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We consider the recently introduced ``Galileon'' field in a dynamical spacetime. When the Galileon is assumed to be minimally coupled to the metric, we underline that both field equations of the Galileon and the metric involve up to third-order derivatives. We show that a unique nonminimal coupling of the Galileon to curvature eliminates all higher derivatives in all field equations, hence yielding second-order equations, without any extra propagating degree of freedom. The resulting theory breaks the generalized ``Galilean'' invariance of the original model.
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Cédric Deffayet
Centre National de la Recherche Scientifique
Gilles Esposito-Farèse
Institut d'Astrophysique de Paris
Alexander Vikman
Centre National de la Recherche Scientifique
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology
Centre National de la Recherche Scientifique
New York University
Université Paris Cité
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Deffayet et al. (Fri,) studied this question.
synapsesocial.com/papers/6a1bf87c0a1f7575939d47d4 — DOI: https://doi.org/10.1103/physrevd.79.084003
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