Self-ordering physics in an open universe

Details Self-ordering physics in an open universe Self-ordering physics in an open universe

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...412l...5s&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 412, no. 1, p. L5-L8.

Mathematics

Logic

13

Astronomical Models, Background Radiation, Cosmology, Microwaves, Density (Mass/Volume), Pressure Oscillations, Scaling, Variations

Scientific paper

This Letter presents an analytical model for the generation of density fluctuations likely to be appropriate for defects such as gauged and global strings, global monopoles, and textures, as well as for nontopological textures in an open or flat universe. For a reasonable range of parameters, these models in an open universe are compatible with both the level of MW fluctuations detected by COBE and with the fluctuations observed in the galaxy counts.

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