First upper limits from LIGO on gravitational wave bursts

Abbott, B. P.; Abbott, R.; Adhikari, R. X.; Ageev, A.; Allen, B.; Amin, R.; Anderson, S. B.; Anderson, W. G.; Araya, M. C.; Armandula, H.; Asiri, F.; Aufmuth, P.; Aulbert, C.; Babak, S.; Balasubramanian, R.; Ballmer, S. W.; Barish, B.; Barker, D.; Barker-Patton, C.; Barnes, Mónica; Barr, B.; Barton, M. A.; Bayer, K.; Beausoleil, Raymond G.; Belczyński, Krzysztof; Bennett, R.; Berukoff, S. J.; Betzwieser, J.; Bhawal, B.; Bilenko, I. A.; Billingsley, G.; Black, E.; Blackburn, K.; Bland-Weaver, B.; Bochner, B.; Bogue, L.; Bork, R.; Bose, S.; Brady, P. R.; Braginsky, V. B.; Brau, J. E.; Brown, D. A.; Brozek, S.; Bullington, A.; Buonanno, A.; Burgess, R.; Busby, D.; Butler, William E.; Byer, Robert 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.; Chen, Y.; Chickarmane, Vijay; Chin, D.; Christensen, N.; Churches, D.; Colacino, C. N.; Coldwell, R. L.; Coles, M.; Cook, D.; Corbitt, T. R.; Coyne, D. C.; Creighton, J. D. E.; Creighton, T. D.; Crooks, D. R. M.; Csatorday, P.; Cusack, B. J.; Cutler, Curt; D’Ambrosio, E.; Danzmann, K.; Davies, R.; Daw, E. J.; DeBra, D.; Delker, T.; DeSalvo, R.; Dhurandhar, S.; Díaz, M. C.; Ding, H.; Drever, R. W. P.; Dupuis, R. J.; Ebeling, C.; Edlund, Jeffrey A.; Ehrens, P.; Elliffe, E. J.; Etzel, T.; Evans, M.; Evans, T. M.; Fallnich, Carsten; Farnham, D.; Fejer, M. M.; Fine, M.; Finn, L. S.; Flanagan, Éanna É.; Freise, A.; Frey, R.; Fritschel, P.; Frolov, V. V.; Fyffe, M.; Ganezer, K. S.; Giaime, J. A.; Gillespie, A.; Goda, Keisuke; González, Gabriela; Goßler, S.; Grandclément, Philippe; Grant, A.; Gray, C.; Gretarsson, A. M.; Grimmett, D.; Grote, H.; Grünewald, S.; Guenther, M.; Gustafson, E. K.; Gustafson, R.; Hamilton, W. O.; Hammond, M.; Hanson, J.; Hardham, C.; Harry, G. M.; Hartunian, A.; Heefner, J.; Hefetz, Y.; Heinzel, Gerhard; Heng, I. S.; Hennessy, M.; Hepler, N.; Heptonstall, A. W.; Heurs, M.; Hewitson, M.; Hindman, Neil; Hoang, P.; Hough, J.; Hrynevych, M.; Hua, W.; Ingley, Richard; Ito, Masahiro; Itoh, Y.; Ivanov, A.; Jennrich, O.; Johnson, W. W.; Johnston, William R.; Jones, L.; Jungwirth, Dieter; Kalogera, V.; Katsavounidis, E.; Kawabe, K.; Kawamura, Seiji; Kells, W.; Kern, J.; Khan, A.; Killbourn, S.; Killow, C. J.; Kim, C.; King, C.; King, P. J.; Klimenko, S.; Kloevekorn, P.; Koranda, S.; Kötter, K.; Kovalik, J.; Kozak, D. B.; Krishnan, B.; Landry, M.; Langdale, John; Lantz, B.; Lawrence, R.; Lazzarini, A.; Lei, M.; Leonhardt, V.; Leonor, I.; Libbrecht, Kenneth G.; Lindquist, P.; Liu, S.; Logan, J.; Lormand, M.; Łubiński, M.; Lück, H.; Lyons, T. T.; Machenschalk, B.; MacInnis, M.; Mageswaran, M.; Mailand, K.; Majid, Walid