Search results for "Llar"

showing 10 items of 3592 documents

Monte Carlo simulations of the solid-liquid transition in hard spheres and colloid-polymer mixtures

2010

Monte Carlo simulations at constant pressure are performed to study coexistence and interfacial properties of the liquid-solid transition in hard spheres and in colloid-polymer mixtures. The latter system is described as a one-component Asakura-Oosawa (AO) model where the polymer's degrees of freedom are incorporated via an attractive part in the effective potential for the colloid-colloid interactions. For the considered AO model, the polymer reservoir packing fraction is eta_p^r=0.1 and the colloid-polymer size ratio is q=sigma_p/\sigma=0.15 (with sigma_p and sigma the diameter of polymers and colloids, respectively). Inhomogeneous solid-liquid systems are prepared by placing the solid fc…

ANISOTROPIC SURFACE-TENSIONMaterials scienceMonte Carlo methodDegrees of freedom (physics and chemistry)General Physics and AstronomyThermodynamicsCondensed Matter - Soft Condensed MatterCAPILLARY WAVESAtomic packing factorCOMPUTER-SIMULATIONVAPOR INTERFACE3-DIMENSIONAL ISING-MODELColloidsymbols.namesakePhase (matter)Physical and Theoretical ChemistryCOEXISTING PHASESchemistry.chemical_classificationCondensed Matter - Materials ScienceINTERFACIAL FREE-ENERGYPROFILESHard spheresPolymerCondensed Matter::Soft Condensed MatterchemistryCRYSTAL-MELT INTERFACESBoltzmann constantsymbolsCRYSTALLIZATIONThe Journal of Chemical Physics
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A mathematical approach to model diffusion properties of sedimentary rocks relevant to Sicily cultural heritage

2007

Cultural heritage vestiges represent complex physical systems, able to interact with the environment through continuous exchanges of heat and fluids (water, air). In this wide context, particular relevance is assumed by transport phenomena and diffusion of pollutant, vehiculated inside the considered structure by water itself. Interaction mechanisms can be considered at various observation scales, depending on the material provenance and on its geometry and location. Involved materials are commonly constituted by porous rocks - more or less altered - belonging to geological sedimentary formations, as limestone, calcarenite and travertine. Their appreciable porosity affects significantly liq…

ARCHAEOLOGICAL SITE ENVIRONMENTAL RISK CAPILLARITY ABSORPTION MAGNETIC RESONANCE NUMERICAL MODELSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)
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H-He collision-induced satellite in the Lyman alpha profile of DBA white dwarf stars

2020

The spectra of helium-dominated white dwarf stars with hydrogen in their atmosphere present a distinctive broad feature centered around 1160~\AA\/ in the blue wing of the Lyman-$\alpha$ line. It is extremely apparent in WD 1425+540 recently observed with HST COS. With new theoretical line profiles based on ab initio atomic interaction potentials we show that this feature is a signature of a collision-induced satellite due to an asymptotically forbidden transition. This quasi-molecular spectral satellite is crucial to understanding the asymmetrical shape of Lyman-$\alpha$ seen in this and other white dwarf spectra. Our previous work predicting this absorption feature was limited by molecular…

ATOMIC DATALINE: PROFILEAb initiochemistry.chemical_elementBASIS-SETLINEEXCITED-STATEAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral linePhysics - Atomic PhysicsWHITE DWARF0103 physical sciencesRadiative transferABSORPTIONAstrophysics::Solar and Stellar AstrophysicsAB-INITIO CALCULATIONPhysics::Atomic PhysicsELECTRONIC-TRANSITION MOMENT010306 general physicsSTARS: ATMOSPHERE010303 astronomy & astrophysicsHeliumLine (formation)POTENTIAL-ENERGY CURVEPhysics[PHYS]Physics [physics]BALMER-ALPHAWhite dwarfAstronomy and AstrophysicsMOLECULAR DATAPotential energyDipolechemistryAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceATOMIC PROCESSSHAPE[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Atomic physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Alkamides from Echinacea angustifolia Interact with P-Glycoprotein of Primary Brain Capillary Endothelial Cells Isolated from Porcine Brain Blood Ves…

