Search results for "Lambda"

showing 10 items of 632 documents

Polarization effects in the cascade decayΛb→Λ(→pπ−)+J/ψ(→ℓ+ℓ−)in the covariant confined quark model

2013

We calculate the invariant and helicity amplitudes for the nonleptonic decay ${\ensuremath{\Lambda}}_{b}\ensuremath{\rightarrow}\ensuremath{\Lambda}+J/\ensuremath{\psi}$, $\ensuremath{\psi}(2S)$ in the covariant confined quark model. We discuss joint angular decay distributions in the cascade decay ${\ensuremath{\Lambda}}_{b}\ensuremath{\rightarrow}\ensuremath{\Lambda}(\ensuremath{\rightarrow}p{\ensuremath{\pi}}^{\ensuremath{-}})+J/\ensuremath{\psi}$, $\ensuremath{\psi}(2S)(\ensuremath{\rightarrow}{\ensuremath{\ell}}^{+}{\ensuremath{\ell}}^{\ensuremath{-}})$ and calculate some of the asymmetry parameters that characterize the joint angular decay distribution. We confirm expectations from th…

PhysicsBaryonNuclear and High Energy PhysicsParticle physicsLattice (order)High Energy Physics::PhenomenologyQuark modelHyperonHigh Energy Physics::ExperimentSum rule in quantum mechanicsLambdaHelicityLeptonPhysical Review D
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Radiative decay of theΛ*(1520)

2006

A recently developed nonperturbative chiral approach to dynamically generate the 3/2{sup -} baryon resonances has been extended to investigate the radiative decays {lambda}*(1520){yields}{gamma}{lambda}(1116) and {lambda}*(1520){yields}{gamma}{sigma}{sup 0}(1193). We show that the {lambda}*(1520) decay into {gamma}{lambda} is an ideal test for the need of extra components of the resonance beyond those provided by the chiral approach since the largest meson-baryon components give no contribution to this decay. The case is different for {gamma}{sigma} decay, where the theory agrees with experiment, though the large uncertainties of these data call for more precise measurements. Some estimates…

PhysicsBaryonNuclear and High Energy PhysicsParticle physicsMesonUnitarityPartial wave analysisResonanceLambda baryonLambdaSigma baryonPhysical Review C
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Exponential and power-law mass distributions in brittle fragmentation

2004

Generic arguments, a minimal numerical model, and fragmentation experiments with gypsum disk are used to investigate the fragment-size distribution that results from dynamic brittle fragmentation. Fragmentation is initiated by random nucleation of cracks due to material inhomogeneities, and its dynamics are pictured as a process of propagating cracks that are unstable against side-branch formation. The initial cracks and side branches both merge mutually to form fragments. The side branches have a finite penetration depth as a result of inherent damping. Generic arguments imply that close to the minimum strain (or impact energy) required for fragmentation, the number of fragments of size $s…

PhysicsBrittlenessFragmentation (mass spectrometry)NucleationAtomic physicsLambdaPenetration depthPower lawScalingExponential functionPhysical Review E
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Meson-Baryon Interactions in Unitarized Chiral Perturbation Theory

2002

Meson-Baryon Interactions can be successfully described using both Chiral Symmetry and Unitarity. The $s-$wave meson-baryon scattering amplitude is analyzed in a Bethe-Salpeter coupled channel formalism incorporating Chiral Symmetry in the potential. Two body coupled channel unitarity is exactly preserved. The needed two particle irreducible matrix amplitude is taken from lowest order Chiral Perturbation Theory in a relativistic formalism. Off-shell behavior is parameterized in terms of low energy constants. The relation to the heavy baryon limit is discussed. The position of the complex poles in the second Riemann sheet of the scattering amplitude determine masses and widths baryonic reson…

PhysicsChiral perturbation theoryNuclear TheoryMesonUnitarityNuclear TheoryHigh Energy Physics::PhenomenologyFOS: Physical sciencesLambdaBaryonScattering amplitudeNuclear Theory (nucl-th)Riemann hypothesissymbols.namesakeAmplitudesymbolsNuclear ExperimentMathematical physics
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Spontaneous magnon decays in planar ferromagnet

2011

We predict that spin-waves in an easy-plane ferromagnet have a finite lifetime at zero temperature due to spontaneous decays. In zero field the damping is determined by three-magnon decay processes, whereas decays in the two-particle channel dominate in a transverse magnetic field. Explicit calculations of the magnon damping are performed in the framework of the spin-wave theory for the $XXZ$ square-lattice ferromagnet with an anisotropy parameter $\lambda<1$. In zero magnetic field the decays occur for $\lambda^*<\lambda<1$ with $\lambda^*\approx 1/7$. We also discuss possibility of experimental observation of the predicted effect in a number of ferromagnetic insulators.

