Precision NV-Diamond Strain Imaging for Directional Dark Matter Detection

ORAL

Abstract

We use pulsed quantum sensing protocols for improved strain imaging using ensembles of nitrogen-vacancy (NV) centers in diamond. This work is a step toward assessing feasibility of directional dark matter detection in a diamond-based detector. In such a detector, NV-based strain imaging would localize potential dark matter damage tracks in a micron-size voxel within a millimeter-sized diamond detector segment.  Subsequent superresolution NV spectroscopy or high-resolution x-ray tomography, within the voxel of interest, would reveal required directional information. On the other hand, it is well-known that strain inhomogeneities affect magnetic field sensing--one of the main applications of NV centers. These results could also inform new avenues toward material development, enabling higher precision magnetometry. We have applied these methods to a variety of diamond samples grown under different conditions, to characterize the strain distribution and suitability for dark matter detection.  Here, we present our latest results and outlook for future improvements.

*This work was supported by the DOE QuANTISED program under Award No. DE-SC0019396; the Army Research Laboratory MAQP program under Contract No. W911NF-19-2-0181; the DARPA DRINQS program under Grant No. D18AC00033; and the University of Maryland Quantum Technology Center.

Presenters

  • Reza Ebadi

    • University of Maryland, College Park

Authors

  • Reza Ebadi

    • University of Maryland, College Park
  • Mason C Marshall

    • University of Maryland, College Park
  • Connor A Hart

    • University of Maryland, College Park
  • Matthew J Turner

    • University of Maryland, College Park
  • David F Phillips

    • Harvard - Smithsonian Center for Astroph
    • Harvard - Smithsonian Center for Astrophysics
  • Ronald L Walsworth

    • University of Maryland, College Park