Loading…

Quantum cosmology in the energy representation

The Hawking minisuperspace model (closed FRW geometry with a homogeneous massive scalar field) provides a fairly non-trivial testing ground for fundamental problems in quantum cosmology. We provide evidence that the Wheeler-DeWitt equation admits a basis of solutions that is distinguished by analyti...

Full description

Saved in:
Bibliographic Details
Published in:Nuclear physics. B 1996-11, Vol.479 (1), p.461-491
Main Author: Embacher, Franz
Format: Article
Language:English
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:The Hawking minisuperspace model (closed FRW geometry with a homogeneous massive scalar field) provides a fairly non-trivial testing ground for fundamental problems in quantum cosmology. We provide evidence that the Wheeler-DeWitt equation admits a basis of solutions that is distinguished by analyticity properties in a large scale factor expansion. As a consequence, the space of solutions decomposes in a preferred way into two Hilbert spaces with positive and negative definite scalar product, respectively. These results may be viewed as a hint for a deeper significance of analyticity. If a similar structure exists in full (non-minisuperspace) models as well, severe implications on the foundations of quantum cosmology are to be expected. Semiclassically, the elements of the preferred basis describe contracting and expanding universes with a prescribed value of the matter (scalar field) energy. Half of the basis elements have previously been constructed by Hawking and Page in a wormhole context, and they appear in a new light here. The technical tools to arrive at these conclusions are transformations of the wave function into several alternative representations that are based on the harmonic oscillator form of the matter energy operator, and that are called oscillator, energy and Fock representation. The framework defined by these may be of some help in analyzing the Wheeler-De itt equation for other purposes as well.
ISSN:0550-3213
1873-1562
DOI:10.1016/0550-3213(96)00444-0