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- W2018628636 abstract "Gamma-ray bursts (GRBs) are presumed to be powered by the still unknown central engines with timescales in the range from 1 ms to approximately a few seconds. We propose that the GRB central engines would be a viable site for strong meson synchrotron emission if they were compact astrophysical objects, such as neutron stars or rotating black holes with extremely strong magnetic fields (H ~ 1012-1017 G), and if protons or heavy nuclei were accelerated to ultrarelativistic energies on the order of ~1012-1022 eV. We show that the charged scalar mesons like π± and heavy vector mesons like ρ, which have several decay modes onto π±, could be emitted, with a high intensity that is a thousand times larger than photons, through strong couplings to ultrarelativistic nucleons. These meson synchrotron emission processes eventually produce a burst of very high energy cosmic neutrinos with 1012 eV ≤ Eν. These neutrinos are to be detected during the early-time duration of short GRBs." @default.
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- W2018628636 date "1999-11-10" @default.
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- W2018628636 title "Meson Synchrotron Emission from Central Engines of Gamma-Ray Bursts with Strong Magnetic Fields" @default.
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- W2018628636 doi "https://doi.org/10.1086/312348" @default.
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