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Neutrinos from Gamma-ray Bursts
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Gamma-ray bursts (GRBs) are the most luminous electromagnetic burst in the Universe. They occur when a rapidly rotating massive star collapses or a binary neutron star merges. These events leave a newborn central compact object, either a black hole or neutron star, which launches relativistic jets that emit the luminous gamma-ray signals. These jets can accelerate non-thermal protons, which are expected to produce high-energy neutrinos via photohadronic interactions. This Chapter briefly summarizes the current physical picture of GRBs, and discusses neutrino emissions from GRBs, including both prompt and afterglow phases. Neutrinos from sub-classes of GRBs, including low-luminosity GRBs and short GRBs, are also discussed.
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Cited by 2 Pith papers
-
Constraints on Cosmic Rays Acceleration in Bright Gamma-ray Bursts with Observations of Fermi
Using Fermi-LAT GeV upper limits, the baryon loading factor of 12 bright GRBs is constrained to below about 10 in the standard parameter space, challenging GRBs as the dominant UHECR source.
- Testing the universality of quantum gravity theories with cosmic messengers in the context of DSR theories
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