In the \u00a0year 2019\u00a0, a significant advance in our understanding of the universe unfolded deep beneath the surface of Italy. An underground laboratory, located 1.5 kilometers under the Massif of Gran Sasso, hosted a dark matter detector that witnessed an extraordinary event: the \u00a0radioactive disintegration\u00a0 of an atom of \u00a0Xenon-124\u00a0. This remarkable phenomenon represents the slowest and rarest process ever recorded, marking a milestone in experimental physics.<\/p>\n
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They touched the cosmic lottery.<\/strong> Xenon-124 boasts a semi-life of \u00a01.8 \u00d7 10\u00b2\u00b2 years\u00a0. To grasp the scale of this figure, it’s essential to note that 1.8 \u00d7 10\u00b2\u00b2 years translates to \u00a018,000 trillion years\u00a0\u2014a time frame that exceeds the estimated \u00a0age of the universe\u00a0, which is only about \u00a013.8 billion years\u00a0. This means that the process observed by Italian scientists in 2019 is a billion times longer than the universe’s own lifespan. As detailed in the esteemed journal, Nature<\/a>, this groundbreaking discovery has far-reaching implications.<\/p>\n <\/p>\n A little context.<\/strong> The term \u00a0semi-experience\u00a0 refers to a statistical measure akin to half-life. Specifically, it defines how long it takes for half of a large group of Xenon-124 atoms to disintegrate into \u00a0Teluro-124\u00a0. In contrast, elements like Uranium-238 have a semi-life of \u00a04.5 billion years\u00a0. Understanding this process is crucial for researchers studying the stability of atomic structures.<\/p>\n <\/p>\n For an individual atom, disintegration is a \u00a0random event\u00a0. It could decay in the next moment or remain stable for an extended period. However, when observed on a \u00a0statistical scale\u00a0, semi-life becomes a reliable predictor of collective behavior. Observing a container filled with numerous Xenon-124 atoms would require an astonishing \u00a018,000 trillion years\u00a0 for half of them to transform.<\/p>\n <\/p>\n How did they do it?<\/strong> The researchers utilized a colossal container housing \u00a03.2 tons\u00a0 of ultra-pure liquid xenon in the Xenon1T experiment, located at the National Laboratory of Gran Sasso in Italy. This dark matter detector was primarily designed to search for \u00a0Weakly Interacting Massive Particles (WIMPs)\u00a0, which are theoretical candidates believed to constitute dark matter.<\/p>\n <\/p>\n The detector was engineered with extreme sensitivity, carefully constructed beneath a mountain to shield it from \u00a0cosmic radiation\u00a0. Surprisingly, instead of uncovering dark matter, the detector captured the rare event of an atom of Xenon-124 decomposing into Teluro-124. This process is historically unprecedented and represents a landmark achievement in experimental physics.<\/p>\n <\/p>\n It is not a hyperbole.<\/strong> This discovery is a true milestone that researchers did not expect to observe even over a billion lifetimes of the universe. While the probability of a single Xenon-124 atom disintegrating within a year is virtually nonexistent, the detector analyzed nearly \u00a010,000 billion\u00a0 xenon atoms. With such a staggering number of “lottery tickets,” the odds of at least one disintegration occurring during the observation period significantly increased. Over \u00a0177 days of data collection\u00a0, the team observed \u00a0126 events\u00a0 confirming the decay of Xenon-124\u2014an incredibly rare type of radioactive disintegration recognized within the standard model of particle physics.<\/p>\n <\/p>\n What did they see.<\/strong> A Xenon-124 atom disintegrates when its nucleus captures two electrons from its innermost layers. This process converts two protons into neutrons, transforming the atom into Teluro-124. The energy released during this transformation is carried away by two \u00a0neutrinos\u00a0, which elude detection. However, the \u00a0Xenon1T photomultipliers\u00a0 recorded the subsequent \u00a0X-ray bursts\u00a0 and emitted electrons, resulting from the upper-layer electrons cascading to fill the void left by the captured electrons. This energetic signature is the flash that reveals this extraordinary cosmic event.<\/p>\n <\/p>\n Has it served for something?<\/strong> The implications of this discovery extend beyond mere curiosity. While the team did not strike gold in their pursuit of dark matter, the detection showcased the Xenon1T’s ability to capture incredibly weak and rare signals, validating its design. Moreover, the data garnered will be instrumental in refining theoretical models describing atomic nucleus stability.<\/p>\n <\/p>\n This landmark observation serves as a precursor for even more ambitious goals, notably the search for \u00a0double electron captures without neutrinos\u00a0. If such a process is successfully detected, it would provide evidence supporting the hypothesis that neutrinos are, in fact, their own \u00a0antiparticles\u00a0\u2014known as \u00a0Majorana particles\u00a0. This revelation could hold the key to explaining why our universe is predominantly composed of matter rather than antimatter.<\/p>\n <\/p>\n Image | Lngs<\/p>\n In summary, even though the quest for dark matter continues, the unexpected findings from the Xenon1T experiment have unraveled vital information about particle physics. The journey for understanding the fundamental forces that shape our universe is ongoing, and each new discovery brings us a step closer to understanding the cosmic puzzle.<\/p>\n