Search results for "ddc:54"

showing 10 items of 218 documents

When Does Gold Behave as a Halogen? Predicted Uranium Tetraauride and Other MAu4 Tetrahedral Species, (M = Ti, Zr, Hf, Th)

2003

Quantum chemical calculations suggest that a series of molecules with the general formula MAu4 are stable, where M = U, Th, and a group-4 atom. They correspond to Au in the formal valence state -1 and indicate that gold can act as a ligand similar to the halogen series. Of the MAu4 species studied, UAu4, the first predicted mixed gold uranium compound, has a short M-Au bond distance, 2.71 A, which would locate Au between Br and I from the bond length point of view in the U-tetrahalide series. Energetically, the U-Au bond is weaker than the corresponding U-Br and U-I bonds.

Valence (chemistry)LigandStereochemistrychemistry.chemical_elementGeneral MedicineGeneral ChemistryElectronic structureUraniumBiochemistryCatalysisBond lengthCrystallographyColloid and Surface ChemistrychemistryGold CompoundsMolecular vibrationAtomHalogenddc:540TetrahedronMolecule
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Nanodiamond Theranostic for Light-Controlled Intracellular Heating and Nanoscale Temperature Sensing

2021

Temperature is an essential parameter in all biological systems, but information about the actual temperature in living cells is limited. Especially, in photothermal therapy, local intracellular temperature changes induce cell death but the local temperature gradients are not known. Highly sensitive nanothermometers would be required to measure and report local temperature changes independent of the intracellular environment, including pH or ions. Fluorescent nanodiamonds (ND) enable temperature sensing at the nanoscale independent of external conditions. Herein, we prepare ND nanothermometers coated with a nanogel shell and the photothermal agent indocyanine green serves as a heat generato…

ZelleDDC 540 / Chemistry & allied sciencesTechnologyLetterintracellular temperature manipulation and sensingHot TemperatureMaterials scienceNanodiamond nanogel intracellular temperature manipulation and sensing photothermal applicationCellsnanodiamondphotothermal applicationNanoparticleBioengineeringNanotechnology02 engineering and technologyBestrahlungNanodiamondsHeatingGeneral Materials ScienceIrradiationPrecision MedicineNanodiamondNanoscopic scaleMechanical EngineeringTemperatureNanometerbereichGeneral ChemistryNanokristallPhotothermal therapy021001 nanoscience & nanotechnologyCondensed Matter PhysicsFluorescenceNanocrystalsNanoscalenanogelddc:540Nanostrukturiertes MaterialCarbon nanomaterialsIrradiation0210 nano-technologyNanochemistryddc:600IntracellularNanogel
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Monitoring a Mechanochemical Reaction Reveals the Formation of a New ACC Defect Variant Containing the HCO 3 – Anion Encapsulated by an Amorphous Mat…

2020

Crystal growth & design 20(10), 6831 - 6846 (2020). doi:10.1021/acs.cgd.0c00912

[CHIM.INOR]Chemical Sciences/Inorganic chemistry010402 general chemistry01 natural sciencesPyrophosphatelaw.inventionchemistry.chemical_compoundlaw[CHIM.CRIS]Chemical Sciences/CristallographyGeneral Materials ScienceCrystallization010405 organic chemistryGeneral Chemistry[CHIM.MATE]Chemical Sciences/Material chemistryCondensed Matter PhysicsCondensation reactionPhosphate540Amorphous calcium carbonate0104 chemical sciences3. Good healthAmorphous solidCalcium carbonatechemistryChemical engineering13. Climate actionddc:540Carbonate[SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/Mineralogy
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Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

2008

Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival directions of the cosmic rays with the ighest-energies, which are correlated with the positions of relatively nearby active galactic nuclei (AGN) [Pierre Auger Collaboration, Science 318 (2007) 938]. The correlation has maximum significance for cosmic rays with energy greater than ~6 x 1019 eV and AGN at a distance less than ~75 Mpc. We have confirmed the anisotropy at a confidence level of more than 99% through a test with parameters specified a priori, using an independent data set. The observed correlation is compatible with the hypothesis that cosmic rays with the highest-energies originate fro…

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyOsservatorio Pierre AugerAstrophysicsGALAXY CLUSTER SURVEYAstrophysicsauger01 natural sciencesHigh energy cosmic rayRaggi cosmiciAstrophysical jetGMFObservatoryUltra-high-energy cosmic ray010303 astronomy & astrophysicsPhysicsBL-LACERTAEGreisen–Zatsepin–Kuz’min effect[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]ORIGINUHECRAstrophysics (astro-ph)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryGZKRadiación cósmicaAnisotropíaCATALOGobservatoryddc:540EGMFCUTOFFComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRELATIVISTIC JETSActive galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaCosmic background radiationFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsACCELERATION[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesextra-galacticPARTICLESAGNAstrophysics::Galaxy AstrophysicsCiencias ExactasPierre Auger ObservatoryANISOTROPYhigh energy cosmic raysSciami atmosferici010308 nuclear & particles physicsFísicaAstronomyAstronomy and AstrophysicsCENTAURUSGalaxyExperimental High Energy Physics
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Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector

2010

The ANTARES high energy neutrino telescope is a three-dimensional array of about 900 photomultipliers distributed over 12 mooring lines installed in the Mediterranean Sea. Between February and November 2007 it acquired data in a 5-line configuration. The zenith angular distribution of the atmospheric muon flux and the associated depth-intensity relation are measured and compared with previous measurements and Monte Carlo expectations. An evaluation of the systematic effects due to uncertainties on environmental and detector parameters is presented.

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsMonte Carlo methodAtmospheric muonsFluxNeutrino telescope01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)WATER010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)DetectorAstrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAY CASCADES NEUTRINO TELESCOPE PERFORMANCE GENERATOR SYSTEM MODULE LIGHT WATER SITESITEMUON FLUXLIGHTddc:540Física nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsMODULEAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayParticle detectorCOSMIC-RAY CASCADESNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]depth-intensity relation0103 physical sciencesatmospheric muons; depth-intensity relation; neutrino telescope14. Life underwaterInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithRemote sensingatmospheric muonsDepth-intensity relation010308 nuclear & particles physicsneutrino telescopeAstronomy and AstrophysicsCOSMIC RAYSPERFORMANCEGENERATORMeasuring instrumentHigh Energy Physics::ExperimentUNDERWATER DETECTORSYSTEM
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Light-Activated Sensitive Probes for Amine Detection

2017

Our new, simple, and accurate colorimetric method is based on diarylethenes (DAEs) for the rapid detection of a wide range of primary and secondary amines. The probes consist of aldehyde- or ketone-substituted diarylethenes, which undergo an amine-induced decoloration reaction, selectively to give the ring-closed isomer. Thus, these probes can be activated at the desired moment by light irradiation, with a sensitivity that allows the detection of amines at concentrations as low as 10exp−6 M in solution. In addition, the practical immobilization of DAEs on paper makes it possible to detect biogenic amines, such as cadaverine, in the gas phase above a threshold of 12 ppbv within 30 seconds. P…

amines010402 general chemistryPhotochemistry01 natural sciencesRapid detectionAldehydeCatalysisGas phasechemistry.chemical_compoundsensingchemistry.chemical_classificationCadaverine010405 organic chemistryChemistryLight activatedLight irradiationGeneral Chemistryphotochromism0104 chemical sciencesdiarylethenes540 Chemie und zugeordnete Wissenschaftenamineddc:540diaryletheneAmine gas treatingAngewandte Chemie International Edition
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Search for low-energy neutrinos from astrophysical sources with Borexino

2019

We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron antineutrinos ($\bar{\nu}_e$) are detected in an organic liquid scintillator through the inverse $\beta$-decay reaction. In the present work we set model-independent upper limits in the energy range 1.8-16.8 MeV on neutrino fluxes from unknown sources that improve our previous results, on average, by a factor 2.5. Using the same data set, we first obtain experimental constraints on the diffuse supernova $\bar{\nu}_e$ fluxes in the previously unexplored region below 8 MeV. A search for $\bar{\nu}_e$ in the solar ne…

antineutrinosPhysics - Instrumentation and Detectorssolar flaresmagnetic field: highneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidelastic scatteringantineutrino/e: particle identification01 natural sciences7. Clean energyneutrino: fluxlaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: supernova26.65.+t010303 astronomy & astrophysicsBorexinoElastic scatteringPhysicsSolar flareSupernova Relic Neutrinosneutrino: energy spectrumS067EB8neutrinosInstrumentation and Detectors (physics.ins-det)neutrino: magnetic momentDiffuse Supernova Neutrino Background3. Good healthSupernovaHomestakeddc:540neutrino: flavorAntineutrinoBorexinoNeutrino97.60.BwHomestake experimentFlareantineutrino/e: fluxAntineutrinos13.15.+G; 26.65.+T; 29.40.Mc; 97.60.Bw; Antineutrinos; Diffuse supernova neutrino background; Neutrinos; Solar flares; Supernova relic neutrinosAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSupernova relic neutrinosupernova relic neutrinosNONuclear physics13.15.+gPE2_2Antineutrinos; Neutrinos; Diffuse supernova neutrino background; Supernova relic neutrinos; Solar flares0103 physical sciencesNeutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinosdiffuse supernova neutrino background010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsneutrino: particle source29.40.McGran SassoSolar flareSolar Flares13. Climate actionspectralHigh Energy Physics::Experimentexperimental results
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Borexino’s search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts

