Hao
Liang
a,
Tzu-Hao
Chiu
b,
Samia
Kahlal
a,
Jian-Hong
Liao
b,
C. W.
Liu
*b and
Jean-Yves
Saillard
*a
aUniv Rennes, CNRS, ISCR-UMR 6226, F-35000 Rennes, France. E-mail: jean-yves.saillard@univ-rennes1.fr
bDepartment of Chemistry, National Dong Hwa University, Hualien 97401, Taiwan, Republic of China. E-mail: chenwei@gms.ndhu.edu.tw
First published on 15th January 2025
Following several reports on ligand-protected atom-precise nanoclusters which encapsulate hydrides as interstitial dopants within their icosahedral core, the stability, structure and bonding of MHx@Ag12 and MHx@Au12 (M = Mo–Ag; W–Au) 8-electron cores is investigated through DFT calculations. The encapsulation of up to x = 3 hydrides appears to be possible but at the cost of substantial structural distortions. In most of the computed models, the hydrides are found nearly free to move inside their icosahedral cages. Systems with one (nido-type) or two (arachno-type) missing vertices on the icosahedron are also predicted to be viable. In general, the MHx@Au12 species appear to be of lower stability than their MHx@Ag12 homologs. We believe that this the work will provide some new directions for the synthesis of hydride-encapsulating superatoms.
Hydride is one of the many ligands commonly encountered in this chemistry.10–16 This monoatomic monoanionic ligand is to some extent related to halides, with which they can sometimes be exchanged. Hydrides have however unique intrinsic characteristics, of which one is their particularly small size. Whereas ordinary ligands protect the [Mn]p+ inner core from the outside by forming a peripheral outer shell around it, it has been shown very recently that the smaller hydrides can, in some cases, get encapsulated inside the metal core.17–29 The most striking structurally characterized examples concern 8-electron superatoms, the metal core of which describes a centered icosahedron, which in addition contains one19,21,22,28 or even two23,24 hydrogen atom(s). These nanoclusters are gathered in Table 1. Note that all of them are doped silver species. Indeed, no (MHx)@Au12 relative has been isolated so far, although such species have been predicted to exist on the basis of DFT calculations.11 The encapsulated hydrides are mainly bonded to the central metal atom so that the whole cluster core is better viewed as describing a distorted (MHx)@M12 (x = 1, 2) icosahedron.
Compound | Superatomic core | Ref. |
---|---|---|
[(RhH)Ag24(SPhMe2)18]2− | [(RhH)@Ag12]4+ | 19 |
[(RhH)Ag20{S2P(OnPr)2}12] | [(RhH)@Ag12]4+ | 24 |
[(RhH)2Ag33[S2P(OnPr)2]17] | [(RhH)@Ag12]4+ | 29 |
[(IrH)Ag24(SPhMe2)18]2− | [(IrH)@Ag12]4+ | 23 |
[(PdH)Ag19{E2P(OiPr)2}12] (E = S, Se) | [(PdH)@Ag12]5+ | 22 and 27 |
[(PdH)Ag20{E2P(OiPr)2}12]+ (E = S, Se) | [(PdH)@Ag12]5+ | 22 and 27 |
[(PtH)Ag19{S2P(OnPr)2}12] | [(PtH)@Ag12]5+ | 21 |
[(PtH)Ag19{Se2P(OiPr)2}12] | [(PtH)@Ag12]5+ | 21 |
[PtHPtAg32[S2P(OnPr)2]17] | [(PtH)@Ag12]5+ | 29 |
[(RuH2)Ag24(SPhMe2)18]2− | [(RuH2)@Ag12]4+ | 23 |
[(OsH2)Ag24(SPhMe2)18]2− | [(OsH2)@Ag12]4+ | 23 |
[(RhH2)Ag19{S2P(OnPr)2}12] | [(RhH2)@Ag12]5+ | 24 |
It has been shown that the 1s electron of an encapsulated hydride is to be considered as one of the eight superatomic electrons, contrary to the case where hydrides behave as ordinary outer ligands.11–29 In other words, if one assumes that a [Mn]p+ metal core possesses a given “magic” number of (n–p) electrons providing it with closed-shell stability, inserting x hydrogen atoms into it would increase its electron count by x. To maintain stability, the “magic” (n–p) electron count should be preserved, so the inserted hydrogen(s) should be, from the electron counting point of view, considered as formal proton(s), thus increasing the formal core charge to [MnHx](p+x)+. In the case the hydrides are regular external H− ligands, then the metal core should retain its p + charge, resulting in the {[Mn]Hx}(p−x)+ assembly. Of course, in both cases, the p ± x cationic charge will be, in real life, compensated by the presence of various additional peripheral anionic ligands to reach (or approach) neutrality for the whole nanocluster.
