Search results for " Methods"

showing 10 items of 4102 documents

Vibrational analysis of the electronic spectrum of ethylene based onab initio SCF-CI calculations

1972

Ab initio calculations for CH2 twisting and CC stretching vibrational wavefunctions and energy levels are reported for various electronic states of ethylene C2H4. Electronic transition moments between these states are also obtained to allow a calculation of the oscillator strengths for vibrational transitions involved in various electronic band systems; from this study it is concluded that thevertical electronic energy differenceΔE e may differ significantly from the energy of the absorption maximumΔE max with which it is often equated. In particular it is found in the case of theπ→π * singlet-singlet excitation of ethylene that theΔE e value overestimates the most probable vibrational tran…

ChemistryTransition dipole momentAb initioMolecular electronic transitionsymbols.namesakeAb initio quantum chemistry methodsRydberg formulasymbolsChiropracticsPhysics::Chemical PhysicsPhysical and Theoretical ChemistryAtomic physicsAbsorption (electromagnetic radiation)Wave functionExcitationTheoretica Chimica Acta
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General occurrence of polar twisted minima in the ionic singlet excited surfaces of polyenes

1982

Except for a few cases, the lowest closed shell SCF solutions for the twisted geometries of polyenes involves delocalized nonpolarized MO’s, and represents a meaningless mixture of radicalar gound state and ionic excited states. Higher (quasi) solutions allow a realistic approach of the polarized ionic states. Orthogonality to the radicalar ground state may be imposed without important loss of energy. Further extensive CI does not modify significantly the situation. These statements are illustrated through ab initio calculations of butadiene and hexatriene. This approach allows us to show that slight distortions stablize polar minima even in ’’homosymmetric’’ molecules such as all‐trans hex…

ChemistryUNESCO::FÍSICAGeneral Physics and AstronomyIonic bondingElectronic structurePolyenesExcited StatesSelf−Consistent FieldDelocalized electronElectronic StructureAb initio quantum chemistry methods:FÍSICA [UNESCO]Polyenes ; Self−Consistent Field ; Electronic Structure ; Excited StatesExcited statePhysics::Atomic and Molecular ClustersSinglet statePhysical and Theoretical ChemistryAtomic physicsPhysics::Chemical PhysicsGround stateOpen shell
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Effects of Cooking Method upon Flavor of Carrots and Peas

1987

Two modalities of pressure (atmospheric pressure and high-pressure of 5.5.104 Pa) and two modalities of immersion (boiling and cooking in steam) were combined factorially to produce four ways of cooking. These different cooking methods were studied on two vegetables: carrots and peas. Sensory attributes of samples were assessed on an unstructured scale. Steam-cooked vegetables have higher sensory attributes (odor and flavor intensities, typical odor and flavor notes, sweetness). Larger losses of soluble solids and volatiles are believed to account for these differences between vegetables cooked in water and cooked in steam.

Chemistry[SDV]Life Sciences [q-bio]Cooking methodstechnology industry and agriculturefood and beverages04 agricultural and veterinary sciencesSweetness040401 food science[SDV] Life Sciences [q-bio]0404 agricultural biotechnologyOdorSoluble solidsBoilingotorhinolaryngologic diseasesFood scienceComputingMilieux_MISCELLANEOUSFlavorFood ScienceJournal of Food Science
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Comparison of electron diffraction data from non-linear optically active organic DMABC crystals obtained at 100 and 300 kV

2000

During the recent past, we have synthesized a new class of molecules with intramolecular two-dimensional charge transfer upon excitation. The present report presents such a molecule, 2,6-bis(4-dimethylamino-benzylidene)-cyclohexanone (DMABC), with an unusually high value of the second-order non-linear optical (NLO) coefficients. In order to optimize the macroscopic NLO properties of the compounds, it is necessary to relate their first hyperpolarizability tensors at a molecular level to those at a crystal bulk level. This requires a complete structure determination and refinement. However, the growth of sufficiently large single crystals, which are needed for structural analysis and refineme…

Chemistrybusiness.industryDirect methodResolution (electron density)Ab initioHyperpolarizabilityAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsComputational physicsCrystalOpticsElectron diffractionDirect methodsTensorbusinessInstrumentationUltramicroscopy
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Semiconducting Clathrates Meet Gas Hydrates: Xe24[Sn136]

