4D Einstein-Lovelock black holes: Hierarchy of orders in curvature

The Einstein-Lovelock theory contains an infinite series of corrections to the Einstein term with an increasing power of the curvature. It is well-known that for large black holes the lowest (Gauss-Bonnet) term is the dominant one, while for smaller black holes higher curvature corrections become im...

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Main Authors: R.A. Konoplya, A. Zhidenko
Format: Article
Language:English
Published: Elsevier 2020-08-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S037026932030410X
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spelling doaj-9148736aa8964a7981fd358a5fae8a442020-11-25T03:56:50ZengElsevierPhysics Letters B0370-26932020-08-018071356074D Einstein-Lovelock black holes: Hierarchy of orders in curvatureR.A. Konoplya0A. Zhidenko1Institute of Physics and Research Centre of Theoretical Physics and Astrophysics, Faculty of Philosophy and Science, Silesian University in Opava, Bezručovo nám. 13, CZ-746 01 Opava, Czech Republic; Peoples Friendship University of Russia (RUDN University), 6 Miklukho-Maklaya Street, Moscow 117198, Russian Federation; Corresponding author.Institute of Physics and Research Centre of Theoretical Physics and Astrophysics, Faculty of Philosophy and Science, Silesian University in Opava, Bezručovo nám. 13, CZ-746 01 Opava, Czech Republic; Centro de Matemática, Computação e Cognição (CMCC), Universidade Federal do ABC (UFABC), Rua Abolição, CEP: 09210-180, Santo André, SP, BrazilThe Einstein-Lovelock theory contains an infinite series of corrections to the Einstein term with an increasing power of the curvature. It is well-known that for large black holes the lowest (Gauss-Bonnet) term is the dominant one, while for smaller black holes higher curvature corrections become important. We will show that if one is limited by positive values of the coupling constants, then the dynamical instability of black holes serves as an effective cut-off of influence of higher curvature corrections in the 4D Einstein-Lovelock approach: the higher is the order of the Lovelock term, the smaller is the maximal value of the coupling constant allowing for stability, so that effectively only a first few orders can deform the observable values seemingly. For negative values of coupling constants this is not so, and, despite some suppression of higher order terms also occurs due to the decreasing threshold values of the coupling constant, this does not lead to an noticeable opportunity to neglect higher order corrections. In the case a lot of orders of Lovelock theory are taken into account, so that the black-hole solution depends on a great number of coupling constants, we propose a compact description of it in terms of only two or three parameters encoding all the observable values.http://www.sciencedirect.com/science/article/pii/S037026932030410X
collection DOAJ
language English
format Article
sources DOAJ
author R.A. Konoplya
A. Zhidenko
spellingShingle R.A. Konoplya
A. Zhidenko
4D Einstein-Lovelock black holes: Hierarchy of orders in curvature
Physics Letters B
author_facet R.A. Konoplya
A. Zhidenko
author_sort R.A. Konoplya
title 4D Einstein-Lovelock black holes: Hierarchy of orders in curvature
title_short 4D Einstein-Lovelock black holes: Hierarchy of orders in curvature
title_full 4D Einstein-Lovelock black holes: Hierarchy of orders in curvature
title_fullStr 4D Einstein-Lovelock black holes: Hierarchy of orders in curvature
title_full_unstemmed 4D Einstein-Lovelock black holes: Hierarchy of orders in curvature
title_sort 4d einstein-lovelock black holes: hierarchy of orders in curvature
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2020-08-01
description The Einstein-Lovelock theory contains an infinite series of corrections to the Einstein term with an increasing power of the curvature. It is well-known that for large black holes the lowest (Gauss-Bonnet) term is the dominant one, while for smaller black holes higher curvature corrections become important. We will show that if one is limited by positive values of the coupling constants, then the dynamical instability of black holes serves as an effective cut-off of influence of higher curvature corrections in the 4D Einstein-Lovelock approach: the higher is the order of the Lovelock term, the smaller is the maximal value of the coupling constant allowing for stability, so that effectively only a first few orders can deform the observable values seemingly. For negative values of coupling constants this is not so, and, despite some suppression of higher order terms also occurs due to the decreasing threshold values of the coupling constant, this does not lead to an noticeable opportunity to neglect higher order corrections. In the case a lot of orders of Lovelock theory are taken into account, so that the black-hole solution depends on a great number of coupling constants, we propose a compact description of it in terms of only two or three parameters encoding all the observable values.
url http://www.sciencedirect.com/science/article/pii/S037026932030410X
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