Thus, encapsulated hydrides should be considered as inclusion dopants rather than ligands, i.e., somewhat behaving as metal dopants. Because of this metal parentage, they are sometimes named “metallic hydrogens”,11,12,15,16 a designation that should not be confused with the meaning of an electron-conducting material. As any metal dopant in nanoclusters, hydrides play a crucial role in their properties. In particular, it has been shown that Au and Ag nanoclusters containing encapsulated hydrides are efficient electrocatalysts in the hydrogen evolution reaction (HER).11,12,16,23,24
Herein we report a comprehensive computational investigation on the encapsulation of one and several hydrides within the M@Ag12 and M@Au12 (M = Mo–Ag and W–Au) centered icosahedral cores, assuming the “magic” 8-electron count to be maintained. We have restricted this study to the superatomic icosahedral cores. Indeed, it has been shown previously that computing the only superatomic core of a nanocluster in its actual oxidation state, i.e. without considering its passivating shell, allows rationalizing its stability, bonding and superatomic electronic structure.30–32 On the other hand, as far as one is interested in bonding analysis only, this simplification also allows to highlight variations across the periodic table, without the blurring caused by the variation of the ligand and outer metal nature.
[M@Ag12]x+ | [M@Au12]x+ | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
M | Mo | Tc | Ru | Rh | Pd | Ag | M | Mo | Tc | Ru | Rh | Pd | Ag |
x | 0 | 1 | 2 | 3 | 4 | 5 | x | 0 | 1 | 2 | 3 | 4 | 5 |
ΔEH/L (eV) | 1.37 | 1.92 | 1.46 | 1.73 | 2.06 | 2.64 | ΔEH/L (eV) | 1.09 | 1.46 | 1.04 | 1.73 | 2.05 | 1.95 |
M–Ag | 2.761 | 2.753 | 2.760 | 2.783 | 2.824 | 2.899 | M–Au | 2.757 | 2.752 | 2.757 | 2.772 | 2.797 | 2.882 |
WBI | 0.447 | 0.397 | 0.340 | 0.262 | 0.230 | 0.230 | WBI | 0.482 | 0.422 | 0.351 | 0.258 | 0.205 | 0.191 |
Ag–Ag | 2.803 | 2.895 | 2.903 | 2.926 | 2.969 | 3.048 | Au–Au | 2.899 | 2.894 | 2.899 | 2.918 | 2.942 | 3.030 |
WBI | 0.084 | 0.085 | 0.086 | 0.090 | 0.089 | 0.084 | WBI | 0.087 | 0.092 | 0.099 | 0.110 | 0.118 | 0.121 |
qM | −2.50 | −2.22 | −2.05 | −1.95 | −1.56 | −1.30 | q M | −2.23 | −1.93 | −1.69 | −1.54 | −1.09 | −0.69 |
qAg | 0.21 | 0.27 | 0.34 | 0.41 | 0.46 | 0.53 | q Au | 0.19 | 0.24 | 0.31 | 0.38 | 0.42 | 0.47 |
M | W | Re | Os | Ir | Pt | Au | M | W | Re | Os | Ir | Pt | Au |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
x | 0 | 1 | 2 | 3 | 4 | 5 | x | 0 | 1 | 2 | 3 | 4 | 5 |
ΔEH/L (eV) | 1.68 | 2.04 | 1.61 | 1.88 | 2.17 | 2.76 | ΔEH/L (eV) | 1.26 | 1.14 | 1.16 | 1.32 | 2.07 | 2.05 |
M–Ag | 2.761 | 2.756 | 2.765 | 2.786 | 2.826 | 2.895 | M–Au | 2.756 | 2.753 | 2.762 | 2.778 | 2.805 | 2.849 |
WBI | 0.417 | 0.364 | 0.314 | 0.268 | 0.231 | 0.232 | WBI | 0.462 | 0.404 | 0.338 | 0.281 | 0.226 | 0.205 |
Ag–Ag | 2.904 | 2.897 | 2.908 | 2.929 | 2.971 | 3.044 | Au–Au | 2.897 | 2.895 | 2.905 | 2.921 | 2.949 | 2.996 |
WBI | 0.084 | 0.085 | 0086 | 0.086 | 0.086 | 0.082 | WBI | 0.089 | 0.092 | 0.097 | 0.104 | 0.112 | 0.119 |
q M | −3.20 | −2.84 | −2.56 | −2.16 | −1.76 | −1.22 | q M | −2.86 | −2.54 | −2.24 | −1.84 | −1.41 | −0.81 |
q Ag | 0.27 | 0.32 | 0.38 | 0.43 | 0.48 | 0.52 | q Au | 0.24 | 0.30 | 0.35 | 0.40 | 0.45 | 0.48 |
It is known from both experimental and computational investigations that the doping of 8-electron centered Ag and Au icosahedral nanoclusters by a transition metal atom from the second and third row and situated on the left side of Ag and Au results in the occupation of the central position by this atom.33–35 The main reason for this situation originates from a stronger participation of the central atom valence nd orbitals to the nanocluster bonding. This is why in the case of the most left-sided M atoms, their significantly bonding nd shell is sometimes considered as constituting the occupied superatomic 1D level, leading such species to be described as 18-rather than 8-electron superatoms.35–37 Likewise, when both metals are from the same group 11 column, the [Au@Ag12]5+ core is observed whereas [Ag@Au12]5+ is unrealistic.34,35 Note that only the (n + 1)s electrons are considered in the 8-electron count, the M contribution being negative (M = Groups 6–9) or nul (M = Pd, Pt). All the computed models have an 1S2 1P6 closed-shell configuration secured by a significant HOMO–LUMO gap. Although this gap decreases when going from Group 11 to Group 6, it should be noted that the bare [Mo@Au12] and [W@Au12] clusters have been experimentally observed,36 right after the theoretical prediction of [W@Au12].37 This suggests that any of the cations listed in Table 2 (except [Ag@Au12]5+, see above)33,34 is likely to be stable, at least as the ligand-protected superatomic core of a larger species.
