Search results for "Model theory"

showing 10 items of 681 documents

AB Doradus C: age, spectral type, orbit, and comparison to evolutionary models

2005

We expand upon the results of Close et al. 2005 regarding the young, low-mass object AB Dor C and its role as a calibration point for theoretical tracks. We present an improved spectral reduction and a new orbital solution with two additional epochs. Our improved analysis confirms our spectral type of M8 (+/- 1) and mass of 0.090+/-0.003 solar masses for AB Dor C. Comparing the results for AB Dor C with other young, low-mass objects with dynamical masses we find a general trend where current evolutionary models tend to over-predict the temperature (or under-predict the mass) for low mass stars and brown dwarfs. Given our precision, there is a ~99% chance that the mass of AB Dor C is underes…

PhysicsSolar massHertzsprung–Russell diagramAstrophysics (astro-ph)Brown dwarfFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsType (model theory)AstrophysicsOrbitsymbols.namesakeStarsSpace and Planetary SciencesymbolsLow MassAstronomische Nachrichten
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Transient Reversible Growth and Percolation During Phase Separation

1988

Binary mixtures when quenched into the two-phase region exhibit transient percolation phenomena. These transient percolation phenomena and the underlying mechanism of transient reversible growth are investigated. In particular, one of the possible dynamical percolation lines between the dynamical spinodal and the line of macroscopic percolation is traced out. Analyzing the finite size effects with the usual scaling theory one finds exponents which seem to be inconsistent with the universality class of percolation. However, at zero temperature, where the growth is non-reversible and the transition of a sol-gel type, the exponents are consistent with those of random percolation.

PhysicsSpinodalMathematics::ProbabilityCondensed matter physicsPercolationCondensed Matter::Statistical MechanicsTransient (oscillation)Type (model theory)Renormalization groupZero temperatureScaling theoryCondensed Matter::Disordered Systems and Neural NetworksLine (formation)
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Activity, colour anomalies and temperature determination in solar-type stars

2008

PhysicsStarsAstrophysicsType (model theory)Active star
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Low-energy fixed points of random Heisenberg models

2002

The effect of quenched disorder on the low-energy and low-temperature properties of various two- and three-dimensional Heisenberg models is studied by a numerical strong disorder renormalization group method. For strong enough disorder we have identified two relevant fixed points, in which the gap exponent, omega, describing the low-energy tail of the gap distribution, P(Delta) ~ Delta^omega is independent of disorder, the strength of couplings and the value of the spin. The dynamical behavior of non-frustrated random antiferromagnetic models is controlled by a singlet-like fixed point, whereas for frustrated models the fixed point corresponds to a large spin formation and the gap exponent …

PhysicsStatistical Mechanics (cond-mat.stat-mech)Condensed matter physicsInfrared fixed pointFOS: Physical sciencesDisordered Systems and Neural Networks (cond-mat.dis-nn)Type (model theory)Fixed pointRenormalization groupCondensed Matter - Disordered Systems and Neural NetworksOmegaExponentCondensed Matter::Strongly Correlated ElectronsRandomnessCondensed Matter - Statistical MechanicsSpin-½Mathematical physics
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Higher-order correlation functions and nonlinear response functions in a gaussian trap model.

2012

The four-time correlation function of a general dynamical variable obeying Gaussian statistics is calculated for the trap model with a Gaussian density of states. It is argued that for energy-independent variables this function is reminiscent of the four-time functions that have been discussed earlier in the interpretation of the results of four-dimensional NMR experiments on supercooled liquids. Using an approximative relation between the four-time correlation function and the cubic response function the nonlinear susceptibility is calculated and the results are compared with the corresponding ones resulting from an exact calculation. It is found that the results of the approximation chang…

PhysicsStatistical Mechanics (cond-mat.stat-mech)GaussianFOS: Physical sciencesGeneral Physics and AstronomyModulusDisordered Systems and Neural Networks (cond-mat.dis-nn)Function (mathematics)Condensed Matter - Disordered Systems and Neural NetworksInterpretation (model theory)Trap (computing)Nonlinear systemsymbols.namesakeCorrelation function (statistical mechanics)symbolsStatistical physicsPhysical and Theoretical ChemistryCondensed Matter - Statistical MechanicsVariable (mathematics)The Journal of chemical physics
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Sterile Neutrinos with Secret Interactions -- Cosmological Discord?

