New Insights on the Thermodynamic Equilibrium of Black Hole and Thermal Radiation
Ruifeng Zheng

TL;DR
This paper explores the thermodynamic equilibrium between black holes and thermal radiation, revealing that considering quantum effects leads to inevitable fluctuations, offering new insights into the microscopic origins of thermodynamic behavior.
Contribution
It introduces a simplified model of black hole and radiation equilibrium, incorporating quantum effects to explain thermodynamic fluctuations and their microscopic origins.
Findings
Thermal radiation can collapse to form black holes in equilibrium.
Quantum considerations induce inevitable thermodynamic fluctuations.
Energy conservation and second law hold when only one quantum effect is considered.
Abstract
The thermal balance between the black hole and surrounding thermal radiation is an interesting topic. The primordial black hole is a type of black hole formed in the early universe, especially during the thermal radiation period of the early universe. Driven by gravity, thermal radiation will collapse to form a black hole. Because of the complexity of the actual situation, we use the simplest model for simulation under the premise of only considering the thermodynamic properties of the system: in the classic case, an isolated box full of thermal radiation, by adjusting the initial temperature within a reasonable range, the results show that the collapse of part of the thermal radiation to form a black hole and finally achieve thermal equilibrium is an inevitable result of the second law of thermodynamics. We then introduced the quantization of black holes and the number of microscopic…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Astrophysical Phenomena and Observations
