Raúl
Mera-Adasme‡
ab,
Wen-Hua
Xu‡
cd,
Dage
Sundholm
*c and
Fernando
Mendizabal
*ae
aDepartamento de Química, Facultad de Ciencias, Universidad de Chile, P. O. Box 653, Las Palmeras 3425, Ñuñoa, Santiago, Chile. E-mail: hagua@uchile.cl
bDepartamento de Ciencias del Ambiente, Facultad de Qúimica y Biología, Universidad de Santiago de Chile, Av. Libertador B. O'Higgins 3363, Casilla 40, Correo 33, Santiago, Chile
cDepartment of Chemistry, University of Helsinki, P.O. Box 55 (A.I. Virtanens plats 1), FIN-00014 University of Helsinki, Finland. E-mail: sundholm@chem.helsinki.fi
dCollege of Chemistry and Materials Science, Northwest University, 710127, Xi'an, China
eMillennium Nucleus of Molecular Engineering for Catalysis and Biosensors, ICM, Chile
First published on 28th September 2016
Solar power is a strong alternative to the currently used fossil fuels in order to satisfy the world's energy needs. Among them, dye-sensitized solar cells (DSSC) represent a low-cost option. Efficient and cheap dyes are currently needed to make DSSCs competitive. Computational chemistry can be used to guide the design of new light-absorbing chromophores. Here, we have computationally studied the lowest excited states of ZnPBAT, which is a recently synthesized porphyrinoid chromophore with high light-absorption efficiency. The calculations have been performed at ab initio correlated levels of theory employing second-order coupled clusters (CC2) and algebraic diagrammatic construction using second order (ADC(2)) methods and by performing density functional theory (DFT) calculations using the time-dependent DFT (TDDFT) approach for excitation energies. The ultraviolet-visible (UV-vis) spectrum calculated at the ADC(2) and CC2 levels agrees well with the experimental one. The calculations show that ZnPBAT has six electronic transitions in the visible range of the absorption spectrum. The ab initio correlated calculations and previously reported experimental data have been used to assess the performance of several well-known density functionals that have been employed in the present TDDFT study. Solvent effects have been estimated by using the conductor-like screening model (COSMO). The influence of the addition of a TiO2 cluster to the chromophore systems has also been investigated. The results indicate that both CAM-B3LYP and Becke's “half-and-half” (BHLYP) density functionals are appropriate for the studies of excitation energies in the blue range of the visible spectrum for these kinds of porphyrinoid chromophores, whereas the excitation energies of the Q band calculated at the ab initio correlated level are more accurate than those obtained in the present TDDFT calculations. The inclusion of solvent effects has a modest influence on the spectrum of the protonated form of the studied chromophores, whereas solvent models are crucial when studying the absorption spectrum of the anionic chromophore. The calculated UV-vis spectrum for the chromophore anion is not significantly affected by attaching a TiO2 cluster to it.
