0000000000466777

AUTHOR

Luca Bizzocchi

0000-0002-9953-8593

showing 3 related works from this author

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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Improved centrifugal and hyperfine analysis of ND2H and NH2D and its application to the spectral line survey of L1544

2021

Abstract Quantifying molecular abundances of astrochemical species is a key step towards the understanding of the chemistry occurring in the interstellar medium. This process requires a profound knowledge of the molecular energy levels, including their structure resulting from weak interactions between nuclear spins and the molecular rotation. With the aim of increasing the quality of spectral line catalogs for the singly- and doubly-deuterated ammonia (NH2D and ND2H), we have revised their rotational spectra by observing many hyperfine-resolved lines and more accurate high-frequency transitions. The measurements have been performed in the submillimeter-wave region (265–1565 GHz) using a fr…

Rotational spectroscopy010402 general chemistry01 natural sciencesStarless coreSpectral linelaw.inventionDeuterium fractionationAmmoniaInterstellar mediumlaw0103 physical sciencesPhysical and Theoretical ChemistryHyperfine structureAstrophysics::Galaxy AstrophysicsSpectroscopyLine (formation)010304 chemical physicsSpectrometerAtomic and Molecular Physics and OpticsSynchrotron0104 chemical sciencesComputational physicsInterstellar mediumDeuteriumHyperfine structureRotational spectroscopyJournal of Molecular Spectroscopy
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The magnetic hyperfine structure in the rotational spectrum of H2CNH

2010

Abstract The hyperfine structure in the ground-state rotational spectrum of methanimine was studied in the frequency range of 64–172 GHz by means of the Lamb-dip technique. This allowed to resolve, in some hyperfine components due to the 14N nucleus, doublets separated by only some tenth of kHz. We explain the splittings as due to magnetic interactions of the three protons with their molecular environment. The analysis of the experimental spectrum has been guided by quantum-chemical calculations of the hyperfine parameters.

PhysicsRange (particle radiation)Rotational spectrumPhysics::Atomic PhysicsRotational spectroscopyPhysical and Theoretical ChemistryAtomic physicsHyperfine structureSpectroscopyAtomic and Molecular Physics and OpticsJournal of Molecular Spectroscopy
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