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Phys. Rev. D 79, 084003 (2009) [6 pages]

Covariant Galileon

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C. Deffayet*
AstroParticule & Cosmologie, UMR 7164-CNRS, Université Denis Diderot-Paris 7, CEA, Observatoire de Paris, 10 rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France

G. Esposito-Farèse
GReCO, Institut d’Astrophysique de Paris, UMR 7095-CNRS, Université Pierre et Marie Curie-Paris 6, 98bis boulevard Arago, F-75014 Paris, France

A. Vikman
CCPP, New York University, Meyer Hall of Physics, 4 Washington Place, New York, New York 10003, USA

Received 14 January 2009; published 3 April 2009

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.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.79.084003
DOI:
10.1103/PhysRevD.79.084003
PACS:
04.50.−h, 11.10.−z, 98.80.−k

*deffayet@iap.fr

gef@iap.fr

alexander.vikman@nyu.edu