Rotational cross sections and rate coefficients fore-CO ande-HCN collisions under interstellar conditions
作者： Samir Saha , Swati Ray , B. Bhattacharyya , A. K. Barua
关键词: Interstellar cloud 、 Atomic physics 、 Schrödinger equation 、 Excited state 、 Atmospheric temperature range 、 Rotational temperature 、 Electron ionization 、 Physics 、 Differential equation 、 Perturbation (astronomy)
摘要: Rotational cross sections and rate coefficients for $e$-CO $e$-HCN collisions have been calculated in the energy range relevant to dark interstellar clouds by using close-coupling method. Gordon's technique has used solving coupled Schr\"odinger equations. Initial rotational levels $j=0, 1, \mathrm{and} 2$ of CO HCN considered. The 0.0006 0.1 eV temperature 5-100 K. thus obtained compared with Born unitarized time-dependent perturbation calculations.
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