Search results for "Background"

showing 10 items of 556 documents

Combination of Tevatron searches for the standard model Higgs boson in the W+W- decay mode.

2010

11 páginas, 4 figuras, 1 tabla.-- CDF Collaboration: et al.

Particle physicsAstrophysics::High Energy Astrophysical PhenomenaTevatronFOS: Physical sciencesGeneral Physics and AstronomyElementary particleddc:500.2.PARTON DISTRIBUTIONS; HADRON COLLIDERS; QCD; NNLO7. Clean energy01 natural sciences114 Physical sciencesHigh Energy Physics - ExperimentStandard ModelNuclear physicsHigh Energy Physics - Experiment (hep-ex)Particle decay0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Grand Unified TheoryHADRON COLLIDERSFermilabTEVATRONNuclear Experiment010306 general physicsBosonPhysicsHIGGS BOSON010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyQCD3. Good healthPARTON DISTRIBUTIONSHiggs bosonCDFPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNNLOAnti-p p: interaction | Higgs particle: search for | gluon gluon: fusion | intermediate boson: fusion | quark antiquark: annihilation | Higgs particle: decay | Higgs particle --> W+ W- | W: pair production | W: leptonic decay | dilepton: final state | jet: multiplicity | cross section: upper limit | mass dependence | Higgs particle: mass | background | DZERO | CDF | Batavia TEVATRON Coll | anti-p p --> Higgs particle anything | anti-p p --> Higgs particle anything intermediate boson anything | anti-p p --> Higgs particle anything quark antiquark anything | 1960 GeV-cmsPhysical review letters
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Do we have any hope of detecting scattering between dark energy and baryons through cosmology?

2020

We consider the possibility that dark energy and baryons might scatter off each other. The type of interaction we consider leads to a pure momentum exchange, and does not affect the background evolution of the expansion history. We parametrize this interaction in an effective way at the level of Boltzmann equations. We compute the effect of dark energy-baryon scattering on cosmological observables, focusing on the Cosmic Microwave Background (CMB) temperature anisotropy power spectrum and the matter power spectrum. Surprisingly, we find that even huge dark energy-baryon cross-sections $\sigma_{xb} \sim {\cal O}({\rm b})$, which are generically excluded by non-cosmological probes such as col…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundCosmic background radiationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)cosmic background radiationAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesCosmologyGeneral Relativity and Quantum Cosmologycosmic background radiation cosmological parameters cosmology observations dark energy large-scale structure of UniverseHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencescosmological parametersdark energy010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsEquation of state (cosmology)Matter power spectrumSpectral densityAstronomy and AstrophysicsCosmic varianceHigh Energy Physics - Phenomenologyobservations13. Climate actionSpace and Planetary ScienceDark energylarge-scale structure of UniversecosmologyAstrophysics - Cosmology and Nongalactic Astrophysics
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Flavor versus mass eigenstates in neutrino asymmetries: implications for cosmology

2017

We show that, if they exist, lepton number asymmetries ($L_\alpha$) of neutrino flavors should be distinguished from the ones ($L_i$) of mass eigenstates, since Big Bang Nucleosynthesis (BBN) bounds on the flavor eigenstates cannot be directly applied to the mass eigenstates. Similarly, Cosmic Microwave Background (CMB) constraints on mass eigenstates do not directly constrain flavor asymmetries. Due to the difference of mass and flavor eigenstates, the cosmological constraint on the asymmetries of neutrino flavors can be much stronger than conventional expectation, but not uniquely determined unless at least the asymmetry of the heaviest neutrino is well constrained. Cosmological constrain…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)media_common.quotation_subjectHigh Energy Physics::LatticeCosmic microwave backgroundCosmic background radiationFOS: Physical scienceslcsh:AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAsymmetryCosmologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesislcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Eigenvalues and eigenvectorsmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLepton numberHigh Energy Physics - Phenomenologylcsh:QC770-798High Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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New cosmological bounds on hot relics: Axions $\&$ Neutrinos

