Ponderable soliton stars and cosmic background radiation

Details Ponderable soliton stars and cosmic background radiation Ponderable soliton stars and cosmic background radiation

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...365..107c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 365, Dec. 10, 1990, p. 107-114.

Astronomy and Astrophysics

Astronomy

5

Relic Radiation, Solitary Waves, Stellar Interiors, Stellar Mass, Active Galactic Nuclei, Black Holes (Astronomy), Perturbation Theory, Stellar Evolution, Stellar Radiation

Scientific paper

A theory is developed to describe the possible perturbations of the cosmic background radiation (CBR) by radiation from ponderable soliton stars in the early universe. Since the temperature of such stars is in the range of 10 to the 6th K, thermalization of their emitted radiation is possible. Two models are considered: one in which thermalization is ignored and one in which decoupling from thermalization is considered as a sudden process. The expected perturbation of the CBR is probably less than 1 percent and is largely around the short-wavelength end, in the form of point radio sources. This result is consistent with the most recent COBE measurements.

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