Dian Luoa,
Chung-Tsung Hsieha,
Yen-Po Wanga,
Thomas C. Chuangb,
Hsin-Hua Changc and
Chih-Hao Chang*a
aDepartment of Electrical Engineering, Yuan Ze University, Chung-Li, Taiwan 32003. E-mail: chc@saturn.yzu.edu.tw; Fax: +886 34638800 ext. 7517; Tel: +886 34514281
bDepartment of Information Science and Technology, Vanung University, Chung-Li, Taiwan 32061
cDepartment of Aeronautical and Opto-Mechatronic Engineering, Vanung University, Chung-Li, Taiwan 32061
First published on 30th August 2018
An exciplex could be formed by blending a selected hole-transporting material (HTM)/electron-transporting material (ETM) pair, and the corresponding energy band gap is roughly determined by the energy difference between the lowest unoccupied molecular orbital (LUMO) of the ETM and the highest occupied molecular orbital (HOMO) of the HTM. In this study, three HTM/ETM combinations are adopted to generate blue, green, and red exciplexes, allowing us to design precise device architectures for the fabrication of exciplex-based white OLEDs (WOLEDs) with daylight-like emissions. The CIE coordinates of this WOLED varied close to the Planckian locus as the biases increase, with a high color rendering index of about 96. This high performance suggests this exciplex-based WOLED can provide high-quality white-light illumination. Photoluminance and lifetime measurements of the exciplex behavior of the HTM/ETM combinations indicate that the HTM and ETM selected should possess higher triplet energy bandgaps than those of their corresponding exciplex to avoid energy loss.
The exciplex could be easily formed by applying commercially available materials.10,11 Exciplex-based OLEDs can also be very efficient given appropriate HTM and ETM in the emitting layer (EML). In general, an exciplex could be generated using a bilayer structure with both HTM and ETM or by directly mixing an HTM and an ETM. The latter typically results in greater exciplex production yields. In principle, since the exciplex energy band gap is determined by the energy-level difference, the energy band gap could be adjusted by choosing appropriate materials. For instance, the energy band gap could be determined by the energy difference between the lowest unoccupied molecular orbital (LUMO) of the ETM and the highest occupied molecular orbital (HOMO) of the HTM.7–13
OLEDs which can effectively imitate daylight would be of particular use in high-latitude areas where sunlight exposure is highly seasonal.14–16 In 2009, Jou et al. proposed a sunlight-style OLED with a correlated color temperature (CCT) tunable from 2300 to 12000 K, proving the possibility of fabricating a new low color temperature light source.17 In 2013, the same group reported OLEDs with a candle light-style yellowish orange chromaticity with a power efficiency of 29 lm W−1 at 100 cd m−2, a respective color rendering index (CRI) of 87 and a CCT of 2050 K.18 The fabricated device minimized potential harmful effects of excessive blue emission on the human eye. In 2014, they demonstrated the feasibility of creating indoor sunset hues using a dusk-light-style OLED that exhibits a CCT ranging between 1500 and 3000 K.19 The artificial dusk hue shows a 92 color rendering index at 2745 K with an 87% luminance spectrum resemblance with the sunset hue. However, all these devices used the host–guest system in the EML, which not only requires expensive molecular emitters but also suffers from different rates of degradation of the emitters. Herein, we propose a pure exciplex-based white OLED (WOLED) with a delicate device architecture design which can generate emissions that approximate daylight, where the WOLED emission color closely tracks the Planckian locus.20,21
On the other hand, to imitate daylight emissions, the main carrier recombination zone was set at the red EML, producing an intense red emission at lower biases. In addition, a proper device architecture design will allow the carrier recombination zone to progressively extend to the green and blue EMLs as the forward bias increases. Hence, one could expect that the emission color of OLEDs might vary from red to white. Furthermore, a wide energy bandgap material, 2,6-bis(3-(9H-carbazol-9-yl)phenyl)pyridine (26DCzppy),27 with bipolar transport capability was inserted between the green and red EMLs to ensure the recombination zone formed at the red EML at a lower bias. This buffer layer could help adjust the carrier transport and the exciton diffusion.28
Two kinds of exciplex-based WOLEDs are examined. Device A with double EMLs is configured as ITO (120 nm)/TCTA (40 nm)/TCTA 50 wt%:
BP4mPy 50 wt% (29 nm)/26DCzPPy (3 nm)/m-MTDATA 10 wt%
:
B3PyMPM 90 wt% (3 nm)/TmPyPB (50 nm)/LiF (0.8 nm)/Al (150 nm), for which LiF and aluminum are respectively used as the electron injection layer and reflective cathode. The first EML consisting of TCTA 50 wt%
:
BP4mPy 50 wt% is responsible for the blue emission, while the second EML for the red light was set as m-MTDATA 10 wt%
:
B3PyMPM 90 wt%. Moreover, the mixing ratio of the aforementioned exciplex-based EMLs were fine-tuned to generate an appropriate white light emission. The device architecture of devices B1 and B2 with triple EMLs consisted of ITO (120 nm)/TCTA (40 nm)/TCTA 50 wt%
:
BP4mPy 50 wt% (29 nm)/m-MTDATA 80 wt%
:
TmPyPB 20 wt% (x nm)/26DCzPPy (3 nm)/m-MTDATA 10 wt%
:
B3PyMPM 90 wt% (3 nm)/TmPyPB (50 nm)/LiF (0.8 nm)/Al (150 nm). Compared to the architecture of device A, a green EML consisting of m-MTDATA 80 wt%
:
TmPyPB 20 wt% was inserted into the device next to the blue EMLs to improve the color rendering capability of the WOLEDs.29 The thicknesses of the green EMLs were varied to adjust the emission colors, e.g., 1 nm for device B1 and 3 nm for the second set of device B2. The corresponding chemical structures of the materials and the schematic structure of the device architectures are depicted in Fig. 1.
