Narrow Results

Evidence for the possible existence of a superheavy nucleus with atomic mass number A = 292 and abundance of about 1×10^-12 relative to ²³²Th has been found in a study of natural Th using inductively coupled plasma-sector field mass spectrometry. The measured mass is different from any species with molecular mass of 292, but it matches the predictions for the mass of an isotope with atomic number Z = 122 or a nearby element. Its deduced half-life of t_1/2 ≥ 10⁸ y suggests that a long-lived isomeric state exists in this isotope. The possibility that it might belong to a new class of long-lived high spin super- and hyperdeformed isomeric states is discussed.

Current data (by September 2007) on masses of neutron stars in binary systems (X-ray binaries, double neutron star binaries, pulsar–white dwarf binaries, and pulsar–nondegenerate star binaries) are reviewed.