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High-energy gravity and the very early universe

✍ Scribed by Hidezumi Terazawa

Publisher
Springer US
Year
1980
Tongue
English
Weight
263 KB
Volume
12
Category
Article
ISSN
0001-7701

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πŸ“œ SIMILAR VOLUMES

Spin and torsion in the very early unive
Spin and torsion in the very early universe
✍ 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.