Cited by 89Noncommutative and Quantum Gravity TheoriesRelativity and Gravitational TheoryBlack Holes and Theoretical Physics

Large Quantum Gravity Effects: Unforeseen Limitations of the Classical Theory

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Ashtekar, Abhay·1996·Physical Review Letters

Abstract

Three-dimensional gravity coupled to Maxwell (or Klein-Gordon) fields is exactly soluble under the assumption of axisymmetry. The solution is used to probe several quantum gravity issues. In particular, it is found that if there is an electromagnetic wave of Planckian frequency even with such low amplitude that the curvature of the classical solution is small, the uncertainty in the quantum metric can be very large. More generally, the quantum fluctuations in the geometry are large unless the number and frequency of photons satisfy the inequality $N(\ensuremath{\Elzxh}G\ensuremath{\omega}{)}^{2}\ensuremath{\ll}1$. Results hold also for a sector of the four-dimensional theory (consisting of Einstein-Rosen gravitational waves).

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  • There is evidence that the matter Hamiltonian is bounded above in (2+1)-dimensional gravity.

    “For example, there is evidence that the matter Hamiltonian is bounded above in (2 + 1)-dimensional gravity [27]; perhaps this could cut off radiative contributions to the cosmological constant at an interesting scale.”

    From Quantum Gravity in 2 + 1 Dimensions: The Case of a Closed Universe (2005) · cites this paper as [27]

    In section I (p. 3), the paper says the bounded quantity is the total Hamiltonian of the system, explicitly including gravity. Section I (p. 4) distinguishes that Hamiltonian from H₀, the scalar-field energy, so the cited result does not establish an upper bound on the matter Hamiltonian. (LLM, conf=0.84)

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  • Work on circularly symmetric midi-superspace models has led to unexpected bounds on the Hamiltonian.

    “Certain matter couplings in supergravity have been studied [104, 196], and work on circularly symmetric “midi-superspace models” has led to some surprising results, including unexpected bounds on the Hamiltonian [27, 32, 137, 53, 265, 224].”

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Research works printed but not linked: 3

  1. [3][3] L. Susskind, J. Math. Phys. 36 , 6397 (1995); G. 't Hooft, Class. Quantum Grav. 11 , 621 (1994); C. Thorne, in Sakharov Conference in Physics, Moscow, Vol. 91, pp 447-54. -
  2. [7][7] A. Ashtekar and M. Pierri, J. Math. Phys. (in press); gr-qc/9606085. - · arXiv
  3. [9][9] K. Kuchaˇ r, J. Romano and M. Varadarajan, gr-qc/9608011. - · arXiv

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Authors
Ashtekar, A.
Affiliations
Pennsylvania State University (US)
Corresponding author
Ashtekar, Abhay
Venue
Physical Review Letters
Published
1996-12-09
Volume
77
Issue
24
Pages
4864-4867
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W1978295149
Cited by
89
References
0
Citations by year
2022: 3 · 2021: 4 · 2020: 22 · 2017: 2 · 2015: 2 · 2012: 1
FWCI
4.22
Type
journal article
Language
en
Open access
Locations
  • Physical Review Letters (publishedVersion)
  • PubMed (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • National Science Foundation
  • Pennsylvania State University
  • Division of Mathematical Sciences
Topics
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
Keywords
quantum gravity, three-dimensional gravity, axisymmetric solutions, Maxwell field, Klein-Gordon field, quantum geometry

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