Spin and torsion in the very early unive
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G.G.A. BΓ€uerle; Chr.J. Haneveld
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Article
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1983
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Elsevier Science
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English
β 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.