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Gozzard DR, Howard LA, Dix-Matthews BP, Karpathakis SFE, Gravestock CT, Schediwy SW. Ultrastable Free-Space Laser Links for a Global Network of Optical Atomic Clocks. Phys Rev Lett 2022; 128:020801. [PMID: 35089751 DOI: 10.1103/physrevlett.128.020801] [Citation(s) in RCA: 5] [Impact Index Per Article: 2.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/24/2021] [Accepted: 12/02/2021] [Indexed: 06/14/2023]
Abstract
A global network of optical atomic clocks will enable unprecedented measurement precision in fields including tests of fundamental physics, dark matter searches, geodesy, and navigation. Free-space laser links through the turbulent atmosphere are needed to fully exploit this global network, by enabling comparisons to airborne and spaceborne clocks. We demonstrate frequency transfer over a 2.4 km atmospheric link with turbulence comparable to that of a ground-to-space link, achieving a fractional frequency stability of 6.1×10^{-21} in 300 s of integration time. We also show that clock comparison between ground and low Earth orbit will be limited by the stability of the clocks themselves after only a few seconds of integration. This significantly advances the technologies needed to realize a global timescale network of optical atomic clocks.
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Affiliation(s)
- D R Gozzard
- International Centre for Radio Astronomy Research, ICRAR M468, The University of Western Australia, 35 Stirling Hwy, Crawley 6009, Australia
- Australian Research Council Centre of Excellence for Engineered Quantum Systems, Department of Physics, School of Physics, Mathematics & Computing, The University of Western Australia, 35 Stirling Hwy, Crawley 6009, Australia
| | - L A Howard
- International Centre for Radio Astronomy Research, ICRAR M468, The University of Western Australia, 35 Stirling Hwy, Crawley 6009, Australia
| | - B P Dix-Matthews
- International Centre for Radio Astronomy Research, ICRAR M468, The University of Western Australia, 35 Stirling Hwy, Crawley 6009, Australia
- Australian Research Council Centre of Excellence for Engineered Quantum Systems, Department of Physics, School of Physics, Mathematics & Computing, The University of Western Australia, 35 Stirling Hwy, Crawley 6009, Australia
| | - S F E Karpathakis
- International Centre for Radio Astronomy Research, ICRAR M468, The University of Western Australia, 35 Stirling Hwy, Crawley 6009, Australia
| | - C T Gravestock
- International Centre for Radio Astronomy Research, ICRAR M468, The University of Western Australia, 35 Stirling Hwy, Crawley 6009, Australia
| | - S W Schediwy
- International Centre for Radio Astronomy Research, ICRAR M468, The University of Western Australia, 35 Stirling Hwy, Crawley 6009, Australia
- Australian Research Council Centre of Excellence for Engineered Quantum Systems, Department of Physics, School of Physics, Mathematics & Computing, The University of Western Australia, 35 Stirling Hwy, Crawley 6009, Australia
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Abbott BP, Abbott R, Adhikari R, Ajith P, Allen B, Allen G, Amin RS, Anderson SB, Anderson WG, Arain MA, Araya M, Armandula H, Armor P, Aso Y, Aston S, Aufmuth P, Aulbert C, Babak S, Baker P, Ballmer S, Bantilan H, Barish BC, Barker C, Barker D, Barr B, Barriga P, Barsotti L, Barton MA, Bartos I, Bassiri R, Bastarrika M, Behnke B, Benacquista M, Betzwieser J, Beyersdorf PT, Bilenko IA, Billingsley G, Biswas R, Black E, Blackburn JK, Blackburn L, Blair D, Bland B, Bodiya TP, Bogue L, Bork R, Boschi V, Bose S, Brady PR, Braginsky VB, Brau JE, Brinkmann M, Brooks AF, Brown DA, Brunet G, Bullington A, Buonanno A, Burmeister O, Byer RL, Cadonati L, Cagnoli G, Camp JB, Cannizzo J, Cannon KC, Cao J, Cardenas L, Cardoso V, Caride S, Casebolt T, Castaldi G, Caudill S, Cavaglià M, Cepeda C, Chalkley E, Charlton P, Chatterji S, Chelkowski S, Chen Y, Christensen N, Clark D, Clark J, Clayton JH, Cokelaer T, Conte R, Cook D, Corbitt TRC, Cornish N, Coyne DC, Creighton JDE, Creighton TD, Cruise AM, Cumming A, Cunningham L, Cutler RM, Danzmann K, Daudert B, Davies G, Debra D, Degallaix J, Dergachev V, Desai S, Desalvo R, Dhurandhar S, Díaz M, Dickson J, Dietz A, Donovan F, Dooley KL, Doomes EE, Drever RWP, Duke I, Dumas JC, Dwyer J, Echols C, Edgar M, Effler A, Ehrens P, Ely G, Espinoza E, Etzel T, Evans M, Evans T, Fairhurst S, Faltas Y, Fan Y, Fazi D, Fejer MM, Finn LS, Flasch K, Foley S, Forrest C, Fotopoulos N, Franzen A, Frei Z, Freise A, Frey R, Fricke TT, Fritschel P, Frolov VV, Fyffe M, Garofoli JA, Gholami I, Giaime JA, Giampanis S, Giardina