Constraint on Light Dipole Dark Matter from Helioseismology
  We investigate the effects of a magnetic dipole moment of asymmetric dark
matter (DM) in the evolution of the Sun. The dipole interaction can lead to a
sizable DM scattering cross section even for light DM, and the asymmetric dark
matter can lead to a large DM number density in the Sun. We find that solar
model precision tests, using as diagnostic the sound speed profile obtained
from helioseismology data, exclude dipolar dark matter particles with a mass
larger than 4.3 GeV and magnetic dipole moment larger than 1.6 $\times
\;10^{-17}$ e cm.
