Search for compressed electroweak SUSY production in final states with two -leptons in and $13.6pp$ collisions with the ATLAS detector
Using 140 fb⁻¹ of 13 TeV and 53 fb⁻¹ of 13.6 TeV proton-proton collision data, the ATLAS collaboration searched for compressed electroweak SUSY scenarios involving -sleptons, charginos, and neutralinos in final states with two -leptons, setting mass exclusion limits up to 200 GeV for electroweakinos while observing no significant deviations from the Standard Model that would allow for the exclusion of direct -slepton production when combining all channels.
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The universe is built on a foundation of particles and forces that we can see and measure, yet much of what makes up the cosmos remains hidden. Scientists have long suspected that the visible world is only a small fraction of reality, with a vast, invisible sector of particles waiting to be discovered. This hidden sector is predicted by a theory called supersymmetry, which suggests that every known particle has a heavier, unseen partner. If these partners exist, they could explain why the universe has the mass it does and might even account for the mysterious dark matter that holds galaxies together. The challenge is that these partners, if they exist, are likely very heavy or hide in ways that make them incredibly difficult to spot. They might decay into other particles so quickly that they vanish before we can see them, or they might be so similar in mass to their decay products that the energy difference is too small to notice.
A researcher using the ATLAS detector at the Large Hadron Collider has taken a fresh look at this problem, specifically hunting for a type of hidden particle known as a tau-slepton. These are the supersymmetric partners of the tau lepton, a heavy cousin of the electron. The researcher focused on a tricky scenario where the tau-slepton is only slightly heavier than the lightest stable particle in the supersymmetric family. In this "compressed" situation, the energy released when the tau-slepton decays is very low, making the resulting particles move slowly and blend in with the background noise of ordinary particle collisions. To find them, the researcher looked for events where a high-energy jet of particles, created by the collision, gives a sudden push to the entire system, making the hidden particles easier to spot. They analyzed data from 140 fb⁻¹ and 53 fb⁻¹ of proton-proton collisions, combining records from two different periods of operation to maximize their chances of seeing something new.
The search involved looking for specific signatures in the debris of these collisions, particularly events containing tau leptons that decay into other particles. The researcher split their investigation into several different approaches to cover all possible ways these particles could appear. Some searches looked for collisions with no extra jets, while others focused on events where a single high-energy jet was present to provide that necessary boost. They used advanced computer algorithms to sift through the data, distinguishing between the rare signals of new physics and the overwhelming flood of ordinary events. The analysis was rigorous, comparing the observed data against detailed simulations of what should happen if only known particles existed. The researcher also paid close attention to the "fake" signals that occur when ordinary jets are mistaken for tau leptons, using data-driven methods to ensure these errors were accounted for.
After examining the vast amount of data, the results showed that the universe, at least in the energy ranges explored, behaves generally as the Standard Model of physics predicts, although several deviations with local significances of 2.1–2.4σ were observed. These deviations weaken the observed exclusion limits. While there were a few small fluctuations in the data that stood out slightly from the average, none were large enough to be considered a discovery. These small deviations were consistent with random statistical variations. Consequently, the researcher was able to set strict limits on where these hidden particles could be hiding in specific channels, though no exclusion limits were set for direct tau-slepton production when statistically combining all considered channels. In the ISR channel alone, they ruled out the existence of tau-sleptons with masses up to 115 gigaelectronvolts if the mass difference between the slepton and the lightest partner was 30 gigaelectronvolts. Similarly, they excluded charginos, another type of supersymmetric particle, with masses up to 175 gigaelectronvolts under the same conditions. For scenarios involving pairs of charginos or mixtures with neutralinos, the limits extended to masses of 200 gigaelectronvolts.
The study did not find the new particles it was looking for, but it significantly narrowed the search space. By pushing the boundaries of what is known, the researcher has eliminated a wide range of possibilities for how these particles might exist. The results are particularly important because they cover a region of mass and energy that was previously difficult to explore due to the subtle nature of the signals. The absence of a discovery does not mean the theory is wrong, but it does mean that if these particles exist, they must be heavier or behave in ways that are even more elusive than the models tested in this study. The work demonstrates the power of combining large datasets with sophisticated analysis techniques to probe the deepest layers of reality, bringing us closer to understanding the full composition of the universe.
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