Search results for "oscillations"

showing 10 items of 238 documents

Time course of excitatory and inhibitory states of bulbar respiratory modulated neurons.

1980

In respiratory modulated neurons of rabbits, vagally mediated inhibition is not bound to resting membrane potential oscillations. Latency of spinally evoked antidromical spike invasion, however, is shorter and threshold voltage is lower during the shift of membrane potential towards depolarization accompanying burst discharge.

PharmacologySynaptic potentialMembrane potentialNeuronsSubthreshold membrane potential oscillationsChemistryBrainDepolarizationVagus NerveCell BiologyInhibitory postsynaptic potentialElectric StimulationCellular and Molecular NeuroscienceOxygen ConsumptionSpinal CordThreshold potentialAnesthesiaExcitatory postsynaptic potentialMolecular MedicineAnimalsRabbitsRespiratory systemMolecular BiologyNeuroscienceExperientia
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Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU

2020

Physical review / D 101(3), 032006 (1-19) (2020). doi:10.1103/PhysRevD.101.032006

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsantineutrino/e: energy spectrumJoint analysishiukkasfysiikka7. Clean energy01 natural sciencesString (physics)PINGUHigh Energy Physics - ExperimentSubatomär fysikHigh Energy Physics - Experiment (hep-ex)neutrino: atmosphereSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Particle Physics Experimentsneutrino: massphysics.ins-detPhysicsJUNOPhysicsneutriinotoscillation [neutrino]Instrumentation and Detectors (physics.ins-det)massa (fysiikka)atmosphere [neutrino]tensionneutrino: nuclear reactormass difference [neutrino]ddc:UpgradePhysique des particules élémentairesnuclear reactor [neutrino]proposed experimentNeutrinoperformanceParticle physicsAstrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceFOS: Physical sciencesddc:500.25300103 physical sciencesEnergy spectrumIceCube: upgradeOSCILLATIONSddc:530Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationenergy spectrum [antineutrino/e]hep-ex010308 nuclear & particles physicssensitivityPhysics and Astronomymass [neutrino]stringupgrade [IceCube]High Energy Physics::ExperimentReactor neutrinoneutrino: oscillationMATTER
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PINGU: a vision for neutrino and particle physics at the South Pole

2017

The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful IceCube example, PINGU will provide a 6Mton effective mass for neutrino detection with an energy threshold of a few GeV. With an unprecedented sample of over 60,000 atmospheric neutrinos per year in this energy range, PINGU will make highly competitive measurements of neutrino oscillation parameters in an energy range over an order of magnitude higher than long-baseline neutrino beam experiments. PINGU will measure the mixing parameters $\theta_{\rm 23}$ and $\Delta m^2_{\rm 32}$, including the octan…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsmixing [neutrino]atmospheric neutrinos; IceCube Neutrino Observatory; neutrino oscillations; PINGU; Nuclear and High Energy Physicspole7. Clean energy01 natural sciencesPINGUIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - ExperimentObservatoryPhysicssolar [WIMP]precision measurementAstrophysics::Instrumentation and Methods for Astrophysicsoscillation [neutrino]solar [dark matter]atmosphere [neutrino]threshold [energy]mass difference [neutrino]atmospheric neutrinosobservatoryHigh Energy Physics - PhenomenologyUpgradeNeutrino detectorupgradeNeutrinoKM3NETperformanceParticle physicsNuclear and High Energy Physicssupernova [neutrino]particle identification [neutrino/tau]Astrophysics::High Energy Astrophysical PhenomenaSUPERNOVA DETECTIONIceCube Neutrino Observatory0103 physical sciencesOSCILLATIONSmass: low [dark matter]unitarityddc:530010306 general physicsNeutrino oscillationneutrino oscillations010308 nuclear & particles physicsAstronomysensitivityKM3NeTPhysics and Astronomymass [neutrino]beam [neutrino]High Energy Physics::ExperimentgalaxyATMOSPHERIC NEUTRINOSMATTERSYSTEMLeptonmixing angle [neutrino]experimental results
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Search for heavy neutrinos and right-handed W bosons in events with two leptons and jets in pp collisions at √s=7 TeV with the ATLAS detector

2012

This letter reports on a search for hypothetical heavy neutrinos, N, and right-handed gauge bosons, WR, in events with high transverse momentum objects which include two reconstructed leptons and at least one hadronic jet. The results were obtained from data corresponding to an integrated luminosity of 2.1 fb−1 collected in proton–proton collisions at √s=7 TeV with the ATLAS detector at the CERN Large Hadron Collider. No excess above the Standard Model background expectation is observed. Excluded mass regions for Majorana and Dirac neutrinos are presented using two approaches for interactions that violate lepton and lepton-flavor numbers. One approach uses an effective operator framework, t…

Physics and Astronomy (miscellaneous)Atlas detector01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]w bosonNuclear ExperimentDetectors de radiacióBosonMajorana Neutrinosddc:539PhysicsRight handedSettore FIS/01 - Fisica SperimentaleHadron-Hadron Scattering; ATLAS detectorATLASParityPhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearLHCNeutrinoParticle Physics - ExperimentParticle physicsOscillationsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2530Partícules (Física nuclear)Nuclear physics0103 physical sciencesFysikddc:530High Energy Physics010306 general physicsEngineering (miscellaneous)Ciencias ExactasLEFT-RIGHT SYMMETRYGauge bosonScience & TechnologyATLAS detectorViolation010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaParity (physics)LepMassEnergiesPair productionCol·lisions (Física nuclear)Experimental High Energy Physicsproton-proton collisionsHigh Energy Physics::ExperimentLepton
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Search for Lorentz and CPT violation using sidereal time dependence of neutrino flavor transitions over a short baseline

2017

A class of extensions of the Standard Model allows Lorentz and CPT violations, which can be identified by the observation of sidereal modulations in the neutrino interaction rate. A search for such modulations was performed using the T2K on-axis near detector. Two complementary methods were used in this study, both of which resulted in no evidence of a signal. Limits on associated Lorentz and CPT-violating terms from the Standard Model extension have been derived by taking into account their correlations in this model for the first time. These results imply such symmetry violations are suppressed by a factor of more than 1020 at the GeV scale.

