Predictions in the condensate model of evolution of structures in the Universe

Details Predictions in the condensate model of evolution of structures in the Universe Predictions in the condensate model of evolution of structures in the Universe

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.232..853d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 232, June 15, 1988, p. 853-864.

Astronomy and Astrophysics

Astronomy

4

Astronomical Models, Background Radiation, Cosmic X Rays, Cosmology, Brightness, Condensates, Dark Matter, Galactic Evolution, Microwaves, Red Shift, Virial Theorem

Scientific paper

A model for the origin of the diffuse X-ray background and the formation of structures in the Universe has been proposed which is based upon the existence of massive objects (referred to as condensates). There are two ways in which these can be observed at present. Individual condensates produce observable fluctuations in the temperature characterizing the microwave background radiation and may be of low, yet observable, surface brightness in the optical. The expected observational properties of the condensates and possibilities of their detection are discussed.

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