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Magic nucleus 132Sn and its one-neutron-hole neighbor 131Sn
P Bhattacharyya1, P J Daly, C T Zhang
1Chemistry Department, Purdue University, West Lafayette, Indiana 47907, USA.
Physical Review Letters
|August 11, 2001
Summary
Researchers studied gamma-ray cascades in tin isotopes 132Sn and 131Sn using a Californium-248 fission source. New nuclear structure details were uncovered for these neutron-rich nuclei.
Area of Science:
- Nuclear Physics
- Nuclear Spectroscopy
- Nuclear Structure
Background:
- Doubly magic nucleus 132Sn and its neighbor 131Sn are crucial for understanding nuclear shell structure.
- Previous studies have provided limited information on the excited states and decay properties of these neutron-rich isotopes.
Purpose of the Study:
- To investigate prompt and delayed gamma-ray cascades in 132Sn and 131Sn.
- To assign unknown gamma rays to specific isotopes and nuclear configurations.
- To interpret the observed level spectra using theoretical models of nuclear interactions.
Main Methods:
- Utilized the Gammasphere array with a Californium-248 (248Cm) fission source.
- Analyzed coincidence data between gamma rays and known transitions in Palladium (Pd) fission partners for isotopic assignments.
- Interpreted yrast level spectra using empirical nucleon-nucleon interactions.
Main Results:
- Identified the (νf7/2 h-1 11/2)9+ aligned state in 132Sn.
- Characterized extensive multiplets in 131Sn, including (νf7/2 h-2 11/2), (νf7/2 d-1 3/2 h-1 11/2), and (νh-1 11/2 × 3−) configurations.
- Elucidated the beta- decay of a previously reported 131In high-spin isomer to levels in 131Sn.
Conclusions:
- The study provides detailed insights into the nuclear structure of neutron-rich tin isotopes.
- The identified configurations and interactions contribute to a better understanding of nuclear shell effects near doubly magic nuclei.
- The findings enhance the nuclear data for 132Sn and 131Sn, aiding future theoretical and experimental nuclear physics research.