Singularities in 2D and 3D quantum black holes

被引:4
|
作者
Kolanowski, Maciej [1 ,2 ]
Tomasevic, Marija [3 ,4 ]
机构
[1] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
[2] Univ Warsaw, Inst Theoret Phys, Fac Phys, Pasteura 5, PL-02093 Warsaw, Poland
[3] Inst Polytech Paris, Ecole Polytech, CPHT, CNRS, F-91120 Palaiseau, France
[4] Univ Amsterdam, Inst Theoret Phys, Sci Pk 904, NL-1090 GL Amsterdam, Netherlands
基金
欧洲研究理事会;
关键词
2D Gravity; Black Holes; Spacetime Singularities; MASS-INFLATION; FIELD THEORY; SPACETIME;
D O I
10.1007/JHEP12(2023)102
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 black holes in two and three dimensions that have spacelike curvature singularities behind horizons. The 2D solutions are obtained by dimensionally reducing certain 3D black holes, known as quantum BTZ solutions. Furthermore, we identify the corresponding dilaton potential and show how it can arise from a higher-dimensional theory. Finally, we show that the rotating BTZ black hole develops a singular inner horizon once quantum effects are properly accounted for, thereby solidifying strong cosmic censorship for all known cases.
引用
收藏
页数:45
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