Novel Constraints on Spin-Dependent Light Dark Matter Scattering
Alexander Clarke, Maxim Pospelov

TL;DR
This paper investigates the potential of the SNO experiment and CANDU reactors to detect light spin-dependent dark matter, deriving new constraints on interaction cross sections and exploring detection prospects.
Contribution
It introduces a novel method using heavy water reactors for producing and constraining light spin-dependent dark matter interactions, providing constraints above 10^{-33} cm^2 for masses up to 1.5 MeV.
Findings
CANDU reactors can produce MeV-scale dark matter detectable via nuclear reactions.
New constraints exclude cross sections above 10^{-33} cm^2 for dark matter masses ≤ 1.5 MeV.
Small near detectors have limited sensitivity compared to SNO constraints.
Abstract
We explore the sensitivity of the SNO experiment to light dark matter particles with spin-dependent interactions with nucleons. We show that the pair-production of MeV scale dark matter is possible in heavy water (CANDU) reactors via , and calculate the expected rate within the simplest models of -nucleon interactions. %Heavy water nuclear reactors serve as an excellent production method for spin-dependent dark matter. Owing to a sizable -value for this reaction, a large fraction of DM particles produced this way are above the threshold for deuteron disintegration, , which adds to the SNO neutral current signal. Evaluating the CANDU-to-SNO scheme for the production and detection of DM, we derive novel constraints for the -nucleon spin-dependent cross sections, showing that cross sections above $\sigma_{\chi…
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