2021
DOI: 10.1016/j.nds.2021.05.001
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Nuclear Data Sheets for A=123

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Cited by 7 publications
(2 citation statements)
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“…From the comparison of the experimental data with configuration-constrained potential energy surfaces (CC-PES) [10], projected shell model (PSM) [11], and particle number conserving cranked shell model (PNC-CSM) [12] calculations, we assign one neutron-two proton configurations to the high-spin isomers, two of them involving the π 9/2 + [404] orbital. These are the first reported multiquasiparticle high-K isomers involving the π 9/2[404] orbital in A ≈ 130 nuclei, which previously were only observed in one-quasiparticle bands close to the ground state of odd-even and odd-odd nuclei like the neighboring Pr nuclei (see, e.g., [13]), and in odd-even nuclei just above the Z = 50 closed shell [ [14][15][16][17][18][19][20][21]. No high-K isomers are known in the wellstudied Nd nuclei with N 73 [22][23][24][25][26][27], while high-K isomers with spins 8 − and 7 − built on two-neutron configurations are known in N = 74 and N = 72 isotopes, respectively (see, e.g., [28]).…”
Section: Introductionmentioning
confidence: 89%
“…From the comparison of the experimental data with configuration-constrained potential energy surfaces (CC-PES) [10], projected shell model (PSM) [11], and particle number conserving cranked shell model (PNC-CSM) [12] calculations, we assign one neutron-two proton configurations to the high-spin isomers, two of them involving the π 9/2 + [404] orbital. These are the first reported multiquasiparticle high-K isomers involving the π 9/2[404] orbital in A ≈ 130 nuclei, which previously were only observed in one-quasiparticle bands close to the ground state of odd-even and odd-odd nuclei like the neighboring Pr nuclei (see, e.g., [13]), and in odd-even nuclei just above the Z = 50 closed shell [ [14][15][16][17][18][19][20][21]. No high-K isomers are known in the wellstudied Nd nuclei with N 73 [22][23][24][25][26][27], while high-K isomers with spins 8 − and 7 − built on two-neutron configurations are known in N = 74 and N = 72 isotopes, respectively (see, e.g., [28]).…”
Section: Introductionmentioning
confidence: 89%
“…Several factors affect the quality of I-123 SPECT images, such as the sensitivity and resolution of the detectors, partial volume effects, attenuation and scattering [5][6][7]. The latter is a main issue since I-123 emits photons of 159 keV (83.4%) and 529 keV (1.3%) [8]. The relatively high-energy 529 keV photons can penetrate the septa of the collimators, backscattering into the SPECT detector and contributing to the main energy window at 159 ± 10 keV [6].…”
Section: Introductionmentioning
confidence: 99%