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Электронный каталог: Avramov, V. - On Thermodynamic Stability of Black Holes. Part. I: Classical Stability
Avramov, V. - On Thermodynamic Stability of Black Holes. Part. I: Classical Stability
Статья
Автор: Avramov, V.
The European Physical Journal C [Electronic resource]: On Thermodynamic Stability of Black Holes. Part. I: Classical Stability
б.г.
ISBN отсутствует
Автор: Avramov, V.
The European Physical Journal C [Electronic resource]: On Thermodynamic Stability of Black Holes. Part. I: Classical Stability
б.г.
ISBN отсутствует
Статья
Avramov, V.
On Thermodynamic Stability of Black Holes. Part. I: Classical Stability / V.Avramov, H.Dimov, [a.o.] // The European Physical Journal C [Electronic resource]. – 2024. – Vol. 84, No. 3. – P. 281. – URL: https://doi.org/10.1140/epjc/s10052-024-12639-3. – Bibliogr.: 53.
We revisit the classical thermodynamic stability of the standard black hole solutions by implementing the intrinsic necessary and sufficient conditions for stable global and local thermodynamic equilibrium. The criteria for such equilibria are quite generic and well-established in classical thermodynamics, but they have not been fully utilized in black hole physics. We show how weaker or incomplete conditions could lead to misleading or incorrect results for the thermodynamic stability of the system. We also stress the importance of finding all possible local heat capacities in order to fully describe the classical equilibrium picture of black holes. Finally, we thoroughly investigate the critical and phase transition curves and the limits of the classical analysis. This paper is the first in the line of intended works on thermodynamic stability of black holes in modified theories of gravity and holography.
ОИЯИ = ОИЯИ (JINR)2024
Спец.(статьи,препринты) = С 322.2 - Космология. Гравитационные волны
Бюллетени = 25/024
Avramov, V.
On Thermodynamic Stability of Black Holes. Part. I: Classical Stability / V.Avramov, H.Dimov, [a.o.] // The European Physical Journal C [Electronic resource]. – 2024. – Vol. 84, No. 3. – P. 281. – URL: https://doi.org/10.1140/epjc/s10052-024-12639-3. – Bibliogr.: 53.
We revisit the classical thermodynamic stability of the standard black hole solutions by implementing the intrinsic necessary and sufficient conditions for stable global and local thermodynamic equilibrium. The criteria for such equilibria are quite generic and well-established in classical thermodynamics, but they have not been fully utilized in black hole physics. We show how weaker or incomplete conditions could lead to misleading or incorrect results for the thermodynamic stability of the system. We also stress the importance of finding all possible local heat capacities in order to fully describe the classical equilibrium picture of black holes. Finally, we thoroughly investigate the critical and phase transition curves and the limits of the classical analysis. This paper is the first in the line of intended works on thermodynamic stability of black holes in modified theories of gravity and holography.
ОИЯИ = ОИЯИ (JINR)2024
Спец.(статьи,препринты) = С 322.2 - Космология. Гравитационные волны
Бюллетени = 25/024