First joint observation by the underground gravitational-wave detector KAGRA with GEO 600

被引：32

作者：

Abbott, R. ^{[1
]}

Abe, H. ^{[2
]}

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

Ackley, K. ^{[5
]}

Adhikari, N. ^{[6
]}

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

Adkins, V. K. ^{[7
]}

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
,23
]}

Alfaidi, R. A. ^{[24
]}

Allocca, A. ^{[4
,25
]}

Altin, P. A. ^{[8
]}

Amato, A. ^{[26
]}

Anand, C. ^{[5
]}

Anand, S. ^{[1
]}

Ananyeva, A. ^{[1
]}

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

Anderson, W. G. ^{[6
]}

Ando, M. ^{[27
,28
]}

Andrade, T. ^{[29
]}

Andres, N. ^{[30
]}

Andres-Carcasona, M. ^{[31
,32
]}

Angelova, S., V ^{[34
]}

Ansoldi, S. ^{[35
,36
]}

Antelis, J. M. ^{[37
]}

Antier, S. ^{[38
,39
,40
]}

Apostolatos, T. ^{[41
]}

Appavuravther, E. Z. ^{[42
,43
]}

Appert, S. ^{[1
]}

Apple, S. K. ^{[44
]}

Arai, K. ^{[1
]}

Araya, A. ^{[45
]}

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

Areeda, J. S. ^{[46
]}

Arene, M. ^{[47
]}

Aritomi, N. ^{[20
]}

Arnaud, N. ^{[48
,49
]}

Arogeti, M. ^{[50
]}

Aronson, S. M. ^{[7
]}

Arun, K. G. ^{[51
]}

机构：

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

[2] Tokyo Inst Technol, Grad Sch Sci, Meguro Ku, Tokyo 1528551, Japan

[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] Univ Wisconsin, Milwaukee, WI 53201 USA

[7] Louisiana State Univ, Baton Rouge, LA 70803 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, Evanston, IL 60208 USA

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

[17] Cardiff Univ, Cardiff CP24 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] Univ Torino, Dipartimento Fis, I-10125 Turin, Italy

[23] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy

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

[25] Univ Napoli Federico II, Complesso Univ Monte S Angelo, I-80126 Naples, Italy

[26] Univ Lyon, Univ Claude Bernard Lyon 1, Inst Lumiere Matiere, CNRS, F-69622 Villeurbanne, France

[27] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan

[28] Univ Tokyo, Res Ctr Early Universe RESCEU, Bunkyo Ku, Tokyo 1130033, Japan

[29] Univ Barcelona, Inst Ciencies Cosmos ICCUB, Barcelona 08028, Spain

[30] Univ Savoie Mt Blanc, Lab Annecy Phys Particules IN2P3, CNRS, F-74000 Annecy, France

[31] Barcelona Inst Sci & Technol, Inst Fis Altes Energies IFAE, E-08193 Barcelona, Spain

[32] ICREA, E-08193 Barcelona, Spain

[33] Gran Sasso Sci Inst GSSI, I-67100 Laquila, Italy

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

[35] Univ Udine, Dipartimento Sci Matemat Informat & Fis, I-33100 Udine, Italy

[36] Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy

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

[38] Univ Cote dAzur, Observ Cote dAzur, CNRS, Artemis, F-06304 Nice, France

[39] Univ Amsterdam, Anton Pannekoek Inst Astron, GRAPPA, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[40] Univ Amsterdam, Inst High Energy Phys, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[41] Natl & Kapodistrian Univ Athens, Sch Sci Bldg,2 Nd Floor, Panepistimiopolis 15771, Ilissia, Greece

[42] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy

[43] Univ Camerino, Dipartimento Fis, I-62032 Camerino, Italy

[44] American Univ, Washington, DC 20016 USA

[45] Univ Tokyo, Earthquake Res Inst, Bunkyo Ku, Tokyo 1130032, Japan

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

[47] Univ Paris, Astroparticule & Cosmol, CNRS, F-75006 Paris, France

[48] Univ Paris Saclay, IJCLab, CNRS IN2P3, F-91405 Orsay, France

[49] European Gravitat Observ EGO, I-56021 Pisa, Italy

[50] Georgia Inst Technol, Atlanta, GA 30332 USA

来源：

PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS | 2022年 / 2022卷 / 06期

基金：

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

关键词：

F31; F32; F33; F34; GAMMA-RAY BURST; BINARY NEUTRON-STAR; 2ND OBSERVING RUN; ADVANCED LIGO; PRECURSOR ACTIVITY; RELATIVISTIC JETS; SEARCH TEMPLATES; HUBBLE CONSTANT; X-RAY; FERMI;

D O I：

10.1093/ptep/ptac073

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We report the results of the first joint observation of the KAGRA detector with GEO600. KAGRA is a cryogenic and underground gravitational-wave detector consisting of a laser interferometer with 3km arms, located in Kamioka, Gifu, Japan. GEO600 is a British-German laser interferometer with 600m arms, located near Hannover, Germany. GEO600 and KAGRA performed a joint observing run from April 7 to 20, 2020. We present the results of the joint analysis of the GEO-KAGRA data for transient gravitational-wave signals, including the coalescence of neutron-star binaries and generic unmodeled transients. We also perform dedicated searches for binary coalescence signals and generic transients associated with gamma-ray burst events observed during the joint run. No gravitational-wave events were identified. We evaluate the minimum detectable amplitude for various types of transient signals and the spacetime volume for which the network is sensitive to binary neutron-star coalescences. We also place lower limits on the distances to the gamma-ray bursts analyzed based on the non-detection of an associated gravitational-wave signal for several signal models, including binary coalescences. These analyses demonstrate the feasibility and utility of KAGRA as a member of the global gravitational-wave detector network.

引用

页数：37

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