Detecting Dark Matter with Molecules

ORAL

Abstract

The evidence for the existence of dark matter, which makes up about 85$\%$ of the matter density in the Universe, is overwhelming. Efforts to detect galactic dark matter particles in the laboratory are crucial for revealing the particle nature of dark matter. We propose a detection concept based on molecular excitations caused by the dark matter-nucleus scattering within the molecule. By mixing molecules of different isotopes, including those with an odd number of neutrons, we obtain sensitivity to both spin-independent interactions and spin-dependent interactions with the neutron. In addition, we explore various halides and hydrides molecules, which can provide sensitivity to spin-dependent interactions with the proton.

Authors

  • Jesus Perez-Rios

    • Fritz Haber Institute of the Max Planck Society
    • Fritz-Haber-Institut der Max-Planck-Gesellschaft, Faradayweg 4-6, D-14195 Berlin, Germany
    • Fritz-Haber Institute of the Max-Planck Society
  • Harikrishnan Ramani

    • Berkeley Center for Theoretical Physics, Department of Physics, University of California, Berkeley, California 94720, USA
  • Oren Slone

    • Princeton Center for Theoretical Science, Princeton University, Princeton, New Jersey 08544, USA
  • Rouven Essig

    • C. N. Yang Institute for Theoretical Physics, Stony Brook University, New York 11794-384, USA