TY - JOUR
T1 - Direct detection of light dark matter and solar neutrinos via color center production in crystals
AU - Budnik, Ranny
AU - Cheshnovsky, Ori
AU - Slone, Oren
AU - Volansky, Tomer
N1 - Publisher Copyright:
© 2018 The Authors
PY - 2018/7/10
Y1 - 2018/7/10
N2 - We propose a new low-threshold direct-detection concept for dark matter and for coherent nuclear scattering of solar neutrinos, based on the dissociation of atoms and subsequent creation of color center type defects within a lattice. The novelty in our approach lies in its ability to detect single defects in a macroscopic bulk of material. This class of experiments features ultra-low energy thresholds which allows for the probing of dark matter as light as O(10) MeV through nuclear scattering. Another feature of defect creation in crystals is directional information, which presents as a spectacular signal and a handle on background reduction in the form of daily modulation of the interaction rate. We discuss the envisioned setup and detection technique, as well as background reduction. We further calculate the expected rates for dark matter and solar neutrinos in two example crystals for which available data exists, demonstrating the prospective sensitivity of such experiments.
AB - We propose a new low-threshold direct-detection concept for dark matter and for coherent nuclear scattering of solar neutrinos, based on the dissociation of atoms and subsequent creation of color center type defects within a lattice. The novelty in our approach lies in its ability to detect single defects in a macroscopic bulk of material. This class of experiments features ultra-low energy thresholds which allows for the probing of dark matter as light as O(10) MeV through nuclear scattering. Another feature of defect creation in crystals is directional information, which presents as a spectacular signal and a handle on background reduction in the form of daily modulation of the interaction rate. We discuss the envisioned setup and detection technique, as well as background reduction. We further calculate the expected rates for dark matter and solar neutrinos in two example crystals for which available data exists, demonstrating the prospective sensitivity of such experiments.
KW - Color center
KW - Direct detection
KW - Light dark matter
KW - Solar neutrinos
UR - http://www.scopus.com/inward/record.url?scp=85047260483&partnerID=8YFLogxK
U2 - 10.1016/j.physletb.2018.04.063
DO - 10.1016/j.physletb.2018.04.063
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AN - SCOPUS:85047260483
SN - 0370-2693
VL - 782
SP - 242
EP - 250
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
ER -