KD, Goda K, Goetz E, Goggin LM, González G, Gossler S, Gouaty R, Grant A, Gras S, Gray C, Gray M, Greenhalgh RJS, Gretarsson AM, Grimaldi F, Grosso R, Grote H, Grunewald S, Guenther M, Gustafson EK, Gustafson R, Hage B, Hallam JM, Hanna C, Hanson J, Harms J, Harry GM, Harstad ED, Haughian E, Hayama K, Hayler T, Heefner J, Heng IS, Heptonstall A, Hewitson M, Hild S, Hirose E, Hoak D, Holt K, Hosken D, Hough J, Huttner SH, Ingram D, Ito M, Ivanov A, Johnson B, Johnson WW, Jones DI, Jones G, Jones R, Ju L, Kalmus P, Kalogera V, Kamat S, Kanner J, Kasprzyk D, Katsavounidis E, Kawabe K, Kawamura S, Kawazoe F, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khan R, Khazanov E, King P, Kissel JS, Klimenko S, Kocsis B, Kokeyama K, Kondrashov V, Kopparapu R, Koranda S, Kozak D, Kozhevatov I, Krishnan B, Kwee P, Landry M, Lantz B, Lazzarini A, Lei M, Leonor I, Li C, Lin H, Lindquist PE, Littenberg TB, Lockerbie NA, Lodhia D, Lormand M, Lu P, Lubinski M, Lucianetti A, Lück H, Machenschalk B, Macinnis M, Mageswaran M, Mailand K, Mandel I, Mandic V, Márka S, Márka Z, Markosyan A, Markowitz J, Maros E, Martin IW, Martin RM, Marx JN, Mason K, Matichard F, Matone L, Matzner R, Mavalvala N, McCarthy R, McClelland DE, McGuire SC, McHugh M, McIntyre G, McKechan D, McKenzie K, Mehmet M, Melissinos A, Mendell G, Mercer RA, Meshkov S, Messenger CJ, Meyers D, Miller A, Miller J, Minelli J, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Miyakawa O, Moe B, Mohanty SD, Moreno G, Mors K, Mossavi K, Mowlowry C, Mueller G, Muhammad D, Mukherjee S, Mukhopadhyay H, Mullavey A, Müller-Ebhardt H, Munch J, Murray PG, Myers E, Myers J, Nash T, Nelson J, Newton G, Nishizawa A, Numata K, Ochsner E, O'Dell J, Ogin G, O'Reilly B, O'Shaughnessy R, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Pan Y, Pankow C, Papa MA, Parameshwaraiah V, Patel P, Pedraza M, Penn S, Perraca A, Petrie T, Pinto IM, Pitkin M, Pletsch HJ, Plissi MV, Postiglione F, Principe M, Prix R, Quetschke V, Raab FJ, Rabeling DS, Radkins H, Raffai P, Rainer N, Rakhmanov M, Ramsunder M, Reed T, Rehbein H, Reid S, Reitze DH, Riesen R, Riles K, Rivera B, Robertson NA, Robinson C, Robinson EL, Roddy S, Rogan AM, Rollins J, Romano JD, Romie JH, Rowan S, Rüdiger A, Ruet L, Russell P, Ryan K, Sakata S, Sancho de la Jordana L, Sandberg V, Sannibale V, Santamaria L, Saraf S, Sarin P, Sathyaprakash BS, Sato S, Saulson PR, Savage R, Savov P, Scanlan M, Schediwy SW, Schilling R, Schnabel R, Schofield R, Schutz BF, Schwinberg P, Scott J, Scott SM, Searle AC, Sears B, Seifert F, Sellers D, Sengupta AS, Sergeev A, Shapiro B, Shawhan P, Shoemaker DH, Sibley A, Siemens X, Sigg D, Sinha S, Sintes AM, Slagmolen BJJ, Slutsky J, Smith JR, Smith MR, Smith ND, Somiya K, Sorazu B, Stein LC, Strain KA, Stuver A, Summerscales TZ, Sun KX, Sung M, Sutton PJ, Takahashi H, Tanner DB, Taylor R, Taylor R, Thacker J, Thorne KA, Thorne KS, Thüring A, Tokmakov KV, Torres C, Torrie C, Traylor G, Trias M, Ugolini D, Urbanek K, Vahlbruch H, Van Den Broeck C, van der Sluys MV, van Veggel AA, Vass S, Vaulin R, Vecchio A, Veitch JD, Veitch P, Villar A, Vorvick C, Vyachanin SP, Waldman SJ, Wallace L, Ward H, Ward RL, Weinert M, Weinstein AJ, Weiss R, Wen L, Wen S, Wette K, Whelan JT, Whitcomb SE, Whiting BF, Wilkinson C, Willems PA, Williams HR, Williams L, Willke B, Wilmut I, Winkler W, Wipf CC, Wiseman AG, Woan G, Wooley R, Worden J, Wu W, Yakushin I, Yamamoto H, Yan Z, Yoshida S, Zanolin M, Zhang J, Zhang L, Zhao C, Zotov N, Zucker ME, Zur Mühlen H, Zweizig J. All-sky LIGO search for periodic gravitational waves in the early fifth-science-run data. Phys Rev Lett 2009; 102:111102. [PMID: 19392186 DOI: 10.1103/physrevlett.102.111102] [Citation(s) in RCA: 11] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/18/2008] [Indexed: 05/11/2023]
Abstract
We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50-1100 Hz and with the frequency's time derivative in the range -5 x 10{-9}-0 Hz s{-1}. Data from the first eight months of the fifth LIGO science run (S5) have been used in this search, which is based on a semicoherent method (PowerFlux) of summing strain power. Observing no evidence of periodic gravitational radiation, we report 95% confidence-level upper limits on radiation emitted by any unknown isolated rotating neutron stars within the search range. Strain limits below 10{-24} are obtained over a 200-Hz band, and the sensitivity improvement over previous searches increases the spatial volume sampled by an average factor of about 100 over the entire search band. For a neutron star with nominal equatorial ellipticity of 10{-6}, the search is sensitive to distances as great as 500 pc.
