Pairing in the cosmic neutrino background

Details Pairing in the cosmic neutrino background Pairing in the cosmic neutrino background

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ncimb..67..213a&link_type=abstract

Nuovo Cimento B, Serie 11, vol. 67B, Feb. 11, 1982, p. 213-222. Consejo Nacional de Investigaciones Cientificas y Tecnologicas

Physics

Condensed Matter

Superconductivity

Astronomical Models, Background Radiation, Cosmic Rays, Neutrinos, Superfluidity, Hydrodynamic Equations, Magnetic Fields, Relativistic Effects, Superconductivity, Universe, Vortex Generators

Scientific paper

A theoretical model of a superfluid neutrino background in the Universe is developed, and the consequences of mechanical destruction of the superfluid state are reviewed. A hydrodynamic approach is used to examine the possibility of a superfluid state of matter, and the existence of magnetic fields is noted to be sufficient to create a mixed state from the superconductivity of the superfluid state. Further discussion is given to the vortex generated by the rotation of the Universe and the Hawking-Collins parameter for a limitation on the universal rotation is shown to lie within bounds which allow a large value for the neutrino mass. The same Hawking-Collins parameter is also found to be large enough to discount the presence of a superfluid state.

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