Diego
Sorbelli
*ac,
Paola
Belanzoni
*ac,
Trond
Saue
*b and
Leonardo
Belpassi
*c
aDepartment of Chemistry, Biology and Biotechnology, University of Perugia, Via Elce di Sotto 8, 06123 Perugia, Italy. E-mail: diggus18@gmail.com; paola.belanzoni@unipg.it
bLaboratoire de Chimie et Physique Quantiques, UMR 5626 CNRS – Université Toulouse III-Paul Sabatier, 118 route de Narbonne, F-31062 Toulouse, France. E-mail: trond.saue@irsamc.ups-tlse.fr
cInstitute of Chemical Science and Technologies “Giulio Natta” (CNR-SCITEC) c/o Department of Chemistry, Biology and Biotechnology, University of Perugia, via Elce di Sotto 8, 06123 Perugia, Italy. E-mail: leonardo.belpassi@cnr.it
First published on 2nd November 2020
Photoelectron spectroscopy (PES) is a well-known technique which provides unique information about the electronic structure of anionic and neutral species of simple molecules containing heavy elements; however, the detailed interpretation of the resulting experimental spectra can be very complex and theoretical support is mandatory. In this work, based on the available vibrationally resolved PES experiments for gold dihydride (Liu, H.-T. et al., Chem. Sci., 2012, 3, 3286), we have employed several relativistic theoretical approaches with the aim of reproducing experimental photoelectron Detachment Energies (DEs) of AuH2− to give a neutral open-shell molecule, AuH2. The results are discussed in terms of relativistic effects, orbital relaxation and electron correlation. In order to reproduce accurate DEs it has been necessary to include all these effects in a consistent manner at a high degree of accuracy, by means of the equation-of-motion coupled-cluster theory (EOM-IP-CCSD) based on the relativistic exact two-component Hamiltonian (Shee A. et al. J. Chem. Phys., 2018, 174113). This method has also been applied for investigating the ground and low-lying electronic potential energy surfaces of the neutral open shell AuH2 species. The equilibrium geometry of the AuH2 ground state is found to be bent, which is fully consistent with the experimental findings, while all the excited states, including the first, which was previously suggested to have a slightly bent structure, are found to be linear. In the linear centrosymmetric nuclear configuration (which corresponds to the equilibrium geometry of the anion, AuH2−), we find that the first excited state and ground state are very close in energy and the ground state is characterized by an unexpected symmetry breaking in the direction of the asymmetric stretching, due to the pseudo-Jahn–Teller effect. This effect depends on the energy difference between these two electronic states and disappears when the spin–orbit coupling is neglected. The picture that emerges here is intriguing and demonstrates that the interpretation, for which the vibronic transitions that were previously assigned to a slightly bent structure of the first excited state needs to be revised and that a full rationalization of the PES spectra would require the explicit inclusion of the nuclear dynamical effects, beyond the Born–Oppenheimer (BO) approximation. From a methodological point of view, the relativistic EOM-IP-CCSD method results are highly accurate and capable of giving a well-balanced description of the anionic and neutral species, which is a key aspect for the interpretation of the PES spectra in open-shell heavy element compounds.
In this work we have employed various theoretical methods which include relativistic effects and electron correlation with increasing accuracy for the evaluation of the electron detachment energies of AuH2− to reproduce the experimental PES and to give detailed information about the ground and excited states of the AuH2 molecule. The role of relativistic effects, orbital relaxation and electron correlation has been analyzed in detail. In order to include both relativistic effects and the electron correlation in a consistent manner, we have also applied the recently developed and current state-of-the-art relativistic approach for the prediction of the detachment energies, the relativistic ionization-potential-equation-of-motion coupled cluster approach,29 based on the exact two-component (X2C) Dirac–Coulomb–Gaunt Hamiltonian using a molecular mean-field approach30 (hereafter simply referred to as “X2C-EOM-CCSD”). This method has been also employed for investigating the Adiabatic Potential Energy Surfaces (APESs) of the ground and excited electronic states of AuH2. This will shed light on the peculiarities of gold dihydride's electronic structure and reveal intriguing features of the ground state potential energy surface in order to build a bridge between the interpretation of the experimental spectra and the theoretical calculations.
