Search for Subsolar-Mass Ultracompact Binaries in Advanced LIGO's First Observing Run

被引：82

作者：

Abbott, B. P. ^{[1
]}

Abbott, R. ^{[1
]}

Abbott, T. D. ^{[2
]}

Acernese, F. ^{[3
,4
]}

Ackley, K. ^{[5
]}

Adams, C. ^{[6
]}

Adams, T. ^{[7
]}

Addesso, P. ^{[8
,9
]}

Adhikari, R. X. ^{[1
]}

Adya, V. B. ^{[10
,11
]}

Affeldt, C. ^{[10
,11
]}

Agarwal, B. ^{[12
]}

Agathos, M. ^{[13
]}

Agatsuma, K. ^{[14
]}

Aggarwal, N. ^{[15
]}

Aguiar, O. D. ^{[16
]}

Aiello, L. ^{[17
,18
]}

Ain, A. ^{[19
]}

Ajith, P. ^{[20
]}

Allen, B. ^{[10
,11
,21
]}

Allen, G. ^{[12
]}

Allocca, A. ^{[22
,23
]}

Aloy, M. A. ^{[24
]}

Altin, P. A. ^{[25
]}

Amato, A. ^{[26
]}

Ananyeva, A. ^{[1
]}

Anderson, S. B. ^{[1
]}

Anderson, W. G. ^{[21
]}

Angelova, S., V ^{[27
]}

Antier, S. ^{[28
]}

Appert, S. ^{[1
]}

Arai, K. ^{[1
]}

Araya, M. C. ^{[1
]}

Areeda, J. S. ^{[29
]}

Arene, M. ^{[30
]}

Arnaud, N. ^{[28
,31
]}

Arun, K. G. ^{[32
]}

Ascenzi, S. ^{[33
,34
]}

Ashton, G. ^{[5
]}

Ast, M. ^{[35
]}

Aston, S. M. ^{[6
]}

Astone, P. ^{[36
]}

Atallah, D., V ^{[37
]}

Aubin, F. ^{[7
]}

Aufmuth, P. ^{[11
]}

Aulbert, C. ^{[10
]}

AultOneal, K. ^{[38
]}

Austin, C. ^{[2
]}

Avila-Alvarez, A. ^{[29
]}

Babak, S. ^{[30
,39
]}

机构：

[1] CALTECH, LIGO, Pasadena, CA 91125 USA

[2] Louisiana State Univ, Baton Rouge, LA 70803 USA

[3] Univ Salerno, Fisciano, I-84084 Salerno, Italy

[4] Complesso Univ Monte S Angelo, Sez Napoli, INFN, 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 Grenoble Alpes, Univ Savoie Mont Blanc, LAPP, CNRS,IN2P3, F-74941 Annecy, France

