The evolution of the giant dipole resonance (GDR) in ~2ยฐSn and 2ยฐ8pb nuclei at excitation energies in the range of 30-130 MeV and 40-110 MeV, respectively, were studied by measuring high energy y rays from the decay of the resonance. The excited states were populated by inelastic scattering of a par
Behavior of the giant-dipole resonance in 120Sn and 208Pb at high excitation energy
โ Scribed by W.E. Ormand; P.F. Bortignon; R.A. Broglia; A. Bracco
- Publisher
- Elsevier Science
- Year
- 1997
- Tongue
- English
- Weight
- 1019 KB
- Volume
- 614
- Category
- Article
- ISSN
- 0375-9474
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โฆ Synopsis
The properties of the giant-dipole resonance (GDR) are calculated as a function of excitation energy, angular momentum, and the compound nucleus particle decay width in the nuclei 12ยฐSn and 2ยฐspb, and are compared with recent experimental data. Differences observed in the behavior of the full-width-at-half-maximum of the GDR for ~2ยฐSn and maPb are attributed to the fact that shell corrections in 2ยฐspb are stronger than in ~2ยฐSn, and favor the spherical shape at low temperatures. The effects shell corrections have on both the free energy and the moments of inertia are discussed in detail. At high temperature, the FWHM in mยฐSn exhibits effects due to the evaporation width of the compound nucleus, while these effects are predicted for 2ยฐspb.
๐ SIMILAR VOLUMES
The giant resonance regions ofgยฐzr, UfSn, t44Sm and 2ยฐspb were investigated using 240 MeV et particle scattering at small angles including 0 ยฐ. E1 strengths corresponding to 91+11%, 89\_+10%, 105+12% and 95+13% of the isoscalar E1 energy-weighted sum rule were identified between 18<\_E~<31 MeV, 16<\