DE = Eneutral − Eanion | (1) |
In this work, various theoretical methods have been employed for the prediction of the VDEs. The methods have been chosen according to their computational complexity and with the specific aim of emphasizing those contributions (such as relativistic effects, orbital relaxation and electron correlation) which are required to obtain accurate VDEs.31,32 The simplest approach is to approximate the VDEs using Koopmans’ theorem (KT).33 This requires a simple Hartree–Fock (HF) calculation on the anion and may be considered as a useful reference since it includes neither the orbital relaxation nor electron correlation (usually, these two factors tend to cancel each other when dealing with valence ionization34). The ΔSCF approach35 has been applied to include the effect of the orbital relaxation (i.e. the response of the electronic structure to a hole created in the occupied orbitals32). In this case VDEs are calculated as in eqn (1) where the energies of the neutral molecule (ground and excited states) are computed by forcing the occupation of the orbitals and then by self-consistently solving the HF or the Kohn–Sham (KS) equation with this excited state population. In these cases in which this procedure properly converges, this approach remains computationally very cheap with the advantage that the orbital relaxation is included in the calculations. With the ΔSCF approach the electron correlation can be neglected (in the case of ΔHF) or included through an exchange–correlation functional at the Kohn–Sham level (ΔKS). Reliable results for the VDEs can be obtained within the framework of the Ionization-Potential-Equation-of-Motion Coupled Cluster (EOM-IP-CCSD)36,37 method, which is known to include in a consistent manner both the orbital relaxation and electron correlation. The method has a computational cost comparable to that of the CCSD method for the ground state (scaling is approximately N6).36 We refer interested readers to a few pedagogical reviews which explain how the EOM (and EOM-IP) theory works and illustrate its applicability on typical target systems.38–41
Unless otherwise stated, all the reported calculations have been carried out using the relativistic quantum chemistry code DIRAC42,43 (released 2018) which implements all the methods mentioned above in combination with accurate relativistic Hamiltonians. In particular, in order to investigate the impact of relativistic effects on VDEs we employed exact 2-component44–48 (X2C) and 4-component (4c) Hamiltonians, with the latter also in its spinfree (SF) form.49
Dyall's Gaussian-type basis sets of different qualities, double-, triple-, and quadruple-zeta with polarization functions (dyall.dzp, dyall,tzp, dyall.qzp respectively) for both gold50 and hydrogen51 were employed for the KT, ΔHF and ΔKS calculations. In the ΔKS case the PBE52 exchange–correlation functional was applied. The SCF convergence on the excited state of the AuH2 molecule was obtained by overlap selection.42,43 Correlated EOM-IP-CCSD calculations are based on the recent relativistic formulation29 and have been carried out using both Dyall valence (dyall.vdz, dyall.vtz, and dyall.vqz) and core-valence (dyall.cvdz, dyall.cvtz, and dyall.cvqz) basis sets.50,51 For the former calculations the 5s, 5p, 5d and 6s electrons for Au are correlated, whereas for the latter the n = 4 shell electrons of Au were included in the active space as well. The X2C-Dirac–Coulomb–Gaunt (DCG) Hamiltonian has been employed in the molecular mean field (mmf) approach.30 This method (in the following simply referred to as “X2C-EOM-CCSD”) represents an excellent compromise between a good accuracy and a reasonable computational cost; the latter has been shown to yield results largely indistinguishable from their 4-component counterparts.29 The X2C-EOM-CCSD approach has been used for the numerical optimization of the minimum energy structures of the AuH2 molecule in its ground and (five) low-lying excited states and to investigate selected cuts of Adiabatic Potential Energy Surfaces (APESs). The calculation of the expectation values of the electric dipole moment for the ground state of AuH2 was carried out using analytical gradients as implemented in ref. 53. For calculating the VDEs, the geometry from ref. 22 has been used for AuH2− (rAu−H = 1.647 Å; αH−Au−H = 180 degrees).
