Electroweak renormalization of neutralino-Higgs interactions at one-loop and its impacts on spin-independent direct detection of Wino-like dark matter
Subhadip Bisal, Arindam Chatterjee, Debottam Das, and Syed Adil Pasha

TL;DR
This paper improves the theoretical calculation of Wino-like neutralino dark matter interactions by including one-loop electroweak corrections, significantly impacting predictions for direct detection experiments.
Contribution
It provides the first comprehensive one-loop electroweak correction calculation for neutralino-Higgs interactions, including counterterms, enhancing the accuracy of DM-nucleon cross-section predictions.
Findings
Cross-sections can vary by over 100% with corrections.
Electroweak corrections significantly affect direct detection prospects.
Inclusion of counterterms refines theoretical estimates.
Abstract
A Wino-like neutralino dark matter (DM) in the form of the lightest supersymmetric particle (LSP) has been considered one of the popular paradigms that can naturally accommodate {\it new physics} at a relatively higher scale, typically beyond the reach of the LHC. The constraint on the DM relic density typically implies a lightest neutralino mass TeV. Its observational signature through nuclear recoil experiments, specifically involving DM-nucleon spin-independent (SI) scattering, is not impressive, following its high masses and tiny Higgsino fractions. The theoretical calculations can be improved when we compute all the one-loop electroweak (EW) corrections to the three-point vertices for the neutralino (Wino)-Higgs interactions, which in turn boosts the DM-nucleon scattering cross-sections through the SM-like Higgs exchange. Importantly, we include the counterterm…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Atomic and Subatomic Physics Research
