Search results for "Pitzer."

showing 10 items of 28 documents

Modeling S-carboxymethyl-L-cysteine protonation and activity coefficients in sodium and tetramethylammonium chloride aqueous solutions by SIT and Pit…

2007

Solubility and acid–base properties of S-carboxymethyl-l-cysteine (carbocysteine, ccys) in NaClaq and tetramethylammonium chloride, (CH3)4NClaq ,a tt =2 5 ◦ C and at different ionic strengths were investigated. Solubility was studied at 1.0 ≤ I (mol L −1 ) ≤ 5.0 for NaClaq and 1.0 ≤ I (mol L −1 ) ≤ 3.0 for (CH3)4NClaq, while potentiometric measurements (by ISE-H + , glass electrode) were performed at 0.1 ≤ I (mol L −1 ) ≤ 5.0 for NaClaq and 0.5 ≤ I (mol L −1 ) ≤ 3.0 for (CH3)4NClaq. Solubility data allowed us to determine Setschenow constants and activity coefficients of neutral carbocysteine (H2ccys). Dependence on ionic strength and ionic medium of protonation constants and activity coeff…

Activity coefficientChemistryGeneral Chemical EngineeringPotentiometric titrationInorganic chemistryAnalytical chemistryGeneral Physics and AstronomyProtonationchemistry.chemical_compoundSpecific ion interaction theoryIonic strengthTetramethylammonium chloridePitzer equationsPhysical and Theoretical ChemistrySolubilityCarbocysteine; Solubility; Protonation; Activity coefficients; Dependence on medium and ionic strength
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Hydrolysis and chemical speciation of dioxouranium(VI) ion in aqueous media simulating the major ion composition of seawater

2004

Abstract The hydrolysis and chemical speciation of the dioxouranium(VI) ion at 25 °C was studied in a number of binary electrolytes (LiCl, NaCl, MgCl2, CaCl2, Na2SO4) and some mixtures (NaCl–Na2SO4, NaNO3–Na2SO4, CaCl2–MgCl2) as well as artificial seawater (SSWE) as a function of ionic strength. The results in LiCl, CaCl2 and MgCl2 solutions confirmed the formation of (UO2)2(OH)22+, (UO2)3(OH)42+, (UO2)3(OH)5+ and (UO2)3(OH)7− species (at I=0 mol l−1: log Tβ22=−5.76, log Tβ34=−11.82, log Tβ35=−15.89 and log Tβ37=−29.26). For NaNO3, NaCl and artificial seawater the hydrolysis constant for the formation of the UO2(OH)+ species was also determined (at I=0 mol l−1: log Tβ11=−5.19). The results …

Activity coefficientHydrolysis constantUranium speciationAqueous solutionChemistryHydrolysisInorganic chemistryPitzer parametersIonic bondingArtificial seawaterGeneral ChemistryDependence on ionic strengthOceanographyUranylIon pair formationIonDioxouranium(VI)chemistry.chemical_compoundIonic strengthEnvironmental ChemistryChemical speciationHydrolysis; Dioxouranium(VI); Chemical speciation; Seawater; Dependence on ionic strength; Dependence on ionic medium; Pitzer parameters; Ion pair formationSeawaterDependence on ionic mediumWater Science and Technology
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Novel solutions for closed-loop Reverse Electrodialysis: thermodynamic characterisation and perspective analysis

2019

Abstract Closed-loop Reverse Electrodialysis is a novel technology to directly convert low-grade heat into electricity. It consists of a reverse electrodialysis (RED) unit where electricity is produced exploiting the salinity gradient between two salt-water solutions, coupled with a regeneration unit where waste-heat is used to treat the solutions exiting from the RED unit and restore their initial composition. One of the most important advantages of closed-loop systems compared to the open systems is the possibility to select ad-hoc salt solutions to achieve high efficiencies. Therefore, the properties of the salt solutions are essential to assess the performance of the energy generation a…

Activity coefficientMaterials science020209 energyThermodynamicschemistry.chemical_elementSalt (chemistry)02 engineering and technologyIndustrial and Manufacturing Engineering020401 chemical engineeringReversed electrodialysis0202 electrical engineering electronic engineering information engineeringOsmotic coefficient0204 chemical engineeringElectrical and Electronic EngineeringCivil and Structural Engineeringchemistry.chemical_classificationMolalityAqueous solutionMechanical EngineeringBuilding and ConstructionPollution6. Clean waterGeneral EnergyElectricity generationchemistryCaesiumClosed loop reverse electrodialysis Multi-stage evaporative regeneration unit Potassium acetate Caesium acetate Osmotic coefficient Pitzer's model.
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Modeling ATP protonation and activity coefficients in NaClaq and KClaq by SIT and Pitzer equations.

