Search results for " statistical"

showing 10 items of 1649 documents

Community Turnover of Wood-Inhabiting Fungi across Hierarchical Spatial Scales

2014

For efficient use of conservation resources it is important to determine how species diversity changes across spatial scales. In many poorly known species groups little is known about at which spatial scales the conservation efforts should be focused. Here we examined how the community turnover of wood-inhabiting fungi is realised at three hierarchical levels, and how much of community variation is explained by variation in resource composition and spatial proximity. The hierarchical study design consisted of management type (fixed factor), forest site (random factor, nested within management type) and study plots (randomly placed plots within each study site). To examine how species richne…

Conservation geneticsBiodiversityBeta diversityhabitatlcsh:MedicineForestseastern deciduous forestsfragmentationhabitat structureSpatial and Landscape Ecologyspecies richnesslcsh:SciencebiodiversityConservation ScienceMultidisciplinaryEcologyEcologymetsänkäsittelyconservationForestryBiodiversityTerrestrial EnvironmentsWoodHabitatCommunity Ecology1181 Ecology evolutionary biologyfungal communityTemperate ForestsmanagementResearch ArticleConservation of Natural Resourcesbeta-diversityForest EcologyeducationRare speciesMycologyBiologypopulation distributionModels Biologicaleliömaantiedeplan-species diversityPLANT-SPECIES DIVERSITYForest ecologyCommunity Structure1172 Environmental sciencesdead woodnonhumanModels Statisticalspecies diversitylcsh:REcology and Environmental SciencesFungiSpecies diversityBiology and Life Sciencesympäristönsuojelulandscape15. Life on landbiodiversiteettita1181species distributionlcsh:QSpecies richnessPLoS ONE
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Automatic regrouping of strata in the goodness-of-fit chi-square test

2019

Pearson’s chi-square test is widely employed in social and health sciences to analyze categorical data and contingency tables. For the test to be valid, the sample size must be large enough to provide a minimum number of expected elements per category. This paper develops functions for regrouping strata automatically no matter where they are located, thus enabling the goodness-of-fit test to be performed within an iterative procedure. The functions are written in Excel VBA (Visual Basic for Applications) and in Mathematica. The usefulness and performance of these functions is illustrated by means of a simulation study and the application to different datasets. Finally, the iterative use of …

Contingency tableComputer scienceContinuous Sample of Working Lives62G10 62P25MathematicaSample (statistics):62 Statistics::62P Applications [Classificació AMS]Visual Basic for ApplicationsEconomiaTest (assessment):62 Statistics::62G Nonparametric inference [Classificació AMS]Goodness of fitFinancesSample size determination:Matemàtiques i estadística::Estadística matemàtica [Àrees temàtiques de la UPC]StatisticsVisual Basic for ApplicationsChi-square testGoodness-of-fit chi-square test statistical software Visual Basic for Applications Mathematica Continuous Sample of Working Livesstatistical softwareGoodness-of-fit chi-square testEconometríaCategorical variable
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Efficient simulation of the random-cluster model

2013

The simulation of spin models close to critical points of continuous phase transitions is heavily impeded by the occurrence of critical slowing down. A number of cluster algorithms, usually based on the Fortuin-Kasteleyn representation of the Potts model, and suitable generalizations for continuous-spin models have been used to increase simulation efficiency. The first algorithm making use of this representation, suggested by Sweeny in 1983, has not found widespread adoption due to problems in its implementation. However, it has been recently shown that it is indeed more efficient in reducing critical slowing down than the more well-known algorithm due to Swendsen and Wang. Here, we present…

Continuous phase modulationRandom clusterStatistical Mechanics (cond-mat.stat-mech)Critical phenomenaMonte Carlo methodHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesComputational Physics (physics.comp-ph)CombinatoricsHigh Energy Physics - LatticeCluster (physics)Representation (mathematics)Physics - Computational PhysicsAlgorithmCondensed Matter - Statistical MechanicsMathematicsPotts model
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Role of conditional probability in multiscale stationary markovian processes.

2010

The aim of the paper is to understand how the inclusion of more and more time-scales into a stochastic stationary Markovian process affects its conditional probability. To this end, we consider two Gaussian processes: (i) a short-range correlated process with an infinite set of time-scales bounded from below, and (ii) a power-law correlated process with an infinite and unbounded set of time-scales. For these processes we investigate the equal position conditional probability P(x,t|x,0) and the mean First Passage Time T(L). The function P(x,t|x,0) can be considered as a proxy of the persistence, i.e. the fact that when a process reaches a position x then it spends some time around that posit…

Continuous-time stochastic processPure mathematicsStationary processStationary distributionStatistical Mechanics (cond-mat.stat-mech)Stochastic processStochastic ProcesseFokker-Plank EquationFOS: Physical sciencesOrnstein–Uhlenbeck processConditional probability distributionSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)CombinatoricsStable processPhysics - Data Analysis Statistics and ProbabilityMarkovian processeFirst-hitting-time modelCondensed Matter - Statistical MechanicsData Analysis Statistics and Probability (physics.data-an)MathematicsPhysical review. E, Statistical, nonlinear, and soft matter physics
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Wavelet analysis of baryon acoustic structures in the galaxy distribution

