Wave-like spatially homogeneous models of Stackel spacetimes (2.1) type in the scalar-tensor theory of gravity
arXiv:2006.01373 · doi:10.1142/S0217732320502752
Abstract
Six exact solutions are obtained in the general scalar-tensor theory of gravity related to spatially homogeneous wave-like models of the Universe. Wave-like space-time models allow the existence of privileged coordinate systems where the eikonal equation and the Hamilton-Jacobi equation of test particles can be integrated by the method of complete separation of variables with the separation of isotropic (wave) variables on which the space metric depends (non-ignored variables). An explicit form of the scalar field and two functions of the scalar field that are part of the general scalar-tensor theory of gravity are found. The explicit form of the eikonal function and the action function for test particles in the considered models is given. The obtained solutions are of type III according to the classification Bianchi and type N according to the classification of Petrov.
11 pages
References in corpus (2)
Cited by in corpus (7)
- Maxwell equations in homogeneous spaces with solvable groups of motions
- Classification of the non-null electrovacuum solution of Einstein-Maxwell equations with three-parameter abelian group of motions
- Classification of Petrov Homogeneous Spaces
- Exact models of pure radiation in R^2 gravity for spatially homogeneous Shapovalov spacetimes type II
- Type I Shapovalov wave spacetimes in the Brans-Dicke scalar-tensor theory of gravity
- Quadratic theory of gravity with a scalar field and type I Shapovalov wave spacetimes
- Gravitational wave of the Bianchi VII universe: particle trajectories, geodesic deviation and tidal accelerations