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:
-
[1];
[3];
[4];
[4]
- 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)
- Univ. of California, Los Angeles, CA (United States); Univ. of Tokyo (Japan)
- RIKEN, Saitama (Japan)
- 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. 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. 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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