ChemComm
Communication
Table 1 Relative stability of the C4H7+ species adsorbed on Chabazite (values in
Based on the relative stability it is possible to explain the
dominance of certain C4H7+ isomers in the MD trajectories. The
bicyclobutonium cation is the most stable C4H7 ion, which
kJ molꢀ1
)
+
Species
DU (kJ molꢀ1
)
justifies its predominance in the trajectories calculated at 50 K.
In addition, the small difference in stability between the
bicyclobutonium and cyclopropylcarbinyl cations explains the
fast interconversion between them in the trajectories calculated
at room temperature and above. This result indicates that
rearrangement of carbocations on zeolites is fast near room
Allylcarbinyl cation
75.3
69.1
66.6
0.0
Cyclopropylcarbinyl cation
Bicyclobutonium cation
Allylcarbinyl alkoxide
the probability density of the C2–C4 distance along the MD temperature and occurs within the picosecond time scale. The
trajectories. As the interconversion takes place, with formation allylcarbinyl cation is rarely observed in the trajectories calcu-
of the cyclopropylcarbinyl cation, this distance may stretch up lated at 300 K, but is more frequently observed in the trajec-
to 2.8 Å. At 50 K, due to the low thermal energy available, the tories calculated at 500 K. These data indicate that less stable
bicyclobutonium ion prevails, as observed in the C2–C4 dis- carbocations can be formed inside the zeolite surface at higher
tance within 1.2 and 1.8 Å. At higher temperatures, there is temperatures, having enough time to be converted into pro-
significant probability of the C2–C4 distance to be within 2.1 ducts, before going to alkoxides. This may explain several
and 2.8 Å, indicative of the interconversion into the cyclopro- hydrocarbon processes on zeolites, such as cracking, which
pylcarbinyl cation.
occur at high temperatures.
In addition to the bicyclobutonium and the cyclopropyl-
carbinyl cations, the allylcarbinyl isomer was also observed in
some of the trajectories calculated at 300 K and in all trajec-
tories calculated at 500 K. This result is consistent with
previous calculations10 that point out the higher energy of the
allylcarbinyl cation relative to the bicyclobutonium and cyclo-
propylcarbinyl isomers. In one of the trajectories calculated at
500 K, the allylcarbinyl cation interacted with the framework
oxygen atom near the aluminium atom to yield the respective
alkoxide, which persisted till the end of the path.
Notes and references
N
N
ꢀ
ꢁ
ꢂ
ꢃ
P
P
1
1
2
† MSDðtÞ ¼ Drj2ðtÞ
¼
Drj2
¼
rjðtÞ ꢀ rjð0Þ
N j¼1
N j¼1
1 A. Corma, Chem. Rev., 1995, 95, 559.
2 (a) J. F. Haw, B. R. Richardson, I. S. Oshiro, N. D. Lazo and
J. A. Speed, J. Am. Chem. Soc., 1989, 111, 2052; (b) J. B. Nicholas,
T. Xu and J. F. Haw, Top. Catal., 1998, 6, 141; (c) J. F. Haw, Phys.
Chem. Chem. Phys., 2002, 4, 5431; (d) C. Tuma and J. Sauer, Angew.
Chem., Int. Ed., 2005, 44, 4769; (e) M. Boronat and A. Corma, Appl.
Catal., A, 2008, 336, 2; ( f ) A. S. S. Sido, J. Barbiche and J. Sommer,
Chem. Commun., 2010, 46, 2913.
3 (a) R. J. Correa and C. J. A. Mota, Phys. Chem. Chem. Phys., 2002,
4, 4268; (b) R. J. Correa and C. J. A. Mota, Appl. Catal., A, 2003,
255, 255; (c) N. Rosenbach Jr., A. P. A. dos Santos, M. Franco and
C. J. A. Mota, Chem. Phys. Lett., 2010, 485, 124.
4 M. Franco, N. Rosenbach, G. B. Ferreira, A. C. O. Guerra,
W. B. Kover, C. C. Turci and C. J. A. Mota, J. Am. Chem. Soc., 2008,
130, 1592–1600.
5 R. H. Mazur, W. N. White, D. A. Semenow, C. C. Lee, M. S. Silver and
J. D. Roberts, J. Am. Chem. Soc., 1959, 81, 4390.
6 (a) G. A. Olah, C. L. Jeuell, D. P. Kelly and R. D. Porter, J. Am. Chem.
Soc., 1972, 94, 146; (b) J. S. Staral, I. Yavari and J. D. Roberts, J. Am.
