Search results for "530"

showing 10 items of 1476 documents

Consistent Searches for SMEFT Effects in Non-Resonant Dilepton Events

2019

Employing the framework of the Standard Model Effective Field Theory, we perform a detailed reinterpretation of measurements of the Weinberg angle in dilepton production as a search for new-physics effects. We truncate our signal prediction at order $1/\Lambda^2$, where $\Lambda$ denotes the new-physics mass scale, and introduce a theory error to account for unknown contributions of order $1/\Lambda^4$. Two linear combinations of four-fermion operators with distinct angular behavior contribute to dilepton production with growing impact at high energies. We define suitable angular observables and derive bounds on those two linear combinations using data from the Tevatron and the LHC. We find…

Nuclear and High Energy Physics530 PhysicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesEffective Field Theories10192 Physics InstituteHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Beyond Standard Modellcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. Radioactivity3106 Nuclear and High Energy Physics
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First Muon-Neutrino Disappearance Study with an Off-Axis Beam

2012

We report a measurement of muon-neutrino disappearance in the T2K experiment. The 295-km muon-neutrino beam from Tokai to Kamioka is the first implementation of the off-axis technique in a long-baseline neutrino oscillation experiment. With data corresponding to 1.43 × 10(20) protons on target, we observe 31 fully-contained single μ-like ring events in Super-Kamiokande, compared with an expectation of 104 ± 14(syst) events without neutrino oscillations. The best-fit point for two-flavor νμ → ντ oscillations is sin 2(2θ(23)) = 0.98 and |Δm(2)(32)| = 2.65 × 10(−3) eV2. The boundary of the 90% confidence region includes the points (sin2 (2θ(23)), |Δm(2)(32)|) = (1.0, 3.1 × 10(−3) eV2), (0.84, …

Nuclear and High Energy Physics530 PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.27. Clean energy01 natural sciencesNeutrino scatteringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Muon neutrino010306 general physicsNeutrino oscillationQCPhysics010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologyT2K experimentFísicaPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentBeam (structure)
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Searching for Physics Beyond the Standard Model in an Off-Axis DUNE Near Detector

2021

Next generation neutrino oscillation experiments like DUNE and T2HK are multi-purpose observatories, with a rich physics program beyond oscillation measurements. A special role is played by their near detector facilities, which are particularly well-suited to search for weakly coupled dark sector particles produced in the primary target. In this paper, we demonstrate this by estimating the sensitivity of the DUNE near detectors to the scattering of sub-GeV DM particles and to the decay of sub-GeV sterile neutrinos ("heavy neutral leptons"). We discuss in particular the importance of the DUNE-PRISM design, which allows some of the near detectors to be moved away from the beam axis. At such o…

Nuclear and High Energy Physics530 Physicshep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFOS: Physical scienceshep-ph10192 Physics InstituteQC770-79801 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. RadioactivityBeyond Standard Model0103 physical sciencesNeutrino PhysicsHigh Energy Physics::Experiment3106 Nuclear and High Energy Physics010306 general physicsParticle Physics - ExperimentParticle Physics - Phenomenology
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Mass and half-life measurements of neutron-deficient iodine isotopes

2020

The European physical journal / A 56(5), 143 (2020). doi:10.1140/epja/s10050-020-00153-5

Nuclear and High Energy PhysicsALPHA-DECAYSEPARATORMass spectrometry01 natural sciences530Ionjodi0103 physical sciencesNuclear fusionNeutronddc:530010306 general physicsNuclear ExperimentPhysicsisotoopitIsotope010308 nuclear & particles physicsPERFORMANCESPECTROMETRYQuadrupoleFRS; PROJECTILEAlpha decayAtomic physicsydinfysiikkaGround stateSYSTEM
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Performance of a high repetition pulse rate laser system for in-gas-jet laser ionization studies with the Leuven laser ion source @ LISOL

2012

The Leuven Isotope Separator On-Line (LISOL) facility at the Cyclotron Research Center (CRC) Louvain-la-Neuve; The laser ionization efficiency of the Leuven gas cell-based laser ion source was investigated under on- and off-line conditions using two distinctly different laser setups: a low-repetition rate dye laser system and a high-repetition rate Ti:sapphire laser system. A systematic study of the ion signal dependence on repetition rate and laser pulse energy was performed in off-line tests using stable cobalt and copper isotopes. These studies also included in-gas-jet laser spectroscopy measurements on the hyperfine structure of 63Cu. A final run under on-line conditions in which the ra…

Nuclear and High Energy PhysicsActive laser medium29.25.Ni 29.25.Rm 41.85.ArPhysics::OpticsLaser pumping[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesAtmospheric-pressure laser ionizationlaw.inventionlaw0103 physical sciencesUltrafast laser spectroscopyddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Physics::Atomic Physics010306 general physicsInstrumentationDye laserta114010308 nuclear & particles physicsChemistryLaserIon sourceAtomic physicsAtomic vapor laser isotope separationNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Amplitude analysis and branching-fraction measurement of D-s(+) -> K-S(0)pi(+)pi(0)

