Setting upper limits on the strength of periodic gravitational waves from PSR [Formula Presented] using the first science data from the GEO 600 and LIGO detectors

Data collected by the GEO 600 and LIGO interferometric gravitational wave detectors during their first observational science run were searched for continuous gravitational waves from the pulsar [Formula Presented] at twice its rotation frequency. Two independent analysis methods were used and are demonstrated in this paper: Frequency domain method and a time domain method. Both achieve consistent null results, placing new upper limits on the strength of the pulsar’s gravitational wave emission. A model emission mechanism is used to interpret the limits as a constraint on the pulsar’s equatorial ellipticity. © 2004 The American Physical Society.

Setting upper limits on the strength of periodic gravitational waves from PSR [Formula Presented] using the first science data from the GEO 600 and LIGO detectors

Abbott B.;Abbott R.;Adhikari R.;Ageev A.;Allen B.;Amin R.;Anderson S. B.;Anderson W. G.;Araya M.;Armandula H.;Asiri F.;Aufmuth P.;Aulbert C.;Babak S.;Balasubramanian R.;Ballmer S.;Barish B. C.;Barker D.;Barker-Patton C.;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.;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 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.;Chen Y.;Chickarmane V.;Chin D.;Christensen N.;Churches D.;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.;Davies R.;Daw E.;DeBra D.;Delker T.;DeSalvo R.;Dhurandhar S.;Diaz M.;Ding H.;Drever R. W. P.;Dupuis R. J.;Ebeling C.;Edlund J.;Ehrens P.;Elliffe E. J.;Etzel T.;Evans M.;Evans T.;Fallnich C.;Farnham D.;Fejer M. M.;Fine M.;Finn L. S.;Flanagan E.;Freise A.;Frey R.;Fritschel P.;Frolov V.;Fyffe M.;Ganezer K. S.;Giaime J. A.;Gillespie A.;Goda K.;Gonzalez G.;Gossler S.;Grandclement 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.;Harry G.;Hartunian A.;Heefner J.;Hefetz Y.;Heinzel G.;Heng I. S.;Hennessy M.;Hepler N.;Heptonstall A.;Heurs M.;Hewitson M.;Hindman N.;Hoang P.;Hough J.;Hrynevych M.;Hua W.;Ingley R.;Ito M.;Itoh Y.;Ivanov A.;Jennrich O.;Johnson W. W.;Johnston W.;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.;Kloevekorn P.;Koranda S.;Kotter K.;Kovalik J.;Kozak D.;Krishnan B.;Landry M.;Langdale J.;Lantz B.;Lawrence R.;Lazzarini A.;Lei M.;Leonhardt V.;Leonor I.;Libbrecht K.;Lindquist P.;Liu S.;Logan J.;Lormand M.;Lubinski M.;Luck H.;Lyons T. T.;Machenschalk B.;MacInnis M.;Mageswaran M.;Mailand K.;Majid W.;Malec M.;Mann F.;Marin A.;Marka S.;Maros E.;Mason J.;Mason K.;Matherny O.;Matone L.;Mavalvala N.;McCarthy R.;McClelland D. E.;McHugh M.;McNamara P.;Mendell G.;Meshkov S.;Messenger C.;Mitrofanov V. P.;Mitselmakher G.;Mittleman R.;Miyakawa O.;Miyoki S.;Mohanty S.;Moreno G.;Mossavi K.;Mours B.;Mueller G.;Mukherjee S.;Myers J.;Nagano S.;Nash T.;Naundorf H.;Nayak R.;Newton G.;Nocera F.;Nutzman P.;Olson T.;O'Reilly B.;Ottaway D. J.;Ottewill A.;Ouimette D.;Overmier H.;Owen B. J.;Papa M. A.;Parameswariah C.;Parameswariah V.;Pedraza M.;Penn S.;Pitkin M.;Plissi M.;Pratt M.;Quetschke V.;Raab F.;Radkins H.;Rahkola R.;Rakhmanov M.;Rao S. R.;Redding D.;Regehr M. W.;Regimbau T.;Reilly K. T.;Reithmaier K.;Reitze D. H.;Richman S.;Riesen R.;Riles K.;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.;Rudiger A.;Russell P.;Ryan K.;Salzman I.;Sanders G. H.;Sannibale V.;Sathyaprakash B.;Saulson P. R.;Savage R.;Sazonov A.;Schilling R.;Schlaufman K.;Schmidt V.;Schofield R.;Schrempel M.;Schutz B. F.;Schwinberg P.;Scott S. M.;Searle A. C.;Sears B.;Seel S.;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.;Skeldon K.;Smith J. R.;Smith M.;Smith M. R.;Sneddon P.;Spero R.;Stapfer G.;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. S.;Tibbits M.;Tilav S.;Tinto M.;Tokmakov K. V.;Torres C.;Torrie C.;Traeger S.;Traylor G.;Tyler W.;Ugolini D.;Vallisneri M.;van Putten M.;Vass S.;Vecchio A.;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.;Willems P. A.;Williams P. R.;Williams R.;Willke B.;Wilson A.;Winjum B. J.;Winkler W.;Wise S.;Wiseman A. G.;Woan G.;Wooley R.;Worden J.;Yakushin I.;Yamamoto H.;Yoshida S.;Zawischa I.;Zhang L.;Zotov N.;Zucker M.;Zweizig J.

2004

Abstract

Data collected by the GEO 600 and LIGO interferometric gravitational wave detectors during their first observational science run were searched for continuous gravitational waves from the pulsar [Formula Presented] at twice its rotation frequency. Two independent analysis methods were used and are demonstrated in this paper: Frequency domain method and a time domain method. Both achieve consistent null results, placing new upper limits on the strength of the pulsar’s gravitational wave emission. A model emission mechanism is used to interpret the limits as a constraint on the pulsar’s equatorial ellipticity. © 2004 The American Physical Society.

Scheda breve

Scheda completa

Scheda completa (DC)

	Anno
	
				2004
			
	Rivista su cui è pubblicata l'opera
	
				PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY
			
	Codice DOI
	
				https://dx.doi.org/10.1103/PhysRevD.69.082004
			
	Codice Scopus
	
				2-s2.0-37649028596
			
	Appare nelle tipologie:
	
				01.01 - Articolo in rivista

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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/3578199

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