Schwarzschild-type black holes in Starobinsky-Bel-Robinson gravity
arXiv:2209.01574 · doi:10.1016/j.physletb.2023.137690
Abstract
We study physical properties of a Schwarzschild-type black hole in the framework of the recently proposed Starobinsky-Bel-Robinson (SBR) modified theory of gravity, working perturbatively in the new coupling constant. In particular, we compute the temperature, entropy, pressure and lifetime of a Schwarzschild-type black hole.
10 pages; v3: one more reference added, final version accepted for publication in Physics Letters B
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Cited by in corpus (9)
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- Geometric and topological corrections to Schwarzschild black hole
- Stability investigations of isotropic and anisotropic exponential inflation in the Starobinsky-Bel-Robinson gravity
- Black Holes and Wormholes Beyond Classical General Relativity
- Starobinsky inflation beyond the leading order
- Black Hole Shadows in Einstein-Bel-Robinson Gravity
- Black hole solutions to Einstein-Bel-Robinson gravity
- On the stability of de Sitter inflationary solution in the Starobinsky-Bel-Robinson gravity
- Universality on thermodynamic relation with corrections in Einstein-Bel-Robinson gravity Black hole