Green-Solvent Processed Blade-Coating Organic Solar Cells with an Efficiency Approaching 19% Enabled by Alkyl-Tailored Acceptors

Highlights Alkyl-tailored Y-SMAs named YR-SeNF series with near-infrared absorption, different molecular crystallinity and self-assembly abilities are developed. The related organic solar cells (OSCs) with an active layer processed from halogen-free solvents and spin-coating-free technologies achieve a ~ 19% efficiency. Ternary OSCs offer a robust operating stability under MPP tracking and well-keep > 80% of the initial efficiency for even over 400 h. Supplementary Information The online version contains supplementary material available at 10.1007/s40820-023-01208-0.


Introduction
Organic solar cells (OSCs) have attracted great attention due to the advantages of low-cost, versatile applications in flexible electronics, and potential large-area printing processability [1][2][3][4][5][6].Mainly due to the remarkable breakthrough of non-fullerene small molecule acceptors (SMAs) recently, especially superstar Y-series SMAs (Y-SMAs) with a donor-acceptor-donor (DAD)-fused central-core and two benzene-fused electron-deficient end-groups, OSCs have achieved impressively high-power conversion efficiencies (PCEs) of over 19%, which greatly lights up the commercial prospect of OSCs [7][8][9][10][11][12][13][14][15].However, these high PCEs are usually obtained from spin-coating process and low-boilingpoint toxic halogenated solvents such as chloroform, while the former limits the large-area fabrication of OSCs, and the latter will cause serious environmental pollution [16,17].When turning to the blade-coating process toward large-scale printing and high-boiling-point eco-friendly solvents required for industrial development, there is usually a marked PCE drop.
The PCE drop of OSCs processed from halogen-free highboiling point solvents is mainly due to the poor solubility of photovoltaic materials, such as Y6 with short sized alkyl chains shows low solubility in o-xylene, leading to strong self-aggregation thus serious phase separation in active layers [18,19].Previous researches have attempted to carry out alkyl chain engineering on Y-SMAs to solve the solubility challenge, so as to be able to use halogen-free highboiling-point solvents to fabricate efficient OSCs [20][21][22][23][24][25][26].However, while improving the solubility, long-sized alkyl chains usually break the tight packing of backbone, which leads to weak molecular ordered assembly and poor charge transfer properties [27][28][29][30][31][32].On the other hand, the PCE drop of OSCs processed with blade-coating technology is mainly due to the difficulty in precise control of the crystallization and phase separation kinetics during film formation, commonly resulting in undesirable active layer morphology [33][34][35][36][37][38][39].As a result, although great efforts have been made to alter the alkyl chains of Y-SMAs and optimize the filmformation process, the success in achieving high-efficiency OSCs processed with eco-friendly solvents and blade-coating technology so far is still constrained.

3
Here, a series of newly designed N-alkyl-tailored Y-SMAs (named YR-SeNF, including YBO-SeNF, YHD-SeNF, and YDT-SeNF) are developed by combining selenophene (Se)-fused central-core with naphthalene (Np)-fused end-groups (Fig. 1a), which show near-infrared (NIR)-absorption, different molecular crystallinity and self-assembly abilities.The studies exhibit that these N-alkyl-tailored YR-SeNF as the key guest components in binary PM6:L8-BO host system can well manipulate morphologies of blade-coating active layers processed with halogen-free and highboiling-point o-xylene solvent, such as molecular packing, crystallinity, and vertical distribution, resulting in the improved charge transfer dynamics and stability for OSCs.Benefiting from the above advantages, we successfully achieve a record-high PCE approaching 19% in the blade-coating OSCs processed from o-xylene solvent.Notably, due to the outstanding compatibility between guest YHD-SeNF and host L8-BO, ternary OSCs offer robust operating stability under maximumpower-point (MPP) tracking and well-keep > 80% of the initial PCEs for even over 400 h.

