Black holes in f(T,B) gravity: exact and perturbed solutions

DOI10.1088/1475-7516/2022/01/037zbMath1486.83091arXiv2110.04087OpenAlexW4205745871MaRDI QIDQ5863305

Jackson Levi Said, Christian Pfeifer, María-José Guzmán, Sebastian Bahamonde, Alexey V. Golovnev

Publication date: 11 March 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2110.04087

zbMATH Keywords

gravityexact solutionsmodified gravityblack holes and black hole thermodynamics in GR and beyond

Mathematics Subject Classification ID

Black holes (83C57) Special connections and metrics on vector bundles (Hermite-Einstein, Yang-Mills) (53C07) Classical and relativistic thermodynamics (80A10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Spherical and hyperbolic convexity (52A55)

Related Items (13)

A frame based approach to computing symmetries with non-trivial isotropy groups ⋮ Quasinormal modes of black holes in f(T) gravity ⋮ Scalarized black holes in teleparallel gravity ⋮ Confronting quantum-corrected teleparallel cosmology with observations ⋮ The effective field theory approach to the strong coupling issue in f(T) gravity ⋮ Cosmological perturbations in the teleparallel analog of Horndeski gravity ⋮ Black hole solutions in scalar-tensor symmetric teleparallel gravity ⋮ f(T, B) gravity with statistically fitting of H(z) ⋮ Thick accretion disk configurations around a compact object in the brane-world scenario ⋮ Static spherically symmetric solutions in new general relativity ⋮ Inhomogeneous solutions in f(T,B) gravity ⋮ Scalar-multi-tensor approach to fT,B,∇μT,∇μB teleparallel gravity ⋮ f(T,B) gravity in a Friedmann–Lemaître–Robertson–Walker universe with nonzero spatial curvature

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