2014
DOI: 10.1140/epjc/s10052-014-3073-2
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Counter-rotational effects on stability of $$2+1$$ 2 + 1 -dimensional thin-shell wormholes

Abstract: The role of angular momentum in a 2 + 1-dimensional rotating thin-shell wormhole (TSW) is considered. Particular emphasis is given to stability when the shells (rings) are counter-rotating. We find that counter-rotating halves make the TSW supported by the equation of state of a linear gas more stable. Under a small velocity dependent perturbation, however, it becomes unstable.

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Cited by 22 publications
(4 citation statements)
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“…где точка обозначает производную по τ . Тогда ненулевые компоненты внешней кривизны (11) записываются как…”
Section: устойчивость кнтоunclassified
See 1 more Smart Citation
“…где точка обозначает производную по τ . Тогда ненулевые компоненты внешней кривизны (11) записываются как…”
Section: устойчивость кнтоunclassified
“…Как было показано, количество экзотической материи [10] вокруг горловины можно минимизировать, выбирая подходящую геометрию кротовой норы. В настоящее время в литературе имеется много работ, авторы которых, следуя рекомендациям Виссера, сосредоточены на построении КНТО, описываемых в произвольной (низкой или высокой) размерности (см., например, работы [11]- [33]). В настоящей статье мы рассматриваем черную дыру со скалярными волосами (ЧДСВ) в размерности 2 + 1, которая является решением в теории Эйнштейна-Максвелла с самодействующим скалярным полем, описываемым потенциалом Лиувилля V (φ) [34].…”
Section: Introductionunclassified
“…Such investigation for the Schwarzschild TSW was performed by Poisson and Visser in [25]. Ever since, using the same formalism as [25], there have been diligent investigations on the stability of different TSWs against such a radial perturbation [26][27][28][29][30][31][32][33][34][35][36][37][38][39][40][41][42][43]. Concerning the TSW in regular spacetime, we refer to [44] where the authors investigated the mechanical stability of a TSW in the regular Hayward black hole.…”
Section: Introductionmentioning
confidence: 99%
“…This method was applied to construct a number of thinshell wormholes (TSW), including charged TSW [11,12], TSW with a cosmological constant [13], TSW in dilaton gravity [14], TSW from the regular Hayward black hole [15], TSW in higher-dimensional Einstein-Maxwell theory [16,17], rotating TSW [18,19], quantum corrected TSW in Bohmian quantum mechanics [20], primordial wormholes induced from Grand Unified Theories (GUTs) [21,22], canonical acoustic TSW, charged TSW with dilaton field, TSW with a Chaplygin gas, traversable wormholes in the anti-de Sitter space-time, TSW with a negative cosmological 2 Advances in High Energy Physics constant, wormholes in mimetic gravity, TSW from charged black string, cylindrical TSW, and many other interesting papers , while the stability analysis is investigated by different models, for example, linear perturbations [9] and specific equations of state (EoS) such as linear barotropic gas (LBG), Chaplygin gas (CG), and logarithmic gas (LogG) for the exotic matter [14,[59][60][61][62].…”
Section: Introductionmentioning
confidence: 99%