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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.

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