Gamma-ray bursts from closed and filled neutron star magnetospheres

Details Gamma-ray bursts from closed and filled neutron star magnetospheres Gamma-ray bursts from closed and filled neutron star magnetospheres

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..428..808b&link_type=abstract

Fourth Huntsville gamma-ray burst symposium. AIP Conference Proceedings, Volume 428, pp. 808-812 (1998).

Mathematics

Logic

Gamma-Ray Sources, Gamma-Ray Bursts, Neutron Stars, Radiation Mechanisms, Polarization

Scientific paper

The beaming of curvature radiation from closed and filled neutron star magnetospheres can overcome a number of well-known problems associated with older γ-ray burst models invoking dead pulsars. Our calculations naturally explain the spectral evolution of γ-ray bursts, while sufficiently reducing the energy required to produce them as compared to isotropic emission, making it possible to observe these events at cosmological distances.

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