Self-similar evolution of magnetized plasmas. 2: Nonequilibrium solutions and Hubble's expansion

Details Self-similar evolution of magnetized plasmas. 2: Nonequilibrium solutions and Hubble's expansion Self-similar evolution of magnetized plasmas. 2: Nonequilibrium solutions and Hubble's expansion

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...425..439y&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 425, no. 2, p. 439-441

Astronomy and Astrophysics

Astrophysics

1

Cosmology, Equilibrium Equations, Gravitational Effects, Magnetic Clouds, Nonequilibrium Plasmas, Doppler Effect, Equations Of Motion, Force Distribution, Galactic Evolution, Hubble Constant, Mass Distribution

Scientific paper

The self-similar dynamic equation is solved for a gamma = 4/3 polytrope. We include gravitational terms attributed to mass distribution of an evolving plasma cloud and a possible compact parent object as well. The evolving patterns can be classified as deceleration, acceleration, and expanding equilibria. The solutions verify the possibility of linear expansion of magnetized plasmas. Their implications on Hubble's law of the expanding universe are discussed.

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