Effective field theory methods to model compact binaries

dc.contributorUniv Geneva
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-12-03T13:11:23Z
dc.date.available2014-12-03T13:11:23Z
dc.date.created2014-12-03T13:11:23Z
dc.date.issued2014-02-01
dc.identifierClassical And Quantum Gravity. Bristol: Iop Publishing Ltd, v. 31, n. 4, 34 p., 2014.
dc.identifier0264-9381
dc.identifierhttp://hdl.handle.net/11449/113069
dc.identifier10.1088/0264-9381/31/4/043001
dc.identifierWOS:000331089800002
dc.description.abstractIn this short review we present a self-contained exposition of the effective field theory method approach to model the dynamics of gravitationally bound compact binary systems within the post-Newtonian approximation to General Relativity. Applications of this approach to the conservative sector, as well as to the radiation emission by the binary system are discussed in their salient features. Most important results are discussed, as in-depths and details can be found in the referenced papers.
dc.languageeng
dc.publisherIop Publishing Ltd
dc.relationClassical and Quantum Gravity
dc.relation3.283
dc.relation1,809
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectpost-Newtonian approximation to general relativity
dc.subjecteffective field theory
dc.subjectgravitational waves
dc.subjectgravitational 2-body problem
dc.titleEffective field theory methods to model compact binaries
dc.typeArtículos de revistas


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