2020

Axions, if realized in nature, can be copiously produced in the early universe via thermal processes, contributing to the mass-energy density of thermal hot relics. In light of the most recent cosmological observations, we analyze two different thermal processes within a realistic mixed hot-dark-matter scenario which includes also massive neutrinos. Considering the axion-gluon thermalization channel we derive our most constraining bounds on the hot relic masses $m_a < 7.46$ eV and $\sum m_��< 0.114$ eV both at 95 per cent CL; while studying the axion-pion scattering, without assuming any specific model for the axion-pion interactions and remaining in the range of validity of the chira…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectorsmedia_common.quotation_subjectDark matterCosmic background radiationFOS: Physical sciencescosmic background radiation; cosmological parameters; dark matter; early Universe; cosmology: observations;7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciences010306 general physicsAxionmedia_commonPhysics010308 nuclear & particles physicsHot dark matterHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsUniverseHigh Energy Physics - Phenomenology13. Climate actionSpace and Planetary ScienceStrong CP problemNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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How to relax the cosmological neutrino mass bound

2019

We study the impact of non-standard momentum distributions of cosmic neutrinos on the anisotropy spectrum of the cosmic microwave background and the matter power spectrum of the large scale structure. We show that the neutrino distribution has almost no unique observable imprint, as it is almost entirely degenerate with the effective number of neutrino flavours, $N_{\mathrm{eff}}$, and the neutrino mass, $m_{\nu}$. Performing a Markov chain Monte Carlo analysis with current cosmological data, we demonstrate that the neutrino mass bound heavily depends on the assumed momentum distribution of relic neutrinos. The message of this work is simple and has to our knowledge not been pointed out cle…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)cosmological neutrinosPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicscosmological parameters from LSS01 natural sciencesCosmologyMomentumsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)cosmological0103 physical sciencesPhysicsCOSMIC cancer database010308 nuclear & particles physicsMatter power spectrumHigh Energy Physics::Phenomenologycosmological parameters from CMBRAstronomy and AstrophysicsObservableMarkov chain Monte Carloneutrino masses from cosmologyHigh Energy Physics - Phenomenologyparameters from CMBRsymbolsHigh Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Asymmetric Dark Matter and Dark Radiation

2012

Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymmetry, similar to the one observed in the Baryon sector, to account for the Dark Matter (DM) abundance. Both asymmetries are usually generated by the same mechanism and generally related, thus predicting DM masses around 5 GeV in order to obtain the correct density. The main challenge for successful models is to ensure efficient annihilation of the thermally produced symmetric component of such a light DM candidate without violating constraints from collider or direct searches. A common way to overcome this involves a light mediator, into which DM can efficiently annihilate and which subsequently decays into Standard Mod…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic microwave backgroundDark matterFOS: Physical sciences01 natural sciencesStandard Modelsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010306 general physicsParticle Physics - Phenomenologymedia_commonPhysicsCosmologia010308 nuclear & particles physicsMatter power spectrumAstronomy and AstrophysicsUniverseBaryonHigh Energy Physics - Phenomenology13. Climate actionDark radiationsymbolsAstrophysics - Cosmology and Nongalactic Astrophysics
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Search for diphoton events with large missing transverse energy in 7 TeV proton-proton collisions with the ATLAS detector.

2011

A search for diphoton events with large missing transverse energy is presented. The data were collected with the ATLAS detector in proton-proton collisions at √s=7  TeV at the CERN Large Hadron Collider and correspond to an integrated luminosity of 3.1  pb−1. No excess of such events is observed above the standard model background prediction. In the context of a specific model with one universal extra dimension with compactification radius R and gravity-induced decays, values of 1/R<729  GeV are excluded at 95% C. L., providing the most sensitive limit on this model to date.

Particle physicsMISSING TRANSVERSE ENERGYCiências Naturais::Ciências FísicasAtlas detector:Ciências Físicas [Ciências Naturais]FIS/04 - Fisica Nucleare e SubnucleareGeneral Physics and AstronomyFOS: Physical sciencestransverse energy: missing-energy ; ATLAS ; universal extra dimension ; compactification ; CERN LHC Coll ; background ; p p: interaction ; final state: two-photon ; photon: Kaluza-Klein ; electroweak interaction: standard model: validity test ; experimental results ; 7000 GeV-cmsddc:500.201 natural sciences7. Clean energy530High Energy Physics - ExperimentNuclear physicsUniversal extra dimensionHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesddc:550[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]diphoton; events; transverse energy;proton-proton collisions; Hadron;ddc:530High Energy PhysicsSpecific model010306 general physicsNuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCPhysicsLarge Hadron ColliderScience & TechnologyCompactification (physics)010308 nuclear & particles physicsAtlas (topology)Settore FIS/01 - Fisica SperimentaleFísicaFIS/01 - Fisica SperimentaleATLASTransverse planeCol·lisions (Física nuclear)Experimental High Energy PhysicsUniversal Extra DimensionsFísica nuclearHigh Energy Physics::ExperimentLHCParticle Physics - ExperimentPhysical review letters
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Observation and Mass Measurement of the BaryonΞb−