We mention that some test calculations have also been applied including the relativistic effects through the approximate scalar (SR) and spinOrbit (SO) 2-component ZORA Hamiltonians,54–56 for which the Amsterdam Density Functional (ADF) program package57–59 was used, together with Slater-type double- (DZ), triple- (TZ2P) and quadruple-zeta (QZ4P) basis sets. In particular this code has been used to estimate the zero-point-energy (ZPE) and the 0–0 vibrational correction to the ADE.
![]() | ||
Fig. 1 Gray and green diamonds correspond to VDEs estimated using Koopmans’ theorem (KT) at the 4-component (4c-KT) and spin-free (SF-KT) levels, respectively. Black and orange crosses correspond to the 4c-ΔKS and 4c-ΔHF calculations, respectively. The basis set for all the latter is dyall.tzp. Blue dots represent X2C-EOM-CCSD calculations using the dyall.vtz basis set. Red bars represent experimental values from ref. 22. |
State/exp. band | SF-KT | 4c-KT | 4c-ΔHF | 4c-ΔKS | X2C-EOM-CCSD | Exp.a |
---|---|---|---|---|---|---|
a Experimental VDEs (Exp.) are taken from ref. 22. | ||||||
2Σ+1/2u/X | 3.982 (8.3) | 4.021 (9.3) | 3.386 (7.9) | 4.013 (9.1) | 3.667 (0.3) | 3.678 |
2Σ+1/2g/A | 3.676 (5.8) | 3.599 (7.8) | 2.299 (41.1) | 3.848 (1.4) | 3.790 (2.9) | 3.904 |
2Δ5/2g/B | 6.398 (38.1) | 5.699 (22.9) | 2.900 (37.4) | 4.850 (4.6) | 4.731 (2.1) | 4.635 |
2Π3/2g/C | 6.640 (38.8) | 5.878 (22.8) | 3.021 (36.9) | 4.823 (0.8) | 4.825 (0.8) | 4.785 |
2Π1/2g/D | 6.640 (15.4) | 6.933 (20.5) | 4.128 (28.3) | 5.832 (1.5) | 5.765 (0.3) | 5.745 |
2Δ3/2g/E | 6.398 (2.9) | 7.566 (21.5) | 4.477 (28.0) | 6.450 (3.7) | 6.275 (0.8) | 6.22 |
All calculations have been carried out at the linear equilibrium geometry of anion AuH2−, taken from ref. 22 (rAu−H = 1.647 Å; αH−Au−H = 180 degrees). For the sake of simplicity, we keep the same notation used in ref. 22 and label the VDEs using both the experimental bands (X, A, B, C, D and E in energy order) and the spectroscopic terms of the linear centrosymmetric molecules reported as 2Σ+1ΛΩu/g. It should be noted that the first two transitions (corresponding to the ground and first excited states of AuH2) are challenging to assign unambiguously and represent a stringent test for our calculations (these two states are of different parity and are very close in energy, the experimental energy difference is only 0.24 eV).
