The Thomson limit of resonant inverse Compton scattering in the strong magnetic fields of neutron stars is considered as a mechanism for producing gamma-ray burst continuum spectra. Photon production spectra and electron cooling rates are presented using the full magnetic Thomson cross-section. Model emission spectra are obtained as self-consistent solutions of a set of photon and electron kinetic equations, displaying spectral breaks and other structure at gamma-ray energies.


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    Titel :

    Resonant Compton scattering and gamma-ray burst continuum spectra


    Beteiligte:
    Baring, M. G. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.05.1995



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Resonant Compton Scattering and Gamma-Ray Burst Continuum Spectra

    Baring, M. G. / Committee on Space Research; Scientific Commission E | British Library Conference Proceedings | 1995





    On the continuum shape of gamma-ray burst energy spectra

    Eveno, E. / Barat, C. / Chambon, G. et al. | Elsevier | 1986