GRB as a counterpart for Gravitational Wave detection in LCGT

Details GRB as a counterpart for Gravitational Wave detection in LCGT GRB as a counterpart for Gravitational Wave detection in LCGT

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1279..349k&link_type=abstract

DECIPHERING THE ANCIENT UNIVERSE WITH GAMMA-RAY BURSTS. AIP Conference Proceedings, Volume 1279, pp. 349-351 (2010).

Other

Gamma-Ray Sources (Astronomical), Neutron Stars, Black Holes, Gravitational Waves, Gamma-Ray Sources, Gamma-Ray Bursts, Neutron Stars, Galactic Nuclei, Circumnuclear Matter, And Bulges, Gravitational Radiation, Magnetic Fields, And Other Observations

Scientific paper

Short Gamma-ray burst (GRB) progenitors are considered as merger of compact star binaries which consist of neutron stars or blackholes. These compact star binaries will radiate a strong gravitational wave in their coalescence, and gravitational wave detectors aim to detect them. We studied the chance probability of coincidence between GRB and GW detection in LCGT detector. Due to omni-directional acceptance of GW detectors, about 75% of GRB events which closer than cosmological redshift z<0.1 are expected to confirm by GW detection.

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