دورية أكاديمية

First cross-correlation analysis of interferometric and resonant-bar gravitational-wave data for stochastic backgrounds

التفاصيل البيبلوغرافية
العنوان: First cross-correlation analysis of interferometric and resonant-bar gravitational-wave data for stochastic backgrounds
المؤلفون: Abbott, B., Abbott, R., Adhikari, R., Agresti, J., Ajith, P., Allen, B., Amin, R., Anderson, S.B., Anderson, W.G., Arain, M., Araya, M., Armandula, H., Ashley, M., Aston, S., Aufmuth, P., Aulbert, C., Babak, S., Ballmer, S., Bantilan, H., Barish, B.C., Barker, C., Barker, D., Barr, B., Barriga, P., Barton, M.A., Bayer, K., Belczynski, K., Betzwieser, J., Beyersdorf, P.T., Bhawal, B., Bilenko, I.A., Billingsley, G., Biswas, R., Black, E., Blackburn, K., Blackburn, L., Blair, D., Bland, B., Bogenstahl, J., Bogue, L., Bork, R., Boschi, V., Bose, S., Brady, P.R., Braginsky, V.B., Brau, J.E., Brinkmann, M., Brooks, A., Brown, D.A., Bullington, A., Bunkowski, A., Buonanno, A., Burgamy, M., Burmeister, O., Busby, D., Byer, R.L., Cadonati, L., Cagnoli, G., Camp, J.B., Cannizzo, J., Cannon, K., Cantley, C.A., Cao, J., Cardenas, L., Casey, M.M., Castaldi, G., Cepeda, C., Chalkey, E., Charlton, P., Chatterji, S., Chelkowski, S., Chen, Y., Chiadini, F., Chin, D., Chin, E., Chow, J., Christensen, N., Clark, J., Cochrane, P., Cokelaer, T., Colacino, C.N., Coldwell, R., Conte, R., Cook, D., Corbitt, T., Coward, D., Coyne, D., Creighton, J.D.E., Creighton, T.D., Croce, R.P., Crooks, D.R.M., Cruise, A.M., Cumming, A., Dalrymple, J., D’Ambrosio, E., Danzmann, K., Davies, G., DeBra, D., Degallaix, J., Degree, M., Demma, T., Dergachev, V., Desai, S., DeSalvo, R., Dhurandhar, S., Díaz, M., Dickson, J., Di Credico, A., Diederichs, G., Dietz, A., Doomes, E.E., Drever, R.W.P., Dumas, J.-C., Dupuis, R.J., Dwyer, J.G., Ehrens, P., Espinoza, E., Etzel, T., Evans, M., Evans, T., Fairhurst, S., Fan, Y., Fazi, D., Fejer, M.M., Finn, L.S., Fiumara, V., Fotopoulos, N., Franzen, A., Franzen, K.Y., Freise, A., Frey, R., Fricke, T., Fritschel, P., Frolov, V.V., Fyffe, M., Galdi, V., Garofoli, J., Gholami, I., Giaime, J.A., Giampanis, S., Giardina, K.D., Goda, K., Goetz, E., Goggin, L., González, G., Gossler, S., Grant, A., Gras, S., Gray, C., Gray, M., Greenhalgh, J., Gretarsson, A.M., Grosso, R., Grote, H., Grunewald, S., Guenther, M., Gustafson, R., Hage, B., Hamilton, W.O., Hammer, D., Hanna, C., Hanson, J., Harms, J., Harry, G., Harstad, E., Hayler, T., Heefner, J., Heng, I.S., Heptonstall, A., Heurs, Michèle, Hewitson, M., Hild, S., Hirose, E., Hoak, D., Hosken, D., Hough, J., Howell, E., Hoyland, D., Huttner, S.H., Ingram, D., Innerhofer, E., Ito, M., Itoh, Y., Ivanov, A., Jackrel, D., Johnson, B., Johnson, W.W., Jones, D.I., Jones, G., Jones, R., Ju, L., Kalmus, P., Kalogera, V., Kasprzyk, D., Katsavounidis, E., Kawabe, K., Kawamura, S., Kawazoe, F., Kells, W., Keppel, D.G., Khalili, F.Ya., Kim, C., King, P., Kissel, J.S., Klimenko, S., Kokeyama, K., Kondrashov, V., Kopparapu, R.K., Kozak, D., Krishnan, B., Kwee, P., Lam, P.K., Landry, M., Lantz, B., Lazzarini, A., Lee, B., Lei, M., Leiner, J., Leonhardt, V., Leonor, I., Libbrecht, K., Lindquist, P., Lockerbie, N.A., Longo, M., Lormand, M., Lubinski, M., Lück, H., Machenschalk, B., MacInnis, M., Mageswaran, M., Mailand, K., Malec, M., Mandic, V., Marano, S., Márka, S., Markowitz, J., Maros, E., Martin, I., Marx, J.N., Mason, K., Matone, L., Matta, V., Mavalvala, N., McCarthy, R., McCaulley, B.J., McClelland, D.E., McGuire, S.C., McHugh, M., McKenzie, K., McNabb, J.W.C., McWilliams, S., Meier, T., Melissinos, A., Mendell, G., Mercer, R.A., Meshkov, S., Messaritaki, E., Messenger, C.J., Meyers, D., Mikhailov, E., Miller, P., Mitra, S., Mitrofanov, V.P., Mitselmakher, G., Mittleman, R., Miyakawa, O., Mohanty, S., Moody, V., Moreno, G., Mossavi, K., MowLowry, C., Moylan, A., Mudge, D., Mueller, G., Mukherjee, S., Müller-Ebhardt, H., Munch, J., Murray, P., Myers, E., Myers, J., Nash, T., Nettles, D., Newton, G., Nishizawa, A., Numata, K., O’Reilly, B., O’Shaughnessy, R., Ottaway, D.J., Overmier, H., Owen, B.J., Paik, H.