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On the linear instability of the Ellis-Bronnikov-Morris-Thorne wormhole

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arxiv 1805.02602 v3 pith:2VQRSWAH submitted 2018-05-07 gr-qc math-phmath.MP

Francesco Cremona , Francesca Pirotta , Livio Pizzocchero (Universita' di Milano) This is my paper · ORCID
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keywords bronnikovinstabilitylinearwormholearisingcomparisonsconsiderderivation
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We consider the wormhole of Ellis, Bronnikov, Morris and Thorne (EBMT), arising from Einstein's equations in presence of a phantom scalar field. In this paper we propose a simplified derivation of the linear instability of this system, making comparisons with previous works on this subject (and generalizations) by Gonzalez, Guzman, Sarbach, Bronnikov, Fabris and Zhidenko.

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  1. Correspondence between quasinormal modes and grey-body factors of spherically symmetric traversable wormholes

    gr-qc 2024-12 conditional novelty 4.0 of 10

    For three families of traversable wormholes, the authors verify that the WKB correspondence between quasinormal modes and grey-body factors, known for black holes, holds to second order beyond the eikonal limit.

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