Comment on {open_quotes}Structure of neutron-rich nuclei around {sup 132}Sn{close_quotes}

Journal Article · Fri Jan 01 04:00:00 EST 1999 · Physical Review, C

DOI:https://doi.org/10.1103/PhysRevC.59.546· OSTI ID:289072

Blomqvist, J ^[1]; Zhang, C T; Daly, P J ^[2]

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1. Department of Physics Frescati, Royal Institute of Technology, S-10405 Stockholm (Sweden)
2. Chemistry Department, Purdue University, West Lafayette, Indiana 47907 (United States)

Recent shell model calculations using a realistic interaction by Andreozzi {ital et al.} [Phys. Rev. C {bold 56}, R16 (1997)] have given excellent agreement with the experimental level spectra of {sup 134}Te and {sup 135}I. In addition, these authors call into question our contention that there is a serious inconsistency in the measured masses of {ital N}=82 isotones near {sup 132}Sn. In this Comment, we outline the shell model decomposition method and defend our conclusion that the accepted ground state masses of {sup 134}Te and/or {sup 133}Sb must be inaccurate by much more than their assigned errors. thinsp {copyright} {ital 1998} {ital The American Physical Society}

• OSTI ID: 289072
• Journal Information: Physical Review, C, Journal Name: Physical Review, C Journal Issue: 1 Vol. 59; ISSN 0556-2813; ISSN PRVCAN
• Country of Publication: United States
• Language: English

Related Subjects

66 PHYSICS
ANTIMONY 132
BINDING ENERGY
ENERGY LEVELS
IODINE 135
MASS
SHELL MODELS
TELLURIUM 134