Search results for " high energy physics"

showing 10 items of 8412 documents

Rare baryon decaysΛb→Λℓ+ℓ−(ℓ=e,μ,τ) andΛb→Λγ: Differential and total rates, lepton- and hadron-side forward-backward asymmetries

2013

Using the covariant constituent quark model previously developed by us, we calculate the differential rate and the forward-backward asymmetries on the lepton and hadron side for the rare baryon decays ${\ensuremath{\Lambda}}_{b}\ensuremath{\rightarrow}\ensuremath{\Lambda}{\ensuremath{\ell}}^{+}{\ensuremath{\ell}}^{\ensuremath{-}}$ ($\ensuremath{\ell}=e$, $\ensuremath{\mu}$, $\ensuremath{\tau}$) and ${\ensuremath{\Lambda}}_{b}\ensuremath{\rightarrow}\ensuremath{\Lambda}\ensuremath{\gamma}$. We use helicity methods to write down a threefold joint angular decay distribution for the cascade decay ${\ensuremath{\Lambda}}_{b}\ensuremath{\rightarrow}\ensuremath{\Lambda}(\ensuremath{\rightarrow}p{\…

BaryonPhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologyHadronQuark modelHyperonConstituent quarkHigh Energy Physics::ExperimentLambdaHelicityLeptonPhysical Review D
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Measurements of baryon pair decays of chi(cJ) mesons

2013

Using 106 $\times 10^{6}$ $\psi^{\prime}$ decays collected with the BESIII detector at the BEPCII, three decays of $\chi_{cJ}$ ($J=0,1,2$) with baryon pairs ($\llb$, $\ssb$, $\SSB$) in the final state have been studied. The branching fractions are measured to be $\cal{B}$$(\chi_{c0,1,2}\rightarrow\Lambda\bar\Lambda) =(33.3 \pm 2.0 \pm 2.6)\times 10^{-5}$, $(12.2 \pm 1.1 \pm 1.1)\times 10^{-5}$, $(20.8 \pm 1.6 \pm 2.3)\times 10^{-5}$; $\cal{B}$$(\chi_{c0,1,2}\rightarrow\Sigma^{0}\bar\Sigma^{0})$ = $(47.8 \pm 3.4 \pm 3.9)\times 10^{-5}$, $(3.8 \pm 1.0 \pm 0.5)\times 10^{-5}$, $(4.0 \pm 1.1 \pm 0.5) \times 10^{-5}$; and $\cal{B}$$(\chi_{c0,1,2}\rightarrow\Sigma^{+}\bar\Sigma^{-})$ = $(45.4 \pm…

BaryonPhysicsNuclear and High Energy PhysicsParticle physicsMesonBranching fractionPhysics - Data Analysis Statistics and ProbabilityAnalytical chemistrySigmaLambdaHigh Energy Physics - ExperimentPhysical Review D
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Λ(1520)andΣ(1385)in the nuclear medium

2006

Recent studies of the {lambda}(1520) resonance within chiral unitary theory with coupled channels find the resonance as a dynamically generated state from the interaction of the decuplet of baryons and the octet of mesons, essentially a quasibound state of {pi}{sigma}{sup *}(1385) in this case, although the coupling of the {lambda}(1520) to the KN and {pi}{sigma} makes this picture only approximate. The {pi}{sigma}{sup *}(1385) decay channel of the {lambda}(1520) is forbidden in free space for the nominal mass of the {sigma}{sup *}(1385), but the coupling of the {pi} to ph components in the nuclear medium opens new decay channels of the {lambda}(1520) in the nucleus and produces a much larg…

BaryonPhysicsNuclear and High Energy PhysicsParticle physicsPionMesonResonanceSigmaAtomic physicsCoupling (probability)LambdaNuclear matterPhysical Review C
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Weak decay ofΛc+for the study ofΛ(1405)andΛ(1670)

2015

We study the ${\mathrm{\ensuremath{\Lambda}}}_{c}$ decay process to ${\ensuremath{\pi}}^{+}$ and the meson-baryon final state for the analysis of $\mathrm{\ensuremath{\Lambda}}$ resonances. Considering the Cabibbo-Kobayashi-Maskawa matrix, color suppression, diquark correlation, and the kinematical condition, we show that the final meson-baryon state should be in a pure $I=0$ combination, when the meson-baryon invariant mass is small. Because the $I=1$ contamination usually makes it difficult to analyze $\mathrm{\ensuremath{\Lambda}}$ resonances directly from experiments, the ${\mathrm{\ensuremath{\Lambda}}}_{c}$ decay is an ideal process to study $\mathrm{\ensuremath{\Lambda}}$ resonances.…

BaryonPhysicsNuclear and High Energy PhysicsParticle physicsUnitarityCabibbo–Kobayashi–Maskawa matrixHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimentInvariant massCharge (physics)Ideal (ring theory)Lambda baryonLambdaPhysical Review C
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Study ofJ/ψ→pp¯andJ/ψ→nn¯

2012

The decays J/psi -> p (p) over bar and J/psi -> n (n) over bar have been investigated with a sample of 225.2 x 10(6) J/psi events collected with the BESIII detector at the BEPCII e(+)e(-) collider. The branching fractions are determined to be B(J/psi -> p (p) over bar) = (2.112 +/- 0.004 +/- 0.031 x 10(-3) and B(J/psi -> n (n) over bar) =(2.07 +/- 0.01 +/- 0.17) x 10(-3). Distributions of the angle theta between the proton or antineutron and the beam direction are well described by the form 1 + alpha cos(2)theta, and we find alpha = 0.595 +/- 0.012 +/- 0.015 for J/psi -> p (p) over bar and alpha = 0.50 +/- 0.04 +/- 0.21 for J/psi -> n (n) over bar. Our branching- fraction results suggest a …

