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showing 10 items of 3931 documents

Softening Transitions with Quenched 2D Gravity

1996

We perform extensive Monte Carlo simulations of the 10-state Potts model on quenched two-dimensional $\Phi^3$ gravity graphs to study the effect of quenched connectivity disorder on the phase transition, which is strongly first order on regular lattices. The numerical data provides strong evidence that, due to the quenched randomness, the discontinuous first-order phase transition of the pure model is softened to a continuous transition.

PhysicsNuclear and High Energy PhysicsGravity (chemistry)Phase transitionContinuous transitionHigh Energy Physics::LatticeMonte Carlo methodHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesFirst orderAtomic and Molecular Physics and OpticsHigh Energy Physics - LatticeStatistical physicsSofteningRandomnessPotts model
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Nuclear matrix elements of ββ decay from β-decay data

2005

Abstract The evaluation of the nuclear matrix elements (NME) of the two-neutrino double beta ( 2 ν β β ) decay and neutrinoless double beta ( 0 ν β β ) decay using the proton–neutron quasiparticle random-phase approximation (pnQRPA) is addressed. In particular, the extraction of a proper value of the proton–neutron particle–particle interaction parameter, g pp , of this theory is analyzed in detail. Evidence is shown, that it can be misleading to use the experimental half-life of the 2 ν β β decay to extract a value for g pp . Rather, arguments are given in favour of using the available data on single beta decay for this purpose.

PhysicsNuclear and High Energy PhysicsHalf-lifeProton–neutron interactionBeta decayDouble beta decayNuclear physicsDouble beta decayNuclear matrix elementsQuasiparticleQuasiparticle random-phase approximationBeta (velocity)High Energy Physics::ExperimentNeutrinoRandom phase approximationNuclear ExperimentEigenvalues and eigenvectorsPhysics Letters B
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Test of the proton-neutron random-phase approximation method within an extended Lipkin-type model

2001

An extended Lipkin-Meshkov-Glick model for testing the proton-neutron random-phase approximation $(pn\mathrm{RPA})$ method is developed, taking into account explicitly proton and neutron degrees of freedom. Besides the proton and neutron single-particle terms two types of residual proton-neutron interactions, one simulating a particle-particle and the other a particle-hole interaction, are included in the model Hamiltonian so that the model is exactly solvable in an isospin $\mathrm{SU}(2)\ensuremath{\bigotimes}\mathrm{SU}(2)$ basis. The behavior of the first excited (collective) state obtained by (i) exact diagonalization of the Hamiltonian matrix and (ii) with the $\mathrm{pn}\mathrm{RPA}…

PhysicsNuclear and High Energy PhysicsHamiltonian matrixNuclear TheoryDegrees of freedom (physics and chemistry)EigenfunctionType (model theory)symbols.namesakeIsospinQuantum mechanicssymbolsNeutronNuclear ExperimentRandom phase approximationHamiltonian (quantum mechanics)Physical Review C
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Investigation of the decay of to excited states in

1996

The two-neutrino mode of double beta decay of is investigated both theoretically and experimentally. The calculations, using the quasiparticle random phase approximation approach, show that for the detection of transitions to the two first excited states in the daughter nuclide will be possible in the very near future. On the experimental side, new, most stringent limits on half-lives for the double beta decay of to excited states in have been obtained with a `well-type' germanium detector. They range between and years (90% CL).

PhysicsNuclear and High Energy PhysicsInternal conversionDecay schemeExcited stateDouble beta decayQuasiparticleHigh Energy Physics::ExperimentAtomic physicsDecay productRandom phase approximationBeta-decay stable isobarsJournal of Physics G: Nuclear and Particle Physics
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New region of deformation in the neutron-rich 60 24Cr36 and 62 24Cr38

2003

The neutron-rich nuclei 23 60-63V have been produced at GANIL via interactions of a 61.8A·MeV 76Ge beam with a 58Ni target. Beta-decay to 24 60-63Cr has been investigated using combined β- and γ-ray spectroscopy. Half-lives of the 60-63V nuclei have been determined, and the existence of a beta-decay isomer in the 60V nucleus is strongly supported. The observation of low-energy 2+ states in 60Cr (646keV) and 62Cr (446keV) suggests that these isotopes are strongly deformed with β2 ∼ 0.3. This is confirmed by shell model calculations which show the dominant influence of the intruder g and d orbitals to obtain low 2+ energies in the neutron-rich Cr isotopes.

PhysicsNuclear and High Energy PhysicsIsotope010308 nuclear & particles physicsHadron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesmedicine.anatomical_structureAtomic orbital0103 physical sciencesmedicineNuclear fusionNeutronAtomic physics010306 general physicsRandom phase approximationSpectroscopyNucleusThe European Physical Journal A
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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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Enhanced solar anti-neutrino flux in random magnetic fields

2004

We discuss the impact of the recent KamLAND constraint on the solar anti-neutrino flux on the analysis of solar neutrino data in the presence of Majorana neutrino transition magnetic moments and solar magnetic fields. We consider different stationary solar magnetic field models, both regular and random, highlighting the strong enhancement in the anti-neutrino production rates that characterize turbulent solar magnetic field models. Moreover, we show that for such magnetic fields inside the Sun, one can constrain the intrinsic neutrino magnetic moment down to the level of mu_nu lessthan few times 10^-12 x mu_B irrespective of details of the underlying turbulence model. This limit is more str…

PhysicsNuclear and High Energy PhysicsMagnetic momentMagnetismSolar neutrinoAstrophysics (astro-ph)FOS: Physical sciencesFísicaAstrophysicsMagnetic fieldNuclear physicsMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics::Space PhysicsNeutrinoOrder of magnitudeRandomness
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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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