Search results for "thermal [correlation function]"

showing 10 items of 1923 documents

Effect of Innovative Food Processing Technologies on the Physicochemical and Nutritional Properties and Quality of Non-Dairy Plant-Based Beverages

2020

Increase in allergenicity towards cow’s milk, lactose intolerance, the prevalence of hypercholesterolemia, and flexitarian choice of food consumption have increased the market for cow’s milk alternatives. Non-dairy plant-based beverages are useful alternatives because of the presence of bioactive components with health-promoting properties, which attract health-conscious consumers. However, the reduced nutritional value and sensory acceptability of the plant-based beverages (such as flavor, taste, and solubility) compared to cow’s milk pose a big threat to its place in the market. Thermal treatments are commonly used to ensure the quality of plant-based beverages during storage. However, th…

Health (social science)plant-based beveragethermal treatmentsFood consumptionReviewPlant Sciencelcsh:Chemical technologyShelf lifeHealth Professions (miscellaneous)MicrobiologyProtein digestibilitymedicinelcsh:TP1-1185Food scienceFlavorNon dairyLactose intolerancebusiness.industrynon-thermal processing technologiesfood and beveragesPlant basedmedicine.diseasesensorial propertiesFood processingbusinessFood ScienceFoods
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Heat Capacity and entanglement

2012

Starting from a recent result on thermodynamic equilibrium of quantum systems, a connection between thermal properties, originating from Gibbs state probabilistic structure, and quantum correlations is discussed as a consequence of entanglement monogamy. As an example, a simple two-qubit system is analyzed, allowing for an expression of such a connection as an explicit function linking heat capacity to a measure of bipartite entanglement.

Heat capacity entanglement concurrence thermal equilibrium
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Heat Pipe-Mediated Control of Fast and Highly Exothermal Reactions

2011

The synthesis of 1-ethyl-3-methylimidazolium ethyl-sulfate ([EMIM]EtSO4) from 1-methyl-imidazole and diethyl sulfate suffers from highly exothermal behavior. Once the activation energy barrier is reached (EA = 89 kJ mol–1), the bimolecular reaction accelerates with a high reaction enthalpy (ΔH = −130 kJ mol–1).(1-3) The excess of heat has to be concurrently dissipated to avoid hot spots or thermal runaways. Depending on the volume flow velocity of the reactants and the applied reactor temperature, the reaction zone can be shifted inside the reactor from the inlet to the outlet and vice versa. Therefore, a sophisticated thermal control, oscillating between providing activation energy and int…

Heat pipeChemistryOrganic ChemistryEnthalpyThermalReaction zoneThermodynamicsActivation energyPhysical and Theoretical ChemistryThermal controlVolumetric flow rateOrganic Process Research & Development
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Novel Wireless Sensor System for Dynamic Characterization of Borehole Heat Exchangers

2011

The design and field test of a novel sensor system based in autonomous wireless sensors to measure the temperature of the heat transfer fluid along a borehole heat exchanger (BHE) is presented. The system, by means of two specials valves, inserts and extracts miniaturized wireless sensors inside the pipes of the borehole, which are carried by the thermal fluid. Each sensor is embedded in a small sphere of just 25 mm diameter and 8 gr weight, containing a transceiver, a microcontroller, a temperature sensor and a power supply. A wireless data processing unit transmits to the sensors the acquisition configuration before the measurements, and also downloads the temperature data measured by the…

Heat pumpsEngineeringGeography & travelBoreholeMechanical engineeringlcsh:Chemical technologyBiochemistryGeothermal energyArticleAnalytical ChemistryWireless sensorsHeat exchangerThermalWirelesslcsh:TP1-1185Thermal analysisElectrical and Electronic EngineeringThermal analysisInstrumentationddc:910business.industryheat pumps; geothermal energy; thermal analysis; wireless sensorsAtomic and Molecular Physics and OpticsMicrocontrollerThermal response testMAQUINAS Y MOTORES TERMICOSTransceiverbusiness
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Spectral function of fermions in a highly occupied non-Abelian plasma

2022

We develop a method to obtain fermion spectral functions non-perturbatively in a non-Abelian gauge theory with high occupation numbers of gauge fields. After recovering the free field case, we extract the spectral function of fermions in a highly occupied non-Abelian plasma close to its non-thermal fixed point, i.e., in a self-similar regime of the non-equilibrium dynamics. We find good agreement with hard loop perturbation theory for medium-induced masses, dispersion relations and quasiparticle residues. We also extract the full momentum dependence of the damping rate of the collective excitations.

