Optimizing charge breeding techniques for ISOL facilities in Europe: conclusions from the EMILIE project

2015

ThuM07; International audience; The present paper summarizes the results obtained from the past few years in the framework ofthe Enhanced Multi-Ionization of short-Lived Isotopes for Eurisol (EMILIE) project. The EMILIEproject aims at improving the charge breeding techniques with both Electron Cyclotron ResonanceIon Sources (ECRIS) and Electron Beam Ion Sources (EBISs) for European Radioactive Ion Beam(RIB) facilities. Within EMILIE, an original technique for debunching the beam from EBIS chargebreeders is being developed, for making an optimal use of the capabilities of CW post-acceleratorsof the future facilities. Such a debunching technique should eventually resolve duty cycle andtime st…

New exotic beams from the SPIRAL 1 upgrade

2018

Since 2001, the SPIRAL 1 facility has been one of the pioneering facilities in ISOL techniques for reaccelerating radioactive ion beams: the fragmentation of the heavy ion beams of GANIL on graphite targets and subsequent ionization in the Nanogan ECR ion source has permitted to deliver beams of gaseous elements (He, N, O, F, Ne, Ar, Kr) to numerous experiments. Thanks to the CIME cyclotron, energies up to 20 AMeV could be obtained. In 2014, the facility was stopped to undertake a major upgrade, with the aim to extend the production capabilities of SPIRAL 1 to a number of new elements. This upgrade, which is presently under commissioning, consists in the integration of an ECR booster in the…

Production and isobaric separation of 63Ni ions for determination of the 62Ni(n,γ)63Ni reaction cross section at stellar temperatures

2004

Stellar(n,γ)Cross Section ofNi62

2005

The 62Ni(n,gamma)63Ni(t(1/2)=100+/-2 yr) reaction plays an important role in the control of the flow path of the slow neutron-capture (s) nucleosynthesis process. We have measured for the first time the total cross section of this reaction for a quasi-Maxwellian (kT=25 keV) neutron flux. The measurement was performed by fast-neutron activation, combined with accelerator mass spectrometry to detect directly the 63Ni product nuclei. The experimental value of 28.4+/-2.8 mb, fairly consistent with a recent calculation, affects the calculated net yield of 62Ni itself and the whole distribution of nuclei with 62<A<90 produced by the weak s process in massive stars.