Statistics – Computation
Scientific paper
Dec 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.162..129k&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 162, no. 1, Dec. 1989, p. 129-150.
Statistics
Computation
3
Computational Astrophysics, Cosmology, Perturbation Theory, Rotating Matter, Universe, Field Theory (Physics), Scalars, Viscous Fluids
Scientific paper
The dynamics of a slowly rotating charged viscous-fluid universe coupled with a zero-mass scalar field is investigated. The rotational perturbations of such models are studied in order to substantiate the possibility that the universe is endowed with slow rotation. The effects of charged field and scalar field on the rotational motion are discussed. Except for perfect dragging, the scalar field as well as the charged field is found to have a damping effect on the rotation of matter. Rotating models which are expanding as well are obtained, in which cases the rotational velocities are found to decay with the time, and these models may be taken as good examples of real astrophysical situations.
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