Now, focusing on the results, we begin with the analysis of the VDE values based on Koopmans’ theorem (KT). As shown in Fig. 1 and Table 1, the VDEs have been calculated both at the 4c level (4c-KT) and in a spinfree framework (SF-KT). Similar data can be obtained with the 2-component scalar and spinOrbit ZORA Hamiltonian, see Table S1 in the ESI.† The results show that the inclusion of SO coupling is fundamental even for a qualitative description of these quantities. Indeed, concerning the higher-energy detachments (i.e. bands from B to E), when SO coupling is included, the experimental VDE trend is nicely reproduced. The method is able to give the correct assignment of these electronic states even if the calculated VDEs are shifted at somewhat higher energy. In a SF framework, a completely different trend is observed. In this case, the C/D states (and the B/E states) become degenerate since they correspond to the doublet components of the 2Π states (and 2Δ states). This clearly prevents the proper energy order and the correct assignment states. Although the 4c-KT method has only to be considered as a first approximation it is noteworthy that the calculated energy splitting for the C/D and B/E states (numerical values are 1.05 eV and 1.86 eV, respectively) agrees surprisingly well with the experimental values (0.96 eV and 1.59 eV). The inclusion of SO coupling has a positive impact on the results for high energy states (i.e. bands from B to E), nevertheless, the situation is different at lower energies (X and A bands). The highest level calculations from ref. 22 showed that the band X should be related to the electronic state of the ungerade symmetry, corresponding to the 2Σ+1/2u state. In our 4c-HF calculations, the AuH2− HOMO is an orbital of symmetry σ1/2g, whereas the HOMO−1 has a σ1/2u symmetry, thus the application of KT gives a ground state of the incorrect symmetry (2Σ+1/2g). Indeed, there is a swap in energy between the HOMO and the HOMO−1 molecular orbitals of the anion. The 4c-KT method is clearly a too simple approach for an accurate estimation of DEs.
For the evaluation of the orbital relaxation effect, we use the 4c-ΔHF approach. The experimental trend is qualitatively reproduced for bands B-E, although the calculated VDE values are now shifted at lower energies; nevertheless the 4c-ΔHF method still fails to provide the correct energy order of the two lowest-energy states (bands X-A). In general, the error in the higher energy states is increased dramatically, probably because the error compensation (between the orbital relaxation and electron correlation contributions), typically expected in the KT framework, is now missing. The 4c-ΔKS calculations show how including both the orbital relaxation and electron correlation significantly improves the agreement with the experimental values. Unfortunately, the energy swap of the lower-energy states still remains and the method fails to reproduce the correct symmetry of the AuH2 ground state. This finding suggests that a more accurate treatment of the electron correlation is needed for reproducing these quantities. The results reported in Fig. 1 and Table 1 show that the X2C-EOM-CCSD method works exceptionally well. First of all, the order of the electronic states found here fully supports the assignment reported in ref. 22, where, as mentioned in the introduction, a multi-step theoretical recipe was specifically applied to include scalar relativistic effects, electronic correlation and spin-orbit coupling in a balanced way. Our results unambiguously confirm that the ground state of AuH2 at the linear centrosymmetric configuration (i.e. at the minimum energy of the anion) is the electronic state 2Σ+1/2u (ungerade symmetry). The computed VDEs are in very good agreement with the experimental data; indeed, as it can be seen, the percent errors for calculated VDEs are in the range of 2.9–0.3% (Table 1). In addition to this, it must be pointed out that the results displayed in Table 1 can be consistently improved. Indeed, as shown in Table 2, one can increase both the quality of the basis set and