Add to ORKGThe classical first law of thermodynamic for Kerr-Newmann black hole (KNBH) is generalized to that in quantum form on event horizon. Then four quantum conservation laws on the KNBH equilibrium radiation process are derived, and Bekenstein-Hawking's relation S=A/4 is recovered. It can be argued that the classical entropy of black hole arise from the quantum entropy of field quanta or quasi-particles inside the hole
The quantum entropy of the Kerr black hole arising from gravitational perturbation is investigated b...
One of the biggest puzzles in physics today is the reconciliation of quantum mechanics and general r...
This paper comprehensively explores Stephen Hawking’s interaction with Jacob Bekenstein. Both Hawkin...
The classical first law of thermodynamics for a Kerr-Newman black hole (KNBH) is generalized to a la...
We show that essentially pure classical thermodynamics is sufficient to determine Bekenstein's formu...
In the present paper we consider, using our earlier results, the process of quantum gravitational co...
We review the present status of black hole thermodynamics. Our review includes discussion of classic...
We propose a simple procedure for evaluating the main attributes of a Schwarzschild's black hole: Be...
The thermal properties of black holes in the presence of quantum fields can be revealed through solu...
Almost all of the entropy in the universe is in the form of Bekenstein-Hawking (BH) entropy of supe...
Taking the horizon surface of the black hole as a compact membrane and solving the oscillation equat...
Black holes are an important area of research for theoretical physics as the behavior of the strong ...
We discuss the statistical-mechanical entropy of black hole calculated according to 't Hooft. It is ...
Black holes are an important area of research for theoretical physics as the behavior of the strong ...
A brief review of Hawking radiation and black hole thermodynamics is given, based largely upon hep-t...
The quantum entropy of the Kerr black hole arising from gravitational perturbation is investigated b...
One of the biggest puzzles in physics today is the reconciliation of quantum mechanics and general r...
This paper comprehensively explores Stephen Hawking’s interaction with Jacob Bekenstein. Both Hawkin...
The classical first law of thermodynamics for a Kerr-Newman black hole (KNBH) is generalized to a la...
We show that essentially pure classical thermodynamics is sufficient to determine Bekenstein's formu...
In the present paper we consider, using our earlier results, the process of quantum gravitational co...
We review the present status of black hole thermodynamics. Our review includes discussion of classic...
We propose a simple procedure for evaluating the main attributes of a Schwarzschild's black hole: Be...
The thermal properties of black holes in the presence of quantum fields can be revealed through solu...
Almost all of the entropy in the universe is in the form of Bekenstein-Hawking (BH) entropy of supe...
Taking the horizon surface of the black hole as a compact membrane and solving the oscillation equat...
Black holes are an important area of research for theoretical physics as the behavior of the strong ...
We discuss the statistical-mechanical entropy of black hole calculated according to 't Hooft. It is ...
Black holes are an important area of research for theoretical physics as the behavior of the strong ...
A brief review of Hawking radiation and black hole thermodynamics is given, based largely upon hep-t...
The quantum entropy of the Kerr black hole arising from gravitational perturbation is investigated b...
One of the biggest puzzles in physics today is the reconciliation of quantum mechanics and general r...
This paper comprehensively explores Stephen Hawking’s interaction with Jacob Bekenstein. Both Hawkin...