0000000000075453

AUTHOR

Tomás González-lezana

0000-0003-0010-5219

showing 6 related works from this author

Rovibrational transitions of H 2 by collision with H + at high temperature

2017

The H+ + H2 reaction is studied by means of both exact and statistical quantum methods. Integral cross-sections for processes initiated with rotationally excited H2(v, j = 1) to produce molecular hydrogen in its rotational ground state are reported up to a value of the collision energy of 3 eV. Rate constants for state-to-state transitions between different H2 rovibrational states are calculated up to 3000 K. Special emphasis is made on ortho/para conversion processes in which the parity j of the H2(j) states changes.

Physics010304 chemical physicsMolecular dataScatteringAstronomy and AstrophysicsRotational–vibrational spectroscopy010402 general chemistryCollisionMolecular processes01 natural sciences0104 chemical sciencesScatteringSpace and Planetary Science0103 physical sciencesAtomic physicsMonthly Notices of the Royal Astronomical Society
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Ortho-H2 and the age of prestellar cores

2013

Prestellar cores form from the contraction of cold gas and dust material in dark clouds before they collapse to form protostars. Several concurrent theories exist to describe this contraction but they are currently difficult to distinguish. One major difference is the timescale involved in forming the prestellar cores: some theories advocate nearly free-fall speed via, e.g., rapid turbulence decay, while others can accommodate much longer periods to let the gas accumulate via, e.g., ambipolar diffusion. To tell the difference between these theories, measuring the age of prestellar cores could greatly help. However, no reliable clock currently exists. We present a simple chemical clock based…

Physics[PHYS]Physics [physics]AstrochemistryTurbulenceAmbipolar diffusionMolecular cloudAstronomy and AstrophysicsCosmic rayAstrophysics01 natural sciencesChemical clock13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Ionization0103 physical sciencesProtostar010306 general physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUS
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Quasiclassical Trajectory and Statistical Quantum Calculations for the C + OH → CO + H Reaction on the First Excited 12A″ Potential Energy Surface

2013

We report quasiclassical trajectory dynamical calculations for the C( 3P) + OH(X2Π) → CO(a3Π) + H( 2S) using a recently developed ab initio potential energy surface for the first electronic state of HCO of 12A″ symmetry. The dependence of integral cross sections on the collision energy was determined. Product energy and angular distributions have also been calculated. Integral cross sections show no energy threshold and decrease as the collision energy increases. The comparison with results obtained from a statistical quantum method seems to confirm that the reaction is mainly dominated by an indirect mechanism in which a long-lived intermediate complex is involved. © 2013 American Chemical…

PhysicsQuantum mechanicsExcited statePotential energy surfacePhysical and Theoretical ChemistryAtomic physicsTrajectory (fluid mechanics)QuantumThe Journal of Physical Chemistry A
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Ortho−ParaH2Conversion by Proton Exchange at Low Temperature: An Accurate Quantum Mechanical Study

2011

We report extensive, accurate fully quantum, time-independent calculations of cross sections at low collision energies, and rate coefficients at low temperatures for the ${\mathrm{H}}^{+}+{\mathrm{H}}_{2}(v=0,j)\ensuremath{\rightarrow}{\mathrm{H}}^{+}+{\mathrm{H}}_{2}(v=0,{j}^{\ensuremath{'}})$ reaction. Different transitions are considered, especially the ortho-para conversion ($j=1\ensuremath{\rightarrow}{j}^{\ensuremath{'}}=0$) which is of key importance in astrophysics. This conversion process appears to be very efficient and dominant at low temperature, with a rate coefficient of $4.15\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}10}\text{ }\text{ }{\mathrm{cm}}^{3}\text{ }{\ma…

PhysicsCrystallography010304 chemical physicsProton0103 physical sciencesGeneral Physics and AstronomyPhysical chemistry010303 astronomy & astrophysics01 natural sciences7. Clean energyQuantumPhysical Review Letters
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H-2, H-3(+) and the age of molecular clouds and prestellar cores

2012

Measuring the age of molecular clouds and prestellar cores is a difficult task that has not yet been successfully accomplished although the information is of paramount importance to help in understanding and discriminating between different formation scenarios. Most chemical clocks suffer from unknown initial conditions and are therefore difficult to use. We propose a new approach based on a subset of deuterium chemistry that takes place in the gas phase and for which initial conditions are relatively well known. It relies primarily on the conversion of H 3 + into H 2D + to initiate deuterium enrichment of the molecular gas. This conversion is controlled by the ortho/para ratio of H2 that i…

AstrochemistryAbundance (chemistry)General MathematicsGeneral Physics and AstronomySULFUR CHEMISTRYAstrophysicsINITIAL CONDITIONS01 natural sciences7. Clean energySTAR-FORMATION0103 physical sciencesGravitational collapseProtostar010306 general physics010303 astronomy & astrophysicsAMBIPOLAR DIFFUSIONCOSMIC-RAY IONIZATION[PHYS]Physics [physics]INTERSTELLAR-MEDIUMStar formationMolecular cloudTRIPLY DEUTERATED AMMONIAGeneral EngineeringORTHO-PARA TRANSITIONSInterstellar mediumDARK CLOUDSGRAVITATIONAL COLLAPSEDeuterium13. Climate action[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Quantum mechanical study of the proton exchange in the ortho-para H2 conversion reaction at low temperature

2011

Ortho-para H2 conversion reactions mediated by the exchange of a H+ proton have been investigated at very low energy for the first time by means of a time independent quantum mechanical (TIQM) approach. State-to-state probabilities and cross sections for H+ + H 2 (v = 0, j = 0,1) processes have been calculated for a collision energy, Ec, ranging between 10-6 eV and 0.1 eV. Differential cross sections (DCSs) for H+ + H2 (v = 0, j = 1) → H+ + H2 (v′ = 0, j′ = 0) for very low energies only start to develop a proper global minimum around the sideways scattering direction ( ≈ 90°) at Ec = 10-3 eV. Rate coefficients, a crucial information required for astrophysical models, are provided between 10…

PhysicsConversion reaction010304 chemical physicsProtonScatteringMolecular cloudRelaxation (NMR)Hydrogen moleculeGeneral Physics and Astronomy010402 general chemistry7. Clean energy01 natural sciences[PHYS] Physics [physics]0104 chemical sciences[ PHYS.PHYS.PHYS-CHEM-PH ] Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]13. Climate action0103 physical sciences[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Physical and Theoretical ChemistryAtomic physicsQuantumComputingMilieux_MISCELLANEOUSLine (formation)
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