dc.contributor.author |
Sakallı, İzzet |
|
dc.contributor.author |
Övgün, Ali |
|
dc.date.accessioned |
2017-04-20T11:01:30Z |
|
dc.date.available |
2017-04-20T11:01:30Z |
|
dc.date.issued |
2017-02-09 |
|
dc.identifier.citation |
Övgün, A. & Sakalli, I. Theor Math Phys (2017) 190: 120. doi:10.1134/S004057791701010X |
en_US |
dc.identifier.issn |
0040-5779 (print) |
|
dc.identifier.issn |
1573-9333 (online) |
|
dc.identifier.uri |
http://dx.doi.org/10.1134/S004057791701010X |
|
dc.identifier.uri |
http://hdl.handle.net/11129/3219 |
|
dc.description |
The file in this item is the post-print version of the article (author’s copy; author’s final manuscript, accepted for publication after peer-review process). Due to copyright restrictions, the access to the publisher version (published version) of this article is only available via subscription. You may click URI and have access to the Publisher Version of this article through the publisher web site or online databases, if your Library or institution has subscription to the related journal or publication. |
en_US |
dc.description.abstract |
Using a black hole with scalar hair, we construct a scalar thin-shell wormhole (TSW) in 2+1 dimensions by applying the Visser cut and paste technique. The surface stress, which is concentrated at the wormhole throat, is determined using the Darmois–Israel formalism. Using various gas models, we analyze the stability of the TSW. The stability region is changed by tuning the parameters l and u. We note that the obtained TSW originating from a black hole with scalar hair could be more stable with a particular value of the parameter l, but it still requires exotic matter. |
en_US |
dc.language.iso |
eng |
en_US |
dc.publisher |
Springer |
en_US |
dc.relation.isversionof |
10.1134/S004057791701010X |
en_US |
dc.rights |
info:eu-repo/semantics/openAccess |
en_US |
dc.subject |
theoretical physics |
en_US |
dc.subject |
wormhole |
en_US |
dc.subject |
thin-shell |
en_US |
dc.subject |
Darmois–Israel formalism |
en_US |
dc.title |
A particular thin-shell wormhole |
en_US |
dc.type |
article |
en_US |
dc.relation.journal |
Theoretical and Mathematical Physics |
en_US |
dc.contributor.department |
Eastern Mediterranean University, Faculty of Arts and Sciences, Department of Physics |
en_US |
dc.identifier.volume |
190 |
en_US |
dc.identifier.issue |
1 |
en_US |
dc.identifier.startpage |
120 |
en_US |
dc.identifier.endpage |
129 |
en_US |