Search results for "Particles"

showing 10 items of 8085 documents

SYNTHESIS AND CHARACTERIZATION OF NEW AMPHIPHILIC COPOLYMERS BASED ON A POLY(HYDROXYETHYL)-D,L-ASPARTAMIDE (PHEA) FOR THE COATING OF GOLD NANOPARTICL…

2012

GOLD NANOPARTICLES BIOCOMPATIBLE POLYMER POLY(HYDROXYETHYL)-DL-ASPARTAMIDE
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Polyaspartamide-g-Polylactide graft cpolymers able to form nanoparticles obtained by a novel synthetic strategy.

2009

GRAFT COPOLYMERS POLYMERIC NANOPARTICLES POLY(LACTIC ACID)Settore CHIM/09 - Farmaceutico Tecnologico Applicativo
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Test of the electric charge conservation law with Borexino detector

2015

International audience; The new limit on the electron lifetime is obtained from data of the Borexino experiment. The expected signal from the e → γν decay mode is a 256 keV photon detected in liquid scintillator. Because of the extremely low radioactive background level in the Borexino detector it was possible to improve the previous measurement by two orders of magnitude.

GRAN SASSOelectron --> photon neutrinoHistoryPhysics::Instrumentation and Detectorsscintillation counter: liquidElectronScintillator01 natural sciencesParticle detectorPhysics::GeophysicsEducationNuclear physicsSCINTILLATORPhysics and Astronomy (all)background: low0103 physical sciencescharge: conservation law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010303 astronomy & astrophysicsBorexinolifetimePhysicsCharge conservationSTABILITY010308 nuclear & particles physicsDetectorEXPERIMENTAL LIMITSComputer Science ApplicationsNeutrino detectorelectron: lifetimeBorexinoNeutrinoDECAYJournal of Physics: Conference Series
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Search for neutralino pair production at root s = 189 GeV

2001

A search for pair-production of neutralinos at a LEP centre-of-mass energy of 189 GeV gave no evidence for a signal. This limits the neutralino production cross-section and excludes regions in the parameter space of the Minimal Supersymmetric Standard Model (MSSM).

GRAVITINOSParticle physicsCOLLISIONSPhysics and Astronomy (miscellaneous)LOWEST ORDER CALCULATIONSMONTE-CARLO SIMULATIONFOS: Physical sciences2-PHOTON PROCESSESParameter space01 natural sciencesSignalPartícules (Física nuclear)High Energy Physics - ExperimentPHYSICSHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesEVENT GENERATOR[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RADIATIVE-CORRECTIONS010306 general physicsEngineering (miscellaneous)SUPERSYMMETRYDELPHIHIGH-ENERGIESPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLARGE ELECTRON POSITRON COLLIDERPair productionPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHINeutralinoPARTICLE PHYSICSFísica nuclearMONTE-CARLO SIMULATION; LOWEST ORDER CALCULATIONS; RADIATIVE-CORRECTIONS; 2-PHOTON PROCESSES; EVENT GENERATOR; HIGH-ENERGIES; SUPERSYMMETRY; PHYSICS; GRAVITINOS; COLLISIONSHigh Energy Physics::ExperimentEnergy (signal processing)Particle Physics - ExperimentMinimal Supersymmetric Standard ModelEUROPEAN PHYSICAL JOURNAL C
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Coupled theoretical and experimental studies for the radiation hardening of silica-based optical fibers

2014

International audience; We applied theoretical and experimental spectroscopy tools to ad hoc silica-based "canonical" samples to characterize the influence of several dopants and of some drawing process parameters on their radiation sensitivities. We present in this paper, the recent advances and results occurring from our coupled approach. On the experimental side, we studied the doping influence on the response of optical fibers and showed that changing the drawing parameters has a negligible influence on the fiber response in the case of specialty fibers. We focus mainly on the ${rm SiE}^prime$ defect that is observed through Electron Paramagnetic Resonance (EPR) measurements in all cano…

GW approximationNuclear and High Energy PhysicsOptical fiberMaterials scienceoptical fibersSiliconchemistry.chemical_element02 engineering and technology01 natural sciencesMolecular physics030218 nuclear medicine & medical imaginglaw.invention03 medical and health sciences[SPI]Engineering Sciences [physics]0302 clinical medicinelaw0103 physical sciencespoint defectsElectrical and Electronic Engineering010306 general physicsElectron paramagnetic resonanceSpectroscopydefectsdensity functional theoryCondensed matter physics010308 nuclear & particles physicsSettore FIS/01 - Fisica Sperimentale021001 nanoscience & nanotechnologyNuclear Energy and EngineeringchemistryUnpaired electronsilicaradiation effectsDensity functional theorytheoretical spectroscopyAb initio calculationsLocal-density approximation0210 nano-technology
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Impact of gadolinium on the structure and magnetic properties of nanocrystalline powders of iron oxides produced by the extraction-pyrolytic method

2020

The work has been done in frame of the TransFerr project. It has received funding from the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement No. 778070. This research was also supported by Latvian Research Council project lzp-2018/1-0214. A.I.P. appreciates support from the Estonian Research Council grant (PUT PRG619).

