Search results for "Branch"

showing 10 items of 1278 documents

Search for Charged Higgs Bosons in Decays of Top Quarks inpp¯Collisions ats=1.96  TeV

2009

We report on the first direct search for charged Higgs bosons in decays of top quarks in p{bar p} collisions at {radical}s = 1.96 TeV. The search uses a data sample corresponding to an integrated luminosity of 2.2 fb{sup -1} collected by the CDF II detector at Fermilab, and looks for a resonance in the invariant mass distribution of two jets in the lepton+jets sample of t{bar t} candidates. We observe no evidence of charged Higgs bosons in top quark decays. Hence, 95% upper limits on the top quark decay branching ratio are placed at {Beta}(t {yields} H{sup +}b) < 0.1 to 0.3 for charged Higgs boson masses of 60 to 150 GeV/c{sup 2}, assuming {Beta}(H{sup +} {yields} c{bar s}) = 1.0. The upper…

QuarkPhysicsTop quarkParticle physics010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyElementary particle01 natural sciences7. Clean energyStandard ModelNuclear physics0103 physical sciencesHiggs bosonHigh Energy Physics::Experiment010306 general physicsLeptonBosonPhysical Review Letters
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Precision Measurement of the RatioB(t→Wb)/B(t→Wq)and Extraction ofVtb

2011

We present a measurement of the ratio of top quark branching fractions R = B(t -> Wb)/B(t -> Wq), where q can be a d, s or b quark, in the lepton+jets and dilepton ttbar final states. The measurement uses data from 5.4 fb-1 of ppbar collisions collected with the D0 detector at the Fermilab Tevatron Collider. We measure R = 0.90 +/- 0.04, and we extract the CKM matrix element |Vtb| as |Vtb| = 0.95 +/- 0.02, assuming unitarity of the 3x3 CKM matrix.

QuarkPhysicsTop quarkParticle physicsUnitarity010308 nuclear & particles physicsCabibbo–Kobayashi–Maskawa matrixBranching fractionHigh Energy Physics::PhenomenologyTevatronGeneral Physics and Astronomy7. Clean energy01 natural sciencesBottom quarkNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentFermilab010306 general physicsPhysical Review Letters
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Evidence forB0→ρ0ρ0Decays and Implications for the Cabibbo-Kobayashi-Maskawa Angleα

2007

We search for the decays B(0) --> rho(0)rho(0), B(0) --> rho(0)f(0)(980), and B(0) --> f(0)(980)f(0)(980) in a sample of about 384 x 10(6) Upsilon(4S) --> BB[over] decays collected with the BABAR detector at the PEP-II asymmetric-energy e(+)e(-) collider at Stanford Linear Accelerator Center. We find evidence for B(0) --> rho(0)rho(0) with 3.5 sigma significance and measure the branching fraction B = (1.07 +/- 0.33 +/- 0.19) x 10(-6) and longitudinal polarization fraction f(L) = 0.87 +/- 0.13 +/- 0.04, where the first uncertainty is statistical, and the second is systematic. The uncertainty on the Cabibbo-Kobayashi-Maskawa quark-mixing matrix unitarity angle alpha due to penguin contributio…

QuarkPhysicsUnitarity010308 nuclear & particles physicsBranching fractionCabibbo–Kobayashi–Maskawa matrixElectron–positron annihilationCenter (category theory)General Physics and Astronomy01 natural sciencesNuclear physicsParticle decayPair production0103 physical sciences010306 general physicsPhysical Review Letters
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Hindered M1 radiative decay ofϒ(2S)from lattice NRQCD

2015

We present a calculation of the hindered M1 $\mathrm{\ensuremath{\Upsilon}}(2S)\ensuremath{\rightarrow}{\ensuremath{\eta}}_{b}(1S)\ensuremath{\gamma}$ decay rate using lattice nonrelativistic quantum chromodynamics. The calculation includes spin-dependent relativistic corrections to the NRQCD action through $\mathcal{O}({v}^{6})$ in the quark's relative velocity, relativistic corrections to the leading order current which mediates the transition through the quark's magnetic moment, radiative corrections to the leading spin-magnetic coupling and for the first time a full error budget. We also use gluon field ensembles at multiple lattice spacing values, all of which include $u$, $d$, $s$ and…

QuarkQuantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsLattice constantBranching fractionHigh Energy Physics::LatticeLattice (order)Relative velocityHigh Energy Physics::ExperimentVacuum polarizationBottom quarkPhysical Review D
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Determination of the width of the top quark

2011

We extract the total width of the top quark, Gamma_t, from the partial decay width Gamma(t -&gt; W b) measured using the t-channel cross section for single top quark production and from the branching fraction B(t -&gt; W b) measured in ttbar events using up to 2.3 fb^-1 of integrated luminosity collected by the D0 Collaboration at the Tevatron ppbar Collider. The result is Gamma_t = 1.99 +0.69 -0.55 GeV, which translates to a top-quark lifetime of tau_t = (3.3 +1.3 -0.9) x 10^-25 s. Assuming a high mass fourth generation b' quark and unitarity of the four-generation quark-mixing matrix, we set the first upper limit on |Vtb'| &lt; 0.63 at 95% C.L.

