Producing the universal spectrum of cosmological gamma-ray bursts with the Klein-Nishina cross section

Details Producing the universal spectrum of cosmological gamma-ray bursts with the Klein-Nishina cross section Producing the universal spectrum of cosmological gamma-ray bursts with the Klein-Nishina cross section

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...428...21b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 428, no. 1, p. 21-27

Astronomy and Astrophysics

Astronomy

42

Astronomical Models, Color-Color Diagram, Compton Effect, Cosmology, Gamma Ray Bursts, Power Spectra, Black Holes (Astronomy), Galactic Bulge, Lorentz Gas, Molecular Clouds, Optical Thickness

Scientific paper

A power-law spectrum attenuated through Compton scattering by an optically thick medium produces spectra that have a characteristic energy of several hundred keV. Add a redshift, and one finds that this model can qualitatively reproduce the color-color diagrams found for individual gamma-ray bursts. This model is easily tested through model fits to burst spectra and through comparisons of the parameters derived from model fits to the limits on parameters derived from the burst log N - log Pmax curve. The heavy attenuation makes the amount of energy released in the burst approximately equal to 103 times larger than is inferred from the observed flux. The requirements of high optical depth and no photon-photon pair creation place a lower limit on the size of the scattering region. This size suggests that the attenuation occurs in giant molecular clouds in the cores of galaxies. This indicates that gamma-ray bursts are probably from supermassive black holes. If the Lorentz factor of the radiation source is large, the optical depth, and therefore the hardness ratio of a burst, can change over the duration of the burst.

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