0000000000053291

AUTHOR

W.q. Zhang

showing 2 related works from this author

Evidence of oblate-prolate shape coexistence in the strongly-deformed nucleus 119Cs

2021

International audience; Prolate-oblate shape coexistence close to the ground state in the strongly-deformed proton-rich A≈120 nuclei is reported for the first time. One of the four reported bands in 119Cs, built on a 11/2− state at 670 keV, consists of nearly degenerate signature partners, and has properties which unequivocally indicate the strongly-coupled πh11/2[505]11/2− configuration associated with oblate shape. Together with the decoupled πh11/2[541]3/2− band built on the 11/2− prolate state at 110 keV, for which a half-life of T1/2=55(5)μs has been measured, the new bands bring evidence of shape coexistence at low spin in the proton-rich strongly deformed A≈120 nuclei, a phenomenon p…

58Ni(64Zn3p)119CsNuclear reactionNuclear and High Energy PhysicsQC1-999Nuclear TheoryModel calculation-coincidences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesMolecular physicsMeasured γγγ-coincidencescesium0103 physical sciencesmedicineNuclear reaction:58Ni(64Zn3p)119CsZnCovariant transformationCs010306 general physicsSpin (physics)Ni(PhysicsLinear polarization010308 nuclear & particles physicsLinear polarizationPhysicsDegenerate energy levels3p)Oblate-prolate coexistenceNuclear reactionmedicine.anatomical_structureNuclear reaction:Angular correlationsDensity functional theoryydinfysiikkaGround stateMeasuredNucleusPhysics Letters B
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Spectroscopic factor and proton formation probability for the d3/2 proton emitter 151Lu

2017

The quenching of the experimental spectroscopic factor for proton emission from the short-lived $d_{3/2}$ isomeric state in $^{151m}$Lu was a long-standing problem. In the present work, proton emission from this isomer has been reinvestigated in an experiment at the Accelerator Laboratory of the University of Jyv\"{a}skyl\"{a}. The proton-decay energy and half-life of this isomer were measured to be 1295(5) keV and 15.4(8) $\mu$s, respectively, in agreement with another recent study. These new experimental data can resolve the discrepancy in the spectroscopic factor calculated using the spherical WKB approximation. Using the R-matrix approach it is found that the proton formation probabilit…

Nuclear and High Energy PhysicsWork (thermodynamics)Nuclear TheoryProton3106Proton decayFOS: Physical sciencesProton energy01 natural sciencesproton emitterWKB approximationNuclear Theory (nucl-th)Nuclear physicsA=1510103 physical sciencesrecoil-decay taggingddc:530WKB approximationNuclear Experiment (nucl-ex)spectroscopic factorProton emissionNuclear Experiment010306 general physicsNuclear ExperimentCommon emitterPhysicsQuenching (fluorescence)ta114010308 nuclear & particles physicsSpectroscopic factorProton emitterproton formation probabilitylcsh:QC1-999Proton formation probability3. Good healthRecoil-decay taggingAtomic physicslcsh:PhysicsPhysics Letters B
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