2011

Baryon Acoustic Oscillations (BAO) are a feature imprinted in the density field by acoustic waves travelling in the plasma of the early universe. Their fixed scale can be used as a standard ruler to study the geometry of the universe. BAO have been previously detected using correlation functions and power spectra of the galaxy distribution. In this work, we present a new method for the detection of the real-space structures associated with this feature. These baryon acoustic structures are spherical shells with a relatively small density contrast, surrounding high density central regions. We design a specific wavelet adapted to the search for shells, and exploit the physics of the process b…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark mattermedia_common.quotation_subjectFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences0103 physical sciencesDensity contrast010303 astronomy & astrophysicsmedia_commonPhysicsmethods: statistical[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsgalaxies: cluster: generalAstronomy and AstrophysicsAcoustic wavecosmology: distance scalecosmology: large-scale structure of Universemethods: data analysisUniverseGalaxyBaryonSpace and Planetary ScienceBaryon acoustic oscillationsAstrophysics - Cosmology and Nongalactic Astrophysics
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Euclid preparation XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis

2022

The combination and cross-correlation of the upcoming $Euclid$ data with cosmic microwave background (CMB) measurements is a source of great expectation since it will provide the largest lever arm of epochs, ranging from recombination to structure formation across the entire past light cone. In this work, we present forecasts for the joint analysis of $Euclid$ and CMB data on the cosmological parameters of the standard cosmological model and some of its extensions. This work expands and complements the recently published forecasts based on $Euclid$-specific probes, namely galaxy clustering, weak lensing, and their cross-correlation. With some assumptions on the specifications of current and…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundstatistical [methods]FOS: Physical sciencesAstrophysicscosmic background radiationAstrophysics::Cosmology and Extragalactic AstrophysicsJoint analysiskosmologia01 natural sciencesmethodsNOpimeä aine[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]mikroaallotSettore FIS/05 - Astronomia e Astrofisicasurveys0103 physical sciencestszsurvey010303 astronomy & astrophysicsPhysicsmethods: statistical010308 nuclear & particles physicsComputer Science::Information RetrievalmaailmankaikkeusAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicscross-correlation115 Astronomy Space scienceCosmic background radiation; Large-scale structure of Universe; Methods: statistical; Surveyskosminen taustasäteilySpace and Planetary Sciencemethodlarge-scale structure of Universepimeä energia[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statisticalAstrophysics - Cosmology and Nongalactic Astrophysics
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Morphostatistical characterization of the spatial galaxy distribution through Gibbs point processes

2021

This paper proposes a morpho-statistical characterisation of the galaxy distribution through spatial statistical modelling based on inhomogeneous Gibbs point processes. The galaxy distribution is supposed to exhibit two components. The first one is related to the major geometrical features exhibited by the observed galaxy field, here, its corresponding filamentary pattern. The second one is related to the interactions exhibited by the galaxies. Gibbs point processes are statistical models able to integrate these two aspects in a probability density, controlled by some parameters. Several such models are fitted to real observational data via the ABC Shadow algorithm. This algorithm provides …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)InferenceFOS: Physical sciencesProbability density functionAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesPoint processmethods: numerical010104 statistics & probability0103 physical sciencesStatistical physics0101 mathematics010303 astronomy & astrophysicscataloguesgalaxies: statisticsPhysics[STAT.AP]Statistics [stat]/Applications [stat.AP]methods: statisticalEstimation theoryAstronomy and AstrophysicsStatistical modelmethods: data analysisField (geography)GalaxyDistribution (mathematics)Space and Planetary Sciencelarge-scale structure of Universe[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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A search for light dark matter in XENON10 data

2011

We report results of a search for light (3.5x10^{-42} cm^2, for a dark matter particle mass m_{\chi}=8 GeV. We find that our data strongly constrain recent elastic dark matter interpretations of excess low-energy events observed by CoGeNT and CRESST-II, as well as the DAMA annual modulation signal.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)LightDark matterGeneral Physics and AstronomyFOS: Physical sciencesElectronsElementary particleElectron01 natural sciencesParticle detectorHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHumansScattering Radiation010306 general physicsLight dark matterNuclear PhysicsPhysicsPhotons010308 nuclear & particles physicsScatteringFermionBaryonHigh Energy Physics - PhenomenologyData Interpretation StatisticalCosmic RadiationAstrophysics - Cosmology and Nongalactic Astrophysics
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Pattern formation and spatial correlation induced by the noise in two competing species

2004

We analyze the spatio-temporal patterns of two competing species in the presence of two white noise sources: an additive noise acting on the interaction parameter and a multiplicative noise which affects directly the dynamics of the species densities. We use a coupled map lattice (CML) with uniform initial conditions. We find a nonmonotonic behavior both of the pattern formation and the density correlation as a function of the multiplicative noise intensity.

Coupled Map LatticeSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciStatistical Mechanics (cond-mat.stat-mech)Noise-induced pattern formationMultiplicative noiseFOS: Physical sciencesCoupled Map Lattice; Multiplicative noise; Noise-induced pattern formation; Competing speciesCompeting speciesCondensed Matter - Statistical Mechanics
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Nonmonotonic behavior of spatiotemporal pattern formation in a noisy Lotka-Volterra system

2004

The noise-induced pattern formation in a population dynamical model of three interacting species in the coexistence regime is investigated. A coupled map lattice of Lotka-Volterra equations in the presence of multiplicative noise is used to analyze the spatiotemporal evolution. The spatial correlation of the species concentration as a function of time and of the noise intensity is investigated. A nonmonotonic behavior of the area of the patterns as a function of both noise intensity and evolution time is found.

Coupled Map LatticeSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciStatistical Mechanics (cond-mat.stat-mech)Noise-induced pattern formationMultiplicative noiseQuantitative Biology::Populations and EvolutionFOS: Physical sciencesInteracting speciesCoupled Map Lattice; Multiplicative noise; Noise-induced pattern formation; Interacting speciesCondensed Matter - Statistical Mechanics
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