Abstract It is widely accepted that the prompt transient signal in the 10keV–10GeV band from gamma-ray bursts (GRBs) arises from multiple shocks internal to the ultra-relativistic expansion. The detailed understanding of the dissipation and accompanying acceleration at these shocks is a currently topical subject. This paper explores the relationship between GRB prompt emission spectra and the electron (or ion) acceleration properties at the relativistic shocks that pertain to GRB models. The focus is on the array of possible high-energy power-law indices in accelerated populations, highlighting how spectra above 1MeV can probe the field obliquity in GRB internal shocks, and the character of hydromagnetic turbulence in their environs. It is emphasized that diffusive shock acceleration theory generates no canonical spectrum at relativistic MHD discontinuities. This diversity is commensurate with the significant range of spectral indices discerned in prompt burst emission. Such system diagnostics are now being enhanced by the broad-band spectral coverage of bursts by the Fermi Gamma-Ray Space Telescope; while the Gamma-Ray Burst Monitor (GBM) provides key diagnostics on the lower energy portions of the particle population, the focus here is on constraints in the non-thermal, power-law regime of the particle distribution that are provided by the Large Area Telescope (LAT).
Using gamma-ray burst prompt emission to probe relativistic shock acceleration
Advances in Space Research ; 47 , 8 ; 1427-1433
2010-02-11
7 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Using gamma-ray burst prompt emission to probe relativistic shock acceleration
Online Contents | 2011
|Gamma-ray burst prompt emission: Implications from shock acceleration theory
Online Contents | 2006
|