التفاصيل البيبلوغرافية
| العنوان: |
Search for gravitational waves from galactic and extra-galactic binary neutron stars |
| المؤلفون: |
Abbott, B., Abbott, R., Adhikari, R., Ageev, A., Allen, B., 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., Cantley, C.A., 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., D’Ambrosio, E., Danzmann, K., Daw, E., DeBra, D., Delker, T., Dergachev, V., DeSalvo, R., Dhurandhar, S., Di Credico, A., Díaz, M., Ding, H., Drever, R.W.P., Dupuis, R.J., Edlund, J.A., Ehrens, P., Elliffe, E.J., Etzel, T., Evans, M., Evans, T., Fairhurst, S., Fallnich, C., Farnham, D., Fejer, M.M., Findley, T., Fine, M., Finn, L.S., Franzen, K.Y., Freise, A., Frey, R., Fritschel, P., Frolov, V.V., Fyffe, M., Ganezer, K.S., Garofoli, J., Giaime, J.A., Gillespie, A., Goda, K., González, G., Goßler, S., Grandclément, P., Grant, A., Gray, C., Gretarsson, A.M., Grimmett, D., Grote, H., Grunewald, S., Guenther, M., Gustafson, E., Gustafson, R., Hamilton, W.O., Hammond, M., Hanson, J., Hardham, C., Harms, J., Harry, G., Hartunian, A., Heefner, J., Hefetz, Y., Heinzel, G., Heng, I.S., Hennessy, M., Hepler, N., Heptonstall, A., Heurs, Michèle, Hewitson, M., Hild, S., Hindman, N., Hoang, P., Hough, J., Hrynevych, M., Hua, W., Ito, M., Itoh, Y., Ivanov, A., Jennrich, O., Johnson, B., Johnson, W.W., Johnston, W.R., Jones, D.I., Jones, L., Jungwirth, D., Kalogera, V., Katsavounidis, E., Kawabe, K., Kawamura, S., Kells, W., Kern, J., Khan, A., Killbourn, S., Killow, C.J., Kim, C., King, C., King, P., Klimenko, S., Koranda, S., Kötter, K., Kovalik, J., Kozak, D., Krishnan, B., Landry, M., Langdale, J., Lantz, B., Lawrence, R., Lazzarini, A., Lei, M., Leonor, I., Libbrecht, K., Libson, A., Lindquist, P., Liu, S., Logan, J., Lormand, M., Lubinski, M., Lück, H., Lyons, T.T., Machenschalk, B., MacInnis, M., Mageswaran, M., Mailand, K., Majid, W., Malec, M., Mann, F., Marin, A., Márka, S., Maros, E., Mason, J., Mason, K., Matherny, O., Matone, L., Mavalvala, N., McCarthy, R., McClelland, D.E., McHugh, M., McNabb, J.W.C., Mendell, G., Mercer, R.A., Meshkov, S., Messaritaki, E., Messenger, C., Mitrofanov, V.P., Mitselmakher, G., Mittleman, R., Miyakawa, O., Miyoki, S., Mohanty, S., Moreno, G., Mossavi, K., Mueller, G., Mukherjee, S., Murray, P., Myers, J., Nagano, S., Nash, T., Nayak, R., Newton, G., Nocera, F., Noel, J.S., Nutzman, P., Olson, T., O’Reilly, B., Ottaway, D.J., Ottewill, A., Ouimette, D., Overmier, H., Owen, B.J., Pan, Y., Papa, M.A., Parameshwaraiah, V., Parameswaran, A., Parameswariah, C., Pedraza, M., Penn, S., Pitkin, M., Plissi, M., Prix, R., Quetschke, V., Raab, F., Radkins, H., Rahkola, R., Rakhmanov, M., Rao, S.R., Rawlins, K., Ray-Majumder, S., Re, V., Redding, D., Regehr, M.W., Regimbau, T., Reid, S., Reilly, K.T., Reithmaier, K., Reitze, D.H., Richman, S., Riesen, R., Riles, K., Rivera, B., Rizzi, A., Robertson, D.I., Robertson, N.A., Robison, L., Roddy, S., Rollins, J., Romano, J.D., Romie, J., Rong, H., Rose, D., Rotthoff, E., Rowan, S., Rüdiger, A., Russell, P., Ryan, K., Salzman, I., Sandberg, V., Sanders, G.H., Sannibale, V., Sathyaprakash, B., Saulson, P.R., Savage, R., Sazonov, A., Schilling, R., Schlaufman, K., Schmidt, V., Schnabel, R., Schofield, R., Schutz, B.F., Schwinberg, P., Scott, S.M., Seader, S.E., Searle, A.C., Sears, B., Seel, S., Seifert, F., Sengupta, A.S., Shapiro, C.A., Shawhan, P., Shoemaker, D.H., Shu, Q.Z., Sibley, A., Siemens, X., Sievers, L., Sigg, D., Sintes, A.M., Smith, J.R., Smith, M., Smith, M.R., Sneddon, P.H., Spero, R., Stapfer, G., Steussy, D., Strain, K.A., Strom, D., Stuver, A., Summerscales, T., Sumner, M.C., Sutton, P.J., Sylvestre, J., Takamori, A., Tanner, D.B., Tariq, H., Taylor, I., Taylor, R., Thorne, K.A., Thorne, K.S., Tibbits, M., Tilav, S., Tinto, M., Tokmakov, K.V., Torres, C., Torrie, C., Traylor, G., Tyler, W., Ugolini, D., Ungarelli, C., Vallisneri, M., van Putten, M., Vass, S., Vecchio, A., Veitch, J., Vorvick, C., Vyachanin, S.P., Wallace, L., Walther, H., Ward, H., Ware, B., Watts, K., Webber, D., Weidner, A., Weiland, U., Weinstein, A., Weiss, R., Welling, H., Wen, L., Wen, S., Whelan, J.T., Whitcomb, S.E., Whiting, B.F., Wiley, S., Wilkinson, C., Willems, P.A., Williams, P.R., Williams, R., Willke, B., Wilson, A., Winjum, B.J., Winkler, W., Wise, S., Wiseman, A.G., Woan, G., Woods, D., Wooley, R., Worden, J., Wu, W., Yakushin, I., Yamamoto, H., Yoshida, S., Zaleski, K.D., Zanolin, M., Zawischa, I., Zhang, L., Zhu, R., Zotov, N., Zucker, M., Zweizig, J. |
| المصدر: |
Physical Review D - Particles, Fields, Gravitation and Cosmology 72 (2005), Nr. 8 ; Physical Review D - Particles, Fields, Gravitation and Cosmology |
| بيانات النشر: |
American Physical Society |
| سنة النشر: |
2005 |
| المجموعة: |
Institutional Repository of Leibniz Universität Hannover |
| مصطلحات موضوعية: |
inspiraling compact binaries, ligo, templates, events, rates, detectors, systems, pulsars, forms, ddc:530 |
| الوصف: |
We use 373 hours (≈15 days) of data from the second science run of the LIGO gravitational-wave detectors to search for signals from binary neutron star coalescences within a maximum distance of about 1.5 Mpc, a volume of space which includes the Andromeda Galaxy and other galaxies of the Local Group of galaxies. This analysis requires a signal to be found in data from detectors at the two LIGO sites, according to a set of coincidence criteria. The background (accidental coincidence rate) is determined from the data and is used to judge the significance of event candidates. No inspiral gravitational-wave events were identified in our search. Using a population model which includes the Local Group, we establish an upper limit of less than 47 inspiral events per year per Milky Way equivalent galaxy with 90% confidence for nonspinning binary neutron star systems with component masses between 1 and 3M. © 2005 The American Physical Society. |
| نوع الوثيقة: |
article in journal/newspaper |
| اللغة: |
English |
| تدمد: |
1550-7998 |
| Relation: |
http://dx.doi.org/10.15488/12063; https://www.repo.uni-hannover.de/handle/123456789/12160 |
| DOI: |
10.15488/12063 |
| الاتاحة: |
https://www.repo.uni-hannover.de/handle/123456789/12160
https://doi.org/10.15488/12063 |
| Rights: |
Es gilt deutsches Urheberrecht. Das Dokument darf zum eigenen Gebrauch kostenfrei genutzt, aber nicht im Internet bereitgestellt oder an Außenstehende weitergegeben werden. ; frei zugänglich |
| رقم الانضمام: |
edsbas.65F9DD4A |
| قاعدة البيانات: |
BASE |