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Properties of the Binary Neutron Star Merger GW170817

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autorschaft

  • The LIGO Scientific Collaboration
  • Virgo Collaboration
  • Vaishali Adya
  • Christoph Affeldt
  • Bruce Allen
  • Shtefan Danilishin
  • Karsten Danzmann
  • Michele Heurs
  • Harald Lück
  • Daniel Steinmeyer
  • Henning Fedor Cornelius Vahlbruch
  • Li-Wei Wei
  • Dennis Max Wilken
  • Benno Willke
  • Holger Wittel
  • A. Hreibi
  • J. Junker
  • M. A. Papa
  • B. W. Schulte
  • M. Steinke

Externe Organisationen

  • California Institute of Technology (Caltech)
  • Louisiana State University
  • Universita di Salerno
  • Università degli Studi di Napoli Federico II
  • Monash University
  • Université Grenoble Alpes (UGA)
  • University of Sannio
  • Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
  • University of Illinois Urbana-Champaign (UIUC)
  • University of Cambridge
  • LIGO Laboratory
  • Instituto Nacional de Pesquisas Espaciais
  • Gran Sasso Science Institute
  • Tata Institute of Fundamental Research (TIFR HYD)
  • University of Wisconsin Milwaukee
  • Inje University
  • Australian National University
  • Radboud Universität Nijmegen (RU)
  • The Chinese University of Hong Kong
  • Northwestern University
  • Nationaal instituut voor subatomaire fysica (Nikhef)
  • University of Adelaide
  • University of Florida (UF)
  • Inter-University Centre for Astronomy and Astrophysics India
  • University of Glasgow
  • Washington State University Pullman
  • University of Melbourne
  • Observatoire de la Côte d’Azur (OCA)
  • Istituto Nazionale di Fisica Nucleare (INFN)

Details

OriginalspracheEnglisch
Aufsatznummer011001
Seitenumfang32
FachzeitschriftPhysical Review X
Jahrgang9
Ausgabenummer1
PublikationsstatusVeröffentlicht - 2 Jan. 2019

ASJC Scopus Sachgebiete

Zitieren

Properties of the Binary Neutron Star Merger GW170817. / The LIGO Scientific Collaboration; Virgo Collaboration; Adya, Vaishali et al.
in: Physical Review X, Jahrgang 9, Nr. 1, 011001, 02.01.2019.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

