Vector-tensor nature of Bekenstein’s relativistic theory of modified gravity

T. G. Zlosnik, P. G. Ferreira, and Glenn D. Starkman
Phys. Rev. D 74, 044037 – Published 29 August 2006

Abstract

Bekenstein’s theory of relativistic gravity is conventionally written as a bimetric theory. The two metrics are related by a disformal transformation defined by a dynamical vector field and a scalar field. In this paper we show that the theory can be rewritten as vector-tensor theory akin to Einstein-Aether theories with noncanonical kinetic terms. We discuss some of the implications of this equivalence.

  • Received 8 June 2006

DOI:https://doi.org/10.1103/PhysRevD.74.044037

©2006 American Physical Society

Authors & Affiliations

T. G. Zlosnik1, P. G. Ferreira1,2, and Glenn D. Starkman1,3

  • 1Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, United Kingdom
  • 2African Institute for Mathematical Sciences, 6-8 Melrose Road, Muizenberg 7945, South Africa
  • 3Department of Astronomy and Physics, Case Western Reserve, Cleveland, Ohio, USA

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 74, Iss. 4 — 15 August 2006

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×