2004/11/29 by Bianca Dittrich, Thomas Thiemann · 9 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Classical mechanics #Constraint (computer-aided design) #Cosmology and Gravitation Theories #Geometry #Hamiltonian (control theory) #Hamiltonian constraint #Loop (graph theory) #Loop quantum cosmology #Loop quantum gravity #Mathematical optimization #Mathematical physics #Mathematics #Noncommutative and Quantum Gravity Theories #Physics #Quantum #Quantum gravity #Quantum mechanics #Series (stratigraphy) #Theoretical physics #Wheeler–DeWitt equation #gr-qc #hep-th #math-ph #math.MP
paper · pdf · doi:10.1088/0264-9381/23/4/002
published as Class.Quant.Grav. 23 (2006) 1067-1088 · 23 pages, no figures
arxiv created 2004/11/29 · openalex publication_date 2006/01/31 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
This is the second paper in our series of five in which we test the Master Constraint Programme for solving the Hamiltonian constraint in Loop Quantum Gravity. In this work we begin with the simplest examples: Finite dimensional models with a finite number of first or second class constraints, Abelean or non -- Abelean, with or without structure functions.