Static post-Newtonian equivalence of GR and gravity with a dynamical preferred frame

Details Static post-Newtonian equivalence of GR and gravity with a dynamical preferred frame Static post-Newtonian equivalence of GR and gravity with a dynamical preferred frame

2003-10-07

arxiv.org/abs/gr-qc/0310044v3

Phys.Rev. D69 (2004) 064005

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages; v.2: minor editing, signs corrected, version to appear in PRD; v. 3: signs corrected in eqn (3)

Scientific paper

10.1103/PhysRevD.69.064005

A generally covariant extension of general relativity (GR) in which a dynamical unit timelike vector field is coupled to the metric is studied in the asymptotic weak field limit of spherically symmetric static solutions. The two post-Newtonian parameters known as the Eddington-Robertson-Schiff parameters are found to be identical to those in the case of pure GR, except for some non-generic values of the coefficients in the Lagrangian.

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