A.N. Petrov. Noether and Belinfante corrected types of currents for perturbations in the Einstein-Gauss-Bonnet gravity
Submitted on: Sep 06, 2012, 05:50:41
Natural Sciences / Physics / Gravitation Theory (Relativity)
Description: In the framework of an arbitrary D-dimensional metric theory, perturbations are considered on arbitrary backgrounds that are however solutions of the theory. Conserved currents for perturbations are presented following two known prescriptions: canonical Noether theorem and Belinfante symmetrization rule. Using generalized formulae, currents in the Einstein-Gauss-Bonnet (EGB) gravity for arbitrary types of perturbations on arbitrary curved backgrounds (not only vacuum) are constructed in an explicit covariant form. Special attention is paid to the energy-momentum tensors for perturbations which are an important part in the structure of the currents. We use the derived expressions for two applied calculations: a) to present the energy density for weak flat gravitational waves in D-dimensional EGB gravity; b) to construct the mass flux for the Maeda-Dadhich-Molina 3D radiating black holes of a Kaluza-Klein type in 6D EGB gravity. *** This article was published in 'Class. Quantum Grav. 28 (2011) 215021' ***
The Library of Congress (USA) reference page : http://lccn.loc.gov/cn2013300046.
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