Both M–M′ (M′ = Ag, Au) and M′–M′ distances increase when M goes from Group 6 to Group to 11. Consistently, the M–M′ Wiberg bond indices (WBIs) decreases, but their variation is more marked than that of the corresponding distances. The stronger bonding for the left-sided M metals has been shown to originate from the larger participation of their nd valence orbitals to superatomic bonding, in such a way that one can include the electrons occupying this somewhat bonding nd(M) shell into the superatomic electron count, allowing [Mo@Au12] or [W@Au12], for example, to be considered as 18-electrons superatoms with 1S2 1P6 1D10 configuration.35,37 Contrarily to the M–M′ WBIs, the M′–M′ ones vary little, especially in the M′ = Ag case and they are always smaller than their M–M′ homologues.
[(MH)@Ag12]x+ | [(MH)@Au12]x+ | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
M | Mo | Tc | Ru | Rh | Pd | M | Mo | Tc | Ru | Rha | Pda |
x | 1 | 2 | 3 | 4 | 5 | x | 1 | 2 | 3 | 4 | 5 |
CSM | 0.62 | 0.57 | 0.52 | 0.44 | 0.31 | CSM | 1.03 | 1.09 | 1.09 | n/a | n/a |
M–H | 1.837 | 1.742 | 1.679 | 1.658 | 1.703 | M–H | 1.821 | 1.719 | 1.657 | 1.637 | 1.692 |
WBI | 0.471 | 0.428 | 0.371 | 0.297 | 0.206 | WBI | 0.487 | 0.460 | 0.417 | 0.424 | 0.344 |
Ag–H | 2.085 | 2.084 | 2.090 | 2.099 | 2.089 | Au–H | 2.168 | 2.191 | 2.211 | 2.137 | 1.717 |
WBI | 0.102 | 0.105 | 0.109 | 0.116 | 0.123 | WBI | 0.099 | 0.099 | 0.107 | 0.171 | 0.418 |
q M | −2.42 | −2.13 | −1.94 | −1.78 | −1.38 | q M | −1.05 | −1.54 | −1.80 | −2.11 | −0.36 |
q Ag | 0.30 | 0.35 | 0.43 | 0.50 | 0.56 | q Au | 0.27 | 0.32 | 0.38 | 0.42 | 0.45 |
q H | −0.20 | −0.20 | −0.21 | −0.27 | −0.38 | q H | −0.07 | −0.05 | −0.05 | 0.01 | 0.02 |
M | W | Re | Os | Ir | Pt | M | W | Re | Os | Ir | Pta |
---|---|---|---|---|---|---|---|---|---|---|---|
x | 1 | 2 | 3 | 4 | 5 | x | 1 | 2 | 3 | 4 | 5 |
a Optimized structure having lost its icosahedral parentage. | |||||||||||
CSM | 0.69 | 0.67 | 0.64 | 0.63 | 0.66 | CSM | 1.10 | 1.28 | 1.39 | 1.79 | n/a |
M–H | 1.843 | 1.754 | 1.694 | 1.655 | 1.651 | M–H | 1.833 | 1.729 | 1.665 | 1.615 | 1.561 |
WBI | 0.490 | 0.457 | 0.403 | 0.356 | 0.306 | WBI | 0.504 | 0.489 | 0.451 | 0.438 | 0.584 |
Ag–H | 2.106 | 2.114 | 2.133 | 2.168 | 2.234 | Au–H | 2.184 | 2.233 | 2.278 | 2.376 | 3.085 |
WBI | 0.092 | 0.092 | 0.088 | 0.094 | 0.090 | WBI | 0.091 | 0.085 | 0.087 | 0.083 | 0.030 |
q M | −3.00 | −2.64 | −2.36 | −1.94 | −1.49 | q M | −2.59 | −2.26 | −1.96 | −1.51 | −0.66 |
q Ag | 0.35 | 0.40 | 0.46 | 0.51 | 0.57 | q Au | 0.31 | 0.36 | 0.42 | 0.46 | 0.46 |
q H | −0.22 | −0.20 | −0.21 | −0.24 | −0.31 | q H | −0.11 | −0.07 | −0.04 | −0.02 | 0.18 |
All the other structures adopt a distorted icosahedral arrangement of C3v symmetry (see the [(PdH)Ag12]5+ example in Fig. 1), with M lying approximately at its center and the hydride inside a tetrahedron made of M and an Ag3 or Au3 triangular face of the icosahedron. As a result, this face is expanded, leading to significant distortion of the whole icosahedral architecture. The amount of distortion away from ideal Ih symmetry can be evaluated with the continuous symmetry measure38 (CSM, see Tables 3 and S1†). Within the silver series, it tends to decrease when M varies from left to right, whereas a more or less opposite trend is found for the gold series. The CSM values found for the gold series are much larger than their silver counterparts, which might indicate lower stability of the (MH)-centered icosahedral Au12 architecture. Overall our results are in good qualitative agreement with the experimentally known nanoclusters that contain [(MH)@Ag12]4+ (M = Rh, Ir)19,23,24,28,29 and [(MH)@Ag12]5+ (M = Pd, Pt).21,22,28 The fact that the computed CSM values are larger than the experimental ones19,23,24 can be explained by the absence in our models of any templating outer shell that would oppose distortion.
