Nuclear data sheets update for A = 108

Blachot, J.

doi:10.1016/0090-3752(91)80022-x

Cited by 23 publications

(3 citation statements)

References 366 publications

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“…1 and 2 we show the behavior of the states arising from the . We compare our results with the experimental energies [12][13][14][15][16][17][18][19][20][21][22][23][24][25] of those states which can be uniquely associated with the maximally aligned states formed from the two above configurations, namely the 9\ and 10> states. Concerning the latter, the comparison starts from A"112.…”

Section: Iii1 Even-mass Nucleimentioning

confidence: 93%

Pairing effects in Sn isotopes

Andreozzi

Coraggio

Covello

et al. 1996

Z. Phys. A — Hadrons and Nuclei

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An extensive study of pairing effects in the Sn isotopes is carried out. The pairing Hamiltonian is treated by the chain-calculation method which provides practically exact solutions while involving less computational work than a complete-basis diagonalization. The coupling strength is fixed by reproducing the energy of the 9\ state in Sn, while the single-particle energies have been determined by an analysis of the experimental low-energy spectra of the odd-A isotopes. A detailed comparison of the calculated results with experimental data evidences the importance of neutron pairing correlations in the 50-82 shell. The results of this paper complement those of our previous study of the N"82 isotones. It turns out that the role of pairing correlations is similar to a large extent in both cases.

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Section: Iii1 Even-mass Nucleimentioning

confidence: 93%

Pairing effects in Sn isotopes

Andreozzi

Coraggio

Covello

et al. 1996

Z. Phys. A — Hadrons and Nuclei

View full text Add to dashboard Cite

show abstract

“…The energies of the first-excited 2 + 1 states (filled symbols) for Sr (Z = 38), Zr (Z = 40), Mo (Z = 42), and Ru (Z = 44) isotopes with N = 52-64. Data are taken from the Nuclear Data Sheets [9][10][11][12][13][14][15][16][17][18]. Also the B(E 2; 2 + 1 → 0 + 1 ) for the Mo isotopes are shown (open symbols) where the values are taken from Refs.…”

Section: Methodsmentioning

confidence: 99%

“…The strongest γ rays belong to 100 Mo and 102 Mo. An exclusion of the Coulomb excitation channel ( 100 Mo) with the particle gate was not possible due to the energy and angular struggling of the recoiling 18 O and 16 O particles as well as the angular coverage of the solar cells.…”

Section: Methodsmentioning

confidence: 99%