Ab initio studies on amides: acetamide, N-methylformamide and N-methylacetamide

1982 ◽  
Vol 35 (6) ◽  
pp. 1071 ◽  
Author(s):  
L Radom ◽  
NV Riggs

Ab initio molecular orbital theory with the STO-3G and 4-31G basis sets has been used to investigate the geometries, preferred conformations, and barriers to internal rotation for acetamide, N-methylformamide and N-methylacetamide. Results are compared with corresponding previously reported data for formamide. For acetamide, the preferred conformation has the methyl group staggered with respect to the N-C bond whereas for N-methylformamide the methyl group is eclipsed with respect to this bond. Both N-methylformamide and N-methylacetamide prefer a Z-arrangement, i.e. methyl cis to C=O about the N-C bond. Experimentally determined barriers to internal rotation about the N-C bond generally lie within the range spanned by the STO-3G and 4-31G estimates.


1972 ◽  
Vol 25 (8) ◽  
pp. 1601 ◽  
Author(s):  
L Radom ◽  
WA Lathan ◽  
WJ Hehre ◽  
JA Pople

Ab initio molecular orbital theory is used to study internal rotation in 20 organic molecules of the types X-Y, X-CH2-Y, X-SH-Y, X-O-Y, and X-CO-Y-where X and Y are methyl, amino, hydroxy, or formyl groups. In some of these molecules, internal rotation about two bonds is possible. The theoretical results are generally in moderate agreement with available experimental data and, in addition, lead to a number of predictions for molecules for which experimental information is lacking.





1986 ◽  
Vol 119 (2) ◽  
pp. 234 ◽  
Author(s):  
Luigi Olcari


1992 ◽  
Vol 45 (1) ◽  
pp. 285 ◽  
Author(s):  
BJ Smith ◽  
JA Pople ◽  
LA Curtiss ◽  
L Radom

Ab initio molecular orbital theory at the G 2 level has been used to predict new values for the heat of formation of formaldimine (CH2=NH): ?Hfº0 = 94 ±10 kJ mol-1 and ?Hfº298 = 86 ±10 kJ mol-1.





2005 ◽  
Author(s):  
Inke Jones ◽  
Tamath J. Rainsford ◽  
Samuel P. Mickan ◽  
Derek Abbott


1977 ◽  
Vol 8 (47) ◽  
pp. no-no
Author(s):  
W. F. REYNOLDS ◽  
P. G. MEZEY ◽  
W. J. HEHERE ◽  
R. D. TOPSOM ◽  
R. W. TAFT


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