Magnetically Charged AdS Black Holes and Joule–Thomson Expansion
S. I. Kruglov
Abstract
Open-access reader
S. I. Kruglov
Abstract
Open-access reader
The process of the Joule–Thomson adiabatic expansion within rational NED (RNED)-AdS spacetime is investigated. The isenthalpic $$P{-}T$$ diagrams and the inversion temperature are depicted. The inversion temperature depends on the magnetic charge and RNED coupling constant of black holes. When the Joule–Thomson coefficient vanishes, a cooling-heating phase transition occurs. We consider the cosmological constant as a thermodynamic pressure, and the black hole mass is treated as chemical enthalpy.
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The process of the Joule–Thomson adiabatic expansion within rational NED (RNED)-AdS spacetime is investigated. The isenthalpic $$P{-}T$$ diagrams and the inversion temperature are depicted. The inversion temperature depends on the magnetic charge and RNED coupling constant of black holes. When the Joule–Thomson coefficient vanishes, a cooling-heating phase transition occurs. We consider the cosmological constant as a thermodynamic pressure, and the black hole mass is treated as chemical enthalpy.
Key concepts: Joule–Thomson effect, AdS black hole, Adiabatic process, Inversion temperature, Physics, Joule heating, Black hole (networking), Thermodynamics