Search results for "PARTICLES"

showing 10 items of 8085 documents

Implementation of local chiral interactions in the hyperspherical harmonics formalism

2021

With the goal of using chiral interactions at various orders to explore properties of the few-body nuclear systems, we write the recently developed local chiral interactions as spherical irreducible tensors and implement them in the hyperspherical harmonics expansion method. We devote particular attention to three-body forces at next-to-next-to leading order, which play an important role in reproducing experimental data. We check our implementation by benchmarking the ground-state properties of $^3$H, $^3$He and $^4$He against the available Monte Carlo calculations. We then confirm their order-by-order truncation error estimates and further investigate uncertainties in the charge radii obta…

Chiral perturbation theoryNuclear TheoryTruncation error (numerical integration)Formalism (philosophy)Materials Science (miscellaneous)QC1-999Monte Carlo methodBiophysicsGeneral Physics and AstronomyFOS: Physical sciences01 natural scienceschiral effective field theoryNuclear Theory (nucl-th)Theoretical physics0103 physical sciencesPhysical and Theoretical Chemistry010306 general physicsMathematical PhysicsExotic atomPhysics010308 nuclear & particles physicsPhysicsOrder (ring theory)light nucleiCharge (physics)Harmonicshyperspherical harmonicsnuclear interactionsab-initio theory
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Light-harvesting chlorophyll protein (LHCII) drives electron transfer in semiconductor nanocrystals

2017

Type-II quantum dots (QDs) are capable of light-driven charge separation between their core and the shell structures; however, their light absorption is limited in the longer-wavelength range. Biological light-harvesting complex II (LHCII) efficiently absorbs in the blue and red spectral domains. Therefore, hybrid complexes of these two structures may be promising candidates for photovoltaic applications. Previous measurements had shown that LHCII bound to QD can transfer its excitation energy to the latter, as indicated by the fluorescence emissions of LHCII and QD being quenched and sensitized, respectively. In the presence of methyl viologen (MV), both fluorescence emissions are quenched…

ChlorophyllParaquatPhotosynthetic reaction centreMaterials scienceAbsorption spectroscopyLight-Harvesting Protein ComplexesBiophysics02 engineering and technology010402 general chemistryPhotochemistry01 natural sciencesBiochemistryElectron TransportLight-harvesting complexElectron transferQuantum DotsUltrafast laser spectroscopyFluorescence Resonance Energy TransferAction spectrumPeasPhotosystem II Protein ComplexCell Biology021001 nanoscience & nanotechnologyFluorescence0104 chemical sciencesSemiconductorsQuantum dotNanoparticles0210 nano-technologyBiochimica et Biophysica Acta (BBA) - Bioenergetics
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Biogenic synthesis of palladium nanoparticles using Pulicaria glutinosa extract and their catalytic activity towards the Suzuki coupling reaction.

2014

Green synthesis of nanomaterials finds the edge over chemical methods due to its environmental compatibility. Herein, we report a facile and eco-friendly method for the synthesis of palladium (Pd) nanoparticles (NPs) using an aqueous solution of Pulicaria glutinosa, a plant widely found in a large region of Saudi Arabia, as a bioreductant. The as-prepared Pd NPs were characterized using ultraviolet-visible (UV-vis) spectroscopy, powder X-ray diffraction (XRD), transmission electron microscopy (TEM), energy-dispersive X-ray spectroscopy (EDX), and Fourier transform-infrared spectroscopy (FT-IR). The hydroxyl groups of the plant extract (PE) molecules were found mainly responsible for the red…

Chromatography GasMagnetic Resonance SpectroscopyStereochemistrychemistry.chemical_elementNanoparticleLigandsCatalysisCatalysisNanomaterialsPulicariaInorganic ChemistrySuzuki reactionMicroscopy Electron TransmissionX-Ray DiffractionSpectroscopy Fourier Transform InfraredMoleculeAqueous solutionChemistryPlant ExtractsX-RaysTemperatureGreen Chemistry TechnologyTransmission electron microscopyNanoparticlesSpectrophotometry UltravioletPalladiumNuclear chemistryPalladiumBromobenzenesDalton transactions (Cambridge, England : 2003)
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Spray Freeze Dried Lyospheres® for Nasal Administration of Insulin

