Open Access Article
J.
Price
,
B.
Balónová
,
B. A.
Blight
and
S.
Eisler
*
Department of Chemistry, University of New Brunswick, Fredericton, New Brunswick E3B 5A3, Canada. E-mail: seisler@unb.ca
First published on 11th August 2021
Predictable colour tuning in multicomponent photoluminescent (PL) systems is achieved using mixtures of simultaneously emitting organic molecules. By mitigating the potential for energy transfer through the control of concentration, the resulting emission chromaticity of five dichromic PL systems is approximated as a linear combination of the emitting components and their corresponding brightness (χi, ϕi, and Iex,i). Despite being limited to dilute solutions (10−6 M), colour tuning within these systems was controlled by (1) varying the composition of the components and (2) exploiting the differences in the components' excitation intensities at common wavelengths. Using this approach, white light emission (WLE) was realized using a pre-determined mixture of red, green, and blue emitting organic molecules. Based on these results, materials and devices with built-in or programmable emission colour can be achieved, including highly sought-after WLE.
The concept of additive colour-mixing is well established. Combining two or more colours in equal proportion and brightness results in a colour derived from a linear combination of the components.19 However, many multicomponent PL systems possess intra- or intermolecular energy transfer (ET) mechanisms such as Fluorescence Resonance Energy Transfer (FRET).11,13,14,20,21 Accounting for ET processes makes applying colour-mixing theory a challenge since ET differs from system to system. However, what if ET processes were mitigated or suppressed? Ingenious strategies to inhibit ET have been explored, including the use of micelles to spatially isolate PL emitters, leading to the simultaneous emission of each component.14,22 Since ET is distance-dependant, simply controlling the molecular concentration can decrease the possibility of ET, which would allow the resulting emission chromaticity to be approximated as a product of each PL component's emission colour and brightness.
Using the Commission Internationale de l'Eclairage (CIE) 1931 xyz colour-matching functions, the emission spectrum of a PL emitter can be converted into a set of numerical coordinates (x,y) that defines its colour.19 The brightness (a) of a PL emitter is loosely described as a product of (1) how strongly a PL molecule absorbs light at a given wavelength (ε = Acl) and (2) how much of that absorbed light is subsequently emitted (ϕPL).23 Alternatively, one can also describe how strongly a PL molecule absorbs light at a given wavelength by substituting absorption intensity (A) for excitation intensity (Iex). Whereas the absorption intensity is measured as the logarithmic fraction of incident and transmitted light, the signal intensity (counts per second) in the excitation spectrum is directly proportional to the number of photons that are absorbed and emitted. Using excitation intensity (Iex) as a metric to quantify brightness has added benefits such as eliminating the need for a UV-vis spectrophotometer and the advantage of using lower sample concentrations due to the inherent sensitivity of fluorescence spectroscopy. For these reasons, excitation intensity (Iex) can serve as a more useful metric for quantifying molecular brightness.
In the absence of ET processes, we propose that the emission chromaticity of a multicomponent PL system can be approximated as a linear combination of each PL component's CIE coordinates (x,y) and their respective contribution or relative brightness (ai) (eqn (1)). Herein, we define each component's contribution or relative brightness (ai) as the product of the ith components mole fraction (χi), photoluminescent quantum yield (ϕi), and excitation intensity (Iex,i) at a common wavelength (eqn (2)).
| (xmix, ymix) = a1(x1, y1) + a2(x2, y2) +⋯+ ai(xi,yi) | (1) |
![]() | (2) |
To test whether the emission chromaticity of a multicomponent PL system can be described as a linear combination of its components, various commercially available PL emitters including perylene, coumarin 6 (C6), N,N′-bis(3-pentyl)perylene-3,4,9,10-bis(dicarboximide) (PDI), Rhodamine 6G (R6G), and Nile Red (NR) were chosen and subsequently evaluated. Equimolar solutions of each emitter in chloroform (c = 1.2 × 10−6 M) were prepared, and both emission and excitation profiles were obtained at room temperature (Fig. 1a and b; S2–S11, ESI†). The emission maximum (Table 1) of each emitter was identified and then used to record the corresponding emitter's excitation spectrum (p. S3, ESI†).
