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Thermodynamics

New Physics Findings from Department of Physics Published: Thermodynamic Properties of Schwarzschild Black Hole

Strategic Insights

— 2 min read

Physicists have made significant research findings in the field of thermodynamics, specifically focusing on the Schwarzschild black hole embedded in an anti-de Sitter background. This study, conducted by researchers from the Department of Physics, explores the thermodynamic properties of the black hole, including its mass, pressure, and specific heat capacity. The research also examines the effects of external parameters, such as the string cloud and quintessence-like fluid, on the thermal response of the black hole. Furthermore, the study investigates the Joule-Thomson expansion process and its relation to the thermodynamic behavior of the black hole.

Key Takeaways:

  • The researchers derived key thermodynamic quantities, including Gibbs free energy and internal energy, to characterize the energetic behavior of the black hole system.
  • The study found that the geometric and matter fields significantly modify the thermal response of the black hole, affecting its stability and behavior.
  • The researchers computed the specific heat capacity and analyzed its influence on the thermal behavior of the black hole.
  • The study demonstrated the Joule-Thomson expansion process and showed how the external parameters affect the thermodynamic phenomenon, highlighting important aspects of black hole cooling and heating behavior.
  • The research included a comprehensive analysis of the inversion temperature associated with the black hole, distinguishing it from the standard Hawking temperature.
  • The study concluded that the external parameters, such as the string cloud and quintessence-like fluid, play a crucial role in modifying the thermodynamic behavior of the black hole.
  • The researchers identified the importance of extended phase space thermodynamics in understanding the thermodynamic properties of the Schwarzschild black hole.

Statistics:

  • The Schwarzschild black hole has a mass that is formulated in terms of the event horizon radius (Thermodynamics and Joule-Thomson expansion of Schwarzschild-AdS black holes with a cloud of strings and quintessential-like fluid, 2025, 85(10): 1-17).
  • The internal energy of the black hole system is characterized by the Gibbs free energy and internal energy (Thermodynamics and Joule-Thomson expansion of Schwarzschild-AdS black holes with a cloud of strings and quintessential-like fluid, 2025, 85(10): 1-17).
  • The specific heat capacity of the black hole is computed and analyzed to assess its influence on the thermal behavior of the black hole (Thermodynamics and Joule-Thomson expansion of Schwarzschild-AdS black holes with a cloud of strings and quintessential-like fluid, 2025, 85(10): 1-17).

Sources:

  • Thermodynamics and Joule-Thomson expansion of Schwarzschild-AdS black holes with a cloud of strings and quintessential-like fluid. European Physical Journal C: Particles and Fields, 2025, 85(10): 1-17.
  • Department of Physics, Assam Royal Global University.
  • European Physical Journal C: Particles and Fields, SpringerOpen.

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