2018

Several long-standing anomalies from short-baseline neutrino oscillation experiments -- most recently corroborated by new data from MiniBooNE -- have led to the hypothesis that extra, 'sterile', neutrino species might exist. Models of this type face severe cosmological constraints, and several ideas have been proposed to avoid these constraints. Among the most widely discussed ones are models with so-called 'secret interactions' in the neutrino sector. In these models, sterile neutrinos are hypothesized to couple to a new interaction, which dynamically suppresses their production in the early Universe through finite-temperature effects. Recently, it has been argued that the original calcula…

PhysicsSterile neutrinoParticle physics010308 nuclear & particles physicsmedia_common.quotation_subjectHigh Energy Physics::PhenomenologyFOS: Physical scienceshep-phAstronomy and AstrophysicsParameter spaceType (model theory)01 natural sciencesUniverseCosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationParticle Physics - Phenomenologymedia_common
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Future CEvNS experiments as probes of lepton unitarity and light-sterile neutrinos

2020

We determine the sensitivities of short-baseline coherent elastic neutrino-nucleus scattering (CE$\nu$NS) experiments using a pion decay at rest neutrino source as a probe for nonunitarity in the lepton sector, as expected in low-scale type-I seesaw schemes. We also identify the best configuration for probing light sterile neutrinos at future ton-scale liquid argon CE$\nu$NS experiments, estimating the projected sensitivities on the sterile neutrino parameters. Possible experimental setups at the Spallation Neutron Source, Lujan facility and the European Spallation Source are discussed. Provided that systematic uncertainties remain under control, we find that CE$\nu$NS experiments will be c…

PhysicsSterile neutrinoParticle physicsUnitarity010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyFOS: Physical sciencesType (model theory)01 natural sciencesHigh Energy Physics - PhenomenologyPionHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsSpallation Neutron SourceLepton
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Momentum-space structure of surface states in a topological semimetal with a nexus point of Dirac lines

2016

Three-dimensional topological semimetals come in different variants, either containing Weyl points or Dirac lines. Here we describe a more complicated momentum-space topological defect where several separate Dirac lines connect with each other, forming a momentum-space equivalent of the real-space nexus considered before for helium-3. Close to the nexus the Dirac lines exhibit a transition from type I to type II lines. We consider a general model of stacked honeycomb lattices with the symmetry of Bernal (AB) stacked graphite and show that the structural mirror symmetries in such systems protect the presence of the Dirac lines, and also naturally lead to the formation of the nexus. By the bu…

PhysicsSurface (mathematics)topological semimetalsDirac linesCondensed Matter - Mesoscale and Nanoscale Physicsta114Dirac (software)Honeycomb (geometry)FOS: Physical sciencesPosition and momentum space02 engineering and technologyType (model theory)021001 nanoscience & nanotechnologyTopology01 natural sciencesSymmetry (physics)Topological defectQuantum mechanics0103 physical sciencesHomogeneous spaceMesoscale and Nanoscale Physics (cond-mat.mes-hall)010306 general physics0210 nano-technologyPhysical Review B
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Analysis and calibration of absorptive images of Bose-Einstein condensate at non-zero temperatures

2008

We describe the method allowing quantitative interpretation of absorptive images of mixtures of BEC and thermal atoms which reduces possible systematic errors associated with evaluation of the contribution of each fraction. By using known temperature dependence of the BEC fraction, the analysis allows precise calibration of the fitting results. The developed method is verified in two different measurements and compares well with theoretical calculations and with measurements performed by another group.

PhysicsSystematic errorCondensed Matter::Quantum GasesZero (complex analysis)FOS: Physical sciencesInterpretation (model theory)Computational physicslaw.inventionCondensed Matter - Other Condensed MatterlawThermalCalibrationFraction (mathematics)InstrumentationBose–Einstein condensateOther Condensed Matter (cond-mat.other)
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COHERENT constraints after the COHERENT-2020 quenching factor measurement

2020

Recently an improved quenching factor (QF) measurement for low-energy nuclear recoils in CsI[Na] has been reported by the COHERENT Collaboration. The new energy-dependent QF is characterized by a reduced systematic uncertainty and leads to a better agreement between the experimental COHERENT data and the Standard Model (SM) expectation. In this work, we report updated constraints on parameters that describe the process of coherent elastic neutrino-nucleus scattering within and beyond the SM, and we also present how the new QF affects their interpretation.

PhysicsSystematic errorQuenchingWork (thermodynamics)010308 nuclear & particles physicsScatteringFOS: Physical sciences01 natural sciencesInterpretation (model theory)Standard ModelComputational physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physics
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