Search results for "Planck"

showing 10 items of 159 documents

Dynamics of two competing species in the presence of Lévy noise sources

2010

We consider a Lotka-Volterra system of two competing species subject to multiplicative alpha-stable Lévy noise. The interaction parameter between the species is a random process which obeys a stochastic differential equation with a generalized bistable potential in the presence both of a periodic driving term and an additive alpha-stable Lévy noise. We study the species dynamics, which is characterized by two different regimes, exclusion of one species and coexistence of both. We find quasi-periodic oscillations and stochastic resonance phenomenon in the dynamics of the competing species, analysing the role of the Lévy noise sources.

Competitive BehaviorComplex systemsBistabilityStochastic resonancePopulation DynamicsComplex systemModels BiologicalStochastic differential equationControl theoryQuantitative Biology::Populations and EvolutionAnimalsHumansComputer SimulationStatistical physicsEcosystemMathematicsPopulation dynamics and ecological pattern formationModels StatisticalStochastic processDynamics (mechanics)Multiplicative functionStochastic analysis methods (Fokker-Planck Langevin etc.)Adaptation PhysiologicalRandom walks and Lévy flightQuasiperiodic functionPredatory Behavior
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Non-circular rotating beams and CMB experiments

2002

This paper is concerned with small angular scale experiments for the observation of cosmic microwave background anisotropies. In the absence of beam, the effects of partial coverage and pixelisation are disentangled and analyzed (using simulations). Then, appropriate maps involving the CMB signal plus the synchrotron and dust emissions from the Milky Way are simulated, and an asymmetric beam --which turns following different strategies-- is used to smooth the simulated maps. An associated circular beam is defined to estimate the deviations in the angular power spectrum produced by beam asymmetry without rotation and, afterwards, the deviations due to beam rotation are calculated. For a cert…

Cosmic microwave background ; Cosmology theory ; Large-scale structure of the universe ; Numerical method ; Data analysis methodmedia_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciencesAstrophysicsNumerical methodUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsRotationAsymmetryCosmic microwave backgroundlaw.inventionsymbols.namesakelawCosmology theoryLarge-scale structure of the universePlanckAnisotropymedia_commonPhysicsData analysis methodAstrophysics (astro-ph)Spectral densityAstronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]SynchrotronComputational physicsSpace and Planetary SciencesymbolsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Beam (structure)Astronomy & Astrophysics
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Beam deconvolution in noisy CMB maps

2003

The subject of this paper is beam deconvolution in small angular scale CMB experiments. The beam effect is reversed using the Jacobi iterative method, which was designed to solved systems of algebraic linear equations. The beam is a non circular one which moves according to the observational strategy. A certain realistic level of Gaussian instrumental noise is assumed. The method applies to small scale CMB experiments in general (cases A and B), but we have put particular attention on Planck mission at 100 GHz (cases C and D). In cases B and D, where noise is present, deconvolution allows to correct the main beam distortion effect and recover the initial angular power spectrum up to the end…

Cosmic microwave backgroundData analysisJacobi methodFOS: Physical sciencesAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICACosmic microwave backgroundsymbols.namesakeDistortionPlanckPhysicsNumericalAstrophysics (astro-ph)Spectral densityAstronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Computational physicsNoiseSpace and Planetary SciencesymbolsCosmic microwave background ; Numerical ; Data analysisDeconvolutionUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaBeam (structure):ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Cold dark matter plus not-so-clumpy dark relics

2017

Various particle physics models suggest that, besides the (nearly) cold dark matter that accounts for current observations, additional but sub-dominant dark relics might exist. These could be warm, hot, or even contribute as dark radiation. We present here a comprehensive study of two-component dark matter scenarios, where the first component is assumed to be cold, and the second is a non-cold thermal relic. Considering the cases where the non-cold dark matter species could be either a fermion or a boson, we derive consistent upper limits on the non-cold dark relic energy density for a very large range of velocity dispersions, covering the entire range from dark radiation to cold dark matte…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark matterMilky WayCosmic microwave backgroundDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010303 astronomy & astrophysicsCondensed Matter::Quantum GasesPhysics010308 nuclear & particles physicsMatter power spectrumAstronomy and AstrophysicsBaryonHigh Energy Physics - Phenomenology13. Climate actionDark radiationsymbolsAstrophysics - Cosmology and Nongalactic Astrophysics
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Testing theories of Gravity and Supergravity with inflation and observations of the cosmic microwave background

2016

Many extensions of Einstein's theory of gravity have been studied and proposed with various motivations like the quest for a quantum theory of gravity to extensions of anomalies in observations at the solar system, galactic and cosmological scales. These extensions include adding higher powers of Ricci curvature $R$, coupling the Ricci curvature with scalar fields and generalized functions of $R$. In addition when viewed from the perspective of Supergravity (SUGRA) many of these theories may originate from the same SUGRA theory interpreted in different frames. SUGRA therefore serves as a good framework for organizing and generalizing theories of gravity beyond General Relativity. All these …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)General relativitymedia_common.quotation_subjectFOS: Physical sciencesLambda-CDM modelCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)CMBSUGRA01 natural sciencesCosmologyGeneral Relativity and Quantum CosmologyMetric expansion of spacesymbols.namesakeTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanckinflation010306 general physicsMathematical Physicsmedia_commonPhysics010308 nuclear & particles physicsAstronomy and AstrophysicsUniverseHigh Energy Physics - PhenomenologySpace and Planetary SciencesymbolsDark energyCMB; inflation; SUGRAAstrophysics - Cosmology and Nongalactic Astrophysics
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Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample

