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A Lorentzian Signature Model for Quantum General Relativity
General Relativity and Quantum Cosmology · Submitted 9 Apr 1999
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We give a relativistic spin network model for quantum gravity based on the Lorentz group and its q-deformation, the Quantum Lorentz Algebra.
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The abstract, sentence by sentence
We give a relativistic spin network model for quantum gravity based on the Lorentz group and its q-deformation, the Quantum Lorentz Algebra. We propose a combinatorial model for the path integral given by an integral over suitable representations of this algebra. This generalises the state sum models for the case of the four-dimensional rotation group previously studied in gr-qc/9709028. As a technical tool, formulae for the evaluation of relativistic spin networks for the Lorentz group are developed, with some simple examples which show that the evaluation is finite in interesting cases. We conjecture that the `10J' symbol needed in our model has a finite value.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We give a relativistic spin network model for quantum gravity based on the Lorentz group and its q-deformation, the Quantum Lorentz Algebra. | contribution 0.94 | 0.91 | 0.17 | asserted 1.00 |
| s1 | We propose a combinatorial model for the path integral given by an integral over suitable representations of this algebra. | contribution 0.52 | 0.80 | 0.14 | asserted 0.77 |
| s2 | This generalises the state sum models for the case of the four-dimensional rotation group previously studied in gr-qc/9709028. | background 0.73 | 0.19 | 0.06 | asserted 1.00 |
| s3 | As a technical tool, formulae for the evaluation of relativistic spin networks for the Lorentz group are developed, with some simple examples which show that the evaluation is finite in interesting cases. | contribution 0.49 | 0.93 | 0.07 | asserted 1.00 |
| s4 | We conjecture that the `10J' symbol needed in our model has a finite value. | future work 0.42 | 0.20 | 0.19 | speculative 1.00 |
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The paper
Original abstract
We give a relativistic spin network model for quantum gravity based on the Lorentz group and its q-deformation, the Quantum Lorentz Algebra. We propose a combinatorial model for the path integral given by an integral over suitable representations of this algebra. This generalises the state sum models for the case of the four-dimensional rotation group previously studied in gr-qc/9709028. As a technical tool, formulae for the evaluation of relativistic spin networks for the Lorentz group are developed, with some simple examples which show that the evaluation is finite in interesting cases. We conjecture that the `10J' symbol needed in our model has a finite value.
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References
How later papers used it
68 later papers cite it
1 later paper by other authors is listed below: 1 compared its own results with it.
Compares with it 1 of 3 papers with this label
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Said its new Lorentzian model has similar advantages as compared to this paper.
A New Spin Foam Model for 4d Gravity (2007) · 0.88 · paraphrased: the licence does not allow quoting
How the literature uses it
68 arXiv papers cite this in 133 sentences
Papers citing it · 74 sentences without a confident label
Contests it 1 paper
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Unlike the rest of the constraints, the center is imposed strongly in the literature.[We also remind the reader that in the previous Barrett-Crane model [ref] , all constraints were imposed strongly, leading to inconsistencies.] This somewhat uneven procedure for the implementation is a motivation for our present work, where we consider the possibility of treating all constraints on the same footing.
Holomorphic Lorentzian Simplicity Constraints · Introduction · contest 0.84
Builds on it 1 paper
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We constructed the complete BC model by extending existing formulations of the BC model: One which includes timelike normal vectors only [ref] and the other one which exclusively considers spacelike normal vectors [ref] .
The Complete Barrett-Crane Model and its Causal Structure · Relation to other GFT and spin foam models · 1.00
Uses its method or tool 2 papers
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For a spin-network with the invariants from the set described above we can define the evaluation by the method proposed in [ref] . * Firstly, we consider the graph with links labelled by the representations of the principal series $(k_e,ρ_e)$ and nodes labelled by elements of $F$ in the tensor product of the representations associated with the links meeting in the node (as described in the case of compact groups).
All 3-edge-connected relativistic BC and EPRL spin-networks are integrable · The evaluation of the spin-network · 1.00
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This is achieved as follows: * We utilize the rich causal structure of the completion [ref] of the Barrett-Crane (BC) GFT model [ref] , which provides a GFT quantization of first-order Palatini gravity, to causally couple a physical Lorentzian reference frame to the GFT model. * We represent slightly inhomogeneous cosmological geometries via entangled states $|Δ;x^0,*x⟩$.
Scalar Cosmological Perturbations from Quantum Gravitational Entanglement · Introduction · 0.91
Compares with it 3 papers
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agreeing with the results obtained in [ref] .
The Complete Barrett-Crane Model and its Causal Structure · Kernels of non-mixed type · 0.99
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The new Lorentzian model that we obtain has similar advantages as compared to [ref] .
A New Spin Foam Model for 4d Gravity · Introduction · 0.88
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The complicate expressions of the above boost matrix elements can be compared with the much simpler ones appearing in the Lorentzian Barrett-Crane model [ref] .
Boosting Wigner's nj-symbols · Boost matrix elements for simple representations · 1.00
Cites it as background 44 papers
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A main outcome in this longstanding direction of research during the previous decade has been what has become known as the EPRL spinfoam transition amplitude of (covariant) Loop Quantum Gravity [ref] .
Geometry Transition in Spinfoams · Introduction · 0.88
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The two most developed and most studied models are the Barrett-Crane model (BC) [ref] and the Engle-Pereira-Rovelli-Livine (EPRL) model [ref] .
Spinfoam Models for Quantum Gravity: Overview · 4d Quantum Gravity · 0.93
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The Barrett-Crane (BC) model [ref] and the EPRL model [ref] are the most prominent GFT (and spin foam) models, realizing a constrained BF-quantization of first-order Palatini and first-order Palatini-Holst gravity, respectively.
The Complete Barrett-Crane Model and its Causal Structure · Introduction · 0.92
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