Journal of the American Chemical Society
Article
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When these reactions are conducted with para-H2, PHIP is
evident in the hydride signals of 2, 3 and 5. This confirms the
utility of PHIP as a powerful method for examining the
reactivity of polyhydride complexes of this type. Furthermore,
the experimental and computation results also suggest that
nonclassical dihydride complexes do not play a significant role
in the oxidative addition process. In contrast, H2 addition to
W(CO)3(PCy3)2 was shown not to produce detectable PHIP in
the W(H)2(CO)3(PCy3)2 product. In this latter case, a role for
a nonclassical dihydrogen complex in the addition process has
been well established.3−5 The postulation here that 3 and 4
exist as classical W(IV) and W(VI) species was further
supported by the long T1(min) values of the hydride ligands
(>0.3 s), the observation of appropriate JHW couplings and the
detection of 183W signals for 2, 3 and 4. The 183W resonance for
W(VI) 4 appears at the high field value of δ 4000, in
accordance with its high oxidation state. This compares with
values of δ 3363 for 2 and δ 2913 for 3 both of which
complexes exists as W(IV) species. Attempts to locate the
corresponding signal in 5 failed, presumably as a consequence
of its dynamic behavior leading to signal broadening.
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It has previously been reported that UV irradiation of
W(H)4(dppe-κ2P)2 under N2 leads to low yields of ammonia59
and alkene hydrogenation. It has also been reported that H2
loss corresponds to the main photochemical process in such
systems.50,52 Here we have demonstrated that W(H)6(dppe-
κ2P)(dppe-κ1P) (4) is formed under UV irradiation which
suggests that 16-electron W(H)4(dppe-κ2P)(dppe-κ1P) and not
W(H)2(dppe-κ2P)2 is responsible for these conversions.
Thus, the results presented here demonstrate that CH bond
activation, phosphine dechelation, and the oxidative addition of
OH bonds are all important in the chemistry of W(N2)2(dppe-
κ2P)2 (1).
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ASSOCIATED CONTENT
* Supporting Information
Characterization of 3 and 5, and the DFT derived energetics
and coordinates for all the species discussed. This material is
■
S
AUTHOR INFORMATION
Corresponding Author
Notes
(32) Lyon, C. E.; Suh, E. S.; Dobson, C. M.; Hore, P. J. J. Am. Chem.
Soc. 2002, 124, 13018.
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(33) Blazina, D.; Dunne, J. P.; Aiken, S.; Duckett, S. B.; Elkington, C.;
McGrady, J. E.; Poli, R.; Walton, S. J.; Anwar, M. S.; Jones, J. A.;
Carteret, H. A. Dalton Trans. 2006, 2072.
(34) Dunne, J. P.; Blazina, D.; Aiken, S.; Carteret, H. A.; Duckett, S.
B.; Jones, J. A.; Poli, R.; Whitwood, A. C. Dalton Trans. 2004, 3616.
(35) Anwar, M. S.; Blazina, D.; Carteret, H. A.; Duckett, S. B.;
Halstead, T. K.; Jones, J. A.; Kozak, C. M.; Taylor, R. J. K. Phys. Rev.
Lett. 2004, 93, No. 040501.
The authors declare no competing financial interest.
ACKNOWLEDGMENTS
■
We are grateful for financial support from the BBSRC (P.J.C.),
AstraZeneca and the Spanish MEC Consolider Ingenio 2010-
ORFEO-CSD2007-00006 (B.E.) research programme. We also
thank Professor Robin Perutz for helpful discussions.
(36) Duckett, S. B.; Mewis, R. E. Acc. Chem. Res. 2012, 45, 1247.
(37) Benn, R.; Brenneke, H.; Heck, J.; Rufinska, A. Inorg. Chem.
1987, 26, 2826.
(38) Carlton, L.; Emdin, A.; Lemmerer, A.; Fernandes, M. A. Magn.
Reson. Chem. 2008, 46, S56.
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