Selected Publications: α Decay of 109I and Its Implications
for the Proton Decay of 105Sb
and the Astrophysical Rapid Proton-Capture
Process, C. Mazzocchi, Phys. Rev. Lett. 98,
212501 (2007)
First observation of beta-delayed
three-proton emission in 45Fe,
K. Miernik, Phys. Rev. Lett. 99, 192501 (2007)
Discovery of 109Xe and 105Te:
Superallowed α Decay near DoublyMagic 100Sn, S.N. Liddick, Phys. Rev. Lett.
97, 082501 (2006)
Half-life and spin of 60Mng,
S.N. Liddick, Phys.Rev. C 73, 044322 (2006)
Lowest Excitations in 56Ti and the
Predicted N = 34 Shell Closure, S.N.Liddick,
Phys. Rev.Lett. 92, 072502 (2004)
My research focuses on experimentally identifying changes in nuclear structure far from the valley of beta stability. The changes are the result of evolving single-particle level configurations as a progression is made from stability towards more exotic nuclei and leads to specific observables in the low-energy level structure of a nucleus. Decay spectroscopy provides a sensitive and selective means to populate and study low-energy excited states of daughter nuclei looking for the signatures of changing shell structure. A variety of different decay modes can be employed depending on the nucleus of interest and the experimental setup and can include beta, alpha, and proton decay. Experiments have been performed both on the neutron-deficient nuclei near 100Sn and neutron-rich nuclei near 78Ni.
Alpha decay experiments near 100Sn, originally intended to look for fast alpha decays, have instead demonstrated an unexpected inversion in the ordering of the single-particle states along the Sn isotonic chain between 101Sn and 103Sn in comparison to theoretical predictions. The inversion indicates a rapid transition between a nucleus which can be described by single-particle excitations (101Sn) and a nucleus which displays a large amount of collectivity (103Sn). That such a discrepancy occurred demonstrated the danger of extrapolating nuclear structure information from nuclei closer to stability and the need for continued experimental investigation.
Characteristic waveform resulting from the pile-up of two sequential alpha decays: 109Xe -> 105Te (blue) and 105Te -> 101Sn (red). The height of the individual alpha signals are reconstructed offline and the resulting alpha decay energy spectra for both 109Xe and 105Te are shown as insets.
In the neutron-rich region near 78Ni, in additional to exploring the evolution of nuclear structure, decay spectroscopy is also useful in trying to understand explosive astrophysical processes responsible for the synthesis of elements heavier than Fe. The pattern of nuclear abundances following an r-process is significantly influenced by beta-decay half-lives most of which are unknown and extracted from theoretical calculations. Further, the abundances of stable nuclei produced from the r-process is altered as the nuclei produced decay back to stability due to the possibility of beta-delayed neutron emission which shifts abundances to lower mass chains. The probability of beta-delayed neutron emission in neutron-rich nuclei can be large and investigations along the Cu isotonic chain have identified large discrepancies between current and previous experimental values for the neutron emission probabilities.
The development of new detectors and techniques is critical to improving the sensitivity of the experimental system enabling access to increasingly exotic nuclei. The implementation of a digital acquisition system in the detection of alpha decays was critical for the detection of the single-particle level inversion near 100Sn. The digital electronics enabled the capture of two sequential alpha decays from 109Xe and 105Te. In addition to digital electronics, a new planar Ge detector is being developed for decay spectroscopy experiments and the two improvements combined offer both increased detection efficiencies and the ability for novel experiments.