Constraining the fraction of core-collapse supernovae harbouring choked jets with high-energy neutrinos

被引：21

作者：

Guetta, Dafne ^{[1
]}

Rahin, Roi ^{[2
]}

Bartos, Imre ^{[3
]}

Della Valle, Massimo ^{[4
,5
]}

机构：

[1] ORT Braude, IL-216002 Karmiel, Israel

[2] Technion, IL-3200003 Haifa, Israel

[3] Univ Florida, Dept Phys, POB 118440, Gainesville, FL 32611 USA

[4] INAF Naples, Capodimonte Observ, Salita Moiariello 16, I-80131 Naples, Italy

[5] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2020年 / 492卷 / 01期

关键词：

gravitational waves; stars: neutron; GAMMA-RAY BURSTS;

D O I：

10.1093/mnras/stz3245

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The joint observation of core-collapse supernovae with gamma-ray bursts shows that jets can be launched in the aftermath of stellar core collapse, likely by a newly formed black hole that accretes matter from the star. Such gamma-ray bursts have only been observed accompanying Type Ibc supernovae, indicating a stellar progenitor that lost its hydrogen envelope before collapse. According to recent hypothesis, it is possible that jets are launched in core-collapse events even when the progenitors still retain their hydrogen envelopes; however, such jets are not able to burrow through the star and will be stalled into the interior of the progenitor star before escaping. These jets are called choked jets. High-energy neutrinos produced by such choked jets could escape the stellar envelope and could be observed. Here, we examine how multimessenger searches for high-energy neutrinos and core-collapse supernovae can detect or limit the fraction of stellar collapses that produce jets. We find that a high fraction of jet production is already limited by previous observational campaigns. We explore possibilities with future observations using Large Synoptic Survey Telescope, IceCube, and Km3NET.

引用

页码：843 / 847

页数：5

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