Scientists Recreate Rare Cosmic Reaction That Forges Universe's Most Elusive Elements
Breakthrough experiment measures key reaction creating selenium-74, shedding new light on supernova nucleosynthesis while revealing gaps in current theories.
Scientists have achieved a groundbreaking milestone in understanding how some of the universe's rarest elements are forged, directly measuring a cosmic reaction that has never been observed in laboratory conditions before. The experiment focused on selenium-74, one of the mysterious proton-rich isotopes known as p-nuclei that cannot be created through the neutron-capture processes that form most heavy elements.
The research team, led by Artemis Tsantiri at the Facility for Rare Isotope Beams (FRIB), successfully measured how arsenic-73 captures a proton to form selenium-74 using rare isotope beams. This represents the first direct observation of a key reaction in the gamma process, which scientists believe occurs during certain types of supernova explosions when intense gamma rays strip neutrons from existing heavy nuclei.
The findings, published in Physical Review Letters, involved more than 45 scientists from 20 institutions across the United States, Canada, and Europe. The results have cut uncertainty in supernova models by half, providing crucial data for understanding how these rare elements are distributed throughout the universe. However, the measurements also revealed significant gaps in current theoretical predictions.
The gamma process occurs in extreme stellar environments where temperatures reach billions of degrees and gamma radiation is intense enough to fundamentally alter atomic nuclei. During this process, gamma rays strip particles from heavy elements, leaving behind proton-rich isotopes that eventually decay into the stable p-nuclei found in meteorites and planetary materials today.
This breakthrough was only possible due to advances in rare isotope beam technology at facilities like FRIB. The ability to create and study short-lived isotopes like arsenic-73 opens new possibilities for testing theoretical models of stellar nucleosynthesis and understanding the cosmic origins of elements that are essential for planetary formation and life itself.
Originally reported by ScienceDaily Physics.