Physics and Astronomy (miscellaneous)CPT symmetryAstrophysicsKAMIOKANDE01 natural scienceshigh energy physicsPhysics Particles & FieldsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Standard-Model Extension[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: interactionPhysicssymmetry: violationPhysicsJ-PARC LabCPT symmetrysuppressionLorentz symmetryviolation: LorentzmodulationSidereal timePhysical Sciencesneutrino: flavorsymbolsNeutrinoupper limitParticle physicsdata analysis method530 PhysicsLorentz transformationFOS: Physical sciencesCPT: violationAstronomy & AstrophysicsStandard Modelsymbols.namesakenear detectorstatistical analysis0103 physical sciences010306 general physicsNeutrino oscillationneutrino oscillationsScience & Technology010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologySymmetry (physics)neutrino/mu: secondary beamcorrelationtime dependenceHigh Energy Physics::Experimentneutrino: oscillationexperimental results
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Transverse Oscillations in Slender Ca II H Fibrils Observed with Sunrise/SuFI

2016

S. Jafarzadeh et. al.

Physics010504 meteorology & atmospheric sciencesCondensed matter physicsoscillations [Sun]imaging spectroscopy [Techniques]Sun: chromosphereFOS: Physical sciencesAstronomy and Astrophysicschromosphere [Sun]Fibril01 natural sciencesTransverse planemagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesSunriseAstrophysics::Solar and Stellar Astrophysics14. Life underwaterSun: oscillationsTechniques: imaging spectroscopySun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciences
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Collision of Akhmediev Breathers in Nonlinear Fiber Optics

2013

We report here a novel fiber-based test bed using tailored spectral shaping of an optical-frequency comb to excite the formation of two Akhmediev breathers that collide during propagation. We have found specific initial conditions by controlling the phase and velocity differences between breathers that lead, with certainty, to their efficient collision and the appearance of a giant-amplitude wave. Temporal and spectral characteristics of the collision dynamics are in agreement with the corresponding analytical solution. We anticipate that experimental evidence of breather-collision dynamics is of fundamental importance in the understanding of extreme ocean waves and in other disciplines dri…

PhysicsBreatherbusiness.industryPhysicsQC1-999Periodic oscillationsNonlinear fiber opticsGeneral Physics and AstronomyNonlinear opticsCollisionPhysical optics01 natural sciences010305 fluids & plasmasNonlinear Sciences::Exactly Solvable and Integrable SystemsClassical mechanicsOptics0103 physical sciences14. Life underwater010306 general physicsbusinessNonlinear Sciences::Pattern Formation and SolitonsPhysical Review X
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The Large-Scale Structure in the Universe: From Power Laws to Acoustic Peaks

2008

The most popular tools for analysing the large scale distribution of galaxies are second-order spatial statistics such as the two-point correlation function or its Fourier transform, the power spectrum. In this review, we explain how our knowledge of cosmic structures, encapsulated by these statistical descriptors, has evolved since their first use when applied on the early galaxy catalogues to the present generation of wide and deep redshift surveys, incorporating the most challenging discovery in the study of the galaxy distribution: the detection of Baryon Acoustic Oscillations.

PhysicsCOSMIC cancer databaseScale (ratio)Spectral densityAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsBaryon acoustic oscillationsCorrelation function (astronomy)Power lawAstrophysics::Galaxy AstrophysicsGalaxyRedshift
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Bloch oscillations in Fermi gases

2003

The possibility of Bloch oscillations for a degenerate and superfluid Fermi gas of atoms in an optical lattice is considered. For a one-component degenerate gas the oscillations are suppressed for high temperatures and band fillings. For a two-component gas the Landau criterion is used for specifying the regime where Bloch oscillations of the superfluid may be observed. We show how the amplitude of Bloch oscillations varies along the BCS-BEC crossover.

PhysicsCondensed Matter::Quantum GasesOptical latticeCondensed matter physicsCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed Matter::OtherDegenerate energy levelsQuantum oscillationsFOS: Physical sciencesAtomic and Molecular Physics and Opticslaw.inventionSuperfluiditylawQuantum electrodynamicsMesoscale and Nanoscale Physics (cond-mat.mes-hall)Bloch oscillationsFermi gasBose–Einstein condensateBloch wave
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Evidence of charge-carrier compensation effects inLa0.67Ca0.33MnO3

1998

We report on detailed Hall-effect measurements of thin films of ${\mathrm{La}}_{0.67}{\mathrm{Ca}}_{0.33}{\mathrm{MnO}}_{3}$ above and below the metal-insulator transition. In the metallic ferromagnetic regime, we find a temperature-independent holelike nominal charge-carrier density ${n}_{h}^{*}=1.3$ per unit cell, consistent with a partly compensated Fermi surface. The mobility is only 92 ${\mathrm{mm}}^{2}/\mathrm{V}\mathrm{}\mathrm{s}$ at 4 K, and decreases with increasing temperature. Huge negative magnetoresistivity results from an increase in mobility. In low magnetic fields or at high temperatures, an anomalous electronlike contribution dominates the Hall voltage. For possible side …

PhysicsCondensed matter physicsFerromagnetismHall effectThermal Hall effectQuantum oscillationsCondensed Matter::Strongly Correlated ElectronsCharge carrierFermi surfaceElectronMagnetic fieldPhysical Review B
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