0000000000276258

AUTHOR

Alain Faure

showing 3 related works from this author

A KInetic Database for Astrochemistry (KIDA)

2012

We present a novel chemical database for gas-phase astrochemistry. Named the KInetic Database for Astrochemistry (KIDA), this database consists of gas-phase reactions with rate coefficients and uncertainties that will be vetted to the greatest extent possible. Submissions of measured and calculated rate coefficients are welcome, and will be studied by experts before inclusion into the database. Besides providing kinetic information for the interstellar medium, KIDA is planned to contain such data for planetary atmospheres and for circumstellar envelopes. Each year, a subset of the reactions in the database (kida.uva) will be provided as a network for the simulation of the chemistry of dense…

Astrochemistry[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Interstellar cloudFOS: Physical sciencesAstrophysicsKinetic energycomputer.software_genreAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesmiscellaneous [astrochemistry; astronomical databases]010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysics010304 chemical physicsDatabaseKinetic informationAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesInterstellar mediumSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)computerChemical databaseGalaxy Astrophysics
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Rotational excitation of mono- and doubly-deuterated water by hydrogen molecules

2011

Rate coefficients for rotational transitions in HDO and D2O induced by H2 collisions below 300 K are presented. Calculations have been performed at the close-coupling and coupledstates levels with the deuterated variants of the H2O–H2 interaction potential of Valiron et al. The HDO–H2 and D2O–H2 rate coefficients are compared to the corresponding rate coefficients for HDO–He and H2O–H2, respectively. Significant differences are observed. In particular the new HDO rate coefficients are found to be significantly larger (by up to three orders of magnitude) than the corresponding HDO–He rate coefficients. The impact of the new HDO rate coefficients is examined with the help of non-LTE radiative…

PhysicsHydrogen moleculeAstronomy and Astrophysics010402 general chemistry01 natural sciences0104 chemical scienceslaw.inventionInteraction potentialOrders of magnitude (time)DeuteriumSpace and Planetary Sciencelaw0103 physical sciencesRadiative transferMaserAtomic physics010303 astronomy & astrophysicsExcitationMonthly Notices of the Royal Astronomical Society
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Analyzing observations of molecules in the ISM: Theoretical and experimental studies of energy transfer

2012

Our laboratories have recently calculated a set of collision coefficients characterizing the efficiency of energy transfer between helium and/or hydrogen and a large variety of interstellar molecules. We have considered with molecules ranging from light hydrides, observed by the Herschel Space Observatory, to medium size molecules, observed by mm antennas, to heavy complex organic molecules, observed also in the cm range. We present a review of recent theoretical results obtained in our laboratories, for various kinds of commonly observed molecules.

Physics[PHYS]Physics [physics]Range (particle radiation)Hydrogen010308 nuclear & particles physicsEnergy transferGeneral Engineeringchemistry.chemical_elementAstronomy and Astrophysics01 natural sciences7. Clean energyMolecular physicsSpace observatoryOrganic molecules[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry[CHIM.THEO] Chemical Sciences/Theoretical and/or physical chemistrychemistrySpace and Planetary Science0103 physical sciencesMoleculePhysics::Chemical Physics010303 astronomy & astrophysicsHeliumComputingMilieux_MISCELLANEOUS
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