Optically targeted search for gravitational waves emitted by core-collapse supernovae during the first and second observing runs of advanced LIGO and advanced Virgo

verfasst von: The LIGO Scientific Collaboration , Virgo Collaboration , B. P. Abbott, R. Abbott, T. D. Abbott, S. Abraham, F. Acernese, K. Ackley, C. Adams, V. B. Adya, C. Affeldt, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, G. Allen, A. Allocca, M. A. Aloy, P. A. Altin, A. Amato, S. Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, S. V. Angelova, S. Antier, S. Appert, K. Arai, M. C. Araya, J. S. Areeda, M. Arène, N. Arnaud, S. M. Aronson, S. Ascenzi, G. Ashton, S. M. Aston, P. Astone, F. Aubin, P. Aufmuth, S. L. Danilishin, K. Danzmann, M. Heurs, H. Lück, D. Steinmeyer, H. Vahlbruch, L.-w. Wei, D. M. Wilken, B. Willke, H. Wittel, Sukanta Bose, D. D. Brown, Y. B. Chen, Hai-Ping Cheng, J. Gniesmer, Manuela Hanke, J. Hennig, M. T. Hübner, R. N. Lang, C. H. Lee, H. K. Lee, H. W. Lee, J. Lee, K. Lee, X. Li, C. A. Rose, D. Rose, J. R. Sanders, Patricia Schmidt, L. Sun, Y. F. Wang, D. S. Wu, L. Zhang, Minchuan Zhou, X. J. Zhu, G. Bergmann, Aparna Bisht, Nina Bode, P. Booker, Marc Brinkmann, M. Cabero, O. de Varona, S. Hochheim, J. Junker, Stefan Kaufer, S. Khan, R. Kirchhoff, Patrick Koch, N. Koper, S. M. Köhlenbeck, Volker Kringel, C. Krämer, G. Kuehn, S. Leavey, J. Lehmann, James Lough, Moritz Mehmet, Fabian Meylahn, Nikhil Mukund, A. Rüdiger, M. Phelps, F. Ohme, P. Oppermann, B. W. Schulte, Emil Schreiber, M. Nery, Y. Setyawati, M. Standke, M. Steinke, Michael Weinert, F. Wellmann, Peter Weßels, W. Winkler, J. Woehler, Mukherjee Arunava Mukherjee
Abstract: 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 4.27×10-4 M·c2 and 1.28×10-1 M·c2 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.
Organisationseinheit(en): QUEST Leibniz Forschungsschule
Institut für Gravitationsphysik
QuantumFrontiers
Externe Organisation(en): Australian National University
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
Washington State University Pullman
University of Adelaide
University of Florida (UF)
Universität Hamburg
Monash University
LIGO Laboratory
Inje University
Stanford University
California Institute of Technology (Caltech)
California State University Fullerton
The California State University
Radboud Universität Nijmegen (RU)
University of Melbourne
University of Texas Rio Grande Valley
Northwestern University
Typ: Artikel
Journal: Physical Review D
Band: 101
Anzahl der Seiten: 24
ISSN: 2470-0010
Publikationsdatum: 02.04.2020
Publikationsstatus: Veröffentlicht
Peer-reviewed: Ja
ASJC Scopus Sachgebiete: Physik und Astronomie (sonstige)
Elektronische Version(en): https://arxiv.org/abs/1908.03584 (Zugang: Offen)
https://doi.org/10.1103/PhysRevD.101.084002 (Zugang: Geschlossen)
https://doi.org/10.15488/12069 (Zugang: Offen)
: Details im Forschungsportal „Research@Leibniz University“

