Search results for " Phase"

showing 10 items of 1862 documents

β-delayed neutron decay of 104Y, 112Tc, 113Tc and 114Tc: test of half-life predictions for neutron-rich isotopes of refractory elements

1999

Abstract Beta-decay gross properties of neutron-rich isotopes 104Y and 112,113,114Tc produced in 25 MeV proton-induced fission of 238U have been measured. Decays of 104Y with a half-life of 180±60 ms and of 114Tc with a half-life of 150±30 ms are reported for the first time. Beta-delayed neutron emission probabilities of 112,113,114Tc are determined as (1.5±0.2)%, (2.1±0.3)% and (1.3±0.4)%, respectively. Comparison of the observed Pn values with a recent theoretical calculation based on deformed quasiparticle random phase approximation (QRPA) shows good overall agreement for Tc isotopes. However, comparison of beta-decay half-lives of neutron-rich isotopes of Y to Rh with the QRPA model and…

PhysicsNuclear and High Energy PhysicsIsotopeFissionNeutron emissionNuclear TheoryHalf-lifeNuclear physicsQuasiparticleNeutronAtomic physicsNuclear ExperimentRandom phase approximationDelayed neutronPhysics Letters B
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Collective rotational – vibrational transition in the very neutron-deficient nuclei Pt

1998

Excited states have been identified for the first time in very neutron deficient Pt-171.172 nuclei using the recoil-or-decay tagging technique. The ground-state band in Pt-172 has been established up to I-pi = 8+. A similar level sequence, presumably built on the I-pi = 13/2(+) state, is observed for Pt-171. The data are compared with theoretical calculations based on the mean field approach and the random phase approximation and are put into the context of the systematics of platinum isotopes. (C) 1998 Elsevier Science B.V. All rights reserved.

PhysicsNuclear and High Energy PhysicsIsotopechemistryMean field theoryExcited statechemistry.chemical_elementNeutronContext (language use)Atomic physicsRandom phase approximationPlatinumPhysics Letters B
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Fully self-consistent calculations of nuclear Schiff moments

2010

We calculate the Schiff moments of the nuclei 199Hg and 211Ra in completely self-consistent odd-nucleus mean-field theory by modifying the Hartree-Fock-Bogoliubov code HFODD. We allow for arbitrary shape deformation, and include the effects of nucleon dipole moments alongside those of a CP-violating pion-exchange nucleon-nucleon interaction. The results for 199Hg differ significantly from those of previous calculations when the CP-violating interaction is of isovector character.

PhysicsNuclear and High Energy PhysicsIsovectorNuclear TheoryNuclear TheoryFOS: Physical sciencesSelf consistentSymmetry (physics)Nuclear Theory (nucl-th)DipoleMean field theoryCP violationAtomic physicsNucleonRandom phase approximationNuclear Experiment
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Kπ=8−isomers andKπ=2−octupole vibrations inN=150shell-stabilized isotones

2008

Isomers have been populated in {sup 246}Cm and {sup 252}No with quantum numbers K{sup {pi}}=8{sup -}, which decay through K{sup {pi}}=2{sup -} rotational bands built on octupole vibrational states. For N=150 isotones with (even) atomic number Z=94-102, the K{sup {pi}}=8{sup -} and 2{sup -} states have remarkably stable energies, indicating neutron excitations. An exception is a singular minimum in the 2{sup -} energy at Z=98, due to the additional role of proton configurations. The nearly constant energies, in isotones spanning an 18% increase in Coulomb energy near the Coulomb limit, provide a test for theory. The two-quasiparticle K{sup {pi}}=8{sup -} energies are described with single-pa…

PhysicsNuclear and High Energy PhysicsMean field theoryProtonQuasiparticleWoods–Saxon potentialAtomic numberAtomic physicsQuantum numberRandom phase approximationEnergy (signal processing)Physical Review C
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Neutrino propagation and spin zero sound in hot neutron matter with Skyrme interactions

1999

We present microscopic calculations of neutrino propagation in hot neutron matter above nuclear density within the framework of the Random Phase Approximation . Calculations are performed for non- degenerate neutrinos using various Skyrme effective interactions. We find that for densities just above nuclear density, spin zero sound is present at zero temperature for all Skyrme forces considered. However it disappears rapidly with increasing temperature due to a strong Landau damping. As a result the mean-free path is given, to a good approximation, by the mean field value. Because of the renormalization of the bare mass in the mean field, the medium is more transparent as compared to the fr…

PhysicsNuclear and High Energy PhysicsMean free pathBare massNuclear TheoryFOS: Physical sciencesFísicaZero soundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Mean field theoryQuantum mechanicsQuantum electrodynamicsNeutronNeutrinoRandom phase approximationNuclear density
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Finite-size effects and collective vibrations in the inner crust of neutron stars

2010

We study the linear response of the inner crust of neutron stars within the Random Phase Approximation, employing a Skyrme-type interaction as effective interaction. We adopt the Wigner-Seitz approximation, and consider a single unit cell of the Coulomb lattice which constitutes the inner crust, with a nucleus at its center, surrounded by a sea of free neutrons. With the use of an appropriate operator, it is possible to analyze in detail the properties of the vibrations of the surface of the nucleus and their interaction with the modes of the sea of free neutrons, and to investigate the role of shell effects and of resonant states.

