SO(4) Invariant States in Quantum Cosmology

Details SO(4) Invariant States in Quantum Cosmology SO(4) Invariant States in Quantum Cosmology

1992-10-30

arxiv.org/abs/gr-qc/9210020v3

Class.Quant.Grav.10:1435-1446,1993

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

15 pages

Scientific paper

10.1088/0264-9381/10/8/006

The phenomenon of linearisation instability is identified in models of quantum cosmology that are perturbations of mini-superspace models. In particular, constraints that are second order in the perturbations must be imposed on wave functions calculated in such models. It is shown explicitly that in the case of a model which is a perturbation of the mini-superspace which has $S^3$ spatial sections these constraints imply that any wave functions calculated in this model must be SO(4) invariant. (This replaces the previous corrupted version.)

Affiliated with

Also associated with

No associations

Rating

SO(4) Invariant States in Quantum Cosmology does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with SO(4) Invariant States in Quantum Cosmology, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SO(4) Invariant States in Quantum Cosmology will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-417187