Testing general relativity with present and future astrophysical observations

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dc.contributor.authorBerti, Emanuele
dc.contributor.authorBarausse, Enrico
dc.contributor.authorCardoso, Vitor
dc.contributor.authorGualtieri, Leonardo
dc.contributor.authorPani, Paolo
dc.contributor.authorSperhake, Ulrich
dc.contributor.authorStein, Leo C.
dc.contributor.authorWex, Norbert
dc.contributor.authorYagi, Kent
dc.contributor.authorBaker, Tessa
dc.contributor.authorBurgess, C. P.
dc.contributor.authorCoelho, Flávio S.
dc.contributor.authorDoneva, Daniela
dc.contributor.authorDe Felice, Antonio
dc.contributor.authorFerreira, Pedro G.
dc.contributor.authorFreire, Paulo C.C.
dc.contributor.authorHealy, James
dc.contributor.authorHerdeiro, Carlos
dc.contributor.authorHorbatsch, Michael
dc.contributor.authorKleihaus, Burkhard
dc.contributor.authorKlein, Antoine
dc.contributor.authorKokkotas, Kostas
dc.contributor.authorKunz, Jutta
dc.contributor.authorLaguna, Pablo
dc.contributor.authorLang, Ryan N.
dc.contributor.authorLi, Tjonnie G.F.
dc.contributor.authorLittenberg, Tyson
dc.contributor.authorMatas, Andrew
dc.contributor.authorMirshekari, Saeed [UNESP]
dc.contributor.authorOkawa, Hirotada
dc.contributor.authorRadu, Eugen
dc.contributor.authorO'Shaughnessy, Richard
dc.contributor.authorSathyaprakash, Bangalore S.
dc.contributor.authorVan Den Broeck, Chris
dc.contributor.authorWinther, Hans A.
dc.contributor.authorWitek, Helvi
dc.contributor.authorAghili, Mir Emad
dc.contributor.authorAlsing, Justin
dc.contributor.authorBolen, Brett
dc.contributor.authorBombelli, Luca
dc.contributor.authorCaudill, Sarah
dc.contributor.authorChen, Liang
dc.contributor.authorDegollado, Juan Carlos
dc.contributor.authorFujita, Ryuichi
dc.contributor.authorGao, Caixia
dc.contributor.authorGerosa, Davide
dc.contributor.authorKamali, Saeed
dc.contributor.authorSilva, Hector O.
dc.contributor.authorRosa, João G.
dc.contributor.authorSadeghian, Laleh
dc.contributor.authorSampaio, Marco
dc.contributor.authorSotani, Hajime
dc.contributor.authorZilhao, Miguel
dc.contributor.institutionUniversity of Mississippi
dc.contributor.institutionUniversidade de Lisboa
dc.contributor.institutionInstitut d'Astrophysique de Paris
dc.contributor.institutionUMR 7095
dc.contributor.institutionPerimeter Institute for Theoretical Physics
dc.contributor.institutionSezione INFN Roma 1
dc.contributor.institutionUniversity of Cambridge
dc.contributor.institutionCalifornia Institute of Technology
dc.contributor.institutionCornell University
dc.contributor.institutionMax-Planck-Institut für Radioastronomie
dc.contributor.institutionPrinceton University
dc.contributor.institutionMontana State University
dc.contributor.institutionDWB
dc.contributor.institutionMcMaster University
dc.contributor.institutionCIDMA Campus de Santiago
dc.contributor.institutionEberhard Karls University of Tübingen
dc.contributor.institutionNaresuan University
dc.contributor.institutionMinistry of Education
dc.contributor.institutionRochester Institute of Technology
dc.contributor.institutionUniversität Oldenburg
dc.contributor.institutionGeorgia Institute of Technology
dc.contributor.institutionUniversity of Wisconsin-Milwaukee
dc.contributor.institutionUniversity of Florida
dc.contributor.institutionUniversity of Illinois at Urbana-Champaign
dc.contributor.institutionChinese University of Hong Kong
dc.contributor.institutionLIGO-California Institute of Technology
dc.contributor.institutionNorthwestern University
dc.contributor.institutionCase Western Reserve University
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionCardiff University
dc.contributor.institutionScience Park
dc.contributor.institutionImperial College London
dc.contributor.institutionGrand Valley State University
dc.contributor.institutionKyoto University
dc.date.accessioned2018-12-11T16:58:54Z
dc.date.available2018-12-11T16:58:54Z
dc.date.issued2015-12-01
dc.description.abstractOne century after its formulation, Einstein's general relativity (GR) has made remarkable predictions and turned out to be compatible with all experimental tests. Most of these tests probe the theory in the weak-field regime, and there are theoretical and experimental reasons to believe that GR should be modified when gravitational fields are strong and spacetime curvature is large. The best astrophysical laboratories to probe strong-field gravity are black holes and neutron stars, whether isolated or in binary systems. We review the motivations to consider extensions of GR. We present a (necessarily incomplete) catalog of modified theories of gravity for which strong-field predictions have been computed and contrasted to Einstein's theory, and we summarize our current understanding of the structure and dynamics of compact objects in these theories. We discuss current bounds on modified gravity from binary pulsar and cosmological observations, and we highlight the potential of future gravitational wave measurements to inform us on the behavior of gravity in the strong-field regime.en
