메뉴 건너뛰기




Volumn 111, Issue 50, 2007, Pages 12932-12937

Interstellar molecule CCCN may be formed by charge-stripping of [CCCN]- In the gas phase, and when energized, undergoes loss of C with partial carbon scrambling

Author keywords

[No Author keywords available]

Indexed keywords

CHEMICAL IONIZATION; INTERSTELLAR MOLECULES; NEUTRALIZATION;

EID: 38349080769     PISSN: 10895639     EISSN: None     Source Type: Journal    
DOI: 10.1021/jp076315j     Document Type: Article
Times cited : (9)

References (70)
  • 64
    • 38349035402 scopus 로고    scopus 로고
    • Frisch, M. J, Trucks, G. W, Schlegel, H. B, Scuseria, G. E, Robb, M. A, Cheeseman, J. R, Montgomery, J. A, Vreven, T, Kudin. K. N, Burant, J. C, Millam, J. M, Iyengar, S. S, Tomasi, J, Barone, V, Mennucci, B, Cossi, M, Scalmani, G, Rega, N, Petersson, G. A, Nakatsuji, H, Hada, M, Ehara, M, Topyota, K, Fukuda, R, Hasegawa, J, Ishida, M, Makajima, T, Honda, Y, Kitao, O, Nakai, H, Klene, M, Li, X, Know, J. E, Hratchian, H. P, Cross, J. B, Bakken, V, Adamo, C, Jaramillo, J, Gomperts, R, Stratmann, R. E, Yazyev, O, Austlin, A. J, Cammi, R, Pomelli, C, Ochterski, J. W, Ayala, P. Y, Morokuma, K, Voth, G. A, Salvador, P, Dannenberg. J. J, Zakrzewski, V. G, Dapprich, S, Daniels, A. D, Strain, M. C, Farkas, O, Malick, D. K, Rabuck, A. D, Raghavachari, K, Foresman, J. B, Ortiz, J. V, Cui, Q, Baboul, A. G, Cliffors, S, Cioslowski, J, Stefanov, B. B, Liu, G, Liashenko, A, Piskorz, P, Komaromi, L; Martin R. L, Fox, D. J, Keith, T
    • Frisch, M. J.; Trucks, G. W.; Schlegel, H. B.; Scuseria, G. E.; Robb, M. A.; Cheeseman, J. R.; Montgomery, J. A.; Vreven, T.; Kudin. K. N.; Burant, J. C.; Millam, J. M.; Iyengar, S. S.; Tomasi, J.; Barone, V.; Mennucci, B.; Cossi, M.; Scalmani, G.; Rega, N.; Petersson, G. A.; Nakatsuji, H.; Hada, M.; Ehara, M.; Topyota, K.; Fukuda, R.; Hasegawa, J.; Ishida, M.; Makajima, T.; Honda, Y.; Kitao, O.; Nakai, H.; Klene, M.; Li, X.; Know, J. E.; Hratchian, H. P.; Cross, J. B.; Bakken, V.; Adamo, C.; Jaramillo, J.; Gomperts, R.; Stratmann, R. E.; Yazyev, O.; Austlin., A. J.; Cammi, R.; Pomelli, C.; Ochterski, J. W.; Ayala, P. Y.; Morokuma, K.; Voth, G. A.; Salvador, P.; Dannenberg. J. J.; Zakrzewski, V. G.; Dapprich, S.; Daniels, A. D.; Strain, M. C.; Farkas, O.; Malick, D. K.; Rabuck, A. D.; Raghavachari, K.; Foresman, J. B.; Ortiz, J. V.; Cui, Q.; Baboul, A. G.; Cliffors, S.; Cioslowski, J.; Stefanov, B. B.; Liu, G.; Liashenko, A.; Piskorz, P.; Komaromi, L; Martin R. L.; Fox, D. J.; Keith, T.; Al-Latham, M. A.; Peng, C. Y.; Nanayakkara, A.; Challacombe, M.; Gill, P. M. W.; Johnson, B.; Chem, W.; Wong, M. W.; Ganzalez, C.; Pople, J. A. Gaussian 03, Revision C.02; Gaussian, Inc.: Wallingford, CT, 2004.
  • 66
    • 0001138789 scopus 로고    scopus 로고
    • 62
    • 62
  • 69
    • 38349082802 scopus 로고    scopus 로고
    • - is 20:1, which means any such rearrangement is minimal in this system.
    • - is 20:1, which means any such rearrangement is minimal in this system.
  • 70
    • 38349038785 scopus 로고    scopus 로고
    • We have repeated some calculations reported previously, namely, i) CCCN is confirmed as linear at the MP2/6-311 G(d,p) level of theory,33 but (ii) at the B3LYP/6-311G(d) level of theory we find two minima, a stable linear structure (as reported),27 and a bent structure (C1C 2 1.263 Â; C2C31.353 Â; C 3N 1.167 Â: C1C2C3162.1°, C2C3N 178.5°; dihedral angle 180°, The bent structure is the more stable by 6.5 kcal mol-1 [B3LYP/ 6-31lG(d, and 6.9 kcal mol-1 [CCSD(T)aug-cc-pVDZ//B3LYP/6-311G(d, CCCN is also bent (there is no stable linear form) at the B3LYP/6311+G(d) level of theory C1C2 1.266 Â; C2C3 1.351 Â; C3N 1.167 Â; C1C2C3 162.9°; C2C3N 178.4°; dihedral angle 180°
    • 3N 178.4°; dihedral angle 180°).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.