The available data on nuclear fusion cross sections important to energy generation in the
Sun and other hydrogen-burning stars and to solar neutrino production are summarized and …

In this review, we discuss the present status of three indirect techniques that are used to
determine reaction rates for stellar burning processes, asymptotic normalization coefficients …

ABSTRACT STARLIB is a next-generation, all-purpose nuclear reaction-rate library. For the
first time, this library provides the rate probability density at all temperature grid points for …

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 …

A large sample of carbon-enhanced metal-poor stars enriched in s-process elements
(CEMP-s) have been observed in the Galactic halo. These stars of low mass (M∼ 0.9 M⊙) …

We present computations of nucleosynthesis in low-mass (LM) red giant branch (RGB) and
asymptotic giant branch (AGB) stars of Population I experiencing extended mixing. We adopt …

The cross sections of the 2 H (d, p) 3 H and 2 H (d, n) 3 He reactions have been measured
via the Trojan Horse method applied to the quasi-free 2 H (3 He, p 3 H) 1 H and 2 H (3 He, n …

ABSTRACT The 19 F (p, α) 16 O reaction is an important fluorine destruction channel in the
proton-rich outer layers of asymptotic giant branch (AGB) stars and it might also play a role …

The study of energy production and nucleosynthesis in stars requires an increasingly
precise knowledge of the nuclear reaction rates at the energies of interest. To overcome the …

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