Neutron-induced reactions in nuclear astrophysics
Ren\'e Reifarth, David Brown, Saed Dababneh, Yuri A. Litvinov, Shea M., Mosby

TL;DR
This paper discusses the importance of neutron-induced reactions in understanding the origin of elements and proposes advanced experimental methods involving ion storage rings and neutron sources to measure these reactions on radioactive isotopes.
Contribution
It introduces a novel approach combining radioactive ion beams, storage rings, and high-flux neutron sources to measure neutron-induced reactions on short-lived isotopes.
Findings
Proposes a method for direct measurement of neutron reactions on radioactive ions.
Highlights the potential of storage rings with neutron sources for nuclear astrophysics.
Identifies key neutron-induced reactions relevant to element formation.
Abstract
The quest for the origin of the chemical elements, which we find in our body, in our planet (Earth), in our star (Sun), or in our galaxy (Milky Way) could only be resolved with a thorough understanding of the nuclear physics properties of stable and unstable atomic nuclei. While the elements until iron are either created during the big bang or during fusion reactions in stars, most of the elements heavier than iron are produced via neutron-induced reactions. Therefore, neutron capture cross sections of stable and unstable isotopes are important. So far, time-of-flight or activation methods have been applied very successfully, but these methods reach their limits once the isotopes with half-lives shorter than a few months are of interest. A combination of a radioactive beam facility, an ion storage ring and a high flux reactor or a spallation source would allow a direct measurement of…
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Taxonomy
TopicsNuclear physics research studies · Astronomical and nuclear sciences · Nuclear Physics and Applications
