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

verfasst von: Sebastian Bahamonde, Alexey Golovnev, María-josé Guzmán, Jackson Levi Said, Christian Pfeifer
Abstract: Spherically symmetric solutions of theories of gravity built one fundamental class of solutions to describe compact objects like black holes and stars. Moreover, they serve as starting point for the search of more realistic axially symmetric solutions which are capable to describe rotating compact objects. Theories of gravity that do not possess spherically symmetric solutions which meet all observational constraints are easily falsified. In this article, we discuss classes of exact and perturbative spherically symmetric solutions in f(T,B)-gravity. The perturbative solutions add to the ones which have already been found in the literature, while the exact solutions are presented here for the first time. Moreover, we present general methods and strategies, like generalized Bianchi identities, to find spherically solutions in modified teleparallel theories of gravity.
Externe Organisation(en): University of Tartu
Tokyo Institute of Technology
The British University in Egypt
Universidad de La Serena (ULS)
University of Malta
Universität Bremen
Typ: Artikel
Journal: Journal of Cosmology and Astroparticle Physics
Band: 2022
Seiten: 037
ISSN: 1475-7516
Publikationsdatum: 19.01.2022
Publikationsstatus: Veröffentlicht
Peer-reviewed: Ja
ASJC Scopus Sachgebiete: Astronomie und Astrophysik
Elektronische Version(en): https://doi.org/10.1088/1475-7516/2022/01/037 (Zugang: Unbekannt)

BibTeX

@article{5a42ed0370694483a2e9344ec9ba0de9,
title = "Black holes in f(T,B) gravity: exact and perturbed solutions",
abstract = "Spherically symmetric solutions of theories of gravity built one fundamental class of solutions to describe compact objects like black holes and stars. Moreover, they serve as starting point for the search of more realistic axially symmetric solutions which are capable to describe rotating compact objects. Theories of gravity that do not possess spherically symmetric solutions which meet all observational constraints are easily falsified. In this article, we discuss classes of exact and perturbative spherically symmetric solutions in f(T,B)-gravity. The perturbative solutions add to the ones which have already been found in the literature, while the exact solutions are presented here for the first time. Moreover, we present general methods and strategies, like generalized Bianchi identities, to find spherically solutions in modified teleparallel theories of gravity.",
keywords = "black holes and black hole thermodynamics in GR and beyond, Exact solutions, gravity, modified gravity",
author = "Sebastian Bahamonde and Alexey Golovnev and Mar{\'i}a-jos{\'e} Guzm{\'a}n and Said, {Jackson Levi} and Christian Pfeifer",
note = "Publisher Copyright: {\textcopyright} 2022 IOP Publishing Ltd and Sissa Medialab.",
year = "2022",
month = jan,
day = "19",
doi = "10.1088/1475-7516/2022/01/037",
language = "English",
volume = "2022",
pages = "037",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing Ltd.",
number = "1",
}