| 作成者 |
|
|
|
|
|
|
|
|
|
| 本文言語 |
|
| 出版者 |
|
|
|
| 発行日 |
|
| 収録物名 |
|
| 巻 |
|
| 号 |
|
| 開始ページ |
|
| 終了ページ |
|
| 出版タイプ |
|
| アクセス権 |
|
| JaLC DOI |
|
| 関連DOI |
|
|
|
|
|
|
|
| 関連URI |
|
|
|
|
|
|
|
| 関連情報 |
|
|
|
|
|
|
|
| 概要 |
The CS^+(B^2Σ^+-A^2Π_i) emissions have been observed from dissociative charge-transfer reactions of He^+ with CS_2 and OCS in a helium afterglow. The vibrational distribution of CS^+(B) has a peak at ...v'=1 or 2 for both reactions. The average fraction of the total excess energy deposited into vibration of CS^+(B) was estimated to be≤13%, indicating that almost all excess energy is partitioned into the relative translational energy of the products. The higher vibrational excitation than the statistical prediction led us to conclude that CS^+(B) is formed directly through short lived intermediates.続きを見る
|
Mendeley出力
KJ00004507786