Quantum Horizons
| dc.creator | Bai, Hua | |
| dc.creator | Yan, Mu-Lin | |
| dc.date | 2004-03-15 | |
| dc.date | 2005-02-11 | |
| dc.date.accessioned | 2026-07-07T03:28:32Z | |
| dc.date.available | 2026-07-07T03:28:32Z | |
| dc.description | 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. | |
| dc.description | 7 pages, No figures, LaTeX file | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0403064 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0403064 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34869 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Quantum Horizons | |
| dc.type | text |