0000000001252243

AUTHOR

O. Poleshchuk

showing 4 related works from this author

First Exploration of Neutron Shell Structure Below Lead and Beyond $\boldsymbol{N=126}$

2020

The nuclei below lead but with more than 126 neutrons are crucial to an understanding of the astrophysical $r$-process in producing nuclei heavier than $A\sim190$. Despite their importance, the structure and properties of these nuclei remain experimentally untested as they are difficult to produce in nuclear reactions with stable beams. In a first exploration of the shell structure of this region, neutron excitations in $^{207}$Hg have been probed using the neutron-adding ($d$,$p$) reaction in inverse kinematics. The radioactive beam of $^{206}$Hg was delivered to the new ISOLDE Solenoidal Spectrometer at an energy above the Coulomb barrier. The spectroscopy of $^{207}$Hg marks a first step…

Nuclear Theorynucl-thNuclear TheoryFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-exNuclear Theory (nucl-th)Nuclear Physics - TheoryPhysics::Accelerator PhysicsNuclear Physics - ExperimentNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentNuclear Physics
researchProduct

First Exploration of Neutron Shell Structure below Lead and beyond N=126

2020

The nuclei below lead but with more than 126 neutrons are crucial to an understanding of the astrophysical r process in producing nuclei heavier than A∼190. Despite their importance, the structure and properties of these nuclei remain experimentally untested as they are difficult to produce in nuclear reactions with stable beams. In a first exploration of the shell structure of this region, neutron excitations in ^{207}Hg have been probed using the neutron-adding (d,p) reaction in inverse kinematics. The radioactive beam of ^{206}Hg was delivered to the new ISOLDE Solenoidal Spectrometer at an energy above the Coulomb barrier. The spectroscopy of ^{207}Hg marks a first step in improving our…

PhysicsNuclear reactionSpectrometerSolenoidal vector fieldNuclear TheoryGeneral Physics and AstronomyCoulomb barrier01 natural sciencesNuclear physicsLead (geology)0103 physical sciencesr-processPhysics::Accelerator PhysicsNeutron010306 general physicsSpectroscopyNuclear Experimentydinfysiikka
researchProduct

QEC value of the superallowed β emitter Sc42

2017

Precise measurements of superallowed ${0}^{+}\ensuremath{\rightarrow}{0}^{+}$ $\ensuremath{\beta}$ decay presently provide the most precise value for the weak mixing amplitude ${V}_{u\phantom{\rule{0}{0ex}}d}$. As the largest element of the CKM matrix, ${V}_{u\phantom{\rule{0}{0ex}}d}$ is a critical piece of the Standard Model of the electroweak interaction. The new, precise Penning-trap mass measurement of the decay energy for the superallowed transition in ${}^{42}$Sc opens the door for a much more precise $f\phantom{\rule{0}{0ex}}t$ value determination if its half-life can be measured more precisely as well.

PhysicsParticle physics010308 nuclear & particles physicsCabibbo–Kobayashi–Maskawa matrixElectroweak interactionValue (computer science)01 natural sciencesMass measurementStandard ModelAmplitudeDecay energy0103 physical sciences010306 general physicsCommon emitterPhysical Review C
researchProduct

QEC value of the superallowed β emitter 42Sc

2017

The QEC value of the superallowed β+ emitter Sc42 has been measured with the JYFLTRAP Penning-trap mass spectrometer at the University of Jyväskylä to be 6426.350(53) keV. This result is at least a factor of four more precise than all previous measurements, which were also inconsistent with one another. As a byproduct we determine the excitation energy of the 7+ isomeric state in Sc42 to be 616.762(46) keV, which deviates by 8σ from the previous measurement. peerReviewed

Ion Traps (Instrumentation)astrofysiikkasuperallowed emittersAntiprotonsAtomic Weightsydinfysiikkaatomipainot
researchProduct