Patrick
Hummel
,
Jay R.
Winkler
and
Harry B.
Gray
*
California Institute of Technology, 1200 E. California Blvd., Mail Code 139-74, Pasadena, CA 91125, USA. E-mail: hbgray@caltech.edu
First published on 4th November 2005
We have employed computational methods based on density functional theory to elucidate the effects of equatorial ligands on the electronic structures of trans-dioxometal complexes. In complexes with ammine (σ-only) equatorial donors, the 1A1 g(b2 g)2 → 1Eg(b2 g)1(eg)1 excitation energy increases with metal oxidation state: Mo(IV) < Tc(V) < Ru(VI) and W(IV) < Re(V) < Os(VI). Increasing transition energies are attributed to enhanced oxometal π-donor interactions in the higher valent central metals. But in complexes with cyanide equatorial donors, the 1A1 g(b2 g)2 → 1Eg(b2 g)1(eg)1 energy remains roughly independent of metal oxidation state, likely owing to the compensating increased π-donation from the π(CN) orbitals to the metal dxy orbitals as the oxidation state of the metal increases.
Fig. 1 The structure of the [MO2L4]z complexes in question. |
We now report a systematic investigation of the electronic structures of d2-trans-dioxometal complexes. In particular, we use density functional theory (DFT) and time-dependent density functional theory (TDDFT) to analyze the effects of equatorial ligand interactions on the Δ = E[eg(xz, yz)] − E[b2 g(xy)] energy gap as a function of metal oxidation state. For [MO2(NH3)4]z, we note a general increase in Δ with increase in metal oxidation state: Mo(IV) < Tc(V) < Ru(VI) and W(IV) < Re(V) < Os(VI). For [MO2(CN)4]z the values of Δ remain roughly independent of the oxidation state of the central metal.
Expt | B3LYP | B-LYP | BP86 | PBE | |
---|---|---|---|---|---|
[MoO2(NH3)4] | 1.833 | 1.852 | 1.842 | 1.843 | |
[TcO2(NH3)4]+ | 1.747 | 1.763 | 1.787 | 1.777 | 1.777 |
[RuO2(NH3)4]2+ | 1.724 | 1.752 | 1.741 | 1.741 | |
[WO2(NH3)4] | 1.855 | 1.873 | 1.863 | 1.862 | |
[ReO2(NH3)4]+ | 1.765 | 1.790 | 1.812 | 1.803 | 1.803 |
[OsO2(NH3)4]2+ | 1.74 | 1.752 | 1.777 | 1.768 | 1.768 |
[MoO2(CN)4]4− | 1.834 | 1.844 | 1.867 | 1.857 | 1.856 |
[TcO2(CN)4]3− | 1.779 | 1.805 | 1.795 | 1.795 | |
[RuO2(CN)4]2− | 1.740 | 1.771 | 1.760 | 1.760 | |
[WO2(CN)4]4− | 1.842 | 1.866 | 1.886 | 1.875 | 1.875 |
[ReO2(CN)4]3− | 1.781 | 1.806 | 1.830 | 1.819 | 1.818 |
[OsO2(CN)4]2− | 1.75 | 1.767 | 1.796 | 1.786 | 1.786 |
Expt | B3LYP | B-LYP | BP86 | PBE | |
---|---|---|---|---|---|
[MoO2(NH3)4] | 2.303 | 2.322 | 2.287 | 2.283 | |
[TcO2(NH3)4]+ | 2.158 | 2.214 | 2.236 | 2.205 | 2.201 |
[RuO2(NH3)4]2+ | 2.153 | 2.182 | 2.155 | 2.152 | |
[WO2(NH3)4] | 2.304 | 2.320 | 2.288 | 2.284 | |
[ReO2(NH3)4]+ | 2.162 | 2.222 | 2.224 | 2.216 | 2.213 |
[OsO2(NH3)4]2+ | 2.11 | 2.167 | 2.193 | 2.169 | 2.164 |