In previous investigations on nanoclusters containing an [(MH)@Ag12]5+ (M = Pd, Pt) core,21,22,25,26,28 it was found that the 1s(H) AO interacts principally with the dz2(M) orbital, creating an M–H 2-electron bond and leaving the (n + 1)s AO of M almost unperturbed and containing one electron (see Fig. 2). The superatomic orbitals being principally combinations of metallic valence s-type AOs, it follows that the 1s(H) AO is not significantly involved in their composition. From the superatomic point of view, the interstitial hydrogen provides one electron to the 5s(Pd/Pt) AO, which in turn allows the electron count to achieve the closed-shell count of eight. When M varies from Group 11 to Group 6, the participation of its nd orbitals (thus the ndz2 one) to the superatomic orbitals building increases.35,37 Moreover, the 1s(H) AO tends to interact in a somewhat larger extend with the (n + 1)s AO of M. It results that the contribution of the 1s(H) orbital to the composition of the superatomic orbitals increases. This is exemplified by the substantial increase of the M–H WBIs when going from Group 11 to Group 6 (Table 3), whereas the variation of the Ag–H WBIs is much more modest and mainly reflects the variation of the M radius. Consistently, the hydridic character of H decreases from Group 11 to Group 6.
[(MH2)@Ag12]x+ | [(MH2)@Au12]x+ | |||||||
---|---|---|---|---|---|---|---|---|
M | Mo | Tc | Ru | Rh | M | Mo | Tc | Ru |
x | 2 | 3 | 4 | 5 | x | 2 | 3 | 4 |
CSM | 1.58 | 1.55 | 1.43 | 1.37 | CSM | 1.67 | 2.11 | 2.68 |
M–H | 1.809 | 1.718 | 1.663 | 1.658 | M–H | 1.990 | 1.750 | 1.686 |
WBI | 0.483 | 0.440 | 0.377 | 0.296 | WBI | 0.384 | 0.432 | 0.396 |
Ag–H | 2.151 | 2.164 | 2.669 | 2.050 | Au–H | 1.871 | 2.036 | 1.890 |
WBI | 0.092 | 0.093 | 0.097 | 0.123 | WBI | 0.198 | 0.145 | 0.221 |
H–M–H (°) | 70 | 71 | 75 | 84 | H–M–H (°) | 69 | 68 | 70 |
q M | −2.36 | −2.05 | −1.81 | −1.53 | q M | −2.12 | −1.71 | −1.36 |
q Ag | 0.39 | 0.45 | 0.51 | 0.59 | q Au | 0.36 | 0.40 | 0.45 |
q H | −0.16 | −0.15 | −0.18 | −0.26 | q H | −0.08 | −0.03 | −0.02 |
M | W | Re | Os | Ir | M | W | Re | Os |
---|---|---|---|---|---|---|---|---|
x | 2 | 3 | 4 | 5 | x | 2 | 3 | 4 |
CSM | 1.71 | 1.74 | 1.69 | 1.72 | CSM | 3.41 | 2.37 | 2.83 |
M–H | 1.818 | 1.733 | 1.677 | 1.651 | M–H | 1.837 | 1.722 | 1.677 |
WBI | 0.503 | 0.469 | 0.413 | 0.358 | WBI | 0.463 | 0.483 | 0.449 |
Ag–H | 2.175 | 2.198 | 2.225 | 2.138 | Au–H | 1.998 | 1.957 | 2.084 |
WBI | 0.082 | 0.081 | 0.082 | 0.095 | WBI | 0.148 | 0.156 | 0.137 |
H–M–H (°) | 69 | 70 | 73 | 80 | H–M–H (°) | 51 | 57 | 69 |
q M | −2.81 | −2.45 | −2.15 | −1.67 | q M | −2.42 | −2.02 | −1.70 |
q Ag | 0.43 | 0.48 | 0.54 | 0.59 | q Au | 0.37 | 0.42 | 0.48 |
q H | −0.18 | −0.16 | −0.17 | −0.22 | q H | −0.03 | 0.00 | 0.00 |
It is of note that only one energy minimum was found for every computed model and all the energy minima adopt the same C2v configuration, shown in Fig. 1 for the [(RuH2)@Ag12]5+ model. In this structure, the two hydrides are approximately lying below two distant edges belonging to two edge-sharing triangular faces, as sketched in Scheme 1.