dc.description.affiliationDepartment of Physics and Astronomy University of Mississippi
dc.description.affiliationCENTRA Departamento de Física Instituto Superior Técnico Universidade de Lisboa, Avenida Rovisco Pais 1
dc.description.affiliationCNRS UMR 7095 Institut d'Astrophysique de Paris, 98bis Bd Arago
dc.description.affiliationSorbonne Universités UPMC Univ Paris 06 UMR 7095, 98bis Bd Arago
dc.description.affiliationPerimeter Institute for Theoretical Physics
dc.description.affiliationDipartimento di Fisica Sapienza Università di Roma Sezione INFN Roma 1, P.le A. Moro 2
dc.description.affiliationDepartment of Applied Mathematics and Theoretical Physics Centre for Mathematical Sciences University of Cambridge, Wilberforce Road
dc.description.affiliationTheoretical Astrophysics 350-17 California Institute of Technology
dc.description.affiliationCornell Center for Astrophysics and Planetary Science Cornell University
dc.description.affiliationMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69
dc.description.affiliationDepartment of Physics Princeton University
dc.description.affiliationDepartment of Physics Montana State University
dc.description.affiliationAstrophysics University of Oxford DWB, Keble Road
dc.description.affiliationDepartment of Physics and Astronomy McMaster University
dc.description.affiliationDepartamento de Física Universidade de Aveiro CIDMA Campus de Santiago
dc.description.affiliationTheoretical Astrophysics Eberhard Karls University of Tübingen
dc.description.affiliationThEP's CRL NEP Institute for Fundamental Study Naresuan University
dc.description.affiliationThailand Center of Excellence in Physics Ministry of Education
dc.description.affiliationCenter for Computational Relativity and Gravitation School of Mathematical Sciences Rochester Institute of Technology, 85 Lomb Memorial Drive
dc.description.affiliationInstitut für Physik Universität Oldenburg
dc.description.affiliationCenter for Relativistic Astrophysics and School of Physics Georgia Institute of Technology
dc.description.affiliationLeonard e Parker Center for Gravitation Cosmology and Astrophysics University of Wisconsin-Milwaukee
dc.description.affiliationDepartment of Physics University of Florida
dc.description.affiliationDepartment of Physics University of Illinois at Urbana-Champaign
dc.description.affiliationDepartment of Physics Chinese University of Hong Kong
dc.description.affiliationLIGO-California Institute of Technology
dc.description.affiliationCenter for Interdisciplinary Exploration and Research in Astrophysics (CIERA) Dept. of Physics and Astronomy Northwestern University, 2145 Sheridan Rd.
dc.description.affiliationCERCA/Department of Physics Case Western Reserve University, 10900 Euclid Ave
dc.description.affiliationICTP South American Institute for Fundamental Research Instituto de Física Teórica UNESP-Universidade Estadual Paulista, Rua Dr. Bento T. Ferraz 271
dc.description.affiliationSchool of Physics and Astronomy Cardiff University, 5, The Parade
dc.description.affiliationNikhef Science Park
dc.description.affiliationImperial Centre for Inference and Cosmology Imperial College London, Prince Consort Road
dc.description.affiliationDepartment of Physics Grand Valley State University
dc.description.affiliationYukawa Institute for Theoretical Physics Kyoto University
dc.description.affiliationUnespICTP South American Institute for Fundamental Research Instituto de Física Teórica UNESP-Universidade Estadual Paulista, Rua Dr. Bento T. Ferraz 271
dc.identifierhttp://dx.doi.org/10.1088/0264-9381/32/24/243001
dc.identifier.citationClassical and Quantum Gravity, v. 32, n. 24, 2015.
dc.identifier.doi10.1088/0264-9381/32/24/243001
dc.identifier.file2-s2.0-84944745333.pdf
dc.identifier.issn1361-6382
dc.identifier.issn0264-9381
dc.identifier.scopus2-s2.0-84944745333
dc.identifier.urihttp://hdl.handle.net/11449/172143
dc.language.isoeng
dc.relation.ispartofClassical and Quantum Gravity
dc.relation.ispartofsjr1,809
dc.rights.accessRightsAcesso aberto
dc.sourceScopus
dc.subjectblack holes
dc.subjectcompact binaries
dc.subjectgeneral relativity
dc.subjectgravitational waves
dc.subjectneutron stars
dc.titleTesting general relativity with present and future astrophysical observationsen
dc.typeResenha

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