Supernova neutrino light curves and spectra for various progenitor stars: From core collapse to proto-neutron star cooling

Ken'Ichiro Nakazato*, Kohsuke Sumiyoshi, Hideyuki Suzuki, Tomonori Totani, Hideyuki Umeda, Shoichi Yamada

*この研究の対応する著者

研究成果: Article査読

87 被引用数 (Scopus)

抄録

We present a new series of supernova neutrino light curves and spectra calculated by numerical simulations for a variety of progenitor stellar masses (13-50 M⊙) and metallicities (Z = 0.02 and 0.004), which would be useful for a broad range of supernova neutrino studies, e.g., simulations of future neutrino burst detection by underground detectors or theoretical predictions for the relic supernova neutrino background. To follow the evolution from the onset of collapse to 20 s after the core bounce, we combine the results of neutrino-radiation hydrodynamic simulations for the early phase and quasi-static evolutionary calculations of neutrino diffusion for the late phase, with different values of shock revival time as a parameter that should depend on the still unknown explosion mechanism. We describe the calculation methods and basic results, including the dependence on progenitor models and the shock revival time. The neutrino data are publicly available electronically.

本文言語English
論文番号2
ジャーナルAstrophysical Journal, Supplement Series
205
1
DOI
出版ステータスPublished - 2013 3月

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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