2014

Semiconducting Group 14 clathrates are inorganic host–guest materials with a close structural relationship to gas hydrates. Here we utilize this inherent structural relationship to derive a new class of porous semiconductor materials: noble gas filled Group 14 clathrates (Ngx[M136], Ng=Ar, Kr, Xe and M=Si, Ge, Sn). We have carried out high-level quantum chemical studies using periodic Local-MP2 (LMP2) and dispersion-corrected density functional methods (DFT-B3LYP-D3) to properly describe the dispersive host–guest interactions. The adsorption of noble gas atoms within clathrate-II framework turned out to be energetically clearly favorable for several host–guest systems. For the energetically…

Chemistrybusiness.industryOrganic ChemistryClathrate hydrateeducationNoble gasGeneral ChemistryCatalysisSemiconductorAdsorptionChemical physicsComputational chemistryAb initio quantum chemistry methodsAtomNoble gas configurationbusinessPorosityta116
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Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

2023

The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3~PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy $\gamma$-ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs whi…

Cherenkov Telescope ArrayGamma rays: generalstatistical [methods]energy spectrumFOS: Physical sciencesVHESettore FIS/05 - Astronomia E Astrofisicacosmic raysMethods: data analysissupernovadata analysis [methods][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Cosmic raysInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov Telescope Arra ; alactic Supernova Remnants ; PeVatrons ;Methods: statisticalgalactic PeVatronsHigh Energy Astrophysical Phenomena (astro-ph.HE)emission spectrum) supernovae: general [(stars]Astronomy and AstrophysicssensitivityobservatoryGalactic PeVatronscosmic radiationspectralgalaxyhadron(Stars:) supernovae: generalAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statisticalgeneral [gamma rays]signature
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The e-ASTROGAM gamma-ray space observatory for the multimessenger astronomy of the 2030s

2018

e-ASTROGAM is a concept for a breakthrough observatory space mission carrying a gamma-ray telescope dedicated to the study of the non-thermal Universe in the photon energy range from 0.15 MeV to 3 GeV. The lower energy limit can be pushed down to energies as low as 30 keV for gamma-ray burst detection with the calorimeter. The mission is based on an advanced space-proven detector technology, with unprecedented sensitivity, angular and energy resolution, combined with remarkable polarimetric capability. Thanks to its performance in the MeV-GeV domain, substantially improving its predecessors, e-ASTROGAM will open a new window on the non-thermal Universe, making pioneering observations of the…

Cherenkov Telescope ArrayHigh-energy astrophysical phenomenaCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomyenergy resolution7. Clean energy01 natural sciencesSpace missionlaw.inventionIceCubeEinstein TelescopelawObservatoryLIGO010303 astronomy & astrophysicsKM3NeTPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Applied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionGamma-ray astronomyGamma-ray polarizationCondensed Matter Physicsphoton: energyobservatoryNuclear astrophysicsApace missionAstrophysics - High Energy Astrophysical Phenomenaperformancedetector: technologyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstspace missionCompton and pair creation telescopeTelescope0103 physical sciencessupernovaElectroniccalorimetergamma ray: detectorOptical and Magnetic MaterialsKAGRAElectrical and Electronic Engineering010306 general physicsTime domain astronomyLISAGamma-ray astronomyEinstein TelescopeAstronomyInstitut für Physik und AstronomieTime-domain astronomyCherenkov Telescope ArraysensitivityLIGOmessengerKM3NeTVIRGO13. Climate actionCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic Engineeringddc:520galaxyCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic Engineering[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

2021

Full list of authors: Acharyya, A.; Adam, R.; Adams, C.; Agudo, I.; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Alves Batista, R.; Amati, L.; Ambrosi, G.; Angüner, E. O.; Antonelli, L. A.; Aramo, C.; Araudo, A.; Armstrong, T.; Arqueros, F.; Asano, K.; Ascasíbar, Y. Ashley, M.; Balazs, C.; Ballester, O.; Baquero Larriva, A.; Barbosa Martins, V.; Barkov, M.; Barres de Almeida, U.; Barrio, J. A.; Bastieri, D.; Becerra, J.; Beck, G.; Becker Tjus, J.; Benbow, W.; Benito, M.; Berge, D.; Bernardini, E.; Bernlöhr, K.; Berti, A.; Bertucci, B.; Beshley, V.; Biasuzzi, B.; Biland, A.; Bissaldi, E.; Biteau, J.; Blanch, O.; Blazek, J.; Bocchino, F.; Boisson, C.; Bonneau Arbe…

