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Title: Neutrinos from Choked Jets Accompanied by Type-II Supernovae

Abstract

The origin of the IceCube neutrinos is still an open inquiry. Upper limits from diffuse gamma-ray observations predict that the neutrino sources are either distant or hidden from gamma-ray observations. It is possible that the neutrinos are produced in jets that are formed in core-collapsing massive stars and fail to break out, the so-called choked jets. We report neutrinos from the jets choked in the hydrogen envelopes of red supergiant stars. Fast photo-meson cooling softens the neutrino spectrum, making it hard to explain the PeV neutrinos observed by IceCube in a one-component scenario, but a two-component model can explain the spectrum. Moreover, we predict that a newly born jet-driven type-II supernova may be observed to be associated with a neutrino burst detected by IceCube.

Authors:
ORCiD logo [1];  [2]; ORCiD logo [3]; ORCiD logo [4]; ORCiD logo [4]
  1. Chinese Academy of Sciences (CAS), Nanjing (China). Purple Mountain Observatory; RIKEN, Saitama (Japan); Univ. of California, Los Angeles, CA (United States); Univ. of Science and Technology of China, Hefei (China)
  2. Univ. of California, Los Angeles, CA (United States); Univ. of Tokyo (Japan)
  3. RIKEN, Saitama (Japan)
  4. Chinese Academy of Sciences (CAS), Nanjing (China). Purple Mountain Observatory; Univ. of Science and Technology of China, Hefei (China)
Publication Date:
Research Org.:
Univ. of California, Los Angeles, CA (United States)
Sponsoring Org.:
National Natural Science of China (NNSFC); USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1542021
Grant/Contract Number:  
SC0009937
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 856; Journal Issue: 2; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; neutrinos; stars: jets; stars: massive; supergiants; supernovae: general

Citation Formats

He, Hao-Ning, Kusenko, Alexander, Nagataki, Shigehiro, Fan, Yi-Zhong, and Wei, Da-Ming. Neutrinos from Choked Jets Accompanied by Type-II Supernovae. United States: N. p., 2018. Web. doi:10.3847/1538-4357/aab360.
He, Hao-Ning, Kusenko, Alexander, Nagataki, Shigehiro, Fan, Yi-Zhong, & Wei, Da-Ming. Neutrinos from Choked Jets Accompanied by Type-II Supernovae. United States. doi:https://doi.org/10.3847/1538-4357/aab360
He, Hao-Ning, Kusenko, Alexander, Nagataki, Shigehiro, Fan, Yi-Zhong, and Wei, Da-Ming. Fri . "Neutrinos from Choked Jets Accompanied by Type-II Supernovae". United States. doi:https://doi.org/10.3847/1538-4357/aab360. https://www.osti.gov/servlets/purl/1542021.
@article{osti_1542021,
title = {Neutrinos from Choked Jets Accompanied by Type-II Supernovae},
author = {He, Hao-Ning and Kusenko, Alexander and Nagataki, Shigehiro and Fan, Yi-Zhong and Wei, Da-Ming},
abstractNote = {The origin of the IceCube neutrinos is still an open inquiry. Upper limits from diffuse gamma-ray observations predict that the neutrino sources are either distant or hidden from gamma-ray observations. It is possible that the neutrinos are produced in jets that are formed in core-collapsing massive stars and fail to break out, the so-called choked jets. We report neutrinos from the jets choked in the hydrogen envelopes of red supergiant stars. Fast photo-meson cooling softens the neutrino spectrum, making it hard to explain the PeV neutrinos observed by IceCube in a one-component scenario, but a two-component model can explain the spectrum. Moreover, we predict that a newly born jet-driven type-II supernova may be observed to be associated with a neutrino burst detected by IceCube.},
doi = {10.3847/1538-4357/aab360},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 856,
place = {United States},
year = {2018},
month = {3}
}

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Cited by: 8 works
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