The LIGO Scientific Collaboration, Virgo Collaboration, Adya, V, Affeldt, C, Allen, B, Danilishin, S, Danzmann, K, Heurs, M, Lück, H, Steinmeyer, D, Vahlbruch, HFC, Wei, L-W, Wilken, DM, Willke, B, Wittel, H, Zhang, L, Zhang, Y, Brown, DD, Chen, Y, Cheng, HP, Hennig, J, Hreibi, A, Aufmuth, P, Bergmann, G, Bensch, M, Bisht, A, Bode, N, Booker, P, Brinkmann, M, Denker, T, de Varona, O, Doravari, S, Dreissigacker, C, Eggenstein, H-B, Hanke, M, Hochheim, S, Junker, J, Karvinen, KS, Kaufer, S, Khan, S, Kirchhoff, R, Koch, P, Koper, N, Kringel, V, Kuehn, G, Leavey, S, Lehmann, J, Lough, J, Mehmet, M, Mukherjee, A, Mukund, N, Nery, M, Ohme, F, Oppermann, P, Ming, J, Papa, MA, Puncken, O, Rüdiger, A, Schreiber, E, Schulte, BW, Schütte, D, Steinke, M, Steltner, B, Theeg, T, Thies, F, Weinert, M, Wimmer, MH, Winkler, W, Woehler, J, Zhu, SJ, Bose, S, Sun, L, Köhlenbeck, SM, Leonardi, M, Mendoza-Gandara, D, Singh, A, Wellmann, F, Weßels, P & Wu, DS 2019, 'Properties of the Binary Neutron Star Merger GW170817', Physical Review X, Jg. 9, Nr. 1, 011001. https://doi.org/10.1103/PhysRevX.9.011001, https://doi.org/10.15488/11396
The LIGO Scientific Collaboration, Virgo Collaboration, Adya, V., Affeldt, C., Allen, B., Danilishin, S., Danzmann, K., Heurs, M., Lück, H., Steinmeyer, D., Vahlbruch, H. F. C., Wei, L.-W., Wilken, D. M., Willke, B., Wittel, H., Zhang, L., Zhang, Y., Brown, D. D., Chen, Y., ... Wu, D. S. (2019). Properties of the Binary Neutron Star Merger GW170817. Physical Review X, 9(1), Artikel 011001. https://doi.org/10.1103/PhysRevX.9.011001, https://doi.org/10.15488/11396
The LIGO Scientific Collaboration, Virgo Collaboration, Adya V, Affeldt C, Allen B, Danilishin S et al. Properties of the Binary Neutron Star Merger GW170817. Physical Review X. 2019 Jan 2;9(1):011001. doi: 10.1103/PhysRevX.9.011001, 10.15488/11396
The LIGO Scientific Collaboration ; Virgo Collaboration ; Adya, Vaishali et al. / Properties of the Binary Neutron Star Merger GW170817. in: Physical Review X. 2019 ; Jahrgang 9, Nr. 1.
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@article{d6a8d9157e0d43d5b568cd1c08c7d51d,
title = "Properties of the Binary Neutron Star Merger GW170817",
author = "{The LIGO Scientific Collaboration} and {The Virgo Collaboration} and Abbott, {Benjamin P.} and Richard Abbott and Abbott, {T. D.} and Fausto Acernese and Kendall Ackley and C. Adams and T. Adams and P. Addesso and Adhikari, {Rana X.} and Vaishali Adya and Christoph Affeldt and Bhanu Agarwal and Michalis Agathos and Kazuhiro Agatsuma and Nikhil Aggarwal and Aguiar, {Odylio Denys} and Lorenzo Aiello and A. Ain and Parameswaran Ajith and Bruce Allen and Gabrielle Allen and Shtefan Danilishin and Karsten Danzmann and Michele Heurs and Sanjeev Kumar and Lee, {H. K.} and X. Li and Harald L{\"u}ck and Nguyen, {Truc T.} and Patricia Schmidt and Daniel Steinmeyer and Vahlbruch, {Henning Fedor Cornelius} and Wang, {Y. F.} and Li-Wei Wei and Wilken, {Dennis Max} and Benno Willke and Holger Wittel and L. Zhang and Yin Zhang and Minchuan Zhou and Brown, {D. D.} and Yalu Chen and Cheng, {H. P.} and J. Hennig and A. Hreibi and Peter Aufmuth and Gerald Bergmann and Maximilian Bensch and Aparna Bisht and Nina Bode and P. Booker and Marc Brinkmann and Timo Denker and {de Varona}, O. and S. Doravari and C. Dreissigacker and H.-B. Eggenstein and Manuela Hanke and S. Hochheim and J. Junker and Karvinen, {Kai S.} and Stefan Kaufer and S. Khan and R. Kirchhoff and Patrick Koch and N. Koper and Volker Kringel and G. Kuehn and S. Leavey and J. Lehmann and James Lough and Moritz Mehmet and Arunava Mukherjee and Nikhil Mukund and M. Nery and F. Ohme and P. Oppermann and J. Ming and Papa, {M. A.} and O. Puncken and A. R{\"u}diger and Emil Schreiber and Schulte, {B. W.} and Dirk Sch{\"u}tte and M. Steinke and B. Steltner and Thomas Theeg and Fabian Thies and Michael Weinert and Wimmer, {Maximilian H.} and W. Winkler and J. Woehler and Zhu, {S. J.} and Sukanta Bose and L. Sun and K{\"o}hlenbeck, {S. M.} and M. Leonardi and D. Mendoza-Gandara and Avneet Singh and F. Wellmann and Peter We{\ss}els and Wu, {D. S.}",
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 (MPS), 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 EGO 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 (SERB), 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 (SNSF); the Russian Foundation for Basic Research; the Russian Science Foundation; the European Commission; the European Regional Development Funds (ERDF); the Royal Society; the Scottish Funding Council; the Scottish Universities Physics Alliance; the Hungarian Scientific Research Fund (OTKA); the Lyon Institute of Origins (LIO); the Paris {\^I}le-de-France Region; the National Research, Development and Innovation Office Hungary (NKFI); 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 (ICTP-SAIFR); the Research Grants Council of Hong Kong; the National Natural Science Foundation of China (NSFC); the Leverhulme Trust; the Research Corporation; the Ministry of Science and Technology (MOST), Taiwan; and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, Max-Planck-Society (MPS), INFN, CNRS, and the State of Niedersachsen/Germany for provision of computational resources. The GW strain data for this event are available at the LIGO Open Science Center . This article has been assigned the document number LIGO-P1800061.",
year = "2019",
month = jan,
day = "2",
doi = "10.1103/PhysRevX.9.011001",
language = "English",
volume = "9",
journal = "Physical Review X",
issn = "2160-3308",
publisher = "American Physical Society",
number = "1",

}

Download

TY - JOUR

T1 - Properties of the Binary Neutron Star Merger GW170817

AU - The LIGO Scientific Collaboration

AU - The Virgo Collaboration

AU - Abbott, Benjamin P.

AU - Abbott, Richard

AU - Abbott, T. D.

AU - Acernese, Fausto

AU - Ackley, Kendall

AU - Adams, C.

AU - Adams, T.

AU - Addesso, P.

AU - Adhikari, Rana X.