[8] Univ Sannio Benevento, I-82100 Naples, Italy

[9] INFN, Sez Napoli, I-80100 Naples, Italy

[10] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany

[11] Leibniz Univ Hannover, D-30167 Hannover, Germany

[12] Univ Illinois, NCSA, Urbana, IL 61801 USA

[13] Univ Cambridge, Cambridge CB2 1TN, England

[14] Nikhef, Sci Pk 105, NL-1098 XG Amsterdam, Netherlands

[15] MIT, LIGO, Cambridge, MA 02139 USA

[16] Inst Nacl Pesquisas Espaciais, BR-12227010 Sao Jose Dos Campos, SP, Brazil

[17] GSSI, I-67100 Laquila, Italy

[18] INFN, Lab Nazl Gran Sasso, I-67100 Assergi, Italy

[19] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India

[20] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bengaluru 560089, India

[21] Univ Wisconsin, Milwaukee, WI 53201 USA

[22] Univ Pisa, I-56127 Pisa, Italy

[23] INFN, Sez Pisa, I-56127 Pisa, Italy

[24] Univ Valencia, Dept Astron & Astrofis, E-46100 Valencia, Spain

[25] Australian Natl Univ, OzGrav, Canberra, ACT 0200, Australia

[26] CNRS, IN2P3, LMA, F-69622 Villeurbanne, France

[27] Univ Strathclyde, SUPA, Glasgow G1 1XQ, Lanark, Scotland

[28] Univ Paris Sud, Univ Paris Saclay, LAL, CNRS,IN2P3, F-91898 Orsay, France

[29] Calif State Univ Fullerton, Fullerton, CA 92831 USA

[30] Univ Paris Diderot, CNRS, IN2P3, CEA Irfu,Observ Paris,APC, F-75205 Paris 13, France

[31] EGO, I-56021 Pisa, Italy

[32] Chennai Math Inst, Madras 603103, Tamil Nadu, India

[33] Univ Roma Tor Vergata, I-00133 Rome, Italy

[34] INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy

[35] Univ Hamburg, D-22761 Hamburg, Germany

[36] INFN, Sez Roma, I-00185 Rome, Italy

[37] Cardiff Univ, Cardiff CF24 3AA, S Glam, Wales

[38] Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA

[39] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Potsdam, Germany

[40] Korea Inst Sci & Technol Informat, Daejeon 34141, South Korea

[41] West Virginia Univ, Morgantown, WV 26506 USA

[42] Univ Perugia, I-06123 Perugia, Italy

[43] INFN, Sez Perugia, I-06123 Perugia, Italy

[44] Syracuse Univ, Syracuse, NY 13244 USA

[45] Univ Minnesota, Minneapolis, MN 55455 USA

[46] Univ Glasgow, SUPA, Glasgow G12 8QQ, Lanark, Scotland

[47] Hanford Observ, LIGO, Richland, WA 99352 USA

[48] Caltech CaRT, Pasadena, CA 91125 USA

[49] RMKI, Wiper RCP, Konkoly Thege Miklos Ut 29-33, H-1121 Budapest, Hungary

[50] Univ Florida, Gainesville, FL 32611 USA

来源：

PHYSICAL REVIEW LETTERS | 2018年 / 121卷 / 23期

基金：

匈牙利科学研究基金会; 英国科学技术设施理事会; 俄罗斯基础研究基金会; 瑞士国家科学基金会; 俄罗斯科学基金会; 美国国家科学基金会; 新加坡国家研究基金会; 中国国家自然科学基金; 澳大利亚研究理事会;

关键词：

LIMITS;

D O I：

10.1103/PhysRevLett.121.231103

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We present the first Advanced LIGO and Advanced Virgo search for ultracompact binary systems with component masses between 0.2 M-circle dot-1.0 M-circle dot using data taken between September 12, 2015 and January 19, 2016. We find no viable gravitational wave candidates. Our null result constrains the coalescence rate of monochromatic (delta function) distributions of nonspinning (0.2 M-circle dot, 0.2 M-circle dot) ultracompact binaries to be less than 1.0 x 10(6) Gpc(-3) yr(-1) and the coalescence rate of a similar distribution of (1.0 M-circle dot, 1.0 M-circle dot) ultracompact binaries to be less than 1.9 x Gpc(-3) yr(-1) (at 90% confidence). Neither black holes nor neutron stars are expected to form below similar to 1 M-circle dot through conventional stellar evolution, though it has been proposed that similarly low mass black holes could be formed primordially through density fluctuations in the early Universe and contribute to the dark matter density. The interpretation of our constraints in the primordial black hole dark matter paradigm is highly model dependent; however, under a particular primordial black hole binary formation scenario we constrain monochromatic primordial black hole populations of 0.2 M-circle dot to be less than 33% of the total dark matter density and monochromatic populations of 1.0 M-circle dot to be less than 5% of the dark matter density. The latter strengthens the presently placed bounds from microlensing surveys of massive compact halo objects (MACHOs) provided by the MACHO and EROS Collaborations.

引用

页数：13

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