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Affiliation(s)
- B P Abbott
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
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Abbott BP, Abbott R, Adhikari R, Ajith P, Allen B, Allen G, Amin RS, Anderson SB, Anderson WG, Arain MA, Araya M, Armandula H, Armor P, Aso Y, Aston S, Aufmuth P, Aulbert C, Babak S, Baker P, Ballmer S, Bantilan H, Barish BC, Barker C, Barker D, Barr B, Barriga P, Barsotti L, Barton MA, Bartos I, Bassiri R, Bastarrika M, Behnke B, Benacquista M, Betzwieser J, Beyersdorf PT, Bilenko IA, Billingsley G, Biswas R, Black E, Blackburn JK, Blackburn L, Blair D, Bland B, Bodiya TP, Bogue L, Bork R, Boschi V, Bose S, Brady PR, Braginsky VB, Brau JE, Brinkmann M, Brooks AF, Brown DA, Brunet G, Bullington A, Buonanno A, Burmeister O, Byer RL, Cadonati L, Cagnoli G, Camp JB, Cannizzo J, Cannon KC, Cao J, Cardenas L, Cardoso V, Caride S, Casebolt T, Castaldi G, Caudill S, Cavaglià M, Cepeda C, Chalkley E, Charlton P, Chatterji S, Chelkowski S, Chen Y, Christensen N, Clark D, Clark J, Clayton JH, Cokelaer T, Conte R, Cook D, Corbitt TRC, Cornish N, Coyne DC, Creighton JDE, Creighton TD, Cruise AM, Cumming A, Cunningham L, Cutler RM, Danzmann K, Daudert B, Davies G, Debra D, Degallaix J, Dergachev V, Desai S, Desalvo R, Dhurandhar S, Díaz M, Dickson J, Dietz A, Donovan F, Dooley KL, Doomes EE, Drever RWP, Duke I, Dumas JC, Dwyer J, Echols C, Edgar M, Effler A, Ehrens P, Ely G, Espinoza E, Etzel T, Evans M, Evans T, Fairhurst S, Faltas Y, Fan Y, Fazi D, Fejer MM, Finn LS, Flasch K, Foley S, Forrest C, Fotopoulos N, Franzen A, Frei Z, Freise A, Frey R, Fricke TT, Fritschel P, Frolov VV, Fyffe M, Garofoli JA, Gholami I, Giaime JA, Giampanis S, Giardina KD, Goda K, Goetz E, Goggin LM, González G, Gossler S, Gouaty R, Grant A, Gras S, Gray C, Gray M, Greenhalgh RJS, Gretarsson AM, Grimaldi F, Grosso R, Grote H, Grunewald S, Guenther M, Gustafson EK, Gustafson R, Hage B, Hallam JM, Hanna C, Hanson J, Harms J, Harry GM, Harstad ED, Haughian E, Hayama K, Hayler T, Heefner J, Heng IS, Heptonstall A, Hewitson M, Hild S, Hirose E, Hoak D, Holt K, Hosken D, Hough J, Huttner SH, Ingram D, Ito M, Ivanov A, Johnson B, Johnson WW, Jones DI, Jones G, Jones R, Ju L, Kalmus P, Kalogera V, Kamat S, Kanner J, Kasprzyk D, Katsavounidis E, Kawabe K, Kawamura S, Kawazoe F, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khan R, Khazanov E, King P, Kissel JS, Klimenko S, Kocsis B, Kokeyama K, Kondrashov V, Kopparapu R, Koranda S, Kozak D, Kozhevatov I, Krishnan B, Kwee P, Landry M, Lantz B, Lazzarini A, Lei M, Leonor I, Li C, Lin H, Lindquist PE, Littenberg TB, Lockerbie NA, Lodhia D, Lormand M, Lu P, Lubinski M, Lucianetti A, Lück H, Machenschalk B, Macinnis M, Mageswaran M, Mailand K, Mandel I, Mandic V, Márka S, Márka Z, Markosyan A, Markowitz J, Maros E, Martin IW, Martin RM, Marx JN, Mason K, Matichard F, Matone L, Matzner R, Mavalvala N, McCarthy R, McClelland DE, McGuire SC, McHugh M, McIntyre G, McKechan D, McKenzie K, Mehmet M, Melissinos A, Mendell G, Mercer RA, Meshkov S, Messenger CJ, Meyers D, Miller A, Miller J, Minelli J, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Miyakawa O, Moe B, Mohanty SD, Moreno G, Mors K, Mossavi K, Mowlowry C, Mueller G, Muhammad D, Mukherjee S, Mukhopadhyay H, Mullavey A, Müller-Ebhardt H, Munch J, Murray PG, Myers E, Myers J, Nash T, Nelson J, Newton G, Nishizawa A, Numata K, Ochsner E, O'Dell J, Ogin G, O'Reilly B, O'Shaughnessy R, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Pan Y, Pankow C, Papa MA, Parameshwaraiah V, Patel P, Pedraza M, Penn S, Perraca A, Petrie T, Pinto IM, Pitkin M, Pletsch HJ, Plissi MV, Postiglione F, Principe M, Prix R, Quetschke V, Raab FJ, Rabeling DS, Radkins H, Raffai P, Rainer N, Rakhmanov M, Ramsunder M, Reed T, Rehbein H, Reid S, Reitze DH, Riesen R, Riles K, Rivera B, Robertson NA, Robinson C, Robinson EL, Roddy S, Rogan AM, Rollins J, Romano JD, Romie JH, Rowan S, Rüdiger A, Ruet L, Russell P, Ryan K, Sakata S, Sancho de la Jordana L, Sandberg V, Sannibale V, Santamaria L, Saraf S, Sarin P, Sathyaprakash BS, Sato S, Saulson PR, Savage R, Savov P, Scanlan M, Schediwy SW, Schilling R, Schnabel R, Schofield R, Schutz BF, Schwinberg