Device Fabrication and Characterization
The OSCs with a device structure of ITO/2PACz/active layer/PFN−Br/Ag were fabricated under conditions as follows.ITO substrates were first scrubbed, dried overnight in an oven, and then treated by UV−Ozone for 30 min before use.The 2PACz was dissolved in ethanol with a concentration of 0.5 mg mL −1 .ITO substrates were then dipped into 2PACz solution with a temperature of 80 °C for 10 min, then taken out and washed by pure ethanol.PM6:L8−BO:YR−SeNF (1:1.2:0,1:1:0.2,1:0.8:0.4,and 1:0:1.2) blends were dissolved in o−xylene with 1,4−diiodobenzene (DIB) as solid additive (100% in w/w) under 40 °C for 3 h to mix intensively in a N 2 −filled glove box, in which the D:A solid concentration is 25 mg mL −1 in total [40].The blend solutions were blade−coated immediately on the top of 2PACz layer with a speed of 30 mm s −1 followed by a 100 °C thermal annealing.The optimal active layer thickness measured by a Bruker dektak XT stylus profilometer was about 100 nm.Then, a thin PFN−Br layer (0.5 mg mL −1 in methanol with 0.25 wt% melamine) was blade−coated (10 mm s −1 moving speed) on the active layer, followed by the deposition of Ag (evaporated under 5×10 −4 Pa through a shadow mask).The current density-voltage (J−V) curves of OSCs were measured using a keysight B2901A source meter in glove box under AM 1.5G (100 mW cm −2 ) using an Enlitech solar simulator.The device contact area was 0.042 cm 2 , device illuminated area during testing was 0.0324 cm 2 , which was determined by a mask.The external quantum efficiency (EQE) spectra were measured using a solar cell spectral response measurement system QE−R3011 (Enlitech).The light intensity at each wavelength was calibrated using a standard monocrystalline Si photovoltaic cell.The MPP tracking was carried out upon epoxy encapsulated devices under 1−sun white LED array in air.The whole tracking condition (temperature and humidity) is co−controlled by air−conditioner and blowing cooling setups.

Photophysical and Electrochemical Properties
Design strategy and synthetic routes of YR-SeNF series with different N-alkyl substitutions (YBO-SeNF with 2-butyloctyl, YHD-SeNF with 2-hexyldecyl, and YDT-SeNF with 2-decyltetradecyl) are presented in Fig. 1a and S1.The characterizations of molecular structure (including 1 H/ 13 C NMR and mass spectra) for YR-SeNF series are summarized in Figs.S2-S12, respectively.The gradually extended N-alkyl chain length in YR-SeNF series offers better solubility in halogen-free and highboiling-point solvents such as o-xylene.In the grazing incidence wide-angle X-ray scattering (GIWAXS) measurements (Fig. 1d, S13, and Table S1) of the blade-coating neat films, compared to YDT-SeNF with the longest N-alkyl chains has a diffused (100) peak in in-plane (IP) direction, both of YBO-SeNF and YHD-SeNF achieve the sharp (100) peaks.With the N-alkyl sized extension, YR-SeNF series show gradually increased π-π stacking distances of 3.659-3.726Å and decreased crystal coherence lengths (CCLs) of 15.01-16.57Å, indicating that N-alkyl chain engineering successfully regulates the molecular crystallinity and ordered stacking.These properties offer some information in controlling crystallization and morphology of blade-coating active layers, especially when introducing YR-SeNF series as the third component into PM6:L8-BO host system, which well be elaborated in the following sections.
In both dilute o-xylene solutions (Fig. S14) and neat films (Fig. 1e), YR-SeNF series show nearly identical absorption spectra.As shown in Fig. S15 of molecular temperature dependent absorption in dilute o-xylene solution, benefiting from the strong intermolecular interaction caused by the combination of Se-fused central-core and Np-fused end-groups, all of YR-SeNF series only show slightly decreased absorption intensity as the temperature increases from 30-100 °C [41].YR-SeNF series exhibit much sharper 0-0 peaks which belong to J-aggregation compared to L8-BO in films, indicating more orderly intermolecular π-π stacking.Thanks to that selenium atom has a looser delocalized electron cloud than sulfur one to form better orbital overlap and stronger quinoidal character in π-conjugated system [42,43], YR-SeNF series display a 75 nm red-shifted absorption peak, 65 nm extended absorption onset, and much smaller optical bandgap (E g opt ) of 1.27 eV compared to L8-BO (1.36 eV), which is more complementary to PM6 and well-fill in the photon capture deficiency of L8-BO in the NIR region of > 900 nm.As shown in Fig. S16, all of L8-BO:YR-SeNF (0.8:0.4) binary blends with a small amount of YR-SeNF as guest component show obviously red-shifted absorption onsets compared to L8-BO, while they only show slightly blue-shifted absorption spectra compared to YR-SeNF, suggesting that each component kept its own photon capturing behavior to large extent.A similar phenomenon has been observed in ternary PM6:L8-BO:YR-SeNF blends with different component ratios (Fig. S17).As shown in Fig. S18, L8-BO:YR-SeNF binary acceptors have almost same absorption, suggesting a similar compatibility among them.Differently, ternary PM6:L8-BO:YR-SeNF blends show obviously diverse absorption onsets due to different miscibility between PM6 and YR-SeNF series.
Cyclic voltammograms (CV) were performed to study the molecular energy levels of YR-SeNF series.As shown in Fig. 1f and S20, YR-SeNF series with extended N-alkyl chains show similar lowest unoccupied molecular orbital (LUMO) energy levels, which are consistent with their nearly identical absorption spectra.Moreover, compared to L8-BO host [46], YR-SeNF guests have decent LUMO levels (ΔE LUMO = ~ 0.07 eV), even the latter ones have obviously red-shifted absorption onset of 65 nm, which is expected to achieve both high open-circuit voltage (V OC ) and short-circuit current density (J SC ).

