Analog of the 3.00-MeV state of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">P</mml:mi></mml:mrow><mml:mprescripts /><mml:mrow /><mml:mrow><mml:mn>32</mml:mn></mml:mrow><mml:mrow /><mml:mrow /></mml:mmultiscripts></mml:mrow></mml:math>in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">S</mml:mi></mml:mrow><mml:mprescript

Hentelä, R.

doi:10.1103/physrevc.23.1900

Cited by 4 publications

(1 citation statement)

References 9 publications

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“…15 and 32.20a of [10] f Using Γ 2 γ /Γ = 0.36 ± 0.11 eV [11] and the branching ratios of this table, knowing from a weak (p,γ) yield [10] that Γp 0 Γγ g From [10]. A new electron scattering experiment [12] leaves this value unchanged h Obtained from the values of ΓpΓγ /Γ and by assuming Γp < Γγ i Experimental branching ratios from [13] k Experimental branching ratios and radiative width from [15] l Experimental branching ratios from [14] m Experimental branching ratios from [16] the case of the 8729 keV, I π = 3 + 1 , T = 1 state. This level is badly known because 56 percent of its γ-decay has escaped observation.…”

Section: Positive-parity T=1 States and Shell Model Predictionsmentioning

confidence: 97%

The structure of 32S II. Shell model interpretation

Brenneisen

Erhardt

Glatz

et al. 1997

Z Phys A - Particles and Fields

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The properties of positive-parity states in 32 S are compared to predictions of shell model calculations within the complete s-d basis space using the universal s-d shell Hamiltonian. The experimental T = O spectrum is reproduced to excitation energies between 10 and 11.7 MeV, depending on the level spins. The T = 1 spectrum is known and reproduced for the first five 5 MeV in excitation in general and for the first 8 MeV in the case of I π = 1 + states. Altogether the excitation energies of 80 positive-parity states are reproduced with a rms deviation of 200 keV. A calculation of radiative widths and branching ratios for γ-decay which uses effective charges and free-nucleon g-factors yields good general agreement with experiment. The need for effective g-factors is felt only in the rare cases of transitions which are governed by the isovector d 3/2 → d 5/2 M1 matrix element. The spectrum of negative parity, T = 1 states is understood in terms of the weakcoupling model while that of the T = 0 states is comprised of octupole-quadrupole phonon multiplets. Positive-parity states from outside the s-d configuration are first observed between 9.5 and 10.5 MeV excitation energy.

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