Search results for "Number density"

showing 10 items of 19 documents

Modelling accretion disc and stellar wind interactions: the case of Sgr A*

2016

Sgr A* is an ideal target to study low-luminosity accreting systems. It has been recently proposed that properties of the accretion flow around Sgr A* can be probed through its interactions with the stellar wind of nearby massive stars belonging to the S-cluster. When a star intercepts the accretion disk, the ram and thermal pressures of the disk terminate the stellar wind leading to the formation of a bow shock structure. Here, a semi-analytical model is constructed which describes the geometry of the termination shock formed in the wind. With the employment of numerical hydrodynamic simulations, this model is both verified and extended to a region prone to Kelvin-Helmholtz instabilities. …

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural scienceslaw.inventionGravitationlaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSupermassive black holeNumber densityBremsstrahlungAstronomyAstronomy and AstrophysicsAccretion (astrophysics)Stars13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaHeliosphereFlareMonthly Notices of the Royal Astronomical Society
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ELDAR, a new method to identify AGN in multi-filter surveys: the ALHAMBRA test case

2017

We present ELDAR, a new method that exploits the potential of medium- and narrow-band filter surveys to securely identify active galactic nuclei (AGN) and determine their redshifts. Our methodology improves on traditional approaches by looking for AGN emission lines expected to be identified against the continuum, thanks to the width of the filters. To assess its performance, we apply ELDAR to the data of the ALHAMBRA (Advance Large Homogeneous Area Medium Band Redshift Astronomical) survey, which covered an effective area of 2.38 deg2 with 20 contiguous medium-band optical filters down to F814W ≃ 24.5. Using two different configurations of  ELDAR in which we require the detection of at lea…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusactive [Galaxies][ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Continuum (design consultancy)FOS: Physical sciencesAstrophysicsSurveys01 natural sciencestechniques: photometricemission lines [Quasars]Galaxies: distances and redshiftssurveys0103 physical sciencesdistances and redshifts [Galaxies]Emission spectrumOptical filterdata analysis [Methods]010303 astronomy & astrophysicsPhysicsANÁLISE DE DADOSNumber density010308 nuclear & particles physicsphotometric [Techniques]galaxies: active – galaxies: distances and redshiftsAstronomy and AstrophysicsFilter (signal processing)Galaxies: activeAstrophysics - Astrophysics of Galaxiesmethods: data analysisGalaxyRedshiftquasars: emission linesSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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Enhanced crystal stability in a binary mixture of charged colloidal spheres.

2009

We report on the phase behavior of a binary charged sphere mixture of size ratio $\ensuremath{\Gamma}=0.68$ and charge ratio $\ensuremath{\Lambda}\ensuremath{\approx}1$ as a function of composition $p$ and number density $n$. For $p=0.1--0.3$ we observe freezing at densities well below the freezing densities of the pure components. At all compositions our data indicate the formation of substitutional alloy crystals of body centered cubic structure. No indications for compound formation were observed. Rather, our findings point at the first observation of an upper azeotrope. Measurements of the crystallization kinetics reveal a combined density and composition dependence of growth velocities…

CrystalColloidNumber densityMaterials scienceAzeotropePhase (matter)NucleationThermodynamicsCharge (physics)Cubic crystal systemPhysical review. E, Statistical, nonlinear, and soft matter physics
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The role of connectivity in the properties of sedimented materials

2003

Effective-medium theories for both random packings of elastic discs and mats of randomly sedimented elastic fibers can be constructed such that the effective material stiffness depends on the stiffness and geometry of the constituents of the material, and the number density of contacts. It is demonstrated that the number density of contacts together with the geometry of the constituents also determine the porosity of these materials. The simplicity and similar structure of the effective-medium estimates for the properties of these two qualitatively different materials indicate that the number density of contacts may play a similar role in an appropriate effective-medium description of a lar…

Large classNumber densityMaterials scienceMechanics of MaterialsmedicineGeneral Physics and AstronomyDeposition (phase transition)StiffnessGeneral Materials ScienceComposite materialmedicine.symptomElasticity (economics)PorosityGranular Matter
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Solidification of a colloidal hard sphere like model system approaching and crossing the glass transition

2014

We investigated the process of vitrification and crystallization in a model system of colloidal hard spheres. The kinetics of the solidification process was measured using time resolved static light scattering, while the time evolution of the dynamic properties was determined using time resolved dynamic light scattering. By performing further analysis we confirm that solidification of hard sphere colloids is mediated by precursors. Analyzing the dynamic properties we can show that the long time dynamics and thus the shear rigidity of the metastable melt is highly correlated with the number density of solid clusters (precursors) nucleated. In crystallization these objects convert into highly…

Materials scienceNumber densityNucleationGeneral ChemistryHard spheresCondensed Matter Physicslaw.inventionCondensed Matter::Soft Condensed MatterCrystallographyDynamic light scatteringChemical physicslawMetastabilityStatic light scatteringCrystallizationGlass transitionSoft Matter
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High-Yield Growth and Tunable Morphology of Bi2Se3 Nanoribbons Synthesized on Thermally Dewetted Au

