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- Grawe, H, et al.
(author)
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High spin spectroscopy of exotic nuclei
- 1997
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In: PROGRESS IN PARTICLE AND NUCLEAR PHYSICS. - : PERGAMON PRESS LTD. - 0146-6410. ; 38, s. 15-27
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Journal article (other academic/artistic)abstract
- The present status and future development of experimental techniques and approach to Sn-100 in in-beam spectroscopy are reviewed. The structure information obtained from recent studies of the T-x = 1 nuclei Pd-94, Cd-98 and Sn-102 is discussed with respec
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- GRAWE, H, et al.
(author)
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THE SHELL-MODEL AT SN-100 - AN EXPERIMENTAL STATUS-REPORT
- 1995
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In: PHYSICA SCRIPTA. - : ROYAL SWEDISH ACAD SCIENCES. ; T56, s. 71-78
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Journal article (other academic/artistic)abstract
- The present status of the shell model structure at N = Z = 50 is given. On the basis of recent and previous experimental work a shell model description of known nuclei is given resulting in predictions for single particle energies for the doubly magic Sn-
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5. |
- Schubart, R, et al.
(author)
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In-beam spectroscopy and shell model structure of the neutron deficient In-103 and CD-100,CD-102
- 1995
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In: Physica Scripta. - : ROYAL SWEDISH ACAD SCIENCES. - 0031-8949 .- 1402-4896. ; T56, s. 311-315
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Journal article (peer-reviewed)abstract
- The ?-decay of the neutron deficient nuclei 103In and 100,102Cd has been studied following the reactions 58Ni + 50Cr and 58Ni + 46,48Ti at 250 MeV and 230 MeV bombarding energy of the 58Ni beam, respectively. Evaporation neutrons and charged particles were measured in coincidence with prompt and delayed ?-rays with the multidetector array OSIRIS. To investigate the decay of the I? = 8+ isomers of 100,102Cd a recoil catcher setup inside OSIRIS was used. Six new ?-ray transitions of 100Cd and four of 102Cd with intensities of 1-10% of the main ?-ray cascades were found. Two new states of 100Cd were established and firm spin-parity assignments were made to all states below the isomer. These new states were identified as the 4+ and the 6+ members of the proton ?g9/2?2 multiplet. The experimental states of 103In and of 100,102Cd are compared to shell model predictions in the ?(p1/2, g9/2) v(d5/2, g7/2, s1/2, d3/2, h11/2) configuration space.
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