Pure radiation in space-time models that admit integration of the eikonal equation by the separation of variables method
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Publication:4599475
DOI10.1063/1.5003854zbMath1386.83136arXiv1709.01718OpenAlexW2753768710MaRDI QIDQ4599475
Publication date: 2 January 2018
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1709.01718
Related Items (11)
Algebras of symmetry operators of the Klein-Gordon-Fock equation for groups acting transitively on two-dimensional subspaces of a space-time manifold ⋮ Algebras of integrals of motion for the Hamilton–Jacobi and Klein–Gordon–Fock equations in spacetime with four-parameter groups of motions in the presence of an external electromagnetic field ⋮ Hamilton-Jacobi and Klein-Gordon-Fock equations for a charged test particle in space-time with simply transitive four-parameter groups of motions ⋮ Spatially homogeneous conformally Stäckel spaces of type (3.1) ⋮ Spatially homogeneous models Stäckel spaces of type (2.1) ⋮ Deviation of geodesics and particle trajectories in a gravitational wave of the Bianchi type VI universe ⋮ Separation of variables in Hamilton–Jacobi and Klein–Gordon–Fock equations for a charged test particle in the stackel spaces of type (1.1) ⋮ Wave-like spatially homogeneous models of Stäckel spacetimes (2.1) type in the scalar-tensor theory of gravity ⋮ Exact models of pure radiation in R2 gravity for spatially homogeneous wave-like Shapovalov spacetimes type II ⋮ Models of generalized scalar-tensor gravitation theories with radiation allowing the separation of variables in the eikonal equation ⋮ Plane gravitational waves in spatially-homogeneous models of type-(3.1) Stäckel spaces
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- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
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