dc.contributor.author |
Farakos, K |
en |
dc.contributor.author |
Mavromatos, N |
en |
dc.contributor.author |
Pasipoularides, P |
en |
dc.date.accessioned |
2014-03-01T01:56:37Z |
|
dc.date.available |
2014-03-01T01:56:37Z |
|
dc.date.issued |
2008 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/28194 |
|
dc.subject |
Dispersion Relation |
en |
dc.subject |
Lorentz Invariance |
en |
dc.subject |
Refractive Index |
en |
dc.subject |
Speed of Light |
en |
dc.subject |
Active Galactic Nucleus |
en |
dc.subject |
Black Hole |
en |
dc.subject |
reissner nordstrom |
en |
dc.subject |
Space Time |
en |
dc.title |
Bulk photons in Asymmetrically Warped Space-times and Nontrivial Vacuum Refractive Index |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1088/1126-6708/2009/01/057 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1088/1126-6708/2009/01/057 |
en |
heal.publicationDate |
2008 |
en |
heal.abstract |
We consider asymmetrically warped brane models, or equivalently brane modelswhere the background metric is characterized by different time and space warpfactors. The main feature of these models is that 4D Lorentz symmetry isviolated for fields which propagate in the bulk, such as gravitons. In thispaper we examine the case of bulk photons in asymmetrically warped brane |
en |
dc.identifier.doi |
10.1088/1126-6708/2009/01/057 |
en |