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Direct detection of dark matter in universal bound states

Ranjan Laha1,2,* and Eric Braaten2,†

  • 1Center for Cosmology and AstroParticle Physics (CCAPP), Ohio State University, Columbus, Ohio 43210, USA
  • 2Department of Physics, Ohio State University, Columbus, Ohio 43210, USA

  • *laha.1@osu.edu
  • braaten@mps.ohio-state.edu

Phys. Rev. D 89, 103510 – Published 8 May, 2014

DOI: https://doi.org/10.1103/PhysRevD.89.103510

Abstract

We study the signatures for internal structure of dark matter in direct detection experiments in the context of asymmetric self-interacting dark matter. The self-interaction cross section of two dark matter particles at low energies is assumed to come close to saturating the S-wave unitarity bound, which requires the presence of a resonance near their scattering threshold. The universality of S-wave near-threshold resonances then implies that the low-energy scattering properties of a two-body bound state of dark matter particles are completely determined by its binding energy, irrespective of the underlying microphysics. The form factor for elastic scattering of the bound state from a nucleus and the possibility of break up of the bound state produce new signatures in the nuclear recoil energy spectrum. If these features are observed in experiments, it will give a smoking-gun signature for the internal structure of dark matter.

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