On the Quantum Improved Affine Gravity
arXiv:2101.05191 · doi:10.1016/j.dark.2021.100829
Abstract
Improvement of the classical gravity with the running gravitational coupling obtained from asymptotically safe gravity, is a good way of considering the effects of quantum gravity. This is usually done for metric theories of gravity. Here we investigate the effects of such an improvement for pure affine theories of gravity. To motivate the approach, we first consider the effects of quantum improvement on the connection using metric theory and investigate the effects on the causal structure of black hole solution. Next in the framework of Schrödinger-Eddington affine theory, the general way of affine improvement is presented and a spherically symmetric solution is obtained and compared with other ways of improvement.
30 pages, 6 figures
References in corpus (10)
- Metric-affine f(R) theories of gravity
- Renormalization group improved gravitational actions: a Brans-Dicke approach
- Asymptotic safety casts its shadow
- Quantum Gravity Effects in the Kerr Spacetime
- From renormalization group flows to cosmology
- Inflationary solutions in asymptotically safe f(R) theories
- On the nonsymmetric purely affine gravity
- Traversability of quantum improved wormhole solution
- A unified, purely affine theory of gravitation and electromagnetism
- On constructing purely affine theories with matter