0000000000749431

AUTHOR

E. C. Pollacco

showing 3 related works from this author

Structure of theN=27isotones derived from theAr44(d,p)Ar45reaction

2008

The $^{44}\mathrm{Ar}$($d,p$)$^{45}\mathrm{Ar}$ neutron transfer reaction was performed at $10A$ MeV. Measured excitation energies, deduced angular momenta, and spectroscopic factors of the states populated in $^{45}\mathrm{Ar}$ are reported. A satisfactory description of these properties is achieved in the shell model framework using a new $\mathit{sdpf}$ interaction. The model analysis is extended to more exotic even-$Z$ nuclei down to ${}_{14}^{41}{\mathrm{Si}}_{27}$ to study how collectivity impacts the low-lying structure of $N=27$ neutron-rich nuclei.

PhysicsNuclear reactionNuclear and High Energy PhysicsAngular momentum010308 nuclear & particles physicsNuclear TheoryStructure (category theory)01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsNeutronIsotopes of siliconAtomic physicsNuclear Experiment010306 general physicsRadioactive decayExcitationDimensionless quantityPhysical Review C
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Decay spectroscopy for nuclear astrophysics: β- and β-delayed proton decay

2012

In several radiative proton capture reactions important in novae and XRBs, the resonant parts play the capital role. We use decay spectroscopy techniques to find these resonances and study their properties. We have developed techniques to measure beta- and beta-delayed proton decay of sd-shell, proton-rich nuclei produced and separated with the MARS recoil spectrometer of Texas A&M University. The short-lived radioactive species are produced in-flight, separated, then slowed down (from about 40 MeV/u) and implanted in the middle of very thin Si detectors. This allows us to measure protons with energies as low as 200 keV from nuclei with lifetimes of 100 ms or less. At the same time we measu…

Nuclear reactionPhysicsHistoryProtonProton decayAstrophysics::High Energy Astrophysical PhenomenaParticle detectorComputer Science ApplicationsEducationNuclear physicsNuclear astrophysicsProton emissionAtomic physicsNuclear ExperimentNucleonRadioactive decayJournal of Physics: Conference Series
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$^{78}$Ni revealed as a doubly magic stronghold against nuclear deformation

2019

Nuclear magic numbers, which emerge from the strong nuclear force based on quantum chromodynamics, correspond to fully occupied energy shells of protons, or neutrons inside atomic nuclei. Doubly magic nuclei, with magic numbers for both protons and neutrons, are spherical and extremely rare across the nuclear landscape. While the sequence of magic numbers is well established for stable nuclei, evidence reveals modifications for nuclei with a large proton-to-neutron asymmetry. Here, we provide the first spectroscopic study of the doubly magic nucleus $^{78}$Ni, fourteen neutrons beyond the last stable nickel isotope. We provide direct evidence for its doubly magic nature, which is also predi…

1000ProtonNuclear Theorymedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaStrong interactionNuclear TheoryFOS: Physical sciences01 natural sciencesAsymmetryNuclear Theory (nucl-th)Magic number (programming)0103 physical sciencesEffective field theoryPhysics::Atomic and Molecular ClustersNeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear Experimentmedia_commonPhysics[PHYS]Physics [physics]Multidisciplinary010308 nuclear & particles physicsMagic (programming)Atomic nucleusAtomic physics
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