A.; Malec, M.; Mann, F.M.; Marin, A.; Márka, S.; Maros, E.; Mason, James; Mason, K.; Matherny, O.; Matone, L.; Mavalvala, N.; McCarthy, R.; McClelland, D. E.; McHugh, M.; McNamara, P. W.; Mendell, G.; Meshkov, S.; Messenger, C.; Mitrofanov, V. P.; Mitselmakher, G.; Mittleman, R.; Miyakawa, O.; Miyoki, S.; Mohanty, Soumya D.; Moreno, G.; Mossavi, K.; Mours, B.; Mueller, G.; Mukherjee, Soma; Myers, J.; Nagano, S.; Nash, T.; Naundorf, Holger; Nayak, R. K.; Newton, G.; Nocera, F.; Nutzman, P.; Olson, Timothy S.; O’Reilly, B.; Ottaway, D. J.; Ottewill, Adrian C.; Ouimette, D.; Overmier, H.; Owen, B. J.; Papa, M. A.; Parameswariah, C.; Parameswariah, V.; Pedraza, M.; Penn, S.; Pitkin, M.; Plissi, M. V.; Pratt, M. R.; Quetschke, V.; Raab, F. J.; Radkins, H.; Rahkola, R.; Rakhmanov, M.; Rao, Shanti; Redding, David C.; Regehr, M. W.; Regimbau, T.; Reilly, K. T.; Reithmaier, K.; Reitze, D. H.; Richman, S.; Riesen, Rolf; Riles, K.; Rizzi, A.; Robertson, D. I.; Robertson, N. A.; Robison, L.; Roddy, S.; Rollins, J. G.; Romano, Joseph D.; Romie, J. H.; Rong, Haisheng; Rose, D.; Rotthoff, E.; Rowan, S.; Rüdiger, A.; Russell, P.; Ryan, K.; Salzman, I.; Sanders, G. H.; Sannibale, V.; Sathyaprakash, B. S.; Saulson, P. R.; Savage, R. L.; Sazonov, A.; Schilling, R.; Schlaufman, Kevin C.; Schmidt, V.; Schofield, R. M. S.; Schrempel, M.; Schutz, B. F.; Schwinberg, P.; Scott, S. M.; Searle, A. C.; Sears, B.; Seel, S.; Sengupta, A. S.; Shapiro, Charles A.; Shawhan, P.; Shoemaker, D. H.; Shu, Q. Z.; Sibley, A.; Siemens, X.; Sievers, L.; Sigg, D.; Sintes, A. M.; Skeldon, K. D.; Smith, J. R.; Smith, M. R.; Sneddon, P.; Spero, Robert; Stapfer, G.; Strain, K. A.; Strom, D.; Stuver, A. L.; Summerscales, T. Z.; Sumner, M. C.; Sutton, P. J.; Sylvestre, Julien; Takamori, A.; Tanner, D. B.; Tariq, H.; Taylor, Ian; Taylor, Robert W.; Thorne, Kip S.; Tibbits, M.; Tilav, S.; Tinto, Massimo; Tokmakov, K. V.; Torres, C.; Torrie, C. I.; Traeger, S.; Traylor, G.; Tyler, W.; Ugolini, D.; Vallisneri, Michele; Putten, M. van; Vass, S.; Vecchio, A.; Vorvick, C.; Vyachanin, S. P.; Wallace, L.; Walther, H.; Ward, H.; Ware, Brent; Watts, K.; Webber, David; Weidner, A.; Weiland, U.; Weinstein, A. J.; Weiss, R.; Welling, H.; Wen, L.; Wen, S.; Whelan, J. T.; Whitcomb, S. E.; Whiting, B. F.; Willems, P. A.; Williams, Peter; Williams, R. D.; Willke, B.; Wilson, Andrew; Winjum, B. J.; Winkler, W.; Wise, S.; Wiseman, Alan; Woan, G.; Wooley, R.; Worden, J.; Yakushin, I.; Yamamoto, H.; Yoshida, S.; Zawischa, I.; Zhang, L.; Zotov, N.; Zucker, M. E.; Zweizig, J.

