10–12 Jul 2019
Dip. di Fisica - Edificio G. Marconi
Europe/Rome timezone

Toward Directional Detection of Dark Matter Using Spectroscopy of Quantum Defects in Diamond

Not scheduled
15m
Aula Conversi (Dip. di Fisica - Edificio G. Marconi)

Aula Conversi

Dip. di Fisica - Edificio G. Marconi

Piazzale A.Moro, 2 00185 Roma

Speaker

Dr Mason Marshall (Harvard-Smithsonian Center for Astrophysics)

Description

We propose a method to identify weakly interacting massive particle (WIMP) dark matter via induced nuclear recoil in diamond. This 100 nm damage cluster induces stress in the crystal, shifting the energy levels of nearby quantum defects. Crucially, the direction of the track left by the recoil allows us to determine the incoming direction of the particle enabling the possibility of distinguishing between dark matter particles and backgrounds such as solar neutrinos. To measure these damage tracks we will use spectroscopic interrogation of quantum defects such as NV centers in diamond along with other nanoscale imaging techniques. Here we present the proposed technique along with measurements of the pre-existing stress variations in diamond. This method could allow for directional detection of WIMP-induced nuclear recoils at solid-state densities, enabling probes of WIMP parameter space below the solar neutrino floor.

Primary authors

Dr Mason Marshall (Harvard-Smithsonian Center for Astrophysics) Dr Raisa Trubko (Department of Physics, Harvard University) Dr Pauli Kehaiyas (Sandia National Laboratories) Mr Matthew Turner (Department of Physics, Harvard University) Dr David Phillips (Harvard-Smithsonian Center for Astrophysics) Dr Surjeet Rajendran (Department of Physics, University of California at Berkeley) Prof. Alex Sushkov (Department of Physics, Boston University) Dr Ronald Walsworth (Harvard-Smithsonian Center for Astrophysics)

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