 APS April Meeting and HEDP/HEDLA Meeting, April 11-15, 2008, abstract #E8.007

Physics

Scientific paper

We perform numerical simulations of core-collapse supernova using the multi-dimensional hydrodynamics code CHIMERA that includes realistic nuclear reactions as well as spectral neutrino transport. We present gravitational wave signals from progenitor stars with different rotational profiles, studying the effects of neutrino radiation in the emission of gravitational waves. These GW templates can be used to enhance the search for supernovae signals in current and future GW detectors.

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