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arXiv · gr-qc/0403064

Quantum Horizons

Abstract

Treating macro-black hole as quantum states, and using Brown-York quaselocal gravitational energy definition and Heisenberg uncertainty principle, we find out the classical horizon with singularity spreads into a quantum horizon in which the space-time is non-commutative and the spread range is determined dynamically. A Quantum Field Theory (QFT) model in curved space with quantum horizon is constructed. By using it, the black hole entropy and the Hawking temperature are calculated successfully. The $ϕ-$field mode number is predicted and our quantum horizon model favors to support the Minimal Super-symmetric Standard Model.

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BibTeXRIS

Hua Bai, Mu-Lin Yan. 2005-02-11. Quantum Horizons. https://arxiv.org/abs/gr-qc/0403064

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