Figure 1 - uploaded by D. R. Napoli
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Chart of nuclides in region of interest. The target, 124 50 Sn and the beam 96 40 Zr are highlighted as well as the 95 Nb nucleus.
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... desired neutron-rich region is difficult to access with fusion-evaporation reactions using stable nuclear beams. Instead, deep inelastic binary reactions have been successfully utilized in recent years. The reaction presented in this contribution was initiated by a beam of 96 40 Zr incident on a target of 124 50 Sn. Here a study of the 95 41 Nb level scheme constructed from the data obtained of PRISMA-CLARA and GASP experiments is presented. The region of interest of this work can be located in the chart of nuclides in Fig. 1 where the location of the beam, the target and the 95 Nb nuclei has been highlighted. In the next section a description of the experiments is shown. In section 3 the level scheme obtained in this work is compared by the previous one obtained by Bucurescu et al. [3]. Finally, in section 4, a comparison of the experimental results with predictions from shell model calculations is ...
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... It made the projectile-like fragments to stop inside the GASP multidetector array. A complete description of the experiments was made in a previous work [6]. A summary of main experimental details of both experiments is shown in Table 1 From this spectrum most of the lines in the level scheme proposed in the most recent work on excited states of 95 Nb nucleus [3] can be seen, as well as two more peaks at energies 795 keV and 1233 keV. ...
... a Theoretical value of A 2 /A 0 for transitions of the type E2-E2 conecting levels with spins 2 −→ 0 is 0.102 A discussion of the intensities of the γ-rays reported in Table 2 was carried out in a previous work [6]. A special discussion of the ratios A 2 /A 0 in Table 2 is carried out below, for each γ-ray, to explain the spins and parities proposed in Table 2. ...
In this contribution an experimental study of the excited states of 95 Nb, produced by means of the
deep-inelastic reaction 96 Zr+124 Sn at 530 MeV using the G ASP and P RISMA -C LARA arrays, is
presented. Results on the study of the yrast and near-yrast states for 95 Nb are presented. Angular
correlations were performed to determine the spins and parities of some levels. The experimental
results obtained are compared with predictions by shell model calculations.