2006

Abstract The acid–base properties of Adenosine 5′-triphosphate (ATP) in NaCl and KCl aqueous solutions at different ionic strengths (0  I  / mol L − 1  ≤ 5 for NaCl aq , 0  I  / mol L − 1  ≤ 3 for KCl aq ) and at t  = 25 °C were investigated. A selection of literature data on ATP protonation constants and on activity isopiestic coefficients was performed, together with new potentiometric measurements (by ISE-H + , glass electrode). Both literature and new experimental data were used to model the dependence on ionic strength and ionic medium of ATP protonation by SIT (Specific ion Interaction Theory) and Pitzer equations. In addition to values of first and second ATP protonation constants in…

Activity coefficientMolar concentrationactivity coefficientsActivity coefficientPotentiometric titrationInorganic chemistryBiophysicsIonic bondingProtonationProtonationATP; protonation; activity coefficients; Dependence on medium and ionic strength; SIT model; Pitzer modelSodium ChlorideBiochemistryPotassium ChlorideAdenosine TriphosphateElectrochemistrySettore CHIM/01 - Chimica AnaliticaChemistryOrganic ChemistryOsmolar ConcentrationPitzer modelSIT modelATPSpecific ion interaction theoryIonic strengthDependence on medium and ionic strengthPhysical chemistryPitzer equationsBiophysical chemistry
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A stellar flare-coronal mass ejection event revealed by X-ray plasma motions

2019

Coronal mass ejections (CMEs), often associated with flares, are the most powerful magnetic phenomena occurring on the Sun. Stars show magnetic activity levels up to 10^4 times higher, and CME effects on stellar physics and circumstellar environments are predicted to be significant. However, stellar CMEs remain observationally unexplored. Using time-resolved high-resolution X-ray spectroscopy of a stellar flare on the active star HR 9024 observed with Chandra/HETGS, we distinctly detected Doppler shifts in S XVI, Si XIV, and Mg XII lines that indicate upward and downward motions of hot plasmas (~10-25 MK) within the flaring loop, with velocity v~100-400 km/s, in agreement with a model of fl…

Angular momentumX-ray Astronomy010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaStars: flareFOS: Physical sciencesAstrophysicsKinetic energy01 natural scienceslaw.inventionSpitzer Space Telescopelaw0103 physical sciencesCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsStars: coronae010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsStarsAstrophysics - Solar and Stellar AstrophysicsStellar physicsPhysics::Space PhysicsStars: CMEAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFlare
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The interaction of amino acids with the major constituents of natural waters at different ionic strengths

2000

Abstract The interaction of amino acids with the major constituents of natural waters has been studied potentiometrically by determining protonation constants at different ionic strengths (e.g., I ≤5.6 mol (kg H 2 O) −1 (NaCl)) and in artificial seawater (containing Na + , K + , Ca 2+ , Mg 2+ , Cl − and SO 4 2− ) at different salinities. For glycine determinations in mixed NaCl–MgCl 2 , electrolyte solutions were also performed. The data included in this work, together with some already published, make it possible to calculate parameters for dependence on ionic strength using different models, i.e. an extended Debye–Huckel type equation and Pitzer equations. The results can be interpreted b…

Aqueous solutionChemistryInorganic chemistryIonic bondingArtificial seawaterProtonationGeneral ChemistryOceanographyIonic strengthStability constants of complexesEnvironmental ChemistryPitzer equationsSeawaterWater Science and Technology
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Protonation of Carbonate in Aqueous Tetraalkylammonium Salts at 25°C.

