In this review, we discuss recent advancements in the study of clustering phenomena
occurring in light nuclei, and their influence on nuclear structure, dynamics, and …

The C 12/C 13 ratio is a significant indicator of nucleosynthesis and mixing processes during
hydrogen burning in stars. Its value mainly depends on the relative rates of the C 12 (p, γ) N …

The C 12 (p, γ) N 13 reaction is the onset process of both the CNO and hot CNO cycles that
drive massive star, red and asymptotic giant branch star, and novae nucleosynthesis. The C …

Solar neutrino measurements have recently reached a level of sensitivity such that CNO
fluxes can now be experimentally determined. While these first measurements are still only …

Abstract The 11 B (10 B, 9 Be) 12 C reaction was studied at the energy of 41.3 MeV with
transitions to the ground (0+) and low-lying excited 4.44 MeV (2+) and 9.64 MeV (3−) states …

The reactions involving the nucleons transfer in the interactions of light ions near the
Coulomb barrier are very informative on research of the structure of nuclear single-particle …

The astrophysical S-factor of the 12C (p, γ0) 13N reaction at energies from 25 keV to 5 MeV
within the framework of a modified potential cluster model with forbidden states is …

Precise knowledge of the 12 C (p, γ) 13 N reaction cross section is crucial to understand the
evolution of various types of red giant stars and to explain their astronomically observed …

The main purpose of this work is to determine values of the asymptotic normalization coe±-
cients for the virtual decays 6He+ p! 7Li (gs) and 6He+ p! 7Li (0.48 MeV). For this purpose …

Abstract (DE) Ein präzises Verständnis über die Entstehung der Elemente im Universum
stellt ein hoch-relevantes Kernthema der nuklearen Astrophysik dar. Vor diesem …