Search results for "INOS"

showing 10 items of 2075 documents

Observation of Photon Polarization in theb→sγTransition

2014

This Letter presents a study of the flavor-changing neutral current radiative $B^{\pm} \to K^{\pm}\pi^{\mp}\pi^{\pm}\gamma$ decays performed using data collected in proton-proton collisions with the LHCb detector at $7$ and $8\,$TeV center-of-mass energies. In this sample, corresponding to an integrated luminosity of $3\,\text{fb}^{-1}$, nearly $14\,000$ signal events are reconstructed and selected, containing all possible intermediate resonances with a $K^{\pm}\pi^{\mp}\pi^{\pm}$ final state in the $[1.1, 1.9]\,$GeV/$c^{2}$ mass range. The distribution of the angle of the photon direction with respect to the plane defined by the final-state hadrons in their rest frame is studied in interva…

Final statePhotonmedia_common.quotation_subject14.40.NdHadronGeneral Physics and AstronomyLHCb - Abteilung Hofmann12.15.MmAsymmetryHigh energy physics Polarization Tellurium compounds; Center-of-mass energies Direct observations Final state Flavor-changing neutral current Integrated luminosity Photon polarization Proton proton collisions; PhotonsNeutral currentNuclear physicsTellurium compoundsCenter-of-mass energiesPhysics and Astronomy (all)Flavor-changing neutral currentPolarizationPhoton polarizationLeptonic semileptonic and radiative decays of bottom mesonRadiative transferIntermediate stateSDG 7 - Affordable and Clean EnergyHigh energy physicsQCmedia_commonPhysicsIntegrated luminosityPhotons/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyProton proton collisionsNeutral currentDirect observationsParticle physicsRest framePhoton polarizationLHCb13.20.HeBottom mesons (|B|>0)High Energy Physics::ExperimentLHCFísica de partículesExperimentsPhysical Review Letters
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Search forBs0→μ+μ−andB0→μ+μ−Decays with CDF II

2011

A search has been performed for B{sub s}{sup 0} {yields} {mu}{sup +}{mu}{sup -} and B{sup 0} {yields} {mu}{sup +}{mu}{sup -} decays using 7 fb{sup -1} of integrated luminosity collected by the CDF II detector at the Fermilab Tevatron collider. The observed number of B{sup 0} candidates is consistent with background-only expectations and yields an upper limit on the branching fraction of {Beta}(B{sup 0} {yields} {mu}{sup +}{mu}{sup -}) < 6.0 x 10{sup -9} at 95% confidence level. We observe an excess of B{sub s}{sup 0} candidates. The probability that the background processes alone could produce such an excess or larger is 0.27%. The probability that the combination of background and the expe…

Flight directionNuclear and High Energy PhysicsParticle physicsMesonTevatronGeneral Physics and Astronomy01 natural sciences7. Clean energyLuminosityStandard Modellaw.inventionNuclear physicsParticle decaychemistry.chemical_compoundlawTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesInvariant massLimit (mathematics)FermilabCollider010306 general physicsPhysicsMuon010308 nuclear & particles physicsBranching fractionSupersymmetryD0 experimentIMesCrystallographychemistryDecay lengthHigh Energy Physics::ExperimentLeptonPhysical Review Letters
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Dual Enzyme-Responsive Capsules of Hyaluronic Acid-block-Poly(Lactic Acid) for Sensing Bacterial Enzymes.

2015

The synthesis of novel amphiphilic hyaluronic acid (HYA) and poly(lactic acid) (PLA) block copolymers is reported as the key element of a strategy to detect the presence of pathogenic bacterial enzymes. In addition to the formation of defined HYA-block-PLA assemblies, the encapsulation of fluorescent reporter dyes and the selective enzymatic degradation of the capsules by hyaluronidase and proteinase K are studied. The synthesis of the dual enzyme-responsive HYA-b-PLA is carried out by copper-catalyzed Huisgen 1,3-dipolar cycloaddition. The resulting copolymers are assembled in water to form vesicular structures, which are characterized by scanning electron microscopy, transmission electron…

Fluorescence-lifetime imaging microscopyStaphylococcus aureusMaterials sciencePolymers and PlasticsCell SurvivalPolymersDrug CompoundingPolyestersMolecular Sequence DataPrimary Cell CultureHyaluronoglucosaminidaseBiosensing TechniquesFluorescence spectroscopyNanocapsuleschemistry.chemical_compoundDynamic light scatteringBacterial ProteinsNanocapsulesHyaluronidaseAmphiphileMaterials ChemistrymedicineHumansLactic AcidHyaluronic AcidMicellesFluorescent DyesCycloaddition ReactionRhodaminesOrganic Chemistrytechnology industry and agricultureEndothelial CellsDermisLactic acidchemistryBiochemistryCarbohydrate SequencePseudomonas aeruginosaBiophysicsLiberationEndopeptidase Kmedicine.drugMacromolecular rapid communications
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Coronal properties of G-type stars in different evolutionary phases

