1. Results of the deepest all-sky survey for continuous gravitational waves on LIGO S6 data running on the Einstein@Home volunteer distributed computing project
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L. Kleybolte, A. Perreca, Susan M. Scott, Y. Wang, Daniele Trifirò, Chad Hanna, J. Oberling, Jordan Camp, D. B. Kelley, Heinz-Bernd Eggenstein, M. C. Heintze, T. Hardwick, D. Steinmeyer, Fiodor Sorrentino, F. Carbognani, D. Moraru, Gianpietro Cagnoli, F. Nocera, C. Zhao, Rosa Poggiani, F. Travasso, E. O. Lebigot, Thibaut Jacqmin, M. Merzougui, C. I. Torrie, N. Straniero, Z. Patrick, D. R. Ingram, V. Malvezzi, M. Saleem, H. Fair, Andrea Taracchini, J. V. van Heijningen, Eric Thrane, C. Michel, Sarah Caudill, R. Quitzow-James, R. Day, F. Ohme, V. B. Adya, Christopher P. L. Berry, A. D. Silva, P. J. Sutton, V. Frey, T. B. Edo, Alex B. Nielsen, J. H. Romie, Maximiliano Isi, Lionel Martellini, Peter Fritschel, M. Masso-Reid, S. Qiu, Kazuhiro Agatsuma, Enrico Calloni, G. Traylor, Thomas Corbitt, L. Salconi, C. A. Costa, M. K. Gupta, A. Allocca, F. Vetrano, C. C. Arceneaux, J. M. Gonzalez Castro, B. D. Cheeseboro, Archisman Ghosh, G. Cerretani, A. F. Brooks, G. Gemme, M. 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Hanyang Univ, Univ Adelaide, IM PAN, Monash Univ, Seoul Natl Univ, Chinese Univ Hong Kong, Univ Alabama, Univ Massachusetts, Univ Camerino, Southern Univ & A&M Coll, Coll William & Mary, Universidade Estadual Paulista (Unesp), Univ Cambridge, IISER Kolkata, Whitman Coll, Natl Inst Math Sci, Univ Lyon, Hobart & William Smith Coll, Univ Zielona Gora, Univ London, Andrews Univ, Univ Siena, Trinity Univ, Univ Washington, Kenyon Coll, Abilene Christian Univ, Abbott, B. . p., Abbott, T. . d., Abernathy, M. . r., Adhikari, R. . x., Adya, V. . b., Aguiar, O. . d., Altin, P. . a., Anderson, S. . b., Anderson, W. . g., Araya, M. . c., Arceneaux, C. . c., Areeda, J. . s., Arun, K. . g., Aston, S. . m., Bader, M. . k. . m., Baker, P. . t., Ballmer, S. . w., Barayoga, J. . c., Barclay, S. . e., Barish, B. . c., Batch, J. . c., Bell, A. . s., Berger, B. . k., Berry, C. . p. . l., Bilenko, I. . a., Bizouard, M. . a., Blackburn, J. . k., Blair, C. . d., Blair, D. . g., Blair, R. . m., Boom, B. . a., 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- Subjects
Einstein@Home ,Nuclear and High Energy Physics ,[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,gr-qc ,media_common.quotation_subject ,Distributed computing ,Astronomy ,FOS: Physical sciences ,S6 ,Astrophysics ,General Relativity and Quantum Cosmology (gr-qc) ,01 natural sciences ,General Relativity and Quantum Cosmology ,[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] ,0103 physical sciences ,Range (statistics) ,Sensitivity (control systems) ,LIGO ,010306 general physics ,Hardware_REGISTER-TRANSFER-LEVELIMPLEMENTATION ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,STFC ,QC ,media_common ,QB ,Physics ,Gravitational Waves ,010308 nuclear & particles physics ,Gravitational wave ,Physique ,RCUK ,Einstein@Home, LIGO, S6, Gravitational Waves ,Neutron star ,Amplitude ,Physics and Astronomy ,Sky ,[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] ,[ PHYS.ASTR.IM ] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Astrophysics - Instrumentation and Methods for Astrophysics ,astro-ph.IM - Abstract
We report results of a deep all-sky search for periodic gravitational waves from isolated neutron stars in data from the S6 LIGO science run. The search was possible thanks to the computing power provided by the volunteers of the Einstein@Home distributed computing project. We find no significant signal candidate and set the most stringent upper limits to date on the amplitude of gravitational wave signals from the target population. At the frequency of best strain sensitivity, between 170.5 and 171 Hz we set a 90% confidence upper limit of 5.5×10^{-25}, while at the high end of our frequency range, around 505 Hz, we achieve upper limits ≃10^{-24}. At 230 Hz we can exclude sources with ellipticities greater than 10^{-6} within 100 pc of Earth with fiducial value of the principal moment of inertia of 10^{38} kg m^{2}. If we assume a higher (lower) gravitational wave spin-down we constrain farther (closer) objects to higher (lower) ellipticities., National Science Foundation (U.S.), United States. National Aeronautics and Space Administration, Carnegie Trust, Leverhulme Trust, David & Lucile Packard Foundation, Research Corporation, Alfred P. Sloan Foundation
- Published
- 2016