Search results for "Statistical physic"

showing 10 items of 1403 documents

Propagation of uncertainties in the nuclear DFT models

2014

Parameters of the nuclear density functional theory (DFT) models are usually adjusted to experimental data. As a result they carry certain theoretical error, which, as a consequence, carries out to the predicted quantities. In this work we address the propagation of theoretical error, within the nuclear DFT models, from the model parameters to the predicted observables. In particularly, the focus is set on the Skyrme energy density functional models.

PhysicsNuclear and High Energy PhysicsWork (thermodynamics)Nuclear TheoryEnergy density functional010308 nuclear & particles physicsNuclear TheoryFOS: Physical sciencesExperimental dataObservable01 natural sciencesNuclear Theory (nucl-th)Set (abstract data type)0103 physical sciencesStatistical physics010306 general physicsFunctional theoryFocus (optics)Nuclear densityJournal of Physics G: Nuclear and Particle Physics
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Application of ultra-fast timing techniques to the study of exotic and weakly produced nuclei

2005

Ultra-fast time-delayed techniques have been recently applied in a number of studies where exotic nuclei were identified using advanced selection techniques. These include large Compton-suppressed Ge arrays, in-flight separators or recoil separators. Some of the new results are discussed in this presentation. Besides the results for $^{32}$Mg and $^{96}$Pd, they include the first determination of the half-life of the $8^+$ state in $^{80}$Ge, $T_1/2$ = 2.95(6) ns, and significantly more precise results for $^{51}$Mn (3680 keV level) and $^{48}$V (421 keV level), $T_1/2$ = 1760(40) ps and $T_1/2$ $\leq$ 135 ps, respectively. Development of new scintillators will steadily improve precision an…

PhysicsNuclear physicsNuclear and High Energy Physics010308 nuclear & particles physics0103 physical sciencesHardware_INTEGRATEDCIRCUITSUltra fastStatistical physics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]010306 general physics7. Clean energy01 natural sciencesSelection (genetic algorithm)
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β− Strength function phenomena of exotic nuclei: A critical examination of the significance of nuclear model predictions

1984

Abstract Reliable predictions of β-decay properties of nuclei far from stability require knowledge of the β-strength distribution, S β ( E ). By comparison of experimental strength functions of neutron-rich Rb isotopes in the transitional region around A = 100 with S β ( E ) from different nuclear models, the sensitivity and physical significance of S β ( E ) on various integral and spectral β-decay properties are examined. The reliability of extrapolations and the applicability to different fields in nuclear physics, astrophysics and reactor technology are discussed. It is shown that, although there has been considerable progress in the physical understanding of the decay properties of nuc…

PhysicsNuclear physicsNuclear and High Energy PhysicsIsotopeStrength functionStatistical physicsStability (probability)Critical examinationNuclear Physics A
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Joint constraints on galaxy bias and σ8 through the N-pdf of the galaxy number density

2015

We present a full description of the N-probability density function of the galaxy number density fluctuations. This N-pdf is given in terms, on the one hand, of the cold dark matter correlations and, on the other hand, of the galaxy bias parameter. The method relies on the assumption commonly adopted that the dark matter density fluctuations follow a local non-linear transformation of the initial energy density perturbations. The N-pdf of the galaxy number density fluctuations allows for an optimal estimation of the bias parameter (e.g., via maximum-likelihood estimation, or Bayesian inference if there exists any a priori information on the bias parameter), and of those parameters defining …

PhysicsNumber densityCold dark matter010308 nuclear & particles physicsModel selectionDark matterEstimatorAstronomy and AstrophysicsProbability density functionAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy0103 physical sciencesStatistical physics010303 astronomy & astrophysicsGalaxy clusterAstrophysics - Cosmology and Nongalactic Astrophysics
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Modulational stability brought by cubic–quartic interactions of the nearest-neighbor in FK model subjected in a parametrized on-site potential

2022

Abstract This work extends to higher-order interactions the results of Ref. Nguetcho (2021), in which we discussed only on modulational instability in one-dimensional chain made of atoms, harmonically coupled to their nearest neighbors and subjected to an external on-site potential. Here we investigate the competition between cubic-quartic nonlinearities interactions of the nearest-neighbor and substrate’s deformability, and mainly discuss its impact on the modulational instability of the system. This makes it possible to adapt the theoretical model to a real physical system such as atomic chains or DNA lattices. The governing equation, derived from the modified Frenkel-Kontorova model, is …

PhysicsNumerical AnalysisGeneric propertyApplied MathematicsPhysical systemInstabilityk-nearest neighbors algorithmsymbols.namesakeModulational instabilityNonlinear systemModeling and SimulationQuartic functionsymbolsStatistical physicsNonlinear Schrödinger equationCommunications in Nonlinear Science and Numerical Simulation
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Brownian dynamics simulations with hard-body interactions: Spherical particles

