Ouissam
El Bakouri
a,
Miquel
Solà
*a and
Jordi
Poater
*bcd
aInstitut de Química Computacional i Catàlisi (IQCC) and Departament de Química, Universitat de Girona, Campus Montilivi, 17071, Girona, Catalonia, Spain. E-mail: miquel.sola@udg.edu
bDepartament de Química Inorgànica i Orgànica & Institut de Química Teòrica i Computacional (IQTCUB), Universitat de Barcelona, Martí i Franquès 1-11, 08028, Barcelona, Catalonia, Spain. E-mail: jordi.poater@gmail.com
cDepartment of Theoretical Chemistry and Amsterdam Center for Multiscale Modeling, Vrije Universiteit Amsterdam, De Boeleaan 1083, NL-1081HV Amsterdam, The Netherlands
dInstitució Catalana de Recerca i Estudis Avançats (ICREA), Pg. Lluís Companys 23, 08010 Barcelona, Catalonia, Spain
First published on 23rd January 2018
Correction for ‘Planar vs. three-dimensional X62−, X2Y42−, and X3Y32− (X, Y = B, Al, Ga) metal clusters: an analysis of their relative energies through the turn-upside-down approach by Ouissam El Bakouri et al., Phys. Chem. Chem. Phys., 2016, 18, 21102–21110.
B62− | Al62− | Ga62− | |||||||
---|---|---|---|---|---|---|---|---|---|
D 2h + D2h → D2h | O h + Oh → Oh | Δ(ΔE) | D 2h + D2h → D2h | O h + Oh → Oh | Δ(ΔE) | D 2h + D2h → D2h | O h + Oh → Oh | Δ(ΔE) | |
ΔEint | −188.0 | −98.0 | −90.0 | −20.0 | −38.8 | 18.8 | −18.0 | −29.8 | 11.9 |
ΔEPauli | 522.4 | 710.4 | −188.0 | 218.1 | 339.2 | −121.1 | 253.5 | 370.0 | −116.5 |
ΔVelstat | −234.0 | −282.0 | 48.0 | −93.0 | −162.3 | 69.2 | −129.7 | −199.7 | 69.9 |
ΔEoi | −473.4 | −524.4 | 51.1 | −141.9 | −211.9 | 70.0 | −137.9 | −195.7 | 57.8 |
ΔEdisp | −3.1 | −2.0 | −1.1 | −3.1 | −3.8 | 0.7 | −3.8 | −4.5 | 0.7 |
ΔEdist | 25.1 | 2.6 | 22.5 | 0.0 | 3.0 | −3.0 | 0.2 | 2.8 | −2.6 |
ΔE | −162.9 | −95.4 | −67.5 | −20.0 | −35.8 | 15.8 | −17.8 | −27.0 | 9.3 |
ΔEint | ΔEPauli | ΔVelstat | ΔEoi | ΔEdisp | ||
---|---|---|---|---|---|---|
B2Al42− | D 4h | −51.1 | 431.3 | −198.6 | −280.0 | −3.8 |
D 2h | −39.6 | 238.5 | −96.1 | −178.9 | −3.2 | |
ΔE | 11.5 | −192.8 | 102.5 | 101.1 | 0.6 | |
Al2B42− | D 4h | −72.8 | 566.5 | −244.1 | −392.0 | −3.2 |
D 2h | −136.8 | 545.5 | −233.8 | −445.4 | −3.2 | |
ΔE | −64.0 | −21.0 | 10.3 | −53.4 | 0.0 | |
Al2Ga42− | D 4h | −33.6 | 366.0 | −193.0 | −202.2 | −4.4 |
D 2h | −18.8 | 277.4 | −144.2 | −148.4 | −3.7 | |
ΔE | 14.8 | −88.5 | 48.8 | 53.8 | 0.7 | |
Ga2B42− | D 4h | −82.1 | 578.6 | −257.3 | −400.0 | −3.4 |
D 2h | −152.8 | 523.8 | −218.8 | −454.5 | −3.1 | |
ΔE | −70.7 | −54.8 | 38.4 | −54.5 | 0.3 | |
Ga2Al42− | D 4h | −37.6 | 362.7 | −184.2 | −211.8 | −4.2 |
D 2h | −20.2 | 213.6 | −89.0 | −141.5 | −3.5 | |
ΔE | 17.4 | −149.1 | 95.3 | 70.3 | 0.7 | |
Al3Ga32− | D 3h | −35.7 | 369.6 | −191.9 | −209.2 | −4.1 |
C 3v | −19.9 | 244.2 | −117.9 | −142.8 | −3.5 | |
ΔE | 15.8 | −125.3 | 74.0 | 66.5 | 0.6 |
As to the discussion, there are only two paragraphs affected:
(1) Last paragraph on page 21105 that now reads:
