Probing unexplored spin-dependent dark matter-proton coupling with few-photoelectron threshold in COSINE-100

TL;DR

This paper presents new, more sensitive constraints on low-mass spin-dependent dark matter-proton interactions using a novel low-threshold detection method in the COSINE-100 experiment, including the first search in the few-photoelectron regime.

Contribution

It introduces a specialized event selection and noise mitigation technique enabling detection thresholds of 3-4 photoelectrons, extending sensitivity to sub-GeV dark matter masses.

Findings

Established the most stringent limits for 1.75-2.25 GeV/c$^2$ dark matter.

Extended sensitivity to 15-58 MeV/c$^2$ dark matter using the Migdal effect.

No significant annual modulation signal was observed.

Abstract

We report new constraints on the spin-dependent scattering cross section between low-mass dark matter and protons using data collected by the COSINE-100 experiment. By implementing a specialized event selection process using a multi-layer perceptron and robust noise mitigation, this analysis pioneers a detection threshold of 3 and 4 isolated peaks, corresponding to the reconstructed photoelectrons, which is significantly lower than the 8 photoelectron threshold used in previous analyses. In this unstudied few-photoelectron regime, where PMT-induced noise and phosphorescence are prevalent, we utilize a phenomenological background model to search for the annual modulation signal expected from the Standard Halo Model. No statistically significant annual modulation is observed in our data. We derive new 90% confidence level upper limits for the spin-dependent DM-proton cross section, establishing the world's most stringent constraints in the 1.75-2.25 GeV/c$^2$ mass range. Furthermore, by incorporating the Migdal effect, we extend the experimental sensitivity to the sub-GeV/c$^2$ regime, setting world-leading limits in the 15-58 MeV/c$^2$ range. These results demonstrate the capability of NaI(Tl) target materials to probe previously unexplored regions of the dark matter parameter space.