Gamma-ray bursts from comet-antimatter comet collisions in the Oort cloud

Details Gamma-ray bursts from comet-antimatter comet collisions in the Oort cloud Gamma-ray bursts from comet-antimatter comet collisions in the Oort cloud

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..384..744d&link_type=abstract

Gamma-ray bursts: 3rd Huntsville symposium. AIP Conference Proceedings, Volume 384, pp. 744-748 (1996).

Physics

2

Gamma-Ray Sources, Gamma-Ray Bursts, Elementary Particle Processes

Scientific paper

The measured isotropy and inhomogeneity of gamma-ray bursts can be
explained by cometary collisions in the Oort cloud at ~104 AU
from the Sun, provided that ~10-3 of the mass in small comets
is in the form of antimatter. Gamma-ray bursts may therefore signal the
existence of bulk antimatter in the local Solar neighborhood.

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