2013

The blood-brain barrier prevents the passage of toxic compounds from blood circulation into brain tissue. Unfortunately, drugs for the treatment of neurodegenerative diseases, brain tumors, and other diseases also do not cross the blood-brain barrier. In the present investigation, we used isolated porcine brain capillary endothelial cells and a flow cytometric calcein-AM assay to analyze inhibition of P-glycoprotein, a major constituent of the blood-brain barrier. We tested 8 alkamides isolated from Echinacea angustifolia and found that four of them inhibited P-glycoprotein-mediated calcein transport in porcine brain capillary endothelial cells.

ATP Binding Cassette Transporter Subfamily BPolyunsaturated AlkamidesSwinePharmaceutical ScienceATP-binding cassette transporterCapillary endothelial cellsPharmacologyBlood–brain barrierEchinaceaAnalytical Chemistrychemistry.chemical_compoundDrug DiscoverymedicineAnimalsCells CulturedP-glycoproteinPharmacologyDose-Response Relationship DrugMolecular StructurebiologyEchinacea angustifoliaOrganic ChemistryBrainEndothelial CellsBiological TransportFlow CytometryFluoresceinsbiology.organism_classificationCalceinmedicine.anatomical_structureComplementary and alternative medicinechemistryBlood-Brain BarrierBlood circulationbiology.proteinMolecular MedicinePorcine brainPlanta Medica
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A parametric description of the 3D structure of the Galactic bar/bulge using the VVV survey

2017

We study the structure of the inner Milky Way using the latest data release of the Vista Variables in Via Lactea (VVV) survey. The VVV is a deep near-infrared, multi-colour photometric survey with a coverage of 300 square degrees towards the Bulge/Bar. We use Red Clump (RC) stars to produce a high-resolution dust map of the VVV's field of view. From de-reddened colour-magnitude diagrams we select Red Giant Branch stars to investigate their 3D density distribution within the central 4 kpc. We demonstrate that our best-fit parametric model of the Bulge density provides a good description of the VVV data, with a median percentage residual of 5$\%$ over the fitted region. The strongest of the o…

Absolute magnitudeInitial mass functionastro-ph.GAMilky WayFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: bulgeBulge0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsRed clumpGalaxy: structureAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSLuminosity function (astronomy)Physics010308 nuclear & particles physicsGalactic CenterAstronomyAstronomy and AstrophysicsGalaxy: fundamental parametersAstrophysics - Astrophysics of GalaxiesGalaxy: centregalaxies: individual: Milky WayRed-giant branchSpace and Planetary ScienceGalaxy: formationAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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DISTRIBUTION OF CARBON STARS IN THE GALAXY

2018

A search for new faint carbon (C) stars in the Polar region δ > 55o has been accomplished by obtaining objective prism spectra in the near infrared 550 -- 900 nm on images of CCD camera of Baldone Schmidt telescope of Astrophysical observatory. The positions of stars   having color indices (J – K) > 1.3 mag in Two Micron All Sky Infrared Survey (2MASS) were selected to pick out suspicious carbon stars.Our survey is limited in brightness by J < 10 mag. 24 new carbon stars were found and their characteristics obtained. The correlative relation between Teff  and spectral gradient [757 – 685] was confirmed. Such characteristics as Teff, distance from the Sun, absolute Mk  were obtained…

Absolute magnitudePhysicsBrightnessInfraredcircumstellar materlcsh:Astronomymedia_common.quotation_subjectnear infraredAstrophysics::Instrumentation and Methods for Astrophysicsabsolute magnitudeAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSchmidt cameraCarbon starGalaxylcsh:QB1-991StarsSkyAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsdistanceAstrophysics::Galaxy Astrophysicscarbon starsmedia_commoncircumstellar mater; near infrared; carbon stars; absolute magnitude; distanceOdessa Astronomical Publications
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Isocratic and gradient elution in micellar liquid chromatography with Brij-35

