Problems with propagation and time evolution in f(T) gravity

Yen Chin Ong, Keisuke Izumi, James M. Nester, and Pisin Chen
Phys. Rev. D 88, 024019 – Published 10 July 2013

Abstract

Teleparallel theories of gravity have a long history. They include a special case referred to as the teleparallel equivalent of general relativity (TEGR, also known as GR). Recently this theory has been generalized to f(T) gravity. Tight constraints from observations suggest that f(T) gravity is not as robust as initially hoped. This might hint at hitherto undiscovered problems at the theoretical level. In this work, we point out that a generic f(T) theory can be expected to have certain problems including superluminal propagating modes, the presence of which can be revealed by using the characteristic equations that govern the dynamics in f(T) gravity and/or the Hamiltonian structure of the theory via Dirac constraint analysis. We use several examples from simpler gauge field theories to explain how such superluminal modes could arise. We also point out problems with the Cauchy development of a constant time hypersurface in Friedmann-Lemaître-Roberson-Walker (FLRW) spacetime in f(T) gravity. The time evolution from a FLRW (and as a special case, Minkowski spacetime) initial condition is not unique.

  • Received 19 April 2013

DOI:https://doi.org/10.1103/PhysRevD.88.024019

© 2013 American Physical Society

Authors & Affiliations

Yen Chin Ong*

  • Graduate Institute of Astrophysics, National Taiwan University, Taipei 10617, Taiwan and Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei 10617, Taiwan

Keisuke Izumi

  • Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei 10617, Taiwan

James M. Nester

  • Department of Physics, National Central University, Chungli 320, Taiwan; Graduate Institute of Astronomy, National Central University, Chungli 320, Taiwan; Center for Mathematics and Theoretical Physics, National Central University, Chungli 320, Taiwan; and Institute of Physics, Academia Sinica, Taipei 11529, Taiwan

Pisin Chen§

  • Graduate Institute of Astrophysics, National Taiwan University, Taipei 10617, Taiwan; Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei 10617, Taiwan; Department of Physics, National Taiwan University, Taipei 10617, Taiwan; and Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University, Stanford, California 94305, USA

  • *ongyenchin@member.ams.org
  • izumi@phys.ntu.edu.tw
  • nester@phy.ncu.edu.tw
  • §chen@slac.stanford.edu

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Issue

Vol. 88, Iss. 2 — 15 July 2013

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