Page Curve for Eternal Schwarzschild Black Hole in Dimensionally-Reduced Model of Dilaton Gravity
arXiv:2207.07409 · doi:10.1103/PhysRevD.106.105015
Abstract
As a contribution to the subject of the information loss paradox in (1+1)-dimensional gravitational systems, we study a model of (1+1)-dimensional dilaton gravity derived from the four-dimensional Einstein-Hilbert action by dimensional reduction. The reduced action involves the cosmological constant and admits black hole solutions. After including the back-reaction of quantum fields to 1-loop order, we solve the semi-classical field equations perturbatively and compute the quantum correction to the Hawking temperature. We consider the quantum extremal surface approach and invoke the ``island rule'' to compute the fine-grained entropy of the Hawking radiation for an eternal Schwarzschild black hole and demonstrate that it follows the unitary Page curve.
11 pages, 4 figures
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Cited by in corpus (6)
- Cosmological and black hole islands in multi-event horizon spacetimes
- Islands in Non-Minimal Dilaton Gravity: Exploring Effective Theories for Black Hole Evaporation
- Island of Reissner-Nordstrm anti-de Sitter black holes in the large limit
- Infrared Regularization and Finite Size Dynamics of Entanglement Entropy in Schwarzschild Black Hole
- Investigating the role of mutual information in the Page curve for a functional renormalization group improved Schwarzschild black hole
- New insights on mutual information in the island approach to the Page curve