Details
| Original language | English |
|---|---|
| Article number | 134 |
| Journal | JHEP |
| Volume | 2017 |
| Issue number | 7 |
| Publication status | Published - 1 Jul 2017 |
| Externally published | Yes |
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.
Keywords
- Black Holes, Models of Quantum Gravity, Nonperturbative Effects, Thermal Field Theory
ASJC Scopus subject areas
- Physics and Astronomy(all)
- Nuclear and High Energy Physics
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In: JHEP, Vol. 2017, No. 7, 134, 01.07.2017.
Research output: Contribution to journal › Article › Research › 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 -