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Fig. 1 (a) Chemical structures of the materials; (b) the schematic structure of the device architectures. |
Fig. 2 shows the normalized EL spectra and the corresponding CIE coordinates of the tested exciplex-based OLEDs under different biases. From Fig. 2(a), device A exhibited a strong red emission at the lower biases and the blue emission peaks around 440 nm, which increased with the bias.30 However, the blue component was still much weaker than the red one even at higher voltages, resulting in device A's emission presenting a pinkish white color (cf. CIE coordinates shown in Fig. 2(d)). On the other hand, the EL spectra of both B1 and B2 showed three peaks with satisfactory emission color. The wavelengths of the deep-blue, sky-blue, and red emission peaks were respectively recorded at 385 nm, 462 nm, and 652 nm. Although devices B1 and B2 presented similarly intense red emissions at lower biases, and the emissions ranging from blue to green region gradually increased with voltage, the intensity of the emission ranging blue to green rose significantly at higher voltages, as shown in Fig. 2(b) and (c). Furthermore, the CIE coordinates of both devices B1 and B2 displayed pure white emission at higher biases. The varied emission of device B2 was close to the Planckian locus as the biases increased, indicating the sophisticated design of device B2. In addition, device B2 exhibited high CRI values of about 96 in a wide luminance range from 100 to 1000 cd m−2, corresponding to the CCT between 4359 and 7115 K. The numeric data collected from the EL spectra of device B2 are summarized in Table 1. We also included the corresponding data of devices A and B1 in Table S1 in ESI† for comparison. It's notable that the CRI value of device B2 reached the highest level compared to the previous reports.18 These performances demonstrate that this exciplex-based WOLED (i.e. B2) possessed a high-quality white-light illumination.28,31–35
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Fig. 2 EL spectra of the tested exciplex-based white OLEDs with different operating voltages. (a) Device A; (b) device B1; (c) device B2; (d) CIE coordinates. |
Voltage (V) | Luminance (cd m−2) | CIE coordinates (x, y) | CCT (K) | CRI |
---|---|---|---|---|
6 | 1.76 | 0.533, 0.433 | 2071 | 70.20 |
7 | 5.41 | 0.497, 0.429 | 2364 | 75.66 |
8 | 15.13 | 0.456, 0.412 | 2762 | 81.05 |
9 | 36.37 | 0.421, 0.393 | 3201 | 85.77 |
10 | 79.99 | 0.388, 0.372 | 3744 | 89.71 |
11 | 168.75 | 0.363, 0.354 | 4359 | 92.80 |
12 | 302.37 | 0.341, 0.336 | 5162 | 95.06 |
13 | 493.91 | 0.323, 0.320 | 5998 | 96.07 |
14 | 720.35 | 0.309, 0.308 | 6972 | 96.05 |
15 | 914.58 | 0.306, 0.307 | 7115 | 95.69 |
Fig. 3 shows the schematic energy level diagram of the tested OLEDs. Given the large barrier at the B3PyMPM/26DCzPPy interface, the hole injection was smoother than the electron injection in device A. As indicated, the red component dominated the EL emission even as the voltage increased. In addition, abundant hole injection reinforced the carrier recombination occurring in m-MTDATA:
B3PyMPM layer, increasing the possibility of exciton formation on m-MTDATA molecules. The blue emission peak around 430 nm should originate from m-MTDATA, which could be confirmed by the PL spectrum and will be discussed later (cf. Fig. 5(a)). Consequently, the original setting of blue EML (i.e. TCTA
:
BP4mPy) in device A was useless. In contrast, for the green EML inserted into devices B1 and B2, the hole would be partially trapped because of the low HOMO level of m-MTDATA, enabling appropriate adjustment of hole injection into the red EML. Thus, the electron could be transported to the green and blue EMLs and then recombine at higher voltages, creating much stronger green and blue emissions. Furthermore, by increasing the thickness of the green EML, the emission of device B2 could be adjusted to present a pure white color. As indicated, the corresponding CIE coordinates of device B2 vary along the Planckian locus as the biases increase.
