In stars that lie on the main sequence in the Hertzsprung Russel diagram, like our sun,
hydrogen is fused to helium in a number of nuclear reaction chains and series, such as the …

We explore neutrino emission from nonrotating, single-star models across six initial
metallicities and 70 initial masses from the zero-age main sequence to the final fate. Overall …

Classical novae are one of the most frequent explosive nucleosynthesis events in our
universe but are still not sufficiently understood. To this day, nuclear astrophysics cannot …

Low energy particle accelerators, located at deep underground locations, have been
developed over the last three decades, to perform nuclear reaction measurements at nearly …

The star-to-star anticorrelation of sodium and oxygen is a defining feature of globular
clusters, but, to date, the astrophysical site responsible for this unique chemical signature …

The star-to-star anticorrelation of sodium and oxygen is a defining feature of globular
clusters, but, to date, the astrophysical site responsible for this unique chemical signature …

Stars generate a variety of multi-messenger signals throughout their evolution. They radiate
photons from their stellar surface, neutrinos from their interior, and recentlydiscovered …

Stars produce most of elements in the universe out of primordial nuclei, H and He. Nuclear
fusion reactions taking place deep inside stellar cores both provide the energy to keep stars …