[MoO2(CN)4]4− | 2.220 | 2.229 | 2.228 | 2.201 | 2.198 |
[TcO2(CN)4]3− | 2.170 | 2.176 | 2.148 | 2.145 | |
[RuO2(CN)4]2− | 2.124 | 2.145 | 2.113 | 2.110 | |
[WO2(CN)4]4− | 2.177 | 2.224 | 2.226 | 2.202 | 2.198 |
[ReO2(CN)4]3− | 2.124 | 2.178 | 2.181 | 2.160 | 2.157 |
[OsO2(CN)4]2− | 2.139 | 2.151 | 2.128 | 2.125 |
Expt | B3LYP | B-LYP | BP86 | PBE | |
---|---|---|---|---|---|
[MoO2(CN)4]4− | 1.169 | 1.181 | 1.183 | 1.183 | |
[TcO2(CN)4]3− | 1.162 | 1.174 | 1.175 | 1.175 | |
[RuO2(CN)4]2− | 1.157 | 1.169 | 1.169 | 1.169 | |
[WO2(CN)4]4− | 1.169 | 1.182 | 1.183 | 1.183 | |
[ReO2(CN)4]3− | 1.156 | 1.162 | 1.174 | 1.175 | 1.175 |
[OsO2(CN)4]2− | 1.156 | 1.168 | 1.169 | 1.169 |
B3LYP | B-LYP | BP86 | PBE | |
---|---|---|---|---|
[MoO2(NH3)4] | −3.66/0.50 | −2.30/−0.31 | −2.41/−0.43 | −2.30/−0.33 |
[TcO2(NH3)4]+ | −6.79/−2.20 | −5.16/−2.88 | −5.26/−2.99 | −5.13/−2.88 |
[RuO2(NH3)4]2+ | −10.11/−5.33 | −8.38/5.88 | −8.52/−6.00 | −8.40/−5.89 |
[WO2(NH3)4] | −3.21/0.89 | −2.03/0.20 | −2.17/0.06 | −2.05/0.17 |
[ReO2(NH3)4]+ | −6.25/−1.59 | −4.82/−2.31 | −4.96/−2.44 | −4.83/−2.32 |
[OsO2(NH3)4]2+ | −9.65/−4.66 | −8.03/−5.26 | −8.18/−5.40 | −8.06/−5.29 |
[MoO2(CN)4]4− | −3.33/0.88 | −2.34/0.01 | −2.63/−0.22 | −2.50/−0.08 |
[TcO2(CN)4]3− | −5.67/−1.30 | −4.34/−2.04 | −4.60/−2.24 | −4.46/−2.10 |
[RuO2(CN)4]2− | −7.96/−4.02 | −6.51/−4.60 | −6.74/−4.78 | −6.60/−4.64 |
[WO2(CN)4]4− | −3.11/1.14 | −2.24/0.30 | −2.55/0.05 | −2.42/0.18 |
[ReO2(CN)4]3− | −5.33/−0.87 | −4.18/−1.63 | −4.45/−1.83 | −4.31/−1.69 |
[OsO2(CN)4]2− | −7.64/−3.45 | −6.29/−4.07 | −6.53/−4.27 | −6.40/−4.13 |
Expt | B3LYP | B-LYP | BP86 | PBE | |
---|---|---|---|---|---|
[MoO2(NH3)4] | 2.33 | 2.27 | 2.28 | 2.26 | |
[TcO2(NH3)4]+ | 2.53 | 2.71 | 2.56 | 2.58 | 2.57 |
[RuO2(NH3)4]2+ | 2.73 | 3.00 | 2.78 | 2.82 | 2.81 |
[WO2(NH3)4] | 2.55 | 2.47 | 2.49 | 2.48 | |
[ReO2(NH3)4]+ | 2.83 | 2.93 | 2.79 | 2.81 | 2.80 |
[OsO2(NH3)4]2+ | 3.25 | 3.02 | 3.06 | 3.06 | |
[MoO2(CN)4]4− | 2.64 | 2.51 | 2.59 | 2.59 | |
[TcO2(CN)4]3− | 2.71 | 2.51 | 2.58 | 2.58 | |
[RuO2(CN)4]2− | 2.50 | 2.06 | 2.12 | 2.12 | |
[WO2(CN)4]4− | 2.85 | 2.67 | 2.73 | 2.74 | |
[ReO2(CN)4]3− | 3.17 | 2.96 | 2.72 | 2.80 | 2.80 |
[OsO2(CN)4]2− | 2.98 | 2.80 | 2.36 | 2.41 | 2.42 |
As the oxidation state of the central metal atom increases, the eg(xz, yz) orbitals become more π-antibonding, owing to greater oxometal π-donor interactions. It follows that we expect a corresponding increase in the energies of the 1A1 g(b2 g)2 → 1Eg(b2 g)1(eg)1 excitations. This increase is observed for [MO2(NH3)4]z complexes, but not for [MO2(CN)4]z complexes, where the excitation energies remain roughly constant. Clearly for [MO2(CN)4]z there is some other effect that causes significant changes in the relative energies of the b2 g(xy) and eg(xz, yz) orbitals.
