Search results for "Newton"

showing 10 items of 134 documents

2019

Abstract. The flow of fluids through porous media such as groundwater flow or magma migration is a key process in geological sciences. Flow is controlled by the permeability of the rock; thus, an accurate determination and prediction of its value is of crucial importance. For this reason, permeability has been measured across different scales. As laboratory measurements exhibit a range of limitations, the numerical prediction of permeability at conditions where laboratory experiments struggle has become an important method to complement laboratory approaches. At high resolutions, this prediction becomes computationally very expensive, which makes it crucial to develop methods that maximize …

010504 meteorology & atmospheric sciencesStratigraphyFinite differencePaleontologySoil ScienceReynolds numberGeologyMechanics010502 geochemistry & geophysics01 natural sciencesStencilNon-Newtonian fluidPhysics::GeophysicsPhysics::Fluid DynamicsPermeability (earth sciences)symbols.namesakeGeophysicsGeochemistry and PetrologyFluid dynamicsNewtonian fluidsymbolsPorous mediumGeology0105 earth and related environmental sciencesEarth-Surface ProcessesSolid Earth
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Drift and evolutionary forces

2016

This arride analyzes the view of evolutionary theory as a theory of forces. The analogy with Newtonian mechanics has been challenged due to the alleged mismatch between drift and the other evolutionary forces. Since genetic drifr has no direction severa! authors tried to protect its status as a force: denying its lack of directionality, extending the notion of force and looking for a force in physics which also lacks of direction. I analyse these approaches, and although this strategy finally succeeds, this discussion overlooks the crucial point on the debate between causalists and statisticalists: the causal status of evolutionary theoty.; El presente artículo analiza la visión de la teorí…

05 social sciencesAnalogy06 humanities and the artsCausal structure050905 science studies0603 philosophy ethics and religionPhilosophyClassical mechanicsHistory and Philosophy of ScienceGenetic drift060302 philosophyCalculusNewtonian fluid0509 other social sciencesBrownian motionEvolutionary theoryMathematics
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A Note on Laws of Motion for Aggregate Distributions

2020

I derive the law of motion for the aggregate distribution directly from the laws of motion for the individuals’ states. By relying on concepts from measure theory, the derivation is concise and intuitive. I address random shocks both at the micro level and at the macro level. Micro-level shocks completely cancel at the aggregate level provided that a law of large numbers applies. Therefore, the law of motion for the aggregate distribution is a deterministic process in the absence of macro-level uncertainty. If there are macro-level risks, the law of motion for the aggregate distribution exhibits a stochastic component additionally. I illustrate the formalism in a model of wealth accumulatio…

050208 financeFormalism (philosophy)media_common.quotation_subject05 social sciencesAggregate (data warehouse)Newton's laws of motionMotion (physics)Interest rateFormalism (philosophy of mathematics)Classical mechanicsAggregate distributionComponent (UML)0502 economics and businessFokker–Planck equationWealth distributionStatistical physics050207 economicsmedia_commonMathematicsTheoretical Economics Letters
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Sharp capacity estimates for annuli in weighted R^n and in metric spaces

2017

We obtain estimates for the nonlinear variational capacity of annuli in weighted R^n and in metric spaces. We introduce four different (pointwise) exponent sets, show that they all play fundamental roles for capacity estimates, and also demonstrate that whether an end point of an exponent set is attained or not is important. As a consequence of our estimates we obtain, for instance, criteria for points to have zero (resp. positive) capacity. Our discussion holds in rather general metric spaces, including Carnot groups and many manifolds, but it is just as relevant on weighted R^n. Indeed, to illustrate the sharpness of our estimates, we give several examples of radially weighted R^n, which …

31C45 (Primary) 30C65 30L99 31B15 31C15 31E0 (Secondary)annulusmetric spacequasiconformal mappingMathematical Analysisexponent setsp-admissible weightSobolev spaceradial weightMathematics - Analysis of PDEsAnnulus; Doubling measure; Exponent sets; Metric space; Newtonian space; p-admissible weight; Poincare inequality; Quasiconformal mapping; Radial weight; Sobolev space; Variational capacityMatematisk analysPoincaré inequalitydoubling measureFOS: MathematicsNewtonian spacevariational capacityAnalysis of PDEs (math.AP)
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Łojasiewicz exponents, the integral closure of ideals and Newton polyhedra

2003

We give an upper estimate for the Łojasiewicz exponent $\ell(J,I)$ of an ideal $J\subseteq A(K^{n})$ with respect to another ideal I in the ring $A(K^{n})$ of germs analytic functions $f$ : $(K^{n},\mathrm{O})\rightarrow K$ , where $K=C$ or $R$ , using Newton polyhedrons. In particular, we give a method to estimate the Łojasiewicz exponent $\alpha_{0}(f)$ of a germ $f\in A(K^{n})$ that can be applied when $f$ is Newton degenerate with respect to its Newton polyhedron.

