dc.identifier.uri |
http://dx.doi.org/10.15488/12048 |
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dc.identifier.uri |
https://www.repo.uni-hannover.de/handle/123456789/12145 |
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dc.contributor.author |
Abbott, B.
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dc.contributor.author |
Abbott, R.
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dc.contributor.author |
Adhikari, R.
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dc.contributor.author |
Agresti, J.
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dc.contributor.author |
Ajith, P.
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dc.contributor.author |
Allen, B.
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dc.contributor.author |
Amin, R.
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dc.contributor.author |
Anderson, S.B.
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dc.contributor.author |
Anderson, W.G.
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dc.contributor.author |
Arain, M.
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dc.contributor.author |
Araya, M.
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dc.contributor.author |
Armandula, H.
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dc.contributor.author |
Ashley, M.
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dc.contributor.author |
Aston, S.
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dc.contributor.author |
Aufmuth, P.
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dc.contributor.author |
Aulbert, C.
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dc.contributor.author |
Babak, S.
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dc.contributor.author |
Ballmer, S.
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dc.contributor.author |
Bantilan, H.
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dc.contributor.author |
Barish, B.C.
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dc.contributor.author |
Barker, C.
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dc.contributor.author |
Barker, D.
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dc.contributor.author |
Barr, B.
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dc.contributor.author |
Barriga, P.
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dc.contributor.author |
Barton, M.A.
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dc.contributor.author |
Bayer, K.
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dc.contributor.author |
Betzwieser, J.
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dc.contributor.author |
Beyersdorf, P.T.
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dc.contributor.author |
Bhawal, B.
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dc.contributor.author |
Bilenko, I.A.
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dc.contributor.author |
Billingsley, G.
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dc.contributor.author |
Biswas, R.
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dc.contributor.author |
Black, E.
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dc.contributor.author |
Blackburn, K.
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dc.contributor.author |
Blackburn, L.
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dc.contributor.author |
Blair, D.
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dc.contributor.author |
Bland, B.
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dc.contributor.author |
Bogenstahl, J.
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dc.contributor.author |
Bogue, L.
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dc.contributor.author |
Bork, R.
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dc.contributor.author |
Boschi, V.
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Bose, S.
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dc.contributor.author |
Brady, P.R.
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dc.contributor.author |
Braginsky, V.B.
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dc.contributor.author |
Brau, J.E.
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dc.contributor.author |
Brinkmann, M.
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dc.contributor.author |
Brooks, A.
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Brown, D.A.
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dc.contributor.author |
Bullington, A.
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Bunkowski, A.
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Buonanno, A.
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Burmeister, O.
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Busby, D.
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Byer, R.L.
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Cadonati, L.
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dc.contributor.author |
Cagnoli, G.
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dc.contributor.author |
Camp, J.B.
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Cannizzo, J.
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Cannon, K.
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Cantley, C.A.
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Cao, J.
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Cardenas, L.
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Castaldi, G.
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Cepeda, C.
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Chalkley, E.
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Charlton, P.
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Chatterji, S.
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Chelkowski, S.
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dc.contributor.author |
Chen, Y.
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Chiadini, F.
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Christensen, N.
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Clark, J.
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Cochrane, P.
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Cokelaer, T.
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Coldwell, R.
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Conte, R.
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dc.contributor.author |
Cook, D.
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Corbitt, T.
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Coyne, D.
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Creighton, J.D.E.
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Croce, R.P.
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Crooks, D.R.M.
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Cruise, A.M.
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Cumming, A.
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Dalrymple, J.
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D’Ambrosio, E.
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Danzmann, K.
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Davies, G.
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DeBra, D.
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Degallaix, J.
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Degree, M.
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Demma, T.
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Dergachev, V.
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Desai, S.
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DeSalvo, R.
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Dhurandhar, S.
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Díaz, M.
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Dickson, J.
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Di Credico, A.
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Diederichs, G.
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Dietz, A.
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Doomes, E.E.
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Drever, R.W.P.
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Dumas, J.-C.
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Dupuis, R.J.
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Dwyer, J.G.
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Ehrens, P.
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Espinoza, E.
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Etzel, T.
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Evans, M.
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dc.contributor.author |
Evans, T.
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dc.contributor.author |
Fairhurst, S.
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dc.contributor.author |
Fan, Y.
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dc.contributor.author |
Fazi, D.
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Fejer, M.M.
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Finn, L.S.
