Speaker
Description
The solenoidal-spectrometer technique was developed at Argonne over 15 years ago and realized in the form of HELIOS; successful programs have since been established at ISOLDE with the ISS and at FRIB with SOLARIS. I will highlight a few recent developments and results, as well as possible future directions for this technique. An overarching output of the solenoidal-spectrometer programs at Argonne, CERN, and FRIB has been the determination of single-particle energies in weakly bound nuclei across the chart of nuclides, revealing an emerging picture of how structure evolves towards the particle threshold. This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Contract Number DE-
AC02-06CH11357
