出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：In an experiment at the RecoilMass Spectrometer of the HRIBF at ORNL the alpha decay branch
of 109I was discovered. The measurement of its decay energy allowed for the indirect determination
of the proton separation energy in the daughter nucleus 105Sb. The deduced Sp(105Sb)=-
356(22) keV is about 130 keV larger than the previously claimed value. The consequences of this
measurement for the astrophysical rp-process will be discussed.
