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In-beam Spectroscopy

A brief description of in-beam γ-ray spectroscopy techniques is provided aiming at N~Z nuclei at or beyond the proton dripline.

Ground states of odd-Z isotopes with neutron numbers, N, being less than their proton number, Z, are weakly if at all bound against the emission of protons in the region between N=Z=28 56Ni and N=Z=50 100Sn. An explanation for the lack of experimental information on those nuclei thus lies in their intertwined challenge and interest: weak nuclear binding requires comprehensive experiments including dedicated detection systems to be sensitive to fast proton emission in direct competition to γ-ray emission of quasibound nuclear quantum states beyond the proton dripline.

The nuclei of interest are formed in fusion-evaporation reactions such as, for example, 40Ca+24Mg → 64Ge*. Following rare cases of evaporating one proton and two neutrons from a highly-excited 64Ge* compound nucleus, excited states in 61Ga can be populated, which is an exotic N<Z isotope of gallium (Z=31). 

The γ rays are detected in multi-germanium detector arrays such as GAMMASPHERE, illustrated to the right. To associate γ rays with a certain isotope, one can either measure the evaporated particles (see right) or the recoiling nuclei, or both. To conduct proton-γ peak-peak coincidence spectroscopy, the charged particles must be detected in a dedicated detector system, in our case comprising two CD-shaped double-sided Si-strip detectors (DSSD). They provide 2x2048 detector pixels to allow for high angular and thus energy resolution measurements of proton energies as well as beam-position tracking, which is a novel feature in this context.

Owing to the setup's unprecedented in-beam proton spectroscopy and tracking capabilities, a coincidence between a 957.6-keV γ ray and a 1.876-MeV proton line was observed, which identified the quasi-bound proton g9/2 single-particle state in 61Ga. This coincidence is shown in the decay scheme of 61Ga to the right, together with the γ-ray and proton energy spectra. Both spectra are conditioned with a final residue of mass number A=60, because the emission of a proton from states in 61Ga lead to states in N=Z 60Zn, a minimum of three detected γ rays as well as a maximum of two detected protons, and certain sum-energies of γ rays and particles. 

In terms of physics, this observation probes isospin-symmetry at the limit of nuclear binding by providing a unique challenge for the shell-model interpretation of mirror nuclei beyond doubly-magic 56Ni. In terms of instrumentation, the set-up serves as template for future explorations of nuclei along and beyond the proton dripline. 

For more details, see the respective publication in Physical Review Letters or Yuliia Hrabar's PhD thesis.

Gammasphere plus Microball and Neutron Shell
Gammasphere (open) in combination with the ancillary detectors Microball (inside the opened target chamber) and Neutron Shell (red and green elements, downstream). Courtesy D.G. Sarantites.
Proton-gamma coincidence 61Ga
Decay scheme of the proton-dripline nucleus 61Ga together with proton-γ coincidence spectra.