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J. Haseltine, J. W. Runyon / Tetrahedron Letters 51 (2010) 3280–3283
The relative power of such groups depends on their specific elec-
tronic character. If the amide group increases ester reactivity by
acting as an electron-withdrawing group or an electron sink, two
different amides need not be alike in this respect. Different N-acyl
R groups, by sponsoring differences in mean and dynamic amide
geometry, orbital structure, and charge distribution, may afford
differences in electron-withdrawing power and charge
accommodation.
Modeling of the syn conformation in series 1 was done to pre-
dict the impact of R on amide geometry. Some details are shown
in Table 3. As the size of R increases, the R–C–N angle (opposite
the carbonyl oxygen) and the adjacent C–N–C angle are each pre-
dicted to widen. The O@C and C–N bonds of the O@C–N substruc-
ture are each predicted to lengthen slightly.
That the R group does affect amide electronic character is indi-
cated empirically by the amide carbonyl stretching frequencies,
listed in Table 2. The value of mC@O drops significantly from the
smallest to the largest R group within each series. However, the
value of mC@O is almost constant when R = Me, Et, and i-Pr within
each series, so R is probably not affecting C@O stretching by its
Figure 3. Comparison of hybrid states for the amide carbonyl carbon as a function
of R–C–N angle. Only sigma-bonding orbitals of the carbonyl carbon are shown.
gen), thereby favoring an incremental shift of the bond’s electron
density slightly closer to carbon. The carbon might therefore gain
‘extra’ shielding by 13C NMR, appearing further upfield than ex-
pected (as seen for 1e, 2e, and 3e). Each loss in the volume of the
major lobe would also remove density from the C/O internuclear
space, thereby tending to weaken the C@O sigma bond and possi-
bly lowering mC@O as we observe.
Are the data consistent with the hypothesis that differences in
amide electronic character affect ester reactivity? Certainly the
largest decreases in rate constant correspond to the largest de-
creases in mC@O in each series. The hypothesis seems reasonable
for now if we suppose that k and mC@O might each be affected by
multiple factors.
specific mass or by a through-bond effect. The jumps in mC@O corre-
spond to the expected increases in crowding between the R group
and nitrogen’s other substituents. In series 1, for example, while
the size of the R group increases from 1a (R = H) to 1b (R = CH3),
the value of mC@O decreases by about 20 cmꢀ1. From 1b to 1c and
1d, the size of R increases again, but the R groups in 1c and 1d
can be rotated to avoid additional crowding relative to 1b. This
may explain why mC@O varies little over this sub-series. From 1d
(R = i-Pr) to 1e (R = t-Bu), however, an increase in crowding cannot
be avoided through facile bond rotations, and mC@O drops again by
about 20 cmꢀ1. Low values of mC@O are not unusual for crowded
amides and ketones.11–13
The 13C NMR chemical shifts of the amide carbonyl also indicate
an interesting impact by the R group (Table 2). For each series of
compounds, the signal is near 160 ppm when R = H. When
R = Me, it is in the range of 169–172 ppm. When R = Et, it is 3–
4 ppm further downfield, and when R = i-Pr, it is 3–4 ppm still fur-
ther downfield. When R = t-Bu, however, the C@O signal appears at
a frequency similar to that seen when R = i-Pr. A linear trend of
C@O signals toward lower field with increasing alkyl substitution
at the alpha carbon is known for several functional groups.14,15
The chemical shifts of 1e, 2e, and 3e represent deviations from this
trend.
Such deviations have been reported previously for crowded ke-
tones.13,16 They make sense in terms of the expected impact of
crowding on the C@O carbon hybridization. Consider that if the
R–C–N angle of the amide group widens for any reason, carbon’s
atomic orbital in the sigma bond to oxygen would gain in p charac-
ter. This is shown in simple form in Figure 3, comparing three hy-
brid states for the C@O carbon based on benchmark R–C–N angles
of 109°, 120°, and 180°. Only carbon’s sigma-bonding orbitals are
shown. From left to right in this series, carbon uses an sp, sp2, or
p orbital, respectively, to make its sigma bond to oxygen. As the
R–C–N angle widens, each increase in p character increases the rel-
ative volume of the orbital’s minor lobe (pointed away from oxy-
3. Conclusion
The nature of the amide group in N-acyl amino acid esters influ-
ences the acyl transfer reactivity of the ester group. The rate con-
stant varies positively with the infrared stretching frequency of
the amide carbonyl and negatively with the size of the N-acyl
group. A high importance of direct crowding between the N-acyl
and ester groups is not generally indicated by the present data.
Conformation within the amide group is judged to be at least
somewhat important. Crowding within the amide group is proba-
bly most responsible for variation in the amide’s electronic charac-
ter, evident by IR and NMR, which may in turn affect ester
reactivity. Further tests of these ideas with dipeptide and tripep-
tide esters are in progress.
Acknowledgments
We are grateful to the College of Science and Mathematics of
Kennesaw State University for support of this work. We are also
grateful to Mr. Alex M. Morrison and Prof. Kevin P. Gwaltney of
our Department for performing NOE and low-temperature NMR
experiments.
References and notes
Table 3
1. Fan, Y.-H.; Grégoire, C.-A.; Haseltine, J. Bioorg. Med. Chem. 2004, 12, 3097.
2. Amide-esters 1a–e, 2a–e, and 3a–e were prepared by N-acylation of proline
ethyl esterꢁHCl,3 sarcosine ethyl esterꢁHCl (Aldrich), and N-(t-butyl)glycine
ethyl ester,4 respectively. Formylations were performed in ethyl formate using
excess triethylamine and/or heat and pressure. Lactam-ester 4 was prepared by
alkylating the sodium salt of 2-pyrrolidinone (NaH/DMF) with ethyl
bromoacetate. Lactam-ester 5 was prepared from its corresponding methyl
ester by treatment with K2CO3/ethanol.5
Calculated bond angles and bond lengths at the amide group in compounds 1a–e, syn
conformation (Hartree–Fock level, 6-31G* basis set)
Ester
R–C–N
C–N–C
O@C (Å)
C–N (Å)
1a
1b
1c
1d
1e
113.49°
117.13°
117.01°
118.59°
122.31°
125.33°
126.88°
127.06°
127.69°
130.75°
1.197
1.203
1.203
1.205
1.206
1.343
1.355
1.356
1.355
1.362
3. Proline ethyl esterꢁHCl was prepared by applying the method of Garbers, C. F.;
Schmid, H.; Karrer, P. Helv. Chim. Acta 1955, 38, 1490.
4. Gribble, G. W.; Hirth, B. H. J. Heterocycl. Chem. 1996, 33, 719.