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 …

Abstract The Trojan Horse Method (THM) lays its foundations on the cluster structure of light
nuclei which are usually used as “Trojan horses”. Many of them were successfully employed …

The Coulomb-free 1 S 0 proton-proton (pp) scattering length relies heavily on numerous and
distinct theoretical techniques to remove the Coulomb contribution. Here, it has been …

We study the dependence of the primordial nuclear abundances as a function of the
electromagnetic fine-structure constant α, keeping all other fundamental constants fixed. We …

The 26 Al abundance holds a special role in present-day astrophysics, since it is a probe of
active nucleosynthesis in the Galaxy and a valuable constraint of Galactic core-collapse …

A large uncertainty for the slow neutron capture nucleosynthesis (s-process) models is
caused by the amount of neutrons available to the process itself. This quantity is strongly …

Asymptotic Giant Branch (AGB) stars are among the most important astrophysical sites
influencing the nucleosynthesis and the chemical abundances in the Universe. From a pure …

Abstract The 27 Al (p, α) 24 Mg reaction, which drives the destruction of 27 Al and the
production of 24 Mg in stellar hydrogen burning, has been investigated via the Trojan Horse …

Fluorine is one of the most interesting elements in nuclear astrophysics. Its abundance can
provide important hints to constrain the stellar models since fluorine production and …

Abstract Big Bang Nucleosynthesis (BBN) requires several nuclear physics inputs and
nuclear reaction rates. An up-to-date compilation of direct cross sections of is given, being …