BibTeX

@article{bf4d79ada9414ee692cc266bb58ea24c,
title = "Optically targeted search for gravitational waves emitted by core-collapse supernovae during the first and second observing runs of advanced LIGO and advanced Virgo",
abstract = "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 4.27×10-4 M·c2 and 1.28×10-1 M·c2 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.",
author = "{The LIGO Scientific Collaboration} and {The Virgo Collaboration} and B. P. Abbott and R. Abbott and T. D. Abbott and S. Abraham and F. Acernese and K. Ackley and C. Adams and V. B. Adya and C. Affeldt and M. Agathos and K. Agatsuma and N. Aggarwal and O. D. Aguiar and L. Aiello and A. Ain and P. Ajith and G. Allen and A. Allocca and M. A. Aloy and P. A. Altin and A. Amato and S. Anand and A. Ananyeva and S. B. Anderson and W. G. Anderson and S. V. Angelova and S. Antier and S. Appert and K. Arai and M. C. Araya and J. S. Areeda and M. Ar{\`e}ne and N. Arnaud and S. M. Aronson and S. Ascenzi and G. Ashton and S. M. Aston and P. Astone and F. Aubin and P. Aufmuth and S. L. Danilishin and K. Danzmann and M. Heurs and H. L{\"u}ck and D. Steinmeyer and H. Vahlbruch and L.-w. Wei and D. M. Wilken and B. Willke and H. Wittel and Sukanta Bose and Brown, {D. D.} and Chen, {Y. B.} and Hai-Ping Cheng and J. Gniesmer and Manuela Hanke and J. Hennig and H{\"u}bner, {M. T.} and Lang, {R. N.} and Lee, {C. H.} and Lee, {H. K.} and Lee, {H. W.} and J. Lee and K. Lee and X. Li and Rose, {C. A.} and D. Rose and Sanders, {J. R.} and Patricia Schmidt and L. Sun and Wang, {Y. F.} and Wu, {D. S.} and L. Zhang and Minchuan Zhou and Zhu, {X. J.} and G. Bergmann and Aparna Bisht and Nina Bode and P. Booker and Marc Brinkmann and M. Cabero and {de Varona}, O. and S. Hochheim and J. Junker and Stefan Kaufer and S. Khan and R. Kirchhoff and Patrick Koch and N. Koper and K{\"o}hlenbeck, {S. M.} and Volker Kringel and C. Kr{\"a}mer and G. Kuehn and S. Leavey and J. Lehmann and James Lough and Moritz Mehmet and Fabian Meylahn and Nikhil Mukund and A. R{\"u}diger and M. Phelps and F. Ohme and P. Oppermann and Schulte, {B. W.} and Emil Schreiber and M. Nery and Y. Setyawati and M. Standke and M. Steinke and Michael Weinert and F. Wellmann and Peter We{\ss}els and W. Winkler and J. Woehler and {Arunava Mukherjee}, Mukherjee",
note = "Funding Information: The authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS), and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research for the construction and operation of the Virgo detector and the creation and support of the European Gravitational Observatory consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India; the Department of Science and Technology, India; the Science & Engineering Research Board, India; the Ministry of Human Resource Development, India; the Spanish Agencia Estatal de Investigaci{\'o}n; the Vicepresid{\`e}ncia i Conselleria d{\textquoteright}Innovaci{\'o}; Recerca i Turisme and the Conselleria d{\textquoteright}Educaci{\'o} i Universitat del Govern de les Illes Balears; the Conselleria d{\textquoteright}Educaci{\'o}, Investigaci{\'o}, Cultura i Esport de la Generalitat Valenciana; the National Science Centre of Poland; the Swiss National Science Foundation; the Russian Foundation for Basic Research; the Russian Science Foundation; the European Commission; the European Regional Development Funds; the Royal Society; the Scottish Funding Council; the Scottish Universities Physics Alliance; the Hungarian Scientific Research Fund; the Lyon Institute of Origins; the Paris {\^I}le-de-France Region; the National Research, Development and Innovation Office Hungary; the National Research Foundation of Korea; Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation; the Natural Science and Engineering Research Council Canada; the Canadian Institute for Advanced Research; the Brazilian Ministry of Science, Technology, Innovations, and Communications; the International Center for Theoretical Physics South American Institute for Fundamental Research; the Research Grants Council of Hong Kong; the National Natural Science Foundation of China; the Leverhulme Trust; the Research Corporation; the Ministry of Science and Technology, Taiwan; and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, INFN and CNRS for provision of computational resources. Research by D. J. S. is supported by NSF Grants No. AST-1821987, No. AST-1821967, No. AST-1813708, and No. AST-1813466. We thank the Las Cumbres Observatory and its staff for its continuing support of the ASAS-SN project. ASAS-SN is supported by the Gordon and Betty Moore Foundation through Grant No. GBMF5490 to the Ohio State University and NSF Grant No. AST-1515927. Development of ASAS-SN has been supported by NSF Grant No. AST-0908816, the Mt. Cuba Astronomical Foundation, the Center for Cosmology and AstroParticle Physics at the Ohio State University, the Chinese Academy of Sciences South America Center for Astronomy, the Villum Foundation, and George Skestos. K. Z. S. and C. S. K. are supported by NSF Grants No. AST-1515876, No. AST-1515927, and No. AST-1814440. Support for J. L. P. is provided in part by FONDECYT through Grant No. 1191038 and by the Ministry of Economy, Development, and Tourism{\textquoteright}s Millennium Science Initiative through Grant No. IC120009, awarded to The Millennium Institute of Astrophysics, MAS. Research by S. V. is supported by NSF Grant No. AST-1813176. We are thankful to the National Science Foundation for support under Grant No. PHY 1806165. This document has been assigned LIGO Laboratory document number LIGO-P1700177. ",
year = "2020",
month = apr,
day = "2",
doi = "10.1103/PhysRevD.101.084002",
language = "English",
volume = "101",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "8",
}

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