Search for gravitational wave radiation associated with the pulsating tail of the SGR1806−20hyperflare of 27 December 2004 using LIGO

التفاصيل البيبلوغرافية
العنوان: Search for gravitational wave radiation associated with the pulsating tail of the SGR1806−20hyperflare of 27 December 2004 using LIGO
المؤلفون: M. R. Smith, I. Leonor, John K. Cannizzo, Alberto Vecchio, B. Lantz, Gianpietro Cagnoli, J. Myers, Shourov Chatterji, D. Fazi, S. J. Waldman, Suvadeep Bose, J. D. E. Creighton, H. Yamamoto, J. C. Dumas, R. P. Croce, Jong H. Chow, R. M. S. Schofield, B. Lee, Jonathan C. Leiner, R. Taylor, V. Re, Benno Willke, Albert Lazzarini, D. Hoak, J. Clark, G. Mendell, L. Ruet, Benjamin J. Owen, Christopher Wipf, K. V. Tokmakov, Rainer Weiss, D. Barker, G. Diederichs, R. W. P. Drever, K. D. Giardina, K. Kokeyama, W. W. Johnson, David Crooks, B. Bland, F. Ya. Khalili, A. Cumming, Martin Hewitson, Atsushi J. Nishizawa, Junwei Cao, Giuseppe Castaldi, M. V. Plissi, Soumya D. Mohanty, R. L. Savage, S. Roddy, N. Zotov, Alessandra Buonanno, D. J. Hosken, J. G. Rollins, Karel E. Urbanek, J. W C McNabb, David Blair, V. Leonhardt, A. J. Weinstein, K. Mason, Hartmut Grote, A. M. Sintes, Helena Armandula, Ke-Xun Sun, C. A. Cantley, A. M. Rogan, I. Gholami, W. Wu, C. Robinson, Benjamin William Allen, E. Innerhofer, S. Giampanis, Sanichiro Yoshida, A. M. Gretarsson, N. Rainer, G. P. Newton, M. Fyffe, Sanjeev Dhurandhar, S. Saraf, S. Ray-Majumder, Lee Samuel Finn, Karsten Danzmann, Roberto Conte, N. A. Lockerbie, N. Fotopoulos, R. Rahkola, Graham Woan, L. Matone, Robert L. Byer, Stuart Reid, Gabriela Gonzalez, P. T. Beyersdorf, Carlos Cepeda, P. E. Lindquist, Slawomir Gras, Peter Aufmuth, E. Messaritaki, Sheila Rowan, H. Rehbein, H. Bantilan, Jesper Munch, Robert J. McCarthy, C. N. Colacino, Stefano Marano, S. B. Anderson, L. Wallace, D. M. Whitbeck, R. Frey, Shuichi Sato, J. N. Marx, A. Sibley, Erika D'Ambrosio, M. Degree, M. Lormand, David B. Tanner, Stephen Fairhurst, R. J. Dupuis, Ravi Kumar Kopparapu, Bernard F. Schutz, Li Ju, J. Hanson, Yi Chen, B. Bhawal, M. Landry, S. H. Huttner, Vincenzo Galdi, M. A. Barton, R. L. Ward, M. Sung, A. M. Cruise, Guido Mueller, V. Boschi, Joseph D. Romano, Jared Markowitz, A. G. Wiseman, Kasem Mossavi, S. Sakata, S. Wen, A. Dietz, Shantanu Desai, M. Pedraza, Vuk Mandic, A. Bullington, Rahul Biswas, L. Bogue, Sean T. McWilliams, V. V. Frolov, J. H. Romie, Miquel Trias, K. Bayer, Rana X. Adhikari, Gareth Jones, J. A. Giaime, D. C. Coyne, Kip S. Thorne, F. J. Raab, Maria Alessandra Papa, R.L. Coldwell, V. Parameshwaraiah, P. Savov, B. Machenschalk, L. Ribichini, T. T. Fricke, Kevin M. Ryan, I. Yakushin, Hirotaka Takahashi, James Whelan, R. Gustafson, P. Ajith, D.B. DeBra, Kent Blackburn, V. P. Mitrofanov, S. Márka, Jordan Camp, E. Hirose, Juri Agresti, A. Bunkowski, J. Zhang, D. Chin, Supriyo Sinha, Stanislav Babak, M. Ito, N. A. Robertson, T. Meier, Guenakh Mitselmakher, Francesco Chiadini, A. Franzen, Kirk McKenzie, M. C. Araya, Richard