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Fiumara, V.
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dc.contributor.author |
Fotopoulos, N.
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dc.contributor.author |
Franzen, A.
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dc.contributor.author |
Franzen, K.Y.
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Freise, A.
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Frey, R.
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dc.contributor.author |
Fricke, T.
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Fritschel, P.
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Frolov, V.V.
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Fyffe, M.
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Galdi, V.
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dc.contributor.author |
Garofoli, J.
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dc.contributor.author |
Gholami, I.
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Giaime, J.A.
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Giampanis, S.
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Giardina, K.D.
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Goda, K.
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dc.contributor.author |
Goetz, E.
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Goggin, L.M.
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González, G.
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Gossler, S.
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dc.contributor.author |
Grant, A.
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Gras, S.
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Gray, C.
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dc.contributor.author |
Gray, M.
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Greenhalgh, J.
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Gretarsson, A.M.
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Grosso, R.
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Grote, H.
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Grunewald, S.
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Guenther, M.
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dc.contributor.author |
Gustafson, R.
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dc.contributor.author |
Hage, B.
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Hammer, D.
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Hanna, C.
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Hanson, J.
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Harms, J.
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Harry, G.
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Harstad, E.
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Hayler, T.
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dc.contributor.author |
Heefner, J.
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dc.contributor.author |
Heng, I.S.
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Heptonstall, A.
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dc.contributor.author |
Heurs, Michèle
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Hewitson, M.
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Hild, S.
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dc.contributor.author |
Hirose, E.
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dc.contributor.author |
Hoak, D.
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Hosken, D.
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Hough, J.
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Hoyland, D.
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dc.contributor.author |
Huttner, S.H.
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Ingram, D.
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Innerhofer, E.
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dc.contributor.author |
Ito, M.
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dc.contributor.author |
Itoh, Y.
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dc.contributor.author |
Ivanov, A.
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dc.contributor.author |
Johnson, B.
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dc.contributor.author |
Johnson, W.W.
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dc.contributor.author |
Jones, D.I.
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dc.contributor.author |
Jones, G.
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dc.contributor.author |
Jones, R.
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dc.contributor.author |
Ju, L.
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dc.contributor.author |
Kalmus, P.
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dc.contributor.author |
Kalogera, V.
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Kasprzyk, D.
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Katsavounidis, E.
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Kawabe, K.
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Kawamura, S.
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Kells, W.
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Keppel, D.G.
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Khalili, F.Ya.
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Kim, C.
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Mueller, G.
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Munch, J.
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Murray, P.
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Numata, K.
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O’Reilly, B.
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Ottaway, D.J.
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Overmier, H.
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Owen, B.J.
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Parameshwaraiah, V.
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Savov, P.
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Schediwy, S.
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Seifert, F.
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Sengupta, A.S.
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Shawhan, P.
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Shoemaker, D.H.
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Sidles, J.A.
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Siemens, X.
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dc.contributor.author |
Smith, M.R.
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dc.contributor.author |
Somiya, K.
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dc.contributor.author |
Strain, K.A.
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dc.contributor.author |
Strom, D.M.
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dc.contributor.author |
Stuver, A.
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dc.contributor.author |
Summerscales, T.Z.
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dc.contributor.author |
Sun, K.-X.
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dc.contributor.author |
Sung, M.
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dc.contributor.author |
Sutton, P.J.
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dc.contributor.author |
Takahashi, H.
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dc.contributor.author |
Tanner, D.B.
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dc.contributor.author |
Taylor, R.
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dc.contributor.author |
Taylor, R.
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dc.contributor.author |
Thacker, J.
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dc.contributor.author |
Thorne, K.A.
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dc.contributor.author |
Thorne, K.S.
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dc.contributor.author |
Thüring, A.
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dc.contributor.author |
Tokmakov, K.V.
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dc.contributor.author |
Torres, C.
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dc.contributor.author |
Torrie, C.
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dc.contributor.author |
Traylor, G.
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dc.contributor.author |
Trias, M.
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dc.contributor.author |
Tyler, W.
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dc.contributor.author |
Ugolini, D.
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dc.contributor.author |
Urbanek, K.
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dc.contributor.author |
Vahlbruch, H.
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dc.contributor.author |
Vallisneri, M.
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dc.contributor.author |
Van Den Broeck, C.
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dc.contributor.author |
Varvella, M.
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Veitch, J.
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Villar, A.
