SIMBAD references

2000ApJ...541..707W - Astrophys. J., 541, 707-711 (2000/October-1)

Neutrino afterglow from gamma-ray bursts: ∼10¹⁸ eV.

WAXMAN E. and BAHCALL J.N.

Abstract (from CDS):

We show that a significant fraction of the energy of a γ-ray burst (GRB) is probably converted to a burst of 10¹⁷-10¹⁹ eV neutrinos and multiple GeV γ-rays that follow the main GRB by ∼10 s. If GRBs accelerate protons to ∼10²⁰ eV, a suggestion that recently gained support from observations of GRB afterglows, then both the neutrinos and the γ-rays may be detectable.

Abstract Copyright: ∼

Journal keyword(s): Acceleration of Particles - Elementary Particles - Gamma Rays: Bursts

Simbad objects: 1

Full paper

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