Quantization of the black hole area as quantization of the angular momentum component

Kostyantyn Ropotenko

Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2009 · 58 citations · 13 references

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Abstract

In transforming from Schwarzschild to Euclidean Rindler coordinates the Schwarzschild time transforms to a periodic angle. As is well-known, this allows one to introduce the Hawking temperature and is an origin of black hole thermodynamics. On the other hand, according to quantum mechanics this angle is conjugate to the $z$ component of the angular momentum. From the commutation relation and quantization condition for the angular momentum component it is found that the area of the horizon of a Schwarzschild black hole is quantized with the quantum $\ensuremath{\Delta}A=8\ensuremath{\pi}{l}_{P}^{2}$. It is shown that this conclusion is also valid for a generic Kerr-Newman black hole.

References

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