Study of rotation curves of spiral galaxies with a scalar field dark matter model
arXiv:1210.6947 · doi:10.1063/1.4748537
Abstract
In this work we study rotation curves of spiral galaxies using a model of dark matter based on a scalar-tensor theory of gravity. We show how to estimate the scalar field dark matter parameters using a sample of observed rotation curves.
6 pages, 2 figures. arXiv admin note: substantial text overlap with arXiv:1112.5201