Gadolinium impactMaterials scienceiron oxidesValeric acidGadoliniumIron oxidechemistry.chemical_element02 engineering and technologyThermal treatmentCoercivitymagnetization010402 general chemistryValerateExtraction-pyrolitic methodIron oxidesMagnetizationlcsh:Technology7. Clean energy01 natural sciencesArticlechemistry.chemical_compoundnanostructures:NATURAL SCIENCES:Physics [Research Subject Categories]extraction–pyrolitic methodGeneral Materials Sciencecoercivitylcsh:Microscopylcsh:QC120-168.85chemistry.chemical_classificationlcsh:QH201-278.5lcsh:TExtraction (chemistry)gadolinium impact021001 nanoscience & nanotechnologyNanocrystalline materialNanostructures0104 chemical sciencesiron oxides ; nanostructures ; gadolinium impact ; extraction–pyrolitic method ; magnetization ; coercivitychemistrylcsh:TA1-2040Magnetic nanoparticleslcsh:Descriptive and experimental mechanicslcsh:Electrical engineering. Electronics. Nuclear engineeringlcsh:Engineering (General). Civil engineering (General)0210 nano-technologylcsh:TK1-9971Nuclear chemistry
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The ALHAMBRA survey: reliable morphological catalogue of 22 051 early- and late-type galaxies

2013

Advanced Large Homogeneous Area Medium Band Redshift Astronomical (ALHAMBRA) is photometric survey designed to trace the cosmic evolution and cosmic variance. It covers a large area of ~4 deg2 in eight fields, where seven fields overlap with other surveys, allowing us to have complementary data in other wavelengths. All observations were carried out in 20 continuous, medium band (30 nm width) optical and 3 near-infrared (JHK) bands, providing the precise measurements of photometric redshifts. In addition, morphological classification of galaxies is crucial for any kind of galaxy formation and cosmic evolution studies, providing the information about star formation histories, their environme…

Galaxies: fundamental parametersCosmology and Nongalactic Astrophysics (astro-ph.CO)Galaxies: statisticsFOS: Physical sciencesLibrary scienceAstrophysics::Cosmology and Extragalactic AstrophysicsEuropean Social FundSurveys01 natural sciencesstatistics [Galaxies]0103 physical sciences10. No inequality010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]010308 nuclear & particles physicsLate typeAstronomyAstronomy and AstrophysicsSpace and Planetary ScienceResearch councilfundamental parameters [Galaxies]Christian ministry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Data releaseAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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The ALHAMBRA survey: An empirical estimation of the cosmic variance for merger fraction studies based on close pairs

2014

[Aims]: Our goal is to estimate empirically the cosmic variance that affects merger fraction studies based on close pairs for the first time. [Methods]: We compute the merger fraction from photometric redshift close pairs with 10 h−1 kpc ≤ rp ≤ 50 h−1 kpc and Δv ≤ 500 km s−1 and measure it in the 48 sub-fields of the ALHAMBRA survey. We study the distribution of the measured merger fractions that follow a log-normal function and estimate the cosmic variance σv as the intrinsic dispersion of the observed distribution. We develop a maximum likelihood estimator to measure a reliable σv and avoid the dispersion due to the observational errors (including the Poisson shot noise term). [Results]: …

Galaxies: fundamental parametersCosmology and Nongalactic Astrophysics (astro-ph.CO)Stellar massGalaxies: statisticsFOS: Physical sciencesAstrophysicsinteractions [Galaxies]Astrophysics::Cosmology and Extragalactic AstrophysicsPoisson distribution01 natural sciencesLuminositysymbols.namesakestatistics [Galaxies]0103 physical sciences010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhotometric redshiftPhysics[PHYS]Physics [physics]COSMIC cancer database010308 nuclear & particles physicsAstronomy and AstrophysicsCosmic varianceRedshiftGalaxyGalaxies: interactionsSpace and Planetary Sciencefundamental parameters [Galaxies]symbols[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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Evolution of Balmer jump selected galaxies in the ALHAMBRA survey

2016

Extragalactic astronomy.-- et al.

Galaxies: generalAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesevolution [Galaxy]high-redshift [Galaxies]Galactic haloBalmer jump0103 physical sciencesGalaxy formation and evolutionAstrophysics::Solar and Stellar Astrophysicshalo [Galaxy]010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy Astrophysics[PHYS]Physics [physics]PhysicsGalaxy: evolution010308 nuclear & particles physicsphotometry [Galaxies]Astrophysics::Instrumentation and Methods for AstrophysicsGalaxies: high-redshiftGalaxies: evolutiongeneral [Galaxies]Astronomy and AstrophysicsGalaxies: photometryevolution [Galaxies]Astrophysics - Astrophysics of GalaxiesGalaxyPhysics::History of PhysicsGalaxy: haloSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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The ALHAMBRA survey: accurate merger fractions derived by PDF analysis of photometrically close pairs

2015

[Aims]: Our goal is to develop and test a novel methodology to compute accurate close-pair fractions with photometric redshifts. [Methods]: We improved the currently used methodologies to estimate the merger fraction fm from photometric redshifts by (i) using the full probability distribution functions (PDFs) of the sources in redshift space; (ii) including the variation in the luminosity of the sources with z in both the sample selection and the luminosity ratio constrain; and (iii) splitting individual PDFs into red and blue spectral templates to reliably work with colour selections.We tested the performance of our new methodology with the PDFs provided by the ALHAMBRA photometric survey.…

Galaxies: statisticsmedia_common.quotation_subjectAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsEuropean Social Fundinteractions [Galaxies]Public administration01 natural sciencesstatistics [Galaxies]Excellence0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSmedia_commonPhysics[PHYS]Physics [physics]Government010308 nuclear & particles physicsGalaxies: evolutionAstronomy and Astrophysicsevolution [Galaxies]Galaxies: interactionsWork (electrical)Space and Planetary ScienceResearch council[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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