P, Scott J, Scott SM, Searle AC, Sears B, Seifert F, Sellers D, Sengupta AS, Sergeev A, Shapiro B, Shawhan P, Shoemaker DH, Sibley A, Siemens X, Sigg D, Sinha S, Sintes AM, Slagmolen BJJ, Slutsky J, Smith JR, Smith MR, Smith ND, Somiya K, Sorazu B, Stein LC, Strain KA, Stuver A, Summerscales TZ, Sun KX, Sung M, Sutton PJ, Takahashi H, Tanner DB, Taylor R, Taylor R, Thacker J, Thorne KA, Thorne KS, Thüring A, Tokmakov KV, Torres C, Torrie C, Traylor G, Trias M, Ugolini D, Urbanek K, Vahlbruch H, Van Den Broeck C, van der Sluys MV, van Veggel AA, Vass S, Vaulin R, Vecchio A, Veitch JD, Veitch P, Villar A, Vorvick C, Vyachanin SP, Waldman SJ, Wallace L, Ward H, Ward RL, Weinert M, Weinstein AJ, Weiss R, Wen L, Wen S, Wette K, Whelan JT, Whitcomb SE, Whiting BF, Wilkinson C, Willems PA, Williams HR, Williams L, Willke B, Wilmut I, Winkler W, Wipf CC, Wiseman AG, Woan G, Wooley R, Worden J, Wu W, Yakushin I, Yamamoto H, Yan Z, Yoshida S, Zanolin M, Zhang J, Zhang L, Zhao C, Zotov N, Zucker ME, Zur Mühlen H, Zweizig J. All-sky LIGO search for periodic gravitational waves in the early fifth-science-run data. Phys Rev Lett 2009. [PMID: 19392186 DOI: 10.1103/physrevd.80.042003] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/11/2023]
Abstract
We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50-1100 Hz and with the frequency's time derivative in the range -5 x 10{-9}-0 Hz s{-1}. Data from the first eight months of the fifth LIGO science run (S5) have been used in this search, which is based on a semicoherent method (PowerFlux) of summing strain power. Observing no evidence of periodic gravitational radiation, we report 95% confidence-level upper limits on radiation emitted by any unknown isolated rotating neutron stars within the search range. Strain limits below 10{-24} are obtained over a 200-Hz band, and the sensitivity improvement over previous searches increases the spatial volume sampled by an average factor of about 100 over the entire search band. For a neutron star with nominal equatorial ellipticity of 10{-6}, the search is sensitive to distances as great as 500 pc.
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Affiliation(s)
- B P Abbott
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
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Abbott BP, Abbott R, Adhikari R, Ajith P, Allen B, Allen G, Amin RS, Anderson SB, Anderson WG, Arain MA, Araya M, Armandula H, Armor P, Aso Y, Aston S, Aufmuth P, Aulbert C, Babak S, Baker P, Ballmer S, Bantilan H, Barish BC, Barker C, Barker D, Barr B, Barriga P, Barsotti L, Barton MA, Bartos I, Bassiri R, Bastarrika M, Behnke B, Benacquista M, Betzwieser J, Beyersdorf PT, Bilenko IA, Billingsley G, Biswas R, Black E, Blackburn JK, Blackburn L, Blair D, Bland B, Bodiya TP, Bogue L, Bork R, Boschi V, Bose S, Brady PR, Braginsky VB, Brau JE, Brinkmann M, Brooks AF, Brown DA, Brunet G, Bullington A, Buonanno A, Burmeister O, Byer RL, Cadonati L, Cagnoli G, Camp JB, Cannizzo J, Cannon KC, Cao J, Cardenas L, Cardoso V, Caride S, Casebolt T, Castaldi G, Caudill S, Cavaglià M, Cepeda C, Chalkley E, Charlton P, Chatterji S, Chelkowski S, Chen Y, Christensen N, Clark D, Clark J, Clayton JH, Cokelaer T, Conte R, Cook D, Corbitt TRC, Cornish N, Coyne DC, Creighton JDE, Creighton TD, Cruise AM, Cumming A, Cunningham L, Cutler RM, Danzmann K, Daudert B, Davies G, Debra D, Degallaix J, Dergachev V, Desai S, Desalvo R, Dhurandhar S, Díaz M, Dickson J, Dietz A, Donovan F, Dooley KL, Doomes EE, Drever RWP, Duke I, Dumas JC, Dwyer J, Echols C, Edgar M, Effler A, Ehrens P, Ely G, Espinoza E, Etzel T, Evans M, Evans T, Fairhurst S, Faltas Y, Fan Y, Fazi D, Fejer MM, Finn LS, Flasch K, Foley S, Forrest C, Fotopoulos N, Franzen A, Frei Z, Freise A, Frey R, Fricke TT, Fritschel P, Frolov VV, Fyffe M, Garofoli JA, Gholami I, Giaime JA, Giampanis S, Giardina KD, Goda K, Goetz E, Goggin LM, González G, Gossler S, Gouaty R, Grant A, Gras S, Gray C, Gray M, Greenhalgh RJS, Gretarsson AM, Grimaldi F, Grosso R, Grote H, Grunewald S, Guenther M, Gustafson EK, Gustafson R, Hage B, Hallam JM, Hanna C, Hanson J, Harms J, Harry GM, Harstad ED, Haughian E, Hayama K, Hayler T, Heefner J, Heng IS, Heptonstall A, Hewitson M, Hild S, Hirose