Oct 20 – 23, 2026
RIKEN
Asia/Tokyo timezone
Registration deadline is October 12!!

Fine structure and hindrance in the 12C+12C fusion

Oct 20, 2026, 11:45 AM
25m
Headquarters Building 2F (RIKEN)

Headquarters Building 2F

RIKEN

2-1, Hirosawa, Wako, Saitama 351-0198, Japan
Invited Presentation Theoretical nuclear physics for astrophysics Scientific Session

Speaker

Kouichi Hagino (Department of Physics, Kyoto University)

Description

Recent experimental data have demonstrated that the coupled-channels
approach significantly overestimates fusion cross sections at deep subbarrier
energies. This phenomenon, referred to as fusion hindrance,
was first identified in the 60Ni+89Y system, and has subsequently been observed
in several other medium-heavy systems, such as 64Ni+64Ni. However, it remains
unclear to what extent fusion hindrance occurs in lighter systems, such as 12C+12C,
which are of critical importance to nuclear astrophysics.

In this contribution, I will present our recent reanalysis of fusion cross sections for
the 12C+12,13C systems and discuss the presence or absence of the fusion hindrance
phenomenon in these systems. I will also present our recent attempts to describe
fusion cross sections of these systems by combining a reaction model with shell model
calculations for the compound nuclei, 24,25Mg.

Category Theory

Author

Kouichi Hagino (Department of Physics, Kyoto University)

Presentation materials

There are no materials yet.