Search results for "Observable"

showing 10 items of 634 documents

Scalar Dark Matter in the Radio-Frequency Band: Atomic-Spectroscopy Search Results

2019

Among the prominent candidates for dark matter are bosonic fields with small scalar couplings to the Standard-Model particles. Several techniques are employed to search for such couplings and the current best constraints are derived from tests of gravity or atomic probes. In experiments employing atoms, observables would arise from expected dark-matter-induced oscillations in the fundamental constants of nature. These studies are primarily sensitive to underlying particle masses below $10^{-14}$ eV. We present a method to search for fast oscillations of fundamental constants using atomic spectroscopy in cesium vapor. We demonstrate sensitivity to scalar interactions of dark matter associate…

PhysicsAtomic Physics (physics.atom-ph)Dark matterScalar (physics)FOS: Physical sciencesGeneral Physics and AstronomyObservableAtomic spectroscopy01 natural sciencesCesium vaporPhysics - Atomic Physics3. Good healthGravitationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Particle mass0103 physical sciencesRadio frequencyAtomic physics010306 general physicsPhysical Review Letters
researchProduct

A mysterious Universe : revealing the bright and dark sides of the cosmos

2016

Why is our universe as we observe it? Will it be the same forever? Understanding the nature of the main constituents of the universe is crucial to obtain a precise description of the way in which it reached its present state. Nowadays, many independent observations support a picture in which the matter content of the universe is shared between an ordinary and observable baryonic component ( ~ 5?%) and an invisible dark matter ( ~ 23?%). The remaining ~ 72?% of the universe content is in the form of a completely mysterious dark energy field. This composition emphasizes that, while ~ 95?% of our universe represents a major uncertainty for us, even the minor contribution from normal and, appar…

PhysicsBaryonMultidisciplinaryCold dark matterHistory and Philosophy of Sciencemedia_common.quotation_subjectDark matterDark energyObservableAstrophysicsUniversemedia_common
researchProduct

Test of a separable approximation to a local soft-core potential in the three-body system

1975

Three-nucleon observables below the break-up threshold are calculated employing the pole approximation to the soft-core Malfliet-Tjon potentials. The results are compared in detail to those obtained with the local potentials and to those calculated with the usual Yamaguchi interactions.

PhysicsBody systemNuclear and High Energy PhysicsPole approximationNuclear TheoryMathematical analysisObservable/dk/atira/pure/sustainabledevelopmentgoals/clean_water_and_sanitationSeparable spaceSoft coreNuclear cross sectionNuclear drip lineAtomic physicsSDG 6 - Clean Water and SanitationZeitschrift f�r Physik A Atoms and Nuclei
researchProduct

Kadanoff-Baym approach to quantum transport through interacting nanoscale systems: from the transient to the steady-state regime

2009

We propose a time-dependent many-body approach to study the short-time dynamics of correlated electrons in quantum transport through nanoscale systems contacted to metallic leads. This approach is based on the time-propagation of the Kadanoff-Baym equations for the nonequilibrium many-body Green's function of open and interacting systems out of equilibrium. An important feature of the method is that it takes full account of electronic correlations and embedding effects in the presence of time-dependent external fields, while at the same time satisfying the charge conservation law. The method further extends the Meir-Wingreen formula to the time domain for initially correlated states. We stu…

PhysicsCharge conservationSteady stateCondensed Matter - Mesoscale and Nanoscale PhysicsQuantum wireNon-equilibrium thermodynamicsFOS: Physical sciencesObservableElectronCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsSettore FIS/03 - Fisica della MateriaQuantum mechanicsMesoscale and Nanoscale Physics (cond-mat.mes-hall)QuasiparticleTime domain
researchProduct

The <FONT FACE=Symbol>d</font> Expansion and the Principle of Minimal Sensitivity

1998

The d-expansion is a nonperturbative approach for field theoretic models wich combines the techniques of perturbation theory and the variational principle. Different ways of implemeting the principle of minimal sensitivity to the d-expansion produce in general different results for observables. For illustration we use the Nambu- Jona-Lasinio model for chiral symmetry restoration at finite density and compare results with those obtained with the Hartree-Fock approximation.

PhysicsChiral symmetryField (physics)Variational principleHigh Energy Physics::LatticeQuantum electrodynamicsNuclear TheoryHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyApplied mathematicsObservablePerturbation theory (quantum mechanics)Sensitivity (control systems)Brazilian Journal of Physics
researchProduct

Central role of the observable electric potential in transport equations.

