a hyperconjugative interaction between the sp2 σ-radical and
the back lobe of the C-Sn σ-bond, recent ab initio
calculations on comparable â-silyl substituted vinyl radicals
suggest that â-silyl hyperconjugative stabilization is negli-
gible in such systems.13 By analogy, therefore, it is probably
correct to assume that hyperconjugative stabilization of 24
will also be minimal. It is now proposed that the exceedingly
bulky Ph3SnH preferentially donates its H-atom to the vinyl
radical conformer 24 rather than 23, since this will lead to
a far less sterically crowded transition state than the
alternative; this would, of course, preferentially deliver
vinylstannane 25.
Figure 2. Vinylstannanes 32-36.
It is further proposed that the majority of 26 that is formed
will have a very strong tendency to be converted into 25 by
the reversible addition of Ph3Sn radicals to the â-olefinic
carbon of 26.14 In this regard, molecular models of the
transition state for â-addition suggest that it will be far less
sterically crowded than that for R-addition; the â-addition
pathway would also produce a much less sterically encum-
bered tertiary radical 27 that would be doubly stabilized by
the R- and â-stannyl groups. By way of contrast, stannyl
radical addition to the R-carbon of 26 would lead to a much
more severely crowded transition state, and afford a less
stable (but, nevertheless, hyperconjugatively stabilized)
secondary carbon radical. Once generated, radical 27 has the
choice of either dissociating back into 26 or undergoing
immediate C-C bond rotation to place the two bulky Ph3-
Sn substituents as far apart as possible, as in radical rotamer
28; further bond rotation in the direction of rotamer 29 would
then allow the â-C-Sn bond to hyperconjugatively stabilize
the adjacent radical center. Elimination at this stage would
produce 25 and place the R group cis to the R-Ph3Sn group.
In our view, this mechanistic picture most satisfactorily
explains all of the observations made so far on this
remarkable reaction.
The angles subtended at the metal fell within the range
101.75° to 125.27°, with both extremes being found within
the crystal structure of 32. The nonbonded Sn‚‚‚O distances
generally fell within a relatively narrow range (3.09-3.44
Å). The only two exceptions were the structures for 33 and
34, where one molecule in the asymmetric unit had a
“normal” short contact, while the second independent
molecule adopted a different conformation with a much
greater Sn‚‚‚O separation (4.41 Å). Although most of these
distances are less than the sum of the van der Waals radii of
tin and oxygen (3.57 Å) they are much greater than a typical
Sn-O covalent bond distance (2.20-2.25 Å). Since there
are no significant distortions to the tetrahedral geometry of
Sn, we have concluded that, in the solid at least, there is no
evidence for valence expansion at the metal nor for a
consequential selective weakening of any of the aryl C-Sn
bonds within compounds 32-36. This behavior contrasts
with (Z)-disubstituted â-triarylstannylated allyl alcohols
where the central Sn atom is always distorted trigonal
bipyramidal with the apical aryl C-Sn bonds being signifi-
cantly weakened and more readily cleaved by I2. The lack
of internal Sn‚‚‚O coordination in allylically oxygenated
R-triphenylstannylalkenes means that they behave like
normal vinyltrialkylstannanes with respect to the metal-
halogen exchange reaction; in other words, they are converted
to vinyl iodides with retention of olefin geometry.
At this juncture, we would now like to change direction
and comment on the reason why allylically oxygenated R-
triphenylstannylalkenes react successfully with I2, while
allylically oxygenated (Z)-â-triphenylstannylalkenes do not.
To gain some insights into this behavior, we examined the
X-ray crystal structures of 32-36 (see the Supporting
Information). The five studies gave rise to 10 independent
determinations of geometry at the four-coordinate Sn atoms.
In closing, we believe that the mechanistic and structural
insights that we have provided will aid chemists wishing to
apply our methodology soon.
Acknowledgment. We thank the EPSRC (Project Grants
GR/N20959/01 and GR/S27733/01), the University of Lon-
don Central Research Fund, Novartis (Basel/USA), Merck
(Harlow), and Pfizer (Sandwich) for their generous financial
support and Profs. B.P. Roberts and A.G. Davies, FRS, of
UCL for helpful discussions.
(11) The significantly enhanced reactivity of trigonal bipyramidal,
heteroatom-complexed, tin hydrides towards Sn-H homolysis has already
been documented in the literature for the organostannatrane hydride, Me2N-
(CH2)3(Me)2SnH. The latter stannane does not even require any external
initiator to be added for it to mediate its free-radical reduction of
3-iodobenzoic acid to benzoic acid in H2O at rt. For more details, see: Han,
X.; Hartmann, G. A.; Brazzale, A.; Gaston, R. D. Tetrahedron Lett. 2001,
42, 5837.
(12) In light of this, one would expect that complexation of Ph3SnH with
the propargylic O-atom of 20 would likewise cause a significant elongation
and weakening of the Sn-H bond in the resulting complex 21; this would
clearly facilitate H-atom abstraction from its stannyl component as is being
proposed. It is also very reasonable to assume that O-coordinated triphenyltin
radicals such as 22 will have extra longevity than uncoordinated Ph3Sn
radicals due to magnified steric hindrance around the radical center; again,
this should favor the R-mode of addition.
Supporting Information Available: Full experimental
procedures and detailed spectral data, 500 MHz 1H and 125
MHz 13C spectra, and HRMS spectra for all new compounds
are provided, along with X-ray crystallographic data and
product ratio determinations in the hydrostannation reactions.
This material is available free of charge via the Internet at
(13) Lalitha, S.; Chandrasekhar, J. Proc. Indian Acad. Sci. (Chem. Sci.)
1994, 106, 259.
(14) This isomerization will be especially favorable when R1 and R2 are
both alkyl groups due to significant A1, strain being present within 26.
OL051937D
3
5380
Org. Lett., Vol. 7, No. 24, 2005