Cited by 84Noncommutative and Quantum Gravity TheoriesRelativity and Gravitational TheoryBlack Holes and Theoretical Physics

Towards the QFT on curved spacetime limit of QGR: I. A general scheme

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Sahlmann, H, Thiemann, T·2006·Classical and Quantum Gravity

Abstract

In this article and a companion paper we address the question of how one might obtain the semiclassical limit of ordinary matter quantum fields (QFT) propagating on curved spacetimes (CST) from full fledged Quantum General Relativity (QGR), starting from first principles. We stress that we do not claim to have a satisfactory answer to this question, rather our intention is to ignite a discussion by displaying the problems that have to be solved when carrying out such a program. In the present paper we propose a scheme that one might follow in order to arrive at such a limit. We discuss the technical and conceptual problems that arise in doing so and how they can be solved in principle. As to be expected, completely new issues arise due to the fact that QGR is a background independent theory. For instance, fundamentally the notion of a photon involves not only the Maxwell quantum field but also the metric operator - in a sense, there is no photon vacuum state but a "photon vacuum operator"! While in this first paper we focus on conceptual and abstract aspects, for instance the definition of (fundamental) n-particle states (e.g. photons), in the second paper we perform detailed calculations including, among other things, coherent state expectation values and propagation on random lattices. These calculations serve as an illustration of how far one can get with present mathematical techniques. Although they result in detailed predictions for the size of first quantum corrections such as the gamma-ray burst effect, these predictions should not be taken too seriously because a) the calculations are carried out at the kinematical level only and b) while we can classify the amount of freedom in our constructions, the analysis of the physical significance of possible choices has just begun.

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  • Early model calculations suggest that Lorentz-invariance-violation effects may arise from a quantum-gravity granularity of spacetime measured at rest by a preferred frame.

    “In the absence of detailed formulations, certain early pioneering model calculations [192] (see also general treatment [340, 341]) indicate the possibility for certain Lorentz-invariance-violation (LIV) effects associated to a quantum-gravity granularity of spacetime measured at rest by a preferred frame of observers.”

    From The Spin-Foam Approach to Quantum Gravity (2013) · cites this paper as [340]

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References 41 · Cited by 84

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Authors
Sahlmann, H., & Thiemann, T.
Venue
Classical and Quantum Gravity
Published
2006-01-19
Volume
23
Issue
3
Pages
867-908
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2041004793
Cited by
84
References
41
Citations by year
2026: 3 · 2025: 2 · 2023: 4 · 2022: 6 · 2021: 3 · 2020: 2 · 2019: 2 · 2018: 1 · 2017: 1 · 2016: 4 · 2015: 2 · 2014: 3 · 2013: 3 · 2012: 8
FWCI
7.06
Type
journal article
Language
en
Open access
Locations
  • Classical and Quantum Gravity (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
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 general relativity, curved spacetime, semiclassical limit, quantum field theory in curved spacetime, background independence, metric operator, coherent states, random lattices, quantum corrections

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