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• W1968939111 abstract "Highly relativistic jets are a key element of current gamma-ray burst models, where the jet kinetic energy is converted to radiation energy at optically thin shocks. High-energy neutrinos are also expected, from interactions of protons accelerated in the same shocks. Here we revisit the early evolution of a relativistic jet, while the jet is still inside the star, and investigate its neutrino emission. In particular we study propagation of mildly relativistic and ultrarelativistic jets through a type Ib progenitor, and follow reverse shocks as the jets cross the star. We show that protons can be accelerated to ${10}^{4}--{10}^{5}text{ }text{ }mathrm{GeV}$ at reverse shocks, and efficiently produce mesons. The mesons experience significant cooling, suppressing subsequent neutrino emission. We show, however, that the neutrino yield from the reverse shock is still reasonably large, especially for low-luminosity and long-duration jets, where meson cooling is less severe. We discuss implications of our results in the context of neutrinos from choked jets, which are completely shock heated and do not break out of the star. From a choked jet with isotropic equivalent energy of ${10}^{53}text{ }text{ }mathrm{erg}$ at 10 Mpc, we expect $ensuremath{sim}20$ neutrino events at IceCube." @default.
• W1968939111 created "2016-06-24" @default.
• W1968939111 creator A5044567744 @default.
• W1968939111 creator A5074726619 @default.
• W1968939111 date "2008-03-24" @default.
• W1968939111 modified "2023-10-10" @default.
• W1968939111 title "High-energy neutrinos from reverse shocks in choked and successful relativistic jets" @default.
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• W1968939111 doi "https://doi.org/10.1103/physrevd.77.063007" @default.
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