A variant of General Relativity provides a model in which scale invariance of matter is a consistency requirement on its coupling to gravitation. Invariance breaking is introduced by giving a finite (cosmological) range to one of the gravitational variables; the Einstein and cosmological constants a
Local scale invarlance and gravitation
โ Scribed by Peter G.O Freund
- Publisher
- Elsevier Science
- Year
- 1974
- Tongue
- English
- Weight
- 864 KB
- Volume
- 84
- Category
- Article
- ISSN
- 0003-4916
No coin nor oath required. For personal study only.
โฆ Synopsis
A gauge field theory of (local) scale invariance is constructed. When coupled to gravity it yields the old theory of Weyl. A Brans-Dicke scalar field is introduced & la Dbac. With a suitable choice of parameters the theory then reduces in a special gauge to Einstein's theory even in the presence of matter. If the gauge field of scaling (even under charge conjugation) is identified with the gauge field of an internal symmetry, a (spontaneous) breakdown of charge conjugation invariance (and of CP) can follow. This effect has a reasonable order of magnitude if gravity is replaced by strong gravity and the internal charge identified with lepton number of baryon number, or some neutral weak charge. Certain difficulties arise, however, if one insists on the Weyl identification of the gauge field of scaling with the electromagnetic field.
It is shown that the observed tensor mesons (f; f', etc.), while basic in tensor meson dominance, are not the quanta of a gauge field of strong gravity.
๐ SIMILAR VOLUMES
An expression for the semiclassical density of states for a particle in a smooth potential well is obtained from the Kirkwood expansion of the partition function: the result being valid for a finite as well as an infinite potential well. The expression obtained for the semiclassical density of state