E, Hoak D, Holt K, Hosken D, Hough J, Huttner SH, Ingram D, Ito M, Ivanov A, Johnson B, Johnson WW, Jones DI, Jones G, Jones R, Ju L, Kalmus P, Kalogera V, Kamat S, Kanner J, Kasprzyk D, Katsavounidis E, Kawabe K, Kawamura S, Kawazoe F, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khan R, Khazanov E, King P, Kissel JS, Klimenko S, Kocsis B, Kokeyama K, Kondrashov V, Kopparapu R, Koranda S, Kozak D, Kozhevatov I, Krishnan B, Kwee P, Landry M, Lantz B, Lazzarini A, Lei M, Leonor I, Li C, Lin H, Lindquist PE, Littenberg TB, Lockerbie NA, Lodhia D, Lormand M, Lu P, Lubinski M, Lucianetti A, Lück H, Machenschalk B, Macinnis M, Mageswaran M, Mailand K, Mandel I, Mandic V, Márka S, Márka Z, Markosyan A, Markowitz J, Maros E, Martin IW, Martin RM, Marx JN, Mason K, Matichard F, Matone L, Matzner R, Mavalvala N, McCarthy R, McClelland DE, McGuire SC, McHugh M, McIntyre G, McKechan D, McKenzie K, Mehmet M, Melissinos A, Mendell G, Mercer RA, Meshkov S, Messenger CJ, Meyers D, Miller A, Miller J, Minelli J, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Miyakawa O, Moe B, Mohanty SD, Moreno G, Mors K, Mossavi K, Mowlowry C, Mueller G, Muhammad D, Mukherjee S, Mukhopadhyay H, Mullavey A, Müller-Ebhardt H, Munch J, Murray PG, Myers E, Myers J, Nash T, Nelson J, Newton G, Nishizawa A, Numata K, Ochsner E, O'Dell J, Ogin G, O'Reilly B, O'Shaughnessy R, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Pan Y, Pankow C, Papa MA, Parameshwaraiah V, Patel P, Pedraza M, Penn S, Perraca A, Petrie T, Pinto IM, Pitkin M, Pletsch HJ, Plissi MV, Postiglione F, Principe M, Prix R, Quetschke V, Raab FJ, Rabeling DS, Radkins H, Raffai P, Rainer N, Rakhmanov M, Ramsunder M, Reed T, Rehbein H, Reid S, Reitze DH, Riesen R, Riles K, Rivera B, Robertson NA, Robinson C, Robinson EL, Roddy S, Rogan AM, Rollins J, Romano JD, Romie JH, Rowan S, Rüdiger A, Ruet L, Russell P, Ryan K, Sakata S, Sancho de la Jordana L, Sandberg V, Sannibale V, Santamaria L, Saraf S, Sarin P, Sathyaprakash BS, Sato S, Saulson PR, Savage R, Savov P, Scanlan M, Schediwy SW, Schilling R, Schnabel R, Schofield R, Schutz BF, Schwinberg P, Scott J, Scott SM, Searle AC, Sears B, Seifert F, Sellers D, Sengupta AS, Sergeev A, Shapiro B, Shawhan P, Shoemaker DH, Sibley A, Siemens X, Sigg D, Sinha S, Sintes AM, Slagmolen BJJ, Slutsky J, Smith JR, Smith MR, Smith ND, Somiya K, Sorazu B, Stein LC, Strain KA, Stuver A, Summerscales TZ, Sun KX, Sung M, Sutton PJ, Takahashi H, Tanner DB, Taylor R, Taylor R, Thacker J, Thorne KA, Thorne KS, Thüring A, Tokmakov KV, Torres C, Torrie C, Traylor G, Trias M, Ugolini D, Urbanek K, Vahlbruch H, Van Den Broeck C, van der Sluys MV, van Veggel AA, Vass S, Vaulin R, Vecchio A, Veitch JD, Veitch P, Villar A, Vorvick C, Vyachanin SP, Waldman SJ, Wallace L, Ward H, Ward RL, Weinert M, Weinstein AJ, Weiss R, Wen L, Wen S, Wette K, Whelan JT, Whitcomb SE, Whiting BF, Wilkinson C, Willems PA, Williams HR, Williams L, Willke B, Wilmut I, Winkler W, Wipf CC, Wiseman AG, Woan G, Wooley R, Worden J, Wu W, Yakushin I, Yamamoto H, Yan Z, Yoshida S, Zanolin M, Zhang J, Zhang L, Zhao C, Zotov N, Zucker ME, Zur Mühlen H, Zweizig J. All-sky LIGO search for periodic gravitational waves in the early fifth-science-run data. Phys Rev Lett 2009. [PMID: 19392186 DOI: 10.1103/physrevd.79.022001] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/11/2023]
Abstract
We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50-1100 Hz and with the frequency's time derivative in the range -5 x 10{-9}-0 Hz s{-1}. Data from the first eight months of the fifth LIGO science run (S5) have been used in this search, which is based on a semicoherent method (PowerFlux) of summing strain power. Observing no evidence of periodic gravitational radiation, we report 95% confidence-level upper limits on radiation emitted by any unknown isolated rotating neutron stars within the search range. Strain limits below 10{-24} are obtained over a 200-Hz band, and the sensitivity improvement over previous searches increases the spatial volume sampled by an average factor of about 100 over the entire search band. For a neutron star with nominal equatorial ellipticity of 10{-6}, the search is sensitive to distances as great as 500 pc.