The DSSCs originally proposed by Grätzel usually consist of a dye that is adsorbed on a nanocrystalline titanium dioxide (TiO2) electrode.4–9 More recently other semiconductors such as perovskites (CaTiO3) have been found to yield a higher efficiency than with TiO2.10 The light absorbing dyes often consist of metal complexes of, e.g., ruthenium or zinc, with efficiencies between 7% and 11% rendering technical applications feasible.5,11–16 Due to the high price of ruthenium, novel efficient DSSC dyes containing cheaper metals are desirable.5
Another class of potential DSSC dyes is inorganic complexes of organic molecules with extended π–π conjugation, such as metalloporphyrines (MPs), which can be designed to have specific functionalities and properties.17–20 Functionalized MPs can be deposited on semiconductor electrodes for use as dyes in solar energy harvesting devices.4,5 The MP-based DSSCs have good photostability and they are relatively cheap. The use of Zn as the central metal and molecules with metallo-supramolecular interactions has lead to a high efficiency of 6–11%.21–25
One of the Zn porphyrins with the highest solar-light harvesting efficiencies is ZnPBAT, which is a Zn porphyrin with two electron-donating diphenylamine groups in two of the meso positions, a strong electron-withdrawing carboxyphenylethynyl moiety as the anchoring group in one of the meso positions, and a tBu substituted phenyl group in the fourth meso position. The effect of one diarylamino group in meso positions has previously been analyzed.22 The ethynyl group between the anchoring carboxyphenyl group and the porphyrin moiety leads to a slightly improved light-harvesting capability (η) of 10.1% as compared with the similar ZnPBA dye, which has the carboxyphenyl group directly connected to the meso position of the porphyrin ring. The ZnPBA chromophore reaches an η of 8.3%.22 ZnPBAT has broad Soret and Q bands, which enhance light absorption leading to a better performance of the solar cell.22
The interaction between the dye and TiO2 is important for the efficiency of DSSCs. Usually, the dyes have a carboxylate group that binds to TiO2 of the solid electrode. The interaction of the dyes with the (101) plane of TiO2 (anatase) or a TiO2 nanocluster has been studied computationally at quantum and classical levels of theory. The studies show that the dye is attached to titanium dioxide via carboxylate groups.26–34
In this work, we have studied the lowest excited states of the ZnPBAT and ZnPBA dyes at the second-order approximate coupled-cluster (CC2) and the algebraic diagrammatic construction of second order (ADC(2)) levels of theory. The results obtained using the ab initio correlated methods are compared with those calculated at the time-dependent density functional theory (TDDFT) level using a couple of functionals. TDDFT is widely used in excited state studies of large molecules, because of its good performance and its relatively low computational costs.35 However, since TDDFT calculations might suffer from charge transfer problems, the reliability of the obtained results should be assessed by comparing with the results calculated at higher levels of theory.36 Basis-set and solvent effects on the calculated vertical excitation energies have also been investigated. The present CC2 and ADC(2) calculations on the ZnPBAT and ZnPBA molecules and the dyes attached to a TiO2 cluster model are, to the best of our knowledge, the first ab initio study of the excited states of these important DSSC systems, for which experimental ultraviolet-visible (UV-vis) absorption data are available.22
The calculations of the electronic excitation energies were performed at the TDDFT level using the long-range corrected CAM-B3LYP functional38,48,49 and the def2-SVP basis set augmented with diffuse basis functions (def2-SVPD) for the main group atoms.50 For Zn, the def2-SVP basis set was employed. Excited states were calculated using the B3LYP and BHLYP functionals.49,51–54 The CAM-B3LYP functional in combination with the def2-TZVP basis set was also used in the calculations of the excitation energies.
DFT calculations including solvent effects were performed using the conductor-like screening model (COSMO) with a dielectric constant of 24 representing ethanol.55,56 All DFT calculations were performed using the ORCA program package version 3.0.3.57
Excitation energies and oscillator strengths were calculated at the approximative second-order coupled cluster (CC2) and the algebraic diagrammatic construction through second order ADC(2) levels using the scaled opposite-spin approximation and the def2-TZVP basis set.58–60 The def2-SVPD basis set was also employed to assess the size of the basis-set truncation errors of the ab initio correlated calculations. The Laplace transformation (LT) algorithm and the reduced-virtual-space (RVS) approximation were used to speed up the computations.60–64 The RVS cut-off threshold was 60 eV. The COSMO was employed at the ADC(2) level to account for the solvent effects.65 The ab initio correlated calculations were performed using the TURBOMOLE 7.0 package.66–68
Band character | Experimental | ADC(2) (vacuum) | ADC(2) (ethanol) | CC2 (vacuum) | ||||
---|---|---|---|---|---|---|---|---|
λ | Intensity | λ | f | λ | f | λ | f | |
Q | 661 | 0.15 | 639 | 0.17 | 647 | 0.22 | 621 | 0.16 |
Q | 596 | 0.08 | 615 | 0.01 | 618 | 0.01 | 602 | 0.01 |
B | 460 | 0.60 | 463 | 0.16 | 472 | 0.22 | 452 | 0.20 |
B | 448 | 0.42 | 457 | 0.62 | 439 | 0.40 | ||
B | 433 | 0.75 | 435 | 0.51 | 443 | 0.67 | 430 | 0.48 |
B | 418 | 0.15 | 424 | 0.15 | 413 | 0.08 | ||
398 | 1.90 |
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Fig. 2 The calculated exciton density of the selected excited states of ZnPBAT–H. The excited states were obtained at the ADC(2)/def2-TZVP/COSMO (ε = 24) level of theory. The exciton densities are labelled with its absorption wavelength. The exciton density of the strong band at 370 nm reported in the ESI† is also shown. The plots are made using a 0.003 isosurface. Negative exciton densities (holes) are depicted in red and positive in blue. |
The excitation energies calculated at the ADC(2) and CC2 levels are also in excellent agreement with one another. The largest deviation is only 0.07 eV. The solvent effects at the ADC(2) level lead to a redshift of the bands by 3–9 nm (0.01–0.05 eV).
