Cosmological consequences of a homogeneous, homothetic gauge field

Details Cosmological consequences of a homogeneous, homothetic gauge field Cosmological consequences of a homogeneous, homothetic gauge field

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phlb..119...85h&link_type=abstract

Physics Letters B, Volume 119, Issue 1-3, p. 85-88.

Physics

4

Scientific paper

We solve the cosmological equations when the vacuum term is a scular field associated with a simple global symmetry. One solution describes the universe as an expanding zero energy fluctuation wherein matter with positive energy appears spontaneously. Numerical constraints on H0, Λ(ϱvO and current rate of matter creation are given. A high entropy/baryon ratio is produced by the vacuum ``decay''.
The author wishes to acknowledge helpful discussions with Dr. K.W. Lake and other members of the Queen' Astronomy group.

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