AU - Adya, Vaishali

AU - Affeldt, Christoph

AU - Agarwal, Bhanu

AU - Agathos, Michalis

AU - Agatsuma, Kazuhiro

AU - Aggarwal, Nikhil

AU - Aguiar, Odylio Denys

AU - Aiello, Lorenzo

AU - Ain, A.

AU - Ajith, Parameswaran

AU - Allen, Bruce

AU - Allen, Gabrielle

AU - Danilishin, Shtefan

AU - Danzmann, Karsten

AU - Heurs, Michele

AU - Kumar, Sanjeev

AU - Lee, H. K.

AU - Li, X.

AU - Lück, Harald

AU - Nguyen, Truc T.

AU - Schmidt, Patricia

AU - Steinmeyer, Daniel

AU - Vahlbruch, Henning Fedor Cornelius

AU - Wang, Y. F.

AU - Wei, Li-Wei

AU - Wilken, Dennis Max

AU - Willke, Benno

AU - Wittel, Holger

AU - Zhang, L.

AU - Zhang, Yin

AU - Zhou, Minchuan

AU - Brown, D. D.

AU - Chen, Yalu

AU - Cheng, H. P.

AU - Hennig, J.

AU - Hreibi, A.

AU - Aufmuth, Peter

AU - Bergmann, Gerald

AU - Bensch, Maximilian

AU - Bisht, Aparna

AU - Bode, Nina

AU - Booker, P.

AU - Brinkmann, Marc

AU - Denker, Timo

AU - de Varona, O.

AU - Doravari, S.

AU - Dreissigacker, C.

AU - Eggenstein, H.-B.

AU - Hanke, Manuela

AU - Hochheim, S.

AU - Junker, J.

AU - Karvinen, Kai S.

AU - Kaufer, Stefan

AU - Khan, S.

AU - Kirchhoff, R.

AU - Koch, Patrick

AU - Koper, N.

AU - Kringel, Volker

AU - Kuehn, G.

AU - Leavey, S.

AU - Lehmann, J.

AU - Lough, James

AU - Mehmet, Moritz

AU - Mukherjee, Arunava

AU - Mukund, Nikhil

AU - Nery, M.

AU - Ohme, F.

AU - Oppermann, P.

AU - Ming, J.

AU - Papa, M. A.

AU - Puncken, O.

AU - Rüdiger, A.

AU - Schreiber, Emil

AU - Schulte, B. W.

AU - Schütte, Dirk

AU - Steinke, M.

AU - Steltner, B.

AU - Theeg, Thomas

AU - Thies, Fabian

AU - Weinert, Michael

AU - Wimmer, Maximilian H.

AU - Winkler, W.

AU - Woehler, J.

AU - Zhu, S. J.

AU - Bose, Sukanta

AU - Sun, L.

AU - Köhlenbeck, S. M.

AU - Leonardi, M.

AU - Mendoza-Gandara, D.

AU - Singh, Avneet

AU - Wellmann, F.

AU - Weßels, Peter

AU - Wu, D. S.

N1 - 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 (MPS), 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 EGO 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 (SERB), India; the Ministry of Human Resource Development, India; the Spanish Agencia Estatal de Investigación; the Vicepresidència i Conselleria d’Innovació; Recerca i Turisme and the Conselleria d’Educació i Universitat del Govern de les Illes Balears; the Conselleria d’Educació, Investigació, Cultura i Esport de la Generalitat Valenciana; the National Science Centre of Poland; the Swiss National Science Foundation (SNSF); the Russian Foundation for Basic Research; the Russian Science Foundation; the European Commission; the European Regional Development Funds (ERDF); the Royal Society; the Scottish Funding Council; the Scottish Universities Physics Alliance; the Hungarian Scientific Research Fund (OTKA); the Lyon Institute of Origins (LIO); the Paris Île-de-France Region; the National Research, Development and Innovation Office Hungary (NKFI); 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 (ICTP-SAIFR); the Research Grants Council of Hong Kong; the National Natural Science Foundation of China (NSFC); the Leverhulme Trust; the Research Corporation; the Ministry of Science and Technology (MOST), Taiwan; and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, Max-Planck-Society (MPS), INFN, CNRS, and the State of Niedersachsen/Germany for provision of computational resources. The GW strain data for this event are available at the LIGO Open Science Center . This article has been assigned the document number LIGO-P1800061.

PY - 2019/1/2

Y1 - 2019/1/2

UR - http://www.scopus.com/inward/record.url?scp=85061618892&partnerID=8YFLogxK

U2 - 10.1103/PhysRevX.9.011001

DO - 10.1103/PhysRevX.9.011001

M3 - Article

AN - SCOPUS:85061618892

VL - 9

JO - Physical Review X

JF - Physical Review X

SN - 2160-3308

IS - 1

M1 - 011001

ER -

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