作者: Eli Waxman , David Eichler
DOI: 10.1086/430596
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摘要: Afterglow observations are commonly used to determine the parameters of GRB explosions, energy E, surrounding density n, postshock magnetic field equipartition fraction B, and electron e, under frequently made assumption that efficiency "injection" into relativistic shock acceleration is high, i.e., f electrons undergo ≈ 1. We show value cannot be determined by current observations, since currently testable model predictions for a parameter choice {E' = E/f, n' n/f, fB, fe} independent me/mp ≤ Current imply similar highly subrelativistic shocks plausibly suggest ~ 1, quite unlike situation in Crab Nebula. However, values 1 ruled out, implying factor uncertainty determination parameters. early, ≤10 hr, radio afterglow which will far more accessible Swift era, may provide constraints on f. Such therefore powerful diagnostic explosions physics particle collisionless shocks.