International audienceFrom a new two-dimensional Potential Energy Surface (PES), rotational excitation of the C2H−(X1Σ+) anion by collision with He is investigated. PES is obtained in the supermolecular approach based on a single and double-excitation coupled cluster method with perturbative contributions from triple excitations (CCSD(T)).Fully-quantum close-coupling calculations of inelastic integral cross sections are done on a grid of collision energies large enough to insure converged state-to-state rate coefficients for the 13 first rotational levels of C2H− and temperatures ranging from 5 to 100 K. For this collisional system, rate coefficients exhibit a strong propensity in favor of even ΔN transitions
Rate coefficients for rotational transitions in H2 induced by H2 impact are presented. Extensive qua...
Context.Observations of molecular emission at millimeter and infrared wavelengths, supplemented by c...
Context. An accurate analysis of the physical-chemical conditions in the regions of the interstellar...
International audienceFrom a new two-dimensional Potential Energy Surface (PES), rotational excitati...
International audienceFrom a new two-dimensional Potential Energy Surface (PES), rotational excitati...
International audienceFrom a new two-dimensional Potential Energy Surface (PES), rotational excitati...
9 pags., 8 figs., 1 tab.Accurate modeling of anionic abundances in the interstellar and circumstella...
Rates for rotational excitation of HC3N by collisions with He atoms and H2 molecules are computed fo...
International audienceAims.Rates for rotational excitation of HC_3N by collisions with He atoms and ...
International audienceAims.Rates for rotational excitation of HC_3N by collisions with He atoms and ...
Context.Over the next few years, Alma and Herschel missions will open the universe to high spatial a...
Context.Over the next few years, Alma and Herschel missions will open the universe to high spatial a...
Aims. The present paper focuses on the calculation of the collision rate coefficients for rotational...
Context. The Herschel Space Observatory with its high-resolution instrument HIFI on board will obser...
We have studied the fundamental rotational relaxation and excitation collision of OHˉJ = 0 ↔ 1 with ...
Rate coefficients for rotational transitions in H2 induced by H2 impact are presented. Extensive qua...
Context.Observations of molecular emission at millimeter and infrared wavelengths, supplemented by c...
Context. An accurate analysis of the physical-chemical conditions in the regions of the interstellar...
International audienceFrom a new two-dimensional Potential Energy Surface (PES), rotational excitati...
International audienceFrom a new two-dimensional Potential Energy Surface (PES), rotational excitati...
International audienceFrom a new two-dimensional Potential Energy Surface (PES), rotational excitati...
9 pags., 8 figs., 1 tab.Accurate modeling of anionic abundances in the interstellar and circumstella...
Rates for rotational excitation of HC3N by collisions with He atoms and H2 molecules are computed fo...
International audienceAims.Rates for rotational excitation of HC_3N by collisions with He atoms and ...
International audienceAims.Rates for rotational excitation of HC_3N by collisions with He atoms and ...
Context.Over the next few years, Alma and Herschel missions will open the universe to high spatial a...
Context.Over the next few years, Alma and Herschel missions will open the universe to high spatial a...
Aims. The present paper focuses on the calculation of the collision rate coefficients for rotational...
Context. The Herschel Space Observatory with its high-resolution instrument HIFI on board will obser...
We have studied the fundamental rotational relaxation and excitation collision of OHˉJ = 0 ↔ 1 with ...
Rate coefficients for rotational transitions in H2 induced by H2 impact are presented. Extensive qua...
Context.Observations of molecular emission at millimeter and infrared wavelengths, supplemented by c...
Context. An accurate analysis of the physical-chemical conditions in the regions of the interstellar...