Search results for "Chemical model"

showing 10 items of 11 documents

2D Hydro-Mechanical-Chemical Modeling of (De)hydration Reactions in Deforming Heterogeneous Rock: The Periclase-Brucite Model Reaction

2020

Deformation at tectonic plate boundaries involves coupling between rock deformation, fluid flow, and metamorphic reactions, but quantifying this coupling is still elusive. We present a new two-dimensional hydro-mechanical-chemical numerical model and investigate the coupling between heterogeneous rock deformation and metamorphic (de)hydration reactions. We consider linear viscous compressible and power-law viscous shear deformation. Fluid flow follows Darcy's law with a Kozeny-Carman type permeability. We consider a closed isothermal system and the reversible (de)hydration reaction: periclase and water yields brucite. Fluid pressure within a circular or elliptical inclusion is initially bel…

010504 meteorology & atmospheric sciencesShear zoneChemical process modelingMetamorphic rockThermodynamicsNumerical simulationengineering.materialDeformation (meteorology)010502 geochemistry & geophysics01 natural sciencesPhysics::GeophysicsPhysics::Fluid DynamicsGeochemistry and PetrologyFluid dynamicsCoupling (piping)Brucite-Periclase reaction0105 earth and related environmental sciencesBruciteReaction-induced weakeningGeophysics13. Climate actionengineeringHydro-Mechanical-Chemical modelPericlaseShear zoneGeologyRock deformation coupled to reactions
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Oxygen depletion in dense molecular clouds: a clue to a low O2 abundance?

2011

Context: Dark cloud chemical models usually predict large amounts of O2, often above observational limits. Aims: We investigate the reason for this discrepancy from a theoretical point of view, inspired by the studies of Jenkins and Whittet on oxygen depletion. Methods: We use the gas-grain code Nautilus with an up-to-date gas-phase network to study the sensitivity of the molecular oxygen abundance to the oxygen elemental abundance. We use the rate coefficient for the reaction O + OH at 10 K recommended by the KIDA (KInetic Database for Astrochemistry) experts. Results: The updates of rate coefficients and branching ratios of the reactions of our gas-phase chemical network, especially N + C…

AstrochemistryChemical models[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Analytical chemistrychemistry.chemical_elementFOS: Physical sciencesAstrophysicsAstrophysicsKinetic energy01 natural sciencesOxygen[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesSolar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010304 chemical physics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Molecular cloudAstronomy and Astrophysicsastrochemistry; ISM; abundances; ISM; molecules; ISM; individual objects; L134N; ISM; individual objects; TMC-1[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]NitrogenchemistryAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceMolecular oxygenChemical network
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Fluid geochemistry in a low-enthalpy geothermal field along a sector of southern Apennines chain (Italy)

2020

Abstract The chemical and isotopic features of the fluids (water and gases) in the Lucane thermal area (southern Italy) have been investigated in order to verify their origin, water temperature in the geothermal reservoir, and to recognize the main natural processes concerning the water composition during ascent towards the surface. The Lucane geothermal system is placed in the southern sector of the Apennines chains, a seismically active area, close to the southern base of the Mt. Alpi carbonate massif. Along the study area, two main sets of high-angle faults form an almost orthogonal fault system that, as suggested by local structural geology, acts as a preferential pathway for uprising d…

Calcitegeographygeography.geographical_feature_categoryδ18ODolomiteGeochemistryDeep-sourced volatiles Geochemical model Geothermometry and heat discharge Low enthalpy geothermal system Water-rock interaction Mt. Alpi massifMassif010501 environmental sciences010502 geochemistry & geophysics01 natural sciencesSettore GEO/08 - Geochimica E Vulcanologiachemistry.chemical_compoundIsotopic signaturechemistryGeochemistry and PetrologyCarbonateCarbonate rockEconomic GeologyGeothermal gradientGeology0105 earth and related environmental sciences
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Modelling the effect of ascorbic acid, sodium metabisulphite and sodium chloride on the kinetic responses of lactic acid bacteria and yeasts in table…

