Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO's fifth science run
2009
Brooks, A. | Hosken, D. | Munch, J. | Ottaway, D. | Veitch, P. | Abbott, B. | Abbott, R. | Adhikari, R. | Ajith, P. | Allen, B. | Allen, G. | Amin, R. | Anderson, S. | Anderson, W. | Arain, M. | Araya, M. | Armandula, H. | Armor, P. | Aso, Y. | Aston, S. | et al.
We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35M⊙, using LIGO observations between November 14, 2006 and May 18, 2007. No gravitational-wave signals were detected. We report upper limits on the rate of compact binary coalescence as a function of total mass. The LIGO cumulative 90%-confidence rate upper limits of the binary coalescence of neutron stars, black holes and black hole-neutron star systems are 1.4×10-2, 7.3×10-4 and 3.6×10-3 yr-1 L10-1, respectively, where L10 is 1010 times the blue solar luminosity.
Mostrar más [+] Menos [-]B. Abbott... D. J. Hosken... J. Munch... D. J. Ottaway... P. J. Veitch...et al. (LIGO Scientific Collaboration)
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