dc.contributor.author |
Mazharimousavi, S. Habib |
|
dc.contributor.author |
Halilsoy, Mustafa |
|
dc.date.accessioned |
2016-01-05T13:14:12Z |
|
dc.date.available |
2016-01-05T13:14:12Z |
|
dc.date.issued |
2014 |
|
dc.identifier.citation |
S. Habib Mazharimousavi and M. Halilsoy, "Thin-shell wormholes supported by total normal matter" Eur. Phys. J. C (2014) 74:3067. |
en_US |
dc.identifier.issn |
1434-6052 (online) |
|
dc.identifier.issn |
1434-6044 (print) |
|
dc.identifier.other |
DOI: 10.1140/epjc/s10052-014-3067-0 |
|
dc.identifier.uri |
http://hdl.handle.net/11129/1919 |
|
dc.description |
The file in this item is the publisher version (published version) of the article. |
|
dc.description.abstract |
The Zipoy-Voorhees-Weyl (ZVW) spacetime characterized by mass (M) and oblateness (δ) is proposed in the construction of viable thin-shell wormholes (TSWs). Departure from spherical / cylindrical symmetry yields positive total energy in spite of the fact that local energy density may take negative values. We show that oblateness of the bumpy sources / black holes can be incorporated as a new degree of freedom that may play role in the resolution of the exotic matter problem in TSWs. Small velocity perturbation reveals, however, that the resulting TSW is unstable. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.publisher |
The European Physical Journal C, Springer |
en_US |
dc.relation.ispartofseries |
Springer;Eur.Phys.J. C74 (2014) 9, 3067 |
|
dc.subject |
general relativity |
en_US |
dc.subject |
wormhole |
en_US |
dc.title |
Thin-shell wormholes supported by total normal matter |
en_US |
dc.type |
Article |
en_US |
dc.description.version |
Publisher Version; (Publisher’s PDF as it appears in the Journal). |
|