Experiment22 | B3LYP | CAM-B3LYP | CAM-B3LYP (vacuum) | BHLYP | |||||
---|---|---|---|---|---|---|---|---|---|
λ | Intensity | λ | f | λ | f | λ | f | λ | f |
661 | 0.15 | 780 | 0.30 | 610 | 0.33 | 601 | 0.32 | 594 | 0.32 |
596 | 0.08 | 727 | 0.07 | 583 | 0.02 | 579 | 0.02 | 570 | 0.01 |
460 | 0.6 | 691 | 0.08 | 492 | 0.07 | 456 | 0.09 | 487 | 0.06 |
433 | 0.75 | 636 | 0.03 | 463 | 0.21 | 439 | 0.25 | 454 | 0.21 |
526 | 0.04 | 450 | 0.10 | 418 | 0.13 | 450 | 0.14 | ||
526 | 0.10 | 430 | 0.22 | 394 | 0.26 | 432 | 0.21 | ||
516 | 0.18 | ||||||||
474 | 0.04 | ||||||||
452 | 0.20 | ||||||||
407 | 1.78 |
At the B3LYP level, the first two transitions corresponding to the Q band appear at 780 nm and 727 nm. The B band is also significantly redshifted as compared to the experiment. The first strong transition corresponding to the B band appears at 526 nm. In addition, several spurious transitions with small oscillator strengths are obtained in the B3LYP calculations but not at any other level of theory that is employed in this work. The B3LYP calculations of the excitation energies suffer from charge transfer problems, which lead to slightly too low excitation energies and spurious excited states. Thus, the UV-vis spectrum calculated at the B3LYP level is not reliable and is therefore not discussed further in this work.
The shoulder in the experimental spectra at 596 nm is reproduced at the CAM-B3LYP and BHLYP levels. However, the calculated band strength is 4–8 times weaker than the experimental intensity. This weakening is also observed at the ab initio levels. The absorption energies of the strong B bands (Soret) calculated at the CAM-B3LYP and BHLYP levels agree well with the experimental values. The CAM-B3LYP and BHLYP calculations suggest that the B band consists of four transitions, whereas only two peaks are observed in the experimental spectrum.22 It cannot be ruled out that a third strong transition contributes to the strong and broad Soret band in the experimental spectrum. Thus, the experimental UV-vis spectrum is largely reproduced by TDDFT calculations employing the CAM-B3LYP and BHLYP functionals. Since the results obtained at the CAM-B3LYP and BHLYP levels are qualitatively the same, the rest of the BHLYP results are reported only in the ESI.†
The absorption wavelengths and oscillator strengths for ZnPBAT–H calculated at the CAM-B3LYP level are presented in Table 2. Comparing CAM-B3LYP wavelengths with those calculated using the COSMO in Table 2 shows that the solvent contribution is rather small but not negligible especially for the transitions of the B band, which are redshifted by 24–36 nm (0.15–0.26 eV) in the COSMO calculation. For the two transitions of the Q band the solvent shifts are 9 and 4 nm (0.02–0.03 eV), respectively. The inclusion of the solvent effect in the CAM-B3LYP calculation leads to better agreement with experiment for the B band, whereas the Q band is almost unaffected by solvent effects. In the CAM-B3LYP calculation using the COSMO, the lowest transition appears 0.15 eV higher in energy than the maximum of the first peak in the experimental spectrum.
