Black hole - wormhole transitions in two dimensional string theory

被引:0
|
作者
Betzios, Panos [1 ]
Gaddam, Nava [2 ]
Papadoulaki, Olga [3 ]
机构
[1] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 1Z1, Canada
[2] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bengaluru 560089, India
[3] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada
来源
基金
英国工程与自然科学研究理事会; 加拿大自然科学与工程研究理事会;
关键词
Black Holes in String Theory; Matrix Models; Gauge-Gravity Correspondence; Long Strings; FIELD-THEORY; CALOGERO MODEL; MATRIX; SUPERSTRINGS; INSTANTONS;
D O I
10.1007/JHEP05(2024)132
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 charged black hole and wormhole solutions of Type 0A/IIA string theory in two dimensions, by analysing their low energy equations of motion at leading order in alpha ' . There is a competition between Euclidean wormholes and near extremal black holes in the thermodynamic ensemble. In a certain regime of phase space, the former can disassociate into the latter. Since such solutions are of string scale near the wormhole throat that takes an AdS2 form, there is a need for an exact worldsheet description. We discuss relevant WZW coset models which we argue will shed light on this problem. Finally, we present appropriate versions of the Type 0A/IIA matrix quantum mechanics models that are expected to describe these geometries.
引用
收藏
页数:47
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