Search results for "ddc:540"

showing 10 items of 212 documents

A theoretical study of the lowest electronic states of azobenzene: the role of torsion coordinate in the cis-trans photoisomerization

2003

In the present paper we report the results of a multiconigurational computational study on potential- energy curves of azobenzene along the NN twisting to clarify the role of this coordinate in the decay of the S2(pp*) and S1(np*) states. We have found that there is a singlet state, S3 at the trans geometry, on the basis of the doubly excited coniguration n 2 p* 2 , that has a deep minimum at about 90 of twisting, where it is the lowest excited singlet state. The existence of this state provides an explanation for the short lifetime of S2(pp*) and for the wavelength-dependence of azobenzene photochem- istry. We have characterized the S1(np*) state by calcu- lating its vibrational frequencie…

PhotoisomerizationAzobenzeneMulticonfigurational wave function methodschemistry.chemical_compoundsymbols.namesakeAzobenzenechemistryExcited statePhotoisomerizationddc:540symbolsDensity functional theoryExcited electronic statesSinglet statePhysical and Theoretical ChemistryAtomic physicsRaman spectroscopyIsomerizationCis–trans isomerism
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Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope

2010

A new method for the measurement of the muon flux in the deep-sea ANTARES neutrino telescope and its dependence on the depth is presented. The method is based on the observation of coincidence signals in adjacent storeys of the detector. This yields an energy threshold of about 4 GeV. The main sources of optical background are the decay of 40K and the bioluminescence in the sea water. The 40K background is used to calibrate the efficiency of the photo-multiplier tubes.

PhotomultiplierPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAtmospheric muonsFOS: Physical sciencesLINECosmic rayPotassium-4001 natural sciencesParticle detectorNuclear physicsPOTASSIUM-40NEUTRINO TELESCOPESatmospheric muons; depth intensity relation; potassium-400103 physical sciencesDepth intensity relation14. Life underwater010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)ATMOSPHERIC MUONSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPotassium-40DetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsPERFORMANCEDEPTH INTENSITY RELATIONLIGHTNeutrino detector13. Climate actionddc:540Física nuclearHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]SYSTEMLepton
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Upper limit on the cosmic-ray photon flux above 1019 eV using the surface detector of the Pierre Auger Observatory

2008

A method is developed to search for air showers initiated by photons using data recorded by the surface detector of the Auger Observatory. The approach is based on observables sensitive to the longitudinal shower development, the signal risetime and the curvature of the shower front. Applying this method to the data, upper limits on the flux of photons of 3.8 x 10-3, 2.5 x 10-3; and 2.2 x 10-3 km-2 sr-1 yr-1 above 1019 eV, 2 x 1019 eV; and 4 x 1019 eV are derived, with corresponding limits on the fraction of photons being 2.0%, 5.1%, and 31% (all limits at 95% c.l.). These photon limits disfavor certain exotic models of sources of cosmic rays. The results also show that the approach adopted…

Photon[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyFluxFOS: Physical sciencesOsservatorio Pierre AugerCosmic rayFotonesAstrophysicsAstrophysics7. Clean energy01 natural sciencesAugerNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)Raggi cosmiciultra high energy photonsCascada atmosféricaObservatory0103 physical sciences010306 general physicsCiencias ExactasPierre Auger ObservatoryPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)FísicaAstronomy and AstrophysicsPierre Auger ObservatoryEnergia ultra altaCosmic rayHigh Energy Physics - PhenomenologyPair production13. Climate actionFotoniExperimental High Energy Physicsddc:540flux upper limitNeutrinoSciami atmosferici estesi
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The design and performance of IceCube DeepCore

2011

The IceCube neutrino observatory in operation at the South Pole, Antarctica, comprises three distinct components: a large buried array for ultrahigh energy neutrino detection, a surface air shower array, and a new buried component called DeepCore. DeepCore was designed to lower the IceCube neutrino energy threshold by over an order of magnitude, to energies as low as about 10 GeV. DeepCore is situated primarily 2100 m below the surface of the icecap at the South Pole, at the bottom center of the existing IceCube array, and began taking physics data in May 2010. Its location takes advantage of the exceptionally clear ice at those depths and allows it to use the surrounding IceCube detector a…

Physics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAntarticaGeneratorAstrophysicsNeutrino telescope01 natural sciences7. Clean energyHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryAntarctica; DeepCore; Detector; IceCube; NeutrinoIceCubeHigh Energy Physics - Experiment (hep-ex)WIMP0103 physical sciencesNeutrino010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsMuon010308 nuclear & particles physicsIceICEAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsDetectorInstrumentation and Detectors (physics.ins-det)GENERATORDeepCoreSupernovaAir showerPhysics and AstronomyNeutrino detector13. Climate actionddc:540AntarcticaHigh Energy Physics::ExperimentNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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The Monte Carlo simulation of the Borexino detector

