Quantum time evolution of a closed Friedmann model

Warning

This publication doesn't include Faculty of Education. It includes Faculty of Science. Official publication website can be found on muni.cz.
Authors

HINTERLEITNER Franz

Year of publication 2002
Type Article in Periodical
Magazine / Source Classical and Quantum Gravity
MU Faculty or unit

Faculty of Science

Citation
Field Theoretical physics
Keywords Quantum cosmology; Ashtekar variables; time evolution; classical limit
Description The hamiltonian constraint equation is solved for a closed, homogenous, isotropic cosmological model in Ashtekar variables. With the aid of matter in form of incoherent dust a quantum time evolution is introduced. This evolution smoothes out the singularities and approximates classical time evolution in the large-scale limit.
Related projects:

You are running an old browser version. We recommend updating your browser to its latest version.