1999/06/24 by Claus Kiefer
Physics and Astronomy · #gr-qc
published as Lect.Notes Phys. 541 (2000) 158-187 · 31 pages, LATEX, needs Springer macro cl2emult.cls, 3 eps-figures, contribution for the Karpacz winter school 1999
arxiv created 1999/06/24 · arxiv updated 2009/11/30
I give a review of the conceptual issues that arise in theories of quantum cosmology. I start by emphasising some features of ordinary quantum theory that also play a crucial role in understanding quantum cosmology. I then give motivations why spacetime cannot be treated classically at the most fundamental level. Two important issues in quantum cosmology -- the problem of time and the role of boundary conditions -- are discussed at some length. Finally, I discuss how classical spacetime can be recovered as an approximate notion. This involves the application of a semiclassical approximation and the process of decoherence. The latter is applied to both global degrees of freedom and primordial fluctuations in an inflationary Universe.