In most nuclei the protons and neutrons form a roughly spherical core of approximately uniform density. But along the edges—the so-called drip lines—of the chart of nuclides a handful of light nuclei have more nucleons than can be accommodated in the nuclear core. The excess, usually one or two neutrons, form a dilute distribution called a halo that extends far beyond the core. At the RIKEN Nishina Center for Accelerator-Based Science, a Japanese team has studied the reaction of heavy carbon nuclei with hydrogen and identified the extremely neutron-rich carbon-22, with its 6 protons and 16 neutrons, as a halo nucleus, the heaviest one yet found. Nuclear radii generally scale as the cube root of the total number of protons and neutrons, yet based on their cross-section data, the researchers calculated the radius of 22C to be twice that of the much more common isotope 12C; indeed, at 5.4 fm it exceeds the radius of lead-208. The halo of 22C comprises two valence neutrons; determining their distribution and other aspects of the halo structure will require experiments with different target nuclei and different beam energies. (K. Tanaka et al., Phys. Rev. Lett., in press.)—Richard Fitzgerald
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As a physics guy with a love of nuclear physics and QCD, the study of extreme limits of low atomic number elemental isotopes can give us a better understanding of QCD physics.
I am interested in extreme low atomic number isotopes for the possible role they can play in high energy density materials.
Perhaps such high energy density materials might make excellent compact power sources for deep space manned rockets. We need to get beyond chemical combustion rockets if we are going to do manned missions to the outer reaches of the solar system and beyond, and so I am all for any advances in safe ultra-high density nuclear materials.
If nuclear chemists can come up with stable extreme low atomic number isotopes, the controversey over nuclear power systems in space might be effectively eliminated.