Dilatonic black holes in higher curvature string gravity. II. Linear stability
| dc.contributor.author | Kanti, P. | en |
| dc.contributor.author | Mavromatos, N. E. | en |
| dc.contributor.author | Rizos, J. | en |
| dc.contributor.author | Tamvakis, K. | en |
| dc.contributor.author | Winstanley, E. | en |
| dc.date.accessioned | 2015-11-24T18:30:14Z | |
| dc.date.available | 2015-11-24T18:30:14Z | |
| dc.identifier.issn | 0556-2821 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16352 | |
| dc.rights | Default Licence | - |
| dc.subject | arbitrary gauge groups | en |
| dc.subject | yang-mills solitons | en |
| dc.subject | no-hair | en |
| dc.subject | instability | en |
| dc.subject | sphalerons | en |
| dc.subject | systems | en |
| dc.subject | number | en |
| dc.title | Dilatonic black holes in higher curvature string gravity. II. Linear stability | en |
| heal.abstract | We demonstrate the linear stability of dilatonic black holes appearing in a string-inspired higher-derivative gravity theory with a Gauss-Bonnet curvature-squared term. The proof is accomplished by mapping the system to a one-dimensional Schrodinger problem which admits no bound states. This result is important in that it constitutes a linearly stable example of a black hole that bypasses the "no-hair conjecture." However, dilaton hair is secondary in the sense that it is not accompanied by any new quantum number for the black hole solution. | en |
| heal.access | campus | - |
| heal.fullTextAvailability | TRUE | - |
| heal.identifier.secondary | <Go to ISI>://000073767400034 | - |
| heal.journalName | Physical Review D | en |
| heal.journalType | peer reviewed | - |
| heal.language | en | - |
| heal.publicationDate | 1998 | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.type | journalArticle | - |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.type.en | Journal article | en |
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