Aartsen, M. G. and Aasi, J. and Abbott, B. P. and Abbott, R. and Abernathy, M. R. and Adhikari, R. X. and Anderson, R. A. and Anderson, S. B. and Arai, K. and Araya, M. and Barayoga, J. C. and Barish, B. C. and Billingsley, G. and Black, E. and Blackburn, J. K. and Bork, R. and Brooks, A. F. and Cepeda, C. and Chakraborty, R. and Chalermsongsak, T. and Coyne, D. C. and Dergachev, V. and Drever, R. W. P. and Driggers, J. C. and Ehrens, P. and Etzel, T. and Gushwa, K. and Gustafson, E. K. and Hall, E. D. and Harms, J. and Heptonstall, A. W. and Hodge, K. A. and Ivanov, A. and Jacobson, M. and Kalmus, P. and Kanner, J. B. and Kells, W. and King, P. J. and Kondrashov, V. and Korth, W. Z. and Kozak, D. B. and Lazzarini, A. and Lewis, J. and Li, T. G. F. and Libbrecht, K. and Mageswaran, M. and Mailand, K. and Maros, E. and Martynov, D. and Marx, J. N. and McIntyre, G. and Meshkov, S. and Osthelder, C. and Pedraza, M. and Phelps, M. and Price, L. R. and Privitera, S. and Quintero, E. and Raymond, V. and Reitze, D. H. and Robertson, N. A. and Rollins, J. G. and Sannibale, V. and Shao, Z. and Singer, A. and Singer, L. and Smith, M. R. and Smith, R. J. E. and Smith-Lefebvre, N. D. and Taylor, R. and Thirugnanasambandam, M. P. and Thrane, E. and Torrie, C. I. and Vass, S. and Wallace, L. and Weinstein, A. J. and Williams, R. and Yamamoto, H. and Zhang, L. and Zweizig, J. and Chen, Y. and Cutler, C. and Gossan, S. and Miao, H. and Nissanke, S. and Thorne, K. S. and Vallisneri, M. and Yang, H. (2014) Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube. Physical Review D, 90 (10). Art. No. 102002. ISSN 2470-0010. doi:10.1103/PhysRevD.90.102002. https://resolver.caltech.edu/CaltechAUTHORS:20150108-091905659
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Abstract
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_⊙c^2 at ∼150 Hz with ∼60 ms duration, and high-energy neutrino emission of 10^(51) erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6×10^(−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.
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| Additional Information: | © 2014 American Physical Society. Received 14 July 2014; published 17 November 2014. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Economía y Competitividad, the Conselleria d’Economia Hisenda i Innovació of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, Hungarian Scientific Research Fund, the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This article has LIGO document number LIGO-P1400046. We acknowledge the support from the following agencies: U.S. National Science Foundation- Office of Polar Programs, U.S. National Science Foundation-Physics Division, University of Wisconsin Alumni Research Foundation, the Grid Laboratory Of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin, Madison; the Open Science Grid (OSG) grid infrastructure; U.S. Department of Energy, and National Energy Research Scientific Computing Center, the Louisiana Optical Network Initiative (LONI) grid computing resources; Natural Sciences and Engineering Research Council of Canada, WestGrid and Compute/ Calcul Canada; Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Research Department of Plasmas with Complex Interactions (Bochum), Germany; Fund for Scientific Research (FNRS-FWO), FWO Odysseus programme, Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Science Policy Office (Belspo); University of Oxford, U.K.; Marsden Fund, New Zealand; Australian Research Council; Japan Society for Promotion of Science (JSPS); the Swiss National Science Foundation (SNSF), Switzerland; National Research Foundation of Korea (NRF); Danish National Research Foundation, Denmark (DNRF). | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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| DOI: | 10.1103/PhysRevD.90.102002 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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| Official Citation: | Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube M. G. Aartsen et al. (IceCube Collaboration), (LIGO Scientific Collaboration and the Virgo Collaboration) Phys. Rev. D 90, 102002 (2014) – Published 17 November 2014 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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| Deposited By: | Ruth Sustaita | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Deposited On: | 08 Jan 2015 20:05 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Last Modified: | 10 Nov 2021 20:00 |
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