Published September 15, 2010 | Version v1
Journal article

Arbitrary p-form Galileons

  • 1. GRECO, Institut d'Astrophysique de Paris, UMR 7095-CNRS, Universite Pierre et Marie Curie-Paris 6, 98bis boulevard Arago, F-75014 Paris (France)
  • 2. Physics Department, Brandeis University, Waltham Massachusetts 02454, USA, and Lauritsen Laboratory, California Institute of Technology, Pasadena California 91125 (United States)
  • 3. AstroParticule and Cosmologie, UMR 7164-CNRS, Universite Denis Diderot-Paris 7, CEA, Observatoire de Paris, 10 rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France, and Institut d'Astrophysique de Paris, UMR 7095-CNRS, 98bis boulevard Arago, F-75014 Paris (France)

Description

We show that scalar, 0-form, Galileon actions--models whose field equations contain only second derivatives--can be generalized to arbitrary even p-forms. More generally, they need not even depend on a single form, but may involve mixed p combinations, including equal p multiplets, where odd p fields are also permitted: We construct, for given dimension D, general actions depending on scalars, vectors, and higher p-form field strengths, whose field equations are of exactly second derivative order. We also discuss and illustrate their curved-space generalizations, especially the delicate nonminimal couplings required to maintain this order. Concrete examples of pure and mixed actions, field equations, and their curved-space extensions are presented.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
82
Journal Issue
6
Journal Page Range
p. 061501-061501.5
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42015496
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
COUPLING; FIELD EQUATIONS; MATHEMATICAL MODELS; MULTIPLETS; SCALARS; SIMULATION; VECTORS
Descriptors DEC
EQUATIONS; TENSORS

Optional Information

Notes
(c) 2010 American Institute of Physics