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Affiliation(s)
- B P Abbott
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
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Abbott BP, Abbott R, Adhikari R, Ajith P, Allen B, Allen G, Amin RS, Anderson SB, Anderson WG, Arain MA, Araya M, Armandula H, Armor P, Aso Y, Aston S, Aufmuth P, Aulbert C, Babak S, Baker P, Ballmer S, Bantilan H, Barish BC, Barker C, Barker D, Barr B, Barriga P, Barsotti L, Barton MA, Bartos I, Bassiri R, Bastarrika M, Behnke B, Benacquista M, Betzwieser J, Beyersdorf PT, Bilenko IA, Billingsley G, Biswas R, Black E, Blackburn JK, Blackburn L, Blair D, Bland B, Bodiya TP, Bogue L, Bork R, Boschi V, Bose S, Brady PR, Braginsky VB, Brau JE, Brinkmann M, Brooks AF, Brown DA, Brunet G, Bullington A, Buonanno A, Burmeister O, Byer RL, Cadonati L, Cagnoli G, Camp JB, Cannizzo J, Cannon KC, Cao J, Cardenas L, Cardoso V, Caride S, Casebolt T, Castaldi G, Caudill S, Cavaglià M, Cepeda C, Chalkley E, Charlton P, Chatterji S, Chelkowski S, Chen Y, Christensen N, Clark D, Clark J, Clayton JH, Cokelaer T, Conte R, Cook D, Corbitt TRC, Cornish N, Coyne DC, Creighton JDE, Creighton TD, Cruise AM, Cumming A, Cunningham L, Cutler RM, Danzmann K, Daudert B, Davies G, Debra D, Degallaix J, Dergachev V, Desai S, Desalvo R, Dhurandhar S, Díaz M, Dickson J, Dietz A, Donovan F, Dooley KL, Doomes EE, Drever RWP, Duke I, Dumas JC, Dwyer J, Echols C, Edgar M, Effler A, Ehrens P, Ely G, Espinoza E, Etzel T, Evans M, Evans T, Fairhurst S, Faltas Y, Fan Y, Fazi D, Fejer MM, Finn LS, Flasch K, Foley S, Forrest C, Fotopoulos N, Franzen A, Frei Z, Freise A, Frey R, Fricke TT, Fritschel P, Frolov VV, Fyffe M, Garofoli JA, Gholami I, Giaime JA, Giampanis S, Giardina KD, Goda K, Goetz E, Goggin LM, González G, Gossler S, Gouaty R, Grant A, Gras S, Gray C, Gray M, Greenhalgh RJS, Gretarsson AM, Grimaldi F, Grosso R, Grote H, Grunewald S, Guenther M, Gustafson EK, Gustafson R, Hage B, Hallam JM, Hanna C, Hanson J, Harms J, Harry GM, Harstad ED, Haughian E, Hayama K, Hayler T, Heefner J, Heng IS, Heptonstall A, Hewitson M, Hild S, Hirose E, Hoak D, Holt K, Hosken D, Hough J, Huttner SH, Ingram D, Ito M, Ivanov A, Johnson B, Johnson WW, Jones DI, Jones G, Jones R, Ju L, Kalmus P, Kalogera V, Kamat S, Kanner J, Kasprzyk D, Katsavounidis E, Kawabe K, Kawamura S, Kawazoe F, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khan R, Khazanov E, King P, Kissel JS, Klimenko S, Kocsis B, Kokeyama K, Kondrashov V, Kopparapu R, Koranda S, Kozak D, Kozhevatov I, Krishnan B, Kwee P, Landry M, Lantz B, Lazzarini A, Lei M, Leonor I, Li C, Lin H, Lindquist PE, Littenberg TB, Lockerbie NA, Lodhia D, Lormand M, Lu P, Lubinski M, Lucianetti A, Lück H, Machenschalk B, Macinnis M, Mageswaran M, Mailand K, Mandel I, Mandic V, Márka S, Márka Z, Markosyan A, Markowitz J, Maros E, Martin IW, Martin RM, Marx JN, Mason K, Matichard F, Matone L, Matzner R, Mavalvala N, McCarthy R, McClelland DE, McGuire SC, McHugh M, McIntyre G, McKechan D, McKenzie K, Mehmet M, Melissinos A, Mendell G, Mercer RA, Meshkov S, Messenger CJ, Meyers D, Miller A, Miller J, Minelli J, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Miyakawa O, Moe B, Mohanty SD, Moreno G, Mors K, Mossavi K, Mowlowry C, Mueller G, Muhammad D, Mukherjee S, Mukhopadhyay H, Mullavey A, Müller-Ebhardt H, Munch J, Murray PG, Myers E, Myers J, Nash T, Nelson J, Newton G, Nishizawa A, Numata K, Ochsner E, O'Dell J, Ogin G, O'Reilly B, O'Shaughnessy R, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Pan Y, Pankow C, Papa MA, Parameshwaraiah V, Patel P, Pedraza M, Penn S, Perraca A, Petrie T, Pinto IM, Pitkin M, Pletsch HJ, Plissi MV, Postiglione F, Principe M, Prix R, Quetschke V, Raab FJ, Rabeling DS, Radkins H, Raffai P, Rainer N, Rakhmanov M, Ramsunder M, Reed T, Rehbein H, Reid S, Reitze DH, Riesen R, Riles K, Rivera B, Robertson NA, Robinson C, Robinson EL, Roddy S, Rogan AM, Rollins J, Romano JD, Romie JH, Rowan S, Rüdiger A, Ruet L, Russell P, Ryan K, Sakata S, Sancho de la Jordana L, Sandberg V, Sannibale V, Santamaria L, Saraf S, Sarin P, Sathyaprakash BS, Sato S, Saulson PR, Savage R, Savov P, Scanlan M, Schediwy SW, Schilling R, Schnabel R, Schofield R, Schutz BF, Schwinberg