2018

The hot plasma in galaxy clusters is expected to be heated to high temperatures through shocks and adiabatic compression. The thermodynamical properties of the gas encode information on the processes leading to the thermalization of the gas in the cluster's potential well as well as non-gravitational processes such as gas cooling, AGN feedback and kinetic energy. In this work we present the radial profiles of the thermodynamic properties of the intracluster medium (ICM) out to the virial radius for a sample of 12 galaxy clusters selected from the Planck all-sky survey. We determine the universal profiles of gas density, temperature, pressure, and entropy over more than two decades in radius…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)galaxies: clusters: intracluster mediumDark matterPopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesdark matterVirial theoremsymbols.namesakeIntracluster medium0103 physical sciencesGravitational collapsePlanckAdiabatic processeducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGalaxy clusterPhysicseducation.field_of_study[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Settore FIS/05010308 nuclear & particles physicsThermodynamical quantitiesAstronomy and AstrophysicsX-rays: galaxies: clusters; dark matter; galaxies: clusters: intracluster medium; galaxies: clusters: general; Thermodynamical quantitiesgalaxies: clusters: general13. Climate actionSpace and Planetary ScienceX-rays: galaxies: clustersastro-ph.COsymbols[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsAstronomy & Astrophysics
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In the realm of the Hubble tension—a review of solutions

2021

The $\Lambda$CDM model provides a good fit to a large span of cosmological data but harbors areas of phenomenology. With the improvement of the number and the accuracy of observations, discrepancies among key cosmological parameters of the model have emerged. The most statistically significant tension is the $4-6\sigma$ disagreement between predictions of the Hubble constant $H_0$ by early time probes with $\Lambda$CDM model, and a number of late time, model-independent determinations of $H_0$ from local measurements of distances and redshifts. The high precision and consistency of the data at both ends present strong challenges to the possible solution space and demand a hypothesis with en…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)satellite: PlanckPhysics and Astronomy (miscellaneous)gravitation: modelPhysics beyond the Standard ModelCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsbaryon: oscillation: acoustic01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologysymbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)cosmological model: parameter space0103 physical sciencesstructurePlanckinflationcosmic background radiation: power spectrum010306 general physicsdark energyneutrino: interactionPhysicssupernova: Type IHubble constant010308 nuclear & particles physicsnew physicsmagnetic field: primordialtensionredshiftAstrophysics - Astrophysics of GalaxiesRedshiftrecombinationHigh Energy Physics - Phenomenology13. Climate actionAstrophysics of Galaxies (astro-ph.GA)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]relativisticsymbolsDark energy[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Phenomenology (particle physics)statisticalAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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Generalized Wiener Process and Kolmogorov's Equation for Diffusion induced by Non-Gaussian Noise Source

2005

We show that the increments of generalized Wiener process, useful to describe non-Gaussian white noise sources, have the properties of infinitely divisible random processes. Using functional approach and the new correlation formula for non-Gaussian white noise we derive directly from Langevin equation, with such a random source, the Kolmogorov's equation for Markovian non-Gaussian process. From this equation we obtain the Fokker-Planck equation for nonlinear system driven by white Gaussian noise, the Kolmogorov-Feller equation for discontinuous Markovian processes, and the fractional Fokker-Planck equation for anomalous diffusion. The stationary probability distributions for some simple cas…

Diffusion equationStatistical Mechanics (cond-mat.stat-mech)General MathematicsMathematical analysisGeneral Physics and AstronomyFOS: Physical sciencesOrnstein–Uhlenbeck processCondensed Matter - Soft Condensed MatterGaussian random fieldLangevin equationsymbols.namesakeStochastic differential equationAdditive white Gaussian noiseGaussian noisesymbolsProcess and Kolmogorov'sSoft Condensed Matter (cond-mat.soft)Fokker–Planck equationCondensed Matter - Statistical MechanicsMathematics
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International Conference on Functional Materials and Nanotechnologies (FM&NT2012)

2012

The International Conference Functional Materials and Nanotechnologies (FMN ferroics; multiscale and multiphenomenal material modeling and simulation 2. Nanotechnologies including progressive methods, technologies and design for investigation of nanoparticles, nanostructures, nanocomposites, thin films and coatings; 3. Energy including perspective materials and technologies for renewable and hydrogen energy, fuel cells, photovoltaics and developing diverse energy systems. A special section devoted to Organic Materials was organized to commemorate a long-time organizer of the FM&NT conference series, Dr. habil. phys, academician Inta Muzikante who passed away on 15 February 2012. The number …

Engineeringbusiness.industrySolid-stateLatvianLibrary scienceMechanical engineeringlanguage.human_languageMax planck instituteHigh pressureTechnical universitySpecial sectionlanguageTurning pointEnergy structurebusinessIOP Conference Series: Materials Science and Engineering
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A Fisher–Kolmogorov equation with finite speed of propagation

2010

Abstract In this paper we study a Fisher–Kolmogorov type equation with a flux limited diffusion term and we prove the existence and uniqueness of finite speed moving fronts and the existence of some explicit solutions in a particular regime of the equation.

Entropy solutionsPartial differential equationDiffusion equationApplied MathematicsMathematical analysisFlux limited diffusion equationsReaction–diffusion equationsFront propagationReaction–diffusion systemFisher–Kolmogorov equationFokker–Planck equationUniquenessDiffusion (business)Convection–diffusion equationAnalysisMathematicsJournal of Differential Equations
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