2010

he goal of this work was to apply the Quasi-chemical primary model (a system of four ordinary differential equations that derives from a hypothetical four-step chemical mechanism involving an antagonistic metabolite) in the study of the evolution of yeast and lactic acid bacteria populations during the storage of Manzanilla–Aloreña table olives subjected to different mixtures of ascorbic acid, sodium metabisulphite and NaCl. Firstly, the Quasi-chemical model was applied to microbial count data to estimate the growth–decay biological parameters. The model accurately described the evolution of both populations during storage, providing detailed information on the microbial behaviour. Secondly…

Food HandlingTable oliveSodiumColony Count MicrobialQuasi-chemical modelchemistry.chemical_elementAscorbic AcidSodium ChlorideModels BiologicalMicrobiologychemistry.chemical_compoundOleaYeastsLactic acid bacteriaSulfitesPrimary modellingFood sciencebiologyFood preservationGeneral MedicineSodium metabisulfiteLactobacillaceaebiology.organism_classificationAscorbic acidYeastLactic acidchemistryBiochemistryLactobacillaceaeFruitFermentationFood MicrobiologyFermentationFood ScienceInternational Journal of Food Microbiology
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The geochemical riddle of “low-salinity gypsum” deposits

2022

International audience; Gypsum makes up about one fifth of giant salt deposits formed by evaporation of seawater throughout Earth’s history. Although thermodynamic calculations and precipitation experiments predict that gypsum precipitates when the salinity of evaporating seawater attains about 110 g kg-1, gypsum deposits of the Mediterranean Salt Giant often bear the geochemical signature of precipitation from less saline water masses. Addressing this geochemical riddle is important because marine gypsum deposition and continental gypsum erosion affect the global carbon cycle. We investigated gypsum deposits formed in the marginal basins of the Mediterranean Sea during the Messinian Salini…

Geochemistry and Petrology[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/GeochemistryGeochemical modelingLow-salinity gypsumSettore GEO/01 - Paleontologia E PaleoecologiaHydration water isotopes (δBiogeochemical S cycleFluid inclusionsSettore GEO/08 - Geochimica E Vulcanologia
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Geochemical modeling of evaporation processes on Mars: Insight from the sedimentary record at Meridiani Planum

2005

New data returned from the Mars Exploration Rover (MER) mission have revealed abundant evaporites in the sedimentary record at Meridiani Planum. A working hypothesis for Meridiani evaporite formation involves the evaporation of fluids derived from the weathering of martian basalt and subsequent diagenesis. On Earth, evaporite formation in exclusively basaltic settings is rare. However, models of the evaporation of fluids derived from experimentally weathering synthetic martian basalt provide insight into possible formation mechanisms. The thermodynamic database assembled for this investigation includes both Fe2+ and Fe3+ in Pitzer's ion interaction equations to evaluate Fe redox disequilibr…

Meridiani PlanumMartianEvaporiteGeochemistryengineering.materialDiagenesisGeophysicsSpace and Planetary ScienceGeochemistry and PetrologyJarositeEarth and Planetary Sciences (miscellaneous)engineeringSedimentary rockComposition of MarsGeologyGeochemical modelingEarth and Planetary Science Letters
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The 2014 KIDA network for interstellar chemistry

2015

Chemical models used to study the chemical composition of the gas and the ices in the interstellar medium are based on a network of chemical reactions and associated rate coefficients. These reactions and rate coefficients are partially compiled from data in the literature, when available. We present in this paper kida.uva.2014, a new updated version of the kida.uva public gas-phase network first released in 2012. In addition to a description of the many specific updates, we illustrate changes in the predicted abundances of molecules for cold dense cloud conditions as compared with the results of the previous version of our network, kida.uva.2011.