2017

International audience; A search for neutrino and antineutrino events correlated with 2350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No statistically significant excess over background is observed. We look for electron antineutrinos ( ν¯e ) that inverse beta decay on protons with energies from 1.8  MeV to 15  MeV and set the best limit on the neutrino fluence from GRBs below 8  MeV. The signals from neutrinos and antineutrinos from GRBs that scatter on electrons are also searched for, a detection channel made possible by the particularly radio-pure scintillator of Borexino. We obtain currently the best limits on the neutrino f…

antineutrinoselectronAntineutrinosneutrino: solarPhysics::Instrumentation and Detectorsdata acquisitionSolar neutrino[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical Phenomenalow energy/MeV neutrinosElectrongamma ray: burst01 natural sciencesNuclear physicsLow energy/MeV neutrino0103 physical sciencesNeutrinoLow energy/MeV neutrinosNeutrinosNuclear Experiment010303 astronomy & astrophysicsGamma-ray burstBorexinoscintillation counterPhysicsflavor010308 nuclear & particles physicsbackgroundgamma-ray burstsneutrinosAntineutrinos; Gamma-ray bursts; Low energy/MeV neutrinos; Neutrinos; Astronomy and AstrophysicsAstronomy and Astrophysicssemileptonic decayantineutrinocorrelation: timeNeutrino detectorInverse beta decayddc:540Scintillation counterreadoutHigh Energy Physics::ExperimentBorexinoGamma-ray burstsNeutrinoGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Autophagy

2012

Klionsky, Daniel J. et al.

autophagy assays[SDV]Life Sciences [q-bio]AutolysosomeAutophagosome maturationautophagosomeBioinformaticsstressChaperone-mediated autophagyModelsLC3MESH: Animalsguidelinesautolysosome autophagosome flux LC3 lysosome phagophore stress vacuoleSettore BIO/06 - Anatomia Comparata E CitologiaComputingMilieux_MISCELLANEOUSSettore BIO/17Autophagy databaseautolysosome3. Good healthddc:540lysosomeEnergy and redox metabolism Mitochondrial medicine [NCMLS 4]methods [Biological Assay]Biological AssaySettore BIO/17 - ISTOLOGIANeuroniMAP1LC3BHumanautophagygenetics [Autophagy]AutofagiaMESH: Autophagy*/genetics[SDV.BC]Life Sciences [q-bio]/Cellular BiologyAutofagia; Neuroni; istologiaBiologyModels BiologicalLC3; autolysosome; autophagosome; flux; lysosome; phagophore; stress; vacuoleddc:570AutophagyAnimalsHumansAutophagy-Related Protein 7[SDV.BC] Life Sciences [q-bio]/Cellular BiologyBiological Assay/methodsMolecular BiologyBiologyAutophagy; guidelines; autophagy assaysistologiaphagophoreMESH: HumansAnimals; Biological Assay; Humans; Models Biological; AutophagyvacuoleAnimal[ SDV.BC ] Life Sciences [q-bio]/Cellular BiologyMESH: Models BiologicalPathogenesis and modulation of inflammation Infection and autoimmunity [N4i 1]Cell BiologyBiologicalAutophagy/geneticsfluxAutophagosome membraneAutophagy Protein 5Human medicineMESH: Biological Assay/methods*Neuroscienceautolysosome; autophagosome; flux; LC3; lysosome; phagophore; stress; vacuoleAutophagy
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Proton‐Gated Ring‐Closure of a Negative Photochromic Azulene‐Based Diarylethene

2020

Abstract Proton‐responsive photochromic molecules are attractive for their ability to react on non‐invasive rapid optical stimuli and the importance of protonation/deprotonation processes in various fields. Conventionally, their acidic/basic sites are on hetero‐atoms, which are orthogonal to the photo‐active π‐center. Here, we incorporate azulene, an acid‐sensitive pure hydrocarbon, into the skeleton of a diarylethene‐type photoswitch. The latter exhibits a novel proton‐gated negative photochromic ring‐closure and its optical response upon protonation in both open and closed forms is much more pronounced than those of diarylethene photoswitches with hetero‐atom based acidic/basic moieties. …

azulenenegative photochromismProtonation010402 general chemistryPhotochemistry01 natural sciencesCatalysischemistry.chemical_compoundPhotochromismDeprotonationDiaryletheneMoleculeMolecular switchphotochemistryPhotoswitch010405 organic chemistryCommunicationPhotoswitchesGeneral ChemistryAzuleneCommunications3. Good health0104 chemical sciences540 Chemie und zugeordnete Wissenschaftenchemistryacid-base equilibriaddc:540diarylethene
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