2001

Nonequilibrium systems are usually studied in the framework of transport equations that involve the true electric potential (TEP), a nonobservable variable. Nevertheless another electric potential, the observable electric potential (OEP), may be defined to construct a useful set of transport equations. In this paper several basic characteristics of the OEP are deduced and emphasized: (i) the OEP distribution depends on thermodynamic state of the solution, (ii) the observable equations have a reference value for all other transport equations, (iii) the bridge that connects the OEP with a certain TEP is usually defined by the ion activity coefficient, (iv) the electric charge density is a non…

PhysicsClassical mechanicsDistribution (mathematics)Thermodynamic statePhysics::Atomic and Molecular ClustersNon-equilibrium thermodynamicsCharge densityObservableStatistical physicsElectric potentialIonVariable (mathematics)Physical review. E, Statistical, nonlinear, and soft matter physics
researchProduct

Neutrino halos in clusters of galaxies and their weak lensing signature

2011

We study whether non-linear gravitational effects of relic neutrinos on the development of clustering and large-scale structure may be observable by weak gravitational lensing. We compute the density profile of relic massive neutrinos in a spherical model of a cluster of galaxies, for several neutrino mass schemes and cluster masses. Relic neutrinos add a small perturbation to the mass profile, making it more extended in the outer parts. In principle, this non-linear neutrino perturbation is detectable in an all-sky weak lensing survey such as EUCLID by averaging the shear profile of a large fraction of the visible massive clusters in the universe, or from its signature in the general weak …

PhysicsCold dark matterCosmology and Nongalactic Astrophysics (astro-ph.CO)CosmologiaHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and AstrophysicsObservableAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxyBaryonGravitationNeutrinoWeak gravitational lensingGalaxy clusterAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Gravitational waves from galaxy clusters: a new observable effect

1998

A rich galaxy cluster showing strong resemblance with the observed ones is simulated. Cold dark matter spectrum, Gaussian statistics, flat universe, and two components -- baryonic gas plus dark matter particles -- are considered. We have calculated the gravitational-wave output during the epoch of the fully nonlinear and nonsymmetric cluster evolution. The amplitudes and frequencies of the resulting gravitational waves are estimated. Since frequencies are very small --of the order of $10^{-17} Hz$ -- a complete pulse cannot be observed during an admissible integration time; nevertheless, it is proved that these waves can produce an interesting secular effect which appears to be observable w…

PhysicsCold dark matterGravitational waveDark matterAstrophysics (astro-ph)Shape of the universeFOS: Physical sciencesAstronomy and AstrophysicsObservableAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGravitationSpace and Planetary ScienceCluster (physics)Galaxy cluster
researchProduct

Towards an understanding of discrete ambiguities in truncated partial wave analyses

2017

It is well known that the observables in a single-channel scattering problem remain invariant once the amplitude is multiplied by an overall energy- and angle-dependent phase. This invariance is called the continuum ambiguity and acts on the infinite partial wave set. It has also long been known that, in the case of a truncated partial wave set, another invariance exists, originating from the replacement of the roots of partial wave amplitudes with their complex conjugate values. This discrete ambiguity is also known as the Omelaenko-Gersten-type ambiguity. In this paper, we show that for scalar particles, discrete ambiguities are just a subset of continuum ambiguities with a specific phase…

PhysicsComplex conjugateContinuum (measurement)Nuclear Theory010308 nuclear & particles physicsScatteringNumerical analysismedia_common.quotation_subjectFOS: Physical sciencesObservableComputer Science::Computation and Language (Computational Linguistics and Natural Language and Speech Processing)AmbiguityInvariant (physics)01 natural sciencesNuclear Theory (nucl-th)partial wave decomposition continuum and discrete ambiguitiesTheoretical physicsAmplitude0103 physical sciences010306 general physicsmedia_common
researchProduct

Quantum Monte Carlo simulations of antiferromagnetism in ultracold fermions on optical lattices within real-space dynamical mean-field theory

2010

We present a massively parallel quantum Monte Carlo based implementation of real-space dynamical mean-field theory for general inhomogeneous correlated fermionic lattice systems. As a first application, we study magnetic order in a binary mixture of repulsively interacting fermionic atoms harmonically trapped in an optical lattice. We explore temperature effects and establish signatures of the N\'{e}el transition in observables directly accessible in cold-atom experiments; entropy estimates are also provided. We demonstrate that the local density approximation (LDA) fails for ordered phases. In contrast, a "slab" approximation allows us to reach experimental system sizes with O(10^5) atoms …

PhysicsCondensed Matter::Quantum GasesOptical latticeQuantum Monte CarloGeneral Physics and AstronomyBinary numberFOS: Physical sciencesObservableFermionComputational Physics (physics.comp-ph)Hardware and ArchitectureQuantum Gases (cond-mat.quant-gas)Quantum mechanicsLattice (order)AntiferromagnetismLocal-density approximationCondensed Matter - Quantum GasesPhysics - Computational Physics
researchProduct