Chem. Soc., 1978, 100, 8016; (c) G. A. Olah, R. D. Porter, D. P. Kelly
and C. L. Jeuell, J. Am. Chem. Soc., 1972, 94, 146; (d) G. A. Olah and
R. J. Spear, J. Am. Chem. Soc., 1975, 97, 1539; (e) J. S. Staral and
J. D. Roberts, J. Am. Chem. Soc., 1978, 100, 8018.
7 M. Saunders and H. U. Siehl, J. Am. Chem. Soc., 1980, 102, 6868.
8 F. Cacace, B. Chiavarino and M. E. Crestoni, Chem.–Eur. J., 2000, 6,
2024–2030.
9 (a) P. V. Schleyer and G. W. Vandine, J. Am. Chem. Soc., 1966,
88, 2321; (b) B. R. Ree and J. C. Martin, J. Am. Chem. Soc., 1970,
92, 1660; (c) V. Buss, R. Gleiter and P. V. Schleyer, J. Am. Chem. Soc.,
1971, 93, 392; (d) Y. E. Rhodes and V. G. Difate, J. Am. Chem. Soc.,
1972, 94, 7582; (e) M. Saunders, K. E. Laidig, K. B. Wiberg and
P. V. Schleyer, J. Am. Chem. Soc., 1988, 110, 7652.
Geometry optimizations of selected structures along the MD
trajectory calculated at 500 K were performed in order to check
if they correspond to minima on the potential energy surface
(PES). Most of the optimizations systematically yielded the
bicyclobutonium cation as the local minimum, being the most
+
stable C4H7 ion. However, some of the structures corre-
sponded to the cyclopropylcarbinyl and allylcarbinyl cations.
+
Table 1 shows the relative stability of the C4H7 species on
Chabazite calculated from the electron energy differences with-
out considering thermal and vibrational contributions. The
bicyclobutonium cation is more stable than the cyclopropylcar-
binyl isomer by 2.5 kJ molꢀ1 and by 8.7 kJ molꢀ1 in relation to
the allylcarbinyl cation. On the other hand, the allylcarbinyl
alkoxide is the calculated most stable species, lying
66.6 kJ molꢀ1 below the bicyclobutonium cation. Nevertheless,
we were able to observe a trajectory for the formation of the
alkoxide of the carbocation only at 500 K, when the allycarbinyl
cation was formed. This result suggests that, although the
alkoxides are thermodynamically more stable than the carbo-
10 J. Casanova, D. R. Kent, W. A. Goddard and J. D. Roberts, Proc. Natl.
Acad. Sci. U. S. A., 2003, 100, 15–19.
cations, their formation from their ionic counterparts is not 11 (a) S. Raugei and M. L. Klein, J. Phys. Chem. B, 2002, 106, 11596;
(b) S. Raugei, D. Kim and M. L. Klein, Quant. Struct.–Act. Relat., 2002,
21, 149.
12 P. M. Esteves, C. L. Arau´jo, B. A. C. Horta, L. J. Alvarez, C. M. Zicovich-
straightforward. From the calculated trajectories, it is found
that formation of the alkoxide can occur only when the carbo-
´
´
cation is favourably orientated near the framework oxygen
atom. With the increase in temperature and the consequent
mobility of the cation toward the centre of the cavity, the
formation of the alkoxide is less favourable, but when it occurs
it persists for a long period, explaining the spectroscopic
results,15 which normally point out the alkoxides as the long-
living species on the zeolite surface.
Wilson and A. Ramırez-Solıs, J. Phys. Chem. B, 2005, 109, 12946.
13 (a) L. Benco, T. Demuth and F. Hutschka, Comput. Mater. Sci., 2003,
´
27, 87; (b) T. Bucko, L. Benco, J. Hafner and J. G. Angyan, J. Catal.,
2007, 250, 171–183; (c) T. Bucko, L. Benco, J. Hafner and
J. G. Angyan, J. Catal., 2011, 270, 220; (d) L. Benco, T. Bucko and
J. Hafner, J. Catal., 2011, 277, 104.
´
14 G. Kresse and J. Furthmuu¨ller, Phys. Rev. B, 1996, 54, 11169.
15 J. F. Haw, J. B. Nicholas, T. Xu, L. W. Beck and D. B. Ferguson, Acc.
Chem. Res., 1996, 29, 259.
c
4482 Chem. Commun., 2013, 49, 4480--4482
This journal is The Royal Society of Chemistry 2013