𝔖 Bobbio Scriptorium
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Nonequilibrium in the very early universe

✍ Scribed by John Ellis; Gary Steigman


Book ID
113342341
Publisher
Elsevier Science
Year
1980
Tongue
English
Weight
315 KB
Volume
89
Category
Article
ISSN
0370-2693

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A Very Early Universe
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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.