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The neutron-rich nucleus Ba-144 (t(1/2) = 11.5 s) is expected to exhibit some of the strongest octupole correlations among nuclei with mass numbers A less than 200. Until now, indirect evidence for such strong correlations has been...
Carbon burning is a critical phase for nucleosynthesis in massive stars. The conditions for igniting this burning stage, and the subsequent isotope composition of the resulting ashes, depend strongly on the reaction rate for C-12 + C-12...
We have studied the C-14, C-15(d, He-3)B-13, B-14 proton-removing reactions in inverse kinematics. The (d, He-3) reaction probes the proton occupation of the target ground state, and also provides spectroscopic information about the final...
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