Search results for "waves"

showing 10 items of 1766 documents

Solvent-free microwave-assisted extraction of polyphenols from olive tree leaves: Antioxidant and antimicrobial properties

2017

International audience; Response surface methodology (RSM) and artificial neural networks (ANN) were evaluated and compared in order to decide which method was the most appropriate to predict and optimize total phenolic content (TPC) and oleuropein yields in olive tree leaf (Olea europaea) extracts, obtained after solvent-free microwave- assisted extraction (SFMAE). The SFMAE processing conditions were: microwave irradiation power 250-350 W, extraction time 2-3 min, and the amount of sample 5-10 g. Furthermore, the antioxidant and antimicrobial activities of the olive leaf extracts, obtained under optimal extraction conditions, were assessed by several in vitro assays. ANN had better predic…

Antioxidantmedicine.medical_treatment[SDV]Life Sciences [q-bio]Pharmaceutical ScienceAntioxidantsAnalytical Chemistrychemistry.chemical_compoundDrug Discovery[SDV.IDA]Life Sciences [q-bio]/Food engineeringAntimicrobial; Antioxidant; Oleuropein; Olive leaves; Optimization; Solvent-free microwave extraction; Organic ChemistryOlive leavesMicrowaves04 agricultural and veterinary sciences040401 food scienceAnti-Bacterial AgentsChemistry (miscellaneous)Molecular MedicineAntioxidantAntibacterial activityOptimizationStaphylococcus aureusMicrobial Sensitivity TestsArticlelcsh:QD241-4410404 agricultural biotechnologyOlive leaflcsh:Organic chemistryOleuropeinOleaStaphylococcus epidermidismedicine[SPI.GPROC]Engineering Sciences [physics]/Chemical and Process EngineeringResponse surface methodologyPhysical and Theoretical ChemistryOleuropeinolive leaves; solvent-free microwave extraction; oleuropein; antioxidant; antimicrobial; optimizationChromatographyPlant ExtractsExtraction (chemistry)Organic ChemistryPolyphenolsolive leaves;solvent-free microwave extraction;oleuropein;antioxidant;antimicrobial;optimizationPlant LeaveschemistryPolyphenolYield (chemistry)Solvent-free microwave extractionSolventsAntimicrobialNeural Networks Computer
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A study on the essential oil Ferulago campestris. How much does exstraction method influence the oil composition?

2010

The essential oil of different parts of Ferulago campestris (Bess.) collected in Sicily has been extracted by microwave-assisted hydrodistillation (MAHD) and by classic hydrodistillation (HD). A comparative qualitative- quantitative study on the composition of the oils was carried out. A total of 100 compounds were identified in the oils obtained by MAHD, whereas 88 compounds characterized the HD oils. The most prominent components were, in all different parts of F. campestris and in both extraction methods, 2,4,5- trimethylbenzaldehyde and 2,4,6-trimethylbenzaldehyde isomers; the latter was not previously found. The attempt to evaluate where the oil components are located in all parts of t…

Apiaceae / Essential oils / Ferulago campestris / Kinetic of microwave extraction / Microwaves hydrodistillationIsomerismKinetic of microwave extractionMicrowaves hydrodistillationOils VolatilePlant OilsSettore CHIM/06 - Chimica OrganicaMicrowavesEssential oilDistillationApiaceaeFerulago campestri
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On the Computational Aspects of a Symmetric Multidomain Boundary Element Method Approach for Elastoplastic Analysis

2011

The symmetric boundary element method (SBEM) is applied to the elasto-plastic analysis of bodies subdivided into substructures. This methodology is based on the use of: a multidomain SBEM approach, for the evaluation of the elastic predictor; a return mapping algorithm based on the extremal paths theory, for the evaluation of inelastic quantities characterizing the plastic behaviour of each substructure; and a transformation of the domain inelastic integrals of each substructure into corresponding boundary integrals. The elastic analysis is performed by using the SBEM displacement approach, which has the advantage of creating system equations that only consist of nodal kinematical unknowns…

Applied MathematicsMechanical EngineeringMathematical analysisPhase (waves)Boundary (topology)GeometryFunction (mathematics)Displacement (vector)Domain (mathematical analysis)Transformation (function)Mechanics of MaterialsModeling and SimulationSubstructureBoundary element methodMathematicsThe Journal of Strain Analysis for Engineering Design
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Space charge and induced dipole relaxation in solid electrolytes

1996

The space charge relaxation and induced dipole relaxation in solid electrolytes is discussed. The di-electric responses of these relaxations gives a satisfactory fit to the universal conductivity behaviours in the frequency range from DC to infrared.

