Gamma-ray bursts from coalescing strange stars

Details Gamma-ray bursts from coalescing strange stars Gamma-ray bursts from coalescing strange stars

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991nuphs..24..162h&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 24, Issue 2, p. 162-165.

Physics

Nuclear Physics

Scientific paper

The rate of collisions between the neutron stars is ~ 10-4 yr-1 in our Galaxy, and ~ 105 yr-1 within the Hubble distance. The collisions are the final phases of binary orbit decay driven by gravitational radiation. If strange stars exist then their collisions must release ~ 1050 erg in gamma-rays over ~ 0.2 s. Such events should be detectable out to ~ 1 Gpc with the current instruments.

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