Construction of gauge-invariant variables of linear metric perturbations on an arbitrary background spacetime
Open Access
- 1 January 2013
- journal article
- Published by Oxford University Press (OUP) in Progress of Theoretical and Experimental Physics
- Vol. 2013 (4) , 43E02
Abstract
An outline of a proof of the decomposition of linear metric perturbations into gauge-invariant and gauge-variant parts on an arbitrary background spacetime that admits ADM decomposition is discussed. We explicitly construct the gauge-invariant and gauge-variant parts of the linear metric perturbations through the assumption of the existence of some Green functions. We also confirm the result through another approach. This implies that we can develop a higher-order gauge-invariant perturbation theory on an arbitrary background spacetime. Remaining issues to complete the general framework of the general-relativistic higher-order gauge-invariant perturbation theories are also discussed.Keywords
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This publication has 63 references indexed in Scilit:
- Gauge-invariant and coordinate-independent perturbations of stellar collapse. II. Matching to the exteriorPhysical Review D, 2001
- Brane world cosmology: Gauge-invariant formalism for perturbationPhysical Review D, 2000
- Gauge-invariant and coordinate-independent perturbations of stellar collapse: The interiorPhysical Review D, 2000
- Theory of cosmological perturbationsPhysics Reports, 1992
- Cosmological Perturbation TheoryProgress of Theoretical Physics Supplement, 1984
- Gauge-invariant cosmological perturbationsPhysical Review D, 1980
- Gauge-invariant coupled gravitational, acoustical, and electromagnetic modes on most general spherical space-timesPhysical Review D, 1980
- Junction conditions for odd-parity perturbations on most general spherically symmetric space-timesPhysical Review D, 1979
- Even parity junction conditions for perturbations on most general spherically symmetric space–timesJournal of Mathematical Physics, 1979
- Gauge-invariant perturbations on most general spherically symmetric space-timesPhysical Review D, 1979