Search results for "probability"

showing 10 items of 3417 documents

On the measured lifetime of light hypernuclei 3ΛH and 4ΛH

2014

A statistical combination of the experimental lifetime estimations available in the literatures is performed for 3 Λ H and 4 Λ H, including several recent measurements. The combined average values of the lifetime for 3 Λ H and 4 Λ H are respectively 216−16+19 ps and 192−18+20 ps with a reduced χ2 of 0.89 and 0.48. A new insight into the lifetime estimation of the HypHI Phase 0 experiment by a Bayesian approach is also presented. In this approach, several different prior distributions including the combination of previous lifetime data and a Jeffrey prior are used. The principal mode and the smallest credible interval at 68% of the posterior distribution, given by the prior belief of the pre…

PhysicsNuclear physicsNuclear and High Energy PhysicsLifetime measurementPosterior probabilityHypernucleiBayesian approachCredible intervalddc:530LambdaHypertritonAveraged combinationPhysics Letters B
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Near threshold photoproduction of eta mesons off the proton.

1995

We have measured precise total and differential cross sections for the reaction $\ensuremath{\gamma}p\ensuremath{\rightarrow}p\ensuremath{\eta}$ from threshold to 790 MeV at the MAMI accelerator in Mainz with the neutral meson spectrometer TAPS. Resonance parameters of the ${S}_{11}$(1535) resonance and the electromagnetic coupling $\ensuremath{\gamma}p\ensuremath{\rightarrow}{S}_{11}$ have been extracted from the data. Contributions from the ${D}_{13}$(1520) resonance to $\ensuremath{\eta}$ photoproduction in the threshold region have been identified for the first time via interference terms in the angular distributions.

PhysicsNuclear physicsParticle physicsNear thresholdAngular distributionProtonMesonGeneral Physics and AstronomyResonanceElectromagnetic couplingNuclear ExperimentCoupling (probability)Physical review letters
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Structure of the As, Ge, Ga nuclei

2012

Abstract The level structures of the N = 50 83As, 82Ge, and 81Ga isotones have been investigated by means of multi-nucleon transfer reactions. A first experiment was performed with the CLARA–PRISMA setup to identify these nuclei. A second experiment was carried out with the GASP array in order to deduce the γ-ray coincidence information. The results obtained on the high-spin states of such nuclei are used to test the stability of the N = 50 shell closure in the region of 78Ni ( Z = 28 ). The comparison of the experimental level schemes with the shell-model calculations yields an N = 50 energy gap value of 4.7(3) MeV at Z = 28 . This value, in a good agreement with the prediction of the fini…

PhysicsNuclear reactionNuclear and High Energy Physics010308 nuclear & particles physicsBand gapNuclear TheorySHELL modelShell (structure)Structure (category theory)01 natural sciencesStability (probability)Coincidence0103 physical sciencesOrder (group theory)Atomic physics010306 general physicsNuclear Physics A
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Proton distortion effects and meson exchange current contributions in the (e,e′p) reaction

1988

It is demonstrated that proton distortion effects could explain the relative enhancement of transverse to longitudinal response in the recent ($e,{e}^{\ensuremath{'}}p$) reactions on $^{12}\mathrm{C}$. The spin-orbit field is essential to bring about this enhancement. The role of the convection current is pointed out. Favorable contributions from pion-pair and isobar-excitation currents are also found.

PhysicsNuclear reactionNuclear and High Energy PhysicsMesonProtonNuclear TheoryHadronElementary particleCoupling (probability)Nuclear physicsBaryonAtomic physicsNuclear ExperimentNucleonPhysical Review C
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Joint constraints on galaxy bias and σ8 through the N-pdf of the galaxy number density

2015

We present a full description of the N-probability density function of the galaxy number density fluctuations. This N-pdf is given in terms, on the one hand, of the cold dark matter correlations and, on the other hand, of the galaxy bias parameter. The method relies on the assumption commonly adopted that the dark matter density fluctuations follow a local non-linear transformation of the initial energy density perturbations. The N-pdf of the galaxy number density fluctuations allows for an optimal estimation of the bias parameter (e.g., via maximum-likelihood estimation, or Bayesian inference if there exists any a priori information on the bias parameter), and of those parameters defining …