BaryonPhysicsNuclear and High Energy PhysicsQCD sum rulesProtonElectron–positron annihilationPhase angleAnalytical chemistryHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNucleonAntineutronBar (unit)Physical Review D
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Measurement of the production fraction times branching fractionf(b→Λb)·B(Λb→J/ψΛ)

2011

The \Lambda_b(udb) baryon is observed in the decay \Lambda_b --> J/\psi \Lambda using 6.1 fb^{-1} of p\bar{p} collisions collected with the D0 detector at \sqrt{s}=1.96 TeV. The production fraction multiplied by the branching fraction for this decay relative to that for the decay B^0 --> J/\psi K^0_s is measured to be 0.345 \pm 0.034 (stat.) \pm 0.033 (syst.) \pm 0.003 (PDG). Using the world average value of f(b --> B^0)B(B^0 --> J/\psi K^0_s) = (1.74 \pm 0.08) \times 10^{-5}, we obtain f(b --> \Lambda_b)B(\Lambda_{b} --> J/\psi \Lambda) = (6.01 \pm 0.60 (stat.) \pm 0.58 (syst.) \pm 0.28 (PDG)) \times 10^{-5}. This measurement represents an improvement in precision by about a factor of thre…

BaryonPhysicsNuclear and High Energy PhysicsTheoretical physics010308 nuclear & particles physicsBranching fraction0103 physical sciencesAnalytical chemistryProduction (computer science)010306 general physicsLambda01 natural sciencesPhysical Review D
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Infinite momentum frame calculation of semileptonic heavyΛb→Λctransitions including HQET improvements

1997

We calculate the transition form factors that occur in heavy {Lambda}-type baryon semileptonic decays such as, e.g., in {Lambda}{sub b}{r_arrow}{Lambda}{sub c}{sup +}+l{sup {minus}}+{bar {nu}}{sub l}. We use Bauer-Stech-Wirbel-type infinite momentum frame wave functions for the heavy {Lambda}-type baryons which we assume to consist of a heavy quark and a light spin-isospin zero diquark system. The form factors at q{sup 2}=0 are calculated from the overlap integrals of the initial and final {Lambda}-type baryon states. To leading order in the heavy mass scale the structure of the form factors agrees with the HQET predictions including the normalization at zero recoil. The leading order {omeg…

BaryonPhysicsOrientation (vector space)Semileptonic decayNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologyQuark modelForm factor (quantum field theory)Order (ring theory)Lambda baryonLambdaPhysical Review D
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Λb and Λc baryon decays at finite values of heavy quark masses

2000

Semileptonic decays of Lambda_b and Lambda_c baryons are studied within the Relativistic Three-Quark Model using finite heavy quark mass values. Employing the same parameters as have been used previously for the description of exclusive decays of heavy baryons in the heavy quark limit we calculate the six form factors of the process and the corresponding decay rates. Our calculation shows that the ``finite mass'' corrections are important in heavy-to-light transitions and are not negligible in heavy-to-heavy transitions.

BaryonPhysicsQuarkNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimentLimit (mathematics)Nuclear ExperimentLambdaPhysics Letters B
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Including theΔ(1232)resonance in baryon chiral perturbation theory

2005

Baryon chiral perturbation theory with explicit $\ensuremath{\Delta}(1232)$ degrees of freedom is considered. The most general interactions of pions, nucleons, and \ensuremath{\Delta} consistent with all underlying symmetries as well as with the constraint structure of higher-spin fields are constructed. By use of the extended on-mass-shell renormalization scheme, a manifestly Lorentz-invariant effective-field theory with a systematic power counting is obtained. As applications, we discuss the mass of the nucleon, the pion-nucleon \ensuremath{\sigma} term, and the pole of the \ensuremath{\Delta} propagator.

BaryonPhysicsRenormalizationNuclear and High Energy PhysicsParticle physicsChiral perturbation theoryPionNuclear TheoryPropagatorPerturbation theoryQuantum field theoryNuclear ExperimentNucleonPhysical Review C
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Cosmic Dark Radiation and Neutrinos

2013

New measurements of the cosmic microwave background (CMB) by the Planck mission have greatly increased our knowledge about the universe. Dark radiation, a weakly interacting component of radiation, is one of the important ingredients in our cosmological model which is testable by Planck and other observational probes. At the moment, the possible existence of dark radiation is an unsolved question. For instance, the discrepancy between the value of the Hubble constant, H-0, inferred from the Planck data and local measurements of H-0 can to some extent be alleviated by enlarging the minimal ACDM model to include additional relativistic degrees of freedom. From a fundamental physics point of v…

Big BangNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Article SubjectAge of the universeDark matterFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesBayron acoustic-Oscillationssymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Analytic approach0103 physical sciencesPlanck010306 general physicsPhysicsAstrophysics - Cosmology and Extragalactic Astrophysics010308 nuclear & particles physicsHot dark matterFísicalcsh:QC1-999High Energy Physics - Phenomenology13. Climate actionDark radiationDark energysymbolslcsh:PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsAdvances in High Energy Physics
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