Abstract
Abstract
We study conformal transformations in the most general parity-preserving models of the New
General Relativity type. Then we apply them to analysis of cosmological perturbations in the
(simplest) spatially flat cosmologies. Strong coupling issues around Minkowski spacetime are seen
for many special cases of these models. At the same time, the behaviour of the most general
three-parameter case seems to be very robust, presumably always with only the eight first-class
constraints coming from diffeomorphisms. Also the case of the so-called 1-parameter New GR doesn't
show any discontinuity between Minkowski and the cosmology, though without showing any deviations
from GR which would be observable at this level either.
Cited by
2 articles.
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