the number of active electrons. It is evident from the data how increasing simultaneously both of these factors can lead to an even more stringent agreement with the experimental results. For instance, when the electrons of the shell with n = 4 of gold are correlated and a core-valence quadruple-zeta (cvqz) quality basis set is used, the error can be further reduced (the percent errors are in the range of 0.1–1.4%, which corresponds to an absolute error below 0.06 eV). The error on the VDEs for the experimental reference values was estimated in the order of 0.02–0.03 eV.22 The results are consistent (with only a slight increase of the percent error), also if we apply the basis set extrapolation techniques (data labeled as v∞z and cv∞z in Table 2). In particular we have used the three-parameter exponential formula (see eqn (20) in ref. 32) already employed to estimate the ionization energies’ complete basis set limit.32
State/exp. band | Active electrons and basis set | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
5d + 6s | 5s5p5d + 6s | 4s4p4d5s5p5d + 6s | ||||||||||
vdz | vtz | vqz | v∞z | vdz | vtz | vqz | v∞z | cvdz | cvtz | cvqz | cv∞z | |
2Σ+1/2u/X | 3.454 | 3.667 | 3.714 | 3.727 | 3.458 | 3.673 | 3.725 | 3.742 | 3.462 | 3.678 | 3.727 | 3.741 |
(6.1) | (0.3) | (1.0) | (1.3) | (6.0) | (0.1) | (1.3) | (1.7) | (5.9) | (0.0) | (1.3) | (1.7) | |
2Σ+1/2g/A | 3.574 | 3.790 | 3.873 | 3.925 | 3.462 | 3.734 | 3.839 | 3.905 | 3.478 | 3.748 | 3.849 | 3.909 |
(3.8) | (2.9) | (0.8) | (0.5) | (11.3) | (4.3) | (1.7) | (0.2) | (10.9) | (4.0) | (1.4) | (0.1) | |
2Δ5/2g/B | 4.457 | 4.731 | 4.858 | 4.968 | 4.126 | 4.496 | 4.667 | 4.814 | 4.142 | 4.513 | 4.667 | 4.814 |
(3.8) | (2.1) | (4.1) | (7.2) | (11.0) | (3.0) | (0.7) | (3.9) | (10.6) | (2.6) | (0.9) | (3.9) | |
2Π3/2g/C | 4.551 | 4.825 | 4.950 | 5.055 | 4.238 | 4.595 | 4.771 | 4.942 | 4.254 | 4.619 | 4.781 | 4.910 |
(4.9) | (0.8) | (3.4) | (3.8) | (11.4) | (4.0) | (0.3) | (3.3) | (11.1) | (3.6) | (0.1) | (2.6) | |
2Π1/2g/D | 5.500 | 5.765 | 5.884 | 5.981 | 5.259 | 5.593 | 5.764 | 5.943 | 5.274 | 5.621 | 5.773 | 5.891 |
(4.3) | (0.3) | (2.4) | (4.1) | (8.5) | (2.6) | (0.3) | (3.4) | (8.2) | (2.1) | (0.5) | (2.5) | |
2Δ3/2g/E | 5.999 | 6.275 | 6.404 | 6.521 | 5.731 | 6.097 | 6.276 | 6.450 | 5.746 | 6.118 | 6.286 | 6.396 |
(3.5) | (0.8) | (2.9) | (4.8) | (7.9) | (1.9) | (1.0) | (3.7) | (7.6) | (1.6) | (1.1) | (2.8) |
By performing the scan of the APES along both the bond length (maintaining the constraint that the two Au–H remain at the same length) and the bond angle at the X2C-EOM-CCSD level, analogously to what we have done for the first excited state, we have found the equilibrium geometries and the ADEs for all electronic states associated with the experimental bands. The results are reported in Table 3. Concerning the AuH2 ground state, the geometry found here matches quite well the one previously calculated by Liu et al.22 with a bond length of 1.605 Å and a bond angle of 129.2 degrees. Moreover, the ADE value is very close to the one that was determined experimentally and also reported in Table 3. We mention that our theoretical estimate of ADE does not include the 0–0 vibrational correction (the difference in the ZPE of anion AuH2− and of AuH2 at the respective equilibrium geometries). This contribution is relatively small; an estimate at the DFT level gives about 0.03 eV (see Table S7 in the ESI†). Concerning the excited states, even though we have no experimental reference to validate our results, we find that ADEs have only slightly smaller values compared to the VDE values. This is consistent with the small geometrical rearrangements of AuH2 in these electronic states with respect to the anion. The difference between VDE and ADE (ΔVDE−ADE) can be considered as a stringent test for the ability of our calculations to describe the potential energy surface in a well-balanced and consistent manner. We find that the calculated ΔVDE−ADE (0.687 eV) agrees extremely well with the experimental one (0.637 eV). The difference is 0.05 eV, which further demonstrates the consistency of the calculated APESs.
