arXiv · astro-ph/0505602
Scalar Dark Matter and Cold Stars
Abstract
In a medium composed of scalar particles with non-zero mass, the range of Van-der-Waals-type scalar mediated interactions among nucleons becomes infinite when the medium makes a transition to a Bose-Einstein condensed phase. We explore this phenomenon in an astrophysical context. Namely, we study the effect of a scalar dark matter background on the equilibrium of degenerate stars.In particular we focus on white dwarfs and the changes induced in their masses and in their radii.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
J. A. Grifols. 2006-04-03. Scalar Dark Matter and Cold Stars. https://doi.org/10.1016/j.astropartphys.2005.12.004
Cite the original work for its findings. Save a collection to share your selection of sources.