Search results for "Upper Limit"

showing 10 items of 59 documents

Limiting neutrino magnetic moments with Borexino Phase-II solar neutrino data

2017

A search for the solar neutrino effective magnetic moment has been performed using data from 1291.5 days exposure during the second phase of the Borexino experiment. No significant deviations from the expected shape of the electron recoil spectrum from solar neutrinos have been found, and a new upper limit on the effective neutrino magnetic moment of $\mu_{\nu}^{eff}$ $<$ 2.8$\cdot$10$^{-11}$ $\mu_{B}$ at 90\% c.l. has been set using constraints on the sum of the solar neutrino fluxes implied by the radiochemical gallium experiments.Using the limit for the effective neutrino moment, new limits for the magnetic moments of the neutrino flavor states, and for the elements of the neutrino magne…

Physics and Astronomy (miscellaneous)neutrino: solarPhysics::Instrumentation and DetectorsSolar neutrino01 natural sciencesHigh Energy Physics - ExperimentNeutrino detectorHigh Energy Physics - Experiment (hep-ex)SPIN ROTATIONHigh Energy Physics - Phenomenology (hep-ph)electron: recoil[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astrophysics::Solar and Stellar AstrophysicsBorexinoS066MGMgalliumPhysicsMagnetic momentneutrino: magnetic momentHigh Energy Physics - Phenomenologyneutrino: momentNeutrino detectorneutrino: flavorneutrino: MajoranaMeasurements of neutrino speedBorexinoNeutrinoupper limitParticle physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSolar neutrinoDECAYSMagnetic momentNuclear physicsstatistical analysis[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesddc:530010306 general physicsNeutrino oscillationDETECTORELECTROMAGNETIC PROPERTIES010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemMAJORANA NEUTRINOS[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]electron: energy spectrum[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentexperimental resultsPhysical Review D
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Electromagnetic form factors and axial charge of the nucleon from Nf = 2 + 1 Wilson fermions

2018

We present an update on our determination of the electromagnetic form factors and axial charge of the nucleon from theNf= 2 + 1 CLS ensembles with increased statistics and an additional finer lattice spacing. We also investigate the impact ofO(a)-improvement of the currents.

PhysicsCLs upper limitsLattice constant010308 nuclear & particles physicsQuantum electrodynamicsPhysicsQC1-9990103 physical sciencesCharge (physics)Fermion010306 general physicsNucleon01 natural sciencesEPJ Web of Conferences
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Search for an electric charge of the neutron

2018

The electrical neutrality of the neutron is linked to the electric charge quantization. It is not understood yet if the electric charge is quantized or not. Since the discovery of the neutron, many attempts have been made to measure its electric charge ${q}_{n}$ directly and indirectly. We present a method to search for a possible ${q}_{n}$ by means of an optical setup using ultracold neutrons. In a first run, a statistical sensitivity of $\ensuremath{\delta}{q}_{n}=2.4\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}20}\text{ }\text{ }e/\sqrt{\mathrm{day}}$ is achieved. Possible improvements to increase this sensitivity down to $\ensuremath{\delta}{q}_{n}\ensuremath{\approx}1\ifmmode\…

PhysicsMeasurement methodpotential: electrostatic010308 nuclear & particles physicscharge: electricStatistical sensitivitymeasurement methodssensitivity01 natural sciencesElectric chargeelectric fieldcharge: quantizationn: energy eigenstateElectric field0103 physical sciencesoptical[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]NeutronSensitivity (control systems)Atomic physics010306 general physicsmirrorstatisticalexperimental resultsn: charge: upper limit
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Adler function and hadronic vacuum polarization from lattice vector correlators in the time-momentum representation

2014

We study a representation of the hadronic vacuum polarization based on the time-momentum representation of the vector correlator. This representation suggests a way to compute the hadronic vacuum polarization and the associated Adler function for any value of virtuality, irrespective of the flavor structure of the current. We present results on both of these phenomenologically important functions, derived from local-conserved two-point lattice vector correlation functions, computed on a subset of light two-flavor ensembles made available to us through the CLS effort.