Physics[PHYS]Physics [physics][ PHYS ] Physics [physics]Chemical models[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsChemical reactionAstrophysics - Astrophysics of GalaxiesInterstellar medium13. Climate actionSpace and Planetary ScienceChemical physics[ SDU.ASTR.CO ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics of Galaxies (astro-ph.GA)MoleculeChemical compositionComputingMilieux_MISCELLANEOUS
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A Hooke's law-based approach to protein folding rate

2014

Kinetics is a key aspect of the renowned protein folding problem. Here, we propose a comprehensive approach to folding kinetics where a polypeptide chain is assumed to behave as an elastic material described by the Hooke[U+05F3]s law. A novel parameter called elastic-folding constant results from our model and is suggested to distinguish between protein with two-state and multi-state folding pathways. A contact-free descriptor, named folding degree, is introduced as a suitable structural feature to study protein-folding kinetics. This approach generalizes the observed correlations between varieties of structural descriptors with the folding rate constant. Additionally several comparisons am…

Statistics and ProbabilityPROTDCALStructure analysisGeneral Biochemistry Genetics and Molecular BiologyArticleProtein Structure SecondaryAmino acid sequencesymbols.namesakeProtein structureEnergeticsFeature (machine learning)Statistical physicsProtein foldingTheoretical modelProtein secondary structureReaction kineticsGeneral Immunology and MicrobiologyChemical modelApplied MathematicsProteinHooke's lawModelingProteinsGeneral MedicineDNAComputer simulationElasticityFolding degreeFolding (chemistry)ChemistryKineticsModels ChemicalModeling and SimulationPeptidesymbolsProtein structureElastic folding constantPhysical chemistryProtein secondary structureThermodynamicsProtein foldingDownhill foldingPolypeptideGeneral Agricultural and Biological SciencesConstant (mathematics)Folding kinetics
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Fe-periclase reactivity at Earth's lower mantle conditions: Ab-initio geochemical modelling

2017

Intrinsic and extrinsic stability of the (Mg, Fe) O solid mixture in the Fe-Mg-Si-O system at high P, T conditions relevant to the Earth's mantle is investigated by the combination of quantum mechanical calculations (Hartree-26 Fock/DFT hybrid scheme), cluster expansion techniques and statistical thermodynamics. Iron in the (Mg, Fe) O binary mixture is assumed to be either in the low spin (LS) or in the high spin (HS) state. Un-mixing at solid state is observed only for the LS condition in the 23-42 GPa pressure range, whereas HS does not give rise to un-mixing. LS (Mg, Fe) O un-mixings are shown to be able to incorporate iron by subsolidus reactions with a reservoir of a virtual bridgmanit…

Subsolidus reaction modellingMgO-FeO binary010504 meteorology & atmospheric sciencesSilicate perovskiteLower mantle geochemical heterogeneitiesAnalytical chemistryAb initioLower mantle geochemical heterogeneities MgO-FeO binary Mixing Gibbs energy Pyrolitic geochemical mode Subsolidus reaction modellingMineralogyengineering.material010502 geochemistry & geophysics01 natural sciencesMantle (geology)Geochemistry and PetrologyMixing Gibbs energy0105 earth and related environmental sciencesPyrolitic geochemical modeSettore GEO/06 - MineralogiaPyrolitic geochemical modelAmbientaleDiamondHartreePartition coefficientengineeringPericlaseMgO-FeO binaryPyrolitic geochemical modelLower mantle geochemical heterogeneitiesSubsolidus reaction modellingMixing Gibbs energyGeologyCluster expansion
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Building molecular models using screw-on bottle caps

2013

Chemical models can be built using screw-on bottle caps. Two identical caps can be joined together by thermal welding to form atoms, and the resulting atoms can be joined together by welding or by hot polymer glue to form molecules. The method is easy, can be applied at every level of chemical education, and gives access to an unlimited number of models at almost no cost. It inspires hands-on activity of pupils and can be used to show the dependence between the three-dimensional structure of molecules and their chemical, physical, and biological features.

chemistry.chemical_classificationMolecular modelChemical modelsChemistryNanotechnologyGeneral ChemistryWeldingPolymerEducationlaw.inventionlawThermalMoleculeBottle capJournal of Chemical Education
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