Search results for "Spectral"

showing 10 items of 3116 documents

Fine structure in fragment mass-energy distribution from 238U+40Ar (275 MeV)

2003

Existence of a new feature in fragment mass-energy distribution is reported. Careful analysis of the data obtained in the reaction 238U + 40Ar (275 MeV) shows that small but statistically significant ripples visible already in the gross mass spectrum come from extended and regular 2D patterns in the TKE vs. mass matrix. Intensity distributions of these patterns coincide with the location of heavy clusters such as 78Ni, 108Mo, or 132Sn. Presumably, the observed patterns show the dominant trajectories in the elongation vs. mass-asymmetry space of the decaying system. This information, unknown in the past, can shed a new light even on the previously well-studied reactions.

PhysicsNuclear reactionDistribution (mathematics)Fragment (logic)Mass spectrumSpace (mathematics)Mass matrixMolecular physicsIntensity (heat transfer)Spectral line
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Structure ofSb118nucleus

1992

{gamma}, {gamma}{gamma}-coincidence, internal conversion electron, and {gamma}-ray angular distribution spectra of the {sup 118}Sn({ital p},{ital n}{gamma}){sup 118}Sb reaction were measured at different bombarding proton energies between 5.5 and 7.5 MeV. {gamma}, {gamma}{gamma}-coincidence, and internal conversion electron spectra of the {sup 115}In ({alpha},{ital n}{gamma}){sup 118}Sb reaction were also measured at {ital E}{sub {alpha}}=14.5 MeV. Ge(HP), Ge(Li), Ge(LEPS) {gamma}-ray detectors, as well as a superconducting magnetic lens electron spectrometer (with Si(Li) detectors), were used in the experiments. About 210 (including {similar to}130 new) {gamma} rays have been assigned to {…

PhysicsNuclear reactionNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaHadronQuadrupoleNeutronAtomic physicsInelastic scatteringNuclear ExperimentNucleonRadioactive decaySpectral linePhysical Review C
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Lifetimes of odd-spin yrast states inHg182

2010

Lifetimes of excited states in $^{182}\mathrm{Hg}$ were extracted from recoil-gated $\ensuremath{\gamma}$-ray spectra and recoil-gated $\ensuremath{\gamma}\ensuremath{\gamma}$-coincidence matrices using the recoil distance Doppler-shift method. States were populated using the $^{96}\mathrm{Mo}$($^{88}\mathrm{Sr}$,$2n$)$^{182}\mathrm{Hg}$ fusion-evaporation reaction. Measured lifetimes allowed transition probabilities, transition quadrupole moments, quadrupole deformation parameters, and transition dipole moments to be deduced for the band formed by the odd-spin yrast states. The experimental results confirm the low degree of octupole collectivity in this mass region.

PhysicsNuclear reactionNuclear and High Energy PhysicsDegree (graph theory)010308 nuclear & particles physicsYrast01 natural sciencesSpectral lineDipoleExcited state0103 physical sciencesQuadrupolePhysics::Atomic PhysicsAtomic physics010306 general physicsSpin (physics)Physical Review C
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α-Decay branching ratios measured by γ-ray tagging

2008

Abstract The nuclides 168–170Pt were produced by bombarding isotopically enriched 92,94Mo targets with 336, 348 MeV 78Kr ions. Prompt γ rays were detected at the target position and provided a selection criterion for the 168–170Pt nuclei. This technique enables the problem of the background from higher-energy α decays in the spectrum to be circumvented. The Pt nuclei were separated in flight using the gas-filled separator RITU and implanted into the GREAT spectrometer, which was used to study subsequent α decays. The α -decay branching ratios of 164–166Os were deduced from the fraction of selected 168–170Pt nuclei correlated with α decays of 164–166Os. The resulting branching ratios agree w…

PhysicsNuclear reactionNuclear and High Energy PhysicsIsotopeBranching fractionNuclideAlpha decayAtomic physicsInstrumentationRadioactive decayCharged particleSpectral lineNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Emission patterns of neutral pions in40AMeV Ta+Au reactions

2010

Differential cross sections of neutral pions emitted in {sup 181}Ta+{sup 197}Au collisions at a beam energy of 39.5A MeV have been measured with the two-arm photon spectrometer (TAPS). The kinetic energy and transverse momentum spectra of neutral pions cannot be properly described in the framework of the thermal model, nor when the reabsorption of pions is accounted for in a phenomenological model. However, high energy and high momentum tails of the pion spectra can be well fitted through thermal distributions with unexpectedly soft temperature parameters below 10 MeV.

