The steepness of the cosmic spectrum in the 10 - 102Mpc range and COBE's data.

Details The steepness of the cosmic spectrum in the 10 - 102Mpc range and COBE's data. The steepness of the cosmic spectrum in the 10 - 102Mpc range and COBE's data.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ncimb.111..665f&link_type=abstract

Nuovo Cimento B, Vol. 111B, No. 5, p. 665 - 667

Statistics

1

Universe: Dark Matter, Cosmic Microwave Background

Scientific paper

The author shows that cosmic inhomogeneity spectra steeper than CDM in the 10 - 102Mpc range provide better fits to the angular correlation function and the peak statistics in COBE-DMR maps for practically any value of the cosmic density, and give relief to the quadrupole discrepancy. CDM + texture models with Ω0 ≅ 0.7 are especially successful in linking the 10 Mpc and 103Mpc regions.

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