The excitation energies calculated at the CC2 and ADC(2) levels are in excellent agreement. The largest deviation is only 0.07 eV. The calculations at the ab initio levels confirm that ZnPBAT–H has six excited states in the visible range, which is two more than predicted from Gouterman's four-orbital model.70 The trend of the solvent shifts of the ADC(2) excitation energies is similar to the one obtained at the CAM-B3LYP level. However, a solvent redshift of 3–9 nm (0.01–0.05 eV) at the ADC(2) level is observed, although smaller than that obtained in the CAM-B3LYP calculations. The excitation energies calculated at the ADC(2) level using the COSMO are in excellent agreement with the experimental ones with deviations of less than 0.1 eV. However, due to the band broadening of the experimental spectrum, it is hard to determine the exact values for the vertical excitation energies and the number of transitions that contribute to each band. The present calculations suggest that each of the experimental bands at 460 nm and 433 nm comprises two electronic transitions.
TZVP | SVPD | ||
---|---|---|---|
λ | f | λ | f |
609 | 0.32 | 610 | 0.32 |
583 | 0.02 | 583 | 0.02 |
491 | 0.08 | 492 | 0.08 |
462 | 0.22 | 463 | 0.22 |
450 | 0.12 | 450 | 0.12 |
430 | 0.22 | 430 | 0.22 |
TZVP | SVPD | ||
---|---|---|---|
λ | f | λ | f |
647 | 0.22 | 644 | 0.21 |
618 | 0.01 | 616 | 0.01 |
472 | 0.22 | 474 | 0.22 |
457 | 0.62 | 457 | 0.60 |
443 | 0.67 | 443 | 0.64 |
424 | 0.15 | 425 | 0.16 |
ZnPBAT–TiO2 | ZnPBAT–TiO2 (vacuum) | ZnPBAT− | ZnPBA–TiO2 | ZnPBA− | |||||
---|---|---|---|---|---|---|---|---|---|
λ | f | λ | f | λ | f | λ | f | λ | f |
603 | 0.33 | 594 | 0.37 | 602 | 0.28 | 570 | 0.06 | 569 | 0.06 |
583 | 0.03 | 586 | 0.04 | 582 | 0.03 | 568 | 0.05 | 567 | 0.05 |
481 | 0.07 | 421 | 0.25 | 481 | 0.07 | 452 | 0.20 | 454 | 0.18 |
462 | 0.20 | 420 | 0.01 | 462 | 0.20 | 451 | 0.19 | 454 | 0.19 |
448 | 0.07 | 399 | 1.68 | 448 | 0.07 | 414 | 0.18 | 412 | 0.16 |
429 | 0.20 | 392 | 0.01 | 429 | 0.20 | 411 | 0.24 | 409 | 0.23 |
391 | 0.85 |
CAM-B3LYP (vacuum)a | ADC(2) (vacuum)a | ADC(2) (ethanol) | CC2 (vacuum)a | ||||
---|---|---|---|---|---|---|---|
λ | f | λ | f | λ | f | λ | f |
a States obtained in the vacuum calculations with very small oscillator strengths are omitted. The wavelengths omitted in the table are 543, 473, 472, 467, 423, 415 nm at the CAM-B3LYP level; 551, 484, 476, 472, 422 nm at the ADC(2) level; and 493, 445, 440, 432 nm at the CC2 level. | |||||||
597 | 0.40 | 631 | 0.19 | 641 | 0.19 | 618 | 0.03 |
594 | 0.06 | 630 | 0.04 | 616 | 0.01 | 616 | 0.21 |
421 | 0.64 | 427 | 1.44 | 462 | 0.30 | 430 | 1.36 |
415 | 0.47 | 427 | 0.06 | 452 | 0.70 | 416 | 0.72 |
421 | 0.74 | 442 | 0.58 | 410 | 0.44 | ||
422 | 0.14 | 404 | 0.18 | ||||
396 | 1.80 |
A solvation model such as the COSMO is not needed when studying neutral porphyrinoid dyes in solution, whereas it is necessary to enclose anionic chromophores with dielectric media in order to avoid the extra states with small oscillator strengths. Ethanol, which is the solvent used in this work, is rather polar and can form hydrogen bonds with the dye and the semiconductor, which are not considered in the COSMO calculations. We have used the dielectric constant of ethanol in the COSMO calculations, because ethanol was used as solvent in the experimental study by Kurotobi et al.22 Since the solvent effects are