Search results for "Branch"

showing 10 items of 1278 documents

On the Spectral Evolution of Cygnus X-2 along its Color-Color Diagram

2002

We report on the results of a broad band (0.1-200 keV) spectral study of Cyg X-2 using two BeppoSAX observations taken in 1996 and 1997, respectively, for a total effective on-source time of ~100 ks. The color-color (CD) and hardness-intensity (HID) diagrams show that the source was in the horizontal branch (HB) and normal branch (NB) during the 1996 and 1997 observation, respectively. Five spectra were selected around different positions of the source in the CD/HID, two in the HB and three in the NB. These spectra are fit to a model consisting of a disk blackbody, a Comptonization component, and two Gaussian emission lines at ~1 keV and ~6.6 keV, respectively. The addition of a hard power-…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsColor–color diagramAstrophysicsRadiusHorizontal branchaccretion accretion disks / stars: individual: Cyg X–2 / stars: neutron / X-rays: stars / X-rays: binaries / X-rays: generalAstrophysicsSpectral lineLuminosityNOaccretionSpace and Planetary ScienceOptical depth (astrophysics)accretion disks / stars: individual: Cyg X–2 / stars: neutron / X-rays: stars / X-rays: binaries / X-rays: generalElectron temperatureEmission spectrum
researchProduct

On metal-deficient barium stars and their link with yellow symbiotic stars

2005

This paper addresses the question of why metal-deficient barium stars are not yellow symbiotic stars (YSyS). Samples of (suspected) metal-deficient barium (mdBa) stars and YSyS have been collected from the literature, and their properties reviewed. It appears in particular that the barium nature of the suspected mdBa stars needs to be ascertained by detailed abundance analyses. Abundances are therefore derived for two of them, HD 139409 and HD 148897, which reveal that HD 148897 should not be considered a barium star. HD 139409 is a mild barium star, with overabundances observed only for elements belonging to the first s-process peak (Y and Zr). The evidence for binarity among mdBa stars is…

PhysicsBarium starAstrophysics (astro-ph)FOS: Physical scienceschemistry.chemical_elementAstronomy and AstrophysicsBariumAstrophysicsOrbital periodGiant starAstrophysicsStarsOrbitchemistrySpace and Planetary ScienceAsymptotic giant branchLoss rate
researchProduct

Study of the decayB¯0→Λc+p¯π+π−and its intermediate states

2013

We study the decay B^0→Λ_c^+p π^+π^-, reconstructing the Λ_c^+ baryon in the pK^-π^+ mode, using a data sample of 467×10^6 BB pairs collected with the BABAR detector at the PEP-II storage rings at SLAC. We measure branching fractions for decays with intermediate Σ_c baryons to be B[B^0→Σ_c(2455)^(++)pπ^-]=(21.3±1.0±1.0±5.5)×10^(-5), B[B^0→Σ_c(2520)^(++)pπ^-]=(11.5±1.0±0.5±3.0)×10^(-5), B[B^0→Σ_c(2455)^0pπ^+]=(9.1±0.7±0.4±2.4)×10^(-5), and B[B^0→Σ_c(2520)^0pπ^+]=(2.2±0.7±0.1±0.6)×10^(-5), where the uncertainties are statistical, systematic, and due to the uncertainty on the Λ_c^+→pK^-π^+ branching fraction, respectively. For decays without Σ_c(2455) or Σ_c(2520) resonances, we measure B[B^0→…

PhysicsBaryonCharmed baryonsNuclear and High Energy PhysicsCrystallography010308 nuclear & particles physicsBranching fractionElectron–positron annihilation0103 physical sciencesAtomic physics010306 general physics01 natural sciencesPhysical Review D
researchProduct

Study of the baryonicBdecayB−→Σc++p¯π−π−

2012

We report the measurement of the baryonic B decay B- -> SigmaC++ p- pi- pi-. Using a data sample of 467*10^6 B B-bar pairs collected with the BaBar detector at the PEP-II storage ring at SLAC, the measured branching fraction is (2.98 +/- 0.16 (stat) +/- 0.15 (syst) +/- 0.77 (LambdaC+))*10^{-4}, where the last error is due to the uncertainty in the branching fraction of the decay LambdaC+ -> p+ K- pi+. The data suggest the existence of resonant subchannels B- -> LambdaC(2595)+ p- pi- and, possibly, B- -> SigmaC++ anti-Delta-- pi-. We see unexplained structures in m(SigmaC++ pi- pi-) at 3.25 GeV/c^2, 3.8 GeV/c^2, and 4.2 GeV/c^2.

PhysicsBaryonCharmed baryonsNuclear physicsNuclear and High Energy Physics010308 nuclear & particles physicsBranching fractionElectron–positron annihilation0103 physical sciencesPi010306 general physics01 natural sciencesStorage ringPhysical Review D
researchProduct

First observation of the isospin violating decayJ/ψ→ΛΣ¯0+c.c.