Molecular Dynamics Simulations
Molecular dynamics (MD) simulations were carried out to understand the intermolecular packing of alkyl-tailored YR-SeNF series [47,48].As depicted in Fig. 2a, YR-SeNF series with different N-alkyl substitutions have dramatically different packing patterns.Among them, YBO-SeNF and YDT-SeNF show similar rectangle shaped voids with different size, while YHD-SeNF plays a unique role in constructing three-dimensional (3D) network with special S-shaped voids [49].Unique S-shaped voids in YHD-SeNF indicate that molecular packing pattern not only derives from the direct influence of side-chain steric effect but also the indirect influence of side-chain by changing the geometric shape of backbone.With the extension of N-alkyl in YR-SeNF series, the voids increase by ~ 1.6 times from 10.9 × 15.2 to 17.3 × 23.7 Å 2 due to the steric hindrance of N-alkyl chains, which will affect their solution processability especially in halogen-free solvents with high-boiling point.Moreover, the geometries of YR-SeNF series need to be attention due to N-alkyl chains also can effect molecular backbone, which is related to intermolecular aggregation and blend morphology.As illustrated in Fig. 2b, YR-SeNF series show a similar banana curved and helical molecular geometry.Molecular angles built from the two F atoms in end-groups and S atom in center (∠FSF) are 77.81° for YBO-SeNF, 80.15° for YHD-SeNF, and 78.41° for YDT-SeNF, respectively.YHD-SeNF has more twisted backbone with a bigger angle due to its larger N-alkyl chains compared to YBO-SeNF.YHD-SeNF shows a larger torsion angle compared to YDT-SeNF, mainly due to the middle N-alkyl chains in YHD-SeNF can be wrapped within the molecule.In the case of YDT-SeNF, N-alkyl chains are too large to wrap within its molecule and are squeezed onto both the sides of molecular backbone, resulting in a smaller intramolecular steric effect and thus, a smaller molecular twist.The above results partially explain why YR-SeNF acceptors have distinctive packing patterns.As shown in Fig. S21 and Table S2, using the space-charge-limited-current (SCLC) method, YBO-SeNF and YDT-SeNF have slightly higher electron-mobilities (μ e ) of ~ 1.9 × 10 −4 cm 2 V −1 s −1 compared to YHD-SeNF (1.65 × 10 −4 cm 2 V −1 s −1 ), which are also related to their twisted backbone (Fig. 2b).
The packing distance differences of YR-SeNF series are further looked into (Fig. 2c), which more reflects the intermolecular steric hindrance of N-alkyl chains.YBO-SeNF with a relatively small steric hindrance can be together closer (2.9 Å) and thus, may cause excessive aggregation.YDT-SeNF with long-sized N-alkyl chains has far away packing from each other, even up to 6 Å.The middle N-alkyl chains of YHD-SeNF result in a suitable steric hindrance that allows the intermolecular stacking distance to be 3.0-3.2Å, which does not cause excessive aggregation, nor will it be too far apart to facilitate charge transport.The above results indicate that suitable N-alkyl chains may balance intramolecular and intermolecular steric hindrance and thus, form unique stacking structures for improving charge transfer and charge transport dynamics in active layers [50,51].

