First asteroseismic limits on the nature of dark matter
Abstract
We report the first constraints on the properties of weakly interacting low-mass dark matter (DM) particles using asteroseismology. The additional energy transport mechanism due to accumulated asymmetric DM particles modifies the central temperature and density of low-mass stars and suppresses the convective core expected in 1.1-1.3 Ms stars even for an environmental DM density as low as the expected in the solar neighborhood. An asteroseismic modeling of the stars KIC 8006161, HD 52265 and Alpha Cen B revealed small frequency separations significantly deviated from the observations, leading to the exclusion of a region of the DM parameter space mass versus spin-dependent DM-proton scattering cross section comparable with present experimental constraints.
Keywords
Cite
@article{arxiv.1212.2985,
title = {First asteroseismic limits on the nature of dark matter},
author = {Jordi Casanellas and Ilídio Lopes},
journal= {arXiv preprint arXiv:1212.2985},
year = {2013}
}
Comments
5 pages, 3 figures. v2 matches version to be published in ApJL