2012

Using a sample of (225.2 +/- 2.8) x 10(6) J/psi events collected with the BESIII detector, we present results of a study of J/psi -> gamma Lambda(Lambda) over bar and report the first observation of the isospin violating decay J/psi -> Lambda(Sigma) over bar (0) + c.c., in which (Sigma) over bar (0) decays to gamma (Lambda) over bar. The measured branching fractions are B(J/psi -> (Lambda) over bar Sigma(0)) = (1.46 +/- 0.11 +/- 0.12) x 10(-5) and B(J/psi -> Lambda(Sigma) over bar (0)) = (1.37 +/- 0.12 +/- 0.11) x 10(-5). We search for Lambda(1520) -> gamma Lambda decay, and find no evident signal, and an upper limit for the product branching fraction B(J/psi -> Lambda(Lambda) over bar (152…

PhysicsBaryonNuclear and High Energy PhysicsBranching fractionIsospinElectron–positron annihilationQuark modelHyperonAnalytical chemistrySigmaHigh Energy Physics::ExperimentLambdaPhysical Review D
researchProduct

Precision Measurement of the Branching Fractions of η′ Decays

2019

PubMed ID: 31050481

PhysicsBranching fractionElectron–positron annihilationComputerSystemsOrganization_COMPUTER-COMMUNICATIONNETWORKSGeneral Physics and AstronomyBranching (polymer chemistry)01 natural sciencesHigh Energy Physics - Experiment; High Energy Physics - ExperimentNOHigh Energy Physics - ExperimentCrystallographyComputingMilieux_MANAGEMENTOFCOMPUTINGANDINFORMATIONSYSTEMSComputingMethodologies_PATTERNRECOGNITION0103 physical sciencesddc:530InformationSystems_MISCELLANEOUS010306 general physicsPhysical Review Letters
researchProduct

First Observation of theM1Transitionψ(3686)→γηc(2S)

2012

Using a sample of 106×10(6) ψ(3686) events collected with the BESIII detector at the BEPCII storage ring, we have made the first measurement of the M1 transition between the radially excited charmonium S-wave spin-triplet and the radially excited S-wave spin-singlet states: ψ(3686)→γη(c)(2S). Analyses of the processes ψ(3686)→γη(c)(2S) with η(c)(2S)→K(S)(0)K(±)π(∓) and K(+)K(-)π(0) give an η(c)(2S) signal with a statistical significance of greater than 10 standard deviations under a wide range of assumptions about the signal and background properties. The data are used to obtain measurements of the η(c)(2S) mass (M(η(c)(2S))=3637.6±2.9(stat)±1.6(syst) MeV/c(2)), width (Γ(η(c)(2S))=16.9±6.4(…

PhysicsBranching fractionElectron–positron annihilationExcited stateAnalytical chemistryGeneral Physics and AstronomyPhysical Review Letters
researchProduct

Two-Phonon Octupole Excitation in 146Gd

2006

The excited states in 146Gd have been re‐investigated with the 144Sm(α,2n) reaction using a modern Ge γ‐ray array including a polarimeter. Amongst the non‐yrast states populated in this reaction we have identified the aligned 6+ member of the two‐phonon octupole quartet from the observation of the E3 branching to the one phonon 3− state. Our results represent the first observation of a 6+→3−→0+ E3 cascade in an even‐even nucleus.

PhysicsBranching fractionPhononExcited stateYrastNuclear shell modelNeutronGamma spectroscopyAtomic physicsExcitationAIP Conference Proceedings
researchProduct

First Observation ofD0−D¯0Oscillations inD0→K+π−π+π−Decays and Measurement of the Associated Coherence Parameters

2016

Charm meson oscillations are observed in a time-dependent analysis of the ratio of D0→K+π−π+π− to D0→K−π+π−π+ decay rates, using data corresponding to an integrated luminosity of 3.0fb−1 recorded by the LHCb experiment. The measurements presented are sensitive to the phase-space averaged ratio of doubly Cabibbo-suppressed to Cabibbo-favoured amplitudes rK3πD and the product of the coherence factor RK3πD and a charm mixing parameter y′K3π. The constraints measured are rK3πD=(5.67±0.12)×10−2, which is the most precise determination to date, and RK3πD⋅y′K3π=(0.3±1.8)×10−3, which provides useful input for determinations of the CP-violating phase γ in B±→DK±,D→K∓π±π∓π± decays. The analysis also …

PhysicsCoherence factorMeson010308 nuclear & particles physicsBranching fractionGeneral Physics and Astronomy01 natural sciencesStandard deviationNuclear physicsAmplitudePhase space0103 physical sciencesCP violationCoherence (signal processing)010306 general physicsPhysical Review Letters
researchProduct

Electron Capture Processes in Intermediate Mass stars

2015

Intermediate mass stars develop a degenerate core constituted of O, Ne and Mg during their evolution. As the density in the core increases electron capture sets in igniting Ne and O burning. Particularly important is electron capture on 20Ne that has been found recently to be dominated by a second forbidden transition from the 0+ ground state of 20Ne to the 2+ ground state of 20F. We have performed shell–model calculations to determine the transition strength and provide an updated value of the electron capture rate and the expected branching ratio to the corresponding β–decay process. peerReviewed

PhysicsCore (optical fiber)StarsTransition strengthBranching fractionElectron captureelectron capture processesDegenerate energy levelsAtomic physicsGround state
researchProduct