Photovoltaic Properties and Stability
The photovoltaic performances of the OSCs based on binary PM6:YR-SeNF and ternary PM6:L8-BO:YR-SeNF with a device structure of ITO/2PACz/active layer/PFN-Br/Ag were studied by a combining strategy toward industrial development of spin-coating-free (dip-coating for 2PACz layer, blade-coating for active layer and PFN-Br layer) technology and halogen-free high-boiling-point o-xylene solvent processing (Fig. 3a).As shown in Fig. 3b-d of the J-V curves and Table 1 of photovoltaic parameters, with the extension of N-alkyl size in YR-SeNF series, the related OSCs obtained gradually improved PCEs from 16.1 to 17.2%.The PM6:YR-SeNF-based OSCs achieved both lower V OC of 0.824-0.848V and fill factor (FF) of 0.745-0.754but significantly higher J SC of 26.4-27.2mA cm −2 compared to the PM6:L8-BO-based ones (V OC = 0.880 V, J SC = 25.3 mA cm −2 , and FF = 0.779).As we expected, the PM6:YR-SeNF-based OSCs obtained higher V OC × J SC products as 22.33-22.74compared to the PM6:L8-BO-based one (22.26),implying the effectiveness of our strategy to develop NIR-absorbing Y-SMAs for boosting both photo-current and photo-voltage outputs.All these characteristics, such as relatively narrow absorption of < 900 nm, high V OC and FF, suggesting that binary PM6:L8-BO is an ideal candidate to further improve PCE by introducing YR-SeNF series as guest components with high J SC due to the broadened absorptions > 975 nm.
To study the effects of introducing guest YR-SeNF series into binary PM6:L8-BO host system on photovoltaic performance, the PM6:L8-BO:YR-SeNF-based ternary OSCs were fabricated.Surprisingly, all ternary OSCs with different PM6:L8-BO:YR-SeNF ratios (1:1:0.2and 1:0.8:0.4)achieved much superior device performance compared to their parental binary OSCs.For example, ternary OSCs obtained much higher J SC of 27-28 mA cm −2 , well-kept and even higher FF of 0.772-0.789,and only slightly reduced V OC of 0.861-0.874V compared to the PM6:L8-BO-based OSCs.Moreover, ternary OSCs achieved furtherly improved products of V OC × J SC (23.43-24.25)compared to their parental binary ones (22.26-22.74),while the YHD-SeNF-based ternary OSCs achieved the highest value.As a result, these ternary OSCs offered an impressive PCE of 18.2%-18.8%,which is much higher than their parental binary devices (~ 17%) (Fig. 2e).Notably, the PCE of 1 3 18.8% from the YHD-SeNF-based ternary devices is the highest value among the OSCs based on active layers processed from halogen-free solvents (Fig. 2i and Table S3) and spin-coating-free technologies (Fig. 2j and Table S4).Statistical photovoltaic data from 20 independent OSCs with different component ratios were summarized in Table S5-S14.As shown in Fig. 2f-h, the EQE measurements were carried out to verify the reliability of J SC values in OSCs.With the increase in YR-SeNF content in active layers, the OSCs show gradually broadened EQE spectra in NIR direction.The ternary OSCs based on PM6:L8-BO:YR-SeNF (1:0.8:0.4) with a small amount of YR-SeNF show significantly red-shifted response compared to the PM6:L8-BO-based ones but only slightly blue-shifted response in comparison with the PM6:YR-SeNF-based ones, may be due to good compatibility between L8-BO and YR-SeNF in which each component well-kept own photon absorption behavior (Figs.S16-S17).Moreover, ternary OSCs displayed higher EQE values from 400 to 900 nm compared to binary parental OSCs.Especially, ternary OSCs based on PM6:L8-BO:YR-SeNF (1:0.8:0.4)achieved much higher integrated J SC (27.1-27.6 mA cm −2 ) than these of binary OSCs based on PM6:L8-BO (24.7 mA cm −2 ) and PM6:YR-SeNF (25.8-26.7 mA cm −2 ), which are well consistent with the results from J-V curves.
As displayed in Fig. 2k, the operational stability of OSCs at MPP tracking was probed under a continuous illumination of 1-sun solar simulator to evaluate their practical application potential [52,53].The device based on ternary PM6:L8-BO:YHD-SeNF (1:0.8:0.4)displayed excellent stability and kept > 80% of initial PCE after the MPP tracking for even over 400 h, which is much better than its parental OSCs based on binary PM6:L8-BO.