O'Shaughnessy, B. Barr, P. Patel, Malik Rakhmanov, Kenneth A. Strain, Boris Hage, J. Dalrymple, C. Gray, J. Worden, L. Williams, H. Müller-Ebhardt, E. Myers, Duncan A. Brown, K. Y. Franzen, A. Rüdiger, B. O'Reilly, Morag M. Casey, M. Heurs, D. Hammer, F. Seifert, Yi Pan, Eric Howell, Eugeniy E. Mikhailov, S. Chelkowski, J. Dickson, C. I. Torrie, Jan Harms, A. S. Sengupta, J. Zweizig, Michael C. B. Ashley, J. A. Sidles, Matthew Evans, L. Cardenas, Kentaro Somiya, G. Billingsley, A. Grant, D. B. Kozak, C. Vorvick, Kenji Numata, Peter Kalmus, J. Greenhalgh, Innocenzo M. Pinto, R. Riesen, Evan Goetz, A. Thüring, S. Klimenko, A. C. Melissinos, Fabio Postiglione, T. Etzel, Carlo Ungarelli, Roland Schilling, Thomas Cokelaer, T. Z. Summerscales, P. Kwee, Marco G. Tarallo, L. Zhang, J. Slutsky, S. Meshkov, D. Webber, A. Weidner, D. Meyers, P. Schwinberg, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, E. Black, Martin M. Fejer, J. R. Smith, Malcolm B. Gray, R. Bork, T. Nash, A. Brooks, P. Ehrens, Richard J. Abbott, P. J. Veitch, K. Wette, H. Zur Mühlen, W. G. Anderson, S. E. Whitcomb, S. Gossler, Timothy Evans, B. P. Abbott, D. Sigg, S. W. Ballmer, C. Aulbert, Chunnong Zhao, David H. Shoemaker, P. Cochrane, Roman Schnabel, Vincenzo Fiumara, J. E. Brau, G. Moreno, S. Vass, Subhasish Mitra, O. Burmeister, J. Thacker, W. Kells, D. Busby, H. Ward, Soma Mukherjee, Peter King, Drew Keppel, Zewu Yan, B. Johnson, D. Kasprzyk, P. G. Murray, M. Samidi, J. H. Hough, S. Wise, S. Grunewald, Douglas R. Cook, Michele Zanolin, Keisuke Goda, Erik Katsavounidis, Kenneth G. Libbrecht, M. J. Lubinski, D. Jackrel, K. Mailand, Maurizio Longo, John G. Dwyer, Krzysztof Belczynski, Vladimir B. Braginsky, H. Vahlbruch, R. Mittleman, K. Riles, Nelson Christensen, John Veitch, E. Espinoza, M. Weinert, Yousuke Itoh, Sascha Schediwy, M. MacInnis, Vincenzo Matta, R. S. Amin, Andreas Freise, Vincenzo Pierro, Matthew Pitkin, C. Messenger, M. Varvella, R. Wooley, T. Hayler, Ping Koy Lam, S. Kamat, J. Heefner, R. Grosso, M. A. Arain, Gregory M. Harry, I. Wilmut, F. Kawazoe, J. Garofoli, J. S. Kissel, M. Lei, Roger Jones, K. Kawabe, S. M. Aston, B. Rivera, Pablo Barriga, M. Mageswaran, I. W. Martin, Virginio Sannibale, David E. McClelland, Michele Vallisneri, Ik Siong Heng, Emma L. Robinson, V. Kondrashov, R. DeSalvo, E. E. Doomes, L. Sancho De La Jordana, K. Rawlins, C. Torres, A. Rodriguez, C. Barker, Daniel C. Woods, Pankaj Sarin, A. L. Stuver, Martin P McHugh, B. J. J. Slagmolen, K. Watts, E. Maros, P. Shawhan, P. Charlton, A. Di Credico, A. E. Villar, I. A. Bilenko, V. Dergachev, Nergis Mavalvala, Jerome Degallaix, David J. Ottaway, B. C. Barish, David Jones, A. Ivanov, H. Radkins, Damien Mudge, S. P. Vyachanin, Peter R. Saulson, M. Brinkmann, W. Tyler, Walter Winkler, David Coward, Harald Lück, D. S. Rabeling, R. A. Mercer, S. C. McGuire, Lindy Blackburn, Chunglee Kim, V. Sandberg, Massimo Tinto, Nicolás Yunes, Badri Krishnan, E. Chalkey, Antony C. Searle, C. M. Mow-Lowry, D. Hoyland, B. F. Whiting, C. Van Den