Search results for " Oscillation"

showing 10 items of 845 documents

Simulation and experimental investigations on dynamic after cavity interaction (ACI)

2010

In recent years, the so called after cavity interaction (ACI) in high power gyrotrons operating in the 100–200 GHz range gained attention as an influence factor on overall efficiency. While investigations concentrated on ACI as a stationary effect until now, recent simulations show that an undesired interaction in the uptaper region can also result in additional parasitic oscillations. In this paper, such non-stationary, dynamic processes are investigated in first simulations and experiments.

PhysicsInfluence factorModulationTerahertz radiationParasitic oscillationMechanicsOverall efficiencyPower (physics)35th International Conference on Infrared, Millimeter, and Terahertz Waves
researchProduct

On the observability of Bell's inequality violation in the two-atoms optical Stern-Gerlach model

2005

Using the optical Stern-Gerlach model, we have recently shown that the non-local correlations between the internal variables of two atoms that successively interact with the field of an ideal cavity in proximity of a nodal region are affected by the atomic translational dynamics. As a consequence, there can be some difficulties in observing violation of the Bell's inequality for the atomic internal variables. These difficulties persist even if the atoms travel an antinodal region, except when the spatial wave packets are exactly centered in an antinodal point.

PhysicsMECHANICAL DESCRIPTIONTRANSLATIONAL DYNAMICSStern–Gerlach experimentIdeal (set theory)Field (physics)InequalityWave packetmedia_common.quotation_subjectDETERMINISTIC QUANTUM TELEPORTATIONCOMPLEMENTARITYAtomic and Molecular Physics and OpticsRABI OSCILLATIONSATOMSSCALAR PRODUCTHILBERT-SPACEQuantum mechanicsPhysics::Atomic and Molecular ClustersInternal variablePoint (geometry)Physics::Atomic PhysicsObservabilityPHYSICAL REALITYINTERFEROMETERmedia_common
researchProduct

Effect of coronal loop structure on wave heating through phase mixing

2020

Context. The mechanism(s) behind coronal heating still elude(s) direct observation and modelling of viable theoretical processes and the subsequent effect on coronal structures is one of the key tools available to assess possible heating mechanisms. Wave heating via the phase mixing of magnetohydrodynamic (MHD) transverse waves has been proposed as a possible way to convert magnetic energy into thermal energy, but MHD models increasingly suggest this is not an efficient enough mechanism. Aims. We modelled heating by phase mixing transverse MHD waves in various configurations in order to investigate whether certain circumstances can enhance the heating sufficiently to sustain the million deg…

PhysicsMagnetohydrodynamics (MHD)Magnetic energySun: corona010308 nuclear & particles physicsF300Astronomy and AstrophysicsTransverse waveAstrophysicsCoronal loopMechanicsF500Dissipation01 natural sciencesTransverse planeSpace and Planetary Science0103 physical sciencesPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamic driveBoundary value problemSun: oscillationsMagnetohydrodynamics010303 astronomy & astrophysicsSun: atmosphere
researchProduct

Observables sensitive to absolute neutrino masses. II

2008

In this followup to Phys. Rev. D 75, 053001 (2007) [arXiv:hep-ph/0608060] we report updated constraints on neutrino mass-mixing parameters, in light of recent neutrino oscillation data (KamLAND, SNO, and MINOS) and cosmological observations (WMAP 5-year and other data). We discuss their interplay with the final 0nu2beta decay results in 76-Ge claimed by part of the Heidelberg-Moscow Collaboration, using recent evaluations of the corresponding nuclear matrix elements, and their uncertainties. We also comment on the 0nu2beta limits in 130-Te recently set by Cuoricino, and on prospective limits or signals from the KATRIN experiment.

PhysicsMass numberNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics (astro-ph)Cosmic background radiationFOS: Physical sciencesAstrophysicsCMB cold spotHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)MINOSDouble beta decayHigh Energy Physics::ExperimentSensitivity (control systems)Nuclear Experiment (nucl-ex)NeutrinoNeutrino oscillationNuclear ExperimentPhysical Review D
researchProduct

Status of neutrino oscillations 2018: 3 hint for normal mass ordering and improved CP sensitivity

2018

We present a new global fit of neutrino oscillation parameters within the simplest three-neutrino picture, including new data which appeared since our previous analysis [1]. In this update we include new long-baseline neutrino data involving the antineutrino channel in T2K, as well as new data in the neutrino channel, data from NOνA, as well as new reactor data, such as the Daya Bay 1230 days electron antineutrino disappearance spectrum data and the 1500 live days prompt spectrum from RENO, as well as new Double Chooz data. We also include atmospheric neutrino data from the IceCube DeepCore and ANTARES neutrino telescopes and from Super-Kamiokande. Finally, we also update our solar oscillat…

PhysicsNOνANuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsOscillationAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyCHOOZ01 natural scienceslcsh:QC1-999Neutrino detector0103 physical sciencesCP violationHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationElectron neutrinolcsh:PhysicsPhysics Letters
researchProduct

