Reentrant phase transitions of quantum black holes

被引:9
|
作者
Frassino, Antonia M. [1 ,2 ]
Pedraza, Juan F. [3 ]
Svesko, Andrew [4 ,5 ]
Visser, Manus R. [6 ]
机构
[1] Univ Alcala, Campus Univ, Dept Fis & Matemat, Alcala De Henares 28805, Madrid, Spain
[2] Univ Barcelona, Inst Ciencies Cosmos, Dept Fis Quant & Astrofis, Barcelona 08028, Spain
[3] CSIC, Inst Fis Teor UAM, Calle Nicolas Cabrera 13-15, Madrid 28049, Spain
[4] UCL, Dept Phys & Astron, London WC1E 6BT, England
[5] Kings Coll London, Dept Math, London WC2R 2LS, England
[6] Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 0WA, England
基金
英国工程与自然科学研究理事会; 瑞士国家科学基金会;
关键词
THERMODYNAMICS; GRAVITY;
D O I
10.1103/PhysRevD.109.124040
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that backreaction of quantum fields on black hole geometries can trigger new thermal phase transitions. Specifically, we study the phase behavior of the three-dimensional quantum-corrected static Ba & ntilde;ados-Teitelboim-Zanelli black hole, an exact solution to specific semiclassical gravitational equations due to quantum conformal matter, discovered through braneworld holography. Focusing on the canonical ensemble, for large backreaction, we find novel reentrant phase transitions as the temperature monotonically increases, namely, from thermal anti-de Sitter space to the black hole and back to thermal anti-de Sitter. The former phase transition is first-order, a quantum analog of the classical Hawking-Page phase transition, while the latter is zeroth order and has no classical counterpart.
引用
收藏
页数:7
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