Self-accelerating massive gravity: Covariant perturbation theory

Pavel Motloch and Wayne Hu
Phys. Rev. D 90, 104027 – Published 19 November 2014

Abstract

We undertake a complete and covariant treatment for the quadratic Lagrangian of all of the degrees of freedom of massive gravity with a fixed flat fiducial metric for arbitrary massive gravity parameters around any isotropic self-accelerating background solution. Generically, three out of four Stückelberg degrees of freedom propagate in addition to the usual two tensor degrees of freedom of general relativity. The complete kinetic structure typically is only revealed at an order in the graviton mass that is equivalent to retaining curvature terms in a locally flat expansion. These results resolve several apparent discrepancies in the literature where zero degrees of freedom propagate in either special cases or approximate treatments as well as decoupling limit analyses which attempt to count longitudinal degrees of freedom.

  • Received 8 September 2014

DOI:https://doi.org/10.1103/PhysRevD.90.104027

© 2014 American Physical Society

Authors & Affiliations

Pavel Motloch1 and Wayne Hu2

  • 1Kavli Institute for Cosmological Physics, Department of Physics, University of Chicago, Chicago, Illinois 60637, USA
  • 2Kavli Institute for Cosmological Physics, Department of Astronomy and Astrophysics, Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA

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Issue

Vol. 90, Iss. 10 — 15 November 2014

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