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 …

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

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 …

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 …

Infrared and ultraviolet observations of nova light curves have confirmed grain formation in
their expanding shells that are ejected into the interstellar medium by a thermonuclear …

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 …

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 Trojan Horse Method represents an indirect approach to investigate reactions of
astrophysical relevance at the energies of interest, free of Coulomb suppression and …

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