![]() | ||
Scheme 1 A simplified 2-dimensional representation of the hydride positions in the (MH2)@M′12 (M′ = Ag, Au) computed models. Dotted lines indicate elongated M′–M′ edges. |
Being in addition bonded to the central M atom, the hydrides are only tricoordinated, as opposed to the tetracoordination found in the monohydride models (see above). As a result of this double hydride insertion, several edges are elongated (dotted lines in Scheme 1), resulting in a substantial distortion of the icosahedral architecture, as exemplified by the large CSM values (Table 4). The H–M–H angles in Table 4 lie in the range ∼70–80°. The reported experimental values are a somewhat larger (∼90–100°).19,23,24,28,29 The discrepancy can be attributed to the effect of the peripheral shell on the superatomic core it passivates in the real compounds. Indeed, the potential energy surface associated with a variation of the H–M–H angle in our models is rather flat around its minimum. In any case, the linear H–M–H arrangement inside the Ag12 or Au12 icosahedron, as reported for other types of nanocluster19,23,24,28,29 is by far not favored.
Looking firstly at the silver-rich series, five M@Ag12 structures, labelled A, B, C, D and E, were characterized as true minima in the cases of M = Mo–Ru and W–Os. They are shown in Fig. 4 for the M = Mo example. In the cases of M = Tc and Re, additional secondary minima were obtained in which the hydrides are embedded within an open Ag11 cage capped by one Ag atom. These fairly distorted structures are not commented further on. In the cases of M = Ru and Os, a unique minimum of type B was found. Structures A, B, C, D and E have only approximate Cs, Cs, C3, C2 and Cs symmetry, respectively. As indicated by their large CSM values calculated with respect to the closest ideal polyhedron (Tables 5 and S3†), their Ag12 polyhedral envelope adopts configurations resulting from severe distortions away from ideal icosahedron, cuboctahedron and/or anticuboctahedron.
M | Mo | Tc | Ru | ||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
x | 3 | 4 | 5 | ||||||||
Structure type | A | B | C | D | E | A | B | C | D | E | B |
ΔE (kcal mol−1) | 0.0 | 2.9 | 3.1 | 7.4 | 11.5 | 0.0 | 2.1 | 2.1 | 8.0 | 10.5 | |
CSM | 2.32 | 2.41 | 1.88 | 6.40 | 4.91 | 2.55 | 2.37 | 1.93 | 6.49 | 6.95 | 2.25 |
M–H | 1.791 | 1.798 | 1.797 | 1.794 | 1.808 | 1.703 | 1.707 | 1.717 | 1.733 | 1.711 | 1.659 |
WBI | 0.492 | 0.481 | 0.481 | 0.494 | 0.489 | 0.442 | 0.436 | 0.446 | 0.435 | 0.434 | 0.615 |
Ag–H | 2.074 | 2.085 | 2.153 | 2.055 | 2.168 | 2.065 | 2.214 | 2.167 | 2.148 | 2.067 | 2.138 |
WBI | 0.097 | 0.098 | 0.091 | 0.113 | 0.091 | 0.098 | 0.082 | 0.096 | 0.100 | 0.093 | 0.301 |
q M | −2.27 | −2.30 | −2.18 | −2.30 | −2.27 | −1.97 | −1.99 | −1.93 | −1.92 | −1.97 | −1.70 |
q Ag | 0.47 | 0.48 | 0.48 | 0.46 | 0.48 | 0.52 | 0.53 | 0.52 | 0.54 | 0.53 | 0.60 |
q H | −0.12 | −0.15 | −0.15 | −0.13 | −0.16 | −0.10 | −0.13 | −0.13 | −0.17 | −0.13 | −0.15 |
M | W | Re | Os | ||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
x | 3 | 4 | 5 | ||||||||
Structure type | A | B | C | D | E | A | B | C | D | E | B |
ΔE (kcal mol−1) | 0.0 | 2.8 | 3.3 | 7.2 | 11.3 | 0.0 | 1.9 | 2.1 | 7.7 | 10.4 | |
CSM | 2.43 | 2.66 | 2.17 | 6.49 | 5.28 | 2.54 | 2.75 | 2.44 | 6.64 | 5.27 | 2.98 |
M–H | 1.804 | 1.801 | 1.807 | 1.809 | 1.809 | 1.724 | 1.718 | 1.734 | 1.739 | 1.726 | 1.671 |
WBI | 0.516 | 0.508 | 0.519 | 0.508 | 0.508 | 0.473 | 0.477 | 0.478 | 0.481 | 0.471 | 0.420 |