Heavy-ion collisionsNuclear and High Energy PhysicsNuclear Theoryquark-gluon plasmanonequilibrium QFTThermal QFTHigh Energy Physics - Lattice (hep-lat)Quark-gluon plasmakvarkki-gluoniplasmaFOS: Physical scienceshard-thermal loopheavy-ion collisionsspectral functionhiukkasfysiikkathermal QFT114 Physical sciencesSpectral functionNuclear Theory (nucl-th)High Energy Physics - PhenomenologyHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)Hard-thermal loopkvanttikenttäteoriaNonequilibrium QFT
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Catalytic activity of large-pore high Si/Al zeolites: Cracking of heptane on H-Beta and dealuminated HY zeolites

1987

Abstract The catalytic activity, selectivity, catalyst decay, thermal and hydrothermal stability, and acidity of H-Beta and HY zeolites with Si Al ratios of 7.5 and 10, respectively, have been studied during cracking of n-heptane at 450 °C and atmospheric pressure. It has been found that the H-Beta zeolite is more active and decays more slowly than HY. H-Beta presents a higher steric hindrance for dibranched molecules and therefore its open structure should be smaller than that of HY. A lower hydrogen transfer activity and hydrothermal stability is observed for H-Beta in comparison with the corresponding HY.

Heptanechemistry.chemical_compoundChemistryInorganic chemistryPhysical and Theoretical ChemistryZeoliteFluid catalytic crackingSelectivityChemical reactionPyrolysisCatalysisHydrothermal circulationCatalysisJournal of Catalysis
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Numerical models of blackbody-dominated gamma-ray bursts – I. Hydrodynamics and the origin of the thermal emission

2014

GRB 101225A is a prototype of the class of blackbody-dominated (BBD) gamma-ray bursts (GRBs). It has been suggested that BBD-GRBs result from the merger of a binary system formed by a neutron star and the helium core of an evolved star. We have modelled the propagation of ultrarelativistic jets through the environment left behind the merger by means of relativistic hydrodynamic simulations. In this paper, the output of our numerical models is post-processed to obtain the (thermal) radiative signature of the resulting outflow. We outline the most relevant dynamical details of the jet propagation and connect them to the generation of thermal radiation in GRB events akin to that of GRB 101225A…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curve01 natural sciencesAfterglowNeutron starCommon envelopeSpace and Planetary ScienceThermal radiation0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burst010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsMonthly Notices of the Royal Astronomical Society
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On the observability of T Tauri accretion shocks in the X-ray band

2010

Context. High resolution X-ray observations of classical T Tauri stars (CTTSs) show a soft X-ray excess due to high density plasma (n_e=10^11-10^13 cm^-3). This emission has been attributed to shock-heated accreting material impacting onto the stellar surface. Aims. We investigate the observability of the shock-heated accreting material in the X-ray band as a function of the accretion stream properties (velocity, density, and metal abundance) in the case of plasma-beta<<1 in the post-shock zone. Methods. We use a 1-D hydrodynamic model describing the impact of an accretion stream onto the chromosphere, including the effects of radiative cooling, gravity and thermal conduction. We expl…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRadiative coolingAstrophysics::High Energy Astrophysical Phenomenaaccretion accretion disks hydrodynamics shock waves stars: pre-main sequence X-rays: starsFOS: Physical sciencesAstronomy and AstrophysicsObservableAstrophysics::Cosmology and Extragalactic AstrophysicsPlasmaAstrophysicsThermal conductionAccretion (astrophysics)T Tauri starSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceThermalAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
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Observability and diagnostics in the X-ray band of shock-cloud interactions in supernova remnants

2010

X-ray emitting features originating from the interaction of supernova shock waves with small interstellar gas clouds are revealed in many X-ray observations of evolved supernova remnants (e.g. Cygnus Loop and Vela), but their interpretation is not straightforward. We develop a self-consistent method for the analysis and interpretation of shock-cloud interactions in middle-aged supernova remnants, which can provide the key parameters of the system and the role of relevant physical effects like the thermal conduction, without the need to run ad-hoc numerical simulations and to bother of morphology details. We explore all the possible values of the shock speed and cloud density contrast releva…

High Energy Astrophysical Phenomena (astro-ph.HE)Shock wavePhysicsCygnus LoopRadiative coolingAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsHydrodynamicThermal conductionVelaX-rays: ISMComputational physicsShock (mechanics)SupernovaShock waveISM: cloudSpace and Planetary ScienceDensity contrastAstrophysics - High Energy Astrophysical PhenomenaISM: supernova remnantAstrophysics::Galaxy AstrophysicsAstronomy and Astrophysics
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EINSTEIN–PLANCK FORMULA, EQUIVALENCE PRINCIPLE, AND BLACK HOLE RADIANCE

2005

The presence of gravity implies corrections to the Einstein-Planck formula $E=h \nu$. This gives hope that the divergent blueshift in frequency, associated to the presence of a black hole horizon, could be smoothed out for the energy. Using simple arguments based on Einstein's equivalence principle we show that this is only possible if a black hole emits, in first approximation, not just a single particle, but thermal radiation.

High Energy Physics - TheoryAstrofísicaPhysicsGravitacióAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsEquivalence principle (geometric)General Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyBlueshiftBlack holeGeneral Relativity and Quantum Cosmologysymbols.namesakeHigh Energy Physics - Theory (hep-th)Space and Planetary ScienceThermal radiationQuantum mechanicsHorizon (general relativity)symbolsRadianceCamps Teoria quàntica dePlanckEinsteinMathematical PhysicsInternational Journal of Modern Physics D
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