Bohr's Correspondence Principle and The Area Spectrum of Quantum Black Holes
arXiv:gr-qc/9812002 · doi:10.1103/PhysRevLett.81.4293
Abstract
During the last twenty-five years evidence has been mounting that a black-hole surface area has a {\it discrete} spectrum. Moreover, it is widely believed that area eigenvalues are {\it uniformally} spaced. There is, however, no general agreement on the {\it spacing} of the levels. In this letter we use Bohr's correspondence principle to provide this missing link. We conclude that the area spacing of a black-hole is . This is the unique spacing consistent both with the area-entropy {\it thermodynamic} relation for black holes, with Boltzmann-Einstein formula in {\it statistical physics} and with {\it Bohr's correspondence principle}.
10 pages
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- Schwarzschild-AdS Black Holes with Cloud of Strings and Quintessence: Geodesics, Thermodynamic Topology, and Quasinormal Modes
- Initiating the effective unification of black hole horizon area and entropy quantization with quasi-normal modes
- Stimulated Hawking effect and quasinormal mode resonance in a polariton simulator of field theory on curved spacetime
- Entropy Spectrum of a Carged Black Hole of Heterotic String Theory via Adiabatic Invariance
- Thermodynamics and Quasinormal modes of Park black hole in Hořava gravity
- Testing the Quantum of Entropy
- Spectroscopy of Stringy Black Hole
- Scalar filed evolution and area spectrum for Lovelock-AdS black holes
- Much ado about nothing: a treatise on empty and not-so-empty spacetimes
- Spectroscopy of an AdS Reissner-Nordstrom black hole
- On the degrees of freedom of a black hole
- The Dirac equation in D-dimensional spherically symmetric spacetimes
- Varying Fine Structure Constant and Black Hole Physics
- Scalar Clouds and Quasinormal Modes
- Universality of Highly Damped Quasinormal Modes for Single Horizon Black Holes
- Quantization of horizon entropy and the thermodynamics of spacetime
- An approach to the quantization of black-hole quasi-normal modes
- Area spectrum of extremal black holes with warped AdS near-horizon geometry
- Natural broadening in the quantum emission spectra of higher-dimensional Schwarzschild black holes
- Asymptotic quasinormal frequencies of different spin fields in -dimensional spherically-symmetric black holes
- Horizon quantum geometries and decoherence
- Effects of quantum geometry on the decoherence induced by black holes
- Condensation of area quanta ensembles with quantum statistics in Schwarzschild spacetimes
- Quasinormal modes of a dyonic black hole in Einstein-Euler-Heisenberg theory
- Quasinormal frequencies of the dimensionally reduced BTZ black hole
- Quantization of Black Holes in the Shielded Strong Gravity Scenario (I. Neutral Scalar States)
- Second Order Perturbative Calculation of Quasinormal Modes of Schwarzschild Black Holes
- WKB Approximation for a Deformed Schrodinger-like Equation and its Applications to Quasinormal Modes of Black Holes and Quantum Cosmology
- Classical analog of quantum Schwarzschild black hole: local vs global, and the mystery of log(3)
- Holographic bound in covariant loop quantum gravity
- Signature of Non-uniform Area Quantization on Gravitational Waves
- Quasinormal modes of Bonanno-Reuter black holes via the Spectral Method
- Quasinormal-mode analysis of a massive scalar field in a Schwarzschild background via the spectral method
- Spectral instability of parametrized black hole quasinormal modes in the high-overtone limit via the exact WKB analysis
- A Scenario for Strong Gravity in Particle Physics: An alternative mechanism for black holes to appear at accelerator experiments
- Analysis of spherically symmetric black holes in Braneworld models
- Gravitational Bound State Perturbations Inside Black Holes and Isospectrality
- Probing the Purely Ingoing Nature of the Black-hole Event Horizon
- Hawking Radiation from Boundary Scalar Field
- On black hole spectroscopy via quantum tunneling
- A note on the fuzzy sphere area spectrum, black hole luminosity, and the quantum nature of spacetime