PhysicsParticle physicsCLs upper limitsLattice (order)High Energy Physics::PhenomenologyHadronVacuum polarizationProceedings of 31st International Symposium on Lattice Field Theory LATTICE 2013 — PoS(LATTICE 2013)
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Charmonium resonances from 2+1 flavor CLS lattices

2019

Many exotic charmonium resonances have been identified recently in experiment, however their nature and properties are mostly unknown. Algorithmic and theoretical progress in lattice calculations has enabled reliable numerical investigation of the spectrum below the strong decay threshold, while the study of charmonium resonances remains an open challenge. The main difficulty to overcome is the presence of many open decay channels which are coupled together, resulting in a complex finite volume quantization condition. We report on our recent progress towards the determination of single-channel and coupled-channel scattering matrices in the scalar and vector channels on CLS ensembles. We als…

PhysicsParticle physicsHigh Energy Physics - LatticeCLs upper limitsHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesFlavorProceedings of XIII Quark Confinement and the Hadron Spectrum — PoS(Confinement2018)
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Towards extracting the timelike pion form factor on CLS two-flavour ensembles

2017

35th International Symposium on Lattice Field Theory, Lattice 2017, Granada, Spain, 18 Jun 2017 - 24 Jun 2017; The European physical journal / Web of Conferences 175, 05027 (2018). doi:10.1051/epjconf/201817505027

PhysicsParticle physicsMuon010308 nuclear & particles physicsPhysicsQC1-999High Energy Physics::LatticeHadronHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesFermion01 natural sciences530Formalism (philosophy of mathematics)High Energy Physics - LatticeCLs upper limitsPion0103 physical sciencesddc:530High Energy Physics::ExperimentVacuum polarization010306 general physicsNuclear Experiment
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Towards extracting the timelike pion form factor on CLS 2-flavour ensembles

2016

Results are presented from an ongoing study of the $\rho$ resonance. We use the distillation approach in order to create correlator matrices involving $\rho$ and $\pi\pi$ interpolators. The study is done in a centre-of-mass frame and several moving frames. We are able to extract energy levels by solving the GEVP of those correlator matrices. The initial exploratory study is being done on a CLS 2-flavour lattice with a pion mass of $451$ $\mathrm{MeV}$ using $\mathcal{O}(a)$ improved Wilson fermions. One aim of this work is to extract the timelike pion form factor after applying the L\"uscher formalism. We also plan to integrate this study with the existing Mainz programme for the calculatio…

PhysicsParticle physicsMuonHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)HadronFlavourFOS: Physical sciencesFermionHigh Energy Physics - LatticePionCLs upper limitsLattice (order)High Energy Physics::ExperimentVacuum polarizationNuclear ExperimentProceedings of 34th annual International Symposium on Lattice Field Theory — PoS(LATTICE2016)
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The leading hadronic contribution to (g-2) of the muon: The chiral behavior using the mixed representation method

2015

We extend our analysis of the leading hadronic contribution to the anomalous magnetic moment of the muon using the mixed representation method to study its chiral behavior. We present results derived from local-conserved two-point lattice vector correlation functions, computed on a subset of light two-flavor ensembles made available to us through the CLS effort with pion masses as low as 190 MeV. The data is analyzed also using the more standard four-momentum method. Both methods are systematically compared as the calculations approach the physical point.

PhysicsPhysical pointParticle physicsMuonAnomalous magnetic dipole momentNuclear Theory010308 nuclear & particles physicsHadronHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciences01 natural sciencesNuclear Theory (nucl-th)High Energy Physics - PhenomenologyPionCLs upper limitsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeLattice (order)0103 physical sciences010306 general physics
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Excited state systematics in extracting nucleon electromagnetic form factors

2012

We present updated preliminary results for the nucleon electromagnetic form factors for non-perturbatively $\mathcal{O}(a)$ improved Wilson fermions in $N_f=2$ QCD measured on the CLS ensembles. The use of the summed operator insertion method allows us to suppress the influence of excited states in our measurements. A study of the effect that excited state contaminations have on the $Q^2$ dependence of the extracted nucleon form factors may then be made through comparisons of the summation method to standard plateau fits, as well as to excited state fits.

PhysicsQuantum chromodynamicsParticle physicsOperator (physics)High Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesFermionPlateau (mathematics)CLs upper limitsHigh Energy Physics - LatticeExcited stateQuantum electrodynamicsNucleon
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Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory

2011

Erratum: Phys. Rev. D 85, 029902(E) (2012) [http://dx.doi.org/10.1103/PhysRevD.85.029902]

Physics::Instrumentation and DetectorsSolar neutrinoAstrophysicsUPPER LIMITPHOTON FRACTION01 natural sciences7. Clean energyneutrinoObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsORIGINPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pionAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryCOSMIC-RAYScosmic ray detectorsand other elementary particle detectorsCosmic neutrino backgroundNEUTRINOSFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFLUXFERMI-LATNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]TELESCOPEAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSSURFACE DETECTORCosmic RayPionmuon0103 physical sciencesNeutrino010306 general physicsCosmic raysPierre Auger ObservatoryMuon010308 nuclear & particles physicsFísicaand other elementary particlesUltra-high energy cosmic raysPERFORMANCECosmic rayneutrino flavor; air showers; surface detector; observatory; atmosphere; Auger; cosmic radiation; energy spectrum13. Climate actionHigh Energy Physics::Experiment
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