-J., Pan, Y., Papa, M.A., Parameshwaraiah, V., Patel, P., Pedraza, M., Penn, S., Pierro, V., Pinto, I.M., Pitkin, M., Pletsch, H., Plissi, M.V., Postiglione, F., Prix, R., Quetschke, V., Raab, F., Rabeling, D., Radkins, H., Rahkola, R., Rainer, N., Rakhmanov, M., Ramsunder, M., Rawlins, K., Ray-Majumder, S., Re, V., Rehbein, H., Reid, S., Reitze, D.H., Ribichini, L., Riesen, R., Riles, K., Rivera, B., Robertson, N.A., Robinson, C., Robinson, E.L., Roddy, S., Rodriguez, A., Rogan, A.M., Rollins, J., Romano, J.D., Romie, J., Route, R., Rowan, S., Rüdiger, A., Ruet, L., Russell, P., Ryan, K., Sakata, S., Samidi, M., de la Jordana, L.Sancho, Sandberg, V., Sannibale, V., Saraf, S., Sarin, P., Sathyaprakash, B.S., Sato, S., Saulson, P.R., Savage, R., Savov, P., Schediwy, S., Schilling, R., Schnabel, R., Schofield, R., Schutz, B.F., Schwinberg, P., Scott, S.M., Searle, A.C., Sears, B., Seifert, F., Sellers, D., Sengupta, A.S., Shawhan, P., Shoemaker, D.H., Sibley, A., Sidles, J.A., Siemens, X., Sigg, D., Sinha, S., Sintes, A.M., Slagmolen, B.J.J., Slutsky, J., Smith, J.R., Smith, M.R., Somiya, K., Strain, K.A., Strom, D.M., Stuver, A., Summerscales, T.Z., Sun, 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المصدر: Physical Review D - Particles, Fields, Gravitation and Cosmology 76 (2007), Nr. 2 ; Physical Review D - Particles, Fields, Gravitation and Cosmology
بيانات النشر: American Physical Society
سنة النشر: 2007
المجموعة: Institutional Repository of Leibniz Universität Hannover
مصطلحات موضوعية: rho-pi puzzle, possible explanation, j/psi, psi, decays, ddc:530
الوصف: Data from the LIGO Livingston interferometer and the ALLEGRO resonant-bar detector, taken during LIGO's fourth science run, were examined for cross correlations indicative of a stochastic gravitational-wave background in the frequency range 850-950 Hz, with most of the sensitivity arising between 905 and 925 Hz. ALLEGRO was operated in three different orientations during the experiment to modulate the relative sign of gravitational-wave and environmental correlations. No statistically significant correlations were seen in any of the orientations, and the results were used to set a Bayesian 90% confidence level upper limit of Ωgw(f)≤1.02, which corresponds to a gravitational-wave strain at 915 Hz of 1.5×10-23Hz-1/2. In the traditional units of h1002Ωgw(f), this is a limit of 0.53, 2 orders of magnitude better than the previous direct limit at these frequencies. The method was also validated with successful extraction of simulated signals injected in hardware and software. © 2007 The American Physical Society.
نوع الوثيقة: article in journal/newspaper
اللغة: English
تدمد: 1550-7998
العلاقة: http://dx.doi.org/10.15488/12056Test; https://www.repo.uni-hannover.de/handle/123456789/12153Test
DOI: 10.15488/12056
الإتاحة: https://doi.org/10.15488/12056Test
https://doi.org/10.1103/PhysRevD.76.022001Test
https://www.repo.uni-hannover.de/handle/123456789/12153Test
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رقم الانضمام: edsbas.D7DDDF33
قاعدة البيانات: BASE