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arXiv · 1309.7588

Using the CMB angular power spectrum to study Dark Matter-photon interactions

Ryan J. Wilkinson·Julien Lesgourgues·Celine Boehm
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Abstract

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.

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Ryan J. Wilkinson, Julien Lesgourgues, Celine Boehm. 2014-04-25. Using the CMB angular power spectrum to study Dark Matter-photon interactions. https://doi.org/10.1088/1475-7516%2F2014%2F04%2F026

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