Search results for "Weinberg"

showing 10 items of 53 documents

Le vignoble gallo-romain de Gevrey-Chambertin "Au-dessus de Bergis", Côte d'Or (Ier-IIe s. ap. J.-C.) : Modes de plantation et de conduite de vignes …

2011

Recent excavations at " Au-dessus de Bergis " in Gevrey-Chambertin (Burgundy, France) brought to light in 2008 and 2009 numerous, rectangular aligned pits interpreted as an ancient vineyard dated from the mid-first, mid-second century to the third century AD. The vineyard measured at least one hectare in area and was bounded to the south by a hedge or fence. It was composed of parallel rows oriented 6° N that may have been trained over and along high, inclined wooden frames. Vine stocks were renewed by layering, over several generations of plants. This vineyard attests to the spreading of vineyards from the mid-first century AD, as was initially supposed, and it documents some agricultural …

vignobleAbsenken[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and PrehistoryterroirsprovignagepalissageplantationvineyardAntiquitéRebenBurgundBourgogneVigneAntiquityWeinberg[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and PrehistorytrainingAntikeVineantiquityPflanzung[ SHS.ARCHEO ] Humanities and Social Sciences/Archaeology and PrehistoryvinevigneBurgundyprovining
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Measurement of the Effective Weak Mixing Angle inpp¯→Z/γ*→e+e−Events

2015

We present a measurement of the fundamental parameter of the standard model, the weak mixing angle, in $p\bar{p}\rightarrow Z/\gamma^{*}\rightarrow e^{+}e^{-}$ events at a center of mass energy of 1.96 TeV, using data corresponding to 9.7 fb$^{-1}$ of integrated luminosity collected by the D0 detector at the Fermilab Tevatron. The effective weak mixing angle is extracted from the forward-backward charge asymmetry as a function of the invariant mass around the Z boson pole. The measured value of $\sin^2\theta_{\text{eff}}^{\text{$\ell$}}=0.23146 \pm 0.00047$ is the most precise measurement from light quark interactions to date, with a precision close to the best LEP and SLD results.

PhysicsQuarkParticle physicsHigh Energy Physics::PhenomenologyTevatronGeneral Physics and AstronomyCharge (physics)Weinberg angle7. Clean energyStandard ModelNuclear physicsHigh Energy Physics::ExperimentInvariant massCenter of massEnergy (signal processing)Physical Review Letters
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Improved measurements of electroweak parameters from Z decays into fermion pairs

1992

The properties of the Z resonance are measured on the basis of 190000 Z decays into fermion pairs collected with the ALEPH detector at LEP. Assuming lepton universality, M(Z) = (91.182 +/- 0.009exp +/- 0.020L;P) GeV, GAMMA(Z) = (2484 +/- 17) MeV, sigma(had)0 = (41.44 +/- 0.36) nb, and GAMMA(had)/GAMMA(ll) = 21.00 +/- 0.20. The corresponding number of light neutrino species is 2.97 +/- 0.07. The forward-backward asymmetry in leptonic decays is used to determine the ratio of vector to axial-vector coupling constants of leptons: g(V)2(M(Z)2)/g(A)2(M(Z)2) = 0.0072 +/- 0.0027. Combining these results with ALEPH results on quark charge and bbBAR asymmetries, and tau-polarization, sin2 theta(W)(M(…

QuarkPhysicsParticle physicsPhysics and Astronomy (miscellaneous)Electron–positron annihilationHigh Energy Physics::PhenomenologyElectroweak interactionElementary particleWeinberg angleFermionALEPH detectorNuclear physicsHigh Energy Physics::ExperimentNeutrinoEngineering (miscellaneous)Particle Physics - ExperimentLepton
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Fun with the Abelian Higgs model

2013

In calculations of the elementary scalar spectra of spontaneously broken gauge theories there are a number of subtleties which, though it is often unnecessary to deal with them in the order-of-magnitude type of calculations, have to be taken into account if fully consistent results are sought for. Within the "canonical" effective-potential approach these are, for instance: the need to handle infinite series of nested commutators of derivatives of field-dependent mass matrices, the need to cope with spurious IR divergences emerging in the consistent leading-order approximation and, in particular, the need to account for the fine interplay between the renormalization effects in the one-and tw…

