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Causality and matter propagation in 3d spin foam quantum gravity
General Relativity and Quantum Cosmology · Submitted 27 Aug 2006
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Finally, we show that the corresponding spin foam amplitudes admit a natural approximation as the Feynman amplitudes of a non-commutative quantum field theory, with the appropriate Feynman propagators weighting the lines of propagation, and that this effective field theory reduces to usual QFT in flat space in the no-gravity limit.
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The abstract, sentence by sentence
In this paper we tackle the issue of causality in quantum gravity, in the context of 3d spin foam models. We identify the correct procedure for implementing the causality/orientation dependence restriction that reduces the path integral for BF theory to that of quantum gravity in first order form. We construct explicitly the resulting causal spin foam model. We then add matter degrees of freedom to it and construct a causal spin foam model for 3d quantum gravity coupled to matter fields. Finally, we show that the corresponding spin foam amplitudes admit a natural approximation as the Feynman amplitudes of a non-commutative quantum field theory, with the appropriate Feynman propagators weighting the lines of propagation, and that this effective field theory reduces to usual QFT in flat space in the no-gravity limit.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | In this paper we tackle the issue of causality in quantum gravity, in the context of 3d spin foam models. | background 0.81 | 0.78 | 0.03 | asserted 0.64 |
| s1 | We identify the correct procedure for implementing the causality/orientation dependence restriction that reduces the path integral for BF theory to that of quantum gravity in first order form. | contribution 0.56 | 0.93 | 0.11 | asserted 1.00 |
| s2 | We construct explicitly the resulting causal spin foam model. | contribution 0.92 | 0.96 | 0.10 | asserted 1.00 |
| s3 | We then add matter degrees of freedom to it and construct a causal spin foam model for 3d quantum gravity coupled to matter fields. | contribution 0.97 | 0.96 | 0.10 | asserted 1.00 |
| s4 | Finally, we show that the corresponding spin foam amplitudes admit a natural approximation as the Feynman amplitudes of a non-commutative quantum field theory, with the appropriate Feynman propagators weighting the lines of propagation, and that this effective field theory reduces to usual QFT in flat space in the no-gravity limit. | result 0.96 | 0.94 | 0.59 | asserted 1.00 |
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The paper
Original abstract
In this paper we tackle the issue of causality in quantum gravity, in the context of 3d spin foam models. We identify the correct procedure for implementing the causality/orientation dependence restriction that reduces the path integral for BF theory to that of quantum gravity in first order form. We construct explicitly the resulting causal spin foam model. We then add matter degrees of freedom to it and construct a causal spin foam model for 3d quantum gravity coupled to matter fields. Finally, we show that the corresponding spin foam amplitudes admit a natural approximation as the Feynman amplitudes of a non-commutative quantum field theory, with the appropriate Feynman propagators weighting the lines of propagation, and that this effective field theory reduces to usual QFT in flat space in the no-gravity limit.
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References
How the literature uses it
11 arXiv papers cite this in 27 sentences
Papers citing it · 18 sentences without a confident label
Compares with it 1 paper
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There are several differences, however, between the model proposed here and the one proposed in [ref] , i.e. between ([ref]) and ([ref]).
A New Class of Group Field Theories for 1st Order Discrete Quantum Gravity · Riemannian 3d gravity · 1.00
Cites it as support 2 papers
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More precisely, the amplitudes of BF-theory do not depend on the $2$-complex $Δ^*$, therefore being in particular blind to the orientation of $Δ^*$ [ref] (see also [ref] for earlier and later related results in the 3d case).
The Complete Barrett-Crane Model and its Causal Structure · Spacetime orientation · 0.97
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This same restriction has been argued for as a (pre-)causality condition needed to define causal transition amplitudes for BF theory and gravity in [ref] .
Group field theory and simplicial quantum gravity · Feynman amplitudes: discrete gravity path integrals · 0.96
Cites it as background 4 papers
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For further discussion on this, see [ref] , and for a classic treatment of the issue of causality and different transition amplitudes in quantum gravity, within the covariant path integral approach, see [ref] .
A New Class of Group Field Theories for 1st Order Discrete Quantum Gravity · Causality, orientation dependence, 3rd quantization and quantum (discrete) gravity path integrals · 1.00
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However, discussions on the problem are usually constrained to take place on a formal level (see, e.g., [ref] for an overview, [ref] for the formal construction in quantum gravity path integrals, and [ref] for tentative definitions of causal counterparts of spin foam models for quantum gravity).
Two-point functions in (loop) quantum cosmology · Vertex expansions: Feynman propagator · 1.00
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The role of causality in the spinfoam framework has been studied since the early literature [ref] .
Causal Structure for Generalized Spinfoams · Introduction · 0.99
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