2021

Pharmacologically active macromolecules, such as peptides, are still a major challenge in terms of designing a delivery system for their transport across absorption barriers and at the same time provide sufficiently high long-term stability. Spray freeze dried (SFD) lyospheres® are proposed here as an alternative for the preparation of fast dissolving porous particles for nasal administration of insulin. Insulin solutions containing mannitol and polyvinylpyrrolidone complemented with permeation enhancing excipients (sodium taurocholate or cyclodextrins) were sprayed into a cooled spray tower, followed by vacuum freeze drying. Final porous particles were highly spherical and mean diameters r…

ChromatographyChemistrylyophilizationPharmaceutical ScienceExcipientAbsorption (skin)PermeationArticleBioavailabilitynasal drug deliveryRS1-441Nasal AbsorptionFreeze-dryingPharmacy and materia medicamedicinepeptide formulationsNasal administrationMannitolporous particlespharmacokineticspray freeze dryingmedicine.drugPharmaceutics
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Multicomponent solid dispersion as a formulation strategy to improve drug permeation: A case study on the anti-colorectal cancer irinotecan

2019

Abstract Multicomponent solid dispersions (MSD)s are frequently proposed as efficient drug delivery systems to improve drug solubility and bioavailability. In this study, the effects of specific excipients, such as mannitol, inulin, poly(methyl methacrylate-co-methacrylic)acid (PMMA) and cellulose acetate phthalate (CAP) have been tested to potentially improve irinotecan (IRN) permeation in the intestinal tract with the intention to protect the drug from the gastric environment. MSDs were formulated as microparticles by Spray-Drying technique. Raw materials and microparticles have been characterized by FTIR analysis to determine hydrogen bonding. SEM images were recorded to investigate morp…

ChromatographyPharmaceutical Science02 engineering and technologyPermeation021001 nanoscience & nanotechnology030226 pharmacology & pharmacyBioavailabilityMulticomponent solid dispersion Microparticles Irinotecan Inulin Spray-drying03 medical and health scienceschemistry.chemical_compound0302 clinical medicineCellulose acetate phthalatechemistrySettore CHIM/09 - Farmaceutico Tecnologico ApplicativoDrug deliveryDissolution testingParticle sizeSolubility0210 nano-technologyDissolutionJournal of Drug Delivery Science and Technology
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Chromogenic Detection of Nerve Agent Mimics by Mass Transport Control at the Surface of Bifunctionalized Silica Nanoparticles

2010

Chemical warfare (CW) agents are toxic chemicals that have been used in several terrorist attacks in recent years. Among CW species, nerve agents are probably the most dangerous; their high toxicity and facile synthesis underscores the need to detect these lethal compounds with quick, reliable procedures. Analytical methods based on enzymatic assays and physical measurements have generally been used to detect these hazards. However, these protocols usually have limitations such as low selectivity, poor portability, and a certain level of complexity. In recent years, several chromogenic and fluorogenic sensors, and reagents for the detection of nerve agents have been described. For instance,…

ChromogenicSilicon dioxidePolyethylene TerephthalatesMolecularly imprinted polymerNanoparticleNanotechnologyGeneral ChemistryGeneral MedicineChromogenic CompoundsSilicon DioxideCatalysischemistry.chemical_compoundchemistryChromogenic CompoundsPhenolsReagentNanoparticlesColorimetryNaked eyeChemical Warfare AgentsSulfhydryl CompoundsColorimetryColoring AgentsCyclobutanesAngewandte Chemie
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Detailed study of SNR G306.3–0.9 using XMM-Newton and Chandra observations

2016

Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray emitting plasma of the supernova remnant (SNR) G306.3-0.9 in detail to obtain constraints on its ionization stage, the progenitor supernova explosion, and the age of the remnant. Methods. We used combined data from XMM-Newton and Chandra observatories to study the X-ray morphology of G306.3-0.9 in detail. A spatially resolved spectral analysis was used to obtain physical and geometrical parameters of different regions of the remnant. Spitzer infrared observations, available in the archive, were also used to constrain the progenitor supernova and study the environment in which the remnant evol…

