Search results for "Recession"

showing 10 items of 250 documents

Proposal for a Cosmic Axion Spin Precession Experiment (CASPEr)

2014

We propose an experiment to search for QCD axion and axionlike-particle dark matter. Nuclei that are interacting with the background axion dark matter acquire time-varying CP-odd nuclear moments such as an electric dipole moment. In analogy with nuclear magnetic resonance, these moments cause precession of nuclear spins in a material sample in the presence of an electric field. Precision magnetometry can be used to search for such precession. An initial phase of this experiment could cover many orders of magnitude in axionlike-particle parameter space beyond the current astrophysical and laboratory limits. And with established techniques, the proposed experimental scheme has sensitivity to …

PhysicsParticle physicsCOSMIC cancer database010308 nuclear & particles physicsPhysicsQC1-999Dark matterGeneral Physics and Astronomy7. Clean energy01 natural sciencesElectric field0103 physical sciencesPrecession010306 general physicsSpin (physics)AxionBosonPhysical Review X
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A non-resonant dark-side solution to the solar neutrino problem

2001

We re-analyse spin-flavour precession solutions to the solar neutrino problem in the light of the recent SNO CC result as well as the 1258--day Super-Kamiokande data and the upper limit on solar anti-neutrinos. In a self-consistent magneto-hydrodynamics approach the resulting scheme has only 3 effective parameters: $\Delta m^2$, $\mu B_\perp$ and the neutrino mixing angle $\theta$. We show how a rates-only analysis for fixed $\mu B_\perp$ slightly favours spin-flavour precession (SFP) solutions over oscillations (OSC). In addition to the resonant solution (RSFP for short), there is a new non-resonant solution (NRSFP) in the ``dark-side''. Both RSFP and NRSFP lead to flat recoil energy spect…

PhysicsParticle physicsNuclear and High Energy PhysicsNeutrino mass and mixingCosmologiaMagnetic momentNeutrino oscillationsSolar neutrinosHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemSpectral linePartícules (Física nuclear)Magnetic fieldBohr magnetonNeutrino magnetic momentsymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)symbolsPrecessionHigh Energy Physics::ExperimentNeutrinoMixing (physics)
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Dynamics of anisotropic superparamagnetic particles in a precessing magnetic field.

2013

A bifurcation diagram for anisotropic magnetic particles in a precessing magnetic field is analyzed. It is found that a synchronous regime in the case of a prolate particle exists for all precession angles of the magnetic field if the frequency of field rotation is below some critical value. An oblate particle has a synchronous regime in a limited range of precession angle. To understand the flow of suspensions of these particles in precessing fields, it is essential to take into account the differing dynamics of prolate and oblate particles.

PhysicsRange (particle radiation)Nuclear magnetic resonanceField (physics)Condensed matter physicsPhysics::Space PhysicsPhysics::Atomic and Molecular ClustersPrecessionParticleMagnetic nanoparticlesRotationBifurcation diagramMagnetic fieldPhysical review. E, Statistical, nonlinear, and soft matter physics
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Cyclical behaviour and disc truncation in the Be/X-ray binary A0535+26

2003

A0535+26 is shown to display quantised IR excess flux states, which are interpreted as the first observational verification of the resonant truncation scheme proposed by Okazaki and Negueruela (2001) for BeXRBs. The simultaneity of X-ray activity with transitions between these states strongly suggests a broad mechanism for outbursts, in which material lost from the disc during the reduction of truncation radius is accreted by the NS. Furthermore changes between states are shown to be governed by a 1500 day period, probably due to precession of the Be disc, which profoundly dictates the global behaviour of the system. Such a framework appears to be applicable to BeXRBs in general.

PhysicsSimultaneitySpace and Planetary ScienceTruncationAstrophysics (astro-ph)X-ray binaryPrecessionFluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsRadiusAstrophysics
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The 35-d modulation of the X-ray emission of Her X-1 in the framework of the SOD model: results of a three-dimensional SPH simulation

1994

Several models have been proposed to explain the 35-d X-ray periodicity observed in Her X-1. We present the results of six three-dimensional quasi-polytropic smoothed particle hydrodynamics (SPH) simulations of the tilted, twisted accretion disc of Her X-1 carried out in the light of Roberts' slaved orienting disc model (SOD) with the intention of finding some limits to the inclination of the rotation axis of the secondary and to the value of the polytropic index γ. These results show that a γ value between 1.05 and 1.1 and an inclination angle φ of the order of 45° are the most suitable for enabling the SOD model to work in three-dimensional space. The simulated disc is rather small and th…

PhysicsSmoothed-particle hydrodynamicsClassical mechanicsSpace and Planetary ScienceStellar rotationBinary starPrecessionX-ray binaryAstronomy and AstrophysicsPolytropic processRotationSpace (mathematics)Computational physicsMonthly Notices of the Royal Astronomical Society
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Limit on Lorentz-Invariance- and CPT-Violating Neutron Spin Interactions Using a $^3$He-$^{129}$Xe Comagnetometer

2016

We performed a search for a Lorentz-invariance- and CPT-violating coupling of the $^3$He and $^{129}$Xe nuclear spins to posited background fields. Our experimental approach is to measure the free precession of nuclear spin polarized $^3$He and $^{129}$Xe atoms using SQUID detectors. As the laboratory reference frame rotates with respect to distant stars, we look for a sidereal modulation of the Larmor frequencies of the co-located spin samples. As a result we obtain an upper limit on the equatorial component of the background field $\tilde{b}^n_{\bot}< 8.4 \cdot 10^{-34}$ GeV (68\% C.L.). Furthermore, this technique was modified to search for an electric dipole moment (EDM) of $^{129}$X…