Cherenkov Telescope ArrayMATÉRIA ESCURAscale: TeVAstronomyatmosphere [Cherenkov counter]dark matter experimentDark matter theoryenergy resolutionGamma ray experimentsParticleAstrophysicscosmic background radiation01 natural sciences7. Clean energyHigh Energy Physics - Phenomenology (hep-ph)benchmarkWIMPHESSenergy: fluxTeV [scale]relativistic [charged particle]gamma ray experimentMAGIC (telescope)Monte CarloEvent reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Contractionspatial distributiontrack data analysisPhysicsdensity [dark matter]ClumpyAstrophysics::Instrumentation and Methods for AstrophysicsimagingHigh Energy Physics - Phenomenologydark matter experiments; dark matter theory; gamma ray experiments; galaxy morphologyDark matter experimentsFísica nuclearVERITASAstrophysics - High Energy Astrophysical PhenomenaSimulationsnoiseWIMPAstrophysics::High Energy Astrophysical PhenomenaDark mattersatelliteCosmic background radiationFOS: Physical sciencesAnnihilationdark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsCherenkov counter: atmosphereheavy [dark matter]530annihilation [dark matter]GLASTDark matter experiments; Dark matter theory; Galaxy morphology; Gamma ray experimentscosmic radiation [p]0103 physical sciencesCherenkov [radiation]Candidatesddc:530AGNCherenkov radiationRadiative Processesthermal [cross section]010308 nuclear & particles physicsFísicadark matter: annihilationGamma-Ray SignalsCherenkov Telescope Array ; dark matter ; Galactic Center ; TeV gamma-ray astronomyAstronomy and AstrophysicsMassCherenkov Telescope Arrayradiation: CherenkovsensitivityMAGICGalaxyAstronomíadark matter: heavygamma rayp: cosmic radiation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]correlationcharged particle: relativisticflux [energy]Galaxy morphology/dk/atira/pure/subjectarea/asjc/3100/3103galaxysupersymmetry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cross section: thermal
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Combination of clinical risk profile, early exercise testing and circulating biomarkers for evaluation of patients with acute chest pain without ST-s…

2007

Objective: To investigate the combination of clinical data, exercise testing and biomarkers for the evaluation of patients with chest pain without ST-segment deviation or troponin elevation. Design: Prospective cohort design. Settting: Two teaching hospitals in Spain. Patients: 422 patients presenting to the emergency department were studied. Leukocyte count, C-reactive protein (CRP), pregnancy-associated plasma protein A (PAPP-A) and N-terminal pro-brain natriuretic peptide (NTproBNP) were determined. A validated clinical risk score (number of points according to pain characteristics and risk factors) was used for clinical evaluation and early exercise testing was performed. Main outcome m…

Chest Painmedicine.medical_specialtyMyocardial InfarctionPhysical exerciseChest painInternal medicineNatriuretic Peptide BrainmedicineHumansMyocardial infarctionRisk factorProspective cohort studyFramingham Risk Scorebiologybusiness.industryST elevationMiddle Agedmedicine.diseaseTroponinPeptide FragmentsTroponinSurgeryExercise Testbiology.proteinCardiologymedicine.symptomEpidemiologic MethodsCardiology and Cardiovascular MedicinebusinessBiomarkersHeart
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County-level socioeconomic and crime risk factors for substantiated child abuse and neglect.

2019

Rates of substantiated child abuse and neglect vary significantly across counties. Despite strong cross-sectional support for links between social-contextual characteristics and abuse and neglect, few longitudinal studies have tested relations between these risk factors and substantiated rates of abuse/neglect. The goal of this study was to identify county-level socioeconomic and crime factors associated with substantiated abuse/neglect rates over 13 years (2004-2016). Annual county-level data for Tennessee, obtained from the KIDS COUNT Data Center, included rates of substantiated child abuse and neglect, children's race and ethnicity, births to unmarried women, teen birth rate, children in…

Child abuseAdultMale050103 clinical psychologyAdolescentmedia_common.quotation_subjectPoison controlSuicide preventionArticleNeglectBirth rateYoung AdultInjury preventionDevelopmental and Educational PsychologyHumans0501 psychology and cognitive sciencesChild AbuseChildSocioeconomic statusmedia_common05 social sciencesSex OffensesInfant NewbornHuman factors and ergonomicsInfantHispanic or LatinoTennesseeBlack or African AmericanPsychiatry and Mental healthSocioeconomic FactorsChild PreschoolPediatrics Perinatology and Child HealthFemaleCrimePsychologyEpidemiologic Methods050104 developmental & child psychologyDemographyChild abuseneglect
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