Saturated Compton cooling model of cosmological gamma-ray bursts

Details Saturated Compton cooling model of cosmological gamma-ray bursts Saturated Compton cooling model of cosmological gamma-ray bursts

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..428..813l&link_type=abstract

Fourth Huntsville gamma-ray burst symposium. AIP Conference Proceedings, Volume 428, pp. 813-814 (1998).

Astronomy and Astrophysics

Astrophysics

1

Gamma-Ray Sources, Gamma-Ray Bursts, Fundamental Aspects Of Astrophysics

Scientific paper

We generalize the saturated Compton cooling model of gamma-ray burst spectral evolution to the cosmological context. In order for this model to be self-consistent, the Compton cooling plasma must be a relativistically expanding thin shell of bulk Lorentz factor >102, consisting of mostly thermal leptons of keV comoving temperature and less than a few percent nonthermal population.

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