Phase transition of quantum-corrected Schwarzschild black hole

2012/07/31 by Wontae Kim, Yong‐Wan Kim, Yongwan Kim · 4 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #General relativity #Gravitation #Noncommutative and Quantum Gravity Theories #Phase transition #Physics #Quantum #Quantum electrodynamics #Quantum mechanics #Quantum phase transition #Schwarzschild metric #Schwarzschild radius #Theoretical physics #gr-qc #hep-th

paper · pdf · doi:10.1016/j.physletb.2012.11.017

published as Phys.Lett.B 718:687-691,2012 · 12 pages, 4 figures, added : version accepted for publication in PLB

arxiv created 2012/11/07 · openalex publication_date 2012/11/08 · arxiv updated 2013/02/15 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We study the thermodynamic phase transition of a quantum-corrected Schwarzschild black hole. The modified metric affects the critical temperature which is slightly less than the conventional one. The space without black holes is not the hot flat space but the hot curved space due to vacuum fluctuations so that there appears a type of Gross–Perry–Yaffe phase transition even for the very small size of black hole, which is impossible for the thermodynamics of the conventional Schwarzschild black hole. We discuss physical consequences of the new phase transition in this framework.

Citations

• Thermodynamics of black holes in anti-de Sitter space
• Particle creation by black holes
• Generalized second law of thermodynamics in black-hole physics
• Black Holes and Entropy

Cited by

• Late-Time Cosmology and Structure Formation in Quadratic f(Q) Gravity
• Two critical phenomena in the exactly soluble quantized Schwarzschild black hole
• New rotating black holes in nonlinear Maxwell f(R) gravity
• Energy and Thermodynamics of the Quantum-Corrected Schwarzschild Black Hole