Clustering Scale of Dark Matter

Details Clustering Scale of Dark Matter Clustering Scale of Dark Matter

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007acppb..38.3859j&link_type=abstract

Acta Physica Polonica B, vol. 38, Issue 12, p.3859

Physics

1

Scientific paper

We obtain mass distribution for flattened galaxies M94 and M101 whose rotation curves fail sphericity test in thin disk approximation by applying Iterative Spectral Method. The results obtained suggest smaller amount of dark matter (if any) than predicted by classical approach to modelling of rotation curves customarily assuming massive spherical halo.

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