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Several calculations in conformally static spacetimes rely on the introduction of an ultrastatic background.
T. Fulton, F. Rohrlich and L. Witten, “Conformal invariance in physics”, Rev. Mod. Phys
1962
Earlier work this paper cites.
S. A. Fulling, “Alternative vacuum states in static space-times with horizons”, J. Phys. A
1977
Earlier work this paper cites.
J. S. Dowker and G. Kennedy, “Finite temperature and boundary effects in static space-times”, J. Phys. A
1978
Earlier work this paper cites.
W. Rindler,
1979
Earlier work this paper cites.
M. R. Brown, A. C. Ottewill and S. T. C. Siklos, “Comments on conformal Killing vector fields and quantum field theory”, Phys. Rev. D
1983
Cited alongside, same era.
R. M. Wald,
1984
Cited alongside, same era.
M. A. Abramowicz and A. R. Prasanna, “Centrifugal-force reversal near a Schwarzschild black hole”, Mon. Not. R. Astron. Soc
1990
Cited alongside, same era.
M. A. Abramowicz, B. Carter and J. P. Lasota, “Optical reference geometry for stationary and static dynamics”, Gen. Relativ. Gravit
1993
Cited alongside, same era.
Latin letters
Cited in the paper.
I focus on transformations that admit generators, so in particular I am not dealing with discrete transformations
Cited in the paper.
In fact, it is a subspace of the larger space of transformations that preserve the synchronous gauge for an arbitrary metric, when the coefficients
Cited in the paper.
This result could also be obtained looking for the
Cited in the paper.
The two-dimensional metrics are both flat iff their scalar curvatures (containing the same information as the full Riemann tensor) are
Cited in the paper.
This idea has been made more precise in a series of papers about the notion of inertial forces in general relativity
1996
Later among the works it cites.
M. Kaku,
1997
Later among the works it cites.
H. Stephani,
2003
Later among the works it cites.
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