Black Holes and Non-perturbative Gravitational Waves in Gravity
arXiv:2312.12702 · doi:10.1140/epjc/s10052-023-12261-9
Abstract
Exact solutions of spherically symmetric black hole and gravitational wave are explored in gravity in arbitrary dimension. We find two exact solutions for the radiation and absorption of null dust. In the framework of general relativity, the Birkhoff theorem strictly forbids the existence of spherical gravitational waves in vacuum space. We find spherical non-perturbative gravitational waves, which are shear-free, twist-free, but expanding.
13 pages
References in corpus (19)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- Disappearing cosmological constant in f(R) gravity
- Class of viable modified gravities describing inflation and the onset of accelerated expansion
- Modified f(R) gravity unifying R^m inflation with \LambdaCDM epoch
- Spherically symmetric solutions of modified field equations in f(R) theories of gravity
- Concepts and status of Chinese space gravitational wave detection projects
- Spherically symmetric solutions in f(R)-gravity via Noether Symmetry Approach
- Modified non-local-F(R) gravity as the key for the inflation and dark energy
- FRW Cosmology in F(R,T) gravity
- Spherical symmetry in -gravity
- 6+1 lessons from f(R) gravity
- Misner-Sharp Mass in -dimensional Gravity
- First Principle Study of Gravitational Pressure and Thermodynamics of FRW Universe
- Black holes and gravitational waves in three-dimensional f(R) gravity
- Novel black holes in higher derivative gravity
- From thermodynamics to the solutions in gravity theory
- Non perturbative spherical gravitational waves
- Sky localization of space-based detectors with time-delay interferometry