2004
DOI: 10.1103/physrevd.69.064005
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Static post-Newtonian equivalence of general relativity and gravity with a dynamical preferred frame

Abstract: 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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Cited by 120 publications
(139 citation statements)
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“…Gravitational effects of dynamical Lorentz-violating vector fields have been considered previously in the literature [56,57,58,59,60,61].…”
Section: Inflation Model With a Preferred Directionmentioning
confidence: 99%
“…Gravitational effects of dynamical Lorentz-violating vector fields have been considered previously in the literature [56,57,58,59,60,61].…”
Section: Inflation Model With a Preferred Directionmentioning
confidence: 99%
“…The reason is clear. In the J&M aether these terms arise, see [17], p.2, "from varying the metric dependence of the connection." However, in our case the connection is an independent variable.…”
Section: Curvaturementioning
confidence: 99%
“…In an attempt to violate Lorentz invariance locally, J&M [37] introduced an extra timelike 4-vector field u of unit length, see also [8,12,17,18,21,26,36,46] and the earlier work of Gasperini [23,24] and Kostelecky and Samuel [42]. This "aether field" is governed by a Lagrangian carrying a kinetic term ∼ (∇u) 2 and a massive term ∼ u 2 .…”
Section: Introductionmentioning
confidence: 99%
“…Theoretical and observational constraints on the coupling parameters c i have been determined from parameterized postNewtonian analysis [26,27,28], stability and linearized energy positivity [29,30,31,32], primordial nucleosynthesis [25], and vacuum Cerenkov radiation [31]. The combined constraints from all of these are reviewed in Ref.…”
Section: Observational Constraints On the Parameters C Imentioning
confidence: 99%