Search results for "background"

showing 10 items of 556 documents

Probing interactions within the dark matter sector via extra radiation contributions

2013

The nature of dark matter is one of the most thrilling riddles for both cosmology and particle physics nowadays. While in the typical models the dark sector is composed only by weakly interacting massive particles, an arguably more natural scenario would include a whole set of gauge interactions which are invisible for the standard model but that are in contact with the dark matter. We present a method to constrain the number of massless gauge bosons and other relativistic particles that might be present in the dark sector using current and future cosmic microwave background data, and provide upper bounds on the size of the dark sector. We use the fact that the dark matter abundance depends…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectDark matterCosmic microwave backgroundFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCosmologyPartícules (Física nuclear)symbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)PlanckDigital sky surveymedia_commonPhysicsHigh Energy Physics::PhenomenologyUniverseHigh Energy Physics - PhenomenologyWeakly interacting massive particlessymbolsBaryon acoustic-oscillationsBaryon acoustic oscillationsAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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Limits on tau lepton-flavor violating decays into three charged leptons

2010

A search for the neutrinoless, lepton-flavor violating decay of the tau lepton into three charged leptons has been performed using an integrated luminosity of 468 fb(-1) collected with the BABAR detector at the PEP-II collider. In all six decay modes considered, the numbers of events found in data are compatible with the background expectations. Upper limits on the branching fractions are set in the range (1.8-3.3) x 10(-8) at 90% confidence level.

Nuclear and High Energy PhysicsParticle physicsElectron–positron annihilationBABARFOS: Physical sciencesElementary particletau: branching ratioelectron positron: annihilationmeson01 natural sciencesPARTICLE PHYSICS; PEP2; BABARHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Particle decaytau: leptonic decay; lepton: flavor: violation; tau: branching ratio; BaBar; background; SLAC PEP Stor; electron positron: annihilation; tau: pair production; final state: (0neutrino); upper limit; tau- --> lepton+ 2lepton-; 10.54: 10.58 GeV-cms quark: angular momentum; positron electron --> quark antiquark; excited state; mesonexcited state0103 physical sciencesPEP2[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]10.54: 10.58 GeV-cms quark: angular momentumpositron electron --> quark antiquark010306 general physicsfinal state: (0neutrino)PACS: 13.35.DxFlavorPhysicstau- --> lepton+ 2lepton-tau: pair productionlepton flavor violationbackground010308 nuclear & particles physicsQuark modelHigh Energy Physics::Phenomenologylepton: flavor: violationParticle physicsFermionBABAR detectorSLAC PEP StorHEPCharged particletau: leptonic decayPARTICLE PHYSICSHigh Energy Physics::ExperimentFísica de partículesExperimentsupper limitLeptonPhysical Review D
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Pinch technique for Schwinger-Dyson equations

2007

40 pages, 11 figures.-- ISI Article Identifier: 000245922000041.-- ArXiv pre-print available at: http://arxiv.org/abs/hep-ph/0611354

Nuclear and High Energy PhysicsParticle physicsGeneralizationStructure (category theory)FOS: Physical sciencesContext (language use)Skeleton (category theory)Theoretical physicsHigh Energy Physics - Phenomenology (hep-ph)Self-energiesBackground-field MethodAbelian Gauge TheoriesPhysicsBackground field methodScalar (physics)FísicaPerturbation-theoryEffective ChargeFundamental interaction3-point VertexHigh Energy Physics - PhenomenologyNonperturbative EffectsQuantum Chromodynamics (QCD)Gauge SymmetryPinchBRST SymmetryJournal of High Energy Physics
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The neutron background of the XENON100 dark matter search experiment

2013

TheXENON100 experiment, installed underground at the LaboratoriNazionali del Gran Sasso, aims to directly detect dark matter in the form of weakly interacting massive particles (WIMPs) via their elastic scattering off xenon nuclei. This paper presents a study on the nuclear recoil background of the experiment, taking into account neutron backgrounds from (alpha, n) reactions and spontaneous fission due to natural radioactivity in the detector and shield materials, as well as muon-induced neutrons. Based on MonteCarlo simulations and using measured radioactive contaminations of all detector components, we predict the nuclear recoil backgrounds for the WIMP search results published by theXENO…

Nuclear and High Energy PhysicsParticle physicsLarge Underground Xenon experimentPhysics::Instrumentation and DetectorsDark matterGeant4Astrophysics::Cosmology and Extragalactic AstrophysicsWIMP Argon Programme01 natural sciencesNuclear physicsWIMPNuclear and High Energy Physics Neutron Background Dark Matter Search XENON TPC0103 physical sciencesNeutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)ComputingMilieux_MISCELLANEOUSSpontaneous fissionPhysicsElastic scatteringFluxMuons010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsWeakly interacting massive particlesHigh Energy Physics::ExperimentSimulation
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Measurement of the intrinsic electron neutrino component in the T2K neutrino beam with the ND280 detector

2014

The T2K experiment has reported the first observation of the appearance of electron neutrinos in a muon neutrino beam. The main and irreducible background to the appearance signal comes from the presence in the neutrino beam of a small intrinsic component of electron neutrinos originating from muon and kaon decays. In T2K, this component is expected to represent 1.2% of the total neutrino flux. A measurement of this component using the near detector (ND280), located 280 m from the target, is presented. The charged current interactions of electron neutrinos are selected by combining the particle identification capabilities of both the time projection chambers and electromagnetic calorimeters…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 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 physicsNeutrino oscillationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyT2K experimentFísicaSolar neutrino problem3. Good healthCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Light sterile neutrino sensitivity at the nuSTORM facility

