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- W2038688001 abstract "We present a covariant decomposition of Einstein's field equations which is particularly suitable for perturbations of spherically symmetric---and general locally rotationally symmetric---spacetimes. Based upon the utility of the $1+3$ covariant approach to perturbation theory in cosmology, the semi-tetrad, $1+1+2$ approach presented here should be useful for analyzing perturbations of a variety of systems in a covariant and gauge-invariant manner. Such applications range from stellar objects to cosmological models such as the spherically symmetric Lema^{i}tre-Tolman-Bondi solutions or the class of locally rotationally symmetric Bianchi models." @default.
- W2038688001 created "2016-06-24" @default.
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- W2038688001 date "2007-11-19" @default.
- W2038688001 modified "2023-10-02" @default.
- W2038688001 title "Covariant approach for perturbations of rotationally symmetric spacetimes" @default.
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- W2038688001 doi "https://doi.org/10.1103/physrevd.76.104034" @default.
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