Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2009-01-14
Phys.Rev.D79:021301,2009
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
4 pages, accepted for publication in Phys. Rev. D as a Rapid Communication
Scientific paper
10.1103/PhysRevD.79.021301
For an unsteady baryonic gamma-ray burst (GRB) outflow, the fast and slow proton shells collide with each other and produce energetic soft gamma-ray emission. If the outflow has a significant neutron component, the ultra-relativistic neutrons initially expand freely until decaying at a larger radius. The late time proton shells ejected from the GRB central engine, after powering the regular internal shocks, will sweep these $\beta-$decay products and give rise to very bright UV/optical emission. The naked-eye optical flash from GRB 080319B, an energetic explosion in the distant universe, can be well explained in this way.
Fan Yi-Zhong
Wei Da-Ming
Zhang Bing
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