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Preprint . 1995
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Thin-shell wormholes: Linearization stability

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 15 Dec 1995Embargo end date: 01 Jan 1995 English Publisher:American Physical Society (APS)Journal:Physical Review D, volume 52, pages 7,318-7,321 (issn: 0556-2821, Copyright policy )
Authors: Poisson, Eric; Visser, Matt;

doi: 10.1103/physrevd.52.7318 , 10.48550/arxiv.gr-qc/9506083

pmid: 10019270

arXiv: gr-qc/9506083

Thin-shell wormholes: Linearization stability

Abstract

The class of spherically-symmetric thin-shell wormholes provides a particularly elegant collection of exemplars for the study of traversable Lorentzian wormholes. In the present paper we consider linearized (spherically symmetric) perturbations around some assumed static solution of the Einstein field equations. This permits us to relate stability issues to the (linearized) equation of state of the exotic matter which is located at the wormhole throat.

4 pages; ReV_TeX 3.0; one postscript figure

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Keywords

FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), General Relativity and Quantum Cosmology

  • BIP!
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    selected citations
    These citations are derived from selected sources.
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 338
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    		 Top 1%
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 Top 1%
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
338
Top 1%
Top 1%
Average
Green