2021
DOI: 10.1016/j.dark.2020.100754
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Nonsingular black holes and nonsingular universes in the regularized Lovelock gravity

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Cited by 10 publications
(12 citation statements)
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“…Such a regularized theory can evade the Lovelock theorem [18], which states that only the metric tensor and Einstein tensor contribute to the dynamics of 4-dimensional spacetime. Besides usual black holes in this theory [16,[19][20][21], regular black holes are also admitted in the Einstein-Lovelock theory [22]. We find that ultracompact objects are as well permitted in such a theory.…”
Section: Introductionmentioning
confidence: 64%
See 1 more Smart Citation
“…Such a regularized theory can evade the Lovelock theorem [18], which states that only the metric tensor and Einstein tensor contribute to the dynamics of 4-dimensional spacetime. Besides usual black holes in this theory [16,[19][20][21], regular black holes are also admitted in the Einstein-Lovelock theory [22]. We find that ultracompact objects are as well permitted in such a theory.…”
Section: Introductionmentioning
confidence: 64%
“…where the parameter η • with the dimension of [length] 2 has to be introduced to balance the dimension of Eq. ( 6), the explicit form of ψ is, therefore, found as [22]…”
Section: Einstein-lovelock Ultracompact Objectmentioning
confidence: 99%
“…We will return to more general solutions, and possible restrictions on solutions in the context of regularised theories below, and for now focus on the behaviours prescribed by Eqs. ( 130)- (131).…”
Section: Background Cosmologymentioning
confidence: 99%
“…In principle, the background evolution, and the evolution of perturbations encoded in Eqs. ( 130)- (131) and Eqs. ( 136)- (138), can be used to constrain 4D Einstein-Gauss-Bonnet, by comparing predictions of the theory against observation, thereby putting constraints on allowed values of α.…”
Section: Constraints On αmentioning
confidence: 99%
“…Here, we investigate this question within the framework of the so-called regularized 4D Einstein-Lovelock gravity. Recently, a simple dimensional regularization of Lovelock gravity has been discussed in a number of research papers by which the effects of ghost-free, higher-order curvatures can be extended to four-dimensional spacetimes [1,[50][51][52][53][54][55]. As a result of this trick, it is expected that some features of Lovelock gravity may be observed again, or may be lost, or may undergo fundamental changes in four dimensions.…”
mentioning
confidence: 99%