1994/10/11 by J. Fernando Barbero G., J. Fernando Barbero · 60 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Classical mechanics #Computer science #Constraint (computer-aided design) #Cosmology and Gravitation Theories #Formalism (music) #General relativity #Geometry #Hamiltonian (control theory) #Hamiltonian constraint #Loop quantum gravity #Mathematical optimization #Mathematical physics #Mathematics #Noncommutative and Quantum Gravity Theories #Phase space #Physics #Quantum #Quantum gravity #Quantum mechanics #Theoretical physics #Wheeler–DeWitt equation #gr-qc
paper · pdf · doi:10.1103/physrevd.51.5507
published as Phys.Rev.D51:5507-5510,1995 · 10 pages, LATEX, Preprint CGPG-94/10-3
arxiv created 1994/10/11 · openalex publication_date 1995/05/15 · arxiv updated 2017/03/24 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
I suggest in this paper a new strategy to attack the problem of the reality conditions in the Ashtekar approach to classical and quantum general relativity. By writing a modified Hamiltonian constraint in the usual SO(3) Yang-Mills phase space I show that it is possible to describe space-times with a Lorentzian signature without the introduction of complex variables. All the features of the Ashtekar formalism related to the geometrical nature of the new variables are retained; in particular, it is still possible, in principle, to use the loop variables approach in the passage to the quantum theory. The key issue in the new formulation is how to deal with the more complicated Hamiltonian constraint that must be used in order to avoid the introduction of complex fields.