QuarkTop quarkParticle physicsTevatronGeneral Physics and AstronomyFOS: Physical sciencesElementary particle01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsPhysicsLuminosity (scattering theory)Unitarity010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHigh Energy Physics::Experiment14.65.Ha 14.65.Jk 12.15.HhBar (unit)
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Single and Double Beta-DecayQValues among the TripletZr96,Nb96, andMo96

2016

The atomic mass relations among the mass triplet ^{96}Zr, ^{96}Nb, and ^{96}Mo have been determined by means of high-precision mass measurements using the JYFLTRAP mass spectrometer at the IGISOL facility of the University of Jyvaskyla. We report Q values for the ^{96}Zr single and double β decays to ^{96}Nb and ^{96}Mo, as well as the Q value for the ^{96}Nb single β decay to ^{96}Mo, which are Q_{β}(^{96}Zr)=163.96(13), Q_{ββ}(^{96}Zr)=3356.097(86), and Q_{β}(^{96}Nb)=3192.05(16)  keV. Of special importance is the ^{96}Zr single β-decay Q value, which has never been determined directly. The single β decay, whose main branch is fourfold unique forbidden, is an alternative decay path to the…

QuenchingCoupling constantPhysics010308 nuclear & particles physicsQ valueGeneral Physics and AstronomyMass spectrometry7. Clean energy01 natural sciencesAtomic massMain branchDouble beta decay0103 physical sciencesUniquenessAtomic physics010306 general physicsPhysical Review Letters
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Including Covariates in the ETAS Model Triggered Seismicity

2020

The paper proposes a stochastic process that improves the assessment of seismic events in space and time, considering a contagion model (branching process) within a regression-like framework to take covariates into account. The proposed approach develops the Forward Likelihood for prediction (FLP) method for estimating the ETAS model, including covariates in the model specification of the epidemic component. A simulation study is carried out for analysing the misspecification model effect under several scenarios. Also an application to the Italian catalogue is reported, together with the reference to the developed R package.

R packageSpecificationSpacetimeComputer scienceStochastic processComponent (UML)CovariateEconometricsStatistics::MethodologyInduced seismicityBranching processSSRN Electronic Journal
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Understanding Prediction Limits Through Unbiased Branches

2006

The majority of currently available branch predictors base their prediction accuracy on the previous k branch outcomes. Such predictors sustain high prediction accuracy but they do not consider the impact of unbiased branches which are difficult-to-predict. In this paper, we quantify and evaluate the impact of unbiased branches and show that any gain in prediction accuracy is proportional to the frequency of unbiased branches. By using the SPECcpu2000 integer benchmarks we show that there are a significant proportion of unbiased branches which severely impact on prediction accuracy (averaging between 6% and 24% depending on the prediction context used).

Ramification (botany)StatisticsEconometricsContext (language use)Unbiased EstimationBest linear unbiased predictionBranch predictorMathematicsInteger (computer science)
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Untersuchungen von polymeren im massenspektrometer, 4. Abbaureaktionen von polybenzylen

1974

Die Abbaureaktionen von unsubstituierten Poly(1,4-phenylenmethylen)en (A) (Polybenzylen), Poly[(2,5-dimethyl-1,4-phenylen)methylen] [Poly(2,5-dimethylbenzyl)] (B), Poly[(2,3,5,6-tetramethyl-1,4-phenylen)methylen] [Poly(2,3,5,6-tetramethylbenzyl)] (C) und Poly(1,4-phenylenathyliden) [Poly(α-methylbenzyl)] (D) wurden durch direkte Pyrolyse im Massenspektrometer untersucht. Die Massenpyrogramme von unter verschiedenen Reaktionsbedingungen dargestellten Polybenzylen wurden verglichen, mit dem Ziel, direkt Informationen uber Strukturunterschiede wie Kettenverzweigung und unterschiedliche Verknupfung der Benzyleinheiten zu erhalten; hierbei konnten in einem Falle auf hohere Kettenverzweigung deut…

Reaction conditionschemistry.chemical_classificationSteric effectschemistry.chemical_compoundMonomerchemistryPolymer chemistryDisproportionationMethyleneBranching (polymer chemistry)AlkylThermostabilityDie Makromolekulare Chemie
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High-resolution spectroscopy of two metal-poor red giants: HD 232078 and HD 218732

2010

An abundance analysis for 35 chemical elements based on a high-resolution (R = 67 000) optical spectra of two metal-poor ([Fe/H] ≈ - 1.50) halo red giants, HD 232078 and HD 218732, is presented. Abundances of 10 chemical elements were derived for the first time. Both red giants are chromospherically active and optically variable, located close to the red giant branch tip. Abundances of both stars generally follow typical halo star abundance distribution, while HD 218732 should have experienced a deep mixing episode and could be a first ascent asymptotic giant branch star.

Red-giant branchPhysicsStarsSpace and Planetary ScienceGalaxy formation and evolutionAsymptotic giant branchAstronomyAstronomy and AstrophysicsAstrophysicsHaloA-type main-sequence starSpectroscopyO-type main-sequence starMonthly Notices of the Royal Astronomical Society
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