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• W2011861974 abstract "The structure of ${}^{58}$Fe was investigated at Gammasphere using ${}^{48}$Ca(${}^{13,14}$C,$x$$n$) fusion-evaporation reactions at a beam energy of 130 MeV. The level scheme has been revised and extended to $Jensuremath{sim}17ensuremath{hbar}$ and an excitation energy of 16.6 MeV. Regular band structures consisting of low-energy $ensuremath{Delta}J=1ensuremath{hbar}$ transitions have been observed at moderate spin ($Jensuremath{sim}8ensuremath{hbar}$--15$ensuremath{hbar}$) and are candidates for magnetic rotational bands. Self-consistent tilted-axis-cranking calculations within a relativistic mean-field theory were applied to investigate these bands and were found to reproduce the experimental results well. In other parts of the level scheme, quasirotational bands composed of stretched-$E2$ transitions have been extended to high spin, and other new bands have been identified. Positive-parity experimental states were compared to predictions of the spherical shell model using the GXPF1A, KB3G, and FPD6 effective interactions in the $fp$ model space. The projected shell model, with a deformed quasiparticle basis including the neutron $ensuremath{nu}{g}_{9/2}$ orbital, was applied to interpret regular $ensuremath{Delta}J=2ensuremath{hbar}$ band structures that extend beyond the maximum spin available for $ensuremath{pi}$[(${f}_{7/2}$)${}^{ensuremath{-}2}$] $ensuremath{bigotimes}$ $ensuremath{nu}$[(${p}_{3/2}{f}_{5/2}{p}_{1/2}$)${}^{4}$] configurations and exhibit features characteristic of rotational alignment. It is clear that the $ensuremath{nu}{g}_{9/2}$ intruder orbital plays a crucial role in describing the quasirotational structures in this nucleus, even starting as low as $Jensuremath{sim}5ensuremath{hbar}$." @default.
• W2011861974 created "2016-06-24" @default.
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• W2011861974 date "2012-04-16" @default.
• W2011861974 modified "2023-10-03" @default.
• W2011861974 title "Magnetic rotation and quasicollective structures in<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:msup><mml:mrow /><mml:mn>58</mml:mn></mml:msup></mml:math>Fe: Influence of the<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:mi>ν</mml:mi><mml:msub><mml:mi>g</mml:mi><mml:mrow><mml:mn>9</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math>orbital" @default.
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• W2011861974 doi "https://doi.org/10.1103/physrevc.85.044316" @default.
• W2011861974 hasPublicationYear "2012" @default.
• W2011861974 type Work @default.

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