Ag–H | 2.063 | 2.103 | 2.146 | 2.060 | 2.103 | 2.121 | 2.203 | 2.196 | 2.194 | 2.225 | 2.220 |
WBI | 0.091 | 0.085 | 0.086 | 0.089 | 0.086 | 0.085 | 0.085 | 0.097 | 0.085 | 0.071 | 0.074 |
q M | −2.61 | −2.59 | −2.51 | −2.59 | −2.59 | −2.27 | −2.27 | −2.18 | −2.23 | −2.26 | −1.94 |
q Ag | 0.50 | 0.51 | 0.50 | 0.51 | 0.51 | 0.55 | 0.55 | 0.55 | 0.56 | 0.56 | 0.61 |
q H | −0.14 | −0.17 | −0.16 | −0.17 | −0.17 | −0.12 | −0.13 | −0.14 | −0.18 | −0.14 | −0.12 |
With respect to the gold-rich series, only M = Mo, W, Tc and Re provided converged systems with M@Au12 architectures and again structure-types A, B, C, D, and E were found (Table 6), but the number of isomers per M element does not exceed two.
M | Mo | W | Tc | Re | |||
---|---|---|---|---|---|---|---|
x | 3 | 3 | 4 | 4 | |||
Structure type | B | C | A | C | C | E | C |
CSM | 3.60 | 3.34 | 2.25 | 3.33 | 3.81 | 3.22 | 4.19 |
ΔEH/L (eV) | 1.85 | 1.71 | 1.98 | 1.78 | 1.54 | 1.24 | 1.64 |
ΔE (kcal mol−1) | 2.9 | 0.0 | 1.6 | 0.0 | 0.0 | 17.4 | |
M–Au | 2.977 | 3.004 | 2.924 | 2.999 | 3.039 | 2.934 | 3.031 |
WBI | 0.347 | 0.343 | 0.354 | 0.345 | 0.296 | 0.307 | 0.301 |
Au–Au | 2.823 | 2.816 | 2.852 | 2.816 | 2.827 | 2.873 | 2.829 |
WBI | 0.135 | 0.137 | 0.113 | 0.133 | 0.143 | 0.123 | 0.138 |
M–H | 1.824 | 1.791 | 1.927 | 1.806 | 1.719 | 1.846 | 1.728 |
WBI | 0.475 | 0.494 | 0.439 | 0.526 | 0.454 | 0.357 | 0.491 |
Au–H | 1.847 | 1.831 | 1.897 | 1.858 | 1.830 | 1.852 | 1.907 |
WBI | 0.198 | 0.211 | 0.167 | 0.179 | 0.236 | 0.212 | 0.180 |
q M | −1.87 | −1.81 | −2.43 | −2.10 | −1.45 | −1.69 | −1.75 |
q Au | 0.41 | 0.40 | 0.47 | 0.43 | 0.46 | 0.49 | 0.48 |
q H | −0.02 | 0.01 | −0.06 | −0.03 | 0.03 | −0.08 | 0.01 |
The bonding within these 8-electron superatomic models is related to that of their mono- and di-hydride relatives. Although more hypothetical (no such system experimentally reported to date), the lowest energy structures A, B and C, all of icosahedral parentage, are likely to constitute superatomic cores of viable ligand-protected nanoclusters. It is of note that, as this manuscript was under revision, an 8-electron copper-rich cluster with a (PtH3)@Cu12 core having a structure more or less related to the E anticuboctahedral arrangement was just published.39
![]() | ||
Fig. 5 The pathway of the hydride movement in [(RuH)Ag12]3+.(Agaro: Ag atoms around the H atom in the starting structure. Agico: Ag atoms not around the H atom in the starting structure.). |
M | ΔE (kcal mol−1) | M–H | Ag–H | Ag–H–Ag (°) | H–M–Ag (°) |
---|---|---|---|---|---|
Mo | 5.6 | 1.823 | 1.830 | 161 | 99 |
Tc | 4.6 | 1.740 | 1.844 | 155 | 103 |
Ru | 4.3 | 1.669 | 1.871 | 149 | 106 |
Rh | 3.4 | 1.648 | 1.889 | 145 | 108 |
Pd | 2.0 | 1.693 | 1.883 | 143 | 109 |
W | 1.8 | 1.840 | 1.791 | 162 | 99 |
Re | 5.2 | 1.743 | 1.868 | 156 | 102 |
Os | 4.2 | 1.686 | 1.898 | 151 | 104 |
Ir | 3.3 | 1.655 | 1.938 | 148 | 106 |
Pt | 1.7 | 1.644 | 2.005 | 145 | 108 |
We also tested the hydride dynamics on the dihydride series (MH2)@Ag12. With two hydrides moving either sequentially or in a concerted fashion, several pathways are a priori possible. The concerted least-motion pathway illustrated in Fig. 6 was investigated. Selected computed data associated with the transition state are given in Table 8. The activation barriers remain lower than 3 kcal mol−1, except for M = Ir and Rh, with barriers of 5.1 and 7.2 kcal mol−1, respectively.
