Formation of pregalactic dust and the cosmic microwave background spectrum

Details Formation of pregalactic dust and the cosmic microwave background spectrum Formation of pregalactic dust and the cosmic microwave background spectrum

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..673v&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, July-Aug. 1991, p. 673-680. In Russian.

Mathematics

Logic

1

Cosmic Dust, Microwave Spectra, Relic Radiation, Astronomical Models, Kinetic Theory, Red Shift

Scientific paper

The process of dust-grain formation in a cosmological model with population III stars at redshifts between 30 and 50 is examined. The kinetic theory of nucleation is used to show that the complexes H(+)(H2O) are the condensation centers of saturated water vapor. The relative contribution of 'polluted' ice to the total matter mass can reach an Omega(d) value of 0.00005, which makes it necessary to consider the interaction of dust and radiation when analyzing the cosmic microwave background spectrum.

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