Search results for "descriptive"

showing 10 items of 494 documents

The scale dependent nuclear effects in parton distributions for practical applications

1999

The scale dependence of the ratios of parton distributions in a proton of a nucleus $A$ and in the free proton, $R_i^A(x,Q^2)=f_{i/A}(x,Q^2)/f_i(x,Q^2)$, is studied within the framework of the lowest order leading-twist DGLAP evolution. By evolving the initial nuclear distributions obtained with the GRV-LO and CTEQ4L sets at a scale $Q_0^2$, we show that the ratios $R_i^A(x,Q^2)$ are only moderately sensitive to the choice of a specific modern set of free parton distributions. We propose that to a good first approximation, this parton distribution set-dependence of the nuclear ratios $R_i^A(x,Q^2)$ can be neglected in practical applications. With this result, we offer a numerical parametriz…

PhysicsParticle physicsPhysics and Astronomy (miscellaneous)ProtonNuclear TheoryFOS: Physical sciencesDrell–Yan processOrder (ring theory)Scale (descriptive set theory)PartonNuclear Theory (nucl-th)Nuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Distribution (mathematics)DGLAPEngineering (miscellaneous)Parametrization
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New opportunities at the next-generation neutrino experiments I: BSM neutrino physics and dark matter

2020

Abstract The combination of the high intensity proton beam facilities and massive detectors for precision measurements of neutrino oscillation parameters including the charge-parity violating (CPV) phase will open the door to help make beyond the standard model (BSM) physics reachable even in low energy regimes in the accelerator-based experiments. Large-mass detectors with highly precise tracking and energy measurements, excellent timing resolution, and low energy thresholds will enable the searches for BSM phenomena from cosmogenic origin, as well. Therefore, it is also conceivable that BSM topics in the next-generation neutrino experiments could be the dominant physics topics in the fore…

PhysicsParticle physicsSterile neutrinoPhysics beyond the Standard ModelDark matterGeneral Physics and AstronomyScale (descriptive set theory)Tracking (particle physics)01 natural sciences0103 physical sciencesDeep Underground Neutrino ExperimentHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationReports on Progress in Physics
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Charm-beauty meson bound states from B(B*)D(D*) and B(B*)D¯(D¯*) interaction

2017

We evaluate the $s$-wave interaction of pseudoscalar and vector mesons with both charm and beauty to investigate the possible existence of molecular $BD$, ${B}^{*}D$, $B{D}^{*}$, ${B}^{*}{D}^{*}$, $B\overline{D}$, ${B}^{*}\overline{D}$, $B{\overline{D}}^{*}$, or ${B}^{*}{\overline{D}}^{*}$ meson states. The scattering amplitude is obtained implementing unitarity starting from a tree level potential accounting for the dominant vector meson exchange. The diagrams are evaluated using suitable extensions to the heavy flavor sector of the hidden gauge symmetry Lagrangians involving vector and pseudoscalar mesons, respecting heavy quark spin symmetry. We obtain bound states at energies above 7 Ge…

PhysicsParticle physicsUnitarityMeson010308 nuclear & particles physicsHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::Phenomenology01 natural sciencesPseudoscalar mesonTree (descriptive set theory)Isospin0103 physical sciencesBound stateHigh Energy Physics::ExperimentVector mesonExotic meson010306 general physicsPhysical Review D
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Lepton-number violation with quasi-Dirac neutrinos

1983

We investigate lepton-number violation in weak interactions with massive Dirac neutrinos. In the framework of a simple $\mathrm{SU}{(3)}_{L}\ifmmode\times\else\texttimes\fi{}\mathrm{U}(1)$ electroweak model we find that neutrinos naturally acquire only Dirac masses at tree level, and for an odd number of lepton families, one neutrino remains massless. After a spontaneous breakdown of symmetry we find that the SU(2)\ifmmode\times\else\texttimes\fi{}U(1) effective theory has lepton-number-violating currents which couple to the standard gauge bosons. Flavorconserving $|\ensuremath{\Delta}l|=2$ processes such as neutrinoless double-$\ensuremath{\beta}$ decay are forbidden in the simplest model,…

PhysicsSemileptonic decayGauge bosonParticle physicsMuonHigh Energy Physics::PhenomenologyFísicaElementary particleLepton numberMassless particleTree (descriptive set theory)Particle decayHigh Energy Physics::ExperimentPhysical Review D
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A large rotating structure around AB Doradus A at VLBI scale

2019

AbstractWe report the results of three VLBI observations of the pre-main-sequence star AB Doradus A at 8.4 GHz. With almost three years between consecutive observations, we found a complex structure at the expected position of this star for all epochs. Maps at epochs 2007 and 2010 show a double core-halo morphology while the 2013 map reveals three emission peaks with separations between 5 and 18 stellar radii. Furthermore, all maps show a clear variation of the source structure within the observing time. We consider a number of hypothesis in order to explain such observations, mainly: magnetic reconnection in loops on the polar cap, a more general loop scenario and a close companion to AB D…

