التفاصيل البيبلوغرافية
العنوان:
Upper limits on gravitational wave bursts in LIGO's second science run
المؤلفون:
J. Logan , R. K. Nayak , R. Rahkola , I. Yakushin , Michael E Zucker , R. J. Dupuis , Guenakh Mitselmakher , Manuel Luna , Curt Cutler , Marco Aurelio Diaz , O. Spjeld , R. Zhu , M. C. Araya , A. Wilson , H. Ward , Roy Williams , Y. Hefetz , Gerhard Heinzel , C. Hardham , Benno Willke , T. Findley , Peter Fritschel , D. Ouimette , A. J. Weinstein , W. Wu , Amber Stuver , Sanichiro Yoshida , Graham Woan , Robert L. Byer , Stuart Reid , A. M. Gretarsson , M. Rakhmanov , R. L. Ward , E. Messaritaki , Badri Krishnan , Antony C. Searle , Frank Seifert , Joseph M. Kovalik , K. S. Ganezer , K. Watts , L. Ruet , Albert Lazzarini , E. Rotthoff , Bernard F. Schutz , G. Stapfer , J. Hanson , J. H. Romie , K. C. Cannon , K. Bayer , Sheila Rowan , Stefan Goßler , K. T. Reilly , Seiji Kawamura , Reinhard Prix , Alessandra Buonanno , L. Sievers , John Veitch , Guido Mueller , Morag M. Casey , M. Heurs , Robert J. McCarthy , M. Ito , Shinji Miyoki , B. J. Winjum , S. Wise , S. Grunewald , J. G. Rollins , Thomas Cokelaer , Rana X. Adhikari , Gareth Jones , A. Gillespie , T. Delker , Linqing Wen , Juri Agresti , A. Rizzi , R. Gustafson , B. Machenschalk , Osamu Miyakawa , David H. Reitze , Kevin C. Schlaufman , Kevin M. Carter , A. Grant , S. Liu , M. MacInnis , Herbert Welling , Nergis Mavalvala , C. Aulbert , R. S. Amin , S. Márka , A. Ageev , H. Tariq , T. Summerscales , Christian J. Killow , C. A. Cantley , Pankaj Sarin , A. C. Melissinos , Peter H. Sneddon , Kenneth G. Libbrecht , L. Zhang , Kenneth A. Strain , D. Farnham , Philippe Grandclément , Jan Harms , V. V. Frolov , B. C. Barish , J. Zweizig , V. Parameshwaraiah , Keisuke Goda , C. Robinson , A. Weidner , Benjamin William Allen , Michael Landry , P. J. Sutton , D. Barker , R. A. Mercer , Karsten Danzmann , M. C. Sumner , M. R. Smith , C. A. Shapiro , Adrian C. Ottewill , Joseph D. Romano , C. King , Kasem Mossavi , G. Billingsley , Haisheng Rong , G. Traylor , S. B. Anderson , K. D. Zaleski , R. DeSalvo , David B. Tanner , B. O'Reilly , S. Chelkowski , B. Lantz , Vuk Mandic , Erik Katsavounidis , S. Nagano , J. Garofoli , V. Schmidt , Peter Aufmuth , I. Salzman , K. Mailand , Robert Spero , Soumya D. Mohanty , N. Zotov , K. Mason , S. Roddy , D. Redding , V. Chickarmane , R. M. S. Schofield , Soma Mukherjee , Benjamin J. Owen , J. A. Giaime , Eric K. Gustafson , M. W. Regehr , P. Ehrens , Krzysztof Belczynski , B. F. Whiting , R. Mittleman , Scott Koranda , L. Matone , Sanjeev Dhurandhar , M. J. Lubinski , Thomas Corbitt , S. Meshkov , P. Hoang , Akiteru Takamori , S. Ray-Majumder , M. Sung , Richard L. Savage , R. Bennett , William E. Butler , E. Myers , K. V. Tokmakov , Erika D'Ambrosio , T. T. Lyons , A. Chandler , Nelson Christensen , B. Bhawal , M. Pedraza , K. Wette , A. Hartunian , H. Overmier , D. Chin , Stanislav Babak , Walid A. Majid , C. N. Colacino , Duncan A. Brown , Kevin M. Ryan , A. M. Sintes , Lee