Preprint Article Version 3 This version is not peer-reviewed

Linearized Stability of Bardeen de-Sitter Thin-Shell Wormholes

Version 1 : Received: 16 September 2019 / Approved: 18 September 2019 / Online: 18 September 2019 (03:36:07 CEST)
Version 2 : Received: 19 September 2019 / Approved: 20 September 2019 / Online: 20 September 2019 (05:05:09 CEST)
Version 3 : Received: 5 October 2019 / Approved: 7 October 2019 / Online: 7 October 2019 (12:35:21 CEST)

How to cite: Alshal, H. Linearized Stability of Bardeen de-Sitter Thin-Shell Wormholes. Preprints 2019, 2019090196 (doi: 10.20944/preprints201909.0196.v3). Alshal, H. Linearized Stability of Bardeen de-Sitter Thin-Shell Wormholes. Preprints 2019, 2019090196 (doi: 10.20944/preprints201909.0196.v3).

Abstract

A thin-shell wormhole is crafted by the cut-and-paste method of two Bardeen de-Sitter black holes using Darmois-Israel formalism. Energy conditions are considered for different values of magnetic charge while both mass and cosmological constant are fixed. The attractive and repulsive characteristics of the throat of the thin-shell wormhole are also examined through the radial acceleration. Dynamics and stability of the wormhole are studied around the static solutions of the linearized radial perturbations at the throat of the wormhole. The regions of stability are determined by checking out the condition of concavity of the potential as a function in the throat radius for different values of magnetic charges.

Subject Areas

Bardeen; black hole; de-Sitter; thin-shell; wormhole

Comments (1)

Comment 1
Received: 7 October 2019
Commenter: Hassan Alshal
Commenter's Conflict of Interests: Author
Comment: Abstract expanded, more citations added, made in 2 columns style
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