2012

A novel approach to account for hard-body interactions in (overdamped) Brownian dynamics simulations is proposed for systems with non-vanishing force fields. The scheme exploits the analytically known transition probability for a Brownian particle on a one-dimensional half-line. The motion of a Brownian particle is decomposed into a component that is affected by hard-body interactions and into components that are unaffected. The hard-body interactions are incorporated by replacing the affected component of motion by the evolution on a half-line. It is discussed under which circumstances this approach is justified. In particular, the algorithm is developed and formulated for systems with spa…

PhysicsNumerical analysisFOS: Physical sciencesGeneral Physics and AstronomyProteinsComputational Physics (physics.comp-ph)Condensed Matter - Soft Condensed MatterModels BiologicalDiffusionMotionProbability theoryModels ChemicalProtein Interaction MappingBrownian dynamicsSoft Condensed Matter (cond-mat.soft)Computer SimulationStatistical physicsColloidsPhysical and Theoretical ChemistryPhysics - Computational PhysicsBrownian motionAlgorithms
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Multi-Scale Modeling of Quantum Semiconductor Devices

2006

This review is concerned with three classes of quantum semiconductor equations: Schrodinger models, Wigner models, and fluid-type models. For each of these classes, some phenomena on various time and length scales are presented and the connections between micro-scale and macro-scale models are explained. We discuss Schrodinger-Poisson systems for the simulation of quantum waveguides and illustrate the importance of using open boundary conditions. We present Wigner-based semiconductor models and sketch their mathematical analysis. In particular we discuss the Wigner-Poisson-Focker-Planck system, which is the starting point of deriving subsequently the viscous quantum hydrodynamic model. Furt…

PhysicsOpen quantum systemsymbols.namesakeSemiconductor device modelingInelastic collisionsymbolsWigner distribution functionBoundary value problemStatistical physicsSemiconductor process simulationQuantumSchrödinger's cat
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Oscillation Phenomena Leading to Chaos in a Stochastic Surface Reaction Model

1998

A microscopic lattice gas model for the $\mathrm{CO}+\mathrm{NO}$ reaction on Pt(100) is studied by means of Monte Carlo simulations. It shows different kinetical phenomena such as steady state reaction, damped, regular, and irregular oscillations, as well as a transition into chaotical behavior via the Feigenbaum route. Because of its small number of parameters, each with a specific physical meaning, it enables the investigation of the whole parameter regime leading to a deeper insight to the mechanisms which create the oscillations and chaotical behavior.

PhysicsOscillationLattice (order)Monte Carlo methodGeneral Physics and AstronomyStatistical physicsSurface reactionPhysical Review Letters
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On the dynamics of dislocation patterning

1997

Recent computer simulations on dislocation patterning have provided remarkable results in accordance with empirical laws. Moreover, several analytical models on dislocation dynamics have provided qualitative insight on dislocation patterning. However, a model, based on partial differential equations, which gives a dynamical evolution of dislocation patterns in function of measurable variables still missing. Here, we give a re-formulation of a model proposed some years ago. From this formulation, we obtained that the onset of a dislocation instability is related to the applied stress. The analytical and numerical results reported are partial and studies on this direction are under developmen…

PhysicsPartial differential equationDiffusion equationComputer simulationMechanical EngineeringCondensed Matter PhysicsInstabilityStress (mechanics)Condensed Matter::Materials ScienceClassical mechanicsMechanics of MaterialsReaction–diffusion systemGeneral Materials ScienceStatistical physicsDislocationBifurcationMaterials Science and Engineering: A
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Bs0lifetime measurement in theCP-odd decay channelBs0→J/ψ f0(980)

2016

The lifetime of the $B^{0}_{s}$ meson is measured in the decay channel $B^{0}_{s} \to J/\psi\mbox{ }\pi^+ \pi^-$ with $880 \leq M_{\pi^+\pi^-} \leq 1080$ MeV/$c^2$, which is mainly a CP-odd state and dominated by the $f_{0}(980)$ resonance. In 10.4 fb$^{-1}$ of data collected with the D0 detector in Run II of the Tevatron, the lifetime of the $B^{0}_{s}$ meson is measured to be $\tau(B^{0}_{s}) = 1.70\pm 0.14 \mbox{ (stat)} \pm 0.05 \mbox{ (syst) ps}$. Neglecting CP violation in $B_s^0/\bar{B}_s^0$ mixing, the measurement can be translated into the width of the heavy mass eigenstate of the $B^0_s$, $\Gamma_H = 0.59 \pm 0.05 \mbox{ (stat)} \pm 0.02 \mbox{ (syst)} \mbox{ ps$^{-1}$}$.

PhysicsParticle physicsMeson010308 nuclear & particles physics0103 physical sciencesTevatronCP violationResonanceStatistical physics010306 general physics01 natural sciencesPhysical Review D
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