PhysicsNuclear reactionNuclear and High Energy PhysicsPhotonMeson010308 nuclear & particles physicsNuclear TheoryHadronKinetic energy7. Clean energy01 natural sciencesSpectral lineNuclear physicsPion0103 physical sciencesPhenomenological modelAtomic physicsNuclear Experiment010306 general physicsPhysical Review C
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The distribution of the rotational transition strength in warm nuclei studied through γ-ray correlations

1995

Abstract The study of damping of rotational motion applying te rotational plane mapping (RPM) method is presented and discussed. The aim of this technique is to extract the distribution of the rotational transition strength from an analysis of the shape of the “central valley” of two- and three-dimensional γ-ray spectra. The method is applied to a triple γ-coincidence data set of 162,163Tm nuclei formed in 37Cl+130Te reactions. The rotational transition strength is obtained as a function of rotational frequency for selected regions of entry states, and the width is found to be rather constant and approximately equal to 80 keV. This value is significantly smaller than the value predicted the…

PhysicsNuclear reactionNuclear and High Energy PhysicsRotation around a fixed axisRotational transitionRotational temperatureRotational–vibrational spectroscopyAtomic physicsResidualRotational partition functionSpectral lineNuclear Physics A
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Nuclear structure of 157Gd

2003

Abstract The energy levels of 157 Gd have been investigated using the (n,  γ ) and (n, n′ γ ) reactions. As a result of the analysis of the γ -ray spectra from 16 isolated neutron resonances, a level scheme with a complete set of levels with spins J =1/2, 3/2 has been established up to 1.86 MeV excitation energy. A part of the level scheme is interpreted in more detail on the basis of Coriolis and Δ N =2 coupled Nilsson configurations. Slightly different sets of shape parameters are deduced for negative- and positive-parity levels. A large excess of unassigned 1/2 and 3/2 levels evidently requires an explanation in terms of inclusion of new additional degrees of freedom.

PhysicsNuclear reactionNuclear and High Energy PhysicsSpinsBasis (linear algebra)Degrees of freedom (physics and chemistry)Nuclear structureNeutronAtomic physicsExcitationSpectral lineNuclear Physics A
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Silicon Oxysulfide, OSiS: Rotational Spectrum, Quantum-Chemical Calculations, and Equilibrium Structure.

2011

Silicon oxysulfide, OSiS, and seven of its minor isotopic species have been characterized for the first time in the gas phase at high spectral resolution by means of Fourier transform microwave spectroscopy. The equilibrium structure of OSiS has been determined from the experimental data using calculated vibration-rotation interaction constants. The structural parameters (rO-Si = 1.5064 A and rSi-S = 1.9133 A) are in very good agreement with values from high-level quantum chemical calculations using coupled-cluster techniques together with sophisticated additivity and extrapolation schemes. The bond distances in OSiS are very short in comparison with those in SiO and SiS. This unexpected fi…

PhysicsOSiSequilibrium structureSiliconrotational spectrumTriatomic moleculeExtrapolationchemistry.chemical_elementMolecular physicsPartial chargesymbols.namesakeFourier transformchemistryAdditive functionsymbolsPhysical chemistryGeneral Materials ScienceRotational spectroscopyPhysical and Theoretical ChemistrySpectral resolutionquantum chemical calculationComputer Science::Cryptography and SecurityThe journal of physical chemistry letters
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Aluminum cluster anions: Photoelectron spectroscopy andab initiosimulations

2000

Atomic structures and geometries, electronic structure, and temperature-dependent photoelectron spectra of ${\mathrm{Al}}_{N}^{\ensuremath{-}} (N=19\ensuremath{-}102)$ clusters are studied both theoretically via ab initio local-density-functional simulations, and experimentally with high-resolution measurements. The use of a theoretically well-defined energy shift in conjunction with a generalized Koopmans' theorem enables direct comparisons between the calculated density of states and the experimental photoelectron spectrum. Such comparisons, using photoelectron spectra calculated for various relaxed cluster geometries, enables a determination of the optimal structures of the clusters. The…

PhysicsOctahedronX-ray photoelectron spectroscopyPhotoemission spectroscopyPhysics::Atomic and Molecular ClustersAb initioDensity of statesCluster (physics)Electronic structureAtomic physicsSpectral linePhysical Review B
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Pulsating B and Be Stars in the Magellanic Clouds

2010

Stellar pulsations in main-sequence B-type stars are driven by the κ-mechanism due to the Fe-group opacity bump. The current models do not predict the presence of instability strips in the B spectral domain at very low metallicities. As the metallicity of the Magellanic Clouds (MC) has been measured to be around Z = 0. 002 for the Small Magellanic Cloud (SMC) and Z = 0. 007 for the Large Magellanic Cloud (LMC), they constitute a very suitable objects to test these predictions. The aim of this work is to investigate the existence of B-type pulsators at low metallicities, searching for short-term periodic variability in a large sample of B and Be stars from the MC with accurately determined f…

PhysicsOpacityAstrophysics::High Energy Astrophysical PhenomenaMetallicitySpectral domainAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsInstabilityLarge sampleStars13. Climate actionAstrophysics::Solar and Stellar AstrophysicsSmall Magellanic CloudLarge Magellanic CloudAstrophysics::Galaxy Astrophysics
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