期刊
ASTROPHYSICAL JOURNAL LETTERS
卷 848, 期 1, 页码 -出版社
IOP Publishing Ltd
DOI: 10.3847/2041-8213/aa8d14
关键词
binaries: close; gamma-ray burst: general; gravitational waves; neutrinos; stars: neutron
资金
- Alfred P Sloan Foundation
- NSF grant [PHY-1620777]
- NASA [NNX13AH50G]
- IGC post-doctoral fellowship program
- JSPS KAKENHI grant [17H06361, 16H02183, 15K05077]
- post-K computer project of Japanese MEXT [9]
- [YITP-17-96]
- Direct For Mathematical & Physical Scien
- Division Of Physics [1620777] Funding Source: National Science Foundation
- Grants-in-Aid for Scientific Research [15K05077, 17H06357] Funding Source: KAKEN
We investigate current and future prospects for coincident detection of high-energy neutrinos and gravitational waves (GWs). Short gamma-ray bursts (SGRBs) are believed to originate from mergers of compact star binaries involving neutron stars. We estimate high-energy neutrino fluences from prompt emission, extended emission (EE), X-ray flares, and plateau emission, and we show that neutrino signals associated with the EE are the most promising. Assuming that the cosmic-ray loading factor is similar to 10 and the Lorentz factor distribution is lognormal, we calculate the probability of neutrino detection from EE by current and future neutrino detectors, and we find that the quasi-simultaneous detection of high-energy neutrinos, gamma-rays, and GWs is possible with future instruments or even with current instruments for nearby SGRBs having EE. We also discuss stacking analyses that will also be useful with future experiments such as IceCube-Gen2.
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