Flat rotation curves in scalar field galaxy halos

Details Flat rotation curves in scalar field galaxy halos Flat rotation curves in scalar field galaxy halos

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007gregr..39.1279m&link_type=abstract

General Relativity and Gravitation, Volume 39, Issue 8, pp.1279-1286

Physics

10

Scientific paper

We start with a model where the dark matter is of scalar field nature, which condensates and form the dark halos of galaxies. In this work we study Bose Einstein condensates (BEC) where the scalar field particles are in many different states, and not only in the ground state, as in a realistic BEC. We find that this model is in better agreement with the rotation curves of galaxies than previous models with scalar field dark matter.

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