State-to-state cross sections are reported for vibrational-rotational transitions for HF in collisions with He, at collisional energies of 0.5 and 1.0 eV. These were computed within the infinite-order sudden (IOS) approximation using adiabatic, distorted-wave techniques. Values are tabulated for the vibrational-rotational deexcitation sequences (v,j)→(v-1, 0), with v=1, 2, 3, 4 and j=0-40. These quenching cross sections can be used in conjunction with IOS factorization formulas to compute VRT cross sections for final rotational states other jf=0. In addition to IOS results, vibrational quenching cross sections were computed using the much more simple breathing-sphere technique. The breathing-sphere results compare favorably to the more accu...
Rate coefficients for pure rotational quenching in H2(ν 1 = 0, j 1) + H2(ν 2 = 0, j 2) collisions fr...
Context. Because of their high reactivity, the CH and OH radicals are of particular interest in astr...
The HD molecule is an important coolant in early universe chemistry models and a tracer of H2 in sta...
State-to-state cross sections are reported for vibrational-rotational transitions for HF in collisio...
Context. Collisional excitation rate coefficients play an important role in the dynamics of energy t...
The results of close coupling (CC) and infinite order sudden (IOS) approximation calculations of...
Parity resolved state-to-state cross sections for rotational excitation of OH(X¿2¿) colliding with H...
Collisional quenching of molecular species is an important process in a variety of astrophysical env...
Abstract. Rate coecients for rovibrational transitions induced in HD by collisions with He are prese...
Cross sections have been computed for non-reactive rovibrational transitions of H(_2) and HD, induce...
Energy loss distributions of He+ ions after collisions with HF molecules in a secondary beam at labo...
Results of a fully three‐dimensional classical trajectory calculation of vibrational energy transfer...
A simple model potential energy surface is constructed and used in both quasiclassical trajectory ca...
Vibrational (v) state-selected reaction probabilities (PvjJ) have been calculated for the reaction H...
Relative state-to-state cross sections are obtained for OH colliding with CO, N2, and CO2. Hexapole ...
Rate coefficients for pure rotational quenching in H2(ν 1 = 0, j 1) + H2(ν 2 = 0, j 2) collisions fr...
Context. Because of their high reactivity, the CH and OH radicals are of particular interest in astr...
The HD molecule is an important coolant in early universe chemistry models and a tracer of H2 in sta...
State-to-state cross sections are reported for vibrational-rotational transitions for HF in collisio...
Context. Collisional excitation rate coefficients play an important role in the dynamics of energy t...
The results of close coupling (CC) and infinite order sudden (IOS) approximation calculations of...
Parity resolved state-to-state cross sections for rotational excitation of OH(X¿2¿) colliding with H...
Collisional quenching of molecular species is an important process in a variety of astrophysical env...
Abstract. Rate coecients for rovibrational transitions induced in HD by collisions with He are prese...
Cross sections have been computed for non-reactive rovibrational transitions of H(_2) and HD, induce...
Energy loss distributions of He+ ions after collisions with HF molecules in a secondary beam at labo...
Results of a fully three‐dimensional classical trajectory calculation of vibrational energy transfer...
A simple model potential energy surface is constructed and used in both quasiclassical trajectory ca...
Vibrational (v) state-selected reaction probabilities (PvjJ) have been calculated for the reaction H...
Relative state-to-state cross sections are obtained for OH colliding with CO, N2, and CO2. Hexapole ...
Rate coefficients for pure rotational quenching in H2(ν 1 = 0, j 1) + H2(ν 2 = 0, j 2) collisions fr...
Context. Because of their high reactivity, the CH and OH radicals are of particular interest in astr...
The HD molecule is an important coolant in early universe chemistry models and a tracer of H2 in sta...