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 …

Atomic nuclei are composite systems, and they may be dynamically excited during nuclear
reactions. Such excitations are not only relevant to inelastic scattering but they also affect …

Carbon burning powers scenarios that influence the fate of stars, such as the late
evolutionary stages of massive stars (exceeding eight solar masses) and superbursts from …

LASER DRIVEN NUCLEAR PHYSICS AT ELINP Page 1 Romanian Reports in Physics, Vol. 68,
Supplement, P. S37–S144, 2016 LASER DRIVEN NUCLEAR PHYSICS AT ELINP F …

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 …

Fluorine abundance determination is of great importance in stellar physics to understand s-
elements production and mixing processes in asymptotic giant branch (AGB) stars. Up to …

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 …

Nuclear reaction rates are among the most important input for understanding primordial
nucleosynthesis and, therefore, for a quantitative description of the early universe. An up-to …

In this review, we discuss the new recent results of the Trojan Horse Method that is used to
determine reaction rates for nuclear processes in several astrophysical scenarios. The …

Experimental studies of nuclear collisions involving light weakly bound nuclei show a
systematic suppression of the complete fusion cross section by∼ 30% with respect to the …