2007

We report the observation and measurement of the mass of the bottom, strange baryon $\Xi^-_b$ through the decay chain $\Xi^-_b \to J/\psi \Xi^-$, where $J/\psi \to \mu^+ \mu^-$, $\Xi^- \to \Lambda \pi^-$, and $\Lambda \to p \pi^-$. Evidence for observation is based on a signal whose probability of arising from the estimated background is 6.6 x 10^{-15}, or 7.7 Gaussian standard deviations. The $\Xi^-_b$ mass is measured to be $5792.9\pm 2.5$ (stat.) $\pm 1.7$ (syst.) MeV/$c^2$.

Particle physicsPhysics MultidisciplinaryHadronGaussian distributionMass measurementGeneral Physics and Astronomyddc:500.2.Lambda baryon01 natural sciencesHigh Energy Physics - ExperimentXi baryonParticle decay0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Measurement theoryNuclear Experiment010306 general physicsProbabilityPhysicsMuon010308 nuclear & particles physicsPhysicsHyperonBackground fluctuationBaryonCrystallography14.20.Mr 13.30.Eg 13.60.RjHigh Energy Physics::ExperimentNucleonPhysical Review Letters
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Measurement of the parity violating asymmetry in the quasielastic electron-deuteron scattering and improved determination of the magnetic strange for…

2016

A new measurement of the parity-violating asymmetry in the electron-deuteron quasielastic scattering for backward angles at $⟨{Q}^{2}⟩=0.224\text{ }\text{ }{(\mathrm{GeV}/c)}^{2}$, obtained in the A4 experiment at the Mainz Microtron accelerator (MAMI) facility, is presented. The measured asymmetry is ${A}_{PV}^{d}=(\ensuremath{-}20.11\ifmmode\pm\else\textpm\fi{}0.8{7}_{\mathrm{stat}}\ifmmode\pm\else\textpm\fi{}\phantom{\rule{0ex}{0ex}}1.0{3}_{\mathrm{sys}})\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}6}$. A combination of these data with the proton measurements of the parity-violating asymmetry in the A4 experiment yields a value for the effective isovector axial-vector form facto…

Particle physicsacceleratorparity: violation: asymmetrymedia_common.quotation_subjectLattice field theoryisovectorelectron deuteron: inelastic scatteringpolarized beamElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]form factor: axial-vector01 natural sciencesAsymmetryMainz Linac0103 physical sciencesdeuterium: targetradiative correctionelectron: beam010306 general physicsmedia_commonPhysicsQuasielastic scatteringIsovector010308 nuclear & particles physicsScatteringbackgroundlattice field theoryParity (physics)helicityanapoleHelicityelectron deuteron: scatteringexperimental results
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Paleolimnological evidence of environmental changes in seven subtropical reservoirs based on metals, nutrients, and sedimentation rates

2021

Made available in DSpace on 2022-04-28T19:40:54Z (GMT). No. of bitstreams: 0 Previous issue date: 2021-11-01 Paleolimnological research can shed light on a broad range of environmental concerns; however, such studies are scarce in reservoirs. To address this lack of knowledge, a paleolimnological investigation was conducted to determine historical changes in sedimentation rates (SR), using 210Pb geochronology, and concentrations of nutrients and metals (Cr, Cu, Ni, Pb, Zn, Al, Mn, Fe) in seven subtropical reservoirs (São Paulo, Brazil). Sediment cores were collected in the dam areas. Increasing SR was observed in all reservoirs and was mainly attributed to eutrophication and changes in land…

Phosphoruschemistry.chemical_elementSedimentBackground levelsEcological RiskSubtropicsSedimentationContaminationNutrientchemistryWastewaterContaminationEnvironmental chemistryEnvironmental scienceEutrophicationMetal MigrationCopperEarth-Surface Processes
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