All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run

被引:57
作者
Abbott, R. [1 ]
Abbott, T. D. [2 ]
Acernese, F. [3 ,4 ]
Ackley, K. [5 ]
Adams, C. [6 ]
Adhikari, N. [7 ]
Adhikari, R. X. [1 ]
Adya, V. B. [8 ]
Affeldt, C. [9 ,10 ]
Agarwal, D. [11 ]
Agathos, M. [12 ,13 ]
Agatsuma, K. [14 ]
Aggarwal, N. [15 ]
Aguiar, O. D. [16 ]
Aiello, L. [17 ]
Ain, A. [18 ]
Ajith, P. [19 ]
Akutsu, T. [20 ,21 ]
Albanesi, S. [22 ]
Allocca, A. [4 ,23 ]
Altin, P. A. [8 ]
Amato, A. [24 ]
Anand, C. [5 ]
Anand, S. [1 ]
Ananyeva, A. [1 ]
Anderson, S. B. [1 ]
Anderson, W. G. [7 ]
Ando, M. [25 ,26 ]
Andrade, T. [27 ]
Andres, N. [28 ]
Angelova, S., V [30 ]
Ansoldi, S. [31 ,32 ]
Antelis, J. M. [33 ]
Antier, S. [34 ]
Appert, S. [1 ]
Arai, Koji [1 ]
Arai, Koya [35 ]
Arai, Y. [35 ]
Araki, S. [36 ]
Araya, A. [37 ]
Araya, M. C. [1 ]
Areeda, J. S. [38 ]
Arene, M. [34 ]
Aritomi, N. [25 ]
Arnaud, N. [39 ,40 ]
Aronson, S. M. [2 ]
Arun, K. G. [41 ]
Asada, H. [42 ]
Asali, Y. [43 ]
Ashton, G. [5 ]
机构
[1] CALTECH, LIGO Lab, Pasadena, CA 91125 USA
[2] Louisiana State Univ, Baton Rouge, LA 70803 USA
[3] Univ Salerno, Dipartimento Farm, I-84084 Salerno, Italy
[4] Complesso Univ Monte S Angelo, Sez Napoli, Ist Nazl Fis Nucl, I-80126 Naples, Italy
[5] Monash Univ, Sch Phys & Astron, OzGrav, Clayton, Vic 3800, Australia
[6] LIGO Livingston Observ, Livingston, LA 70754 USA
[7] Univ Wisconsin, Milwaukee, WI 53201 USA
[8] Australian Natl Univ, OzGrav, Canberra, ACT 0200, Australia
[9] Albert Einstein Inst, Max Planck Inst Gravitat Phys, D-30167 Hannover, Germany
[10] Leibniz Univ Hannover, D-30167 Hannover, Germany
[11] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
[12] Univ Cambridge, Cambridge CB2 1TN, England
[13] Friedrich Schiller Univ Jena, Theoret Phys Inst, D-07743 Jena, Germany
[14] Univ Birmingham, Birmingham B15 2TT, W Midlands, England
[15] Northwestern Univ, Ctr Interdisciplinary Explorat & Res Astrophys CI, Evanston, IL 60208 USA
[16] Inst Nacl Pesquisas Espaciais, BR-12227010 Sao Jose Dos Campos, SP, Brazil
[17] Cardiff Univ, Grav Explorat Inst, Cardiff CF24 3AA, Wales
[18] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy
[19] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bengaluru 560089, India
[20] Natl Astron Observ Japan NAOJ, Gravitat Wave Sci Project, Mitaka, Tokyo 1818588, Japan
[21] Natl Astron Observ Japan NAOJ, Adv Technol Ctr, Mitaka, Tokyo 1818588, Japan
[22] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy
[23] Univ Napoli Federico II, Complesso Univ Monte S Angelo, I-80126 Naples, Italy
[24] Univ Claude Bernard Lyon 1, Univ Lyon, Inst Lumiere Matiere, CNRS, F-69622 Villeurbanne, France
[25] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan
[26] Univ Tokyo, Res Ctr Early Universe RESCEU, Bunkyo Ku, Tokyo 1130033, Japan
[27] Univ Barcelona, Inst Ciencies Cosmos ICCUB, Barcelona 08028, Spain
[28] Univ Grenoble Alpes, Univ Savoie Mt Blanc, Lab Annecy Phys Particules LAPP, CNRS IN2P3, F-74941 Annecy, France
[29] Gran Sasso Sci Inst GSSI, I-67100 Laquila, Italy
[30] Univ Strathclyde, SUPA, Glasgow G1 1XQ, Lanark, Scotland
[31] Univ Udine, Dipartimento Sci Matemat Informat & Fis, I-33100 Udine, Italy
[32] Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy
[33] Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA
[34] Univ Paris, Astroparticule & Cosmol, CNRS, F-75006 Paris, France
[35] Univ Tokyo, Inst Cosm Ray Res ICRR, KAGRA Observ, Kashiwa, Chiba 2778582, Japan
[36] High Energy Accelerator Res Org KEK, Accelerator Lab, Tsukuba, Ibaraki 3050801, Japan
[37] Univ Tokyo, Earthquake Res Inst, Bunkyo Ku, Tokyo 1130032, Japan
[38] Calif State Univ Fullerton, Fullerton, CA 92831 USA
[39] Univ Paris Saclay, IJCLab, CNRS IN2P3, F-91405 Orsay, France
[40] European Gravitat Observ EGO, I-56021 Pisa, Italy
[41] Chennai Math Inst, Chennai 603103, Tamil Nadu, India
[42] Hirosaki Univ, Dept Math & Phys, Gravitat Wave Sci Project, Hirosaki, Aomori 0368561, Japan
[43] Columbia Univ, New York, NY 10027 USA
[44] Natl Astron Observ Japan NAOJ, Kamioka Branch, Kamioka Cho, Hida City, Gifu 5061205, Japan
[45] Grad Univ Adv Studies SOKENDAI, Mitaka, Tokyo 1818588, Japan
[46] Univ Urbino Carlo Bo, I-61029 Urbino, Italy
[47] Ist Nazl Fis Nucl, Sez Firenze, I-50019 Florence, Italy
[48] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy
[49] Catholic Univ Louvain, B-1348 Louvain La Neuve, Belgium
[50] Nikhef, Sci Pk 105, NL-1098 XG Amsterdam, Netherlands
基金
美国国家科学基金会; 英国科学技术设施理事会; 新加坡国家研究基金会; 澳大利亚研究理事会;
关键词
CORE-COLLAPSE; ACCRETION SHOCK; INSTABILITY; GLITCHES;
D O I
10.1103/PhysRevD.104.122004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper presents the results of a search for generic short-duration gravitational-wave transients in data from the third observing run of Advanced LIGO and Advanced Virgo. Transients with durations of milliseconds to a few seconds in the 24-4096 Hz frequency band are targeted by the search, with no assumptions made regarding the incoming signal direction, polarization, or morphology. Gravitational waves from compact binary coalescences that have been identified by other targeted analyses are detected, but no statistically significant evidence for other gravitational wave bursts is found. Sensitivities to a variety of signals are presented. These include updated upper limits on the source rate density as a function of the characteristic frequency of the signal, which are roughly an order of magnitude better than previous upper limits. This search is sensitive to sources radiating as little as X10-10 Moc2 in gravitational waves at -70 Hz from a distance of 10 kpc, with 50% detection efficiency at a false alarm rate of one per century. The sensitivity of this search to two plausible astrophysical sources is estimated: neutron star f modes, which may be excited by pulsar glitches, as well as selected core-collapse supernova models.
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页数:24
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