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Lorentzian LQG vertex amplitude
General Relativity and Quantum Cosmology · Submitted 26 Oct 2007
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim The main features of the Euclidean model are preserved in the Lorentzian one.
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The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
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The abstract, sentence by sentence
We generalize a model recently proposed for Euclidean quantum gravity to the case of Lorentzian signature. The main features of the Euclidean model are preserved in the Lorentzian one. In particular, the boundary Hilbert space matches the one of SU(2) loop quantum gravity. As in the Euclidean case, the model can be obtained from the Lorentzian Barrett-Crane model from a flipping of the Poisson structure, or alternatively, by adding a topological term to the action and taking the small Barbero-Immirzi parameter limit.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We generalize a model recently proposed for Euclidean quantum gravity to the case of Lorentzian signature. | contribution 1.00 | 0.92 | 0.19 | asserted 0.99 |
| s1 | The main features of the Euclidean model are preserved in the Lorentzian one. | result 0.89 | 0.76 | 0.28 | asserted 1.00 |
| s2 | In particular, the boundary Hilbert space matches the one of SU(2) loop quantum gravity. | result 0.99 | 0.72 | 0.19 | asserted 1.00 |
| s3 | As in the Euclidean case, the model can be obtained from the Lorentzian Barrett-Crane model from a flipping of the Poisson structure, or alternatively, by adding a topological term to the action and taking the small Barbero-Immirzi parameter limit. | method 0.87 | 0.55 | 0.15 | asserted 0.94 |
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The paper
Original abstract
We generalize a model recently proposed for Euclidean quantum gravity to the case of Lorentzian signature. The main features of the Euclidean model are preserved in the Lorentzian one. In particular, the boundary Hilbert space matches the one of SU(2) loop quantum gravity. As in the Euclidean case, the model can be obtained from the Lorentzian Barrett-Crane model from a flipping of the Poisson structure, or alternatively, by adding a topological term to the action and taking the small Barbero-Immirzi parameter limit.
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References
How the literature uses it
29 arXiv papers cite this in 53 sentences
Papers citing it · 40 sentences without a confident label
Builds on it 1 paper
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In this section, we use the matrix element approach to construct the physical boundary Hilbert space of the new spin-foam theory with Lorentzian signature [ref] .
Physical boundary Hilbert space and volume operator in the Lorentzian new spin-foam theory · Physical boundary Hilbert space of the new theory · 0.80
Uses its method or tool 2 papers
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We evaluate it in the basis of the coherent states [ref] , so that the expression $⟨A | ψ_H_ℓ ⟩=W(H_ℓ)$ reads [equation] The amplitude is Lorentzian, with an integration over the $(2,)$ elements $G_n$ associated to the edges (see Fig. [ref]).
Learning about Quantum Gravity with a Couple of Nodes · Vertex amplitude · 0.92
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We use the version of the amplitude developed in [ref] generally denoted as the EPRL amplitude.
Numerical analysis of the self-energy in covariant Loop Quantum Gravity · Introduction · 0.80
Compares with it 1 paper
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The model we construct contains in fact a slight modification with respect to the one in [ref] (corresponding to a slightly different factor ordering of the constraints).
Physical boundary Hilbert space and volume operator in the Lorentzian new spin-foam theory · Introduction · 0.83
Cites it as background 8 papers
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Here, we briefly describe in Section II the discrete theory introduced in [ref] (euclidean case) and in [ref] (lorentzian case), in order to make this paper self contained.
LQG vertex with finite Immirzi parameter · Introduction · 0.91
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Currently one of the successful spin foam models is the EPRL/FK model defined in [ref] , whose implementation of simplicity constraint is understood in the sense of [ref] .
Asymptotics of Spinfoam Amplitude on Simplicial Manifold: Euclidean Theory · Introduction · 0.90
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In particular, a vertex amplitude $A_v(j_f,i_e)$ that might define a quantum theory of gravity has been developed in [ref] and is today under intense investigation (see [ref] ).
Face amplitude of spinfoam quantum gravity · Introduction · 0.95
What it cites · 12 sentences without a confident label
Builds on 1 paper
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In [ref] only the Euclidean signature case was considered.
Flipped spinfoam vertex and loop gravity · Introduction · 0.80
Uses the method or tool of 1 paper
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We follow the strategy in [ref] and impose $M_f:=(C_f^i)^2≈0$, allowing at the same time for possible corrections, small in the semiclassical limit.
Flipped spinfoam vertex and loop gravity · Quantization and vertex amplitude · 0.99
Compares with 2 papers
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(iii) Finally, the model defined here is clearly distinct from other models proposed in the literature as alternatives to the Barrett-Crane model [ref] , as it is based solely on the simple representations of the form $(n,0)$.
A New Spin Foam Model for 4d Gravity · Conclusion · 1.00
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(iii) Finally, the model defined here is clearly distinct from other models proposed in the literature as alternatives to the Barrett-Crane model [ref] , as it is based solely on the simple representations of the form $(n,0)$.
Spin foam model from canonical quantization · Conclusion · 1.00
Cites as support 1 paper
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As argued in [ref] the problem can be traced back to the way some of the constraints are imposed in the Barrett-Crane model.
Flipped spinfoam vertex and loop gravity · Introduction · 0.98
Cites as background 3 papers
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Spin foam techniques [ref] have been developed as a possible framework to study the quantum dynamics.
A lattice worldsheet sum for 4-d Euclidean general relativity · Introduction · 0.98
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Loop quantum gravity (LQG) [ref] provides a well defined, background independent, construction of the kinematical Hilbert space of quantum general relativity.
An Introduction to Loop Quantum Gravity Through Cosmology · Introduction · 0.99
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Matters of triangulation independence could be adressed by a group field theory [ref] approach.
The group field theory approach to quantum gravity · Introduction · 0.80
Discussion
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