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Keyword:n_TOF

CERN measures niobium-94 neutron capture for the first time, shedding new light on the mystery of molybdenum abundance in ancient stardust

CERN measures niobium-94 neutron capture for the first time, shedding new light on the mystery of molybdenum abundance in ancient stardust

The n_TOF collaboration at CERN recently reported that researchers have for the first time measured the probability of neutron capture by niobium-94. The results, published in Physical Review Letters, provide new experimental evidence for explaining the anomalous abundance of molybdenum-94 in presolar grains. The EAR2 facility in the n_TOF experiment at CERN produces intense neutron beams, opening new possibilities for nuclear research. Credit: CERN Niobium-94 is a niobium isotope containing 41 protons and 53 neutrons, occupying a critical juncture in the nuclear reaction chain that produces heavy elements in dying stars. Researchers are interested in it because niobium-94 is very close to molybdenum-94, differing by just one fewer proton and one more neutron. Under the high-temperature, high-pressure conditions inside stars, niobium-94 may either transform into molybdenum-94 through beta decay or form niobium-95 through neutron capture. The competition between these two reaction pathways directly affects scientists' understanding of the origin of molybdenum-94.

2026-08-20

International Team Measures Niobium-94 Neutron Reactions, Explaining Anomalous Molybdenum-94 Abundance in the Solar System

International Team Measures Niobium-94 Neutron Reactions, Explaining Anomalous Molybdenum-94 Abundance in the Solar System

An international team of physicists has, for the first time, conducted a comprehensive study of the interactions between neutrons and the niobium-94 isotope. The findings have been published in Physical Review Letters. The study suggests that the elevated abundance of molybdenum-94 in the primordial material of the solar system can be explained by a series of neutron-involving nuclear reaction processes inside old stars, without requiring the introduction of previously unknown special formation mechanisms. The research was led by Alberto Mengoni, a researcher at the Italian National Institute for Nuclear Physics. The team conducted experiments using the n_TOF facility at CERN, focusing on tracking the interactions between neutrons and niobium-94 atoms. The n_TOF facility is used to...

2026-08-11