PhysicsSpinsField (physics)Atomic Physics (physics.atom-ph)FOS: Physical sciences02 engineering and technologyLorentz covariance021001 nanoscience & nanotechnology01 natural sciencesPhysics - Atomic PhysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Sidereal timeQuantum electrodynamics0103 physical sciencesPrecessionNeutron010306 general physics0210 nano-technologyAnisotropySpin (physics)
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Spin clocks: Probing fundamental symmetries in nature

2013

The detection of the free precession of co-located 3He/129Xe nuclear spins (clock comparison) is used as ultra-sensitive probe for non-magnetic spin interactions, since the magnetic dipole interaction (Zeeman-term) drops out in the weighted frequency difference, i.e., Δω = ωHe- γHe/γXe·ωXe of the respective Larmor frequencies. Recent results are reported on searches for (i) short-range P- and T-violating interactions between nucleons, and (ii) Lorentz violating signatures by monitoring the Larmor frequencies as the laboratory reference frame rotates with respect to distant stars (sidereal modulation). Finally, a new experimental initiative to search for an electric dipole moment of 129Xe (C…

Physicssymbols.namesakeElectric dipole momentSpinsSidereal timeLorentz transformationQuantum mechanicsPrecessionsymbolsGeneral Physics and AstronomySpin (physics)NucleonMagnetic dipoleAnnalen der Physik
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Measurement of the anomalous precession frequency of the muon in the Fermilab Muon g−2 Experiment

2021

The Muon g-2 Experiment at Fermi National Accelerator Laboratory (FNAL) has measured the muon anomalous precession frequency $\omega_a$ to an uncertainty of 434 parts per billion (ppb), statistical, and 56 ppb, systematic, with data collected in four storage ring configurations during its first physics run in 2018. When combined with a precision measurement of the magnetic field of the experiment's muon storage ring, the precession frequency measurement determines a muon magnetic anomaly of $a_{\mu}({\rm FNAL}) = 116\,592\,040(54) \times 10^{-11}$ (0.46 ppm). This article describes the multiple techniques employed in the reconstruction, analysis and fitting of the data to measure the preces…

Physics::Instrumentation and DetectorsMeasure (physics)FOS: Physical sciences7. Clean energy01 natural sciencesOmegaHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment; High Energy Physics - Experiment; Nuclear ExperimentHigh Energy Physics - Experiment (hep-ex)muon0103 physical sciencesFermilabNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentLarmor precessionPhysicsMuon010308 nuclear & particles physicsSettore FIS/01 - Fisica Sperimentaleanomalous magnetic moment3. Good healthMagnetic fieldPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentStorage ringFermi Gamma-ray Space TelescopePhysical Review
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Cyclic fluctuations, climatic changes and role of noise in planktonic foraminifera in the Mediterranean Sea

2005

The study of Planktonic Foraminifera abundances permits to obtain climatic curves on the basis of percentage ratio between tropical and temperate/polar forms. Climatic changes were controlled by several phenomena as: (i) Milankovitch's cycles, produced by variations of astronomical parameters such as precession, obliquity and eccentricity; (ii) continental geodynamic evolution and orogenic belt; (iii) variations of atmospheric and oceanic currents; (iv) volcanic eruptions; (v) meteor impacts. But while astronomical parameters have a quasi-regular periodicity, the other phenomena can be considered as "noise signal" in natural systems. The interplay between cyclical astronomical variations, t…

Planktonic foraminiferaStochastic resonanceGeneral MathematicsGeneral Physics and AstronomyAtmospheric sciencesQuantitative Biology - Quantitative MethodsPhysics::GeophysicsForaminiferaMediterranean seaGlacial periodQuantitative Biology - Populations and EvolutionPlanktonic foraminifera; Climatic changes; Stochastic resonancePhysics::Atmospheric and Oceanic PhysicsQuantitative Methods (q-bio.QM)Milankovitch cyclesbiologyOcean currentPopulations and Evolution (q-bio.PE)biology.organism_classificationSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Climatic changeOceanographyFOS: Biological sciencesInterglacialPrecessionAstrophysics::Earth and Planetary AstrophysicsGeologyStochastic resonance
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Evaluation of the effectiveness of the photobiomodulation in the treatment of dentin hypersensitivity after basic therapy. A randomized clinical trial

2016

Background: Dentin hypersensitivity (DH) in one of the most common causes of patient discomfort in the general population and its prevalence is higher in patients who have received basic or surgical periodontal treatment. Efficiency of the diode laser with different wavelengths has been studied by several authors, showing an improvement rate of the DH between 60-98%. The aim of the present study was to evaluate the effect of photobiomodulation (PBM) treatment on the reduction of DH after non surgical periodontal treatment. Material and methods: A randomized split mouth clinical trial was performed involving 30 patients (120 teeth) diagnosed with DH after scaling and root planning. Two teeth…

PopulationDentistryOdontologialaw.invention030207 dermatology & venereal diseases03 medical and health sciences0302 clinical medicineThermal stimulationClinical trialsRandomized controlled triallawmedicineeducationGeneral DentistryGingival recessioneducation.field_of_studyLàsersDentin sensitivitybusiness.industryLasers030206 dentistrymedicine.diseaseLaser:CIENCIAS MÉDICAS [UNESCO]PhotobiologyClinical trialFotobiologiaImprovement rateDentistryUNESCO::CIENCIAS MÉDICASDentin hypersensitivitymedicine.symptombusinessHipersensibilitat dentinalAssaigs clínics
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