Ciencias AstronómicasInfraredCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaISM [Infrared]FOS: Physical sciencesthermal [radiation mechanism]individual objects: SNR G306.3–0.9 [ISM]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral line//purl.org/becyt/ford/1 [https]ISM: individual objects: SNR G306.3IonizationISM [X-ray]0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsISM [X-rays]Radio continuum: ISMEjectaSupernova remnant010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy AstrophysicsISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Infrared: ISM010308 nuclear & particles physicssupernova remnants [ISM]Astronomy and AstrophysicsPlasma//purl.org/becyt/ford/1.3 [https]Astronomy and AstrophysicISM: individual objects: SNR G306.3–0.9ISM [Radio continuum]Radiation mechanisms: thermalX-rays: ISMindividual objects: G306.3-0.9 [ISM]Interstellar mediumAstronomíaSupernovathermal [Radiation mechanisms]Space and Planetary ScienceISM; ISM: individual objects: SNR G306.3; ISM: supernova remnants; Radiation mechanisms: thermal; Radio continuum: ISM; X-rays: ISM; Astronomy and Astrophysics; Space and Planetary Science [0.9; Infrared]0.9Astrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS
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Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory.

2012

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineering Radio Array (AERA) addresses both technological and scientific aspects of the radio technique. A first phase of AERA has been operating since September 2010 with detector stations observing radio signals at frequencies between 30 and 80 MHz. In this paper we present comparative studies to identify and optimize the antenna design for the final configuration of AERA consisting of 160 individual radio detector stations. The transient nature of the air shower signal requires a detailed description of the antenna s…

Ciencias Astronómicas[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomyAstrophysics::High Energy Astrophysical Phenomenashowers: atmosphere | cosmic radiation: UHE | polarization: effect | Auger | radio wave: emission | radio wave: detector | galaxy | background | reflection | noise | detector: networkFOS: Physical sciencesCosmic ray01 natural sciencesSignalKASCADEMHZOpticsSIGNALS0103 physical sciencesTransient responseTime domain010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMathematical Physics[PHYS]Physics [physics]PhysicsPierre Auger ObservatorySPECTRUMLarge detector systems for particle and astroparticle physics010308 nuclear & particles physicsbusiness.industryPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsFísica[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]ATMOSFERA (MONITORAMENTO)Air showerAntennaExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRADIATIONAntennasFísica nuclearAntenna (radio)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Instrumentation and Methods for Astrophysicsbusiness
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Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

2016

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the d…

Ciencias FísicasAstronomyGeneral Physics and Astronomyultra-high energy cosmic raysAstrophysics01 natural sciencesHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)CODALEMAObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]GeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRange (particle radiation)Radio detectorTUNKA-REXSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsRadio TechniqueFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsradio emissionCIENCIAS NATURALES Y EXACTASRadio wave[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy (all)0103 physical sciencesextensive air showersHigh Energy Physicsultra-high energy cosmic rays extensive air showers radio emission010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger Observatory010308 nuclear & particles physicsRadiant energyFísicaLOFAR//purl.org/becyt/ford/1.3 [https]LOFARASTROFÍSICASIMULATIONSComputational physicsAstronomíaCOREASExperimental High Energy PhysicsARRAYEMISSION SIMULATIONS LOFAR.EMISSION
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Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory an…

2014

Spherical harmonic moments are well-suited for capturing anisotropy at any scale in the flux of cosmic rays. An unambiguous measurement of the full set of spherical harmonic coefficients requires full-sky coverage. This can be achieved by combining data from observatories located in both the northern and southern hemispheres. To this end, a joint analysis using data recorded at the Telescope Array and the Pierre Auger Observatory above 1019 eV is presented in this work. The resulting multipolar expansion of the flux of cosmic rays allows us to perform a series of anisotropy searches, and in particular to report on the angular power spectrum of cosmic rays above 1019 eV. No significant devia…

Ciencias FísicasAstronomyRaysAstrophysicsAstroparticle physics; Cosmic rays01 natural scienceslaw.inventionPierrelawAnisotropyTelescope010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[PHYS]Physics [physics]Energy[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicRadiación cósmicaAugerCosmicArrivalComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsCIENCIAS NATURALES Y EXACTASHigh[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raySURFACE DETECTORICECUBETelescopeAIR-SHOWER ARRAYDirectionscosmic rays0103 physical sciencesInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysCiencias ExactasPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsArraySpectral densitySpherical harmonicsFísicaAstronomy and AstrophysicsASTROFÍSICAUltra[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomíaDipoleRESOLUTIONSpace and Planetary ScienceExperimental High Energy PhysicsQuadrupoleObservatoryAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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