What can we learn from gravitational waves from nearby core-collapse supernovae?

Yudai Suwa, Takaaki Yokozawa, Mitsuhiro Asano, Tsubasa Kayano, Nobuyuki Kanda, Yusuke Koshio, Mark R. Vagins

研究成果査読

抄録

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.

本文言語English
論文番号012009
ジャーナルJournal of Physics: Conference Series
600
1
DOI
出版ステータスPublished - 4月 28 2015
イベントInternational Scientific Conference on Spanish Relativity Meeting: Almost 100 Years After Einstein's Revolution, ERE 2014 - Valencia
継続期間: 9月 1 20149月 5 2014

ASJC Scopus subject areas

  • 物理学および天文学一般

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