Probing the Scalar WIMP-Pion Coupling with the first LUX-ZEPLIN data
J.Aalbers, D.S.Akerib, A.K.Al Musalhi, F.Alder, C.S.Amarasinghe,, A.Ames, T.J.Anderson, N.Angelides, H.M.Ara\'ujo, J.E.Armstrong, M.Arthurs,, A.Baker, S.Balashov, J.Bang, E.E.Barillier, J.W.Bargemann, K.Beattie,, T.Benson, A.Bhatti, A.Biekert, T.P.Biesiadzinski, H.J.Birch

TL;DR
This paper reports on a search for WIMP-pion interactions using LUX-ZEPLIN data, setting new upper limits and exploring a less-studied interaction channel relevant for certain dark matter models.
Contribution
First experimental constraints on WIMP-pion couplings using LUX-ZEPLIN data, expanding the scope of dark matter interaction searches.
Findings
No significant excess observed in data.
Set upper limit of $1.5\times10^{-46}$ cm$^2$ at 90% CL for 33 GeV/c$^2$ WIMPs.
Demonstrated the importance of considering WIMP-pion interactions in dark matter models.
Abstract
Weakly interacting massive particles (WIMPs) may interact with a virtual pion that is exchanged between nucleons. This interaction channel is important to consider in models where the spin-independent isoscalar channel is suppressed. Using data from the first science run of the LUX-ZEPLIN dark matter experiment, containing 60 live days of data in a 5.5~tonne fiducial mass of liquid xenon, we report the results on a search for WIMP-pion interactions. We observe no significant excess and set an upper limit of ~cm at a 90\% confidence level for a WIMP mass of 33~GeV/c for this interaction.
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Quantum Chromodynamics and Particle Interactions · Dark Matter and Cosmic Phenomena
