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Paper detail

Multimessengers from 3D Core-Collapse Supernovae

We present gravitational wave and neutrino signatures obtained in our first principle 3D core-collapse supernova simulation of 15M non-rotating progenitor with Chimera code. Observations of neutrinos emitted by the forming neutron star, and gravitational waves, which are produced by hydrodynamic instabilities is the only way to get direct information about the supernova engine. Both GW and neutrino signals show different phases of supernova evolution.

preprint2015arXivOpen access
Konstantin N. YakuninPedro MarronettiAnthony MezzacappaO. E. Bronson MesserEric J. LentzStephen W. BruennW. Raphael HixJ. Austin Harris
astro-ph.HE
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Open access8 authors1 topic
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Konstantin N. YakuninPedro MarronettiAnthony MezzacappaO. E. Bronson MesserEric J. LentzStephen W. BruennW. Raphael HixJ. Austin Harris

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