Comparison of simulated neutrino emission models with data on Supernova 1987A

被引：7

作者：

Olsen, Jackson ^{[1
]}

Qian, Yong-Zhong ^{[1
]}

机构：

[1] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA

来源：

PHYSICAL REVIEW D | 2021年 / 104卷 / 12期

关键词：

SN; 1987A; BURST; OSCILLATIONS; DISTANCE;

D O I：

10.1103/PhysRevD.104.123020

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We compare models of supernova (SN) neutrino emission with the Kamiokande II data on SN 1987A using the Bayesian approach. These models are taken from simulations and are representative of current one-dimensional SN models. We find that models with a brief accretion phase of neutrino emission are the most favored. This result is not affected by varying the overall flux normalization or considering neutrino oscillations. We also check the compatibility of the best-fit models with the data.

引用

页数：7

共 50 条

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SATO, K
SUZUKI, H
PHYSICAL REVIEW LETTERS, 1987, 58 (25) : 2722 - 2725
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Beacom, John F.
Roberts, Luke F.
Capozzi, Francesco
PHYSICAL REVIEW D, 2024, 109 (08)
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