PhysicsSource structure010308 nuclear & particles physicsStructure (category theory)Astronomy and AstrophysicsScale (descriptive set theory)Magnetic reconnectionAstrophysicsStar (graph theory)01 natural sciencesSpace and Planetary SciencePosition (vector)0103 physical sciencesVery-long-baseline interferometryVariation (astronomy)010303 astronomy & astrophysicsProceedings of the International Astronomical Union
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Dynamical Heterogeneities Below the Glass Transition

2001

We present molecular dynamics simulations of a binary Lennard-Jones mixture at temperatures below the kinetic glass transition. The ``mobility'' of a particle is characterized by the amplitude of its fluctuation around its average position. The 5% particles with the largest/smallest mean amplitude are thus defined as the relatively most mobile/immobile particles. We investigate for these 5% particles their spatial distribution and find them to be distributed very heterogeneously in that mobile as well as immobile particles form clusters. The reason for this dynamic heterogeneity is traced back to the fact that mobile/immobile particles are surrounded by fewer/more neighbors which form an ef…

PhysicsStatistical Mechanics (cond-mat.stat-mech)General Physics and AstronomyBinary numberFOS: Physical sciencesScale (descriptive set theory)Disordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksCondensed Matter - Soft Condensed MatterKinetic energyMolecular physicsMolecular dynamicsAmplitudePosition (vector)ParticleSoft Condensed Matter (cond-mat.soft)Physical and Theoretical ChemistryGlass transitionCondensed Matter - Statistical Mechanics
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Learning from observations of the microwave background at small angular scales

1996

In this paper, we focus our attention on the following question: How well can we recover the power spectrum of the cosmic microwave background from the maps of a given experiment?. Each experiment is described by a a pixelization scale, a beam size, a noise level and a sky coverage. We use accurate numerical simulations of the microwave sky and a cold dark matter model for structure formation in the universe. Angular scales smaller than those of previous simulations are included. The spectrum obtained from the simulated maps is appropriately compared with the theoretical one. Relative deviations between these spectra are estimated. Various contributions to these deviations are analyzed. The…

PhysicsStructure formationCold dark mattermedia_common.quotation_subjectAstrophysics (astro-ph)Cosmic microwave backgroundFOS: Physical sciencesSpectral densityAstronomy and AstrophysicsScale (descriptive set theory)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSpace and Planetary ScienceSkyPixelizationMicrowavemedia_common
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Cosmological Vector Perturbations and CMB Anomalies

2010

Recently, it has been proved that large scale vector modes could explain most of the CMB anomalies in the first temperature multipoles. Some divergenceless (vortical) velocity fields–which are superimpositions of vector modes–can explain both the alignment of the second and third multipoles and the planar character of the octopole. In this paper we comment: (a) some papers trying to account for the mentioned anomalies, (b) our explanation based on vector modes, and (c) some current ideas about the possible origin of these modes.

PhysicsTheoretical physicsCurrent (mathematics)Character (mathematics)Cosmic microwave backgroundScale (descriptive set theory)
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The loop-tree duality at work

2014

We review the recent developments of the loop-tree duality method, focussing our discussion on analysing the singular behaviour of the loop integrand of the dual representation of one-loop integrals and scattering amplitudes. We show that within the loop-tree duality method there is a partial cancellation of singularities at the integrand level among the different components of the corresponding dual representation. The remaining threshold and infrared singularities are restricted to a finite region of the loop momentum space, which is of the size of the external momenta and can be mapped to the phase-space of real corrections to cancel the soft and collinear divergences.

PhysicsWork (thermodynamics)010308 nuclear & particles physicsFOS: Physical sciencesDuality (optimization)Position and momentum spaceDual representation01 natural sciencesScattering amplitudeLoop (topology)High Energy Physics - PhenomenologyTree (descriptive set theory)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesGravitational singularity010303 astronomy & astrophysicsMathematical physicsProceedings of Loops and Legs in Quantum Field Theory — PoS(LL2014)
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Target localization in the three-dimensional space by wavelength multiplexing.

2002

A method to localize a target in the three-dimensional space is presented. Each different position of the target on the depth axis produces, when captured with a CCD camera, an image of a different size on its sensor plane. The size of this image depends only on the distance between the target and the camera. The use of a white light optical correlator that gives us a different response depending on the scale of the input image permits us to know the depth position of the particular target. The obtained results demonstrate the utility of the newly proposed method.

Physicsbusiness.industryScale (descriptive set theory)02 engineering and technologySpace (mathematics)01 natural sciencesThree-dimensional spaceMultiplexingAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsImage (mathematics)010309 opticsWavelengthOpticsPosition (vector)[INFO.INFO-IR]Computer Science [cs]/Information Retrieval [cs.IR]Computer Science::Computer Vision and Pattern Recognition0103 physical sciencesOptical correlator0202 electrical engineering electronic engineering information engineering020201 artificial intelligence & image processing[INFO.INFO-IR] Computer Science [cs]/Information Retrieval [cs.IR]Electrical and Electronic EngineeringPhysical and Theoretical Chemistrybusiness
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