0000000000362471

AUTHOR

D. Southall

showing 3 related works from this author

Isospin symmetry in B(E2) values: Coulomb excitation study of Mg21

2019

The Tz=−32 nucleus 21Mg has been studied by Coulomb excitation on 196Pt and 110Pd targets. A 205.6(1)-keV γ-ray transition resulting from the Coulomb excitation of the 52+ ground state to the first excited 12+ state in 21Mg was observed for the first time. Coulomb excitation cross-section measurements with both targets and a measurement of the half-life of the 12+ state yield an adopted value of B(E2;52+→12+)=13.3(4) W.u. A new excited state at 1672(1) keV with tentative 92+ assignment was also identified in 21Mg. This work demonstrates a large difference in the B(E2;52+→12+) value between T=32, A=21 mirror nuclei. The difference is investigated in the shell-model framework employing both i…

Physics010308 nuclear & particles physicsNuclear structureAb initioCoulomb excitation01 natural sciencesSymmetry (physics)Excited stateIsospin0103 physical sciencesMirror nucleiAtomic physics010306 general physicsGround statePhysical Review C
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IceCube-Gen2: The Window to the Extreme Universe

2020

The observation of electromagnetic radiation from radio to $\gamma$-ray wavelengths has provided a wealth of information about the universe. However, at PeV (10$^{15}$ eV) energies and above, most of the universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explore the most extreme environments of the universe where black holes, neutron stars, and stellar explosions transform gravitational energy into non-thermal cosmic rays. The discovery of cosmic neutrinos with IceCube has opened this new window on the universe. In this white paper, we present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the proce…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HENuclear and High Energy PhysicsActive galactic nucleus010308 nuclear & particles physicsHigh-energy astronomyGravitational wavemedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFOS: Physical sciencesCosmic ray01 natural sciencesUniverseNeutron star0103 physical sciencesNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsmedia_common
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Isospin symmetry in $B(E2)$ values: Coulomb excitation study of ${}^{21}$Mg

2018

The $T_z$~=~$-\frac{3}{2}$ nucleus ${}^{21}$Mg has been studied by Coulomb excitation on ${}^{196}$Pt and ${}^{110}$Pd targets. A 205.6(1)-keV $\gamma$-ray transition resulting from the Coulomb excitation of the $\frac{5}{2}^+$ ground state to the first excited $\frac{1}{2}^+$ state in ${}^{21}$Mg was observed for the first time. Coulomb excitation cross-section measurements with both targets and a measurement of the half-life of the $\frac{1}{2}^+$ state yield an adopted value of $B(E2;\frac{5}{2}^+\rightarrow\frac{1}{2}^+)$~=~13.3(4)~W.u. A new excited state at 1672(1)~keV with tentative $\frac{9}{2}^+$ assignment was also identified in ${}^{21}$Mg. This work demonstrates large difference…

electromagnetic transitionsenergy levels and level densitiesshell modelFOS: Physical sciencescollective levelscoulomb energies and analogue statesNuclear Experiment (nucl-ex)isomer decaysydinfysiikkaNuclear Experiment
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