P, Scott J, Scott SM, Searle AC, Sears B, Seifert F, Sellers D, Sengupta AS, Sergeev A, Shapiro B, Shawhan P, Shoemaker DH, Sibley A, Siemens X, Sigg D, Sinha S, Sintes AM, Slagmolen BJJ, Slutsky J, Smith JR, Smith MR, Smith ND, Somiya K, Sorazu B, Stein LC, Strain KA, Stuver A, Summerscales TZ, Sun KX, Sung M, Sutton PJ, Takahashi H, Tanner DB, Taylor R, Taylor R, Thacker J, Thorne KA, Thorne KS, Thüring A, Tokmakov KV, Torres C, Torrie C, Traylor G, Trias M, Ugolini D, Urbanek K, Vahlbruch H, Van Den Broeck C, van der Sluys MV, van Veggel AA, Vass S, Vaulin R, Vecchio A, Veitch JD, Veitch P, Villar A, Vorvick C, Vyachanin SP, Waldman SJ, Wallace L, Ward H, Ward RL, Weinert M, Weinstein AJ, Weiss R, Wen L, Wen S, Wette K, Whelan JT, Whitcomb SE, Whiting BF, Wilkinson C, Willems PA, Williams HR, Williams L, Willke B, Wilmut I, Winkler W, Wipf CC, Wiseman AG, Woan G, Wooley R, Worden J, Wu W, Yakushin I, Yamamoto H, Yan Z, Yoshida S, Zanolin M, Zhang J, Zhang L, Zhao C, Zotov N, Zucker ME, Zur Mühlen H, Zweizig J. All-sky LIGO search for periodic gravitational waves in the early fifth-science-run data. Phys Rev Lett 2009. [PMID: 19392186 DOI: 10.1103/physrevd.77.022001] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/11/2023]
Abstract
We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50-1100 Hz and with the frequency's time derivative in the range -5 x 10{-9}-0 Hz s{-1}. Data from the first eight months of the fifth LIGO science run (S5) have been used in this search, which is based on a semicoherent method (PowerFlux) of summing strain power. Observing no evidence of periodic gravitational radiation, we report 95% confidence-level upper limits on radiation emitted by any unknown isolated rotating neutron stars within the search range. Strain limits below 10{-24} are obtained over a 200-Hz band, and the sensitivity improvement over previous searches increases the spatial volume sampled by an average factor of about 100 over the entire search band. For a neutron star with nominal equatorial ellipticity of 10{-6}, the search is sensitive to distances as great as 500 pc.
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Affiliation(s)
- B P Abbott
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
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Abbott B, Abbott R, Adhikari R, Ajith P, Allen B, Allen G, Amin R, Anderson SB, Anderson WG, Arain MA, Araya M, Armandula H, Armor P, Aso Y, Aston S, Aufmuth P, Aulbert C, Babak S, Ballmer S, Bantilan H, Barish BC, Barker C, Barker D, Barr B, Barriga P, Barton MA, Bartos I, Bastarrika M, Bayer K, Betzwieser J, Beyersdorf PT, Bilenko IA, Billingsley G, Biswas R, Black E, Blackburn K, Blackburn L, Blair D, Bland B, Bodiya TP, Bogue L, Bork R, Boschi V, Bose S, Brady PR, Braginsky VB, Brau JE, Brinkmann M, Brooks A, Brown DA, Brunet G, Bullington A, Buonanno A, Burmeister O, Byer RL, Cadonati L, Cagnoli G, Camp JB, Cannizzo J, Cannon K, Cao J, Cardenas L, Casebolt T, Castaldi G, Cepeda C, Chalkley E, Charlton P, Chatterji S, Chelkowski S, Chen Y, Christensen N, Clark D, Clark J, Cokelaer T, Conte R, Cook D, Corbitt T, Coyne D, Creighton JDE, Cumming A, Cunningham L, Cutler RM, Dalrymple J, Danzmann K, Davies G, Debra D, Degallaix J, Degree M, Dergachev V, Desai S, Desalvo R, Dhurandhar S, Díaz M, Dickson J, Dietz A, Donovan F, Dooley KL, Doomes EE, Drever RWP, Duke I, Dumas JC, Dupuis RJ, Dwyer JG, Echols C, Effler A, Ehrens P, Espinoza E, Etzel T, Evans T, Fairhurst S, Fan Y, Fazi D, Fehrmann H, Fejer MM, Finn LS, Flasch K, Fotopoulos N, Freise A, Frey R, Fricke T, Fritschel P, Frolov VV, Fyffe M, Garofoli J, Gholami I, Giaime JA, Giampanis S, Giardina KD, Goda K, Goetz E, Goggin L, González G, Gossler S, Gouaty R, Grant A, Gras S, Gray C, Gray M, Greenhalgh RJS, Gretarsson AM, Grimaldi F, Grosso R, Grote H, Grunewald S, Guenther M, Gustafson EK, Gustafson R, Hage B, Hallam JM, Hammer D, Hanna C, Hanson J, Harms J, Harry G, Harstad E, Hayama K, Hayler T, Heefner J, Heng IS, Hennessy M, Heptonstall A, Hewitson M, Hild S, Hirose E, Hoak D, Hosken D, Hough J, Huttner SH, Ingram D, Ito M, Ivanov A, Johnson B, Johnson WW, Jones DI, Jones G, Jones R, Ju L, Kalmus P, Kalogera V, Kamat S, Kanner J, Kasprzyk