Counterrotational effects on stability of 2+1-dimensional thin-shell wormholes

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The European Physical Journal C, Springer

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Abstract

The role of angular momentum in a 2+1-dimensional rotating thin-shell wormhole (TSW) is considered. Particular emphasis is made on stability when the shells (rings) are counterrotating. 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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The file in this item is the publisher version (published version) of the article.

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general relativity, black holes

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S. HabibMazharimousavi and M. Halilsoy, arXiv:1407.4673 “Counterrotational effects on stability of 2+1-dimensional thin-shell wormholes” Eur. Phys. J. C 74, 3073 (2014).

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