gamma-ray spectroscopy of neutron-rich {sup 40}S
Journal Article
·
· Physical Review. C, Nuclear Physics
- School of Engineering, University of the West of Scotland, Paisley, PA1 2BE, United Kingdom and the Scottish Universities Physics Alliance (SUPA) (United Kingdom)
- IPHC, CNRS-IN2P3 and Universite de Strasbourg, F-67037 Strasbourg Cedex 2 (France)
- IPN, CNRS-IN2P3 and Universite Paris-Sud, F-91406 Orsay Cedex (France)
- INFN, Laboratori Nazionali di Legnaro, I-35020 Legnaro, Padova (Italy)
Yrast states up to (6{sup +}) in the neutron-rich {sup 40}S nucleus have been studied using binary grazing reactions produced by the interaction of a 215 MeV beam of {sup 36}S ions with a thin {sup 208}Pb target. The novel experimental setup that combines the large acceptance magnetic spectrometer, PRISMA, and the high-efficiency gamma-ray detection array, CLARA, was used. A new gamma-ray transition at an energy of 1572 keV was observed and tentatively assigned to the (6{sup +})->(4{sup +}) transition. A comparison of experimental observations and the results of large-scale 0(Planck constant/2pi)omega sd-pf shell-model calculations indicates that one- and two-proton excitations from the 2s{sub 1/2} to the 1d{sub 3/2} orbitals play an important role in reproducing the {sup 40}S yrast level structure and the published B(E2;0{sub g.s.}{sup +}->2{sub 1}{sup +}) value. The structure of the yrast states of the even-A isotopes of sulfur is interpreted in terms of the configurations of valence protons and neutrons within the context of large-scale 0(Planck constant/2pi)omega sd-pf shell-model calculations.
- OSTI ID:
- 21389013
- Journal Information:
- Physical Review. C, Nuclear Physics, Journal Name: Physical Review. C, Nuclear Physics Journal Issue: 5 Vol. 81; ISSN 0556-2813; ISSN PRVCAN
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
73 NUCLEAR PHYSICS AND RADIATION PHYSICS
BARYONS
BEAMS
BETA DECAY RADIOISOTOPES
BETA-MINUS DECAY RADIOISOTOPES
CHARGED PARTICLES
COMPARATIVE EVALUATIONS
CONFIGURATION
DETECTION
EFFICIENCY
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
ENERGY LEVELS
ENERGY RANGE
ENERGY-LEVEL TRANSITIONS
EVALUATION
EVEN-EVEN NUCLEI
EXCITATION
FERMIONS
GAMMA DETECTION
GAMMA RADIATION
GAMMA SPECTROSCOPY
HADRONS
INTERACTIONS
IONIZING RADIATIONS
IONS
ISOTOPES
LEAD 208 TARGET
LIGHT NUCLEI
MAGNETIC SPECTROMETERS
MATHEMATICAL MODELS
MEASURING INSTRUMENTS
MEV RANGE
MEV RANGE 100-1000
NEUTRON-RICH ISOTOPES
NEUTRONS
NUCLEAR MODELS
NUCLEI
NUCLEONS
PROTONS
RADIATION DETECTION
RADIATIONS
RADIOISOTOPES
SECONDS LIVING RADIOISOTOPES
SHELL MODELS
SPECTROMETERS
SPECTROSCOPY
STABLE ISOTOPES
SULFUR 36
SULFUR 40
SULFUR ISOTOPES
TARGETS
YRAST STATES
BARYONS
BEAMS
BETA DECAY RADIOISOTOPES
BETA-MINUS DECAY RADIOISOTOPES
CHARGED PARTICLES
COMPARATIVE EVALUATIONS
CONFIGURATION
DETECTION
EFFICIENCY
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
ENERGY LEVELS
ENERGY RANGE
ENERGY-LEVEL TRANSITIONS
EVALUATION
EVEN-EVEN NUCLEI
EXCITATION
FERMIONS
GAMMA DETECTION
GAMMA RADIATION
GAMMA SPECTROSCOPY
HADRONS
INTERACTIONS
IONIZING RADIATIONS
IONS
ISOTOPES
LEAD 208 TARGET
LIGHT NUCLEI
MAGNETIC SPECTROMETERS
MATHEMATICAL MODELS
MEASURING INSTRUMENTS
MEV RANGE
MEV RANGE 100-1000
NEUTRON-RICH ISOTOPES
NEUTRONS
NUCLEAR MODELS
NUCLEI
NUCLEONS
PROTONS
RADIATION DETECTION
RADIATIONS
RADIOISOTOPES
SECONDS LIVING RADIOISOTOPES
SHELL MODELS
SPECTROMETERS
SPECTROSCOPY
STABLE ISOTOPES
SULFUR 36
SULFUR 40
SULFUR ISOTOPES
TARGETS
YRAST STATES