Fig. 4 and S1† respectively depict the current density–voltage–luminance (J–V–L) curves and efficiency curves. From Fig. 4(a), as expected, devices B1 and B2 possesses additional green EML, showing lower current densities.36 In addition, the current density decreased as the thicknesses of the green EML increased. In contrast, the luminance of device B2 exhibited a higher maximum luminance than the other devices, due to human eye to green.37 The efficiency curves shown in Fig. 4(b) and S1† clearly indicate that a higher carrier balance could be obtained in device B2. The peak external quantum efficiency, luminance efficiency and power efficiency of device B2 were respectively 1.5%, 2.7 cd A−1, and 2.0 lm W−1. This WOLED efficiency was produced using commercially available materials to generate the exciplex. Although the efficiency was much lower than other state-of-art devices, this article focuses on the design of a feasible device architecture for exciplex-based WOLEDs to imitate daylight emissions. Moreover, device efficiency is expected to improve further by replacing the potential HTM/ETM combinations to achieving efficient increased efficiency as well the exciplex emissions.6,8,9,11,12,21
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Fig. 4 EL characteristics of the tested exciplex-based white OLEDs: (a) current density–voltage–luminance characteristics, (b) luminance efficiency vs. luminance of devices A, B1, and B2. |
Fig. 5(c) shows the excited state decay characteristics of the materials in toluene solution. All materials exhibited typical fluorescent decay behavior. On the other hand, the curves exhibited in Fig. 5(d) clearly indicate that samples G and R possess two-component decay including a nanosecond-scale prompt and sub-microsecond-scale delayed components, while sample B had only a nanosecond-scale component. The delayed lifetimes for samples G and R were respectively estimated at 105.1 and 175.7 ns due to the slower reverse intersystem crossing processes from the T1 back to the S1 excited state.40 Moreover, the respective lifetime values of samples B, G, and R were estimated to be 5.3, 27.5, and 28.2 ns attributed to representative fluorescence decay.
From Fig. 5(b) and (d), sample B seems to exhibit the behavior typical of a fluorescent emitter. However, sample B shows a red-shifted spectrum compared to the fluorescence of TCTA and BP4mPy, suggesting that the emission origin of sample B is different from the S1 of TCTA or BP4mPy. Consequently, the phosphorescence of TCTA, BP4mPy, and sample B were measured in 77 K, as shown in Fig. 6(a). Both TCTA and BP4mPy possessed lower triplet energy bandgaps than that of sample B (i.e., TCTA:
BP4mpy mixture). The triplet energy bandgaps of TCTA, BP4mPy, and sample B were evaluated based on the onset of the phosphorescent spectra and were respectively estimated to be 2.92, 2.94, and 3.31 eV. In addition, the phosphorescence of sample B was slightly red-shifted compared to the fluorescence. The small energy difference between the single and triplet excited states (ΔEST ∼0.1 eV) confirmed that the emission originated from the exciplex.7,9,39 Therefore, the related lower T1 states of TCTA and BP4mPy would offer pathways for exothermic energy transfer, leading to energy loss and thus a shorter lifetime for sample B. The photophysical properties of the used materials and the thin-film samples were summarized in Table 2. Furthermore, we measured the phosphorescence of sample B with different delay times, as shown in Fig. 6(b). The phosphorescence of exciplex gradually decayed with the extending delay time, while additional emissions appeared consisting of peaks similar to the BP4mPy's phosphorescence. These additional emissions could be seen as direct evidence of exothermic energy transfer. This was the first demonstration of the assumption indicating that the selected HTM and ETM should possess higher triplet energy bandgaps than those of their corresponding exciplex to avoid energy loss to the composed single molecules.41 Fig. 6(c) shows a schematic diagram of the energy transfers in samples B and R.
Materials | λmax. (nm) | FWHM (nm) | S1a (eV) | T1 (eV) | Lifetime | |
---|---|---|---|---|---|---|
Prompt (ns) | Decay (ns) | |||||
a Estimated from the onset of the fluorescent spectrum.b Evaluated from the onset of the phosphorescent spectrum.c Collected from the previous reports (ref. 17, 20 and 21). | ||||||
TCTA | 385 | 42 | 3.42 | 2.92b | 1.9 | n.d. |
BP4mPy | 351 | 37 | 3.77 | 2.94b | 10.6 | n.d. |
m-MTDATA | 424 | 46 | 3.11 | 2.65c | 1.8 | n.d. |
TmPyPB | 349 | 38 | 3.29 | 2.75c | 11.3 | n.d. |
B3PyMPM | 343 | 45 | 4.01 | 2.70c | 2.6 | n.d. |
TCTA![]() ![]() ![]() ![]() |
399 | 56 | 3.41 | 3.31b | 5.3 | n.d. |
m-MTDATA![]() ![]() ![]() ![]() |
483 | 106 | 3.08 | 3.03b | 27.5 | 105.1 |
m-MTDATA![]() ![]() ![]() ![]() |
616 | 142 | 2.37 | 2.36b | 28.2 | 175.7 |
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c8ra04986f |
This journal is © The Royal Society of Chemistry 2018 |