T. Pennington

Influence of Nuclear Structure on Sub-Barrier Hindrance in Ni + Ni Fusion

Fusion-evaporation cross sections for

Hindrance of heavy-ion fusion at extreme sub-barrier energies in open-shell colliding systems

^{64}

Stellar (n, gamma) Cross Section of ^6^2Ni

Ni+

{sup 40}Ca({alpha},{gamma}){sup 44}Ti Reaction in the Energy Regime of Supernova Nucleosynthesis

^{64}

Branching ratio Γ α / Γ γ of the 4.033 MeV 3 / 2 + state in 19 Ne

Ni have been measured down to the 10 nb level. For fusion between two open-shell nuclei, this is the first observation of a maximum in the

Variation with mass of B ( E 3 ; 0 1 + → 3 1 − ) transition rates in A = 124 − 134 even-mass xenon nuclei

S

Towards measuring the charge radius of 6He and 8He

-factor, which signals a strong sub-barrier hindrance. A comparison with the

Counting 44Ti nuclei from the 40Ca(α,γ)44Ti reaction

^{58}

Systematics of Heavy-Ion Fusion Reactions at Extreme Sub-Barrier Energies

Ni+

Study of the 8B neutrino spectrum with a new technique

^{58}