M | ΔE (kcal mol−1) | M–H | Ag–H | Ag–H–Ag (°) |
---|---|---|---|---|
Mo | 2.8 | 1.794 | 1.932 | 60 |
Tc | 2.6 | 1.706 | 1.946 | 62 |
Ru | 2.4 | 1.650 | 1.943 | 65 |
Rh | 7.2 | 1.659 | 2.067 | 80 |
W | 2.8 | 1.808 | 1.948 | 60 |
Re | 2.5 | 1.724 | 1.971 | 62 |
Os | 2.2 | 1.668 | 1.984 | 65 |
Ir | 5.1 | 1.645 | 2.192 | 73 |
Below we first investigate the 8-electron monohydride series [(MH)@Ag11]x+ and [(MH)@Au11]x+ (M = Mo–Pd, W–Pt), in which the Ag11 or Au11 cages can be viewed as incomplete icosahedra having a missing vertex. The search for energy minima was conducted starting from a M@(Ag11□) (□ = vacancy) skeleton, where the (Ag11□) shape is that of a regular icosahedron (nido-type structure). The hydride was then placed in any of the tetrahedral sites of the centered icosahedron, including those involving the □ vacancy and all these generated starting geometries where fully optimized. It turns out that the same global energy minimum of C5v symmetry was found for all the computed models, but [(PdH)@Ag11]4+. In this C5v structure, exemplified by those of [(RhH)@Ag11]3+ and [(PtH)@Ag11]4+ shown in Fig. 7, the hydride atom sits on the same side as (and close to) the missing vertex of the icosahedron. In the global minimum of [(PdH)@Ag11]4+ (Fig. 7), the hydride sits also on the same open side of the defective icosahedron, but it is now shifted towards an edge of the pentagonal face, leading to Cs symmetry. A secondary minimum, of Cs symmetry, was found for [(PdH)@Ag11]4+ (Fig. 7), where the hydride sits on the other side of the vacancy and is bonded to an icosahedron edge, forcing this part of the structure to distort.
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Fig. 7 The computed isomers of [(RhH)Ag11]3+, [(PdH)Ag11]4+, and [(PtH)Ag11]4+ with corresponding relative energies in kcal mol−1. |
In fact, the C5v structure was found to be the unique minimum for all M dopants, except for M = Rh and Pt, for which one secondary minimum was also found (Fig. 7). The secondary minimum of [(RhH)@Ag11]3+ resembles somewhat the C2v isomer of [(PdH)@Ag11]4+, whereas that of [(PtH)@Ag11]4+ has lost its icosahedral parentage with one Ag atom capping an Ag10 cage. Selected computed data are provided in Table 9.
