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Inflation and broken Lorentz symmetry in the very early universe

✍ Scribed by M. Gasperini


Book ID
113349015
Publisher
Elsevier Science
Year
1985
Tongue
English
Weight
223 KB
Volume
163
Category
Article
ISSN
0370-2693

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Spin and torsion in the very early unive
✍ G.G.A. BΓ€uerle; Chr.J. Haneveld πŸ“‚ Article πŸ“… 1983 πŸ› Elsevier Science 🌐 English βš– 495 KB

In the very early universe with temperature T between 10% K and 103r K the gravitational effect of torsion is dominant if particles with spin are sufficiently polarized. The source of the torsion is the spin density and the latter is usually described by a classical theory of Weyssenhoff and Raabe.