All the results reported above witness the accuracy of the X2C-EOM-CCSD computational protocol in describing the features of gold dihydride's electronic states, in close agreement with the experiment. The only discrepancy that still remains concerns the first excited state, which was expected to be characterized by a slightly bent equilibrium geometry. Returning to the experimental work of Liu et al.,22 we have to observe that the bent structure for the first excited state was drawn on the basis of the presence of a fine structure PES spectrum that emerges at slightly lower energies with respect to the signal assigned to the VDE of the first excited state (band A, in Fig. 3 and Table 1 of ref. 22). These fine band structures are made of three or four vibrational states spaced from about 500 to 200 cm−1 with an increasing anharmonicity and were associated with some bound nuclear states of the bending mode. However, if this would be the case, the energetic range would be consistent with the presence of a double-well in the excited state with a barrier larger than 1600 cm−1 (about 0.2 eV), which is clearly far beyond the accuracy we expect from our level of theory and thus, it would have been easily revealed by our calculations. So, we have to conclude that, on the basis of our extensive theoretical study, the interpretation for which the first excited states should present a bent structure needs to be revised. Furthermore, as a matter of fact the vibrational progression, previously assigned to the first excited state of AuH2 observed in the experiment, occurs at an energy which is between the VDEs of the ground and the first excited state (3.67 and 3.90 eV, respectively) and has a spread of about 0.2 eV, which is really consistent with the small energy difference between these two quasi-degenerate states. We therefore suggest that the mentioned vibrational progression is not a sign of the presence of a bent structure of the first excited state, but may be more likely related to the dynamical effect of the nuclei, which arises from the presence of quasi-degenerate adiabatic states (for which the Born–Oppenheimer approximation cannot be fulfilled).60 In such situations, the fine details of the PES spectra can only be extracted using appropriate nuclear dynamics coupling models based on the results of high-level electronic structure methods.32,60 Precisely because the non-adiabatic dynamics is expected to be very sensitive even to the fine details of the adiabatic potential energy surfaces, especially in the Franck–Condon region, it is highly desirable to investigate whether the presence of these quasi-degenerate states may give peculiar and unexpected features of their topology. In particular, in the following section we will demonstrate that the pseudo-Jahn–Teller effect61,62 gives rise to a symmetry breaking in the adiabatic potential energy surface of the ground state, thus that, right in the Franck–Condon region (i.e. in the linear arrangement), the most stable configuration of AuH2 is a non-centrosymmetric structure with unequal Au–H bond lengths.
The PJTE takes place only when the two (quasi-degenerate) electronic states have symmetry properties which are compatible with the symmetry of the nuclear displacement. In particular, the necessary condition in order to have the PJTE is Γ = Γ′ × Γ′′, where Γ is the irreducible representation of the nuclear displacement and Γ′ and Γ′′ are the irreducible representations to which the lower and higher energy coupled states belong in the high symmetry configuration. The other important factor to have a significant PJTE is the electronic coupling parameter (Δ), which is defined as half of the energy separation between the two coupled states in their high symmetry configuration. The closer these states are in energy (small Δ), the stronger the vibronic coupling is and an actual SB may occur. For gold dihydride in its linear configuration (D∞h symmetry) we have that the ground (2Σ+1/2u) and first excited state (2Σ+1/2g) are very close in energy and are likely to undergo symmetry breaking along the coordinate of the asymmetric stretching (Σ+u symmetry). Note that the necessary condition in order to have the PJTE is fulfilled whether one uses the spin-free notation or the full picture including SO coupling (double group symmetry). In the spin-free framework one only considers spatial symmetry and the direct product of the involved electronic states (Σ+g × Σ+u) gives Σ+u, which is the symmetry of the antisymmetric stretch. In the full picture the direct product of electronic states (E1/2,g × E1/2,u) gives Σ+u + Σ−u + Πu which also includes the symmetry term of the antisymmetric stretch. For an interesting discussion about the impact of SO coupling on the selection rules for PJTE see ref. 73. Since in our case the PJTE can take place by symmetry, the system may be stable in a configuration with unequal Au–H separation, and unstable (saddle point) in the centrosymmetric configuration. At first glance, this seems to be an exotic situation; however, as already mentioned above, it has been observed for a number of linear triatomic open-shell molecules of general formula X–Y–X.62–67
So we have used the X2C-EOM-CCSD approach for investigating the APES along the asymmetric stretching coordinate. The method is expected to be accurate to describe the PJTE.38,69,70 The CI-like form of the EOM excitation operator enables access to multi-configurational open-shell wave functions, including degenerate and nearly degenerate states, as well as interacting states of different character.38 The notorious issue of coupled-cluster theory to treat conical intersections74–76 between states of the same symmetry is not expected to play a role here. The numerical examples of Kohn et al.74 showed that this problem arises only very close to the intersection (within an energy range of ±0.02 eV). This is clearly not the case in point here, in that the involved electronic states have different symmetry for the high symmetry nuclear configuration and their energy gap is above 0.15 eV. For the sake of completeness, we mention that the problem of EOM with treating conical intersections between states of the same symmetry has recently found a solution within the framework of similarity-constrained theory.76 The selected cut of the potential energy surface has been worked out by scanning several distances between the two terminal hydrogen atoms (RH–H′) and by varying the single Au–H bond lengths asymmetrically (the asymmetric displacement with respect to the centrosymmetric structure is indicated as ΔR).
