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• W2080821449 startingPage "824" @default.
• W2080821449 abstract "The one-loop quantum corrections to geometry and thermodynamics of black hole are studied for the two-dimensional RST model. We chose boundary conditions corresponding to the eternal black hole being in the thermal equilibrium with the Hawking radiation. The equations of motion are exactly integrated. The one of the solutions obtained is the constant curvature space-time with dilaton being a constant function. Such a solution is absent in the classical theory. On the other hand, we derive the quantum-corrected metric (ref{solution}) written in the Schwarzschild like form which is a deformation of the classical black hole solution cite{5d}. The space-time singularity occurs to be milder than in classics and the solution admits two asymptotically flat black hole space-times lying at different sides of the singularity. The thermodynamics of the classical black hole and its quantum counterpart is formulated. The thermodynamical quantities (energy, temperature, entropy) are calculated and occur to be the same for both the classical and quantum-corrected black holes. So, no quantum corrections to thermodynamics are observed. The possible relevance of the results obtained to the four-dimensional case is discussed." @default.
• W2080821449 created "2016-06-24" @default.
• W2080821449 creator A5064383464 @default.
• W2080821449 date "1996-01-15" @default.
• W2080821449 modified "2023-10-16" @default.
• W2080821449 title "Two-dimensional quantum-corrected eternal black hole" @default.
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• W2080821449 doi "https://doi.org/10.1103/physrevd.53.824" @default.
• W2080821449 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/10020066" @default.
• W2080821449 hasPublicationYear "1996" @default.
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