On Quantum Nature of Black-Hole Spacetime: A Possible New Source of Intense Radiation
arXiv:astro-ph/9909192 · doi:10.1142/S0218271899000456
Abstract
Atoms and the planets acquire their stability from the quantum mechanical incompatibility of the position and momentum measurements. This incompatibility is expressed by the fundamental commutator [x, p_x]=i hbar, or equivalently, via the Heisenberg's uncertainty principle Delta x Delta p_x sim hbar. A further stability-related phenomenon where the quantum realm plays a dramatic role is the collapse of certain stars into white dwarfs and neutron stars. Here, an intervention of the Pauli exclusion principle, via the fermionic degenerate pressure, stops the gravitational collapse. However, by the neutron-star stage the standard quantum realm runs dry. One is left with the problematic collapse of a black hole. This essay is devoted to a concrete argument on why the black-hole spacetime itself should exhibit a quantum nature. The proposed quantum aspect of spacetime is shown to prevent the general-relativistic dictated problematic collapse. The quantum nature of black-hole spacetime is deciphered from a recent result on the universal equal-area spacing [=lambda_P^2 4 ln(3)] for black holes. In one interpretation of the emergent picture, an astrophysical black hole can fluctuate to sqrt{pi/ln(3)} approx 1.7 times its classical size, and thus allow radiation and matter to escape to the outside observers. These fluctuations I conjecture provide a new source, perhaps beyond Hawking radiation, of intense radiation from astrophysical black holes and may be the primary source of observed radiation from those galactic cores what carry black hole(s). The presented interpretation may be used as a criterion to choose black holes from black hole candidates.
This essay received an "honorable mention" in the 1999 Essay Competition of the Gravity Research Foundation - Ed. Int. J. Mod. Phys. D (1999, in press). For Joseph Knecht
References in corpus (5)
Cited by in corpus (10)
- Quantum-mechanical model of the Kerr-Newman black hole
- A Spacetime Foam approach to the cosmological constant and entropy
- Comparing two approaches to Hawking radiation of Schwarzschild-de Sitter black holes
- Equation of State of the Transplanckian Dark Energy and the Coincidence Problem
- Discrete Black-Hole Radiation and the Information Loss Paradox
- A Spacetime Foam Approach to the Schwarzschild-de Sitter Entropy
- The quantum emission spectra of rapidly-rotating Kerr black holes: discrete or continuous?
- Entropy from the foam II
- What Casimir Energy can suggest about Space Time Foam?
- Natural broadening in the quantum emission spectra of higher-dimensional Schwarzschild black holes