2005

We report on the analysis of XMM-Newton observations of three G-type stars in very different evolutionary phases: the weak-lined T Tauri star HD 283572, the Zero Age Main Sequence star EK Dra and the Hertzsprung-gap giant star 31 Com. They all have high X-ray luminosity (10^31 erg/s for HD 283572 and 31 Com and 10^30 erg/s for EK Dra). We compare the Emission Measure Distributions (EMDs) of these active coronal sources, derived from high-resolution XMM-Newton grating spectra, as well as the pattern of elemental abundances vs. First Ionization Potential (FIP). We also perform time-resolved spectroscopy of a flare detected by XMM from EK Dra. We interpret the observed $EMD$s as the result of …

G-type main-sequence starLINED T TAURIMetallicityAstrophysics::High Energy Astrophysical PhenomenaX-RAY SPECTROSCOPYFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLuminosityEMISSION MEASURE DISTRIBUTIONSAstrophysics::Solar and Stellar AstrophysicsACTIVE STARSAstrophysics::Galaxy AstrophysicsXMM-NEWTONPhysicsSOLAR-TYPE STARSAstrophysics (astro-ph)HERTZSPRUNG-GAPAstronomy and AstrophysicsGiant starSurface gravityStarsT Tauri starSpace and Planetary ScienceANALOG EK DRACONISSTELLAR SURFACE-STRUCTUREMAIN-SEQUENCE STARSMain sequence
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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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Gunilaktāmu totālās sintēzes izstrāde

2020

Darba literatūras apskata daļā ir apkopota informācija par klasiskām (divelektronu) un modernām (radikāļu) ketonu sintēzes metodēm. Darba vispārīgajā un eksperimentālajā daļā aprakstītas gunilaktāma dabas vielas konstruēšanai nepieciešamie būvbloku sintēzes un tā sašušānas metodes. Tika aprakstīta sintēžu gaita, galvenās problēmas un to risinājumi, lai sasniegtu vajadzīgos rezultātus.

GUNILAKTĀMSKETONU SINTĒZETOTĀLĀ SINTĒZEĶīmijaAMINOSKĀBES
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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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SHARDS: A global view of the star formation activity at z~0.84 and z~1.23

2015

et al.

Galaxies: generalAstrofísicaStellar massFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstar formation [Galaxies]Luminosityhigh-redshift [Galaxies]emission lines [Quasars]Stellar evolutionAstrophysics::Galaxy AstrophysicsCosmic dustPhysicsQuasars: emission linesGalaxies: star formationStar formationphotometry [Galaxies]Galaxies: high-redshiftGalaxies: evolutiongeneral [Galaxies]Astronomy and AstrophysicsQuasarGalaxies: photometryevolution [Galaxies]Astrophysics - Astrophysics of GalaxiesRedshiftGalaxyAstronomíaSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)
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Search for Neutrino‐induced Cascades from Gamma‐Ray Bursts with AMANDA

2007

Using the neutrino telescope AMANDA-II, we have conducted two analyses searching for neutrino-induced cascades from gamma-ray bursts. No evidence of astrophysical neutrinos was found, and limits are presented for several models. We also present neutrino effective areas which allow the calculation of limits for any neutrino production model. The first analysis looked for a statistical excess of events within a sliding window of 1 or 100 seconds (for short and long burst classes, respectively) during the years 2001-2003. The resulting upper limit on the diffuse flux normalization times E^2 for the Waxman-Bahcall model at 1 PeV is 1.6 x 10^-6 GeV cm^-2 s^-1 sr^-1 (a factor of 120 above the the…

Gamma rays: burstsNormalization (statistics)PhysicsRange (particle radiation)MuonAstrophysics::High Energy Astrophysical PhenomenaGamma rays: bursts; Neutrinos; TelescopesAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsCoincidenceSpace and Planetary ScienceCascadeAstronomiaDiffuse fluxHigh Energy Physics::ExperimentNeutrinosNeutrinoGamma-ray burstTelescopesThe Astrophysical Journal
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FeOOH and Mn8O10Cl3modified zeolites for As(V) removal in aqueous medium

2017

BACKGROUND Arsenic in drinking water poses serious potential health risks in more than 30 countries with total affected population of around 100 million people. The present study is devoted to the development of innovative sorbents based on zeolite materials for As(V) sorption by modifying raw materials with iron oxyhydroxide and manganese oxychloride. Natural clinoptilolite and synthetic zeolite A were modified in order to obtain improved sorption of As(V). Sorption properties of newly developed sorbents were studied. Zeolites containing natural clinoptilolite are chosen due to relatively low cost and their broad use in industrial production as well as characteristic large surface area. RE…

General Chemical EngineeringInorganic chemistryPopulationchemistry.chemical_element02 engineering and technologyManganese010501 environmental sciences01 natural sciencesInorganic Chemistrysymbols.namesakeAdsorptionAluminosilicateZeoliteeducationWaste Management and Disposal0105 earth and related environmental sciencesClinoptiloliteeducation.field_of_studyRenewable Energy Sustainability and the EnvironmentOrganic ChemistryLangmuir adsorption modelSorption021001 nanoscience & nanotechnologyPollutionFuel Technologychemistrysymbols0210 nano-technologyBiotechnologyJournal of Chemical Technology &amp; Biotechnology
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