2022

Journal of high energy physics 2021(6), 181 (2021). doi:10.1007/JHEP06(2021)181

Nuclear and High Energy PhysicsAnalytical chemistrye+-e− Experiments+53001 natural sciencesBranching fraction; Charm physics; e; +; -e; −; ExperimentsNOSubatomär fysikSubatomic Physics0103 physical sciencesPiddc:530010306 general physicsCharm physicsPhysics-e010308 nuclear & particles physicsBranching fractione(+)-e(-) ExperimentsBranching fraction Charm physics e+-e− ExperimentseAmplitudee-e ExperimentsBranching fractionExperiments
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Search for dark matter from the Galactic halo with the IceCube neutrino telescope

2011

Self-annihilating or decaying dark matter in the Galactic halo might produce high energy neutrinos detectable with neutrino telescopes. We have conducted a search for such a signal using 276 days of data from the IceCube 22-string configuration detector acquired during 2007 and 2008. The effect of halo model choice in the extracted limit is reduced by performing a search that considers the outer halo region and not the Galactic Center. We constrain any large-scale neutrino anisotropy and are able to set a limit on the dark matter self-annihilation cross section of ⟨σAv⟩≃10-22 cm3 s-1 for weakly interacting massive particle masses above 1 TeV, assuming a monochromatic neutrino line spectrum.

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesIceCubeGalactic halo0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsGamma-Ray EmissionHot dark matterAstronomyCosmic-Rays004Dark matter haloParticlesNeutrino detectorAnisotropyHigh Energy Physics::ExperimentHaloDwarf Spheroidal GalaxiesNeutrinoNeutrino astronomyinfo:eu-repo/classification/ddc/004
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IceCube search for dark matter annihilation in nearby galaxies and galaxy clusters

2013

Physical review / D 88(12), 122001 (2013). doi:10.1103/PhysRevD.88.122001

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxy merger53001 natural sciencesSIGNALSGalaxy group0103 physical sciencesPARTICLESHALOESddc:530Interacting galaxy010306 general physicsGalaxy clusterAstrophysics::Galaxy AstrophysicsDwarf galaxyHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstronomyCONSTRAINTSGalaxyEVOLUTIONPhysics and AstronomyElliptical galaxyHigh Energy Physics::ExperimentDark galaxyAstrophysics - High Energy Astrophysical PhenomenaSYSTEM
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Observation of individual spin quantum transitions of a single antiproton

2017

We report on the detection of individual spin quantum transitions of a single trapped antiproton in a Penning trap. The spin-state determination, which is based on the unambiguous detection of axial frequency shifts in presence of a strong magnetic bottle, reaches a fidelity of 92.1% . Spin-state initialization with >99.9% fidelity and an average initialization time of 24 min are demonstrated. This is a major step towards an antiproton magnetic moment measurement with a relative uncertainty on the part-per-billion level. We report on the detection of individual spin quantum transitions of a single trapped antiproton in a Penning trap. The spin-state determination, which is based on the unam…

Nuclear and High Energy PhysicsAtomic Physics (physics.atom-ph)Spin transitionOther Fields of PhysicsInitializationFOS: Physical sciences01 natural sciencesphysics.atom-phPhysics - Atomic Physics010309 optics0103 physical sciencesddc:530Physics::Atomic Physics010306 general physicsQuantumSpin-½PhysicsMeasurement methodMagnetic momentPenning traplcsh:QC1-999AntiprotonDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikAtomic physicsPräzisionsexperimente - Abteilung Blaumlcsh:Physics
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Measurement of branching fractions for D meson decaying into $ϕ$ meson and a pseudoscalar meson

2019

The four decay modes D0→ϕπ0, D0→ϕη, D+→ϕπ+, and D+→ϕK+ are studied by using a data sample taken at the centre-of-mass energy s=3.773 GeV with the BESIII detector, corresponding to an integrated luminosity of 2.93 fb$^{−1}$. The branching fractions of the first three decay modes are measured to be B(D0→ϕπ0)=(1.168±0.028±0.028)×10−3, B(D0→ϕη)=(1.81±0.46±0.06)×10−4, and B(D+→ϕπ+)=(5.70±0.05±0.13)×10−3, respectively, where the first uncertainties are statistical and the second are systematic. In addition, the upper limit of the branching fraction for D+→ϕK+ is given to be 2.1×10−5 at the 90% confidence level. The ratio of B(D0→ϕπ0) to B(D+→ϕπ+) is calculated to be (20.49±0.50±0.45)%, which is c…

Nuclear and High Energy PhysicsBESIII; Branching fractions; D meson; Hadronic decaysMesonAstrophysics::High Energy Astrophysical PhenomenaBESIII; Branching fractions; D meson; Hadronic decays; High Energy Physics - Experiment; High Energy Physics - ExperimentBranching (polymer chemistry)01 natural sciencesPseudoscalar mesonNOHigh Energy Physics - ExperimentSubatomär fysikHadronic decaysD Meson0103 physical sciencesD mesonSubatomic PhysicsHadronic DecaysBranching fractionsddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsBranching fractionBESIIIBranching Fractionslcsh:QC1-999D mesonIsospinHigh Energy Physics::ExperimentAtomic physicslcsh:Physics
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