PhysicsCondensed Matter - Materials ScienceStrongly Correlated Electrons (cond-mat.str-el)Statistical Mechanics (cond-mat.stat-mech)Condensed matter physicsMagnonZero (complex analysis)Materials Science (cond-mat.mtrl-sci)FOS: Physical sciencesGeneral Physics and AstronomyApproxLambdaMagnetic fieldCondensed Matter - Strongly Correlated ElectronsPlanarFerromagnetismCondensed Matter::Strongly Correlated ElectronsAnisotropyCondensed Matter - Statistical Mechanics
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Observational constraints on the LLTB model

2010

We directly compare the concordance LCDM model to the inhomogeneous matter-only alternative represented by LTB void models. To achieve a "democratic" confrontation we explore LLTB models with non-vanishing cosmological constant and perform a global likelihood analysis in the parameter space of cosmological constant and void radius. In our analysis we carefully consider SNe, Hubble constant, CMB and BAO measurements, marginalizing over spectral index, age of the universe and background curvature. We find that the LCDM model is not the only possibility compatible with the observations, and that a matter-only void model is a viable alternative to the concordance model only if the BAO constrain…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Age of the universeFOS: Physical sciencesAstronomy and AstrophysicsLambda-CDM modelCosmological constantAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyMetric expansion of spaceLocal Voidsymbols.namesakesymbolsDark energyBaryon acoustic oscillationsStatistical physicsAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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Clustering of Sloan Digital Sky Survey III Photometric Luminous Galaxies: The Measurement, Systematics and Cosmological Implications

2012

The Sloan Digital Sky Survey (SDSS) surveyed 14,555 square degrees, and delivered over a trillion pixels of imaging data. We present a study of galaxy clustering using 900,000 luminous galaxies with photometric redshifts, spanning between $z=0.45$ and $z=0.65$, constructed from the SDSS using methods described in Ross et al. (2011). This data-set spans 11,000 square degrees and probes a volume of $3h^{-3} \rm{Gpc}^3$, making it the largest volume ever used for galaxy clustering measurements. We present a novel treatment of the observational systematics and its applications to the clustering signals from the data set. In this paper, we measure the angular clustering using an optimal quadrati…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cepheid variablemedia_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciencesFísicaAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLambdaRedshiftGalaxySettore FIS/05 - Astronomia e AstrofisicaSpace and Planetary ScienceSkyBaryon acoustic oscillationsNeutrinoAstrophysics::Galaxy Astrophysicsmedia_commonAstrophysics - Cosmology and Nongalactic Astrophysics
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Improved determination of the β−ν¯e angular correlation coefficient a in free neutron decay with the aSPECT spectrometer

2020

We report on a precise measurement of the electron-antineutrino angular correlation ($a$ coefficient) in free neutron beta-decay from the $a$SPECT experiment. The $a$ coefficient is inferred from the recoil energy spectrum of the protons which are detected in 4$\pi$ by the $a$SPECT spectrometer using magnetic adiabatic collimation with an electrostatic filter. Data are presented from a 100 days run at the Institut Laue Langevin in 2013. The sources of systematic errors are considered and included in the final result. We obtain $a = -0.10430(84)$ which is the most precise measurement of the neutron $a$ coefficient to date. From this, the ratio of axial-vector to vector coupling constants is …

PhysicsCoupling constantSpectrometer010308 nuclear & particles physicsSpectrum (functional analysis)Lambda01 natural sciencesCollimated lightFilter (large eddy simulation)0103 physical sciencesNeutronAtomic physicsNuclear Experiment010306 general physicsAdiabatic processPhysical Review C
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Second sound near lambda transition in presence of quantum vortices

2018

In this paper, temperature waves (also known as second sound) are consid- ered, with their respective coupling with waves in the order parameter describing the transition from normal phase to superfluid phase, and with waves in the vortex length density. We analyze the coupling between these three kinds of waves and explore its relevance in situations not far from the lambda transition. In particular, the expres- sions for the second sound speed and second sound attenuation are explicitly obtained within some approximations, showing the influence of the order parameter and the vortex length density, which is decisive close to the transition.

PhysicsCouplingApplied MathematicsGeneral MathematicsAttenuation010102 general mathematicsPhase (waves)Lambda transition01 natural sciences010305 fluids & plasmasVortexSuperfluidityQuantum electrodynamics0103 physical sciencesSecond sound0101 mathematicsQuantumSettore MAT/07 - Fisica MatematicaSecond sound Lambda phase transition Superfluid helium Quantum vortices
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Limits on anomalous trilinear gauge couplings fromWW→e+e−,WW→e±μ∓, andWW→μ+μ−events frompp¯collisions ats=1.96  TeV

2006

Limits are set on anomalous WW gamma and WWZ trilinear gauge couplings using W+W--> e(+)nu(e)e(-)(nu) over bar (e), W+W--> e(+/-)nu(e)mu(-/+)nu(mu), and W+W-->mu(+)nu(mu)mu(-)(nu) over bar (mu) events. The data set was collected by the Run II D0 detector at the Fermilab Tevatron Collider and corresponds to approximately 250 pb(-1) of integrated luminosity at root s=1.96 TeV. Under the assumption that the WW gamma couplings are equal to the WWZ couplings and using a form factor scale of Lambda=2.0 TeV, the combined 95% C.L. one-dimensional coupling limits from all three channels are -0.32 <Delta kappa < 0.45 and -0.29 <lambda < 0.30.

PhysicsCouplingNuclear and High Energy PhysicsParticle physicsLuminosity (scattering theory)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronLambda01 natural sciences7. Clean energylaw.inventionNuclear physicsParticle decaylaw0103 physical sciencesHigh Energy Physics::ExperimentFermilab010306 general physicsColliderBar (unit)Physical Review D
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