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Physical Restrictions to Cosmological Gamma-Ray Burst Models

  • G.S. Bisnovatyi-Kogan
Conference paper
Part of the Springer Proceedings in Physics book series (SPPHY, volume 99)

Summary

The present common view about GRB origin is related to cosmology, and is based on statistical analysis, and on measurements of the redshifts in the GRB optical afterglows of long GRB. No correlation is found between redshifts, GRB spectrum, and total GRB fluence. Comparison of KONUS and BATSE data about statistics and hard X-ray lines is done, and some differences are noted. Hard gamma-ray afterglows, prompt optical spectra, hard X-ray lines, polarization measurements could be very important for farther insight into GRB origin. Possible connection of short GRB with soft gamma repeaters is discussed.

Keywords

Black Hole Collimation Angle Optical Luminosity Optical Afterglow Cosmological Origin 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2005

Authors and Affiliations

  • G.S. Bisnovatyi-Kogan
    • 1
  1. 1.Space Research InstituteRussian Academy of ScienceMoscowRussia

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