M | Mo | Tc | Ru | Rh | Pd | W | Re | Os | Ir | Pt |
---|---|---|---|---|---|---|---|---|---|---|
x | 0 | 1 | 2 | 3 | 4 | 0 | 1 | 2 | 3 | 4 |
ΔEH/L (eV) | 1.01 | 1.06 | 1.24 | 1.62 | 1.93 | 1.65 | 1.16 | 1.37 | 1.73 | 2.04 |
M–Ag | 2.765 | 2.758 | 2.765 | 2.791 | 2.840 | 2.770 | 2.765 | 2.775 | 2.801 | 2.850 |
WBI | 0.435 | 0.376 | 0.308 | 0.231 | 0.198 | 0.417 | 0.359 | 0.298 | 0.250 | 0.214 |
Ag–Ag | 2.892 | 2.886 | 2.894 | 2.920 | 2.977 | 2.894 | 2.890 | 2.900 | 2.924 | 2.971 |
WBI | 0.092 | 0.093 | 0.093 | 0.094 | 0.092 | 0.090 | 0.091 | 0.091 | 0.090 | 0.087 |
M–H | 1.740 | 1.669 | 1.617 | 1.592 | 1.669 | 1.756 | 1.693 | 1.643 | 1.611 | 1.605 |
WBI | 0.575 | 0.529 | 0.471 | 0.400 | 0.255 | 0.592 | 0.548 | 0.482 | 0.430 | 0.379 |
Ag–H | 2.569 | 2.541 | 2.536 | 2.555 | 2.031 | 2.585 | 2.562 | 2.562 | 2.585 | 2.644 |
WBI | 0.051 | 0.059 | 0.067 | 0.075 | 0.170 | 0.047 | 0.054 | 0.061 | 0.064 | 0.063 |
q M | −2.28 | −2.03 | −1.82 | −1.63 | −1.12 | −2.78 | −2.49 | −2.22 | −1.83 | −1.41 |
q Ag | 0.21 | 0.278 | 0.35 | 0.43 | 0.49 | 0.26 | 0.33 | 0.39 | 0.45 | 0.51 |
q H | −0.08 | −0.05 | −0.06 | −0.09 | −0.27 | −0.13 | −0.09 | −0.07 | −0.09 | −0.15 |
In all the structures of Fig. 7, the hydride is strongly bonded to M and weakly to Ag. In the C5v structure, the M–Ag distances are particularly long and the associated WBIs particularly weak (Table 9). Nevertheless, this is the dominant low-energy structure in the [(MH)@Ag11]x+ series. It is somewhat reminiscent to that of the 8-electron [HAu9(PMe3)]2+ cluster, where the hydride sits over an open face of the Au@Au8 metal kernel.12 Conversely, it is at variance with the 2-electron nido-type nanoclusters [MHCu11{S2P(OiPr)2}6(CCPh)4] (M = Pd, Pt) of cuboctahedral parentage, where the hydride sits at a tetrahedral site opposite to the vacancy.23,24 It is also noteworthy that in the C5v structure the hydride contribution to the superatomic orbitals becomes nonnegligible. In the case of [(PtH)@Ag11]4+ it contributes 35% and 5% to the 1S and 1Pz orbitals respectively. By comparison, in the Cs minimum of [(PdH)@Ag11]4+ (Fig. 7), its contributions are only 2% and 1%, respectively. Thus, in the C5v structure, the hydride tends to some extend to replace the missing Ag atom on the icosahedron and play the role of a superatom constituent, whereas in the other structures it behaves similarly as in the closo-type relatives, i.e. as an inserted dopant.23
Switching from the Ag-rich species to their gold relatives yielded fairly different results. The global minima found for the 8-electron models [(MH)@Au11]x+ (M = Mo–Pd, W–Pt) are shown in Fig. 8. Only five of them have retained their icosahedral parentage, of which only two (corresponding to M = Tc and Re) are of C5v symmetry. Those corresponding to M = Mo, W and Ru derive from the C5v structure by the opening of one edge of the open pentagonal face. The potential energy surfaces of these species were found more complex that in the case of the Ag-rich series, leading to a larger number of isomers. In addition, their lower HOMO–LUMO gaps suggest lower stability, at least in their considered form of unligated superatomic cores. This is why this series will not be discussed further on. In any case, as already found in the other investigated series, gold-rich clusters are more flexible than their silver homologues, leading to a more complex and less predictable structural chemistry.
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Fig. 8 The lowest energy isomers of the 8-electron models [(MH)@Au11]x+ (M = Mo–Pd, W–Pt) with their HOMO–LUMO gap (eV) below. |
Unfortunately, exploring the possibility for 8-electron arachno-type systems with (MH)@Ag10 or (MH)@Au10 architectures was not possible, owing to the huge number of potential isomeric structures to be considered. However, there is one example of such a species, which has been structurally characterized (except with respect to the hydride location) namely [PtH(AgNO3)2(AuPPh3)8]+.41 Its Ag2Au8 polyhedron can be viewed as an icosahedron having two neighboring vertices unoccupied. We thus simplified the superatomic core of this nanocluster into the corresponding bimetallic arachno model [PtHAu10]3+. Only one energy minimum (of C2v symmetry) was found, with the hydride located at the open side of the uncomplete icosahedron, (Fig. 9). Again, the Pt–H bond is strong (1.569 Å, WBI = 0.509), whereas the two shortest Ag–H contacts are fairly long (2.632 Å, WBI = 0.083). The participation of the hydride in the 1S and 1Pz orbitals is non-negligible (10% and 6%, respectively). Very similar results were also found for [PdHAg10]3+. These results suggest that hydride-encapsulating arachno species are also potentially viable cores for ligand-protected superatoms susceptible to be isolated.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4nr04862h |
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