Details
| Originalsprache | Englisch |
|---|---|
| Aufsatznummer | 134 |
| Fachzeitschrift | JHEP |
| Jahrgang | 2017 |
| Ausgabenummer | 7 |
| Publikationsstatus | Veröffentlicht - 1 Juli 2017 |
| Extern publiziert | Ja |
Abstract
We investigate thermal activation of thin-shells around anti-de Sitter black holes. Under the thin-shell approximation, we extensively study the parameter region that allows a bubble nucleation bounded by a thin-shell out of a thermal bath. We show that in general if one fixes the temperature outside the shell, one needs to consider the presence of a conical deficit inside the shell in the Euclidean manifold, due to the lack of solutions with a smooth manifold. We show that for a given set of theoretical parameters, i.e., vacuum and shell energy density, there is a finite range of black hole masses that allow this transition. Most interestingly, one of them describes the complete evaporation of the initial black hole.
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Kern- und Hochenergiephysik
Zitieren
- Standard
- Harvard
- Apa
- Vancouver
- BibTex
- RIS
in: JHEP, Jahrgang 2017, Nr. 7, 134, 01.07.2017.
Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review
}
TY - JOUR
T1 - Thermal activation of thin-shells in anti-de Sitter black hole spacetime
AU - Domènech Fuertes, Guillem
N1 - Publisher Copyright: © 2017, The Author(s).
PY - 2017/7/1
Y1 - 2017/7/1
N2 - We investigate thermal activation of thin-shells around anti-de Sitter black holes. Under the thin-shell approximation, we extensively study the parameter region that allows a bubble nucleation bounded by a thin-shell out of a thermal bath. We show that in general if one fixes the temperature outside the shell, one needs to consider the presence of a conical deficit inside the shell in the Euclidean manifold, due to the lack of solutions with a smooth manifold. We show that for a given set of theoretical parameters, i.e., vacuum and shell energy density, there is a finite range of black hole masses that allow this transition. Most interestingly, one of them describes the complete evaporation of the initial black hole.
AB - We investigate thermal activation of thin-shells around anti-de Sitter black holes. Under the thin-shell approximation, we extensively study the parameter region that allows a bubble nucleation bounded by a thin-shell out of a thermal bath. We show that in general if one fixes the temperature outside the shell, one needs to consider the presence of a conical deficit inside the shell in the Euclidean manifold, due to the lack of solutions with a smooth manifold. We show that for a given set of theoretical parameters, i.e., vacuum and shell energy density, there is a finite range of black hole masses that allow this transition. Most interestingly, one of them describes the complete evaporation of the initial black hole.
KW - Black Holes
KW - Models of Quantum Gravity
KW - Nonperturbative Effects
KW - Thermal Field Theory
UR - http://www.scopus.com/inward/record.url?scp=85026634491&partnerID=8YFLogxK
U2 - 10.1007/JHEP07(2017)134
DO - 10.1007/JHEP07(2017)134
M3 - Article
VL - 2017
JO - JHEP
JF - JHEP
IS - 7
M1 - 134
ER -