PhysicsParticle physicsPhysics and Astronomy (miscellaneous)Bose-Einstein Condensation010308 nuclear & particles physicsScalar (mathematics)Spontaneous Symmetry-BreakingWeinberg ModelFOS: Physical sciencesHierarchy problem01 natural sciencesRenormalizationHigh Energy Physics - PhenomenologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHiggs bosonGauge theoryAbelian group010306 general physicsSpurious relationshipEngineering (miscellaneous)The European Physical Journal C
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Improved tau polarisation measurement

1996

Using 22 pb−1 of data collected at LEP in 1992 on the peak of the Z resonance, the ALEPH collaboration has measured the polarisation of the tau leptons decaying into $$ev\bar v, \mu v\bar v$$ ,πν, ρν and a1 ν from their individual decay product distributions. The measurement of the tau polarisation as a function of the production polar angle yields the two parametersN τ andN e, where, in terms of the axial and vector couplingsg Al andg Vl,N l=2g Vl gAl/(g Vl 2 +g 2 ). This analysis follows to a large extent the methods devised for the 1990 and 1991 data but with improvements which bring a better understanding of the systematic uncertainties. Combining the 1992 measurements with our previous…

Systematic errorPhysicsParticle physicsTime projection chamberPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsElectron–positron annihilationPhysicsWeinberg angle7. Clean energy01 natural sciencesParticle identificationNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Polar coordinate systemDecay product010306 general physicsParticle Physics - ExperimentLepton
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Group-Theoretic analysis of the mixing angle in the electroweak gauge group

1996

In this paper the authors provide strong mathematical support for the idea that the experimentally measured magnitude 1 - M{sub W}{sup 2}/M{sub Z}{sup 2} associated with sin{sup 2}{theta}{sub w} in the standard model of electroweak interactions cannot be simultaneously identified with the squared quotient of the electric charge by the SU(2) charge, e{sup 2}/g{sup 2}. In fact, the natural, mathematical requirement that the Weinberg rotation between the gauge fields associated with the third component of the {open_quotes}weak isospin{close_quotes} (T{sub 3}) and the hypercharge (Y) proceeds from a global Lie-group homomorphism of the SU(2) {circle_times} U(1){sub y} gauge group in some locall…

PhysicsHyperchargeParticle physicsPhysics and Astronomy (miscellaneous)Gauge groupGeneral MathematicsLie algebraElectroweak interactionLie groupGrand Unified TheoryCharge (physics)Weinberg angleMathematical physicsInternational Journal of Theoretical Physics
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Measurement of the forward-backward asymmetry of e(+)e(-)-]z-]b(b)over-bar using prompt leptons and a lifetime tag

1995

The forward-backward asymmetry of the process e+e-→Z→b {Mathematical expression} has been measured using events collected by the DELPHI experiment during the 1991 and 1992 LEP runs. This data sample corresponded to 884 000 hadronic Z decays at a centre-of-mass energy {Mathematical expression}. The tagging of b-quark events was performed using two approaches; the first was based on the semileptonic decay channels b→X+μ and b→X+e, the second used a lifetime tag with jet-charge reconstruction. The results of these two methods were combined to give {Mathematical expression} With the semileptonic sample, the forward-backward asymmetry of the process e+e-→Z→ {Mathematical expression} was also mea…