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Weinstein, A.
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Whelan, J.T.
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Whitcomb, S.E.
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Whiting, B.F.
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Wilkinson, C.
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Willems, P.A.
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Wilmut, I.
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Wipf, C.C.
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Wise, S.
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Wiseman, A.G.
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Woan, G.
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Woods, D.
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Wooley, R.
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Worden, J.
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Wu, W.
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Yakushin, I.
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Yamamoto, H.
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dc.contributor.author |
Yan, Z.
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dc.contributor.author |
Yoshida, S.
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dc.contributor.author |
Yunes, N.
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Zanolin, M.
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dc.contributor.author |
Zhang, J.
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dc.contributor.author |
Zhang, L.
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dc.contributor.author |
Zhao, C.
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dc.contributor.author |
Zotov, N.
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dc.contributor.author |
Zucker, M.
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dc.contributor.author |
Mühlen, H.zur
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dc.contributor.author |
Zweizig, J.
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dc.date.accessioned |
2022-05-12T09:17:16Z |
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dc.date.available |
2022-05-12T09:17:16Z |
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dc.date.issued |
2008 |
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dc.identifier.citation |
Abbott, B.; Abbott, R.; Adhikari, R.; Agresti, J.; Ajith, P. et al.: Search of S3 LIGO data for gravitational wave signals from spinning black hole and neutron star binary inspirals. In: Physical Review D - Particles, Fields, Gravitation and Cosmology 78 (2008), Nr. 4, 042002. DOI: https://doi.org/10.1103/PhysRevD.78.042002 |
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dc.description.abstract |
We report on the methods and results of the first dedicated search for gravitational waves emitted during the inspiral of compact binaries with spinning component bodies. We analyze 788 hours of data collected during the third science run (S3) of the LIGO detectors. We searched for binary systems using a detection template family specially designed to capture the effects of the spin-induced precession of the orbital plane. We present details of the techniques developed to enable this search for spin-modulated gravitational waves, highlighting the differences between this and other recent searches for binaries with nonspinning components. The template bank we employed was found to yield high matches with our spin-modulated target waveform for binaries with masses in the asymmetric range 1.0M <m1<3.0M and 12.0M <m2<20.0M which is where we would expect the spin of the binary's components to have a significant effect. We find that our search of S3 LIGO data has good sensitivity to binaries in the Milky Way and to a small fraction of binaries in M31 and M33 with masses in the range 1.0M <m1, m2<20.0M. No gravitational wave signals were identified during this search. Assuming a binary population with spinning components and Gaussian distribution of masses representing a prototypical neutron star-black hole system with m1 1.35M and m2 5M, we calculate the 90%-confidence upper limit on the rate of coalescence of these systems to be 15.9yr-1L10-1, where L10 is 1010 times the blue light luminosity of the Sun. © 2008 The American Physical Society. |
eng |
dc.language.iso |
eng |
|
dc.publisher |
College Park, MD : American Physical Society |
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dc.relation.ispartofseries |
Physical Review D - Particles, Fields, Gravitation and Cosmology 78 (2008), Nr. 4 |
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dc.rights |
Es gilt deutsches Urheberrecht. Das Dokument darf zum eigenen Gebrauch kostenfrei genutzt, aber nicht im Internet bereitgestellt oder an Außenstehende weitergegeben werden. |
|
dc.subject |
post-newtonian order |
eng |
dc.subject |
compact binaries |
eng |
dc.subject |
constraining population |
eng |
dc.subject |
synthesis models |
eng |
dc.subject |
radiation |
eng |
dc.subject |
objects |
eng |
dc.subject |
forms |
eng |
dc.subject |
interferometer |
eng |
dc.subject |
templates |
eng |
dc.subject |
detector |
eng |
dc.subject.ddc |
530 | Physik
|
ger |
dc.title |
Search of S3 LIGO data for gravitational wave signals from spinning black hole and neutron star binary inspirals |
eng |
dc.type |
Article |
|
dc.type |
Text |
|
dc.relation.issn |
1550-7998 |
|
dc.relation.doi |
https://doi.org/10.1103/PhysRevD.78.042002 |
|
dc.bibliographicCitation.issue |
4 |
|
dc.bibliographicCitation.volume |
78 |
|
dc.bibliographicCitation.firstPage |
042002 |
|
dc.description.version |
publishedVersion |
|
tib.accessRights |
frei zug�nglich |
|