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100 GeV Photons from Gamma-Ray Burst Fireballs

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Gamma-Ray Bursts in the Afterglow Era

Part of the book series: ESO ASTROPHYSICS SYMPOSIA ((ESO))

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Abstract.

We find that there is an efficient way of generating high energy photons (from sub-GeV to 100 GeV) in fireballs of Gamma-Ray Bursts (GRBs). We present analytic theory of the phenomenon, obtain the expected spectra and derive their parameters. The radiation of this kind carries an essential information about GRB sources and can be detected by means of existing (or planned) instruments.

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Enrico Costa Filippo Frontera Jens Hjorth

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Kocharovsky, V.V., Derishev, E.V., Kocharovsky, V.V. 100 GeV Photons from Gamma-Ray Burst Fireballs. In: Costa, E., Frontera, F., Hjorth, J. (eds) Gamma-Ray Bursts in the Afterglow Era. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10853853_93

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  • DOI: https://doi.org/10.1007/10853853_93

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-42771-1

  • Online ISBN: 978-3-540-45505-9

  • eBook Packages: Springer Book Archive

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