Scalar field and electromagnetic perturbations on locally rotationally symmetric spacetimes
From MaRDI portal
Publication:4659406
DOI10.1088/0264-9381/21/23/018zbMath1065.83019arXivgr-qc/0404116OpenAlexW3122743406WikidataQ63390979 ScholiaQ63390979MaRDI QIDQ4659406
Publication date: 21 March 2005
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0404116
Electromagnetic fields in general relativity and gravitational theory (83C50) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (16)
Perturbations of a class of locally rotationally symmetric cosmologies with applications to dissipative fluids ⋮ On the locally rotationally symmetric Einstein-Maxwell perfect fluid ⋮ Modelling the emergence of cosmic anisotropy from non-linear structures ⋮ Geometry of conformally symmetric generalized Vaidya spacetimes ⋮ Geometric properties of a certain class of compact dynamical horizons in locally rotationally symmetric class II spacetimes ⋮ Almost Birkhoff theorem in general relativity ⋮ Existence of conformal symmetries in locally rotationally symmetric spacetimes: Some covariant results ⋮ Some results on cosmological and astrophysical horizons and trapped surfaces ⋮ Matching conditions in locally rotationally symmetric spacetimes and radiating stars ⋮ Tidal forces are gravitational waves ⋮ Birkhoff theorem and matter ⋮ On some locally symmetric embedded spaces with non-negative scalar curvature and their characterization ⋮ Covariant perturbations of Schwarzschild black holes in f(R) gravity ⋮ Aspects of GRMHD in high-energy astrophysics: geometrically thick disks and tori agglomerates around spinning black holes ⋮ Semi-tetrad decomposition of spacetime with conformal symmetry ⋮ Horizon area bound and MOTS stability in locally rotationally symmetric solutions
This page was built for publication: Scalar field and electromagnetic perturbations on locally rotationally symmetric spacetimes
