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• W2104833182 endingPage "1847" @default.
• W2104833182 startingPage "1832" @default.
• W2104833182 abstract "Giant resonance spectra have been measured for $^{208}mathrm{Pb}$, $^{120}mathrm{Sn}$, $^{90}mathrm{Zr}$, $^{58}mathrm{Ni}$, and $^{46}mathrm{Ti}$, using inelastic scattering of 152-MeV alpha particles. In addition to some low-lying states, the spectra were analyzed to yield separate peaks for the giant quadrupole resonance and giant monopole resonance, except in $^{46}mathrm{Ti}$, where no evidence was found for a giant monopole resonance. The results for the monopole resonance when compared to distorted-wave Born-approximation calculations show that ensuremath{sim}100% (ifmmodepmelsetextpmfi{}20%) of the $T=0$, $L=0$ energy weighted sum rule is depleted for nuclei with $A>90$. For $^{58}mathrm{Ni}$ only 40% of the monopole sum rule is found. The excitation energy of the giant monopole resonance follows the systematic trend $ensuremath{sim}80{A}^{ensuremath{-}frac{1}{3}}$ MeV. The data are also compared with folding model calculations using Tassie transition densities and an effective interaction derived from elastic data. Good agreement was obtained for low-lying quadrupole and octopole excitations, but this model yields considerably too little cross section for the monopole resonance. This probably indicates a deficiency in the Tassie model breathing mode transition density.NUCLEAR REACTIONS $^{208}mathrm{Pb}$, $^{120}mathrm{Sn}$, $^{90}mathrm{Zr}$, $^{58}mathrm{Ni}$, $^{46}mathrm{Ti}(ensuremath{alpha}, {ensuremath{alpha}}^{ensuremath{'}})$, ${E}_{ensuremath{alpha}}=152$ MeV, ${E}_{ensuremath{chi}}=0ensuremath{-}40$ MeV; measured $ensuremath{sigma}({E}_{ensuremath{chi}}, ensuremath{theta})$; discuss giant resonances, folding model calculations, deduced $L$, ${ensuremath{beta}}_{L}$." @default.
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• W2104833182 date "1980-11-01" @default.
• W2104833182 modified "2023-09-25" @default.
• W2104833182 title "Giant multipole resonances from inelastic scattering of 152-MeV alpha particles" @default.
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• W2104833182 doi "https://doi.org/10.1103/physrevc.22.1832" @default.
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