Three-component fluid model of the universe of critical density

Details Three-component fluid model of the universe of critical density Three-component fluid model of the universe of critical density

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.159...99c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 159, no. 1, Sept. 1989, p. 99-102. Research supported by CONACYT.

Statistics

Computation

Astronomical Models, Fluid Dynamics, Hydrogen Plasma, Space Density, Computational Astrophysics, Galactic Mass, Perturbation Theory, Universe

Scientific paper

A three-component fluid model of the universe during the recombination
era is analyzed for density = critical density. In addition to the
well-known instability of the Jeans mode at 10 to the 9th solar masses,
two more unstable modes at 10 to the 12th solar masses are found.

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