The different terms of the EDA analysis for B62−, Al62−, and Ga62− clusters are enclosed in Table 2. First, we notice that the total bonding energies (ΔE) are much larger for B62− than for Al62− or Ga62−. For the former, ΔE are −95.4 (Oh) and −162.9 kcal mol−1 (D2h), whereas for the two latter are in between −17.8 and −35.8 kcal mol−1. This trend correlates with the shorter B–B bond lengths mentioned above. Table 2 also encloses the relative EDA energies between the two clusters. The B3− fragment taken from B62− system in its D2h symmetry is the one that suffers the largest deformation, i.e. the largest change in geometry with respect to the fully relaxed B3− cluster in the quintet state (ΔEdist = 25.1 kcal mol−1), whereas the rest of the systems present small values of ΔEdist (0.0–3.0 kcal mol−1). However, differences in ΔE are not due to distortion energies (indeed ΔEdist values follow the opposite trend as ΔE), but to interaction energies (ΔEint).
(2) First paragraph on page 21106 that now reads:
Thus, we focus on the decomposition of ΔEint into ΔEPauli, ΔVelstat, ΔEoi, and ΔEdisp terms. As a general trend, in all three X62− clusters ΔEPauli is larger for the Oh than the D2h cluster (Δ(ΔEPauli) = −188.0, −121.1, and −116.5 kcal mol−1 for B62−, Al62−, and Ga62−, respectively), so making it less stable. The overlaps between doubly occupied MOs are larger in the more compact Oh structure that, consequently, has larger ΔEPauli. The larger difference in ΔEPauli between the Oh and D2h structures in the case of B62− as compared to Al62− and Ga62− is attributed to the particularly short B–B distances that increases the overlap between doubly occupied MOs of each B3− fragment. At the same time, the Oh form presents larger (more negative) electrostatic interactions (Δ(ΔVelstat) = 48.0, 69.2, and 69.9 kcal mol−1 for B62−, Al62−, and Ga62−, respectively). It is usually the case that higher destabilising Pauli repulsions goes with larger stabilising electrostatic interactions. The reason has to be found in the fact that both interactions increase in absolute value when electrons and nuclei are confined in a relatively small space. The electrostatic interaction together with orbital interaction (Δ(ΔEoi) = 51.1, 70.0, and 57.8 kcal mol−1 for B62−, Al62−, and Ga62−, respectively) terms favour the Oh structure. In the case of Oh B62−, however, Δ(ΔVelstat) and Δ(ΔEoi) cannot compensate Δ(ΔEPauli), which causes the D2h system to be the lowest in energy. The opposite happens for Al62− and Ga62−. Finally, the dispersion term does almost not affect the relative energies, as the difference in dispersion is only in the order of ca. 1.0 kcal mol−1. Therefore, what causes the different trend observed for B62− on one side, and Al62− and Ga62− on the other side is basically the ΔEoi term, which combined with the ΔVelstat component does (Al62− and Ga62−) or does not (B62−) compensate for the higher ΔEPauli of the Oh form.
As to the conclusions, the sentence “From one side the D2hHOMO-1(b2u) formed from two tangential SOMO σT(b2) orbitals” should read “From one side the D2hHOMO-2(b2u) formed from two tangential SOMO σT(b2) orbitals”.
The Royal Society of Chemistry apologises for these errors and any consequent inconvenience to authors and readers.
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