Core-collapse supernova is one of the expected sources of gravitational wave (GW). The GW detection can be a smoking gun to probe the still unknown explosion mechanism. In the coming era of "multi-messenger astronomy", we can use photons, neutrinos and GW simultaneously to investigate these objects. By performing multi-dimensional simulations of neutrino-radiation hydrodynamics systematically, we calculate the gravitational wave and neutrino signals from nearby (galactic) core-collapse supernova. Based on these signals we will discuss the extractable information about the very central part of core-collapse supernovae.
|Journal||Journal of Physics: Conference Series|
|Publication status||Published - Apr 28 2015|
|Event||International Scientific Conference on Spanish Relativity Meeting: Almost 100 Years After Einstein's Revolution, ERE 2014 - Valencia, Spain|
Duration: Sep 1 2014 → Sep 5 2014
ASJC Scopus subject areas
- Physics and Astronomy(all)