2015

Polyoxyethylene(23)lauryl ether (known as Brij-35) is a nonionic surfactant, which has been considered as an alternative to the extensively used in micellar liquid chromatography anionic surfactant sodium lauryl (dodecyl) sulfate, for the analysis of drugs and other types of compounds. Brij-35 is the most suitable nonionic surfactant for micellar liquid chromatography, owing to its commercial availability, low cost, low toxicity, high cloud temperature, and low background absorbance. However, it has had minor use. In this work, we gather and discuss some results obtained in our laboratory with several β-blockers, sulfonamides, and flavonoids, concerning the use of Brij-35 as mobile phase mo…

Absorbancechemistry.chemical_compoundChromatographyAqueous solutionPulmonary surfactantchemistryMicellar liquid chromatographyPhase (matter)Filtration and SeparationEtherAcetonitrileMicellar electrokinetic chromatographyAnalytical ChemistryJournal of Separation Science
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Micellar liquid chromatography for prediction of drug transport.

2000

Abstract The vast majority of well absorbed drugs are transported passively across the cell membranes. Physicochemical descriptors of drug molecules that are believed to influence transcellular transport are routinely used to predict drug absorption by means of complex mathematical models. In this paper, a new in vitro method, based on the retention data in micellar liquid chromatography (MLC), is validated for the prediction of passive drug absorption. The retention of a heterogeneous drugs set in MLC using Brij 35 as surfactant in the mobile phase is compared with the retention data reported in literature obtained in red cell membrane lipid liposomes, human red cell membranes vesicles (ve…

Absorption (pharmacology)LiposomeChromatographyChemistryVesicleOrganic ChemistryCell MembraneAdministration OralGeneral MedicineBiochemistryHigh-performance liquid chromatographyAnalytical ChemistryMembranePulmonary surfactantMicellar liquid chromatographyParacellular transportHumansPharmacokineticsSpectrophotometry UltravioletMicellesChromatography LiquidJournal of chromatography. A
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Contribution à l'étude des liaisons optiques atmosphériques : propagation, disponibilité et fiabilité.

2005

In this work we study the fog attenuation in the visible and infrared spectral band related to Free Space Optics (FSO). Based on the Mie scattering theory, fog extinction coefficients for different particle size distributions as a function of wavelength were derived. A simple analytical model allowing the prediction of atmospheric transmission for the 0.69 - 1.55 µm spectral band was developed. This model is valid for advection and convection fog and for visibility range between 50 to 1000 m. This model, implemented into software developed at FT R&D, allows the prediction of the Quality of Service of FSO links. Finally, we performed an experimental study to compare the fog effect on two FSO…

Absorption moléculairePropagation optique dans l'atmosphèreAtténuation atmosphérique.[ PHYS.PHYS.PHYS-ATOM-PH ] Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]Mie scattering theoryvisible and infrared wave propagation in the atmosphereLiaisons optiques atmosphériquesDistribution de taille de particulesfogFree space opticsatmospheric attenuation.AérosolsBrouillardparticle size distribution[PHYS.PHYS.PHYS-ATOM-PH] Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]Atténuation atmosphériqueThéorie de diffusion de Miemolecular absorption
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An Introduction to Soil and Water Infiltration

2016

This chapter provides a short presentation of general characteristics of the soil. Basic concepts concerning soil water content and potential and flow of water in the porous medium are then reported since these concepts are diffusely used throughout this book. The infiltration process is finally illustrated considering different modeling approaches. In particular, development of analytical infiltration models is described with reference to one-dimensional gravity-free water absorption, one-dimensional gravity driven infiltration, one-dimensional gravity and capillary driven infiltration and, finally, three-dimensional gravity and capillary driven infiltration.

Absorption of waterCapillary actionQuantitative Biology::Tissues and OrgansPhysics::OpticsSoil science04 agricultural and veterinary sciences010501 environmental sciences01 natural sciencesPhysics::GeophysicsPressure headInfiltration (hydrology)Hydraulic conductivitySoil water040103 agronomy & agriculture0401 agriculture forestry and fisheriesEnvironmental sciencePorous mediumWater content0105 earth and related environmental sciences
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