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Signature of collapsars as sources for high-energy neutrinos and r-process nuclei

Gang Guo1,*, Yong-Zhong Qian2,†, and Meng-Ru Wu3,4,‡

  • 1School of Mathematics and Physics, China University of Geosciences, Wuhan 430074, China
  • 2School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
  • 3Institute of Physics, Academia Sinica, Taipei 11529, Taiwan
  • 4Institute of Astronomy and Astrophysics, Academia Sinica, Taipei 10617, Taiwan

  • *guogang@cug.edu.cn
  • †qian@physics.umn.edu
  • ‡mwu@gate.sinica.edu.tw

Phys. Rev. D 108, L021303 – Published 21 July, 2023

DOI: https://doi.org/10.1103/PhysRevD.108.L021303

Abstract

If collapsars are sources for both high-energy (HE) neutrinos and r-process nuclei, then the profuse low-energy antineutrinos from the β decay of the newly synthesized nuclei can annihilate the HE neutrinos. Considering HE neutrinos produced at internal shocks induced by intermittent mildly magnetized jets, we show that such annihilation suppresses the overall HE neutrino spectrum at ≳300  TeV and produces a corresponding flavor composition of (Fνe+ν¯e:Fνμ+ν¯μ:Fντ+ν¯τ)⋆≈(1:10:1) at source. We find that the emergent HE neutrino flux can well fit the diffuse flux observed at IceCube if contributions from all similar sources are taken into account. Our results highlight the unique role of HE neutrinos in supporting collapsars as sources for r-process nuclei, and can be tested by detection of HE neutrinos from individual sources and accurate measurement of the diffuse HE neutrino flux spectrum and flavor composition.

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