Nuclear reactions induced by photons play a vital role for very different aspects of basic
research and applications in physics. They are a key ingredient for the synthesis of nuclei in …

The Trojan Horse Method (THM) represents an indirect path to determine the bare nucleus
astrophysical S-factor for reactions among charged particles at astrophysical energies. This …

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 …

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 …

Classical novae are dramatic stellar explosions with an energy release that is only
overcome by supernovae and gamma-ray bursts. These unique cataclysmic events …

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

Classical novae are fascinating stellar explosions at the crossroads of stellar astrophysics,
nuclear physics, and cosmochemistry. In this review, we briefly summarize 30 years of …

The best examples of halo nuclei, exotic systems with a diffuse nuclear cloud surrounding a
tightly bound core, are found in the light, neutron-rich region, where the halo neutrons …

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

Measurement of nuclear cross sections at astrophysical energies involving unstable species
is one of the most challenging tasks in experimental nuclear physics. The use of indirect …