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Thin-shell wormholes: Linearization stability
Open accessAbstract
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. \textcopyright{} 1995 The American Physical Society.
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Cited by
Harko, T., Lobo, F. S. N., Nojiri, S., & Odintsov, S. D. (2011) · Physical Review D · doi:10.1103/physrevd.84.024020 · Cited by 2,772
Modified gravity theories on a nutshell: Inflation, bounce and late-time evolution
Nojiri, S., Odintsov, S. D., & Oikonomou, V. K. (2017) · Physics Reports · doi:10.1016/j.physrep.2017.06.001 · Cited by 2,734
Wormholes and holography: an introduction
Kundu, A. (2022) · The European Physical Journal C · doi:10.1140/epjc/s10052-022-10376-z · Cited by 48
Metadata
- Authors
- Poisson, E., & Visser, M.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1995-12-15
- Volume
- 52
- Issue
- 12
- Pages
- 7318-7321
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W2131770312
- Cited by
- 502
- References
- 0
- FWCI
- 0.41
- Type
- journal article
- Language
- en
- Open access
- green
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- Poisson, E., & Visser, M. (1995). Thin-shell wormholes: Linearization stability. Physical Review D. https://doi.org/10.1103/physrevd.52.7318
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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