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Gauge-invariant description of weak gravitational field on a spherically symmetric background with cosmological constant
We present a formalism for analysis of linear Cauchy data on a Kottler metric. Our approach is based on the ADM formulation of the problem of evolution. It removes redundancy due to gauge transformations and geometric constraints. A set of four gauge-invariant, scalar functions on the Cauchy surface...
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Published in: | Classical and quantum gravity 2019-11, Vol.36 (21), p.215006 |
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Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | We present a formalism for analysis of linear Cauchy data on a Kottler metric. Our approach is based on the ADM formulation of the problem of evolution. It removes redundancy due to gauge transformations and geometric constraints. A set of four gauge-invariant, scalar functions on the Cauchy surface is produced and shown to contain full physical information from the initial data. The symplectic form of the theory and equations of motion are reformulated in terms of these invariants and an expression for the energy and angular momentum of the perturbation is produced. We also obtain a basic classification of stationary solutions. |
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ISSN: | 0264-9381 1361-6382 |
DOI: | 10.1088/1361-6382/ab42c8 |