2014

A facility that can deliver beams of electron and muon neutrinos from the decay of a stored muon beam has the potential to unambiguously resolve the issue of the evidence for light sterile neutrinos that arises in short-baseline neutrino oscillation experiments and from estimates of the effective number of neutrino flavors from fits to cosmological data. In this paper, we show that the nuSTORM facility, with stored muons of 3.8 GeV/c $\pm$ 10%, will be able to carry out a conclusive muon neutrino appearance search for sterile neutrinos and test the LSND and MiniBooNE experimental signals with 10$\sigma$ sensitivity, even assuming conservative estimates for the systematic uncertainties. This…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy & AstrophysicsComputer Science::Digital LibrariesPartícules (Física nuclear)High Energy Physics - ExperimentMiniBooNENuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0201 Astronomical and Space SciencesTOOLKITNeutrino oscillationDETECTOR0206 Quantum PhysicsPhysicsGALLEXScience & Technologyhep-exPhysicsPHYSICS PARTICLES & FIELDSHigh Energy Physics::Phenomenologyhep-phSolar neutrino problemNuclear & Particles PhysicsCosmic neutrino backgroundHigh Energy Physics - PhenomenologyNeutrino detectorPhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma PhysicsComputer Science::Mathematical SoftwareMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrinoParticle Physics - Experiment
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Quintessence, inflation and baryogenesis from a single pseudo-Nambu-Goldstone boson

2007

15 pages, 3 figures.-- ISI Article Identifier: 000250759700079.-- ArXiv pre-print available at: http://arxiv.org/abs/0707.3999

Nuclear and High Energy PhysicsParticle physicsProton decayCosmic microwave backgroundGenerationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicssymbols.namesakePlanckBosonPhysicsHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)BaryogenesisFísicaCosmology of Theories beyond the SMWater Cherenkov DetectorBaryogenesisGoldstone bosonLeptogenesissymbolsDark energyHigh Energy Physics::ExperimentQuintessence
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Pileup and underlying event mitigation with iterative constituent subtraction

2019

Abstract The hard-scatter processes in hadronic collisions are often largely contaminated with soft background coming from pileup in proton-proton collisions, or underlying event in heavy-ion collisions. This paper presents a new background subtraction method for jets and event observables (such as missing transverse energy) which is based on the previously published Constituent Subtraction algorithm. The new subtraction method, called Iterative Constituent Subtraction, applies event-wide implementation of Constituent Subtraction iteratively in order to fully equilibrate the background subtraction across the entire event. Besides documenting the new method, we provide guidelines for setting…

Nuclear and High Energy PhysicsParticle physicsSubtraction methodFOS: Physical sciences01 natural sciencesMinimum biasHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Hadron-Hadron scattering (experiments)0103 physical sciencesJetslcsh:Nuclear and particle physics. Atomic energy. RadioactivityHardware_ARITHMETICANDLOGICSTRUCTURES010306 general physicsNuclear ExperimentEvent (probability theory)PhysicsBackground subtractionHard scattering010308 nuclear & particles physicsSubtractionObservableHigh Energy Physics - Phenomenologylcsh:QC770-798AlgorithmJet substructureEnergy (signal processing)Underlying eventFree parameterJournal of High Energy Physics
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Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope

2012

The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximal mixing, a mass …

Nuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2Neutrino telescope01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Experiment0103 physical sciencesNeutrinsHigh Energy PhysicsNeutrinos010306 general physicsNeutrino oscillationPhysicsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsNeutrino oscillations[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologySolar neutrino problemNeutrino astrophysicsCosmic neutrino backgroundNeutrino detectorFISICA APLICADAMeasurements of neutrino speedFísica nuclearHigh Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physics Letters B
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Search for two-neutrino double electron capture of $^{124}$Xe with XENON100

2017

Two-neutrino double electron capture is a rare nuclear decay where two electrons are simultaneously captured from the atomic shell. For $^{124}$Xe this process has not yet been observed and its detection would provide a new reference for nuclear matrix element calculations. We have conducted a search for two-neutrino double electron capture from the K-shell of $^{124}$Xe using 7636 kg$\cdot$d of data from the XENON100 dark matter detector. Using a Bayesian analysis we observed no significant excess above background, leading to a lower 90 % credibility limit on the half-life $T_{1/2}>6.5\times10^{20}$ yr. We also evaluated the sensitivity of the XENON1T experiment, which is currently bein…

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsElectron captureenergy resolutionFOS: Physical scienceschemistry.chemical_elementelectron: captureElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesBayesianX-rayneutrinoXenon0103 physical sciencesSensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det][ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Experiment (nucl-ex)010306 general physics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear ExperimentPhysicsnucleus: decayTime projection chamberphotomultiplier010308 nuclear & particles physicsbackgroundInstrumentation and Detectors (physics.ins-det)dark matter: detectorAtomic shellsensitivitytime projection chamberGran SassoxenonchemistryNeutrinoAtomic physicsRadioactive decayexperimental results
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