PhysicsNumber densityCold dark matter010308 nuclear & particles physicsModel selectionDark matterEstimatorAstronomy and AstrophysicsProbability density functionAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy0103 physical sciencesStatistical physics010303 astronomy & astrophysicsGalaxy clusterAstrophysics - Cosmology and Nongalactic Astrophysics
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Brownian dynamics simulations with hard-body interactions: Spherical particles

2012

A novel approach to account for hard-body interactions in (overdamped) Brownian dynamics simulations is proposed for systems with non-vanishing force fields. The scheme exploits the analytically known transition probability for a Brownian particle on a one-dimensional half-line. The motion of a Brownian particle is decomposed into a component that is affected by hard-body interactions and into components that are unaffected. The hard-body interactions are incorporated by replacing the affected component of motion by the evolution on a half-line. It is discussed under which circumstances this approach is justified. In particular, the algorithm is developed and formulated for systems with spa…

PhysicsNumerical analysisFOS: Physical sciencesGeneral Physics and AstronomyProteinsComputational Physics (physics.comp-ph)Condensed Matter - Soft Condensed MatterModels BiologicalDiffusionMotionProbability theoryModels ChemicalProtein Interaction MappingBrownian dynamicsSoft Condensed Matter (cond-mat.soft)Computer SimulationStatistical physicsColloidsPhysical and Theoretical ChemistryPhysics - Computational PhysicsBrownian motionAlgorithms
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Generation and detection of optical rogue-wave-like fluctuations in fiber Raman amplifiers

2009

Rogue wave-like statistics is reported in a fiber Raman amplifier. The pump-signal noise transfer leads to the development of large peak-power fluctuations following a powerlaw probability distribution. Discrimination of the rarest events is demonstrated.

PhysicsOptical fiberbusiness.industryPhysics::OpticsNonlinear opticsNoise (electronics)law.inventionOptical pumpingOpticslawOptoelectronicsProbability distributionStimulated emissionFiberRogue wavebusiness2009 IEEE/LEOS Winter Topicals Meeting Series
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Periodic Motion for an Imperfect Solar Sail Near an Asteroid

2014

In this paper we consider the Hill 3-body problem with the extra effect of the solar radiation pressure as a model for the motion of a solar sail close to an asteroid. To model the sail’s acceleration, we include both reflectivity and absorption of the sail’s material. We describe the most relevant dynamical properties of the system for different reflectivity and absorption coefficients as well as different fixed sail orientations. We show families of periodic orbits, describe how they relate to the parameters of the sail and discuss their stability.

PhysicsOrbital planeAstronomySolar sailMechanicsQuantitative Biology::OtherStability (probability)Periodic functionPhysics::Popular PhysicsAccelerationRadiation pressureAsteroidPhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsAbsorption (electromagnetic radiation)
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Neutrino anarchy and renormalization group evolution

2015

The observed pattern of neutrino mixing angles is in good agreement with the hypothesis of neutrino anarchy, which posits that Nature has chosen the entries of the leptonic mixing matrix at random. In this paper we investigate how stable this conclusion is under renormalization group effects. Working in the simplest type-I seesaw model and two variants of the inverse seesaw model we study how the statistical distributions of the neutrino mixing parameters evolve between the Grand Unification scale and the electroweak scale. Especially in the inverse seesaw case we find significant distortions: mixing angles tend to be smaller after RG running, and the Dirac CP phase tends to be closer to ze…

PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyInverseFOS: Physical sciencesRenormalization group01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesProbability distributionGrand Unified TheoryNeutrinoElectroweak scale010306 general physicsPhysical Review D
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Light-by-light forward scattering sum rules for charmonium states

2017

We apply three forward light-by-light scattering sum rules to charmonium states. We show that these sum rules imply a cancellation between charmonium bound state contributions, which are mostly known from the $\gamma \gamma$ decay widths of these states, and continuum contributions above $D \bar D$ threshold, for which we provide a duality estimate. We also show that two of these sum rules allow to predict the yet unmeasured $\gamma^\ast \gamma$ coupling of the $\chi_{c1}(1P)$ state, which can be tested at present high-luminosity $e^+ e^-$ colliders.

PhysicsParticle physics010308 nuclear & particles physicsScatteringAstrophysics::High Energy Astrophysical PhenomenaQuark modelDuality (optimization)FOS: Physical sciencesState (functional analysis)Coupling (probability)01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBound stateHigh Energy Physics::ExperimentContinuum (set theory)Sum rule in quantum mechanics010306 general physics
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