Surprisingly, the results support our hypothesis: the ground state APES of gold dihydride is not centrosymmetric around its linear configuration (as demonstrated by the lower sheet in Fig. 3, showing a double-well APES for the ground state), whereas the first excited state is linear and centrosymmetric. We find the minimum equilibrium structure to be at RH–H′ = 3.3 Å with the minimum energy asymmetric displacement being ΔR = 0.06 Å. For a more quantitative perspective on the energies, we also performed calculations with larger basis sets (i.e. vtz, vqz, with n = 5 and 6s electrons correlated) and by correlating more electrons (i.e. cvtz, cvqz basis, with n = 4, n = 5 and 6s electrons correlated) by keeping fixed the overall RH–H′ distance at 3.3 Å. As shown in Table 4, a SB is always observed, with the minimum energy asymmetric displacement being ΔR = 0.06 Å. Both the PJTE stabilization energy separating the minimum energy asymmetric structure from the centrosymmetric one (EPJTE) and the electronic coupling parameter Δ change, becoming smaller and greater respectively; indeed, the most accurate calculations we performed (i.e. with a cvqz basis set) yield an EPJTE of 31 cm−1, which is small, yet is perfectly compatible with previous data referred to other systems in which the same phenomenon takes place.62 One of the most important and straightforward parameters for the evaluation of the PJTE (see eqn (S3)–(S6) in the ESI†) and SB is the electron coupling parameter, Δ, which can be directly evaluated from the APES. We see, in Table 4, how actually this value is related to the depth of the double-well: when, with smaller basis-sets, we have a greater PJTE stabilization energy, we observe a smaller Δ and vice versa with a larger basis set. One may argue that this symmetry breaking could be an artefact of the calculation; nevertheless, we have means to point out that we avoid artificial SB. First of all, as already mentioned, the X2C-EOM-CCSD method, which is based on EOM-IP-CCSD, is an accurate approach since it recovers most of the necessary correlation needed for treating these phenomena.37,38,65,69,70
Basis set | vdz | vtz | vqz | cvtz | cvqz |
---|---|---|---|---|---|
E PJTE (cm−1) | 268 | 126 | 34 | 150 | 31 |
Δ (cm−1) | 23 | 221 | 466 | 186 | 472 |
ΔR (Å) | 0.06 | 0.06 | 0.06 | 0.06 | 0.06 |
Furthermore, as commonly used in the literature, in order to demonstrate that the SB is a real effect and not an artefact of the calculations is to ascertain that the wavefunction modifies its character continuously as the geometrical parameters are modified along a symmetry breaking mode. Thus, for the linear AuH2 molecule, we calculate the expectation values of the dipole moment for the ground state at different asymmetric displacement (ΔR). A real SB should feature a zero dipole moment when ΔR = 0 and a continuous curve for other values of ΔR65,67 (reflecting a wavefunction which varies continuously as a consequence of the physical mixing of the coupled electronic states). This criterion is fully respected by our calculations: the dipole moment expectation value is zero at ΔR = 0 and as the geometry undergoes distortion the corresponding dipole varies with continuity as shown in the previous cited examples.65,67 The numerical data are reported in the ESI,† see Table S8.
