“…where ε F , m, and r 2 are the Fermi energy, nucleon mass, and mean square radius, respectively. Initial indications of the excitation of the ISGDR were reported as early as the beginning of the 1980s [4][5][6]. However, the first direct evidence for this mode, based on the differences in angular distribution of the ISGDR from that of the nearby highenergy octupole resonance (HEOR), was provided by Davis et al [7], who demonstrated that in 200 MeV inelastic α-scattering near 0 • , the giant resonance "bump" at 3hω excitation energy could be separated into two components, with the higher-energy component corresponding to the ISGDR.…”