High-energy neutrinos from the gravitational wave event GW150914 possibly associated with a short gamma-ray burst

被引：15

作者：

Moharana, Reetanjali ^{[1
]}

Razzaque, Soebur ^{[1
]}

Gupta, Nayantara ^{[2
]}

Meszaros, Peter ^{[3
,4
]}

机构：

[1] Univ Johannesburg, Dept Phys, POB 524, ZA-2006 Auckland Pk, South Africa

[2] Raman Res Inst, Bangalore 560080, Karnataka, India

[3] Penn State Univ, Dept Astron & Astrophys, Ctr Particle & Gravitat Astrophys, 525 Davey Lab, University Pk, PA 16802 USA

[4] Penn State Univ, Dept Phys, 104 Davey Lab, University Pk, PA 16802 USA

来源：

PHYSICAL REVIEW D | 2016年 / 93卷 / 12期

基金：

新加坡国家研究基金会;

关键词：

NONDETECTION; EMISSION;

D O I：

10.1103/PhysRevD.93.123011

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

High-energy neutrinos (HEN) and gravitational waves (GW) can probe astrophysical sources in addition to electromagnetic observations. Multimessenger studies can reveal the nature of the sources, which may not be discerned from one type of signal alone. We discuss HEN emission in connection with the Advanced Laser Interferometer Gravitational-Wave Observatory event GW150914, which could be associated with a short gamma-ray burst detected by the Fermi Gamma-Ray Burst Monitor 0.4 s after the GW event and within localization uncertainty of the GWevent. We calculate HEN flux from this short gamma-ray burst, GW150914-GBM, and show that nondetection of a high-energy starting event by the IceCube Neutrino Observatory can constrain the total isotropic-equivalent jet energy of this short burst to be less than 3 x 10(52) erg.

引用

页数：4

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