Arrhenius equationCondensed matter physicsChemistryInfraredGeneral ChemistryConductivityCondensed Matter PhysicsPolarization (waves)Space chargeDipolesymbols.namesakeElectrical resistivity and conductivityFast ion conductorsymbolsPhysical chemistryGeneral Materials Science
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Stability of impulsive differential systems

2013

The asymptotic phase property and reduction principle for stability of a trivial solution is generalized to the case of the noninvertible impulsive differential equations in Banach spaces whose linear parts split into two parts and satisfy the condition of separation.

Article SubjectDifferential equationlcsh:MathematicsApplied MathematicsMathematical analysisPhase (waves)Banach spacelcsh:QA1-939Differential systemsStability (probability)Trivial solution:MATHEMATICS::Applied mathematics [Research Subject Categories]Reduction (mathematics)AnalysisMathematics
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Simultaneous segmentation and beam-hardening correction in computed microtomography of rock cores

2013

We propose a post-reconstruction correction procedure for the beam-hardening artifact that neither requires knowledge of the X-ray spectrum nor of the attenuation coefficients in multi-mineral geologic samples. The beam-hardening artifact in polychromatic X-ray computer tomography (CT) hampers segmentation of the phase assemblage in geologic samples. We show that in cylindrically shaped samples like rock cores, the X-ray attenuation value for a single phase depends mainly on the distance from the center of the cylinder. This relationship could be easily extracted from the CT data for every phase and used to infer the presence of these phases at all positions in the sample. Our new approach …

Artifact (error)Materials scienceAttenuationPhase (waves)MineralogyCylinderGeometrySegmentationImage segmentationTomographyComputers in Earth SciencesSample (graphics)Information SystemsComputers & Geosciences
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Astrophysics with the Laser Interferometer Space Antenna

2023

Full list of authors: Amaro-Seoane, Pau; Andrews, Jeff; Sedda, Manuel Arca; Askar, Abbas.; Baghi, Quentin; Balasov, Razvan; Bartos, Imre; Bavera, Simone S.; Bellovary, Jillian; Berry, Christopher P. L.; Berti, Emanuele; Bianchi, Stefano; Blecha, Laura; Blondin, Stephane; Bogdanovic, Tamara; Boissier, Samuel; Bonetti, Matteo; Bonoli, Silvia; Bortolas, Elisa; Breivik, Katelyn; Capelo, Pedro R.; Caramete, Laurentiu; Cattorini, Federico; Charisi, Maria; Chaty, Sylvain; Chen, Xian; Chruslinska, Martyna; Chua, Alvin J. K.; Church, Ross; Colpi, Monica; D'Orazio, Daniel; Danielski, Camilla; Davies, Melvyn B.; Dayal, Pratika; De Rosa, Alessandra; Derdzinski, Andrea; Destounis, Kyriakos; Dotti, Massi…

AstrofísicaACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Black holeAstronomyStellar remnantFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)TIDAL DISRUPTION EVENTSGeneral Relativity and Quantum CosmologyGravitational wavesMOCCA-SURVEY DATABASESettore FIS/05 - Astronomia e AstrofisicaStellar remnantsSoftware ScienceMulti-messengerGRAVITATIONAL-WAVE SOURCESInstrumentation and Methods for Astrophysics (astro-ph.IM)Extreme mass ratio in-spiralsSolar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)Black holes; Extreme mass ratio in-spirals; Gravitational waves; Multi-messenger; Stellar remnantsBlack holesData ScienceAstrophysics::Instrumentation and Methods for AstrophysicsExtreme mass ratio in-spiralAM-CVN STARSAstrophysics - Astrophysics of GalaxiesWHITE-DWARF BINARIESDOUBLE NEUTRON-STARSAstrophysics - Solar and Stellar Astrophysics[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)AstronomiaMASSIVE BLACK-HOLEAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsX-RAY BINARIESCOMMON-ENVELOPE EVOLUTIONGravitational waveAstrophysics - Cosmology and Nongalactic Astrophysics
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Polarization calibration techniques for the new-generation VLBI

