作者
B Abbott, Robert Abbott, Rana Adhikari, J Agresti, P Ajith, B Allen, R Amin, SB Anderson, WG Anderson, M Arain, M Araya, H Armandula, M Ashley, S Aston, P Aufmuth, C Aulbert, S Babak, S Ballmer, H Bantilan, BC Barish, C Barker, D Barker, B Barr, Pablo Barriga, MA Barton, K Bayer, K Belczynski, J Betzwieser, PT Beyersdorf, B Bhawal, IA Bilenko, G Billingsley, R Biswas, E Black, K Blackburn, L Blackburn, David Blair, B Bland, J Bogenstahl, L Bogue, R Bork, V Boschi, S Bose, PR Brady, VB Braginsky, JE Brau, M Brinkmann, A Brooks, DA Brown, A Bullington, A Bunkowski, A Buonanno, O Burmeister, D Busby, WE Butler, RL Byer, L Cadonati, G Cagnoli, JB Camp, J Cannizzo, K Cannon, CA Cantley, J Cao, L Cardenas, K Carter, MM Casey, G Castaldi, C Cepeda, E Chalkey, P Charlton, S Chatterji, S Chelkowski, Y Chen, Francesco Chiadini, D Chin, E Chin, J Chow, N Christensen, James Clark, P Cochrane, Thomas Cokelaer, CN Colacino, R Coldwell, Roberto Conte, D Cook, T Corbitt, David Coward, D Coyne, JDE Creighton, TD Creighton, RP Croce, DRM Crooks, AM Cruise, A Cumming, J Dalrymple, E D’Ambrosio, K Danzmann, Geraint Davies, D DeBra, Jerome Degallaix, T Demma, V Dergachev, S Desai, R Desalvo, S Dhurandhar, M Díaz, J Dickson, A Di Credico, G Diederichs, Alexander Dietz, EE Doomes, RWP Drever, J-C Dumas, RJ Dupuis, JG Dwyer, P Ehrens, E Espinoza, T Etzel, M Evans, T Evans, Stephen Fairhurst, Y Fan, D Fazi, MM Fejer, LS Finn, V Fiumara, N Fotopoulos, A Franzen, KY Franzen, A Freise, R Frey, T Fricke, P Fritschel, VV Frolov, M Fyffe, V Galdi, KS Ganezer, J Garofoli, I Gholami, JA Giaime, S Giampanis, KD Giardina, K Goda, E Goetz, L Goggin, G González, S Gossler, A Grant, Slawomir Gras, C Gray
发表日期
2008/3/7
期刊
Physical Review D
卷号
77
期号
6
页码范围
062002
出版商
American Physical Society
简介
We report on a search for gravitational waves from the coalescence of compact binaries during the third and fourth LIGO science runs. The search focused on gravitational waves generated during the inspiral phase of the binary evolution. In our analysis, we considered three categories of compact binary systems, ordered by mass:(i) primordial black hole binaries with masses in the range 0.35 M⊙< m 1, m 2< 1.0 M⊙,(ii) binary neutron stars with masses in the range 1.0 M⊙< m 1, m 2< 3.0 M⊙, and (iii) binary black holes with masses in the range 3.0 M⊙< m 1, m 2< m max with the additional constraint m 1+ m 2< m max, where m max was set to 40.0 M⊙ and 80.0 M⊙ in the third and fourth science runs, respectively. Although the detectors could probe to distances as far as tens of Mpc, no gravitational-wave signals were identified in the 1364 hours of data we analyzed. Assuming a binary population with a …
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B Abbott, R Abbott, R Adhikari, J Agresti, P Ajith… - Physical Review D, 2008