We study the s-process abundances (A≳ 90) at the epoch of the solar system formation.
Asymptotic giant branch yields are computed with an updated neutron capture network and …

We provide a set of stellar evolution and nucleosynthesis calculations that applies
established physics assumptions simultaneously to low-and intermediate-mass and massive …

Nuclear data in general, and neutron-induced reaction cross sections in particular, are
important for a wide variety of research fields. They play a key role in the safety and criticality …

Neutron-induced nuclear reactions are of key importance for a variety of applications in
basic and applied science. Apart from nuclear reactors, accelerator-based neutron sources …

The competing $^{22} $ Ne ($\alpha,\gamma $) $^{26} $ Mg and $^{22} $ Ne ($\alpha, n $)
$^{25} $ Mg reactions control the production of neutrons for the weak $ s $-process in …

This paper provides a detailed analysis of the main component of the slow neutron capture
process (the s-process), which accounts for the solar abundances of half of the nuclei with …

The interplay and correlation between the 22 Ne (α, γ) 26 Mg and the competing 22 Ne (α, n)
25 Mg reaction plays an important role for the interpretation of the 22 Ne (α, n) 25 Mg …

Abstract i-TED is an innovative detection system which exploits Compton imaging
techniques to achieve a superior signal-to-background ratio in (n, γ) cross-section …

Neutron capture cross section measurements in time-of-flight facilities are usually performed
by detecting the prompt γ-rays emitted in the capture reactions. One of the difficulties to be …

The radioisotope 26 Al is a key observable for nucleosynthesis in the Galaxy and the
environment of the early Solar System. To properly interpret the large variety of astronomical …