The structure of 100Sn and neighbouring nuclei

Saved in:
Bibliographic Details
Title: The structure of 100Sn and neighbouring nuclei
Authors: Faestermann, T.1 thomas.faestermann@tum.de, Górska, M.2, Grawe, H.2
Source: Progress in Particle & Nuclear Physics. Mar2013, Vol. 69, p85-130. 46p.
Subjects: Strontium isotopes, Nuclear structure, Physics experiments, Radioactive nuclear beams, Exotic nuclei, Neutron-proton interactions
Abstract: Abstract: The nuclear structure in the 100Sn region is reviewed. State-of-the-art experimental techniques involving stable and radioactive beam facilities have enabled access to exotic nuclei in its next neighbourhood. The analysis of experimental data has established the shell structure and its evolution towards , seniority conservation and proton–neutron interaction in the g9/2 orbit, the super-allowed Gamow–Teller decay of 100Sn, masses and half lives along the -path, and super-allowed decay beyond 100Sn. The status of theoretical approaches in shell model and mean-field investigations is described and their predictive power assessed. Structure features of 100Sn and its doubly-magic neighbours 56Ni at , 132Sn and 78Ni at are compared. An outlook is given on future developments of experimental and theoretical methods. [Copyright &y& Elsevier]
Copyright of Progress in Particle & Nuclear Physics is the property of Pergamon Press - An Imprint of Elsevier Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
Description
Abstract:Abstract: The nuclear structure in the 100Sn region is reviewed. State-of-the-art experimental techniques involving stable and radioactive beam facilities have enabled access to exotic nuclei in its next neighbourhood. The analysis of experimental data has established the shell structure and its evolution towards , seniority conservation and proton–neutron interaction in the g9/2 orbit, the super-allowed Gamow–Teller decay of 100Sn, masses and half lives along the -path, and super-allowed decay beyond 100Sn. The status of theoretical approaches in shell model and mean-field investigations is described and their predictive power assessed. Structure features of 100Sn and its doubly-magic neighbours 56Ni at , 132Sn and 78Ni at are compared. An outlook is given on future developments of experimental and theoretical methods. [Copyright &y& Elsevier]
ISSN:01466410
DOI:10.1016/j.ppnp.2012.10.002