Physics
Scientific paper
Apr 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..aprb10007m&link_type=abstract
American Physical Society, APS April Meeting, April 16-19, 2005, abstract #B10.007
Physics
Scientific paper
The LIGO Scientific Collaboration is currently involved in various searches for gravitational waves from coalescences of low-mass binary systems. In this talk we report on the search for coalescences of neutron star binaries, with component masses between 1 and 3 solar masses, and on the search for coalescences of primordial black hole binaries, with component masses between 0.2 and 1 solar masses, using the data from the second science run of the 3 LIGO intereferometers. No candidate gravitational wave signals were identified. The results have been used to calculate upper limits on the rate of low-mass compact binary coalescences in the universe.
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