2017

We describe the Monte Carlo (MC) simulation package of the Borexino detector and discuss the agreement of its output with data. The Borexino MC 'ab initio' simulates the energy loss of particles in all detector components and generates the resulting scintillation photons and their propagation within the liquid scintillator volume. The simulation accounts for absorption, reemission, and scattering of the optical photons and tracks them until they either are absorbed or reach the photocathode of one of the photomultiplier tubes. Photon detection is followed by a comprehensive simulation of the readout electronics response. The algorithm proceeds with a detailed simulation of the electronics c…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsSolar neutrinoMonte Carlo methodscintillation counter: liquidSolar neutrinosenergy resolution01 natural sciences7. Clean energyLarge volume liquid scintillator detectorHigh Energy Physics - Experiment[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Large volume liquid scintillator detectorsBorexinoPhysicsphotomultipliertrack data analysisDetectorefficiency: quantumddc:540GEANTBorexinoNeutrinophoton: yieldnumerical calculations: Monte CarloPhotomultiplierdata analysis methodenergy lossScintillatorSolar neutrinoprogrammingphoton: reflectionMonte Carlo simulationsNuclear physics0103 physical sciencesphoton: scattering[INFO]Computer Science [cs][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsbackground: radioactivityMonte Carlo simulationdetector: designScintillation010308 nuclear & particles physicsbibliographyAstronomy and AstrophysicscalibrationLarge volume liquid scintillator detectors; Monte Carlo simulations; Solar neutrinos; Astronomy and Astrophysicsattenuation: lengthpile-upelectronics: readout
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Taming conformational heterogeneity in and with vibrational circular dichroism spectroscopy

2019

Chemical science 10, 7680 -7689 (2019). doi:10.1039/C9SC02866H

PhysicsFlexibility (engineering)FELIX Condensed Matter PhysicsQuantitative Biology::Biomolecules/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energy010405 organic chemistryMolecular and BiophysicsGeneral ChemistryFunction (mathematics)540010402 general chemistry01 natural sciencesSpectral line3. Good health0104 chemical sciencesHighly sensitiveChemistryddc:540Vibrational circular dichroismStatistical physicsSDG 7 - Affordable and Clean EnergySpectroscopyConformational isomerismReliability (statistics)
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Local properties of quantum chemical systems: the LoProp approach.

2004

A new method is presented, which makes it possible to partition molecular properties like multipole moments and polarizabilities, into atomic and interatomic contributions. The method requires a subdivision of the atomic basis set into occupied and virtual basis functions for each atom in the molecular system. The localization procedure is organized into a series of orthogonalizations of the original basis set, which will have as a final result a localized orthonormal basis set. The new localization procedure is demonstrated to be stable with various basis sets, and to provide physically meaningful localized properties. Transferability of the methyl properties for the alkane series and of t…

Polarisabilitybusiness.industryChemistryGeneral Physics and AstronomyBasis functionQuantum chemistryQuantum mechanicsddc:540Theoretical chemistryPhysics::Atomic and Molecular ClustersPartition (number theory)Molecular momentsOrthonormal basisStatistical physicsSet theoryPhysical and Theoretical ChemistrybusinessMultipole expansionQuantum chemistryBasis setSubdivisionThe Journal of chemical physics
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Surface induced smectic order in ionic liquids - an X-ray reflectivity study of [C(22)C(1)im](+)[NTf2](-)

2017

Physical chemistry, chemical physics 19(39), 26651 - 26661 (2017). doi:10.1039/C7CP04852A

Polarized light microscopyMaterials scienceCondensed matter physicsScatteringGeneral Physics and Astronomy02 engineering and technology010402 general chemistry021001 nanoscience & nanotechnology54001 natural sciences0104 chemical sciencesX-ray reflectivityCondensed Matter::Soft Condensed Matterchemistry.chemical_compoundCrystallographychemistryMetastabilityPhase (matter)Ionic liquidddc:540Melting pointPhysical and Theoretical Chemistry0210 nano-technologySupercooling
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Diffusion of single molecular and macromolecular probes during the free radical bulk polymerization of MMA : towards a better understanding of the Tr…

2016

Free radical bulk polymerizations exhibit complex kinetics due to the viscosity increase during the polymerization process. Especially the termination rate constant can be strongly influenced by the mobility of polymer chains in the polymerization mixture. As a consequence an autoacceleration period, the so-called Trommsdorff effect, can be observed often. In order to investigate this behaviour on a nanoscopic scale, we directly visualized the mobility of molecules and macromolecules in polymerizing MMA solutions using a combination of highly sensitive fluorescence correlation spectroscopy and widefield fluorescence microscopy. For this purpose, rather monodisperse PMMA chains were synthesi…

Polymers and PlasticsBulk polymerizationDispersityBioengineeringFluorescence correlation spectroscopy02 engineering and technologymacromolecular substances010402 general chemistry01 natural sciencesBiochemistryAutoaccelerationPolymer chemistryReversible addition−fragmentation chain-transfer polymerizationchemistry.chemical_classificationOrganic Chemistrytechnology industry and agriculturePolymer021001 nanoscience & nanotechnology0104 chemical sciencesChemical engineeringPolymerizationchemistryddc:540MMA; Trommsdorff effect0210 nano-technologyMacromolecule
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Monolayers of rod-shaped and disc-shaped liquid crystalline compounds at the air-water interface

2008

Calamitic (rod-shaped) and discotic (disc-shaped) thermotropic liquid crystalline (LC) compounds were spread at the air-water interface, and their ability to form monolayers was studied. The calamitic LCs investigated were found to form monolayers which behave analogously to conventional amphiphiles such as fatty acids. The spreading of the discotic LCs produced monolayers as well, but with a behaviour different from classical amphiphiles. The areas occupied per molecule are too small to allow the contact of all hydrophilic groups with the water surface and the packing of all hydrophobic chains. Various molecular arrangements of the discotics at the water surface to fit the spreading data a…

Polymers and PlasticsChemistryAir water interfaceLiquid crystallineThermotropic crystalExternColloid and Surface ChemistryChemical engineeringLiquid crystalAmphiphileMonolayerddc:540Materials ChemistryMoleculeOrganic chemistryInstitut für ChemiePhysical and Theoretical Chemistry
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