Search for gravitational waves from binary black hole inspirals in LIGO data

We report on a search for gravitational waves from binary black hole inspirals in the data from the second science run of the LIGO interferometers. The search focused on binary systems with component masses between 3 and 20M{sub {center_dot}}. Optimally oriented binaries with distances up to 1 Mpc c...

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Veröffentlicht in:Physical review. D, Particles and fields Particles and fields, 2006-03, Vol.73 (6), Article 062001
Hauptverfasser: Abbott, B., Abbott, R., Adhikari, R., Ageev, A., Agresti, J., Ajith, P., Allen, B., Allen, J., Amin, R., Anderson, S. B., Anderson, W. G., Araya, M., Armandula, H., Ashley, M., Asiri, F., Aufmuth, P., Aulbert, C., Babak, S., Balasubramanian, R., Ballmer, S., Barish, B. C., Barker, C., Barker, D., Barnes, M., Barr, B., Barton, M. A., Bayer, K., Beausoleil, R., Belczynski, K., Bennett, R., Berukoff, S. J., Betzwieser, J., Bhawal, B., Bilenko, I. A., Billingsley, G., Black, E., Blackburn, K., Blackburn, L., Bland, B., Bochner, B., Bogue, L., Bork, R., Bose, S., Brady, P. R., Braginsky, V. B., Brau, J. E., Brown, D. A., Bullington, A., Bunkowski, A., Buonanno, A., Burgess, R., Busby, D., Butler, W. E., Byer, R. L., Cadonati, L., Cagnoli, G., Camp, J. B., Cannizzo, J., Cannon, K., Cantley, C. A., Cao, J., Cardenas, L., Carter, K., Casey, M. M., Castiglione, J., Chandler, A., Chapsky, J., Charlton, P., Chatterji, S., Chelkowski, S., Chen, Y., Chickarmane, V., Chin, D., Christensen, N., Churches, D., Cokelaer, T., Colacino, C., Coldwell, R., Coles, M., Cook, D., Corbitt, T., Coyne, D., Creighton, J. D. E., Creighton, T. D., Crooks, D. R. M., Csatorday, P., Cusack, B. J., Cutler, C., Dalrymple, J., D’Ambrosio, E., Danzmann, K., Davies, G., Daw, E., DeBra, D., Delker, T., Dergachev, V., Desai, S., DeSalvo, R., Dhurandhar, S., Di Credico, A.
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Sprache:eng
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Zusammenfassung:We report on a search for gravitational waves from binary black hole inspirals in the data from the second science run of the LIGO interferometers. The search focused on binary systems with component masses between 3 and 20M{sub {center_dot}}. Optimally oriented binaries with distances up to 1 Mpc could be detected with efficiency of at least 90%. We found no events that could be identified as gravitational waves in the 385.6 hours of data that we searched.
ISSN:1550-7998
0556-2821
1550-2368
1089-4918
DOI:10.1103/PhysRevD.73.062001