X-ray binaries are among the brightest extra-solar objects in the sky and are characterized
by dramatic variabilities in brightness on timescales ranging from milliseconds to months …

New experimental methods and techniques, combined with the development of new
theoretical tools, have opened new avenues to explore nuclear reactions of significance for …

We present results from the JINA REACLIB project, an ongoing effort to maintain a current
and accurate library of thermonuclear reaction rates for astrophysical applications. Ongoing …

Numerical values of charged-particle thermonuclear reaction rates for nuclei in the A= 14 to
40 region are tabulated. The results are obtained using a method, based on Monte Carlo …

Isospin-symmetry breaking is responsible for the energy difference of excited states in mirror
nuclei. It also influences the coefficient of the isobaric multiplet mass equation. In the present …

We investigate the effects of thermonuclear reaction-rate uncertainties on nova
nucleosynthesis. One-zone nucleosynthesis calculations have been performed by adopting …

Nuclear astrophysics is a field at the intersection of nuclear physics and astrophysics, which
seeks to understand the nuclear engines of astronomical objects and the origin of the …

The nuclear physics input used to compute the Monte Carlo reaction rates and probability
density functions that are tabulated in the second paper of this series (Paper II) is presented …

Abstract Knowledge of the astrophysical rate of the 18 F (p, α) 15 O reaction is important for
understanding the γ-ray emission expected from novae and heavy-element production in x …

The quest to comprehend how nuclear processes influence astrophysical phenomena is
driving experimental and theoretical research programs worldwide. One of the main goals in …