dc.contributor.author |
Amirabi, Zahra |
|
dc.contributor.author |
Halilsoy, Mustafa |
|
dc.contributor.author |
Mazharimousavi, S. Habib |
|
dc.date.accessioned |
2016-01-15T13:34:41Z |
|
dc.date.available |
2016-01-15T13:34:41Z |
|
dc.date.issued |
2013 |
|
dc.identifier.citation |
Z. Amirabi, M. Halilsoy and S. HabibMazharimousavi, arXiv:1103.3019 "Stable thin-shell wormholes with a Chaplygin gas in Einstein-Maxwell-Gauss-Bonnet gravity". Phys. Rev. D 88, 124023 (2013). |
en_US |
dc.identifier.issn |
1550-7998 |
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dc.identifier.other |
DOI: 10.1103/PhysRevD.88.124023 |
|
dc.identifier.uri |
http://hdl.handle.net/11129/1989 |
|
dc.description |
The file in this item is the publisher version (published version) of the article. |
en_US |
dc.description.abstract |
We study the stability of thin-shell wormholes in Einstein-Maxwell-Gauss-Bonnet gravity. The equation of state of the thin shell wormhole is considered first to obey a generalized Chaplygin gas and then we generalize it to an arbitrary state function which covers all known cases studied so far. In particular we study the modified Chaplygin gas and give an assessment for a general parotropic fluid. Our study is in d-dimensions and with numerical analysis in d=5 we show the effect of the GB parameter in the stability of thin-shell wormholes against the radial perturbations. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.publisher |
Physical Review D, American Physical Society (APS) |
en_US |
dc.relation.ispartofseries |
;Phys. Rev. D 88, 124023 (2013) |
|
dc.subject |
thin-shell wormholes |
en_US |
dc.subject |
general relativity |
en_US |
dc.subject |
wormholes |
en_US |
dc.subject |
gravity |
en_US |
dc.subject |
Einstein-Maxwell-Gauss-Bonnet gravity |
en_US |
dc.title |
Stable thin-shell wormholes with a Chaplygin gas in Einstein-Maxwell-Gauss-Bonnet gravity |
en_US |
dc.type |
Article |
en_US |
dc.description.version |
Publisher Version (Published Version). |
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