0000000000411857

AUTHOR

Tibor Kibedi

showing 5 related works from this author

Microsecond isomers in 187Tl and 188Pb

2000

Lifetime measurements of states in nuclei with A=187 and 188 have been performed, using reactions between 155Gd and 36Ar and following the transport of evaporation residues to the focal plane of a gas-filled recoil separator. In a separate experiment using the 159Tb(32S, 4n) reaction the γ-decay of isomeric levels in 187Tl has been studied using delayed γ-γ coincidence measurements. From observation of their subsequent γ decay, the mean lifetimes were measured to be 1000 ± 55 ns and 1600 ± 100 ns. Although it was not possible to characterize the isomers completely, they are proposed as candidates for one-proton, two-neutron excitations. In the course of this study, the decay of an isomer in…

Nuclear physicsPhysicsNuclear and High Energy PhysicsMicrosecondHadronEvaporationNuclear fusionAtomic physicsCoincidenceRecoil separatorThe European Physical Journal A
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Structure ofIn112nucleus

1988

The \ensuremath{\gamma}-ray spectra of the $^{112}\mathrm{Cd}$(p,n\ensuremath{\gamma}${)}^{112}$In and $^{109}\mathrm{Ag}$(\ensuremath{\alpha},n\ensuremath{\gamma}${)}^{112}$In reactions were measured with Ge(Li) spectrometers for bombarding energies of 4.8 MeV protons and 17.1 MeV \ensuremath{\alpha} particles. The energies and relative intensities of 79 $^{112}\mathrm{In}$ \ensuremath{\gamma}-ray transitions have been determined. The electron spectra were measured with combined magnet plus Si(Li) as well as superconducting magnetic lens plus Si(Li) spectrometers. Internal conversion coefficients of 40 $^{112}\mathrm{In}$ transitions have been determined, and the level scheme of $^{112}\ma…

Nuclear reactionPhysicsBaryonNuclear and High Energy PhysicsBranching fractionAstrophysics::High Energy Astrophysical PhenomenaQuadrupoleHadronElementary particleAtomic physicsNuclear ExperimentNucleonSpectral linePhysical Review C
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Towards an Experimental Determination of the Transition Strength Between the Ground States of $^{20}$F and $^{20}$Ne

2017

Electron capture on $^{20}$Ne is thought to play a crucial role in the final evolution of electron-degenerate ONe stellar cores. Recent calculations suggest that the capture process is dominated by the second-forbidden transition between the ground states of $^{20}$Ne and $^{20}$F, making an experimental determination of this transition strength highly desirable. To accomplish this task we are refurbishing an intermediate-image magnetic spectrometer capable of focusing 7 MeV electrons, and designing a scintillator detector surrounded by an active cosmic-ray veto shield, which will serve as an energy-dispersive device at the focal plane.

Physicsstellar evolutionPhysics - Instrumentation and Detectorsta114Condensed matter physicsPhysics::Instrumentation and Detectorsweak-interaction ratesnuclear experimentFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)Transition strengthAstrophysics - Solar and Stellar Astrophysicsbeta-decaySolar and Stellar Astrophysics (astro-ph.SR)
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Assignment of levels in 208Fr and 10- isomers in the odd-odd isotones 206At and 208Fr

2009

Excited states in 208 Fr have been identified using the 197 Au( 16 O, 5n) 208 Fr reaction and a variety of time-correlated γ-ray and conversion electron spectroscopic techniques. Transitions above and below a τ = 623(16) ns 10 − isomer are placed in the level scheme. This isomer is analogous to that observed in the odd-odd isotone 206 At for which additional spectroscopic information is also obtained, including a precise lifetime of τ = 1173(30) ns. The γ-rays assigned to 208 Fr are the same as the main transitions erroneously assigned to 209 Fr in previous work.

PhysicsNuclear and High Energy PhysicsExcited stateIsotoneHadronNuclear fusionElectronAtomic physicsThe European Physical Journal A
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Conversion-electron study of 0+excitations in208Pb

2005

The 208Pb(p,p'e−) reaction has been studied at a proton energy of 17.3 MeV. Singles data show E0 transitions from the 0+2 and 0+3 states at 4868 and 5241 keV, respectively, to the ground state. Proton–electron gated spectra indicate that few electrons from the 0+2 state are in coincidence with backscattered protons, while those from the 0+3 state are somewhat more abundant. From the singles spectra, an upper limit for the E3(0+3 → 3−1)/E0(0+3 → 0+1) branching ratio of less than four has been measured. This observation is in agreement with previous predictions for a two-phonon octupole excitation.

PhysicsNuclear and High Energy PhysicsProtonBranching fractionPhononElectronAtomic physicsNuclear ExperimentGround stateExcitationCoincidenceSpectral lineJournal of Physics G: Nuclear and Particle Physics
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