58A20Ring (mathematics)32S05General MathematicsDegenerate energy levelsClosure (topology)Łojasiewicz exponentsreal analytic functionsCombinatoricsPolyhedronExponentNewton polyhedronsIdeal (ring theory)Analytic functionMathematicsJournal of the Mathematical Society of Japan
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Accretion in strong field gravity with eXTP

2019

In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced 'spectral-timing-polarimetry' techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process.

ACTIVE GALACTIC NUCLEIAccretionaccretion; black holes physics; X-ray; Physics and Astronomy (all)black holes physicAstronomyAstrophysics::High Energy Astrophysical PhenomenaBlack holes physicsPolarimetryFOS: Physical sciencesBLACK-HOLE SPINGeneral Physics and AstronomyStrong fieldAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesX-rayPhysics and Astronomy (all)ELECTROMAGNETIC EMISSIONSettore FIS/05 - Astronomia e Astrofisicablack holes physicsaccretion0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)XMM-NEWTONPhysicsLENS-THIRRING PRECESSION[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]QUASI-PERIODIC OSCILLATIONS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]IRON KAccretion (astrophysics)X ray[SDU]Sciences of the Universe [physics]ULTRA-FAST OUTFLOWSAstrophysics::Earth and Planetary AstrophysicsSPECTRAL FEATURESAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-RAY BINARIESScience China Physics, Mechanics & Astronomy
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The flaring afterglow of GRB 050730

2006

We present a detailed spectral and temporal analysis of Swift and XMM-Newton observations of GRB 050730. The X-ray afterglow of GRB 050730 was found to decline with time with intense flaring activity superimposed. Evidence of flaring activity in the early UVOT optical afterglow, simultaneous with that observed in the X-ray band, was found. Strong spectral evolution in the X-ray energy band during the flaring activity was present.

Afterglows X Rays XMM-Newton Telescope
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On strong solutions of the differential equations modeling the steady flow of certain incompressible generalized Newtonian fluids

2007

In this paper we discuss a system of partial differential equations describing the steady flow of an incompressible fluid and prove the existence of a strong solution under suitable assumptions on the data. In the 2D-case this solution turns out to be of class C^{1,\alpha}.

Algebra and Number TheoryPartial differential equationDifferential equationApplied MathematicsMathematical analysis510Physics::Fluid DynamicsStrong solutionsGeneralized Newtonian fluidFlow (mathematics)CompressibilityNewtonian fluidAnalysisMathematicsSt. Petersburg Mathematical Journal
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A generalized Newton iteration for computing the solution of the inverse Henderson problem

2020

We develop a generalized Newton scheme IHNC for the construction of effective pair potentials for systems of interacting point-like particles.The construction is made in such a way that the distribution of the particles matches a given radial distribution function. The IHNC iteration uses the hypernetted-chain integral equation for an approximate evaluation of the inverse of the Jacobian of the forward operator. In contrast to the full Newton method realized in the Inverse Monte Carlo (IMC) scheme, the IHNC algorithm requires only a single molecular dynamics computation of the radial distribution function per iteration step, and no further expensive cross-correlations. Numerical experiments…

Applied MathematicsGeneral EngineeringInverseNumerical Analysis (math.NA)010103 numerical & computational mathematicsRadial distribution function01 natural sciencesComputer Science Applications010101 applied mathematicssymbols.namesakeScheme (mathematics)FOS: MathematicssymbolsApplied mathematicsMathematics - Numerical AnalysisGranularity0101 mathematicsNewton's method65Z05 82B21MathematicsInverse Problems in Science and Engineering
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A regularized Newton method for locating thin tubular conductivity inhomogeneities

2011

We consider the inverse problem of determining the position and shape of a thin tubular object, such as for instance a wire, a thin channel or a curve-like crack, embedded in some three-dimensional homogeneous body from a single measurement of electrostatic currents and potentials on the boundary of the body. Using an asymptotic model describing perturbations of electrostatic potentials caused by such thin objects, we reformulate the inverse problem as a nonlinear operator equation. We establish Frechet differentiability of the corresponding operator, compute its Frechet derivative and set up a regularized Newton scheme to solve the inverse problem numerically. We discuss our implementation…

Applied MathematicsOperator (physics)Mathematical analysisFréchet derivativeBoundary (topology)Inverse problemComputer Science ApplicationsTheoretical Computer Sciencesymbols.namesakeNewton fractalPosition (vector)Signal ProcessingsymbolsDifferentiable functionNewton's methodMathematical PhysicsMathematicsInverse Problems
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