To probe this effect, we analyze average changes in orbital energies per unit increase in the charge of the central metal. The average change in E[eg(xz, yz)] is −2.78 eV for [MO2(NH3)4]z, and −2.26 eV for [MO2(CN)4]z. For E[b2 g(xy)], the average change is −2.89 eV for [MO2(NH3)4]z and −2.10 eV for [MO2(CN)4]z. Consistent with the trends in energies of the 1A1 g(b2 g)2 → 1Eg(b2 g)1(eg)1 excitation, the average change in E[eg(xz, yz)] is greater (less negative) than the average change in E[b2 g(xy)] for [MO2(NH3)4]z, but the average change in E[b2 g(xy)] is greater than the average change in E[eg(xz, yz)] for [MO2(CN)4]z. The energy changes cited here do not vary strongly with exchange–correlation functional or central metal.
The 1Eg(b2 g)1(eg)1 excited state of a [MO2(CN)4]z complex is stabilized by backbonding from the metal (dxz, dyz) orbitals to the cyanide π* orbitals. Thus one possible explanation for the differing trends in [MO2(NH3)4]z and [MO2(CN)4]z is that greater bonding overlap between the (dxz, dyz) and π*(CN) orbitals is achieved as metal oxidation state increases. However, our calculations are not in accord with this explanation. For [MO2(NH3)4]z, the average change in E[eg(xz, yz)] per unit increase in the charge of the central metal is 0.52 eV less than the average change for [MO2(CN)4]z, indicating a trend opposite of that postulated here. Also, the calculated electron density pictures of the LUMO orbitals (performed with MOLDEN39) indicate that there is slightly less bonding overlap between (dxz, dyz) and π*(CN) for the complexes with higher charge (see, e.g., Fig. 2).
Fig. 2 Electron density pictures of the eg(xz, yz) orbitals calculated with B-LYP for MO2(CN)4 with M = W, Re, and Os. |
Another attractive possibility is that increasing the charge of the central metal atom decreases the amount of dxy → π*(CN) backbonding, thereby destabilizing the b2 g(xy) orbital, and in turn decreasing Δ. While variations in backbonding may affect the orbital splitting, they do not account for the observed trends. The metal oxidation states in these complexes range from IV–VI, and there is very little backbonding in complexes with such high oxidation states. Also, there is little variation in the C–N bond distances in these complexes, suggesting only minor variations in π*(CN) populations. For [MO2(NH3)4]z, the average change in E[b2 g(xy)] per unit increase in the charge of the central metal atom is 0.79 eV less than the average change for [MO2(CN)4]z. Such a small change in backbonding cannot be the primary cause for the large difference noted here.
We are left with one last explanation: For σ-only equatorial ligands such as NH3, the b2 g(xy) orbital is virtually nonbonding. But for equatorial ligands such as CN−, there will be an antibonding interaction between the dxy orbital and cyanide π-orbitals. As the metal oxidation state increases, there will be more π-donation from the filled π(CN) orbitals to the metal dxy orbital, thereby destabilizing b2 g(xy). Since the extent of π-donation increases significantly per unit increase in metal oxidation state, this trend could easily account for the relative destabilization of b2 g(xy) in [MO2(CN)4]z compared to [MO2(NH3)4]z. We conclude that variations in cyanide donor interactions with metal oxidation state account for the observed trends in 1A1 g(b2 g)2 → 1Eg(b2 g)1(eg)1 energies.
This journal is © The Royal Society of Chemistry 2006 |