Oscillations in the primeval ambiplasma in the universe

Details Oscillations in the primeval ambiplasma in the universe Oscillations in the primeval ambiplasma in the universe

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.109...63s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 109, no. 1, Feb. 1985, p. 63-75.

Statistics

Computation

1

Computational Astrophysics, Plasma Oscillations, Universe, Wave Propagation, Antimatter, Leptons, Nucleons, Rarefied Plasmas

Scientific paper

This paper discusses the propagation of waves in the early Universe simulated by rarefied, homogeneous ambiplasma (a mixed matter-antimatter ionized gas) placed in a uniform magnetic field. A rich variety of oscillations appear due to enhanced degrees of freedom in the ambiplasma. These oscillations have been analyzed for the propagation vector along and across the direction of magnetic field both in a symmetric and asymmetric ambiplasma. It is found that the oscillations do not grow in different situations which have been discussed. Dispersion curves have been drawn and various cut-offs and resonances have been found out. The study is concluded by highlighting some characteristic features of the waves in the ambiplasma.

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