Search results for "Spectral"

showing 10 items of 3116 documents

Age‐induced change in the color of the human crystalline lens

2011

Purpose To determine the chromatic coordinates of different human crystalline lenses to analyze the age-induced change in the color of the crystalline. Methods The spectral transmission of nine human crystalline lenses of different ages were measured by using a Perkin-Elmer 800 UV/VIS spectrophotometer. Using these data we calculated the chromatic coordinates of each crystalline lens for both solar and incandescent illumination. The study adheres to the tenets of the Declaration of Helsinki for Research Including Human Subjects and was approved by the Institutional Review Board. Results The results show a greater saturation of color with the increase of age. In principle, the change tends t…

Incandescent light bulbMaterials sciencebusiness.industrySpectral transmissionGeneral Medicineeye diseaseslaw.inventionLens (optics)OphthalmologyOpticslawTotal transmissionSolar lightsense organsChromatic scalebusinessActa Ophthalmologica
researchProduct

Continuous spectrum for a two phase eigenvalue problem with an indefinite and unbounded potential

2020

Abstract We consider a two phase eigenvalue problem driven by the ( p , q ) -Laplacian plus an indefinite and unbounded potential, and Robin boundary condition. Using a modification of the Nehari manifold method, we show that there exists a nontrivial open interval I ⊆ R such that every λ ∈ I is an eigenvalue with positive eigenfunctions. When we impose additional regularity conditions on the potential function and the boundary coefficient, we show that we have smooth eigenfunctions.

Indefinite unbounded potentialPure mathematicsNehari manifoldApplied Mathematics010102 general mathematicsContinuous spectrumBoundary (topology)Function (mathematics)Robin boundary conditionMathematics::Spectral TheoryEigenfunction01 natural sciences(pq)-LaplacianRobin boundary condition010101 applied mathematicsSettore MAT/05 - Analisi MatematicaLagrange multiplier rule0101 mathematicsSobolev embedding theoremNehari manifoldLaplace operatorAnalysisEigenvalues and eigenvectorsMathematicsJournal of Differential Equations
researchProduct

Neural network prediction of the AE index from the PC index

1999

Abstract It is shown that although the power spectra of the AE and PC data are quite similar they show differencies in structure function analysis. While the AE time series has a clear drop in the slope of the structure function (SF) after the first 2 hours, the slope of the SF of the PC data decreases gradually and at a little longer time scale. It is also shown by using 15-min averaged data, that both SFs are periodic with a clear diurnal variation. The PC time series seems to have a more pronounced periodicity, probably because it is measured at a single station at Thule. The AE index has been derived from the PC index for 7.5 minutes ahead by different methods. All these predictions gav…

Index (economics)MeteorologySeries (mathematics)Correlation coefficientArtificial neural networkDiurnal temperature variationStructure functionGeneral Earth and Planetary SciencesSingle stationSpectral lineMathematicsComputational physicsPhysics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science
researchProduct

Analysis of spectral irradiance distribution for PV applications at high latitude

2020

The spectral distribution of global tilted irradiance measured in Grimstad, Norway, is analyzed in terms of the average photon energy ( $APE$ ) blue fraction ( $BF$ ) and useful fraction ( $UF$ ). The results based on eight months of recorded data show a general shift of the $APE,\ BF$ , and $UF$ values to higher values than reference AM1.5G spectrum, with 1.63 eV, 0.45, and 0.88 being the average indices, respectively. The statistical coefficient of variation ( $CV$ ) is used to determine the variation of indices. The $CV$ for $APE,\ BF$ , and $UF$ are calculated to be 20.1%, 26.1%, and 25.7%, respectively confirming the earlier findings on $APE$ being a more accurate index for the quantif…

Index (economics)Spectral power distribution020209 energymedia_common.quotation_subjectCoefficient of variationIrradiance02 engineering and technologyPhoton energy021001 nanoscience & nanotechnologyAtmospheric sciencesSpectroradiometerDistribution (mathematics)Sky0202 electrical engineering electronic engineering information engineering0210 nano-technologyMathematicsmedia_common2020 47th IEEE Photovoltaic Specialists Conference (PVSC)
researchProduct

Harrison-Zel'dovich primordial spectrum is consistent with observations

2010

Inflation predicts primordial scalar perturbations with a nearly scale-invariant spectrum and a spectral index approximately unity (the Harrison--Zel'dovich (HZ) spectrum). The first important step for inflationary cosmology is to check the consistency of the HZ primordial spectrum with current observations. Recent analyses have claimed that a HZ primordial spectrum is excluded at more than 99% c.l.. Here we show that the HZ spectrum is only marginally disfavored if one considers a more general reionization scenario. Data from the Planck mission will settle the issue.

Inflation (cosmology)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Spectral densityFOS: Physical sciencesFísicaAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCMB cold spotGeneral Relativity and Quantum CosmologyCosmologyHigh Energy Physics - Phenomenologysymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Observational cosmologysymbolsPlanckAstrophysics - High Energy Astrophysical PhenomenaReionizationAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Impact of general reionization scenarios on extraction of inflationary parameters

2010

Determination of whether the Harrison-Zel'dovich spectrum for primordial scalar perturbations is consistent with observations is sensitive to assumptions about the reionization scenario. In light of this result, we revisit constraints on inflationary models using more general reionization scenarios. While the bounds on the tensor-to-scalar ratio are largely unmodified, when different reionization schemes are addressed, hybrid models are back into the inflationary game. In the general reionization picture, we reconstruct both the shape and amplitude of the inflaton potential. We discuss how relaxing the simple reionization restriction affects the reconstruction of the potential through the c…

