期刊
JOURNAL OF HIGH ENERGY PHYSICS
卷 -, 期 2, 页码 -出版社
SPRINGER
DOI: 10.1007/JHEP02(2022)090
关键词
AdS-CFT Correspondence; Black Holes; Spacetime Singularities
资金
- ERC [GravBHs-692951]
- MICINN [PID2019-105614GB-C22]
- AGAUR [2017SGR 754]
- State Research Agency of MICINN through the Unit of Excellence Maria de Maeztu [CEX2019-000918-M]
- JSPS KAKENHI [JP18K13541]
- Osaka City University Advanced Mathematical Institute (MEXT Joint Usage/Research Center on Mathematics and Theoretical Physics)
- European Research Council (ERC) under the European Union [852386]
- Minerva Fellowship of the Minerva Stiftung Gesellschaft fuer die Forschung mbH
- European Research Council (ERC) [852386] Funding Source: European Research Council (ERC)
We study the evolution of the Gregory-Laflamme instability for black strings in global AdS spacetime, and investigate the CFT dual of the formation of a bulk naked singularity. Using an effective theory in the large D limit, we uncover a rich variety of dynamical behaviour, depending on the thickness of the string and on initial perturbations. These include large inflows of horizon generators from the asymptotic boundary (a 'black tsunami'), a pinch-off of the horizon that likely reveals a naked singularity, and competition between these two behaviours, such as a nakedly singular pinch-off that subsequently gets covered by a black tsunami.
We study the evolution of the Gregory-Laflamme instability for black strings in global AdS spacetime, and investigate the CFT dual of the formation of a bulk naked singularity. Using an effective theory in the large D limit, we uncover a rich variety of dynamical behaviour, depending on the thickness of the string and on initial perturbations. These include: large inflows of horizon generators from the asymptotic boundary (a 'black tsunami'); a pinch-off of the horizon that likely reveals a naked singularity; and competition between these two behaviours, such as a nakedly singular pinch-off that subsequently gets covered by a black tsunami. The holographic dual describes different patterns of heat flow due to the Hawking radiation of two black holes placed at the antipodes of a spherical universe. We also present a model that describes, in any D, the burst in the holographic stress-energy tensor when the signal from a bulk self-similar naked singularity reaches the boundary. The model shows that the shear components of the boundary stress diverge in finite time, while the energy density and pressures from the burst vanish.
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