Search results for " equilibrium"

showing 10 items of 533 documents

Approximations of Parabolic Equations at the Vicinity of Hyperbolic Equilibrium Point

2014

This article is devoted to the numerical analysis of the abstract semilinear parabolic problem u′(t) = Au(t) + f(u(t)), u(0) = u 0, in a Banach space E. We are developing a general approach to establish a discrete dichotomy in a very general setting and prove shadowing theorems that compare solutions of the continuous problem with those of discrete approximations in space and time. In [3] the discretization in space was constructed under the assumption of compactness of the resolvent. It is a well-known fact (see [10, 11]) that the phase space in the neighborhood of the hyperbolic equilibrium can be split in a such way that the original initial value problem is reduced to initial value prob…

Control and OptimizationDiscretizationMathematical analysisBanach spaceSpace (mathematics)Linear subspaceComputer Science ApplicationsCompact spaceBounded functionSignal ProcessingInitial value problemAnalysisMathematicsHyperbolic equilibrium pointNumerical Functional Analysis and Optimization
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Teoria dell’equilibrio del controllo di Tittle

2021

Viene analizzata la teoria elaborata da Charles R. Tittle che combina assunti derivati da una serie di teorie, come la teoria del controllo sociale, l’associazione differenziale, l’anomia, le teorie del conflitto, l’etichettamento, la scelta razionale e la teoria delle attività di routine. The theory developed by Charles R. Tittle is analyzed which combines assumptions derived from a series of theories, such as the theory of social control, differential association, anomie, conflict theories, labeling, rational choice and theory of routine activities.

Control equilibrium theorySettore SPS/12 - Sociologia Giuridica Della Devianza E Mutamento SocialeTittleTeoria dell'equilibrio del controllo
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Power spectrum of turbulent convection in the solar photosphere

2020

The solar photosphere provides us with a laboratory for understanding turbulence in a layer where the fundamental processes of transport vary rapidly and a strongly superadiabatic region lies very closely to a subadiabatic layer. Our tools for probing the turbulence are high-resolution spectropolarimetric observations such as have recently been obtained with the two balloon-borne SUNRISE missions, and numerical simulations. Our aim is to study photospheric turbulence with the help of Fourier power spectra that we compute from observations and simulations. We also attempt to explain some properties of the photospheric overshooting flow with the help of its governing equations and simulations…

Convection010504 meteorology & atmospheric sciencesphotosphere [Sun]FOS: Physical sciencesAstrophysicsConvection01 natural sciencesPower lawlaw.inventionMomentumAtmospherelaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Optical depth0105 earth and related environmental sciencesPhysicsPhotosphereTurbulenceSun: photosphereAstronomy and AstrophysicsComputational physicsTurbulenceAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceHydrostatic equilibrium
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What causes the large extensions of red-supergiant atmospheres? Comparisons of interferometric observations with 1-D hydrostatic, 3-D convection, and…

2015

We present the atmospheric structure and the fundamental parameters of three red supergiants, increasing the sample of RSGs observed by near-infrared spectro-interferometry. Additionally, we test possible mechanisms that may explain the large observed atmospheric extensions of RSGs. We carried out spectro-interferometric observations of 3 RSGs in the near-infrared K-band with the VLTI/AMBER instrument at medium spectral resolution. To comprehend the extended atmospheres, we compared our observational results to predictions by available hydrostatic PHOENIX, available 3-D convection, and new 1-D self-excited pulsation models of RSGs. Our near-infrared flux spectra are well reproduced by the P…

ConvectionPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicslaw.inventionInterferometryAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencelawAstrophysics::Solar and Stellar AstrophysicsRed supergiantChristian ministryAstrophysics::Earth and Planetary AstrophysicsSupergiantHydrostatic equilibriumSolar and Stellar Astrophysics (astro-ph.SR)
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Modeling X-ray emission from stellar coronae

2008

By extrapolating from observationally derived surface magnetograms of low-mass stars we construct models of their coronal magnetic fields and compare the 3D field geometry with axial multipoles. AB Dor, which has a radiative core, has a very complex field, whereas V374 Peg, which is completely convective, has a simple dipolar field. We calculate global X-ray emission measures assuming that the plasma trapped along the coronal loops is in hydrostatic equilibrium and compare the differences between assuming isothermal coronae, or by considering a loop temperature profiles. Our preliminary results suggest that the non-isothermal model works well for the complex field of AB Dor, but not for the…

ConvectionPhysicsopacity and line formation Magnetic and electric fieldField (physics)Astrophysics (astro-ph)FOS: Physical sciencesCoronal loopAstrophysicsPlasmapolarization of starlightAstrophysicsMagnetic fieldlaw.inventionStarsSettore FIS/05 - Astronomia E Astrofisicaradiative transferlawX-ray emission spectra and fluorescence Stellar atmospheresRadiative transferAstrophysics::Solar and Stellar AstrophysicsHydrostatic equilibrium
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ON the NATURE of HYDROSTATIC EQUILIBRIUM in GALAXY CLUSTERS

