Neutrino burst from failed supernovae as a promising target of neutrino astronomy

Kohsuke Sumiyoshi, Ken'ichiro Nakazato, Hideyuki Suzuki, Shoichi Yamada

Research output: Contribution to journalConference article

Abstract

We study the unique characteristics of neutrino bursts from the black-hole-forming collapse of non-rotational massive stars, which is a definite branch among other core-collapse supernovae. We clarify that the neutrino signals from the failed supernovae are short and energetic, being different from the ordinary supernova neutrinos, by performing the numerical simulations of the general relativistic neutrino-radiation hydrodynamics with the neutrino reactions rates. Based on the calculated spectra of neutrino emission, we predict that the number of neutrino detection at the Super-Kamiokande is large enough to discuss the detailed differences of the neutrino signals using the sets of equation of state including hyperons and quarks. Therefore, the massive stellar collapse with the short neutrino burst is an important target of neutrino astronomy to probe the properties of dense matter.

Original languageEnglish
JournalProceedings of Science
Publication statusPublished - 2010 Dec 1
Event11th Symposium on Nuclei in the Cosmos, NIC 2010 - Heidelberg, Germany
Duration: 2010 Jul 192010 Jul 23

    Fingerprint

ASJC Scopus subject areas

  • General

Cite this