Observer reference triad rotation, magnetic fields, and rotation in Euclidean cosmological models

Details Observer reference triad rotation, magnetic fields, and rotation in Euclidean cosmological models Observer reference triad rotation, magnetic fields, and rotation in Euclidean cosmological models

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...252..410f&link_type=abstract

Astrophysical Journal, Part 1, vol. 252, Jan. 15, 1982, p. 410-417.

Mathematics

Logic

5

Astronomical Models, Cosmology, Fluid Flow, Formalism, Intergalactic Media, Magnetic Fields, Background Radiation, Conservation Equations, Einstein Equations, Magnetohydrodynamics, Maxwell Equation, Microwaves, Vorticity

Scientific paper

It is shown that a cosmological model with Euclidean space sections admits fluid flows if a magnetic field is present. Further, if observer reference frames spin in their response to the universe, a vorticity may exist. Limits can be set on any present intergalactic magnetic field of less than 5.38 x 10 to the -10th gauss (for a model with the chosen symmetry and choice of initial field and fluid velocity components).

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