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：82

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; 中国国家自然科学基金; 新加坡国家研究基金会; 俄罗斯科学基金会; 匈牙利科学研究基金会;

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.

引用

页数：24

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