2006

Protonation constants of carbonate were determined in tetramethylammonium chloride (Me4NClaq 0.1≤I/mol kg−1 ≤4) and tetraethylammonium iodide (Et4NIaq 0.1≤I/mol kg−1 ≤1) by potentiometric ([H+]-glass electrode) measurements. Dependence of protonation constants on ionic strength was taken into account by modified specific ion interaction theory (SIT) and by Pitzer models. Literature data on the protonation of carbonate in NaClaq (0.1≤I/mol kg−1 ≤6) were also critically analysed. Both protonation constants of carbonate follow the trend Et4NI>Me4NCl > NaCl. An ion pair formation model designed to take into account the different protonation behaviours of carbonate in different supporting electr…

Aqueous solutionProtonation of carbonateSpecific ion interaction theory (SIT)Ion pair formation modelChemistryInorganic chemistryTetraalkylammonium saltProtonationDependence on ionic strengthElectrolyteIon pairsAnalytical Chemistrychemistry.chemical_compoundIonic strengthTetramethylammonium chlorideAqueous solutionPitzer equationsCarbonateSettore CHIM/01 - Chimica AnaliticaProtonation of carbonate; Dependence on ionic strength; Aqueous solution; Tetraalkylammonium salts; Ion pair formation model; Specific ion interaction theory (SIT); Pitzer equationPitzer equation
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SAX J1808.4-3658, an accreting millisecond pulsar shining in gamma rays?

2016

We report the detection of a possible gamma-ray counterpart of the accreting millisecond pulsar SAX J1808.4-3658. The analysis of ~6 years of data from the Large Area Telescope on board the Fermi Gamma-ray Space Telescope (Fermi-LAT) within a region of 15deg radius around the position of the pulsar reveals a point gamma-ray source detected at a significance of ~6 sigma (Test Statistic TS = 32), with position compatible with that of SAX J1808.4-3658 within 95% Confidence Level. The energy flux in the energy range between 0.6 GeV and 10 GeV amounts to (2.1 +- 0.5) x 10-12 erg cm-2 s-1 and the spectrum is well-represented by a power-law function with photon index 2.1 +- 0.1. We searched for si…

Astrophysics::High Energy Astrophysical PhenomenaPulsar planetEnergy fluxFOS: Physical sciencesGamma-rays: starAstrophysics01 natural sciencesBinary pulsarSettore FIS/05 - Astronomia E AstrofisicaSpitzer Space TelescopePulsarMillisecond pulsar0103 physical sciences010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsStars: neutronStars: individual: SAX J1808.4-3658Space and Planetary ScienceOrbital motionstars; Stars: individual: SAX J1808.4-3658; Stars: neutron; Space and Planetary Science; Astronomy and Astrophysics [Gamma-rays]Astrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space Telescope
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Multiple accelerated particle populations in the Cygnus Loop with Fermi-LAT

2021

The Cygnus Loop (G74.0-8.5) is a very well-known nearby supernova remnant (SNR) in our Galaxy. Thanks to its large size, brightness, and angular offset from the Galactic plane, it has been studied in detail from radio to $\gamma$-ray emission. The $\gamma$ -rays probe the populations of energetic particles and their acceleration mechanisms at low shock speeds. We present an analysis of the $\gamma$-ray emission detected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope over 11 years in the region of the Cygnus Loop. We performed detailed morphological and spectral studies of the $\gamma$-ray emission toward the remnant from 100 MeV to 100 GeV and compared it with X-ra…

Astrophysics::High Energy Astrophysical Phenomenabrightnesscosmic radiation: energyFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeV01 natural sciencesGLASTthermalX-raycosmic raysSpitzer Space Telescope0103 physical sciencesultravioletsupernovaRadiative transferopticalcloudcosmic radiation: acceleration010306 general physicsSupernova remnant010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsacceleration of particlesISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cygnus LoopAstronomy and Astrophysicsshock wavesGalactic planeGalaxy13. Climate actionSpace and Planetary Sciencegamma raystatisticsspectralgalaxyAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Fermi Gamma-ray Space Telescope
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Evaluation of saltwork ponds operation through brine characterization and geochemical modelling using PHREEQC code integrating the Pitzer correction

2021

Seawater represents a potential resource for the extraction of salts and raw materials [1]. About one-third of the global table-salt production is manufactured in solar saltworks [2], being the most representative product of seawater processing. However, other valuable compounds such as Magnesium, Lithium and trace elements belonging to the alkaline/alkaline-earth metals (e.g. Rb, Cs, Sr) and transition/post-transition metals (e.g. Co, Ga, Ge) are present. Many of these elements are included in the EU Critical Raw Materials (CRM) list, grouping natural assets classified as fundamental for the wealth of the socio-economic structure of Europe [3]. In saltworks, natural evaporation of seawater…

BrineCritical Raw MaterialSaltworkPitzer.PHREEQCTrace element
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