Samuel Finn , Vladimir B. Braginsky , Timothy Evans , P. G. Murray , K. Riles , Jeffrey A. Edlund , S. J. Berukoff , K. Kawabe , R. Coldwell , D. Sellers , A. Sibley , Yi Chen , Eugeniy E. Mikhailov , D. B. Kozak , M. Hennessy , Q. Z. Shu , Maria Alessandra Papa , B. Rivera , M. Hrynevych , C. Vorvick , Martin P McHugh , T. Regimbau , C. I. Torrie , A. Heptonstall , D. Sigg , S. W. Ballmer , M. Barnes , Julien Sylvestre , R. Burgess , Daniel C. Woods , M. Mageswaran , J. H. Hough , J. Allen , P. Csatorday , N. Hepler , D. I. Robertson , G. Moreno , W. G. Anderson , M. V. Plissi , Kent Blackburn , K. Reithmaier , L. Wallace , Andreas Freise , I. Leonor , John K. Cannizzo , R. Frey , Shantanu Desai , M. H. P. M. van Putten , A. Libson , S. Tilav , Peter Shawhan , J. Heefner , M. Tibbits , B. P. Abbott , Kip S. Thorne , S. Vass , Douglas R. Cook , David Crooks , Michele Zanolin , S. Seel , M. Coles , Hartmut Grote , M. Guenther , Matthew Pitkin , R. Wooley , P. J. King , D. Grimmett , Philip Nutzman , M. Malec , W. R. Johnston , Phil Willems , W. Kells , M. A. Barton , D. Busby , Brent Ware , Yousuke Itoh , E. Maros , A. G. Wiseman , D. Jungwirth , P. E. Lindquist , E. J. Daw , D. C. Coyne , D.B. DeBra , Michele Vallisneri , V. P. Mitrofanov , I. Zawischa , D. M. Strom , K. Rawlins , Ik Siong Heng , Patrick Brady , Roman Schnabel , N. Hindman , K. Y. Franzen , J. E. Brau , M. Hammond , Walter Winkler , C. Messenger , Subhasish Mitra , Lindon J. Robison , Harald Lück , Helena Armandula , E. J. Elliffe , T. Etzel , A. Bunkowski , W. Hua , M. W.E. Smith , J. Kern , H. Yamamoto , P. R. Williams , Lisa M. Goggin , D. Churches , N. A. Robertson , Gavin Davies , D. Steussy , B. Sears , L. Jones , S. Wen , Laura Cadonati , Vicky Kalogera , Susan M. Scott , Teviet Creighton , Herbert Walther , Gregory M. Harry , F. Raab , A. Marin , M. Lei , X. Siemens , K. Kötter , C. Wilkinson , J. Mason , T. Olson , B. Bochner , David H. Shoemaker , G. H. Sanders , R. Lawrence , P. Schwinberg , F. Nocera , Martin Hewitson , A. Khan , Jordan Camp , Massimo Tinto , Carlo Ungarelli , W. O. Hamilton , J. Dalrymple , D. Webber , Virginio Sannibale , David E. McClelland , S. Penn , S. Killbourn , A. S. Sengupta , Pamela J. Russell , S. Richman , V. Quetschke , James Whelan , F. Mann , C. Torres , Oliver Jennrich , P. Ajith , H. Ding , K. A. Thorne , J. Betzwieser , Bangalore Suryanarayana Sathyaprakash , E. Black , Martin M. Fejer , D. Ugolini , Carsten Fallnich , A. Rodriguez , C. Barker , Stefan Hild , J. R. Smith , R. Bork , T. Nash , Matthew Evans , L. Cardenas , Yi Pan , S. Klimenko , B. Johnson , B. J. Cusack , M. Lormand , M. Fine , A. Sazonov , G. Mendell , Richard J. K. Taylor , S. R. Rao , A. Bullington , C. Parameswariah , L. Bogue , J. Chapsky , J. Langdale , G. P. Newton , M. Fyffe , Sandra E. Wiley , Gabriela Gonzalez , M. Ashley , C. Gray , Gianpietro Cagnoli , D. Rose , V. Re , Jolien D. E. Creighton , Lindy Blackburn , Chunglee Kim , V. Sandberg , Rainer Weiss , R. W. P. Drever , W. W. Johnson , A. Ivanov , H. Radkins , S. P. Vyachanin , W. Tyler , Raymond G. Beausoleil , R. Balasubramanian , J. Myers , Shourov Chatterji , Suvadeep Bose , Alberto Vecchio , J. S. Noel , J. Castiglione , P. Charlton , A. Di Credico , I. A. Bilenko , V. Dergachev , Ian Taylor , David J. Ottaway , David Jones , Peter R. Saulson , R. Abbott , B. Bland , U. Weiland , S. E. Seader , Stephen Fairhurst , O. Matherny , B. Barr , J. Worden , A. Rüdiger , R. Riesen , Roland Schilling , F. Asiri , S. E. Whitcomb
المساهمون:
The LIGO Scientific Collaboration
المصدر:
Physical Review D
سنة النشر:
2005
مصطلحات موضوعية:
Nuclear and High Energy Physics , FOS: Physical sciences , Astrophysics , General Relativity and Quantum Cosmology (gr-qc) , 01 natural sciences , rotational core collapse , General Relativity and Quantum Cosmology , Constant false alarm rate , 0103 physical sciences , DETECTORS , Waveform , ddc:530 , ALGORITHM , 010306 general physics , QC , detectors , Physics , algorithm , 010308 nuclear & particles physics , Gravitational wave , Detector , PERFORMANCE , Noise floor , LIGO , SIGNAL , Amplitude , ROTATIONAL CORE COLLAPSE , Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik , signal , Noise (radio) , performance
الوصف:
We perform a search for gravitational wave bursts using data from the second science run of the LIGO detectors, using a method based on a wavelet time-frequency decomposition. This search is sensitive to bursts of duration much less than a second and with frequency content in the 100-1100Hz range. It features significant improvements in the instrument sensitivity and in the analysis pipeline with respect to the burst search previously reported by LIGO. Improvements in the search method allow exploring weaker signals, relative to the detector noise floor, while maintaining a low false alarm rate, O(0.1) microHz. The sensitivity in terms of the root-sum-square (rss) strain amplitude lies in the range of hrss~10^{-20} - 10^{-19}/sqrt(Hz) No gravitational wave signals were detected in 9.98 days of analyzed data. We interpret the search result in terms of a frequentist upper limit on the rate of detectable gravitational wave bursts at the level of 0.26 events per day at 90% confidence level. We combine this limit with measurements of the detection efficiency for given waveform morphologies in order to yield rate versus strength exclusion curves as well as to establish order-of-magnitude distance sensitivity to certain modeled astrophysical sources. Both the rate upper limit and its applicability to signal strengths improve our previously reported limits and reflect the most sensitive broad-band search for untriggered and unmodeled gravitational wave bursts to date.
وصف الملف:
application/pdf
اللغة:
English
تدمد:
1550-2368
الوصول الحر:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::915d9ca771d3af5e5984afe01ad8e5e6Test http://arxiv.org/abs/gr-qc/0505029Test
حقوق:
OPEN
رقم الانضمام:
edsair.doi.dedup.....915d9ca771d3af5e5984afe01ad8e5e6
قاعدة البيانات:
OpenAIRE
