General Relativity and Gravitation

, Volume 44, Issue 12, pp 3103–3109

Linking covariant and canonical general relativity via local observers

Authors

  • Steffen Gielen
    • Perimeter Institute for Theoretical Physics
    • Institute for Quantum GravityUniversität Erlangen-Nürnberg
Research Article

DOI: 10.1007/s10714-012-1443-3

Cite this article as:
Gielen, S. & Wise, D.K. Gen Relativ Gravit (2012) 44: 3103. doi:10.1007/s10714-012-1443-3

Abstract

Hamiltonian gravity, relying on arbitrary choices of ‘space,’ can obscure spacetime symmetries. We present an alternative, manifestly spacetime covariant formulation that nonetheless distinguishes between ‘spatial’ and ‘temporal’ variables. The key is viewing dynamical fields from the perspective of a field of observers—a unit timelike vector field that also transforms under local Lorentz transformations. On one hand, all fields are spacetime fields, covariant under spacetime symmeties. On the other, when the observer field is normal to a spatial foliation, the fields automatically fall into Hamiltonian form, recovering the Ashtekar formulation. We argue this provides a bridge between Ashtekar variables and covariant phase space methods. We also outline a framework where the ‘space of observers’ is fundamental, and spacetime geometry itself may be observer-dependent.

Keywords

Lorentz covariance Lorentz symmetry breaking Covariant real Ashtekar variables Observer space Relative locality

Copyright information

© Springer Science+Business Media, LLC 2012