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Journal ArticleDOI

On the third quantization of general relativity

Y. Peleg
- 05 May 1991 - 
- Vol. 8, Iss: 5, pp 827-842
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TLDR
In this paper, the authors studied the possibility of defining a Hilbert space for n=(d+1)-dimensional general relativity in some asymptotic regions of Wheeler's superspace.
Abstract
The author studies the possibility of defining a Hilbert space for n=(d+1)-dimensional general relativity in some asymptotic regions of Wheeler's superspace. The author distinguishes two asymptotic regions: (i) the 'classical asymptotic region', which contains geometries with a volume much larger than the Planck volume and (ii) the 'quantum asymptotic region', which contains geometries with a volume much smaller than the Planck volume. It is shown that for n>or=4 one can define a Hilbert space only in the classical asymptotic region of superspace, while for n(4 one can define a Hilbert space in the quantum asymptotic region or in the classical asymptotic region, but not both. It is argued that in a good theory of quantum gravity one should be able to define a Hilbert space in the two asymptotic regions. Therefore it seems that Einstein's general relativity is not a good candidate for a quantum theory of gravitation. But it (the 3+1)-dimensional case) can be a good classical limit of that theory. The above criterion can serve in the search for a quantum theory of gravitation.

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Citations
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Operator Ordering and the Flatness of the Universe

TL;DR: In this paper, the Laplacian operator on superspace is defined and the probability of finding the 3-metric and matter field configuration in a given region of superspace was shown to be bounded by the proper time that the solutions spend in that region.
Journal ArticleDOI

Some aspects of virtual black holes

TL;DR: The area and hence the entropy of a real macroscopic black hole is quantized in this model, which gives an intrinsic entropy to all physical systems that can be used to define a direction of time and hence provide a solution to the problem of time.
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Third Quantization and Quantum Universes

TL;DR: In this paper, the third quantization of the Friedmann-Robertson-Walker cosmology with N-minimal massless fields was studied in the minisuperspace, and a pair of invariant operators for each universe with conserved momenta of the fields that play a role of the annihilation and the creation operators and construct various quantum states for the universe.
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Discreteness of time in the evolution of the universe

TL;DR: In this paper, a deformed version of the Wheeler-DeWitt equation for the generalized geometry which occurs in M-theory was derived and analyzed in the minisuperspace approximation.
References
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Journal ArticleDOI

Quantum Theory of Gravity. I. The Canonical Theory

TL;DR: In this article, a 6-dimensional hyperbolic Riemannian manifold is introduced, which takes for its metric the coefficient of the momenta in the Hamiltonian constraint and the geodesic incompletability of this manifold, owing to the existence of a frontier of infinite curvature, is demonstrated.
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(2+1)-Dimensional Gravity as an Exactly Soluble System

TL;DR: By disentangling the hamiltonian constraint equations, 2 + 1 dimensional gravity (with or without a cosmological constant) is shown to be exactly soluble at the classical and quantum levels.

Quantum Theory of Gravity. I. The Canonical Theory

TL;DR: In this article, a 6-dimensional hyperbolic Riemannian manifold is introduced, which takes for its metric the coefficient of the momenta in the Hamiltonian constraint and the geodesic incompletability of this manifold, owing to the existence of a frontier of infinite curvature, is demonstrated.
Journal ArticleDOI

Gravitation and hamiltonian structure in two spacetime dimensions

TL;DR: In this article, a non-trivial analog of gravitation theory in two dimensional spacetime is built upon this fact, with the inverse of the central charge playing the role of the gravitational constant.