Optically targeted search for gravitational waves emitted by core-collapse supernovae during the first and second observing runs of advanced LIGO and advanced Virgo

被引：76
|
作者：
Abbott, B. P. [1 ]
Abbott, R. [1 ]
Abbott, T. D. [2 ]
Abraham, S. [3 ]
Acernese, F. [4 ,5 ]
Ackley, K. [6 ]
Adams, C. [7 ]
Adya, V. B. [8 ]
Affeldt, C. [9 ,10 ]
Agathos, M. [11 ,12 ]
Agatsuma, K. [13 ]
Aggarwal, N. [14 ]
Aguiar, O. D. [15 ]
Aiello, L. [16 ,17 ]
Ain, A. [3 ]
Ajith, P. [18 ]
Allen, G. [19 ]
Allocca, A. [20 ,21 ]
Aloy, M. A. [22 ]
Altin, P. A. [8 ]
Amato, A. [23 ]
Anand, S. [1 ]
Ananyeva, A. [1 ]
Anderson, S. B. [1 ]
Anderson, W. G. [24 ]
Angelova, S., V [25 ]
Antier, S. [26 ]
Appert, S. [1 ]
Arai, K. [1 ]
Araya, M. C. [1 ]
Areeda, J. S. [27 ]
Arene, M. [26 ]
Arnaud, N. [28 ,29 ]
Aronson, S. M. [30 ]
Ascenzi, S. [16 ,31 ]
Ashton, G. [6 ]
Aston, S. M. [7 ]
Astone, P. [32 ]
Aubin, F. [33 ]
Aufmuth, P. [10 ]
AultONeal, K. [34 ]
Austin, C. [2 ]
Avendano, V [35 ]
Avila-Alvarez, A. [27 ]
Babak, S. [26 ]
Bacon, P. [26 ]
Badaracco, F. [16 ,17 ]
Bader, M. K. M. [36 ]
Bae, S. [37 ]
Baird, J. [26 ]
机构：
[1] CALTECH, LIGO, Pasadena, CA 91125 USA
[2] Louisiana State Univ, Baton Rouge, LA 70803 USA
[3] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
[4] Univ Salerno, Dipartimento Farm, I-84084 Salerno, Italy
[5] INFN, Sez Napoli, Complesso Univ Monte S Angelo, I-80126 Naples, Italy
[6] Monash Univ, Sch Phys & Astron, OzGrav, Clayton, Vic 3800, Australia
[7] LIGO Livingston Observ, Livingston, LA 70754 USA
[8] Australian Natl Univ, OzGrav, Canberra, ACT 0200, Australia
[9] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany
[10] Leibniz Univ Hannover, D-30167 Hannover, Germany
[11] Friedrich Schiller Univ Jena, Theoret Phys Inst, D-07743 Jena, Germany
[12] Univ Cambridge, Cambridge CB2 1TN, England
[13] Univ Birmingham, Birmingham B15 2TT, W Midlands, England
[14] MIT, LIGO, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[15] Inst Nacl Pesquisas Espaciais, BR-12227010 Sao Jose Dos Campos, SP, Brazil
[16] GSSI, I-67100 Laquila, Italy
[17] INFN, Lab Nazl Gran Sasso, I-67100 Assergi, Italy
[18] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bengaluru 560089, India
[19] Univ Illinois, NCSA, Urbana, IL 61801 USA
[20] Univ Pisa, I-56127 Pisa, Italy
[21] INFN, Sez Pisa, I-56127 Pisa, Italy
[22] Univ Valencia, Dept Astron & Astrofis, E-46100 Valencia, Spain
[23] CNRS, IN2P3, LMA, F-69622 Villeurbanne, France
[24] Univ Wisconsin, Milwaukee, WI 53201 USA
[25] Univ Strathclyde, SUPA, Glasgow G1 1XQ, Lanark, Scotland
[26] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, Irfu,APC,AstroParticule & Cosmol,CNRS IN2P3,CEA, F-75205 Paris 13, France
[27] Calif State Univ Fullerton, Fullerton, CA 92831 USA
[28] Univ Paris Sud, Univ Paris Saclay, IN2P3, CNRS,LAL, F-91898 Orsay, France
[29] EGO, I-56021 Pisa, Italy
[30] Univ Florida, Gainesville, FL 32611 USA
[31] INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy
[32] INFN, Sez Roma, I-00185 Rome, Italy
[33] Univ Grenoble Alpes, Univ Savoie Mt Blanc, LAPP, IN2P3,CNRS, F-74941 Annecy, France
[34] Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA
[35] Montclair State Univ, Montclair, NJ 07043 USA
[36] Nikhef, Sci Pk 105, NL-1098 XG Amsterdam, Netherlands
[37] Korea Inst Sci & Technol Informat, Daejeon 34141, South Korea
[38] West Virginia Univ, Morgantown, WV 26506 USA
[39] Univ Perugia, I-06123 Perugia, Italy
[40] INFN, Sez Perugia, I-06123 Perugia, Italy
[41] Syracuse Univ, Syracuse, NY 13244 USA
[42] Univ Minnesota, Minneapolis, MN 55455 USA
[43] Univ Milano Bicocca, I-20126 Milan, Italy
[44] INFN, Sez Milano Bicocca, I-20126 Milan, Italy
[45] Univ Glasgow, SUPA, Glasgow G12 8QQ, Lanark, Scotland
[46] LIGO Hanford Observ, Richland, WA 99352 USA
[47] Caltech CaRT, Pasadena, CA 91125 USA
[48] Univ Salerno, Scuola Med Salemitana, Dipartimento Med Chirurg & Odontoiatria, I-84081 Salerno, Italy
[49] RMKI, Wigner RCP, Konkoly Thege Miklos Ut 29-33, H-1121 Budapest, Hungary
[50] Stanford Univ, Stanford, CA 94305 USA
来源：
PHYSICAL REVIEW D | 2020年 / 101卷 / 08期
基金：
美国国家科学基金会; 瑞士国家科学基金会; 俄罗斯基础研究基金会; 俄罗斯科学基金会; 匈牙利科学研究基金会; 新加坡国家研究基金会; 中国国家自然科学基金;
关键词：
BAR-MODE INSTABILITY; II-P SUPERNOVA; NEUTRINO BURST; SHOCK BREAKOUT; EXPLOSION MECHANISM; STARS; SIMULATIONS; PROGENITOR; CURVE; RADIATION;
D O I：
10.1103/PhysRevD.101.084002
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present the results from a search for gravitational-wave transients associated with core-collapse supernovae observed within a source distance of approximately 20 Mpc during the first and second observing runs of Advanced LIGO and Advanced Virgo. No significant gravitational-wave candidate was detected. We report the detection efficiencies as a function of the distance for waveforms derived from multidimensional numerical simulations and phenomenological extreme emission models. The sources with neutrino-driven explosions are detectable at the distances approaching 5 kpc, and for magnetorotationally driven explosions the distances are up to 54 kpc. However, waveforms for extreme emission models are detectable up to 28 Mpc. For the first time, the gravitational-wave data enabled us to exclude part of the parameter spaces of two extreme emission models with confidence up to 83%, limited by coincident data coverage. Besides, using ad hoc harmonic signals windowed with Gaussian envelopes, we constrained the gravitational-wave energy emitted during core collapse at the levels of 4.27 x 10(-4) M(circle dot)c(2) and 1.28 x 10(-1) M(circle dot)c(2) for emissions at 235 and 1304 Hz, respectively. These constraints are 2 orders of magnitude more stringent than previously derived in the corresponding analysis using initial LIGO, initial Virgo, and GEO 600 data.
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页数：24
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