Titan is the largest satellite of
Saturn. In its
atmosphere, CH
4 is the most abundant neutral after nitrogen. Inthis paper, the complex doublet potential-energy surface related to the reaction between HCN
+ and CH
4 isinvestigated at the B3LYP/6-311G(d,p), CCSD(T)/6-311G++(3df,2pd)(single-point), and QCISD/6-311G(d,p) computational levels. A total of seven products are located on the PES. The initial association of HCN
+with CH
4 is found to be a prereaction complex
1 (HCNHCH
3+) without barrier. Starting from
1, the mostfeasible pathway is the direct H-abstraction process (the internal C-H bond dissociation) leading to the product
P1 (HCNH
++CH
3). By C-C addition, prereaction complex
1 can form intermediate
2 (HNCHCH
3+) andthen lead to the product
P2 (CH
3CNH
++H). The rate-controlling step of this process is only 25.6 kcal/mol.It makes the Path
P2 (1)
R
1
TS1/2
2
TS2/P2
P2 another possible way for the reaction.
P3 (HCNCH
3+ + H),
P5 (cNCHCH
2+ + H
2), and
P6 (NCCH
3+ + H
2) are exothermic products, but theyhave higher barriers (more than 40.0 kcal/mol);
P4 (H + HCN + CH
3+) and
P7 (H + H
2 + HCCNH
+)are endothermic products. They should be discovered under different experimental or interstellarconditions. The present study may be helpful for investigating the analogous ion-molecule reaction in Titan's
atmosphere.