2020

The calibration and analysis of polarization observations in Very Long Baseline Interferometry (VLBI) requires the use of specific algorithms that suffer from several limitations, closely related to assumptions in the data properties that may not hold in observations taken with new-generation VLBI equipment. Nowadays, the instantaneous bandwidth achievable with VLBI backends can be as high as several GHz, covering several radio bands simultaneously. In addition, the sensitivity of VLBI observations with state-of-the-art equipment may reach dynamic ranges of tens of thousands, both in total intensity and in polarization. In this paper, we discuss the impact of the limitations of common VLBI …

AstrofísicaAstronomyAstrophysics::High Energy Astrophysical PhenomenaPolarimetryFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio spectrumInstantaneous bandwidthSoftware0103 physical sciencesVery-long-baseline interferometry010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsRemote sensingPhysicsEvent Horizon Telescope010308 nuclear & particles physicsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsPolarization (waves)Nonlinear systemSpace and Planetary ScienceAstronomiabusinessAstrophysics - Instrumentation and Methods for Astrophysics
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The Polarized Image of a Synchrotron-emitting Ring of Gas Orbiting a Black Hole

2021

Full list of authors: Narayan, Ramesh; Palumbo, Daniel C. M.; Johnson, Michael D.; Gelles, Zachary; Himwich, Elizabeth; Chang, Dominic O.; Ricarte, Angelo; Dexter, Jason; Gammie, Charles F.; Chael, Andrew A.; Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Algaba, Juan Carlos; Anantua, Richard; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David Baloković, Mislav; Barrett, John; Benson, Bradford A.; Bintley, Dan; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Domini…

AstrofísicaCamps magnèticsAccretion010504 meteorology & atmospheric sciencesAstronomyAstrophysics::High Energy Astrophysical PhenomenaStrong gravitational lensingSynchrotron radiationFOS: Physical sciencesF50001 natural sciencesAstrophysics - high energy astrophysical phenomena994General Relativity and Quantum Cosmology0103 physical sciencesPolarimetrySchwarzschild metric010303 astronomy & astrophysics0105 earth and related environmental sciences162astro-ph.HEEvent Horizon TelescopePhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)1278Accretion (meteorology)Black holes14Astronomy and AstrophysicsPolarization (waves)Computational physicsMagnetic fieldBlack holeSpace and Planetary ScienceMagnetic fields14 162 1278 994
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GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

2019

We present the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1$\mathrm{M}_\odot$ during the first and second observing runs of the Advanced gravitational-wave detector network. During the first observing run (O1), from September $12^\mathrm{th}$, 2015 to January $19^\mathrm{th}$, 2016, gravitational waves from three binary black hole mergers were detected. The second observing run (O2), which ran from November $30^\mathrm{th}$, 2016 to August $25^\mathrm{th}$, 2017, saw the first detection of gravitational waves from a binary neutron star inspiral, in addition to the observation of gravitational waves from a total of seven binary …

AstrofísicaDYNAMICSGravitacióneutron star: binaryAstronomyGeneral Physics and AstronomyBinary numberAstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology010305 fluids & plasmasgravitational waves black holesAstrophysicSIGNALSPopulation DistributionsLIGOQCQBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HESettore FIS/01gravitational radiation detector: networkPROGENITORSPhysicsgravitational wavesPhysical Sciencesastro-ph.CO[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaMETALLICITYAstrophysics - Cosmology and Nongalactic AstrophysicsGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)QC1-999gr-qcAstrophysics::High Energy Astrophysical PhenomenaPhysics MultidisciplinaryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsMASSAstrophysics; GravitationGeneral Relativity and Quantum CosmologyBinary black holebinary: coalescenceSYSTEMS0103 physical sciences010306 general physicsSTFCScience & TechnologyGravitational wavegravitational radiationRCUKGravitational Wave Physicsbinary: compactLIGOEVOLUTIONBlack holeNeutron starVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionBLACK-HOLERADIATIONINFERENCE[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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