Using the CMB angular power spectrum to study Dark Matter-photon
  interactions
  In this paper, we explore the impact of Dark Matter-photon interactions on
the CMB angular power spectrum. Using the one-year data release of the Planck
satellite, we derive an upper bound on the Dark Matter-photon elastic
scattering cross section of sigma_{DM-photon} < 8 x 10^{-31} (m_DM/GeV) cm^2
(68% CL) if the cross section is constant and a present-day value of
sigma_{DM-photon} < 6 x 10^{-40} (m_DM/GeV) cm^2 (68% CL) if it scales as the
temperature squared. For such a limiting cross section, both the B-modes and
the TT angular power spectrum are suppressed with respect to LCDM predictions
for l > 500 and l > 3000 respectively, indicating that forthcoming data from
CMB polarisation experiments and Planck could help to constrain and
characterise the physics of the dark sector. This essentially initiates a new
type of dark matter search that is independent of whether dark matter is
annihilating, decaying or asymmetric. Thus, any CMB experiment with the ability
to measure the temperature and/or polarisation power spectra at high l should
be able to investigate the potential interactions of dark matter and contribute
to our fundamental understanding of its nature.