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundCosmic background radiationAstrophysics::Instrumentation and Methods for AstrophysicsSpectral densityFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsInflatonCMB cold spotCosmologyGeneral Relativity and Quantum CosmologyFísica nuclearReionizationAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Primordial power spectrum features in phenomenological descriptions of inflation

2016

We extend an alternative, phenomenological approach to inflation by means of an equation of state and a sound speed, both of them functions of the number of $e$-folds and four phenomenological parameters. This approach captures a number of possible inflationary models, including those with non-canonical kinetic terms or scale-dependent non-gaussianities. We perform Markov Chain Monte Carlo analyses using the latest cosmological publicly available measurements, which include Cosmic Microwave Background (CMB) data from the Planck satellite. Within this parametrization, we discard scale invariance with a significance of about $10\sigma$, and the running of the spectral index is constrained as …

Inflation (cosmology)PhysicsSpectral indexCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsEquation of state (cosmology)Cosmic microwave backgroundFOS: Physical sciencesSpectral densityAstronomy and AstrophysicsMarkov chain Monte CarloAstrophysics::Cosmology and Extragalactic AstrophysicsScale invariance01 natural sciencessymbols.namesakeSpace and Planetary Science0103 physical sciencessymbolsStatistical physicsPlanck010303 astronomy & astrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics of the Dark Universe
researchProduct

Regional Susceptibility in VCD Spectra to Dynamic Molecular Motions

2018

Experimental and theoretical studies of the vibrational circular dichroism (VCD) spectrum of 3-methyl-1-(methyldiphenlsilyl)-1-phenylbutan-1-ol, whose absolute configuration is key to elucidating the Brook rearrangement of tertiary benzylic α-hydroxylsilanes, are presented. It is found that the entire OH-bending region in this spectrum—a region that provides important marker bands—cannot be reproduced at all by standard theoretical approaches even though other regions are well described. Using a novel approach to disentangle contributions to the rotational strength of these bands, internal coordinates are identified that critically influence the appearance of this part of the spectrum. We s…

Infrared spectroscopy02 engineering and technology010402 general chemistry01 natural sciencesMolecular physicsSpectral lineForce field (chemistry)COUPLED OSCILLATOR MECHANISMconformations analysisMolecular motionIMPLEMENTATIONPhysical and Theoretical Chemistrydensity functional theoryPhysicsconfiguration determinationVIBRATIONAL CIRCULAR-DICHROISMOLD CONCEPTAbsolute configurationCORRELATION-ENERGYBrook rearrangement021001 nanoscience & nanotechnologyvibrational circular dichroismAtomic and Molecular Physics and Opticsvibrational spectroscopy0104 chemical sciencesMODELLARGE-AMPLITUDE MOTIONSVibrational circular dichroismFORCE-FIELDDensity functional theory0210 nano-technologyAPPROXIMATIONChemphyschem
researchProduct

Unveiling the nature of six HMXBs through IR spectroscopy

2008

The International Gamma-Ray Astrophyiscs Laboratory (INTEGRAL) is discovering a large number of new hard X-ray sources, many of them being HMXBs. The identification and spectral characterization of their optical/infrared counterparts is a necessary step to undertake detailed study of these systems. In particular, the determination of the spectral type is crucial in the case of the new class of Supergiant Fast X-ray Transients (SFXTs), which show X-ray properties common to other objects. We used the ESO/NTT SofI spectrograph to observe proposed IR counterparts to HMXBs, obtaining Ks medium resolution spectra (R = 1320) with a S/N >= 100. We classified them through comparison with publishe…

InfraredAstrophysics::High Energy Astrophysical PhenomenaExtinction (astronomy)FOS: Physical sciencesInfrared spectroscopyAstrophysicsAstrophysicsStellar classificationSpectral line:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos X [UNESCO]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos XSpectroscopySpectrographAstrophysics::Galaxy AstrophysicsPhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsAccretion accretion disksX-rays : binaries; Stars : supergiants; Accretion accretion disks; Infrared : starsSpace and Planetary Sciencestars [Infrared]binaries [X-rays]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasSupergiantsupergiants [Stars]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]Astronomy & Astrophysics
researchProduct

Vibrational Sum Frequency Generation Spectroscopy of the Water Liquid–Vapor Interface from Density Functional Theory-Based Molecular Dynamics Simulat…

2013

International audience; The vibrational sum frequency generation (VSFG) spectrum of the water liquid-vapor (LV) interface is calculated using density functional theory-based molecular dynamics simulations. The real and imaginary parts of the spectrum are in good agreement with the experimental data, and we provide an assignment of the SFG bands according to the dipole orientation of the interfacial water molecules. We use an instantaneous definition of the surface, which is more adapted to the study of interfacial phenomena than the Gibbs dividing surface. By calculating the vibrational (infrared, Raman) properties for interfaces of varying thickness, we show that the bulk spectra signature…

InfraredBulk spectra02 engineering and technologyMolecular dynamicsVibrational sum-frequency generations010402 general chemistry01 natural sciencesMolecular physicsSpectral lineInterfacial phenomenaLiquid-vapor interfaceMolecular dynamicssymbols.namesakeDipole orientationComputational chemistryGeneral Materials SciencePhysical and Theoretical ChemistryDividing surfacesDensity functionalsSum-frequency generationMolecular dynamics simulationsChemistryInterfacial water moleculesThin layers021001 nanoscience & nanotechnologyLiquid-vapor0104 chemical sciencesDipoleImaginary partsDensity functional theoryVaporssymbolsDensity functional theory[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]0210 nano-technologyRaman spectroscopyVarying thicknessSum frequency generation spectroscopyThe Journal of Physical Chemistry Letters
researchProduct