Search for Gravitational Waves from Low Mass Binary Coalescences In the First Year of LIGO's S5 Data
Document Type
Article
Publication Date
6-5-2009
Journal / Book Title
Physical Review D
Abstract
We have searched for gravitational waves from coalescing low mass compact binary systems with a total mass between 2M and 35 and a minimum component mass of 1M using data from the first year of the fifth science run of the three LIGO detectors, operating at design sensitivity. Depending on the mass, we are sensitive to coalescences as far as 150Mpc from the Earth. No gravitational-wave signals were observed above the expected background. Assuming a population of compact binary objects with a Gaussian mass distribution representing binary neutron star systems, black hole-neutron star binary systems, and binary black hole systems, we calculate the 90% confidence upper limit on the rate of coalescences to be 3.9×10-2yr-1L10-1, 1.1×10-2yr-1L10-1, and 2.5×10-3yr-1L10-1, respectively, where L10 is 1010 times the blue solar luminosity. We also set improved upper limits on the rate of compact binary coalescences per unit blue-light luminosity, as a function of mass.
DOI
10.1103/PhysRevD.79.122001
MSU Digital Commons Citation
Abbott, B. P.; Abbott, R.; Adhikari, R.; Ajith, P.; Allen, B.; Allen, G.; Amin, R. S.; Anderson, S. B.; Anderson, W. G.; and Martin, Rodica, "Search for Gravitational Waves from Low Mass Binary Coalescences In the First Year of LIGO's S5 Data" (2009). Department of Physics and Astronomy Faculty Scholarship and Creative Works. 118.
https://digitalcommons.montclair.edu/physics-astron-facpubs/118
Published Citation
Abbott, B. P., Abbott, R., Adhikari, R., Ajith, P., Allen, B., Allen, G., ... & Giaime, J. A. (2009). Search for gravitational waves from low mass binary coalescences in the first year of LIGO’s S5 data. Physical Review D, 79(12), 122001.