Crystallinity, Morphological Properties, and Vertical Phase Distribution
As displayed in Fig. S22 and Table S15, the molecular crystallinity, orientation, and packing properties of binary L8-BO:YR-SeNF (1:0.2 and 0.8:0.4) were performed by using GIWAXS measurements [54][55][56].With the extension of N-alkyl size in YR-SeNF series, binary L8-BO:YR-SeNF achieve gradually increased π-π stacking distances in out-of-plane (OOP) direction, which is consistent with the YR-SeNF films.In IP direction, binary L8-BO:YR-SeNF shows two independent (100) diffraction peaks.With the increase in YR-SeNF content, these blends display the weakened (100) diffraction peaks of L8-BO but well-keep the ones from YR-SeNF.The above results suggest that YR-SeNF series are good compatible with L8-BO, where each component has its own aggregation behavior, and thus, morphology can be optimized by inserting YR-SeNF series as guest acceptors.
Atomic force microscopy (AFM) and transmission electron microscopy (TEM) measurements were carried out to study surface and bulk morphologies of blend films.As shown in Fig. S25, with the N-alkyl sized extension of YR-SeNF series, binary PM6:YR-SeNF blends show gradually decreased root-mean-square (RMS) roughness and reduced fiber size, which is consistent with their improved miscibility between them (Fig. S19).Ternary PM6:L8-BO:YR-SeNF blends show decreased RMS roughness as the content of YR-SeNF increases (Figs.S26-S28), which may be due to the fact that the RMS roughness of PM6:L8-BO (2.47 nm) is greater than that of PM6:YR-SeNF (~ 1.3 nm).As shown in Fig. 4c, ternary PM6:L8-BO:YR-SeNF (1:0.8:0.4)blends with uniform fiber structure have similar but gradually decreased RMS roughness from 1.44 to 1.35 nm as the N-alkyl sized extension of YR-SeNF series.In the TEM images (Fig. 4d), with the N-alkyl sized extension of YR-SeNF series, ternary PM6:L8-BO:YR-SeNF (1:0.8:0.4)blends also show gradually reduced phase separation in accordance with expectation.
Film-depth-dependent light absorption spectrometry (FLAS) was performed to study the effects of inserting guest YR-SeNF series on vertical phase distribution 1 3 between donor and acceptor components [57].As shown in Fig. 5a-d, all of blends show the same absorption peak positions of PM6 at ~ 620 nm throughout whole film, implying the similar molecular packing at different depths, which may help to minimize energetic disorder.By fitting the FLAS curves with the individual absorption of PM6, L8-BO, and YR-SeNF neat films, the composition ratios of active layer materials at different film-depths can be extracted (Fig. 5e-h).PM6:L8-BO:YR-SeNF ternary blends show more balanced vertical phase distribution between PM6 and L8-BO throughout the entire active layers compared to PM6:L8-BO one.Among these ternary blends, PM6:L8-BO:YHD-SeNF displays more uniform vertical phase distribution of guest acceptor, which may help to form smoother energy level gradient in OSCs and thus reduce V OC loss (Fig. 3b-d).As displayed in Fig. 5i-l, the exciton generation contour of OSCs was numerically simulated by combining the above FLAS information with an optical transfer matrix model.Compared to YBO-SeNFbased ternary blend, both ternary blends based on YHD-SeNF and YDT-SeNF yielded higher number of excitons from acceptors phase (800 nm), which partly explains their higher J SC values in OSCs.

