Original title: Confronting the Higgsino Interpretation of the LZ Event with the High-Energy Sideband
Nicholas L. Rodd, Benjamin R. Safdi, Tracy R. Slatyer, Weishuang Linda Xu · September 2026
Scientists are trying to detect dark matter, the invisible substance filling the universe. The LZ detector recorded a single high-energy collision of 248 keV when a particle struck a xenon atom. Lower-energy hits were completely missing. A proposed explanation was a theoretical particle called a 1.1 TeV higgsinoA theoretical particle from supersymmetry that could be a candidate for dark matter. that scatters inelastically, meaning it absorbs energy and jumps to a higher state during a bounce. This process naturally pushes recoil energies upward. However, researchers checked this idea against another detector region called a high-energy sidebandA region in the data spectrum used to check for background or additional signals.. They found that this thermal higgsino should have triggered extra, even higher-energy hits there, but LZ observed none. Instead, a lighter, non-thermal ~500 GeV higgsino might evade this problem. Future detectors with heavy targets could test these ideas.
Imagine you hear a single clap in a quiet room and suspect it's from a specific person clapping their hands. But that person, when they clap, always claps twice in quick succession. Here, LZ heard one clap (the event), but the paper shows that if it were from that person (higgsino), there should have been a second clap at a different time (higher energy), which wasn't heard. This makes you doubt your initial guess.
This affects physicists trying to identify dark matter, as a single event could be misinterpreted without checking all energy ranges. Correctly interpreting signals ensures we don't chase false leads in one of science's biggest mysteries.
The abstract notes that the acceptance in the high-energy bin is not public, so the tension is not fully verified. It also shows that a non-thermal higgsino might evade the constraint, indicating the analysis isn't conclusive. The work relies on assumptions about dark matter velocity distribution, which can vary.
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Confronting the Higgsino Interpretation of the LZ Event with the High-Energy Sideband — Nicholas L. Rodd, Benjamin R. Safdi, Tracy R. Slatyer et al.
Abstract licence: CC0
Explanation generated by Synthesis from the abstract — it is not the original paper. This is a preprint, so it hasn't necessarily been peer reviewed.