Demonstrating topological identification capabilities of the NEXT experiment at low pressure
This paper reports the first validation of the NEXT-100 detector's topological discrimination capabilities at low pressure (~4 bar), demonstrating a signal efficiency of 75.6% and background acceptance of 14.7% for distinguishing neutrinoless double beta decay-like events from background, which aligns with the performance of its predecessor, NEXT-White.
Original paper licensed under CC BY 4.0 (http://creativecommons.org/licenses/by/4.0/). This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer
Deep within the subatomic world, there is a rare and mysterious event that physicists have been hunting for decades: the moment when two neutrons inside an atomic nucleus transform into two protons and two electrons, but without releasing the usual pair of ghostly particles known as neutrinos. If this happens, it would prove that the neutrino is its own antiparticle, a discovery that would rewrite the fundamental laws of physics and explain why the universe is made of matter rather than being annihilated by antimatter. To catch this fleeting event, scientists build massive, ultra-sensitive detectors filled with a heavy gas, waiting for the specific signature of two electrons emerging from a single point. The challenge is not just seeing them, but distinguishing them from the constant rain of background radiation that mimics their appearance.
A team of researchers working on the NEXT-100 experiment has taken a significant step forward in this search by proving that their detector can successfully tell the difference between a signal and background noise, even when the gas inside is kept at a lower pressure than originally planned. The experiment is housed in an underground laboratory in Spain, shielded from cosmic rays, where a large cylinder filled with xenon gas acts as a three-dimensional camera. When a particle passes through, it leaves a trail of light that the detector records, allowing scientists to reconstruct the path of the particle in three dimensions. The key to identifying the rare decay is the shape of that path: the signal they want looks like two distinct tracks starting from the same spot and ending with two bright, heavy "blobs" of energy, while most background noise looks like a single track with only one heavy end.
In this recent study, the team focused on a specific phase of their operation where the xenon gas was held at a pressure of about 4 bar, roughly four times the pressure of the atmosphere at sea level. This was a lower pressure than the 10 bar they intend to use for their main data collection, but it offered a unique opportunity to test how the detector performs under different conditions. The researchers wanted to know if the lower pressure, which allows the electron tracks to stretch out longer and become more diffuse, would ruin their ability to identify the correct shapes. To find out, they used a powerful computer simulation to predict how the tracks would behave at both low and high pressures, and then compared those predictions to real data collected from the detector. The simulation showed that at the lower pressure, the tracks do indeed become longer and the energy deposits at the ends become larger and fuzzier, but the fundamental difference between a two-track signal and a single-track background remains visible.
To test this in the real world, the scientists introduced a specific type of radioactive source into the detector that produces pairs of electrons and positrons, creating events that look very similar to the signal they are searching for. They then applied a series of careful filters to the data, removing events that were too close to the edges of the detector or that had overlapping tracks, leaving them with a clean sample to analyze. They focused on the energy deposits at the ends of the tracks, looking for the tell-tale sign of two heavy blobs versus one. By adjusting the size of the area they examined around the ends of the tracks, they found a sweet spot that maximized their ability to keep the good events while rejecting the bad ones.
The results were encouraging. The team demonstrated that even at this lower pressure, the detector could identify the double-electron tracks with an efficiency of about 76 percent, meaning it successfully kept three-quarters of the true signals. At the same time, it rejected about 85 percent of the background noise, accepting only about 15 percent of the unwanted single-electron tracks. These numbers are comparable to the performance of their previous, smaller detector, which operated at a higher pressure, proving that the technology is robust and scalable. The study confirms that the lower pressure does not prevent the detector from seeing the crucial topological features needed for the search. While the researchers note that their current computer models do not yet capture every detail of the low-pressure environment, the agreement between their simulations and the real data gives them confidence that their methods are sound. This work establishes a solid baseline for the next phase of the experiment, where the detector will operate at full pressure, bringing the hunt for neutrinoless double beta decay closer to a definitive answer.
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