PhysicsNuclear and High Energy PhysicsNuclear Theory010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryFOS: Physical sciencesElementary particle01 natural sciencesNuclear Theory (nucl-th)Nuclear physicsBaryonNeutron starStars0103 physical sciencesCoulombNeutronAtomic physics010306 general physicsRandom phase approximationNucleonNuclear Experiment
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An extended Lipkin-type model with residual proton-neutron interaction

1997

Abstract The Lipkin-Meshkov-Glick (LMG) model is extended to explicitly take into account the proton and neutron degrees of freedom. The proton and neutron Hamiltonians are taken to be of the LMG form, and, in addition, a residual proton-neutron interaction is include. Exact solutions in an SU (2) ⊗ SU (2) basis as well as the RPA solutions for the energy spectrum of the model Hamiltonian are obtained. The spectrum of the exact solutions is degenerate in the limit of no proton-neutron residual interaction, but this degeneracy is totally removed when this type of residual interaction is turned on. The spectrum obtained with RPA is compressed or expanded, as compared to the LMG model with the…

PhysicsNuclear and High Energy PhysicsNuclear TheoryDegenerate energy levelsResidualsymbols.namesakeQuantum mechanicsExcited stateEnergy spectrumsymbolsNeutronRandom phase approximationNucleonHamiltonian (quantum mechanics)Nuclear Physics A
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Linear response of light deformed nuclei investigated by self-consistent quasiparticle random-phase approximation

2010

We present a calculation of the properties of vibrational states in deformed, axially-symmetric even-even nuclei, within the framework of a fully self-consistent quasiparticle random phase approximation (QRPA). The same Skyrme energy density and density-dependent pairing functionals are used to calculate the mean field and the residual interaction in the particle-hole and particle-particle channels. We have tested our software in the case of spherical nuclei against fully self-consistent calculations published in the literature, finding excellent agreement. We investigate the consequences of neglecting the spin-orbit and Coulomb residual interactions in QRPA. Furthermore we discuss the impr…

PhysicsNuclear and High Energy PhysicsNuclear TheoryIsovectorIsoscalarNuclear TheoryFOS: Physical sciencesNuclear Theory (nucl-th)Mean field theoryQuantum mechanicsPairingQuasiparticleCoulombAtomic physicsSpin (physics)Random phase approximationPhysical Review C
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Linear response strength functions with iterative Arnoldi diagonalization

2009

We report on an implementation of a new method to calculate RPA strength functions with iterative non-hermitian Arnoldi diagonalization method, which does not explicitly calculate and store the RPA matrix. We discuss the treatment of spurious modes, numerical stability, and how the method scales as the used model space is enlarged. We perform the particle-hole RPA benchmark calculations for double magic nucleus 132Sn and compare the resulting electromagnetic strength functions against those obtained within the standard RPA.

PhysicsNuclear and High Energy PhysicsNuclear TheoryIterative methodNuclear TheoryFOS: Physical sciencesCalculation methodsNuclear Theory (nucl-th)Quantum mechanicsIsotopes of tinPhysics::Atomic and Molecular ClustersApplied mathematicsSpurious relationshipRandom phase approximationNuclear theoryNumerical stability
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Short-range correlations and neutrinoless double beta decay

2007

In this work we report on the effects of short-range correlations upon the matrix elements of neutrinoless double beta decay. We focus on the calculation of the matrix elements of the neutrino-mass mode of neutrinoless double beta decays of 48Ca and 76Ge. The nuclear-structure components of the calculation, that is the participant nuclear wave functions, have been calculated in the shell-model scheme for 48Ca and in the proton-neutron quasiparticle random-phase approximation (pnQRPA) scheme for 76Ge. We compare the traditional approach of using the Jastrow correlation function with the more complete scheme of the unitary correlation operator method (UCOM). Our results indicate that the Jast…

PhysicsNuclear and High Energy PhysicsNuclear TheoryOperator (physics)Nuclear TheoryNuclear structureUnitary correlation operator methodFOS: Physical sciencesFísicaNuclear physicsNuclear Theory (nucl-th)Matrix (mathematics)Correlation functionDouble beta decayNuclear matrix elementsNeutronHigh Energy Physics::ExperimentNeutrinoless double beta decayWave functionRandom phase approximationNuclear ExperimentShort-range correlations
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