Nucleosynthesis in gamma-ray bursts outflows
arXiv:astro-ph/0205093 · doi:10.1051/0004-6361:20020939
Abstract
It is shown that fusion of neutrons and protons to He-4 nuclei occurs in gamma-ray burst outflows in a process similar to big-bang nucleosynthesis in the early Universe. Only the surviving free neutrons can then decouple kinematically from the charged fluid so that the multi-GeV neutrino signal predicted from inelastic nuclear n-p collisions is significantly reduced. It is also argued that a sizeable fraction of ultra-high energy cosmic rays accelerated in gamma-ray bursts should be He-4 nuclei.
4 pages, v2: minor modifications, to appear in A&A Letters
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