Neutrinos from decaying muons, pions, neutrons and kaons in gamma ray bursts
R Moharana, N Gupta - Astroparticle Physics, 2012 - Elsevier
In the internal shock model of gamma ray bursts ultrahigh energy muons, pions, neutrons
and kaons are likely to be produced in the interactions of shock accelerated relativistic
protons with low energy photons (KeV–MeV). These particles subsequently decay to high
energy neutrinos/antineutrinos and other secondaries. In the high internal magnetic fields of
gamma ray bursts, the ultrahigh energy charged particles (μ+, π+, K+) lose energy
significantly due to synchrotron radiations before decaying into secondary high energy …
and kaons are likely to be produced in the interactions of shock accelerated relativistic
protons with low energy photons (KeV–MeV). These particles subsequently decay to high
energy neutrinos/antineutrinos and other secondaries. In the high internal magnetic fields of
gamma ray bursts, the ultrahigh energy charged particles (μ+, π+, K+) lose energy
significantly due to synchrotron radiations before decaying into secondary high energy …
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