We have shown that the PJTE is very sensitive to the energy separation of the electronic states at their highest symmetric configuration (Δ parameter). Since AuH2 is a heavy-element containing molecule (to our knowledge the first that displays a SB in the asymmetric stretching direction due to PJTE), it is interesting to investigate whether the distortion in the asymmetric direction can be affected by spin–orbit coupling. The answer to this question can be given by scanning the APESs with the EOM-IP-CCSD approach, using a spinfree Hamiltonian in order to switch off spin–orbit interaction. The spinfree APESs are reported in Fig. 4, where, by using a spinfree Hamiltonian in the calculations, there is no evidence of a SB in the asymmetric stretching direction. Indeed, the APES for the ground state is found to be very flat, but both the ground and first excited state's APESs show a minimum at ΔR = 0, i.e. the minimum configuration is the centrosymmetric one when spin–orbit coupling is neglected. This finding is surprisingly in that the symmetry analysis just reported above shows that PJTE is also allowed within the spinfree framework. A more quantitative perspective can be obtained by considering the electronic coupling parameter (and therefore the separation of the two states at ΔR = 0, 2Δ). Indeed, as shown in Table 4, where relativistic effects (including spin–orbit coupling) are considered, the separation between these ground and first excited states in their linear nuclear configuration (when using the same computational setup, i.e. the dyall.vtz basis set) is less than 1000 cm−1 (2Δ = 932 cm−1). In the case of spinfree calculations instead, switching off the spin–orbit interaction, the separation is much larger and almost the double (1724 cm−1). This is consistent with the PJTE theory, where to larger Δ should correspond weaker couplings between states.
In particular, on the basis of our X2C-EOM-CCSD calculations we have demonstrated that the interpretation which suggested for a slightly bent structure of the first excited state of AuH2 needs to be revised. The first excited state in AuH2 is found to be linear and, in this nuclear configuration (which also corresponds to the equilibrium geometry of the anion, AuH2−, and characterizes the vertical detachment process), it is quasi-degenerate with the ground electronic state. Surprisingly, these states are found to be coupled by the pseudo-Jahn–Teller effect (PJTE) which induces a symmetry breaking along the asymmetric stretching coordinate, for which the centrosymmetric nuclear configuration becomes a saddle point and the asymmetric configuration (two Au–H bonds with different lengths) is the most stable. Even though similar triatomic open-shell molecules have been reported to be affected by this phenomenon, this is, to our knowledge, the first reported example of a heavy-metal-containing molecule affected by PJTE in the direction of the asymmetric stretching. Since AuH2 is a heavy metal containing compound, the role of the spin–orbit coupling has been analyzed. Its effect is to reduce the energy gap between these quasi-degenerate states and to enhance the PJTE. Interestingly, thus, we have shown how the symmetry breaking is observed only when the calculations accurately account for spin–orbit coupling. Our findings strongly suggest that the mentioned vibrational progression observed in the reference experiment is not a sign of the presence of a bent structure of the first excited state, but, more likely, may be related to the dynamical effect of the nuclei, due to the presence of quasi-degenerate adiabatic states (for which the Born–Oppenheimer approximation may not be fulfilled) in the Franck–Condon region associated with the photodetachment process. It is clear that in order to confirm the last hypothesis a full treatment of the nuclear degrees of freedom would be required. The latter, together with the surprising symmetry breaking reported here, paves the way for further theoretical and experimental investigation on the peculiar electronic structure of AuH2, which is a simple molecular system only in appearance.
Footnote |
† Electronic supplementary information (ESI) available: A brief summary of the basic theory of the pseudo Jahn–Teller effect, vertical detachment energies calculated using 2-component scalar and spin–orbit ZORA Hamiltonian, X2C-EOM-CCSD calculated energies using different basis sets and dipole moments in different geometrical arrangements of AuH2. See DOI: 10.1039/d0cp05204c |
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