In the neutron-rich internal shocks model for gamma-ray bursts (GRBs), the Lorentz factors (LFs) of ion shells are variable, and so are the LFs of accompanying neutron shells. For slow neutron shells with a typical
CITATION STYLE
Fan, Y. Z., & Wei, D. M. (2004). The Ultraviolet Flash Accompanying Gamma-Ray Bursts from Neutron-rich Internal Shocks. The Astrophysical Journal, 615(2), L69–L72. https://doi.org/10.1086/426476
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