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Perturbation theory and harmonic gauge propagation in general relativity, a particular example. (English) Zbl 1327.83070

Summary: We study how the changes of coordinates between the class of harmonic coordinates affect the analytical solutions of Einstein’s equations and we apply it to an analytical approach for stationary and axisymmetric solutions of Einstein equation used by J. A. Cabezas et al. [Gen. Relativ. Gravitation 39, No. 6, 707–736 (2007; Zbl 1157.83311)] and J. E. Cuchí et al. [Gen. Relativ. Gravitation 45, No. 7, 1433–1456 (2013; Zbl 1271.83027); erratum ibid. 45, No. 7, 1457 (2013)] to solve the problem of a self-gravitating rigidly rotating perfect fluid compact source.

MSC:

83C15 Exact solutions to problems in general relativity and gravitational theory
83C05 Einstein’s equations (general structure, canonical formalism, Cauchy problems)
53Z05 Applications of differential geometry to physics
83C25 Approximation procedures, weak fields in general relativity and gravitational theory
83C55 Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.)

References:

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[2] Cuchí, JE; Gil-Rivero, A.; Molina, A.; Ruiz, E., No article title, Gen. Relativ. Gravit., 45, 1433-1456 (2013) · Zbl 1271.83027 · doi:10.1007/s10714-013-1528-7
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