Search results for "Millimeter"

showing 4 items of 44 documents

Universal charts for optical difference frequency generation in the terahertz domain

2010

We present a universal and rigorous approach to study difference frequency generation in the terahertz domain, keeping the number of degrees of freedom to a minimum, through the definition of a suitable figure of merit. The proposed method relies on suitably normalized charts, that enable to predict the optical-to-terahertz conversion efficiency of any system based on wave propagation in quadratic nonlinear materials. The predictions of our approach are found to be in good agreement with the best experimental results reported to date, enabling also to estimate the d22 nonlinear coefficient of high quality GaSe.

Wave propagationComputer scienceTerahertz radiationDegrees of freedom (statistics)FOS: Physical sciencesFrequency conversionSettore ING-INF/01 - ElettronicaOptical pulse generationDomain (software engineering)Semiconductor materialsQuadratic equationQuality (physics)Submillimeter wave transmittersFigure of meritOptical parametric amplifiersElectrical and Electronic EngineeringOptical propagation in nonlinear mediaOptical frequency conversionSettore ING-INF/02 - Campi ElettromagneticiCondensed Matter PhysicsAtomic and Molecular Physics and Opticsoptical parametric amplifiersemiconductor materialNonlinear systemAlgorithmOptics (physics.optics)Physics - OpticsIEEE Journal of Quantum Electronics
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Analysis of highly excited 'hot' bands in the SO2 molecule: ν2 + 3ν3 - ν2 and 2ν1 + ν2 + ν3 - ν2

2010

International audience; We set up a variational procedure of assignments of transitions and we applied it to the analysis very weak 'hot' bands, v(2) + 3v(3) - v(2) and 2v(1) + v(2) + v(3) - v(2), of the SO2 molecule. As the first step of the study, the 'cold' bands, 3v(3) and 2v(1) + v(3), are re-analysed and transitions belonging to those bands are assigned up to the values of quantum numbers J(max.) = 60, K-a(max.) = 19, and J(max.) = 69, K-a(max.) = 20 for the bands 3v(3) and 2v(1) + v(3), respectively. After 'cleaning' the experimental spectrum from transitions belonging to the 3v(3) and 2v(1) + v(3) bands, a variational procedure was used that allowed us to assign 230 and 115 transiti…

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]high-resolution spectraHIGH-RESOLUTION ANALYSISBiophysics02 engineering and technology01 natural sciences[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesMoleculespectroscopic parametersHigh resolution spectraPhysical and Theoretical ChemistrySpectroscopyLASER SPECTROSCOPYMolecular BiologyHigh resolution analysis010304 chemical physicsChemistryCOMBINATION BAND021001 nanoscience & nanotechnologyCondensed Matter PhysicsQuantum numberNU-3 BANDINTENSITIESSULFUR-DIOXIDEExcited stateLINE POSITIONSVIBRATIONAL-STATESsulphur dioxideEQUILIBRIUM ROTATIONAL-CONSTANTSAtomic physics0210 nano-technologySUBMILLIMETER-WAVE SPECTRUM
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The Born–Oppenheimer equilibrium bond distance of GeO from millimetre- and submillimetre-wave spectra and quantum-chemical calculations

2014

The millimetre- and submillimetre-wave spectra of the five common isotopologues of (GeO)-O-16 in their electronic and vibrational ground state have been recorded in the spectral region 115-732GHz; for (GeO)-Ge-74-O-16, the rotational spectrum in the v = 1 state has been detected as well. Exploiting the high precision of the measurements, the Born-Oppenheimer breakdown parameter Delta(Ge)(01) could be determined from a Dunham analysis of the spectral data, whereas Delta(O)(01) was obtained from quantum-chemical calculations, because of the lack of high-precision measurements for the (GeO)-O-18 isotopologues. From the rotational equilibrium constant, the Born-Oppenheimer equilibrium distance …

equilibrium bond distanceBorn-Oppenheimer breakdownrotational spectrumChemistryBiophysicsBorn–Oppenheimer approximationCondensed Matter PhysicsSpectral linequantum-chemical calculationBond lengthsymbols.namesakeRotational spectrumsymbolsMillimeterIsotopologuePhysical and Theoretical ChemistryAtomic physicsGround stateMolecular BiologyAstrophysics::Galaxy AstrophysicsEquilibrium constant
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Laboratory measurements and astronomical search for the HSO radical

2016

[Context] Despite the fact that many sulfur-bearing molecules, ranging from simple diatomic species up to astronomical complex molecules, have been detected in the interstellar medium, the sulfur chemistry in space is largely unknown and a depletion in the abundance of S-containing species has been observed in the cold, dense interstellar medium. The chemical form of the missing sulfur has yet to be identified.

inorganic chemicalsMethods: laboratory: molecularHydrogenLine: identificationlaboratory: molecular [Methods]chemistry.chemical_elementContext (language use)ISM: moleculeAstrophysics7. Clean energy01 natural sciencesArticleAbundance (ecology)0103 physical sciencesPhysics::Chemical Physicsidentification [Line]Spectral resolutionSubmillimeter: ISM010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmolecules [ISM]Radio lines: ISMPhysics010304 chemical physicsMolecular dataTriatomic moleculeISM [Submillimeter]AstronomyAstronomy and AstrophysicsAstronomy and AstrophysicSulfurDiatomic moleculeISM: moleculesISM [Radio lines]Interstellar mediumchemistry13. Climate actionSpace and Planetary ScienceAstronomy & Astrophysics
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