Loop quantum gravity is a mature theory. To proceed to explicit calculations in cosmology, it is necessary to make assumptions and simplifications based on the symmetries of the cosmological setting. Symmetry reduction is especially critical when dealing with cosmological perturbations. The present paper reviews several approaches to the problem of building a consistent formalism that describes the dynamics of perturbations on a quantum spacetime and tries to address their respective strengths and weaknesses. We also review the main open issues in loop quantum cosmology.
机构:
Penn State Univ, Dept Phys, Inst Gravitat & Cosmos, University Pk, PA 16802 USAPenn State Univ, Dept Phys, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
机构:
Penn State Univ, Inst Gravitat Phys & Geometry, Davey Lab 104, University Pk, PA 16802 USAPenn State Univ, Inst Gravitat Phys & Geometry, Davey Lab 104, University Pk, PA 16802 USA