Published August 15, 2011 | Version v1
Journal article

Nonlinear Fierz-Pauli theory from torsion and bigravity

  • 1. APC, UMR 7164 (CNRS, Universite Paris 7, CEA, Observatoire de Paris), 10 rue Alice Domon et Leonie Duquet, 75205 Paris Cedex 13 (France)
  • 2. Abdus Salam International Centre for Theoretical Physics, Trieste (Italy)

Description

The nonlinear aspects of a recently proposed model of massive spin-2 particles with propagating torsion are studied. We obtain a nonlinear equation which reduces at linear order to a generalized Fierz-Pauli equation in any background space-time with or without a vanishing torsion. We contrast those results with properties of a class of bigravity theories in an arbitrary background Einstein manifold. It is known that the nonperturbative spectrum of the bigravity model has 8 propagating physical degrees of freedom. This is identical to the physical propagating degrees of freedom of the massive spin-2 torsion model at the linearized order. The obtained nonlinear version of the Fierz-Pauli field equations, however, contains terms absent in the bigravity case which indicates that the curved space generalization of the unique flat space Fierz-Pauli equation is not unique. Moreover, in the torsion massive gravity model the Fierz-Pauli field appears as a derivative of fundamental fields. This, however, does not generate any unwanted pole once coupled to some external sources.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
84
Journal Issue
4
Journal Page Range
p. 044053-044053.8
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43083231
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
DEGREES OF FREEDOM; FIELD EQUATIONS; FIERZ-PAULI THEORY; GRAVITATION; NONLINEAR PROBLEMS; SPACE-TIME; SPECTRA; SPIN; TORSION
Descriptors DEC
ANGULAR MOMENTUM; EQUATIONS; PARTICLE PROPERTIES

Optional Information

Notes
(c) 2011 American Institute of Physics