Quantum Mixtures in the Early Universe

Details Quantum Mixtures in the Early Universe Quantum Mixtures in the Early Universe

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997gregr..29.1555s&link_type=abstract

General Relativity and Gravitation, Vol. 29, p. 1555-1582 (1997)

Physics

Scientific paper

In Relativistic Schrödinger Theory for spinning matter, there exist mixtures which have vanishing spin density ($S_{\mu \nu} \equiv 0$). Such a fermionic, but spinless quantum fluid is studied in detail. Its energy- momentum density can develop negative pressure which is able to accelerate the expansion of the universe and to create matter energy through continuous bouncing at minimal radius (``cosmic pumping'').

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