6533b7d6fe1ef96bd1266611
RESEARCH PRODUCT
Radioactivity of neutron-rich oxygen fluorine and neon isotopes
BurjanJouni SuhonenN. A. OrrA.t. ReedS. M. VincentR. AnneW. N. CatfordF. M. MarquésM. G. Saint-laurentC. BorceaJ. C. AngéliqueP. H. ReganO. SorlinS. M. LukyanovJ. NovákTeemu SiiskonenRobert PageS. GrévyD. Guillemaud-muellerF. PougheonR. G. AllattYu. E. PenionzhkevichE. SokolC. DonzaudZ. DlouhyW. TrinderA.c. MuellerM. LewitowiczOleg B. TarasovG. MartínezP. J. Nolansubject
PhysicsNuclear and High Energy PhysicsIsotopes of germanium010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaGamma ray[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyNuclear physicsInternal conversionIsotopes of neon13. Climate action0103 physical sciencesBeta particleIsotopes of zirconiumNuclear Experiment010306 general physicsRadioactive decayEnergy (signal processing)description
The $\ensuremath{\gamma}$ radiation and neutrons emitted following the $\ensuremath{\beta}$ decays of ${}^{24}\mathrm{O},$ ${}^{25--27}\mathrm{F},$ and ${}^{28\ensuremath{-}30}\mathrm{Ne}$ have been measured. The nuclides were produced in the quasifragmentation of a 2.8 GeV ${}^{36}\mathrm{S}$ beam, separated in-flight and identified through time-of-flight and energy-loss measurements. The ions were stopped in a silicon detector telescope, which was used to detect the $\ensuremath{\beta}$ particles emitted in their subsequent radioactive decay. The coincident $\ensuremath{\gamma}$ rays were measured using four large volume germanium detectors mounted close to the implantation point and the neutrons were detected using 42 ${}^{3}\mathrm{He}$ proportional counters. The measured $\ensuremath{\gamma}$-ray energy spectra are compared with shell model calculations and, where available, the level energies deduced from multinucleon transfer reactions.
year | journal | country | edition | language |
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1999-07-20 |