RED-SUPERGIANT AND SUPERNOVA RATE PROBLEMS: IMPLICATION FOR THE RELIC SUPERNOVA NEUTRINO SPECTRUM

被引：17

作者：

Hidaka, J. ^{[1
,2
]}

Kajino, T. ^{[2
,3
]}

Mathews, G. J. ^{[2
,4
]}

机构：

[1] Meisei Univ, Dept Mech Engn, 2-1-1 Hodokubo, Hino, Tokyo 1918506, Japan

[2] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[3] Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan

[4] Univ Notre Dame, Dept Phys, Ctr Astrophys, Notre Dame, IN 46556 USA

来源：

ASTROPHYSICAL JOURNAL | 2016年 / 827卷 / 01期

关键词：

diffuse radiation; neutrinos; stars: formation; stars: massive; supernovae: general; CORE-COLLAPSE SUPERNOVAE; STAR-FORMATION RATE; EQUATION-OF-STATE; GAMMA-RAY BURSTS; PROGENITOR; CONSTRAINTS; EVOLUTION; LUMINOSITY; MECHANISM; HISTORY;

D O I：

10.3847/0004-637X/827/1/85

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Direct observations of core-collapse supernovae (SNe) and their red supergiant (RSG) progenitors suggest that the upper mass limit of RSGs may be only about 16.5-18M(circle dot), while the standard theoretical value is as much as 25M(circle dot). We investigate the possibility that RSGs with m > 16.5-18M(circle dot) end their lives as failed supernovae (fSNe) and analyze their contribution to the relic supernova neutrino spectrum. We show that adopting this mass limit simultaneously solves both the RSG problem and the supernova rate problem. In addition, energetic neutrinos that originated from fSNe are sensitive to the explosion mechanism, and in particular, to the nuclear equation of state (EOS). We show that this solution to the RSG problem might also be used to constrain the EOS for failed supernovae.

引用

页数：6

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