Search results for "PARTICLE PHYSICS"

showing 10 items of 6826 documents

Systematic uncertainties from halo asphericity in dark matter searches

2015

Although commonly assumed to be spherical, dark matter halos are predicted to be non-spherical by N-body simulations and their asphericity has a potential impact on the systematic uncertainties in dark matter searches. The evaluation of these uncertainties is the main aim of this work, where we study the impact of aspherical dark matter density distributions in Milky-Way-like halos on direct and indirect searches. Using data from the large N-body cosmological simulation Bolshoi, we perform a statistical analysis and quantify the systematic uncertainties on the determination of local dark matter density and the so-called $J$ factors for dark matter annihilations and decays from the galactic …

N-body SimulationsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Milky WayDwarf galaxy problemDark matterScalar field dark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesMany-body problemHigh Energy Physics - Phenomenology (hep-ph)Baryonic dark matter0103 physical sciencesDark matter010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsPotential impactAnnihilation010308 nuclear & particles physicsHot dark matterGalactic CenterAstronomyAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxiestriaxial halosDark matter haloHigh Energy Physics - Phenomenology13. Climate actionAstrophysics of Galaxies (astro-ph.GA)Cuspy halo problemHaloDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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Update of the search for supersymmetric particles in scenarios with Gravitino LSP and Sleptons NLSP

2001

An update of the search for sleptons, neutralinos and charginos in the context of scenarios where the lightest supersymmetric particle is the gravitino and the next-to-lightest supersymmetric particle is a slepton, is presented, together with the update of the search for heavy stable charged particles in light gravitino scenarios and Minimal Supersymmetric Standard Models. Data collected in 1999 with the DELPHI detector at centre-of-mass energies around 192, 196, 200 and 202 GeV were analysed. No evidence for the production of these supersymmetric particles was found. Hence, new mass limits were derived at 95% confidence level.

NEUTRALINOSNuclear and High Energy PhysicsParticle physicsMONTE-CARLO SIMULATION; LOWEST ORDER CALCULATIONS; E(+)E(-) COLLISIONS; 2-PHOTON PROCESSES; PAIR PRODUCTION; MISSING ENERGY; STAU NLSP; BREAKING; SUPERGRAVITY; NEUTRALINOSLOWEST ORDER CALCULATIONSPAIR PRODUCTIONMONTE-CARLO SIMULATIONFOS: Physical sciences2-PHOTON PROCESSESContext (language use)01 natural sciencesLightest Supersymmetric ParticlePartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)E(+)E(-) COLLISIONS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SUPERGRAVITY010306 general physicsDELPHIPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLARGE ELECTRON POSITRON COLLIDERCharged particleSTAU NLSPPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIParticlePARTICLE PHYSICSMISSING ENERGYGravitinoFísica nuclearHigh Energy Physics::ExperimentParticle Physics - ExperimentBREAKING
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Photon events with missing energy at root s=183 to 189 GeV

2000

The production of single photons has been studied in the reaction e+e- -> gamma + invisible particles at centre-of-mass energies of 183 GeV and 189 GeV. A previously published analysis of events with multi-photon final states accompanied by missing energy has been updated with 189 GeV data. The data were collected with the DELPHI detector and correspond to integrated luminosities of about 51 pb^{-1} and 158 pb^{-1} at the two energies. The number of light neutrino families is measured to be 2.84 +/- 0.15(stat) +/- 0.14(syst). The absence of an excess of events beyond that expected from Standard Model processes is used to set limits on new physics as described by supersymmetric and compos…

NEUTRALINOSParticle physicsDIMENSIONSPhotonPhysics and Astronomy (miscellaneous)Physics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaSTANDARD MODELFOS: Physical sciencesScale (descriptive set theory)7. Clean energy01 natural sciencesPartícules (Física nuclear)Standard ModelHigh Energy Physics - ExperimentGravitationHigh Energy Physics - Experiment (hep-ex)E(+)E(-) COLLISIONSSIGNALSSEARCH0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNuclear ExperimentEngineering (miscellaneous)DELPHIPhysicsMissing energy010308 nuclear & particles physicsSUPERLIGHT GRAVITINOLEPLARGE ELECTRON POSITRON COLLIDERSINGLE-PHOTONCOLLIDERSPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSProduction (computer science)Física nuclearHigh Energy Physics::ExperimentNeutrinoE(+)E(-) COLLISIONS; SUPERLIGHT GRAVITINO; STANDARD MODEL; SINGLE-PHOTON; COLLIDERS; SEARCH; LEP; NEUTRALINOS; DIMENSIONS; SIGNALSParticle Physics - Experiment
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Search for supersymmetric particles in scenarios with a gravitino LSP and stau NLSP

2000

Sleptons, neutralinos and charginos were searched for in the context of scenarios where the lightest supersymmetric particle is the gravitino. It was assumed that the stau is the next-to-lightest supersymmetric particle. Data collected with the DELPHI detector at a centre-of-mass energy near 189 GeV were analysed combining the methods developed in previous searches at lower energies. No evidence for the production of these supersymmetric particles was found. Hence, limits were derived at 95% confidence level.