Broeck, P. J. Sutton, J. Bogenstahl, Michael E Zucker, E. Chin, Marco Aurelio Diaz, S. Penn, Pamela J. Russell, Roger K. Route, K. A. Thorne, J. Betzwieser, D. Ugolini, Stefan Hild, H. Overmier, D. Sellers, M. Guenther, Patrick Brady, Seiji Kawamura, Reinhard Prix, Elizabeth Harstad, Osamu Miyakawa, David H. Reitze, Gavin Davies, B. Sears, Vicky Kalogera, Yaohui Fan, Laura Cadonati, A. Moylan, Susan M. Scott, Teviet Creighton, Chad Hanna, X. Siemens, C. Wilkinson, T. Demma, Peter Fritschel, K. C. Cannon, H. J. Pletsch, G. Traylor, Thomas Corbitt, A. Heptonstall, M. Malec, D. R. Ingram, Phil Willems, D. M. Strom, Lisa M. Goggin
المصدر: Physical Review D. 76
بيانات النشر: American Physical Society (APS), 2007.
سنة النشر: 2007
مصطلحات موضوعية: Physics, Nuclear and High Energy Physics, 010308 nuclear & particles physics, Gravitational wave, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, Astrophysics, Light curve, 01 natural sciences, Electromagnetic radiation, Asteroseismology, LIGO, law.invention, Neutron star, Amplitude, law, 0103 physical sciences, 010303 astronomy & astrophysics, Flare
الوصف: We have searched for gravitational waves (GWs) associated with the SGR 1806−20 hyperflare of 27 December 2004. This event, originating from a Galactic neutron star, displayed exceptional energetics. Recent investigations of the x-ray light curve’s pulsating tail revealed the presence of quasiperiodic oscillations (QPOs) in the 30–2000 Hz frequency range, most of which coincides with the bandwidth of the LIGO detectors. These QPOs, with well-characterized frequencies, can plausibly be attributed to seismic modes of the neutron star which could emit GWs. Our search targeted potential quasimonochromatic GWs lasting for tens of seconds and emitted at the QPO frequencies. We have observed no candidate signals above a predetermined threshold, and our lowest upper limit was set by the 92.5 Hz QPO observed in the interval from 150 s to 260 s after the start of the flare. This bound corresponds to a (90% confidence) root-sum-squared amplitude h^(90%)_(rss-det) =4.5×10^(−22) strain Hz^(−1/2) on the GW waveform strength in the detectable polarization state reaching our Hanford (WA) 4 km detector. We illustrate the astrophysical significance of the result via an estimated characteristic energy in GW emission that we would expect to be able to detect. The above result corresponds to 7.7×10^(46) erg (=4.3×10^(−8) M_⊙c^2), which is of the same order as the total (isotropic) energy emitted in the electromagnetic spectrum. This result provides a means to probe the energy reservoir of the source with the best upper limit on the GW waveform strength published and represents the first broadband asteroseismology measurement using a GW detector.
تدمد: 1550-2368
1550-7998
URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_________::dd7962c852b64ad4e5ac4b2707dc9802
https://doi.org/10.1103/physrevd.76.062003
حقوق: OPEN
رقم الأكسشن: edsair.doi...........dd7962c852b64ad4e5ac4b2707dc9802
قاعدة البيانات: OpenAIRE