Stability of topological solitons, and black string to bubble transition

被引:16
作者
Bah, Ibrahima [1 ,2 ]
Dey, Anindya [1 ]
Heidmann, Pierre [1 ]
机构
[1] Johns Hopkins Univ, Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA
[2] Inst Adv Study, 1 Einstein Dr, Princeton, NJ 08540 USA
关键词
Black Holes; Classical Theories of Gravity; Models of Quantum Gravity; GRAVITATIONAL-FIELD; HOLE; INSTABILITY; THERMODYNAMICS;
D O I
10.1007/JHEP04(2022)168
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We study the existence of smooth topological solitons and black strings as locally-stable saddles of the Euclidean gravitational action of five dimensional Einstein-Maxwell theory. These objects live in the Kaluza-Klein background of four dimensional Minkowski with an S-1. We compute the off-shell gravitational action in the canonical ensemble with fixed boundary data corresponding to the asymptotic radius of S-1, and to the electric and magnetic charges that label the solitons and black strings. We show that these objects are locally-stable in large sectors of the phase space with varying lifetime. Furthermore, we determine the globally-stable phases for different regimes of the boundary data, and show that there can be Hawking-Page transitions between the locally-stable phases of the topological solitons and black strings. This analysis demonstrates the existence of a large family of globally-stable smooth solitonic objects in gravity beyond supersymmetry, and presents a mechanism through which they can arise from the black strings.
引用
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页数:34
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