Exploring the Fate of Stellar Core Collapse with Supernova Relic Neutrinos

被引:11
作者
Ashida, Yosuke [1 ,2 ]
Nakazato, Kenichiro [3 ]
机构
[1] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[2] Univ Wisconsin, Wisconsin IceCube Particle Astrophys Ctr, Madison, WI 53706 USA
[3] Kyushu Univ, Fac Arts & Sci, Fukuoka 8190395, Japan
关键词
NUCLEAR-EQUATION; MASS-DISTRIBUTION; NEUTRON-STAR; WHITE-DWARFS; SIMULATIONS; BURST; TELESCOPE; EVOLUTION; 1987A;
D O I
10.3847/1538-4357/ac8a46
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Core collapse of massive stars leads to different fates for various physical factors, which gives different spectra of the emitted neutrinos. We focus on the supernova relic neutrinos (SRNs) as a probe to investigate the stellar collapse fate. We present the SRN fluxes and event rate spectra at a detector for three resultant states after stellar core collapse, the typical mass neutron star, the higher mass neutron star, or the failed supernova forming a black hole, based on different nuclear equations of state. Then possible SRN fluxes are formed as mixtures of the three components. We also show the expected sensitivities at the next-generation water-based Cherenkov detectors, SK-Gd and Hyper-Kamiokande, as constraining the mixture fractions. This study provides a practical example of extracting astrophysical constraints through SRN measurement.
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页数:11
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