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(c) 2011 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
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[en] The 160Gd(9Be,α3n)162Dy reaction has been used to study high-spin states in 162Dy. Pulsed beam conditions were utilized for enhanced isomer sensitivity. An isomer at 2188.1(3) keV with a half-life of 8.3(3) μs has been discovered and assigned Kπ= 8+ with a two-quasineutron configuration. Among 11 γ-ray decay branches, an E2, ΔK=8 transition to the ground-state band was observed with a reduced hindrance of fν=35, agreeing well with systematics correlating fν with the product of the valence neutron and proton numbers (NpNn) over an extended N,Z range. Small deviations from NpNn dependence are analyzed for a range of two-quasiparticle isomer decays and interpreted as arising from a weak dependence on the isomer excitation energy relative to the yrast line.
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(c) 2011 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
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BARYONS, DECAY, DYSPROSIUM ISOTOPES, ELECTROMAGNETIC RADIATION, ELEMENTARY PARTICLES, EMISSION, ENERGY LEVELS, ENERGY RANGE, ENERGY-LEVEL TRANSITIONS, EVEN-EVEN NUCLEI, FERMIONS, HADRONS, HEAVY ION REACTIONS, INTERMEDIATE MASS NUCLEI, IONIZING RADIATIONS, ISOTOPES, NUCLEAR DECAY, NUCLEAR REACTIONS, NUCLEI, NUCLEONS, RADIATIONS, RARE EARTH NUCLEI, STABLE ISOTOPES, TARGETS
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[en] P-type InAs excited by ultrashort optical pulses has been shown to be a strong emitter of terahertz radiation. In a direct comparison between a p-InAs emitter and conventional thermal radiation sources, we demonstrate that under typical excitation conditions p-InAs produces more radiation below 1.2 THz than a globar. By treating the globar as a blackbody emitter we calibrate a silicon bolometer which is used to determine the power of the p-InAs emitter. The emitted terahertz power was found to be 98±10 nW in this experiment
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(c) 2009 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
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