Semileptonic decayParticle physicsFERMION PAIR PRODUCTIONPhysics and Astronomy (miscellaneous)LUND MONTE-CARLOENERGIESElectron–positron annihilationQED CORRECTIONSD-MESONSEMILEPTONIC DECAY01 natural sciencesJET FRAGMENTATIONb-taggingPartícules (Física nuclear)PHYSICSNuclear physics0103 physical sciencesDELPHI; forward-backward asymmetry; b-tagging; jet reconstructionFERMION PAIR PRODUCTION; LUND MONTE-CARLO; E+E-ANNIHILATION; SEMILEPTONIC DECAY; JET FRAGMENTATION; QED CORRECTIONS; FINAL-STATES; D-MESON; ENERGIES; PHYSICS010306 general physicsEngineering (miscellaneous)jet reconstructionDetectors de radiacióDELPHIPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyWeinberg angleE+E-ANNIHILATIONLARGE ELECTRON POSITRON COLLIDERFINAL-STATESb-taggingPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHILarge Electron–Positron ColliderPARTICLE PHYSICSHigh Energy Physics::Experimentforward-backward asymmetryEnergy (signal processing)Particle Physics - ExperimentLeptonBar (unit)
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Weakly interacting dark matter from the minimal walking technicolor

2009

We study a superweakly interacting dark matter particle motivated by minimal walking technicolor theories. Our WIMP is a mixture of a sterile state and a state with the charges of a standard model fourth family neutrino. We show that the model can give the right amount of dark matter over a range of the WIMP mass and mixing angle. We compute bounds on the model parameters from the current accelerator data including the oblique corrections to the precision electroweak parameters, as well as from cryogenic experiments, Super-Kamiokande and from the IceCube experiment. We show that consistent dark matter solutions exist which satisfy all current constraints. However, almost the entire paramete…

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterElectroweak interactionFOS: Physical sciencesAstronomy and AstrophysicsTechnicolorWeinberg angleCosmologyStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)WIMPHigh Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Testing for goodness rather than lack of fit of an X–chromosomal SNP to the Hardy-Weinberg model

2019

The problem of checking the genotype distribution obtained for some diallelic marker for compatibility with the Hardy-Weinberg equilibrium (HWE) condition arises also for loci on the X chromosome. The possible genotypes depend on the sex of the individual in this case: for females, the genotype distribution is trinomial, as in the case of an autosomal locus, whereas a binomial proportion is observed for males. Like in genetic association studies with autosomal SNPs, interest is typically in establishing approximate compatibility of the observed genotype frequencies with HWE. This requires to replace traditional methods tailored for detecting lack of fit to the model with an equivalence test…

HeredityNormal DistributionDistance MeasurementTrinomial01 natural sciencesLinkage Disequilibrium010104 statistics & probabilityStatisticsLack-of-fit sum of squaresMathematicsVenous ThrombosisMeasurement0303 health sciencesMultidisciplinaryQRSoftware EngineeringGenomicsHardy–Weinberg principleGenetic MappingPhysical SciencesEngineering and TechnologyMedicineResearch ArticleComputer and Information SciencesScienceGeometryAsymptotic distributionVariant GenotypesPolymorphism Single NucleotideMolecular Genetics03 medical and health sciencesGenome-Wide Association StudiesGeneticsTest statisticHumansComputer Simulation0101 mathematicsMolecular BiologyGenetic Association Studies030304 developmental biologyChromosomes Human XModels StatisticalModels GeneticSoftware ToolsBiology and Life SciencesComputational BiologyHuman GeneticsGenome AnalysisProbability TheoryProbability DistributionGenotype frequencyRadiiSample size determinationSample SizeBinomial proportion confidence intervalMathematicsPLOS ONE
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Decoherence in supernova neutrino transformations suppressed by deleptonization

2007

16 pages, 12 figures.-- PACS nrs.: 14.60.Pq; 97.60.Bw.-- ISI Article Identifier: 000251987300100.-- ArXiv pre-print available at: http://arxiv.org/abs/0706.2498

HistoryParticle physicsNuclear and High Energy PhysicsQuantum decoherence[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PACS] Supernovae[PACS] Neutrino mass and mixingAstrophysicsAsymmetryMeasure (mathematics)01 natural sciences7. Clean energyEarly UniverseStandard ModelEducationLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesInvariant massddc:530High Energy Physics010306 general physicsMixing (physics)media_commonPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaWeinberg angleFunction (mathematics)Atomic and Molecular Physics and OpticsComputer Science Applications3. Good healthSupernovaHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]PhenomenologyHigh Energy Physics::ExperimentNeutrino
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