Gravitational waves in dynamical spacetimes with matter content in the fully constrained formulation

2012

The Fully Constrained Formulation (FCF) of General Relativity is a novel framework introduced as an alternative to the hyperbolic formulations traditionally used in numerical relativity. The FCF equations form a hybrid elliptic-hyperbolic system of equations including explicitly the constraints. We present an implicit-explicit numerical algorithm to solve the hyperbolic part, whereas the elliptic sector shares the form and properties with the well known Conformally Flat Condition (CFC) approximation. We show the stability andconvergence properties of the numerical scheme with numerical simulations of vacuum solutions. We have performed the first numerical evolutions of the coupled system of…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsGeneral relativityGravitational waveRotational symmetryFOS: Physical sciencesSpherical coordinate systemGeneral Relativity and Quantum Cosmology (gr-qc)Neutron-star oscillationSystem of linear equations01 natural sciencesGeneral Relativity and Quantum CosmologyNeutron starNumerical relativityClassical mechanicsAstrophysics - Solar and Stellar Astrophysics0103 physical sciences010306 general physicsSolar and Stellar Astrophysics (astro-ph.SR)Physical Review D
researchProduct

Neutrino oscillation probabilities through the looking glass

2019

In this paper we review different expansions for neutrino oscillation probabilities in matter in the context of long-baseline neutrino experiments. We examine the accuracy and computational efficiency of different exact and approximate expressions. We find that many of the expressions used in the literature are not precise enough for the next generation of long-baseline experiments, but several of them are while maintaining comparable simplicity. The results of this paper can be used as guidance to both phenomenologists and experimentalists when implementing the various oscillation expressions into their analysis tools.

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsOscillationmedia_common.quotation_subjectFOS: Physical sciencesContext (language use)01 natural scienceslcsh:QC1-999Theoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesSimplicityAnalysis toolsNeutrino010306 general physicsNeutrino oscillationlcsh:Physicsmedia_common
researchProduct

Reactor antineutrino detection in Double Chooz experiment: Techniques for background reduction

2014

Abstract A crucial task for the Double Chooz reactor antineutrino experiment is the thorough study of the different backgrounds in the detector. Newly developed background reduction techniques minimize the impact of the backgrounds on our sensitivity. Moreover, only a precision and accuracy measurement of the residual background would allow to measure the mixing angle θ 13 with high precision. Neutrino coincidence signals are imitated by signals produced in several others physics processes: accidental coincidences of single events (accidental background), as well as correlated events induced by cosmic muons, including stopping muons, fast neutrons and spallation isotopes Li 9 /He 8 . The Do…

PhysicsNuclear and High Energy PhysicsAccuracy and precisionParticle physicsMuon010308 nuclear & particles physicsCHOOZ[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesNeutron temperatureCoincidenceNuclear physics13. Climate action0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SpallationNeutrino010306 general physicsNeutrino oscillationComputingMilieux_MISCELLANEOUSbackground neutrino oscillation θ13 reactor
researchProduct

Neutrinoless double electron capture as a tool to measure the electron neutrino mass

1983

Abstract A nucleus (Z, A) may capture two atomic electrons to become (Z − 2, A). For Majorana neutrinos this may occur with no neutrino emission, the process is a virtual mixing of the parent atom and the daughter atom with two electron holes. The process becomes real as the daughter atom de-excites. In some cases where the daughter nucleus is excited, the neutrinoless decay may be enhanced by its proximity to a virtual resonance. We identify the 112 Sn → 112 Cd transition as a good case. The no-neutrino lifetime for mν = 30 eV ranges from 1022 to 1027 years as a function of the insufficiently well determined distance to resonance. The signatures of the two- or no-neutrino modes are very di…

PhysicsNuclear and High Energy PhysicsElectron captureHigh Energy Physics::PhenomenologyFísicaWeak interactionNuclear physicsMAJORANAExcited stateAtomHigh Energy Physics::ExperimentAtomic physicsNeutrinoNuclear ExperimentNeutrino oscillationElectron neutrinoGeneral Theoretical PhysicsNuclear Physics B
researchProduct

Neutron Fermi liquids under the presence of a strong magnetic field with effective nuclear forces

2009

Landau's Fermi liquid parameters are calculated for non-superfluid pure neutron matter in the presence of a strong magnetic field at zero temperature. The particle-hole interactions in the system, where a net magnetization may be present, are characterized by these parameters in the framework of a multipolar formalism. We use either zero- or finite-range effective nuclear forces to describe the nuclear interaction. Using the obtained Fermi liquid parameters, the contribution of a strong magnetic field on some bulk magnitudes such as isothermal compressibility and spin susceptibility is also investigated.

PhysicsNuclear and High Energy PhysicsFermi contact interactionNuclear TheoryCondensed matter physicsFOS: Physical sciencesFísicaQuantum oscillationsNuclear matterNuclear Theory (nucl-th)MagnetizationNuclear forceNeutronFermi liquid theoryFermi gas
researchProduct