dc.contributor.author |
Koutsoumbas, G |
en |
dc.contributor.author |
Musiri, S |
en |
dc.contributor.author |
Papantonopoulos, E |
en |
dc.contributor.author |
Siopsis, G |
en |
dc.date.accessioned |
2014-03-01T11:44:43Z |
|
dc.date.available |
2014-03-01T11:44:43Z |
|
dc.date.issued |
2006 |
en |
dc.identifier.issn |
1126-6708 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/37111 |
|
dc.subject |
Black Holes |
en |
dc.subject |
Classical Theories of Gravity |
en |
dc.subject.classification |
Physics, Particles & Fields |
en |
dc.subject.other |
DE-SITTER SPACE |
en |
dc.subject.other |
FIELD HAIR |
en |
dc.subject.other |
STABILITY |
en |
dc.subject.other |
SUPERGRAVITY |
en |
dc.subject.other |
HORIZONS |
en |
dc.title |
Quasi-normal modes of electromagnetic perturbations of four-dimensional topological black holes with scalar hair |
en |
heal.type |
other |
en |
heal.identifier.primary |
10.1088/1126-6708/2006/10/006 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1088/1126-6708/2006/10/006 |
en |
heal.identifier.secondary |
006 |
en |
heal.language |
English |
en |
heal.publicationDate |
2006 |
en |
heal.abstract |
We study the perturbative behaviour of topological black holes with scalar hair. We calculate both analytically and numerically the quasi-normal modes of the electromagnetic perturbations. In the case of small black holes we find evidence of a second-order phase transition of a topological black hole to a hairy configuration. © SISSA 2006. |
en |
heal.publisher |
INT SCHOOL ADVANCED STUDIES |
en |
heal.journalName |
Journal of High Energy Physics |
en |
dc.identifier.doi |
10.1088/1126-6708/2006/10/006 |
en |
dc.identifier.isi |
ISI:000242714400084 |
en |
dc.identifier.volume |
2006 |
en |
dc.identifier.issue |
10 |
en |