Wave-like exact models with symmetry of spatial homogeneity in the quadratic theory of gravity with a scalar field
arXiv:2105.14123 · doi:10.3390/sym13071173
Abstract
Exact solutions are obtained in the quadratic theory of gravity with a scalar field for wave-like models of space-time with spatial homogeneity symmetry and allowing the integration of the equations of motion of test particles in the Hamilton-Jacobi formalism by the method of separation of variables with separation of wave variables (Shapovalov spaces of type II). The form of the scalar field and the scalar field functions included in the Lagrangian of the theory is found. The obtained exact solutions can describe the primary gravitational wave disturbances in the Universe (primary gravitational waves).
24 pages
References in corpus (14)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Inflationary cosmology in modified gravity theories
- Gauss-Bonnet term corrections in scalar field cosmology
- Separation of variables in Hamilton-Jacobi equation for a charged test particle in the Stackel spaces of type (2.0)
- Pure radiation in space-time models that admit integration of the eikonal equation by the separation of variables method
- Shapovalov wave-like spacetimes
- Canonical Scalar Field Inflation with String and -Corrections
- Separation of variables in Hamilton-Jacobi and Klein-Gordon-Fock equations for a charged test particle in the Stackel spaces of type (1.1)
- Separation of variables in Hamilton-Jacobi equation for a charged test particle in the Stackel spaces of type (2.1)
- On stable exponential solutions in Einstein-Gauss-Bonnet cosmology with zero variation of G
- Spatially homogeneous models of Stäckel spacetimes of type (2.1)
- Early universe in view of a modified theory of gravity
- Horndeski theories and beyond from higher dimensions