Paper
Dalton Transactions
of (PNP)RhO generated from 29 mg of (PNP*)RhH and N2O in is the reason why it is possible to find a temperature where
0.5 mL of d8 THF at −30 °C during 1 h. The solution contain- this path to (PNP)Rh(H)2 is slower than the reaction via H2
1
ing water was monitored by H and 31P NMR and showed no addition to (PNP)RhH(OH).
reaction even after 24 h at −30 °C. An additional 0.001 mL of
H2O was then added by vacuum transfer and no reaction was
seen after 24 h at −30 °C. The H2O 1H NMR peak is seen at
2.7 ppm (it became taller after the second addition of H2O,
Acknowledgements
showing that it had not been frozen to ice) together with para- This work was supported by the National Science Foundation
magnetic (PNP)RhO. Overall observation time for no reaction (NSF-CHE-0544829).
was over 48 hours at −30 °C. Higher temperature observations
are precluded by the background reaction (Scheme 1) of
addition of one methyl C–H bond across the Rh/O bond.
Notes and references
Attempts to establish possible small 1H NMR chemical shift
changes due to equilibrium formation of a hydrogen bonded
pair {(PNP)RhO; H2O} were frustrated by the strong T−1 chemi-
cal shift dependence due to the paramagnetism of (PNP)RhO.
1 K. P. O’Halloran, C. Zhao, N. S. Ando, A. J. Schultz,
T. F. Koetzle, P. M. B. Piccoli, B. Hedman, K. O. Hodgson,
E. Bobyr, M. L. Kirk, S. Knottenbelt, E. C. Depperman,
B. Stein, T. M. Anderson, R. Cao, Y. V. Geletii,
K. I. Hardcastle, D. G. Musaev, W. A. Neiwert, X. Fang,
K. Morokuma, S. Wu, P. Kögerler and C. L. Hill, Inorg.
Chem., 2012, 51, 7025–7031.
2 E. Spaltenstein, R. R. Conry, S. C. Critchlow and
J. M. Mayer, J. Am. Chem. Soc., 1989, 111, 8741–8742.
3 A. Y. Verat, H. Fan, M. Pink, Y. S. Chen and K. G. Caulton,
Chem.–Eur. J., 2008, 14, 7680–7686.
4 Compare this to the isoelectronic triplet (PNP)RuCl.
L. A. Watson, O. V. Ozerov, M. Pink and K. G. Caulton, J.
Am. Chem. Soc., 2003, 125, 8426.
5 A. Y. Verat, M. Pink, H. Fan, J. Tomaszewski and
K. G. Caulton, Organometallics, 2008, 27, 166–168.
6 A. Walstrom, M. Pink, N. P. Tsvetkov, H. Fan, M. Ingleson
and K. G. Caulton, J. Am. Chem. Soc., 2005, 127, 16780–16781.
7 A. Walstrom, L. A. Watson, M. Pink and K. G. Caulton,
Organometallics, 2004, 23, 4814–4816.
Computational details
All calculations were carried out on the full set of atoms
present, using Density Functional Theory with the B3LYP26–28
functional and the 6-31G** basis set with no symmetry restric-
tions, which has been shown to work well for many transition
metal-containing systems.29 All transition metals were rep-
resented using the Los Alamos basis set (LACVP).30,31 Energies
of the optimized structures were reevaluated by additional
single-point calculations on each optimized geometry using
Dunning’s correlation-consistent triple-ζ basis set,32 cc-pVTZ
(-f). Since we calculate all intermediates as singlets here, we
chose to use the B3LYP functional in spite of its overstabiliza-
tion of higher spin states (i.e., the singlet was previously3 cal-
culated to lie 15.3 kcal mol−1 above the triplet using a single
determinant method). The B3LYP choice was also bench-
marked by its calculation of ΔG° > 0 for the addition of H2 to
(PNP)RhO. In any event, our calculations fully establish mech-
anism on the singlet surface. A similar situation was recently
reported33 for S = 3/2 Mo[N(tBu)Ar]3 reacting with nitriles to
finally give doublet products; on the quartet surface, binding
the nitrile was repulsive, and the mechanism was mapped out
on the doublet surface.
8 E. Poverenov, I. Efremenko, A. I. Frenkel, Y. Ben-David,
L. J. W. Shimon, G. Leitus, L. Konstantinovski,
J. M. L. Martin and D. Milstein, Nature, 2008, 455, 1093–
1096.
9 I. Efremenko, E. Poverenov, J. M. L. Martin and D. Milstein,
J. Am. Chem. Soc., 2010, 132, 14886–14900.
Efforts to find a TS for direct addition of H2 to the terminal 10 A. Vigalok, Y. Ben-David and D. Milstein, Organometallics,
oxo of (PNP)RhO: step-scans, beginning from (PNP)Rh(H2O) 1996, 15, 1839–1844.
but with the H/H distance fixed between 1.54 to 0.9 Å never 11 See ESI.‡
reached a maximum, and the energy rises fast since the O/H 12 L. A. Watson and O. Eisenstein, J. Chem. Educ., 2002, 79,
distances remain within bonding range, hence exhibit repul-
sion. A step-scan search with two fixed OH distances in the 13 M. J. Ingleson, M. Pink and K. G. Caulton, J. Am. Chem.
range 0.74 to 1.37 Å showed no mutual approach of the two H, Soc., 2006, 128, 4248–4249.
but instead showed one H bridging O and Rh, with the other 14 C. E. Housmekerides, D. L. Ramage, C. M. Kretz,
1269–1277.
H terminal on O. A search for a TS1–4 for [2 + 2] addition of the
H–H bond directly across the Rh/O bond collapsed towards 3,
J. T. Shontz, R. S. Pilato, G. L. Geoffroy, A. L. Rheingold and
B. S. Haggerty, Inorg. Chem., 1992, 31, 4453–4468.
hence showed no new approach trajectory distinct from 15 C. E. Housmekerides, R. S. Pilato, G. L. Geoffroy and
passing through (PNP)Rh(H2)O. The calculations show that
(PNP*)Rh(OH) is more stable than both singlet and triplet
A. L. Rheingold, J. Chem. Soc., Chem. Commun., 1991, 563–
566.
(PNP)RhO, as observed experimentally, and providing another 16 M. R. Churchill, G. Davies, M. A. El-Sayed and
benchmark to the utility of the B3LYP functional. Finally (see J. P. Hutchinson, Inorg. Chem., 1982, 21, 1002–1007.
ESI‡), the energy of the H2 adduct of (PNP*)Rh(OH) lies so 17 J. Fujita, A. E. Martell and K. Nakamoto, J. Chem. Phys.,
high (+20.3 kcal mol−1 relative to (PNP)RhO + free H2) that this
1962, 36, 339–345.
6754 | Dalton Trans., 2013, 42, 6745–6755
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