small, considering the solvent effects is less crucial when investigating neutral chromophores in non-polar solvents. The inclusion of a solvent model is important for a proper treatment of chromophores bound to TiO2 when simulating the light absorption spectra of DSSCs. In the absence of the dielectricum, the calculated UV-vis spectrum for ZnBAT–(Ti6O21H18) differs from the one calculated for the same system when it is surrounded by a solvent model. The UV-vis spectra of ZnBAT–(Ti6O21H18) and ZnBAT–H calculated in vacuo also differ significantly. For ZnBAT–(Ti6O21H18), states with very small oscillator strengths appear as for the anionic chromophore when the dielectricum is not considered in the calculation. Another important change in the calculated spectra is that one of the strong transitions in the Soret band disappears in the vacuum calculation on ZnBAT–(Ti6O21H18). Thus, in the vacuum calculation ZnBAT–(Ti6O21H18) has only one strong transition in the Soret region with an absorption wavelength of 421 nm. The present study shows that the interaction between the porphyrinoid dye and the TiO2 cluster is altered by the surrounding dielectricum.
Calculations at the time-dependent density functional theory (TDDFT) level show that a significant share of Hartree–Fock (HF) exchange has to be included in the functional in order to avoid spurious charge-transfer states. Calculations using the B3LYP functional with 20% HF exchange result in too small excitation energies and spurious charge-transfer states in the visible range, which disappear when the BHLYP functional with 50% HF exchange, or the long-range corrected CAM-B3LYP is used. The excitation energies calculated using the BHLYP and CAM-B3LYP functionals also agree with the experimental data. Our results suggest that these functionals can be employed in the studies of the light absorption properties of these kinds of porphyrinoids. However, the present study shows that TDDFT calculations on large chromophores should, due to charge-transfer problems, be benchmarked against ab initio data whenever possible. Our results indicate that the def2-SVPD basis set can be employed in TDDFT and ab initio correlated studies of the light-absorption properties of porphyrin-based DSSC chromophores. However, at the ab initio correlated levels the computational time does not increase much when using the larger basis set, because most of the virtual orbitals will be omitted in the calculation of excitation energies when the reduced virtual space (RVS) approximation is employed.64
For the neutral porphyrinoid chromophores, the inclusion of solvent effects via the COSMO55 approach has a modest effect on the calculated light-absorption wavelengths and oscillator strengths. For the anionic (deprotonated) chromophores, it is crucial to consider solvent effects because unphysical diffuse excited states are obtained for the anion when solvent effects are omitted. The diffuse states with small oscillator strengths disappear when the chromophore is surrounded by a dielectricum simulating the solvent.
Footnotes |
† Electronic supplementary information (ESI) available: Coordinates for the systems studied and additional computationally obtained excitation energies and oscillator strengths. See DOI: 10.1039/c6cp04627d |
‡ These authors contributed equally to this work. |
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