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

Journal Article · · The Astrophysical Journal (Online)
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); DOE/OSTI
  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)
+ Show Author Affiliations

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.

Research Organization:
Univ. of California, Los Angeles, CA (United States)
Sponsoring Organization:
National Natural Science of China (NNSFC); USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
Grant/Contract Number:
SC0009937
OSTI ID:
1542021
Journal Information:
The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 2 Vol. 856; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English

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Cited By (14)

Estimating the neutrino flux from choked gamma-ray bursts journal September 2021
Tidally disrupted stars as a possible origin of both cosmic rays and neutrinos at the highest energies text January 2017
Astrophysics Uniquely Enabled by Observations of High-Energy Cosmic Neutrinos text January 2019
Tidally disrupted stars as a possible origin of both cosmic rays and neutrinos at the highest energies journal July 2018
Scale dependence of energy transfer in turbulent plasma journal November 2018
Constraining the fraction of core-collapse supernovae harbouring choked jets with high-energy neutrinos journal January 2020
Multimessenger tests of cosmic-ray acceleration in radiatively inefficient accretion flows journal October 2019
Tidally disrupted stars as a possible origin of both cosmic rays and neutrinos at the highest energies text January 2017
Tidally disrupted stars as a possible origin of both cosmic rays and neutrinos at the highest energies text January 2018
On the common origin of cosmic rays across the ankle and diffuse neutrinos at the highest energies from low-luminosity Gamma-Ray Bursts text January 2018
On the Common Origin of Cosmic Rays across the Ankle and Diffuse Neutrinos at the Highest Energies from Low-luminosity Gamma-Ray Bursts journal February 2019
Tidally disrupted stars as a possible origin of both cosmic rays and neutrinos at the highest energies text January 2017
Scale dependence of energy transfer in turbulent plasma text January 2018
Constraining the Fraction of Core-Collapse Supernovae Harboring Choked Jets with High-energy Neutrinos text January 2019

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