D, Katsavounidis E, Kawabe K, Kawamura S, Kawazoe F, Kells W, Keppel DG, Khalili FY, Khan R, Khazanov E, Kim C, King P, Kissel JS, Klimenko S, Kokeyama K, Kondrashov V, Kopparapu RK, Kozak D, Kozhevatov I, Krishnan B, Kwee P, Lam PK, Landry M, Lang MM, Lantz B, Lazzarini A, Lei M, Leindecker N, Leonhardt V, Leonor I, Libbrecht K, Lin H, Lindquist P, Lockerbie NA, Lodhia D, Lormand M, Lu P, Lubinski M, Lucianetti A, Lück H, Machenschalk B, Macinnis M, Mageswaran M, Mailand K, Mandic V, Márka S, Márka Z, Markosyan A, Markowitz J, Maros E, Martin I, Martin RM, Marx JN, Mason K, Matichard F, Matone L, Matzner R, Mavalvala N, McCarthy R, McClelland DE, McGuire SC, McHugh M, McIntyre G, McIvor G, McKechan D, McKenzie K, Meier T, Melissinos A, Mendell G, Mercer RA, Meshkov S, Messenger CJ, Meyers D, Miller J, Minelli J, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Miyakawa O, Moe B, Mohanty S, Moreno G, Mossavi K, Mowlowry C, Mueller G, Mukherjee S, Mukhopadhyay H, Müller-Ebhardt H, Munch J, Murray P, Myers E, Myers J, Nash T, Nelson J, Newton G, Nishizawa A, Numata K, O'Dell J, Ogin G, O'Reilly B, O'Shaughnessy R, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Pan Y, Pankow C, Papa MA, Parameshwaraiah V, Patel P, Pedraza M, Penn S, Perreca A, Petrie T, Pinto IM, Pitkin M, Pletsch HJ, Plissi MV, Postiglione F, Principe M, Prix R, Quetschke V, Raab F, Rabeling DS, Radkins H, Rainer N, Rakhmanov M, Ramsunder M, Rehbein H, Reid S, Reitze DH, Riesen R, Riles K, Rivera B, Robertson NA, Robinson C, Robinson EL, Roddy S, Rodriguez A, Rogan AM, Rollins J, Romano JD, Romie J, Route R, Rowan S, Rüdiger A, Ruet L, Russell P, Ryan K, Sakata S, Samidi M, de la Jordana LS, Sandberg V, Sannibale V, Saraf S, Sarin P, Sathyaprakash BS, Sato S, Saulson PR, Savage R, Savov P, Schediwy SW, Schilling R, Schnabel R, Schofield R, Schutz BF, Schwinberg P, Scott SM, Searle AC, Sears B, Seifert F, Sellers D, Sengupta AS, Shawhan P, Shoemaker DH, Sibley A, Siemens X, Sigg D, Sinha S, Sintes AM, Slagmolen BJJ, Slutsky J, Smith JR, Smith MR, Smith ND, Somiya K, Sorazu B, Stein LC, Stochino A, Stone R, Strain KA, Strom DM, Stuver A, Summerscales TZ, Sun KX, Sung M, Sutton PJ, Takahashi H, Tanner DB, Taylor R, Taylor R, Thacker J, Thorne KA, Thorne KS, Thüring A, Tokmakov KV, Torres C, Torrie C, Traylor G, Trias M, Tyler W, Ugolini D, Ulmen J, Urbanek K, Vahlbruch H, Van Den Broeck C, van der Sluys M, Vass S, Vaulin R, Vecchio A, Veitch J, Veitch P, Villar A, Vorvick C, Vyachanin SP, Waldman SJ, Wallace L, Ward H, Ward R, Weinert M, Weinstein A, Weiss R, Wen S, Wette K, Whelan JT, Whitcomb SE, Whiting BF, Wilkinson C, Willems PA, Williams HR, Williams L, Willke B, Wilmut I, Winkler W, Wipf CC, Wiseman AG, Woan G, Wooley R, Worden J, Wu W, Yakushin I, Yamamoto H, Yan Z, Yoshida S, Zanolin M, Zhang J, Zhang L, Zhao C, Zotov N, Zucker M, Zweizig J, Barthelmy S, Gehrels N, Hurley KC, Palmer D. Search for gravitational-wave bursts from soft gamma repeaters. Phys Rev Lett 2008; 101:211102. [PMID: 19113401 DOI: 10.1103/physrevlett.101.211102] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/01/2008] [Indexed: 05/11/2023]
Abstract
We present a LIGO search for short-duration gravitational waves (GWs) associated with soft gamma ray repeater (SGR) bursts. This is the first search sensitive to neutron star f modes, usually considered the most efficient GW emitting modes. We find no evidence of GWs associated with any SGR burst in a sample consisting of the 27 Dec. 2004 giant flare from SGR 1806-20 and 190 lesser events from SGR 1806-20 and SGR 1900+14. The unprecedented sensitivity of the detectors allows us to set the most stringent limits on transient GW amplitudes published to date. We find upper limit estimates on the model-dependent isotropic GW emission energies (at a nominal distance of 10 kpc) between 3x10;{45} and 9x10;{52} erg depending on waveform type, detector antenna factors and noise characteristics at the time of the burst. These upper limits are within the theoretically predicted range of some SGR models.
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Affiliation(s)
- B Abbott
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
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