Rotational (de-) excitation of C3N- by collision with He atoms

被引:13
作者
Lara-Moreno, Miguel [1 ,2 ]
Stoecklin, Thierry [1 ]
Halvick, Philippe [1 ]
机构
[1] Univ Bordeaux, ISM, UMR 5255, F-33405 Talence, France
[2] Inst Super Tecnol & Ciencias Aplicadas, Plaza Revoluc, 10600 Havana, Cuba
关键词
astrochemistry; molecular data; molecular processes; scattering; ISM: molecules; RATE COEFFICIENTS; ASTRONOMICAL DETECTION; INTERSTELLAR ANION; TEMPERATURE; SCATTERING; MOLECULE; CLOUDS; IONS; C4H;
D O I
10.1093/mnras/stx434
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Since their recent detection in the interstellar medium, anions have raised the question of their possible mechanisms of formation, destruction and excitation. Among the observed anions, C3N- is an interesting species owing to its large dipole moment and its remarkable stability, since the electron affinity of C3N is particularly large. In this work, a quantum mechanical treatment of the rotational (de-)excitation of C3N- in collisions with He is reported. Full close-coupling calculations are performed within the rigid rotor approximation for the j = 0 up to 15 rotational levels of C3N- and for collision energies in the range 0.1-2000 cm(-1). These results are complemented for the j = 16 up to 30 rotational levels of C3N-by using two different approximations whose accuracies are tested against close-coupling results. The uniform J-shifting is found to give the most accurate results. At high collision energy, a strong propensity to favour |Delta j| = 2 transitions is observed and discussed. The rate coefficients for the rotational transitions between 1 and 300 K are reported.
引用
收藏
页码:4174 / 4179
页数:6
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