Mathematics – Logic
Scientific paper
Oct 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvd..32.1889s&link_type=abstract
Physical Review D (Particles and Fields), Volume 32, Issue 8, 15 October 1985, pp.1889-1898
Mathematics
Logic
46
Origin And Formation Of The Universe
Scientific paper
Of particular interest is the behavior of the wave function of minimum excitation for compact cosmologies as the three-geometry becomes small. Information on its qualitative behavior is contained in the scaling behavior of the semiclassical approximation of the wave function. For small three-geometries, the scaling of the semiclassical wave function is determined by the scaling of the prefactor. We expect that the scaling of the prefactor for small arbitrary three-geometries is qualitatively the same as that of the prefactor for the simple geometry of a three-sphere. We compute the scaling of the prefactor for the geometry of Euclidean flat space with a three-sphere boundary; this geometry corresponds to that for a three-sphere boundary with a positive cosmological constant in the small-volume limit. For this geometry, the scaling of the prefactor entirely determines its form.
No associations
LandOfFree
Semiclassical wave function of the Universe at small three-geometries 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 Semiclassical wave function of the Universe at small three-geometries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Semiclassical wave function of the Universe at small three-geometries will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1548084