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We propose an explicit spin-foam amplitude for Lorentzian gravity in three dimensions, allowing for both space- and time-like boundaries. The model is based on two main requirements: that it should be structurally similar to its well-known…

General Relativity and Quantum Cosmology · Physics 2024-09-04 José Diogo Simão

In a recent paper [1] we have constructed the spin and tensor representations of SO(4) from which the invariant weight can be derived for the Barrett-Crane model in quantum gravity. By analogy with the SO(4) group, we present the…

General Relativity and Quantum Cosmology · Physics 2007-05-23 M. Lorente

We present the construction of a new state sum model for $4d$ Lorentzian quantum gravity based on the description of quantum simplicial geometry in terms of edge vectors. Quantum states and amplitudes for simplicial geometry are built from…

General Relativity and Quantum Cosmology · Physics 2025-01-20 Roukaya Dekhil , Matteo Laudonio , Daniele Oriti

This thesis is developed in the context of the spin-foam approach to quantum gravity; all results are concerned with the Lorentzian theory and with semiclassical methods. A correspondence is given between Majorana 2-spinors and time-like…

General Relativity and Quantum Cosmology · Physics 2024-06-12 José Diogo Simão

We show that the degenerate sector of Spin(4) Plebanski formulation of four-dimensional gravity is exactly solvable and describes covariantly embedded SU(2) BF theory. This fact ensures that its spin foam quantization is given by the SU(2)…

General Relativity and Quantum Cosmology · Physics 2012-10-12 Sergei Alexandrov

We show how Feynman amplitudes of standard QFT on flat and homogeneous space can naturally be recast as the evaluation of observables for a specific spin foam model, which provides dynamics for the background geometry. We identify the…

High Energy Physics - Theory · Physics 2008-11-26 Aristide Baratin , Laurent Freidel

We give an overview of the current issues in early universe cosmology and consider the potential resolution of these issues in an as yet nascent spin foam cosmology. The model is the Barrett-Crane Model for quantum gravity along with a…

General Relativity and Quantum Cosmology · Physics 2007-05-23 S. Alexander , L. Crane , M. D. Sheppeard

We construct and analyse a quantum deformation of the Lorentzian EPRL model. The model is based on the representation theory of the quantum Lorentz group with real deformation parameter. We give a definition of the quantum EPRL intertwiner,…

General Relativity and Quantum Cosmology · Physics 2011-12-13 Winston J. Fairbairn , Catherine Meusburger

We give a general definition of spin foam models, and then of models of 4d quantum gravity based on constraining BF theory. We highlight the construction and quantization ambiguities entering model building, among which the choice of…

General Relativity and Quantum Cosmology · Physics 2019-06-19 Marco Finocchiaro , Daniele Oriti

In this article we give a systematic definition of the recently introduced spin foam models for four dimensional quantum gravity reviewing the main results on their semiclassical limit on fixed discretizations.

General Relativity and Quantum Cosmology · Physics 2012-05-07 Alejandro Perez

The amplitude for the 4-simplex in a spin foam model for quantum gravity is defined using a graphical calculus for the unitary representations of the Lorentz group. The asymptotics of this amplitude are studied in the limit when the…

General Relativity and Quantum Cosmology · Physics 2014-11-20 John W. Barrett , Richard J. Dowdall , Winston J. Fairbairn , Frank Hellmann , Roberto Pereira

Spin foams are candidate state-sum models for transition amplitudes in quantum gravity. An active research subject is to identify the possible divergences of spin foam models, or alternatively to show that models are finite. We will discuss…

General Relativity and Quantum Cosmology · Physics 2013-12-16 Valentin Bonzom , Bianca Dittrich

We prove that a certain spinfoam model for euclidean quantum general relativity, recently defined, is finite: all its all Feynman diagrams converge. The model is a variant of the Barrett-Crane model, and is defined in terms of a field…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Alejandro Perez

We study the behavior of holonomy spin foam partition functions, a form of lattice gauge gravity, on generic 4d-triangulations using micro local analysis. To do so we adapt tools from the renormalization theory of quantum field theory on…

General Relativity and Quantum Cosmology · Physics 2012-10-22 Frank Hellmann , Wojciech Kaminski

We construct an effective cosmological spin-foam model for a (2+1) dimensional spatially flat universe, discretized on a hypercubical lattice, containing both space- and time-like regions. Our starting point is the recently proposed…

General Relativity and Quantum Cosmology · Physics 2025-04-17 Alexander F. Jercher , José Diogo Simão , Sebastian Steinhaus

We present a spin foam model in which the fundamental ``bubble amplitudes'' (the analog of the one-loop corrections in quantum field theory) are finite as the cutoff is removed. The model is a natural variant of the field theoretical…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Alejandro Perez , Carlo Rovelli

A key point in the spin foam approach to quantum gravity is the implementation of simplicity constraints in the partition functions of the models. Here, we discuss the imposition of these constraints in a phase space setting corresponding…

General Relativity and Quantum Cosmology · Physics 2014-11-21 Bianca Dittrich , James P. Ryan

We define a four-dimensional spin-foam perturbation theory for the ${\rm BF}$-theory with a $B\wedge B$ potential term defined for a compact semi-simple Lie group $G$ on a compact orientable 4-manifold $M$. This is done by using the formal…

Mathematical Physics · Physics 2017-05-23 Joao Faria Martins , Aleksandar Mikovic

Spin foam models are an attempt for a covariant, or path integral formulation of canonical loop quantum gravity. The construction of such models usually rely on the Plebanski formulation of general relativity as a constrained BF theory and…

General Relativity and Quantum Cosmology · Physics 2015-05-13 Aristide Baratin , Cecilia Flori , Thomas Thiemann

The model of Lorentzian three-dimensional dynamical triangulations provides a non-perturbative definition of three-dimensional quantum gravity. The theory has two phases: a weak-coupling phase with quantum fluctuations around a…

High Energy Physics - Lattice · Physics 2009-11-07 J. Ambjorn , J. Jurkiewicz , R. Loll