NEUTRALINOSParticle physicsPhysics and Astronomy (miscellaneous)LOWEST ORDER CALCULATIONSPAIR PRODUCTIONENERGIESMONTE-CARLO SIMULATIONpluridisciplinarityFOS: Physical sciences2-PHOTON PROCESSESContext (language use)01 natural sciencesLightest Supersymmetric ParticlePartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)E(+)E(-) COLLISIONS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RADIATIVE-CORRECTIONSontology010306 general physicsEngineering (miscellaneous)DELPHIPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyreflexivityLEPscience studiesepistemologieLARGE ELECTRON POSITRON COLLIDERhistory of sciencePARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIMONTE-CARLO SIMULATION; LOWEST ORDER CALCULATIONS; RADIATIVE-CORRECTIONS; PAIR PRODUCTION; E(+)E(-) COLLISIONS; 2-PHOTON PROCESSES; ENERGIES; BREAKING; LEP; NEUTRALINOSParticlePARTICLE PHYSICSGravitinoFísica nuclearHigh Energy Physics::ExperimentcomplexityParticle Physics - ExperimentBREAKING
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Nonzero |U_e3| from charged lepton corrections and the atmospheric neutrino mixing angle

2013

After the successful determination of the reactor neutrino mixing angle theta(13) not equal 0.16 not equal 0, a new feature suggested by the current neutrino oscillation data is a sizeable deviation of the atmospheric neutrino mixing angle theta(23) from pi/4. Using the fact that the neutrino mixing matrix U = (UeU nu)-U-dagger, where U-e and U-nu result from the diagonalisation of the charged lepton and neutrino mass matrices, and assuming that U-nu has a i) bimaximal (BM), H) tri-bimaximal (TBM) form, or else Hi) corresponds to the conservation of the lepton charge L' = L-e - L mu - L-tau (LC), we investigate quantitatively what are the minimal forms of U-e, in terms of angles and phases …

NEUTRINO MIXING CP VIOLATION CHOOZ ANGLE ATMOSPHERIC NEUTRINO MIXING ANGLE CHERGED LEPTON CORRECTIONSNuclear and High Energy PhysicsParticle physicsSolar neutrinoCHOOZ ANGLEPontecorvo–Maki–Nakagawa–Sakata matrixInverseFOS: Physical sciencesType (model theory)7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)CHERGED LEPTON CORRECTIONS0103 physical sciencesNeutrino Physics010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsATMOSPHERIC NEUTRINO MIXING ANGLENEUTRINO MIXINGSettore FIS/02 - Fisica Teorica Modelli e Metodi MatematiciHigh Energy Physics - PhenomenologyCP violationCP violationCP VIOLATIONNeutrinoLepton
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Gain fractions of future neutrino oscillation facilities over T2K and NOvA

2013

We evaluate the probability of future neutrino oscillation facilities to discover leptonic CP violation and/or measure the neutrino mass hierarchy. We study how this probability is affected by positive or negative hints for these observables to be found at T2K and NO nu A. We consider the following facilities: LBNE; T2HK; and the 10 GeV Neutrino Factory (NF10), and show how their discovery probabilities change with the running time of T2K and NO nu A conditioned to their results. We find that, if after 15 years T2K and NO nu A have not observed a 90% CL hint of CP violation, then LBNE and T2HK have less than a 10% chance of achieving a 5 sigma discovery, whereas NF10 still has a similar to …

NOνAPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsPhysics beyond the Standard ModelFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentRunning timeHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)CP violationHigh Energy Physics - Phenomenology (hep-ph)Physical Sciences0103 physical sciencesFysikCP violationNeutrino PhysicsNeutrino FactoryFermilabNeutrino010306 general physicsNeutrino oscillationJournal of High Energy Physics
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Probing atmospheric mixing and leptonic CP violation in current and future long baseline oscillation experiments

2017

We perform realistic simulations of the current and future long baseline experiments such as T2K, NO$\nu$A, DUNE and T2HK in order to determine their ultimate potential in probing neutrino oscillation parameters. We quantify the potential of these experiments to underpin the octant of the atmospheric angle $\theta_{23}$ as well as the value and sign of the CP phase $\delta_{CP}$.

NOνAPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsPhysics beyond the Standard ModelSolar neutrinoFOS: Physical sciencesSolar neutrino problem01 natural scienceslcsh:QC1-999High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesCP violationMeasurements of neutrino speedNeutrino010306 general physicsNeutrino oscillationlcsh:PhysicsPhysics Letters B
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Neutrino interaction classification with a convolutional neural network in the DUNE far detector

2020

The Deep Underground Neutrino Experiment is a next-generation neutrino oscillation experiment that aims to measure CP-violation in the neutrino sector as part of a wider physics program. A deep learning approach based on a convolutional neural network has been developed to provide highly efficient and pure selections of electron neutrino and muon neutrino charged-current interactions. The electron neutrino (antineutrino) selection efficiency peaks at 90% (94%) and exceeds 85% (90%) for reconstructed neutrino energies between 2–5 GeV. The muon neutrino (antineutrino) event selection is found to have a maximum efficiency of 96% (97%) and exceeds 90% (95%) efficiency for reconstructed neutrino…

Neutrino Oscillations. Neutrino detectors.Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsfar detector01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - Experimentcharged currentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Particle Physics ExperimentsMuon neutrinoneutrino/e: particle identificationNeutrino detectorsDetectors and Experimental Techniquesphysics.ins-detCharged currentneutrino: interactionInformáticaPhysicsTelecomunicacionesNeutrino oscillationsPhysicsNeutrino interactions neural network DUNE Deep Underground Neutrino ExperimentInstrumentation and Detectors (physics.ins-det)Experiment (hep-ex)Neutrino detectorPhysical SciencesCP violationNeutrinoParticle Physics - ExperimentParticle physicsdata analysis method530 Physicsneural networkAstrophysics::High Energy Astrophysical PhenomenaCONSERVATIONFOS: Physical sciencesAstronomy & AstrophysicsDeep Learningneutrino: deep underground detectorneutrino physics0103 physical sciencesNeutrino Oscillations. Neutrino detectorsObject DetectionNeutrinoCP: violationDeep Underground Neutrino ExperimentHigh Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinos010306 general physicsNeutrino oscillationneutrino/mu: particle identificationIOUScience & TechnologyDUNENeutrino interactions010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologyFísicaNeutrino InteractionDetector530 PhysiksensitivityefficiencyHigh Energy Physics::ExperimentElectron neutrino
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The next-generation liquid-scintillator neutrino observatory LENA

2012

We propose the liquid-scintillator detector LENA (Low Energy Neutrino Astronomy) as a next-generation neutrino observatory on the scale of 50 kt. The outstanding successes of the Borexino and KamLAND experiments demonstrate the large potential of liquid-scintillator detectors in low-energy neutrino physics. LENA's physics objectives comprise the observation of astrophysical and terrestrial neutrino sources as well as the investigation of neutrino oscillations. In the GeV energy range, the search for proton decay and long-baseline neutrino oscillation experiments complement the low-energy program. Based on the considerable expertise present in European and international research groups, the …

Neutrino detectors; Liquid-scintillator detectors; Low-energy neutrinos; Proton decay; Longbaseline neutrino beamsParticle physicsPhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaLongbaseline neutrino beamsFOS: Physical sciencesLow-energy neutrinos7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNONuclear physicsLiquid-scintillator detectorsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrino detectorsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsBorexinoPhysics010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Proton decaySolar neutrino problem[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Neutrino detectorddc:540Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - Instrumentation and Methods for Astrophysics
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Neutrino transition magnetic moments within the non-standard neutrino-nucleus interactions

2015

Tensorial non-standard neutrino interactions are studied through a combined analysis of nuclear structure calculations and a sensitivity $\chi^2$-type of neutrino events expected to be measured at the COHERENT experiment, recently planned to operate at the Spallation Neutron Source (Oak Ridge). Potential sizeable predictions on transition neutrino magnetic moments and other electromagnetic parameters, such as neutrino milli-charges, are also addressed. The non-standard neutrino-nucleus processes, explored from nuclear physics perspectives within the context of quasi-particle random phase approximation, are exploited in order to estimate the expected number of events originating from vector …

Neutrino magnetic moment and interactionsParticle physicsNuclear and High Energy PhysicsReactor neutrinosPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaSpallation neutron source neutrinosFOS: Physical sciencesContext (language use)Nuclear physicsHigh Energy Physics - Phenomenology (hep-ph)Quasi-particle random phase approximationNon-standard electroweak interactionsNeutrino oscillationPhysicsHigh Energy Physics::PhenomenologyNuclear structureSolar neutrino problemlcsh:QC1-999Lepton flavour violationHigh Energy Physics - PhenomenologyNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinolcsh:Physics
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