doi:10.1103/physrevd.69.102001

Cited by 115 publications

(63 citation statements)

References 29 publications

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“…The catalog of waveforms produced by Zwerger and Müller [10] have become a reference point to calibrate searches for gravitational wave bursts [18]. The catalog provides the mass quadrupole wave amplitudes A I (t) from axi-symmetric simulations of core-collapse.…”

Section: Example Of the Zwerger-müller Catalogmentioning

confidence: 99%

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Incorporating information from source simulations into searches for gravitational-wave bursts

Brady¹,

Ray‐Majumder

2004

Class. Quantum Grav.

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Abstract. The detection of gravitational waves from astrophysical sources of gravitational waves is a realistic goal for the current generation of interferometric gravitational-wave detectors. Short duration bursts of gravitational waves from core-collapse supernovae or mergers of binary black holes may bring a wealth of astronomical and astrophysical information. The weakness of the waves and the rarity of the events urges the development of optimal methods to detect the waves. The waves from these sources are not generally known well enough to use matched filtering however; this drives the need to develop new ways to exploit source simulation information in both detections and information extraction. We present an algorithmic approach to using catalogs of gravitational-wave signals developed through numerical simulation, or otherwise, to enhance our ability to detect these waves. As more detailed simulations become available, it is straightforward to incorporate the new information into the search method. This approach may also be useful when trying to extract information from a gravitational-wave observation by allowing direct comparison between the observation and simulations.

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Section: Example Of the Zwerger-müller Catalogmentioning

confidence: 99%

“…Searches for gravitational-wave bursts have been made by a number of groups [16,17,18,19]. These searches generally take an unbiased approach by using time-frequency methods to identify excess power in the data stream.…”

Section: Introductionmentioning

confidence: 99%

Incorporating information from source simulations into searches for gravitational-wave bursts

Brady¹,

Ray‐Majumder

2004

Class. Quantum Grav.

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“…Intuitively, it is clear that measuring these waves must be difficult -the weakness of the gravitational interaction ensures that the response of any detector to gravitational waves is very small. Nonetheless, technology has brought us to the point where detectors are now beginning to set interesting upper limits on GWs from some sources [84][85][86][87]. The first direct detection could be,hopefully, not too far in the future.…”

Section: B Gravitomagnetically Corrected Orbitsmentioning

confidence: 99%

The Newtonian and Relativistic Theory of Orbits and the Emission of Gravitational Waves

Laurentis¹

2011

TOAAJ

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“…Intuitively, it is clear that measuring these waves must be difficult -the weakness of the gravitational interaction ensures that the response of any detector to gravitational waves is very small. Nonetheless, technology has brought us to the point where detectors are now beginning to set interesting upper limits on GWs from some sources [79][80][81][82]. The first direct detection could be,hopefully, not too far in the future.…”

Section: Production and Signature Of Gravitational Wavesmentioning

confidence: 99%

The Newtonian and Relativistic Theory of Orbits and the Emission of Gravitational Waves

Laurentis¹

2009

TOAAJ

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This review paper is devoted to the theory of orbits. We start with the discussion of the Newtonian problem of motion then we consider the relativistic problem of motion, in particular the post-Newtonian (PN) approximation and the further gravitomagnetic corrections. Finally by a classification of orbits in accordance with the conditions of motion, we calculate the gravitational waves luminosity for different types of stellar encounters and orbits.

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First upper limits from LIGO on gravitational wave bursts

Cited by 115 publications

References 29 publications

Incorporating information from source simulations into searches for gravitational-wave bursts

Incorporating information from source simulations into searches for gravitational-wave bursts

The Newtonian and Relativistic Theory of Orbits and the Emission of Gravitational Waves

The Newtonian and Relativistic Theory of Orbits and the Emission of Gravitational Waves

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