C O M M U N I C A T I O N S
to 1 as compared to the heavier homologues. In contrast, however,
we found a higher reactivity of the silicon propellane.
The first experimental evidence came from observations regarding
the moisture sensitivity of 1. Note that Sn5Dep6 (Dep ) 2,6-Et2C6H3)14
and Ge5Mes617 are stable toward degassed water, without any sign of
decomposition and/or reaction. Hydrocarbon solutions of 1, however,
rapidly decolorize when exposed to traces of water. In order to address
this as well as the general reactivity of 1 a little further, we performed
some preliminary NMR tube scale reactions using selected reagents.
It appears that 1 shows both closed-shell and radical-type reactivity.
Several reagents, such as H2O, PhSH, PhOH, and Me3SnH (not
Me3SiH), can readily be added across the bridge, furnishing the
corresponding bicyclo[1.1.1]pentasilane derivatives (see Supporting
Information). Evidence for biradicaloid reactivity of 1 came from
studies using typical reagents for radical-type reactivity, such as
Me3SnH or 9,10-dihydroanthracene. The latter gave the dihydrogen
adduct H21 in low yield after prolonged reaction times.
Figure 2. (a) Experimental UV-vis spectrum of 1 in THF and most relevant
TD-DFT calculated UV-vis transitions of A2 and E symmetry (b) DFT
calculated frontier orbitals of Si5Dmp6 (1q): HOMO-1 (a1, -5.86 eV); HOMO
(e, -5.64 eV); and LUMO (a2, -1.77 eV).
in 1 a little further, both experimentally by Raman spectroscopy and
theoretically by time-dependent (TD)-DFT calculations on Si5Dmp6
(1q, Dmp ) 2,6-Me2C6H3, see Supporting Information). However, the
aim to extract the contribution of the restoring Sib · · ·Sib bond forces
from the totally symmetric Raman bands cannot be achieved for 1
with the desired accuracy, because too many internal coordinates are
involved in each of the totally symmetric normal modes observed at
ν ) 479, 370, and 340 cm-1 (νcalcd ) 455, 349, and 312 cm-1). In
order to obtain at least an estimation of the Sib · · ·Sib bond strength in
1, we calculated the reaction energy for the process 1q + H2 f H21q.
Accordingly, the addition of H2 to the bridgehead Si atoms is
exothermic by ∆H°(0 K) ) -90 kJ mol-1. By using D(H2) ) 436 kJ
mol-1 and assuming a Si-H bond strength of ∼350 kJ mol-1 for silyl-
substituted silanes,19 the Sib · · ·Sib bond strength can be estimated to
amount to ∼174 kJ mol-1. Based on this approximation and as
expected, the Sib · · ·Sib interaction is considerably weaker than in
normal disilanes (ca. 306-332 kJ mol-1).19
All these promising results clearly indicate distinctive peculiarities
of the stretched bond between the bridgehead atoms in heavy
propellanes in general, and in particular in 1. Once designated as
synthetic challenge and targeted by theory over 2 decades ago,
pentasila[1.1.1]propellane is indeed revealed to be an intriguing species
from the perspectives of both bonding and reactivity.
Acknowledgment. We thank the Fonds der Chemischen Industrie,
the German Science Foundation (CFN, Project No. C3.3), and the
Ministry of Science, Research and the Arts of Baden-Wu¨rttemberg
(Az: 7713.14-300).
Supporting Information Available: Details of experimental proce-
dures, preliminary reactivity studies, analytical data, X-ray structure
determination, and quantum chemical calculations (PDF, CIF). This
Alongside these remarkable bonding features, we determined some
interesting electronic properties for 1. The electronic transitions
observed in the experimental UV-vis spectrum of 1 in THF fit
perfectly to the TD-DFT calculated singlet excitations for the model
compound 1q (Figure 2).17 The calculated vertical singlet excitation
wavelength of 325.7 nm (1A2, HOMO-1 (a1) f LUMO (a2)) directly
corresponds to the experimentally observed absorption at λ ) 325 nm,
whereas λmax ) 396 nm belongs to electronic transitions between the
cluster-bonding HOMO (e) and the LUMO (a2) (Figure 2). The
excitation to the first excited triplet state (3A2) was calculated to
correspond to a wavelength of 546.8 nm.17 Usually, these transitions
are not visible in the UV-vis spectrum. The experimental spectrum
of 1, however, shows a broad absorption of very low intensity at λ )
546 nm (Figure 2). Its wavelength corresponds to an excitation energy
of 219 kJ mol-1, that is, about 25 and 10 kJ mol-1 below the respective
excitation energies of its Ge and Sn analogues.17 This is remarkable,
because the first singlet A2 excitation energy of 1q is larger than those
of its analogues. Whereas the increase in the HOMO-1 f LUMO
gaps along the series Sn f Ge f Si is consistent with the computed
singlet excitation energies, the close proximity (reflected by the rather
localized excited ground state difference densities of the 1A2 and 3A2
states, see Supporting Information) of the orbitals involved in 1q leads
to a larger exchange interaction 〈a1a2|a2a1〉 and extra stabilization of
the 3A2 state compared to the Ge and Sn analogues.
The relatively high LUMO energy of 1q (-1.77 eV; cf. -2.10 eV
for Ge5Dmp6 and -2.48 eV for Sn5Dmp5) was experimentally
confirmed by electrochemical studies using cyclic voltammetry under
strictly anaerobic and dry conditions. By analogy to the heavy Ge17
and Sn propellanes,14 1 is quasi-reversibly reduced to the radical anion
[Si5Mes6]•- and dianion [Si5R6]2- at potentials of E°1/2 ) -2.88 and
-3.12 V, respectively. Compared to the heavier homologues, however,
both half-wave potentials are more cathodically shifted, which is in
accord with an energetically destabilized LUMO. On the basis of these
findings, one would a priori expect a less facile addition of nucleophiles
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