Holographic complexity: stretching the horizon of an evaporating black hole
| Autor: | Lukas Schneiderbauer, Larus Thorlacius, Watse Sybesma |
|---|---|
| Přispěvatelé: | Raunvísindastofnun (HÍ), Science Institute (UI), Verkfræði- og náttúruvísindasvið (HÍ), School of Engineering and Natural Sciences (UI), Háskóli Íslands, University of Iceland |
| Jazyk: | angličtina |
| Rok vydání: | 2020 |
| Předmět: |
High Energy Physics - Theory
Nuclear and High Energy Physics Gravity (chemistry) Black Holes Astrophysics::High Energy Astrophysical Phenomena Holography FOS: Physical sciences General Relativity and Quantum Cosmology (gr-qc) 01 natural sciences General Relativity and Quantum Cosmology 010305 fluids & plasmas law.invention RST model law 0103 physical sciences Þyngdarafl lcsh:Nuclear and particle physics. Atomic energy. Radioactivity 010306 general physics Early onset Physics Horizon Mechanics Black hole High Energy Physics - Theory (hep-th) lcsh:QC770-798 Dilaton Svarthol (stjörnufræði) Classical Theories of Gravity 2D Gravity Rate of growth |
| Zdroj: | Journal of High Energy Physics Journal of High Energy Physics, Vol 2020, Iss 3, Pp 1-16 (2020) |
| Popis: | Publisher's version (útgefin grein) We obtain the holographic complexity of an evaporating black hole in the semi-classical RST model of two-dimensional dilaton gravity, using a volume prescription that takes into account the higher-dimensional origin of the model. For classical black holes, we recover the expected late time behaviour of the complexity, but new features arise at the semi-classical level. By considering the volume inside the stretched horizon of the evolving black hole, we obtain sensible results for the rate of growth of the complexity, with an early onset of order the black hole scrambling time followed by an extended period where the rate of growth tracks the shrinking area of the stretched horizon as the black hole evaporates. |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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