1986
DOI: 10.1103/physrevc.33.2054
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Inelastic proton excitation of high-lying giant resonances

Abstract: Inelastic scattering of 800 Me Y protons has been studied for targets of~Pb, '~Sm, and " Sn. At excitation energies above particle emission threshold a spectrum of giant resonances is clearly in evidence. Angular distributions~ere extracted for the high-lying peaks (-20 MeV excitation energy) in Pb and ' Sm. Collective model distorted-wave Born approximation analyses of these data show that isoscalar octupole and dipole states dominate the spectra.

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Cited by 29 publications
(16 citation statements)
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“…The mode is viewed as a compression wave in a definite direction and so is related to the nuclear incompressibility [16,19]. The isoscalar (T=0) TM and CM were observed in (α, α ′ )-reaction as broad low-energy (TM dominated) and high-energy (CM dominated) electric dipole distributions [14,18,[20][21][22][23][24][25]. The TM was also investigated in the region of the pygmy resonance in 208 Pb in a nuclear fluorescence experiment [26].…”
Section: Introductionmentioning
confidence: 99%
“…The mode is viewed as a compression wave in a definite direction and so is related to the nuclear incompressibility [16,19]. The isoscalar (T=0) TM and CM were observed in (α, α ′ )-reaction as broad low-energy (TM dominated) and high-energy (CM dominated) electric dipole distributions [14,18,[20][21][22][23][24][25]. The TM was also investigated in the region of the pygmy resonance in 208 Pb in a nuclear fluorescence experiment [26].…”
Section: Introductionmentioning
confidence: 99%
“…Although measurements of the giant monopole resonance [10,11] and the isoscalar giant dipole resonance [12][13][14] have existed for some time, the field has seen a revitalization due to new and improved measurements of both compressional modes [15][16][17]. The field has also seen significant advances in the theoretical domain.…”
Section: Introductionmentioning
confidence: 99%
“…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.…”
mentioning
confidence: 99%
“…The problem arose when one compared the available ISGDR data with the theoretical centroids of the ISGDR, calculated using the same interactions that appear to reproduce the available ISGMR data well [11][12][13][14][15][16]. The experimental centroids reported by Clark et al [8] were significantly lower than the calculated centroids; for example, in 208 Pb, Clark et al reported the ISGDR centroid at 19.9 ± 0.8 MeV lower than previous experimental results [4][5][6][7] and also lower than theoretical values of E x > 22 MeV. The low values for the centroids in the data of Clark et al evidently resulted from their background-subtraction procedure which rendered the ISGDR strength zero at E x > 24 MeV.…”
mentioning
confidence: 99%