Shell model based Coulomb excitation gamma-ray intensity calculations in Sn-107

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Shell model based Coulomb excitation gamma-ray intensity calculations in Sn-107. / DiJulio, Douglas; Cederkäll, Joakim; Ekström, Andreas; Fahlander, Claes; Hjorth-Jensen, M.

In: Physica Scripta, Vol. T150, 014012, 2012.

Research output: Contribution to journalArticle

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TY - JOUR

T1 - Shell model based Coulomb excitation gamma-ray intensity calculations in Sn-107

AU - DiJulio, Douglas

AU - Cederkäll, Joakim

AU - Ekström, Andreas

AU - Fahlander, Claes

AU - Hjorth-Jensen, M.

PY - 2012

Y1 - 2012

N2 - In this work, we present recent shell model calculations, based on a realistic nucleon-nucleon interaction, for the light Sn-107,Sn-109 nuclei. By combining the calculations with the semi-classical Coulomb excitation code GOSIA, a set of gamma-ray intensities has been generated. The calculated intensities are compared with the data from recent Coulomb excitation studies in inverse kinematics at the REX-ISOLDE facility with the nucleus Sn-107. The results are discussed in the context of the ordering of the single-particle orbits relative to Sn-100.

AB - In this work, we present recent shell model calculations, based on a realistic nucleon-nucleon interaction, for the light Sn-107,Sn-109 nuclei. By combining the calculations with the semi-classical Coulomb excitation code GOSIA, a set of gamma-ray intensities has been generated. The calculated intensities are compared with the data from recent Coulomb excitation studies in inverse kinematics at the REX-ISOLDE facility with the nucleus Sn-107. The results are discussed in the context of the ordering of the single-particle orbits relative to Sn-100.

U2 - 10.1088/0031-8949/2012/T150/014012

DO - 10.1088/0031-8949/2012/T150/014012

M3 - Article

VL - T150

JO - Physica Scripta

JF - Physica Scripta

SN - 0031-8949

M1 - 014012

ER -