2021

The yield and morphology (length, width, thickness) of stoichiometric Bi2Se3 nanoribbons grown by physical vapor deposition is studied as a function of the diameters and areal number density of the Au catalyst nanoparticles of mean diameters 8–150 nm formed by dewetting Au layers of thicknesses 1.5–16 nm. The highest yield of the Bi2Se3 nanoribbons is reached when synthesized on dewetted 3 nm thick Au layer (mean diameter of Au nanoparticles ~10 nm) and exceeds the nanoribbon yield obtained in catalyst-free synthesis by almost 50 times. The mean lengths and thicknesses of the Bi2Se3 nanoribbons are directly proportional to the mean diameters of Au catalyst nanoparticles. In contrast, the me…

Materials scienceNumber densityYield (engineering)synthesisGeneral Chemical EngineeringAnalytical chemistryNanoparticleBi<sub>2</sub>Se<sub>3</sub>ChemistryPhysical vapor depositionnanoribbonGeneral Materials ScienceDewettingQD1-999physical vapor depositionNanoscopic scaleStoichiometryDeposition (law)Nanomaterials
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Influence of corona poling procedures on linear and non-linear optical properties of polymer materials containing indandione derivatives as a cromoph…

2008

SHG efficiency of the poled guest - host polymer system is proportional to the concentration and orientation degree of NLO active molecules (chromophores). Corona poling realized at elevated temperatures could cause concentration decrease of NLO- active molecules due to centrosymmetric crystallization. Our studies showed that number density of crystallites is depending on orientation procedure. To obtain the best orientation procedure for guest - host systems containing four different chromophores based on dimethylaminobenzylidene 1, 3 - indandione we have compared optical images and SHG efficiency of corona poled films. According to our observations external poling electric field applied f…

Materials scienceNumber densitybusiness.industryPolingNonlinear opticsSecond-harmonic generationMolecular physicsCorona polinglaw.inventionCorona (optical phenomenon)lawOptoelectronicsCrystalliteCrystallizationbusinessSPIE Proceedings
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Molecular dynamics simulations of colloids: Supercooled Yukawa systems

2007

We performed molecular dynamics simulations on one and two component Yukawa systems. Cooling the system down and inspecting pair distribution functions (pdf) and bond correlation functions (bcf) we found the one component system to crystallize into a bcc-like lattice rather than an fcc lattice which is the stable phase of the simulated system at low temperatures. Upon cooling the two component system freezes into a glassy state without exhibiting crystalline structure in pdf or bcf. We define particle excess functions which show that spacial fluctuations in the number density of particles of the different components decay quite slowly. Therefore we believe that a well defined state of the t…

Molecular dynamicsNumber densityDistribution functionCondensed matter physicsChemistryChemical physicsLattice (order)Yukawa potentialPair distribution functionSupercoolingRadial distribution function
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Thermodynamics of Toda lattice models: application to DNA

1993

Abstract Our generalised Bethe ansatz method is used to formulate the statistical mechanics of the classical Toda lattice in terms of a set of coupled integral equations expressed in terms of appropriate action-angle variables. The phase space as coordinatised by these action-angle variables is constrained; and both the soliton number density and the soliton contribution to the free energy density can be shown to decouple from the phonon degrees of freedom and to depend only on soliton-soliton interactions. This makes it possible to evaluate the temperature dependence of the soliton number density which, to leading order, is found to be proportional to T 1 3 .

Number densityDegrees of freedom (physics and chemistry)Statistical and Nonlinear PhysicsStatistical mechanicsCondensed Matter PhysicsBethe ansatzNonlinear Sciences::Exactly Solvable and Integrable SystemsPhase spaceSolitonPerturbation theory (quantum mechanics)Toda latticeNonlinear Sciences::Pattern Formation and SolitonsMathematicsMathematical physicsPhysica D: Nonlinear Phenomena
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Nucleation and crystal growth in a suspension of charged colloidal silica spheres with bi-modal size distribution studied by time-resolved ultra-smal…

2014

A suspension of charged colloidal silica spheres exhibiting a bi-modal size distribution of particles, thereby mimicking a binary mixture, was studied using time-resolved ultra-small-angle synchrotron X-ray scattering (USAXS). The sample, consisting of particles of diameters d(A) = (104.7 ± 9.0) nm and d(B) = (88.1 ± 7.8) nm (d(A)/d(B) ≈ 1.2), and with an estimated composition A(0.6(1))B(0.4(1)), was studied with respect to its phase behaviour in dependance of particle number density and interaction, of which the latter was modulated by varying amounts of added base (NaOH). Moreover, its short-range order in the fluid state and its eventual solidification into a long-range ordered colloidal…

Number densityMaterials scienceSmall-angle X-ray scatteringScatteringColloidal silicacrystal growthNucleationAnalytical chemistryGeneral Physics and AstronomyCrystal growthColloidal crystalCrystallographyddc:540NucleationCrystallitecolloidal silicaPhysical and Theoretical Chemistry
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