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Электронный каталог: Avramov, V. - Black Holes and Thermogeometric Optimization
Avramov, V. - Black Holes and Thermogeometric Optimization

Статья
Автор: Avramov, V.
The European Physical Journal C: Black Holes and Thermogeometric Optimization
б.г.
ISBN отсутствует
Автор: Avramov, V.
The European Physical Journal C: Black Holes and Thermogeometric Optimization
б.г.
ISBN отсутствует
Статья
Avramov, V.
Black Holes and Thermogeometric Optimization / V.Avramov, H.Dimov, [a.o.]. – Text : electronic // The European Physical Journal C. – 2025. – Vol. 85, No. 5. – P. 587. – URL: https://doi.org/10.1140/epjc/s10052-025-14303-w. – Bibliogr.: 93.
We suggest a finite-time geometric optimization framework to analyze thermal fluctuations and optimal processes in black holes. Our approach implement geodesics in thermodynamic space to define optimal pathways between equilibrium and non-equilibrium states. Since thermodynamic metrics need not be positive-definite, the method ensures a positive thermodynamic length by incorporating simple scale factor into the metric. We show that the thermodynamic length and the scale factor are sensitive to phase transitions in entropy representation, addressing a key gap in Hessian thermodynamic geometry. Additionally, we link the scale factor to the sign of thermodynamic curvature, connecting it to the information geometry governing optimal processes. Our results indicate that optimal fluctuations can drive the evaporation of Schwarzschild and Kerr black holes, which may significantly differ from Hawking radiation. We also explore optimal accretion-driven processes supported by an external inflow of energy.
ОИЯИ = ОИЯИ (JINR)2025
Спец.(статьи,препринты) = С 322.2 - Космология. Гравитационные волны
Бюллетени = 29/025
Avramov, V.
Black Holes and Thermogeometric Optimization / V.Avramov, H.Dimov, [a.o.]. – Text : electronic // The European Physical Journal C. – 2025. – Vol. 85, No. 5. – P. 587. – URL: https://doi.org/10.1140/epjc/s10052-025-14303-w. – Bibliogr.: 93.
We suggest a finite-time geometric optimization framework to analyze thermal fluctuations and optimal processes in black holes. Our approach implement geodesics in thermodynamic space to define optimal pathways between equilibrium and non-equilibrium states. Since thermodynamic metrics need not be positive-definite, the method ensures a positive thermodynamic length by incorporating simple scale factor into the metric. We show that the thermodynamic length and the scale factor are sensitive to phase transitions in entropy representation, addressing a key gap in Hessian thermodynamic geometry. Additionally, we link the scale factor to the sign of thermodynamic curvature, connecting it to the information geometry governing optimal processes. Our results indicate that optimal fluctuations can drive the evaporation of Schwarzschild and Kerr black holes, which may significantly differ from Hawking radiation. We also explore optimal accretion-driven processes supported by an external inflow of energy.
ОИЯИ = ОИЯИ (JINR)2025
Спец.(статьи,препринты) = С 322.2 - Космология. Гравитационные волны
Бюллетени = 29/025