2016

In this paper we investigate the level of hydrostatic equilibrium (HE) in the intra-cluster medium of simulated galaxy clusters, extracted from state-of-the-art cosmological hydrodynamical simulations performed with the Smoothed-Particle-Hydrodynamic code GADGET-3. These simulations include several physical processes, among which stellar and AGN feedback, and have been performed with an improved version of the code that allows for a better description of hydrodynamical instabilities and gas mixing processes. Evaluating the radial balance between the gravitational and hydrodynamical forces, via the gas accelerations generated, we effectively examine the level of HE in every object of the sam…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusgalaxies: clusters: intracluster mediumFOS: Physical sciences01 natural sciencesVirial theoremlaw.inventionmethods: numericalGravitationlawIntracluster medium0103 physical sciencesCluster (physics)clusters: general [galaxies]010303 astronomy & astrophysicsGalaxy clusterPhysics010308 nuclear & particles physicsnumerical [methods]Astronomy and AstrophysicsRadiusAstronomy and AstrophysicComputational physicsclusters: intracluster medium [galaxies]galaxies: clusters: generalSpace and Planetary ScienceHydrostatic equilibriumgalaxies: clusters: general; galaxies: clusters: intracluster medium; methods: numerical; Astronomy and Astrophysics; Space and Planetary ScienceAstrophysics - Cosmology and Nongalactic Astrophysics
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Non-accumulation of critical points of the Poincaré time on hyperbolic polycycles

2007

We call Poincare time the time associated to the Poincar6 (or first return) map of a vector field. In this paper we prove the non-accumulation of isolated critical points of the Poincare time T on hyperbolic polycycles of polynomial vector fields. The result is obtained by proving that the Poincare time of a hyperbolic polycycle either has an unbounded principal part or is an almost regular function. The result relies heavily on the proof of Il'yashenko's theorem on non-accumulation of limit cycles on hyperbolic polycycles.

Critical period; finiteness; non-accumulation; quasi-analyticity; Dulac problem.Applied MathematicsGeneral MathematicsLimit cycleMathematical analysisHyperbolic manifoldPrincipal partUltraparallel theoremVector fieldRelatively hyperbolic groupCritical point (mathematics)Hyperbolic equilibrium pointMathematicsProceedings of the American Mathematical Society
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Cascade complex formation by phosphate in the cobalt(II)/[30]aneN10 anaerobic system

1993

Abstract The interaction of phosphate with the mono- and binuclear cobalt(II) complexes of [30]aneN 10 (1,4,7,10,13,16,19,22,25,28-decaazacyclotriacontane) has been studied by potentiometry in 0.15 mol dm −3 NaClO 4 solution at 298.15 K under anaerobic conditions. The stable species [CoH 2 ([30]aneN 10 )PO 4 ] + , [CoH 4 ([30]aneN 10 )PO 4 ] 3+ , [Co 2 H([30]aneN 10 )PO 4 ] 2+ , [Co 2 H 2 ([30]aneN 10 )PO 4 ] 3+ and [Co 2 H 3 ([30]aneN 10 )PO 4 ] 4+ , where the phosphate anion is directly bound to the metal ions or acts as a second sphere ligand, are formed and their stability constants have been determined. The results obtained allowed for the selection of suitable conditions for the study…

DIOXYGEN CARRIERS; DIOXYGEN BINDING; Co(II) COMPLEXES; POLYAMINE LIGANDS; DITOPIC POLYAMINES; OPEN-CHAIN POLYAZAALKANES; THERMODYNAMICS; ANION COORDINATION CHEMISTRY; INCLUSION COMPLEXESINCLUSION COMPLEXESMetal ions in aqueous solutionComplex formationInorganic chemistryDIOXYGEN BINDINGchemistry.chemical_elementMedicinal chemistryCo(II) COMPLEXESInorganic Chemistrychemistry.chemical_compoundOPEN-CHAIN POLYAZAALKANESANION COORDINATION CHEMISTRYTHERMODYNAMICSMaterials ChemistryDIOXYGEN CARRIERSPhysical and Theoretical ChemistryLigandPhosphatePhosphate anionchemistryDITOPIC POLYAMINESChemical equilibriumAnaerobic exerciseCobaltPOLYAMINE LIGANDS
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Calculation of proton activity in aqueous protolyte solutions

1980

Abstract A general and thermodynamically exact equation for the calculation of the proton (hydroxide ion) activity of aqueous solutions of monoprotic acidic (and basic) species is given. Under certain conditions, various approximate equations can be derived from the exact form; the applicability of these depends mainly on both the thermodynamic equilibrium constant, K p , of the protolytic reaction, and the stoichiometric concentration, C o , of the protolyte. Taking into account the mean ionic activity coefficients which are calculated by means of the Davies equation, diagrams are constructed exhibiting those combinations of K p and C o for which the respective approximations can be applie…

Davies equationActivity coefficientAqueous solutionProtonThermodynamic equilibriumChemistryIonic bondingThermodynamicsBiochemistryAnalytical ChemistryIonchemistry.chemical_compoundEnvironmental ChemistryHydroxideSpectroscopyAnalytica Chimica Acta
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Debt Sustainability and Fiscal Space in a Heterogeneous Monetary Union: Normal Times Vs the Zero Lower Bound

2020

In this paper we study fiscal policy effects and fiscal space for countries in a monetary union with different levels of public debt. We develop a dynamic stochastic general equilibrium (DSGE) model of a two-country monetary union, calibrated to match the characteristics of Spain and Germany, in which debt sustainability is endogenously determined a la Bi (2012) to shape the responses of the risk premium on public debt. Policy shocks change the market’s expectation about future primary surplus, producing a direct effect on the sovereign risk premium and macroeconomic responses of the economy. In normal times the costs of a government spending driven fiscal consolidation in the high-debt cou…

Debtmedia_common.quotation_subjectFiscal spaceRisk premiumZero lower boundMonetary policyEconomicsDynamic stochastic general equilibriumMonetary economicsFiscal sustainabilitymedia_commonFiscal policySSRN Electronic Journal
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