Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube

被引：35

作者：

Aartsen, M. G. ^{[2
]}

Ackermann, M. ^{[50
]}

Adams, J. ^{[16
]}

Aguilar, J. A. ^{[25
]}

Ahlers, M. ^{[30
,31
]}

Ahrens, M. ^{[40
,41
]}

Altmann, D. ^{[24
]}

Anderson, T. ^{[47
]}

Arguelles, C. ^{[30
,31
]}

Arlen, T. C. ^{[47
]}

Auffenberg, J. ^{[1
]}

Bai, X. ^{[38
]}

Barwick, S. W. ^{[27
]}

Baum, V. ^{[32
]}

Beatty, J. J. ^{[18
,19
,20
]}

Tjus, J. Becker ^{[11
]}

Becker, K. -H. ^{[49
]}

BenZvi, S. ^{[30
,31
]}

Berghaus, P. ^{[50
]}

Berley, D. ^{[17
]}

Bernardini, E. ^{[50
]}

Bernhard, A. ^{[34
]}

Besson, D. Z. ^{[28
]}

Binder, G. ^{[8
,9
]}

Bindig, D. ^{[49
]}

Bissok, M. ^{[1
]}

Blaufuss, E. ^{[17
]}

Blumenthal, J. ^{[1
]}

Boersma, D. J. ^{[48
]}

Bohm, C. ^{[40
,41
]}

Bos, F. ^{[11
]}

Bose, D. ^{[43
]}

Boeser, S. ^{[12
]}

Botner, O. ^{[48
]}

Brayeur, L. ^{[14
]}

Bretz, H. -P. ^{[50
]}

Brown, A. M. ^{[16
]}

Casey, J. ^{[5
,6
]}

Casier, M. ^{[14
]}

Chirkin, D. ^{[30
,31
]}

Christov, A. ^{[25
]}

Christy, B. ^{[17
]}

Clark, K. ^{[44
]}

Classen, L. ^{[24
]}

Clevermann, F. ^{[22
]}

Coenders, S. ^{[34
]}

Cowen, D. F. ^{[46
,47
]}

Silva, A. H. Cruz ^{[50
]}

Danninger, M. ^{[40
,41
]}

Daughhetee, J. ^{[5
,6
]}

机构：

[1] Rhein Westfal TH Aachen, Inst Phys 3, D-52056 Aachen, Germany

[2] Univ Adelaide, Sch Chem & Phys, Adelaide, SA 5005, Australia

[3] Univ Alaska Anchorage, Dept Phys & Astron, Anchorage, AK 99508 USA

[4] Clark Atlanta Univ, CTSPS, Atlanta, GA 30314 USA

[5] Georgia Inst Technol, Sch Phys, Atlanta, GA 30332 USA

[6] Georgia Inst Technol, Ctr Relativist Astrophys, Atlanta, GA 30332 USA

[7] Southern Univ, Dept Phys, Baton Rouge, LA 70813 USA

[8] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[9] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA

[10] Humboldt Univ, Inst Phys, D-12489 Berlin, Germany

[11] Ruhr Univ Bochum, Fak Phys & Astron, D-44780 Bochum, Germany

[12] Univ Bonn, Inst Phys, D-53115 Bonn, Germany

[13] Univ Libre Bruxelles, Sci Fac CP230, B-1050 Brussels, Belgium

[14] Vrije Univ Brussel, Dienst ELEM, B-1050 Brussels, Belgium

[15] Chiba Univ, Dept Phys, Chiba 2638522, Japan

[16] Univ Canterbury, Dept Phys & Astron, Christchurch 1, New Zealand

[17] Univ Maryland, Dept Phys, College Pk, MD 20742 USA

[18] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA

[19] Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA

[20] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA

[21] Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark

[22] TU Dortmund Univ, Dept Phys, D-44221 Dortmund, Germany

[23] Univ Alberta, Dept Phys, Edmonton, AB T6G 2E1, Canada

[24] Univ Erlangen Nurnberg, Erlangen Ctr Astroparticle Phys, D-91058 Erlangen, Germany

[25] Univ Geneva, Dept Phys Nucl & Corpusculaire, CH-1211 Geneva, Switzerland

[26] Univ Ghent, Dept Phys & Astron, B-9000 Ghent, Belgium

[27] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[28] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA

[29] Univ Wisconsin, Dept Astron, Madison, WI 53706 USA

[30] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA

[31] Univ Wisconsin, Wisconsin IceCube Particle Astrophys Ctr, Madison, WI 53706 USA

[32] Johannes Gutenberg Univ Mainz, Inst Phys, D-55099 Mainz, Germany

[33] Univ Mons, B-7000 Mons, Belgium

[34] Tech Univ Munich, D-85748 Garching, Germany

[35] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA

[36] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA

[37] Univ Oxford, Dept Phys, Oxford OX1 3NP, England

[38] South Dakota Sch Mines & Technol, Dept Phys, Rapid City, SD 57701 USA

[39] Univ Wisconsin, Dept Phys, River Falls, WI 54022 USA

[40] Stockholm Univ, Oskar Klein Ctr, SE-10691 Stockholm, Sweden

[41] Stockholm Univ, Dept Phys, SE-10691 Stockholm, Sweden

[42] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA

[43] Sungkyunkwan Univ, Dept Phys, Suwon 440746, South Korea

[44] Univ Toronto, Dept Phys, Toronto, ON M5S 1A7, Canada

[45] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA

[46] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA

[47] Penn State Univ, Dept Phys, University Pk, PA 16802 USA

[48] Uppsala Univ, Dept Phys & Astron, S-75120 Uppsala, Sweden

[49] Univ Wuppertal, Dept Phys, D-42119 Wuppertal, Germany

[50] DESY, D-15735 Zeuthen, Germany

来源：

PHYSICAL REVIEW D | 2014年 / 90卷 / 10期

基金：

瑞典研究理事会; 美国国家科学基金会; 澳大利亚研究理事会; 新加坡国家研究基金会; 加拿大自然科学与工程研究理事会; 匈牙利科学研究基金会; 美国国家航空航天局; 英国科学技术设施理事会; 瑞士国家科学基金会;

关键词：

GAMMA-RAY BURSTS; MAGNETIZED NEUTRON-STARS; CORE-COLLAPSE; ASTROPHYSICAL SOURCES; INSTABILITIES; ACCELERATION; SENSITIVITY; TRANSIENTS; MECHANISM; EMISSION;

D O I：

10.1103/PhysRevD.90.102002

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube's observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of gravitational-wave emission energy of 10(-2) M(circle dot)c(2) at similar to 150 Hz with similar to 60 ms duration, and high-energy neutrino emission of 1051 erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6 x 10(-2) Mpc(-3) yr(-1). We also examine how combining information from gravitational waves and neutrinos will aid discovery in the advanced gravitational-wave detector era.

引用

页数：22

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