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  Observational Limit on Gravitational Waves from Binary Neutron Stars in the Galaxy

Allen, B., Blackburn, J. K., Brady, P. R., Creighton, J. D. E., Creighton, T., Droz, S., et al. (1999). Observational Limit on Gravitational Waves from Binary Neutron Stars in the Galaxy. Physical Review Letters, 83(8), 1498-1501. doi:10.1103/PhysRevLett.83.1498.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-584A-8 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-584B-6
Genre: Journal Article

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 Creators:
Allen, Bruce1, Author           
Blackburn, J. K., Author
Brady, P. R., Author
Creighton, J. D. E., Author
Creighton, T., Author
Droz, S., Author
Gillespie, A. D., Author
Hughes, S. A., Author
Kawamura, S., Author
Lyons, T. T., Author
Mason, J. E., Author
Owen, B. J., Author
Raab, F., Author
Regehr, M. W., Author
Sathyaprakash, B. S., Author
Savage, R. L., Author
Whitcomb, S., Author
Wiseman, A. G., Author
Affiliations:
1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              

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 Abstract: Using optimal matched filtering, we search 25 hours of data from the LIGO 40-m prototype laser interferometric gravitational-wave detector for gravitational-wave chirps emitted by coalescing binary systems within our Galaxy. This is the first test of this filtering technique on real interferometric data. An upper limit on the rate R of neutron star binary inspirals in our Galaxy is obtained: with 90% confidence, R<0.5 h-1. Similar experiments with LIGO interferometers will provide constraints on the population of tight binary neutron star systems in the Universe.

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 Dates: 1999-03
 Publication Status: Issued
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 Identifiers: eDoc: 404182
DOI: 10.1103/PhysRevLett.83.1498
URI: http://link.aps.org/doi/10.1103/PhysRevLett.83.1498
URI: http://arxiv.org/abs/gr-qc/9903108
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Title: Physical Review Letters
Source Genre: Journal
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Pages: - Volume / Issue: 83 (8) Sequence Number: - Start / End Page: 1498 - 1501 Identifier: ISSN: 1079-7114