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Home Science News Chemistry

Land Ahoy! GSI/FAIR Experiments Illuminate the Shoreline of Superheavy Element Stability

January 15, 2025
in Chemistry
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Investigating superheavy elements
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A groundbreaking development has emerged in the field of nuclear physics, where a collaborative research team composed of scientists from GSI/FAIR, Johannes Gutenberg University Mainz, and the Helmholtz Institute Mainz has successfully delved deeper into the mysterious realm of superheavy elements. Their pioneering study centers on the unraveling of the properties of rutherfordium-252, a superheavy nucleus that now holds the record for the shortest lifespan among known superheavy nuclei. This remarkable finding garnered attention in the scientific community, culminating in a prestigious publication in the journal Physical Review Letters, where it was distinguished as an “Editor’s suggestion.”

The intricate world of atomic nuclei, governed by the forces of physics, presents scientists with a unique challenge. At the core of this challenge lies the strong nuclear force, which works to bind protons and neutrons together within atomic nuclei. However, a significant hurdle arises due to the repulsion experienced by positively charged protons, especially in nuclei containing an excessive number of these particles. This repulsion can lead to instability and pose formidable challenges in the synthesis of new superheavy elements. Interestingly, researchers have identified specific combinations of protons and neutrons known as “magic numbers.” These combinations lend nuclei an additional degree of stability, effectively enriching the environment surrounding superheavy elements.

For decades, theoretical predictions rooted in nuclear physics have alluded to a metaphysical construct known as the “island of stability.” This hypothetical region is posited to exist amidst a sea of unstable superheavy nuclei. Researchers speculate that certain superheavy nuclei may exhibit exceptionally extended lifetimes, which could even approach geological time scales. The tantalizing notion of this island has gained traction over the years, with observable trends indicating that the half-lives of the heaviest known nuclei tend to increase as they inch closer to the predicted magic number of 184 neutrons.

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Despite the theoretical underpinnings of the island of stability, concrete details regarding its precise location, height, and dimensions remain elusive. The pioneering researchers at GSI/FAIR and their collaborating institutions have made significant strides toward mapping this enigmatic entity by successfully identifying rutherfordium-252, marking a pivotal moment in their exploration of superheavy nuclei. This newfound isotope serves as a crucial indicator that delineates the island’s shoreline, offering insights into the potential limits of stability within heavier elements.

One significant aspect of studying superheavy nuclei is the inherent challenges associated with their detection. To facilitate experimental observation, scientists have determined that the minimum lifetime for these elusive nuclei typically amounts to approximately one-millionth of a second. Such short-lived species often elude direct detection due to their brief existence. Nevertheless, researchers have developed innovative strategies to overcome these obstacles. They have discovered that certain excited states of nuclei can exhibit longer lifetimes, providing a pathway for studying superheavy nuclei that might otherwise remain inaccessible.

Excited states are often stabilized by quantum effects, a phenomenon that holds great promise in the world of nuclear physics. The research team, led by Dr. Khuyagbaatar Jadambaa, posits that these long-lived excited states—affectionately referred to as isomers—frequently occur within superheavy nuclei possessing deformed configurations. These isomers serve to enrich the landscape of the island of stability, creating what can be termed as “clouds of stability” that float above the unstable seas of nuclear existence.

The researchers embarked on an ambitious quest to investigate the long-predicted yet seemingly elusive nucleus, Rf-252, utilizing an intense beam of titanium-50 produced at the renowned GSI/FAIR UNILAC accelerator. By cleverly fusing titanium nuclei with lead targets, the team generated a series of fusion products that were meticulously separated and analyzed using advanced instrumentation. Their experimental setup included the TransActinide Separator and Chemistry Apparatus (TASCA). The resulting products underwent detection through a sophisticated silicon detector following a rapid flight-time of approximately 0.6 microseconds.

Their painstaking efforts led to the successful identification and observation of 27 atoms of Rf-252, which were found to decay via fission, exhibiting a remarkable half-life of 13 microseconds. The rapid detection capabilities afforded by a fast digital data acquisition system, developed by GSI/FAIR’s Experiment Electronics department, facilitated the observation of electrons emitted during the decay process. Notably, traces of the isomer Rf-252m were identified, and in subsequent events, fission occurred within a mere 250 nanoseconds—a testament to the remarkable nature of this research endeavor.

The groundbreaking findings established a new benchmark within the realm of superheavy nuclear physics. The experimental evidence deduced a previously unexpected half-life of merely 60 nanoseconds for the ground state of Rf-252, thus securing its position as the shortest-lived superheavy nucleus known to science. This discovery dramatically shifts the previously established boundaries concerning the lifetimes of the heaviest nuclei, advancing the understanding of their properties, and setting the stage for further inquiries into complex phenomena such as isomer states and inverted fission stability.

Professor Christoph E. Düllmann, who leads the research department for superheavy element chemistry at GSI/FAIR, articulates the implications of this research: “The result decreases the lower limit of the known lifetimes of the heaviest nuclei by almost two orders of magnitude.” This profound revelation not only elevates our comprehension of the intricate behaviors of superheavy nuclei but also opens new avenues for exploration concerning isotopic borders within this scientific realm.

Looking ahead, the research team anticipates further experimental campaigns aimed at measuring isomeric states with inverted fission stability in the next heavier element seaborgium (Sg). The successful synthesis of Sg isotopes with lifetimes below a microsecond could provide a deeper understanding of the isotopic border in superheavy elements. Furthermore, as the international facility FAIR continues construction in Darmstadt, the prospects for future research into novel phenomena related to superheavy elements appear promising.

As the scientific community eagerly reflects on the findings of this research endeavor, it becomes increasingly evident that the study of superheavy nuclei and their associated properties not only captivates the imagination but also has profound implications for the foundational understanding of nuclear stability. The work conducted by the dedicated team sheds light on the intricate balance between forces at play within atomic nuclei, paving the way for novel discoveries that lie beyond the boundaries of current knowledge.

In summary, the exploration of superheavy elements represents a frontier of scientific inquiry that continues to both challenge and invigorate the field of nuclear physics. By successfully identifying the superheavy nucleus rutherfordium-252 and elucidating its properties, researchers are progressively mapping the elusive island of stability—a testament to human curiosity and the relentless pursuit of knowledge in the world of atomic nuclei.

Subject of Research: Exploration of superheavy nuclides and their properties, specifically rutherfordium-252.
Article Title: Stepping into the Sea of Instability: The New Sub-μ⁢s Superheavy Nucleus 252Rf.
News Publication Date: 14-Jan-2025.
Web References: http://dx.doi.org/10.1103/PhysRevLett.134.022501.
References: Physical Review Letters.
Image Credits: Photo: J. Krier, GSI/FAIR.

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