Gravitational radiation in d>4 from effective field theory

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dc.creatorCardoso, Vitor
dc.creatorDias, Oscar J. C.
dc.creatorFigueras, Pau
dc.date2008-07-14
dc.date2008-07-23
dc.date.accessioned2026-07-07T12:15:00Z
dc.date.available2026-07-07T12:15:00Z
dc.descriptionSome years ago, a new powerful technique, known as the Classical Effective Field Theory, was proposed to describe classical phenomena in gravitational systems. Here we show how this approach can be useful to investigate theoretically important issues, such as gravitational radiation in any spacetime dimension. In particular, we derive for the first time the Einstein-Infeld-Hoffman Lagrangian and we compute Einstein's quadrupole formula for any number of flat spacetime dimensions.
dc.description32 pages, 10 figures. v2: Factor in eq. (3.11) fixed. References added
dc.identifierhttps://arxiv.org/abs/0807.2261
dc.identifierhttp://arxiv.org/abs/0807.2261
dc.identifierPhys.Rev.D78:105010,2008
dc.identifierdoi:10.1103/PhysRevD.78.105010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211387
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational radiation in d>4 from effective field theory
dc.typetext

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