Charge Transfer and Exciton Lifetimes
Femtosecond-resolved transient absorption spectra (fs-TAS) of neat films, binary acceptor blends, and ternary blends were measured to study the dynamics of photo-induced charge carriers by using a commonly used excitation fluence of 5 µJ cm −2 [58,59].According to the absorption spectra of PM6, L8-BO, and YR-SeNF series in neat films, the excitation wavelength selective for the acceptors was determined as 800 nm.The fs-TAS of L8-BO and YR-SeNF series in neat films and the related L8-BO:YR-SeNF (1:0.2 and 0.8:0.4)binary acceptor blends were first measured (Figs.S29-S31).The fs-TAS spectral line-cuts immediate after excitation (i.e., 0.5-1 ps) were chosen in the following discussion to represent the singlet excitons as characterized by ground state bleach (GSB) features similar to the absorption spectra (Fig. S16).As exhibited in Fig. 6a, e, i, the features at 670-690 nm are more dominated by L8-BO singlets while at 700-720 nm are more dominated by the singlets of YR-SeNF series, thereby used as the corresponding probe ranges in the following investigations.As shown in Fig. 6b-d, f-h, j-l, based on either range, the singlet exciton lifetime appears to increase upon blending of acceptors, which could be one of the reasons contributing to the higher J SC for ternary OSCs. Figure 6m summarizes the identified singlet excitons lifetime monitored of two wavelength ranges of 700-720 nm (more dominant contribution from L8-BO) and 670-690 nm (more dominant contribution from YR-SeNF series).With introducing appropriate amount of YR-SeNF as a guest acceptor, the resulting exciton lifetime of binary L8-BO:YR-SeNF can be prolonged when compared to either L8-BO or YR-SeNF neat films.Note that YR-SeNF series have red-shifted absorption that is more complementary with L8-BO, so adding more YR-SeNF tends to improve the utilization of solar spectrum.But if exciton lifetimes will be shorter, the advantage might be compensated at certain thresholds.Here, excitons of binary L8-BO:YR-SeNF (0.8:0.4) tend to maintain their lifetime or even slightly increase compared to those at neat films.Consequently, the J SC values of ternary OSCs are effectively enhanced.
As depicted in Figs.S32-S34, the fs-TAS of PM6:L8-BO:YR-SeNF ternary blends with different component ratios also were measured.Here, the wavelength range of 560-580 nm representing the dynamics of free charges on the basis of hole polarons was selected.As shown in Fig. 6n-p, the free charge generation kinetics based on the rise of photobleach appears similar for all the blend systems.Adding YBO-SeNF as guest acceptor clearly has negative impacts on sub-ns free charge recombination for all the investigated blend compositions, consequently slightly decreasing FF values can be observed in the related OSCs.Differently, the introduction of YHD-SeNF or YDT-SeNF as the guest component does not harm the sub-ns free charge recombination.In fact, with the appropriate amount of ternary blends can even slightly reduce the recombination rate (i.e., longer free charge lifetime), which is beneficial in charge transport, evident from their improved FF in OSCs as well [60].Combining with the enhanced photon harvesting, an impressively high PCE of approaching 19% was achieved in spin-coating-free and halogen-free solvent processed OSCs.

Conclusions
A series of newly designed YR-SeNF acceptors with similar NIR-absorption, different crystallinity, packing patterns, and miscibility with polymeric donor are developed.Introducing YR-SeNF guest acceptors associated with tailored N-alkyl chains into PM6:L8-BO host system well manipulate active layer morphologies, such as molecular packing, crystallinity, and vertical distribution, as well as improving charge transfer dynamics and stability in OSCs.As a result, the OSCs with excellent stability achieve a PCE approaching 19%, which is the highest value among OSCs with active layers processed from halogen-free solvents and/or spincoating-free technologies.As such, we believe that our strategy provides a feasible method to print eco-friendly, high-efficiency, and operating stable OSCs, which paves the way for industrial development.

Fig. 1 a
Fig. 1 a Molecular structures and design strategy of YR-SeNF series as guest acceptors used in the PM6:L8-BO host system.b, c Molecular structures of PM6 and L8-BO.d Line-cuts from GIWAXS profiles of the L8-BO and YR-SeNF series in neat films.e Absorption spectra and f energy levels of PM6, L8-BO, and YR-SeNF series

Fig. 2 a
Fig. 2 a Packing patterns of YR-SeNF series from MD simulation, where N-alkyl chains are omitted for clarity.b Geometries of YR-SeNF series.c Tetramer configuration cells of YR-SeNF series, where the numbers in Figures represent the closest distance between adjacent molecular backbones within a cell

Fig. 3 a
Fig. 3 a Device structure of the spin-coating-free OSCs in this work.b-d J-V plots of OSCs under the illumination of AM 1.5G, 100 mW cm 2 .e Comparison of PCEs in column chart form between the YR-SeNF-based binary and ternary OSCs.f-h EQE spectra of OSCs.Statistical PCE vs J SC of the OSCs based on active layers processed from i halogen-free solvents and j spin-coating-free technologies.k MPP tracking for the OSCs based on PM6:YHD-SeNF and PM6:L8-BO:YHD-SeNF under a solar simulator with 1-sun intensity

Fig. 5 a
Fig. 5 a-d Film-depth-dependent light absorption spectra, e-h composition distribution, and i-l exciton generation contour as a function of film depth for PM6:L8-BO and PM6:L8-BO:YR-SeNF (1:0.8:0.4)blend films, where depth 0 and 100 nm represent the active layer/PFN-Br and active layer/2PACz interfaces, respectively.For exciton generation contour, the incident light is from the ITO/2PACz side

Table 1
Photovoltaic parameters of the OSCs based on PM6:L8-BO:YR-SeNF with different weight ratios a The integrated J SC values were calculated from the EQE spectra