A Theoretical Investigation of the Topology of the Cosmic Microwave Background Anisotropy on the Scale approximately 1 degrees

Details A Theoretical Investigation of the Topology of the Cosmic Microwave Background Anisotropy on the Scale approximately 1 degrees A Theoretical Investigation of the Topology of the Cosmic Microwave Background Anisotropy on the Scale approximately 1 degrees

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...471..521n&link_type=abstract

Astrophysical Journal v.471, p.521

Astronomy and Astrophysics

Astronomy

8

Cosmology: Cosmic Microwave Background, Cosmology: Theory

Scientific paper

We have obtained new mathematical results for the theory of clustering of peaks in a Gaussian random field and for the theory of percolation. This new approach can be used for the development of methods for the analysis of the cosmic microwave background. We have simulated 1O° × 1O° sky maps of the cosmic microwave background anisotropy expected from different cosmological models with 0°.5-1° resolution and have demonstrated the usefulness of the topological method to distinguish between different models of the noise.

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