Three-Dimensional Quantum Black Holes: A Primer

We review constructions of three-dimensional ‘quantum’ black holes. Such spacetimes arise via holographic braneworlds and are exact solutions to an induced higher-derivative theory of gravity consistently coupled to a large-<i>c</i> quantum field theory with an ultraviolet cutoff, accoun...

وصف كامل

التفاصيل البيبلوغرافية
الحاوية / القاعدة:Universe
المؤلفون الرئيسيون: Emanuele Panella, Juan F. Pedraza, Andrew Svesko
التنسيق: مقال
اللغة:الإنجليزية
منشور في: MDPI AG 2024-09-01
الموضوعات:
black holes
semi-classical gravity
AdS/CFT
gravitational holography
braneworlds
الوصول للمادة أونلاين:https://www.mdpi.com/2218-1997/10/9/358
الوصف
الملخص:We review constructions of three-dimensional ‘quantum’ black holes. Such spacetimes arise via holographic braneworlds and are exact solutions to an induced higher-derivative theory of gravity consistently coupled to a large-<i>c</i> quantum field theory with an ultraviolet cutoff, accounting for all orders of semi-classical backreaction. Notably, such quantum-corrected black holes are much larger than the Planck length. We describe the geometry and horizon thermodynamics of a host of asymptotically (anti-) de Sitter and flat quantum black holes. A summary of higher-dimensional extensions is given. We survey multiple applications of quantum black holes and braneworld holography.
تدمد:2218-1997

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