| PL emitter | λ em (nm) | ϕ PL | CIE (x,y) | Entry | I ex (cps) | |||||
|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 2 | 3 | 4 | 5 | 6 | |||||
| λ ex 333 nm | λ ex 347 nm | λ ex 356 nm | λ ex 358 nm | λ ex 378 nm | λ ex 389 nm | |||||
| a Reported solution data was measured in aerated chloroform (c = 1.2 × 10−6 M) at room temperature. CIE coordinates (x,y) were extracted from the emission profiles using the Fluoracle® software package. b Absolute photoluminescence quantum yields (ϕPL) were obtained using an Edinburgh FS5 spectrofluorometer equipped with an SC-30 integrating sphere. | ||||||||||
| Perylene | 443 | 0.92 | 0.14, 0.09 | 38 170 |
40 840 |
92 770 |
92 900 |
— | 54 310 |
|
| C6 | 491 | 0.92 | 0.19, 0.53 | 35 630 |
— | — | — | 70 342 |
14 860 |
|
| PDI | 534 | 0.67 | 0.37, 0.61 | — | — | — | 92 670 |
76 520 |
— | |
| R6G | 552 | 1 | 0.42, 0.57 | — | — | 100 800 |
— | — | — | |
| NR | 597 | 0.91 | 0.60, 0.39 | — | 39 300 |
— | — | — | — | |
We then compared each PL components' excitation intensity (Iex) at common wavelengths (Table 1, entries 1–6) within a given system. Consequently, this allowed us to scale each PL component's contribution or relative brightness (eqn (2)) with respect to any excitation wavelength (λex) that is used to excite the system. However, for our initial experiments, an excitation wavelength for each system was chosen such that each emitter shared approximately the same excitation intensity (Iex)—corresponding to the region where the excitation spectra overlap for each respective system (Fig. 1b). Since the excitation intensities for each component were approximately the same (Table 1, entries 1–5), we expected that any observed difference in emission chromaticity would largely depend on the differences in quantum yields and mole fractions of each PL component.
:
χ2 = 1
:
0, 0.75
:
0.25, 0.50
:
0.50, 0.25
:
0.75, 0
:
1) of five different dichromic systems (perylene–C6, perylene–PDI, perylene–R6G, perylene–NR, and PDI–C6) and measured their emission spectra. A total molecular concentration of 1.2 × 10−6 M was chosen to suppress the efficiency of any potential ET processes occurring in solution, such as FRET, which can occur up to 100 angstroms.24 As a result, the average distance between molecules can be approximated to be greater than 1000 angstroms for our studies (Fig. S1, ESI†). By selecting an excitation wavelength (λex) in which each component had similar excitation intensities (Iex), the differences in the measured emission chromaticity were shown to be linearly proportional to the mole fraction (χ) and PLQY (ϕPL) of each component (R2 > 0.98; Fig. S12–S30, ESI†). The experimentally determined CIE coordinates were then compared to the predicted results obtained using eqn (1) (Tables S1–S7, ESI†). To measure the accuracy of the approximation, absolute errors were quantified based on the distance between the measured and predicted CIE coordinates. For all five dichromic PL systems that were explored in this study, the distance between the measured and predicted CIE coordinates never exceeded 0.02 au, which demonstrates that emission chromaticity within these systems can be accurately described as a linear combination of each PL component (Fig. 2a; Tables S1–S7, ESI†). Based on this result, dichromic PL systems can be used to design emissive materials with any desired chromaticity (x,y), given that it traverses the line between each component by simply adjusting the mole fractions (χ) of the PL components.
A linear relationship between excitation wavelength and the emission CIE coordinates of homometallic Ln(III)-complexes has previously been established.17 By varying the excitation wavelength, each component's contribution to the overall chromaticity can be controlled due to their differences in excitation intensity. Therefore, we wanted to show that by accounting for the relative differences in excitation intensities of each PL component, the emission chromaticity resulting from excitation at any wavelength can still be approximated as a linear combination of each emitter. To demonstrate this, the mixtures of perylene and C6 that were excited at 333 nm (Iex,perylene ≅ Iex,C6; Table 1, entry 1), shown in Fig. 2a–c, were excited at 389 nm (Iex,perylene ≠ Iex,C6; Table 1, entry 6) for comparison.
At λex = 333 nm, perylene and C6 have approximately the same excitation intensities (Table 1, entry 1), and therefore the emission chromaticity is shown to be primarily dependent on the differences in mole fractions and PLQYs of each emitter (Fig. 2a–c, S13 and S14, ESI†). In comparison, when the same mixtures of perylene and C6 are excited at 389 nm, a blue shift is observed in the emission chromaticity that is proportional to the difference in the excitation intensities of perylene and C6 (Table 1, entry 6; Fig. 3a, b and S15, S16, ESI†). Good agreement between the measured and predicted CIE coordinates (abs. error < 0.01 au; Tables S1 and S2, ESI†) was obtained by accounting for the different excitation intensities, mole fractions, and PLQYs of perylene and C6. Based on these results, not only is PLCT possible but any desired emission chromaticity that traverses the 1D-line between two PL components can be targeted by (1) adjusting the mole fractions of the components or (2) strategic selection of an excitation wavelength.
![]() | ||
Fig. 4 (a) Overlaid excitation profiles of perylene and R6G in chloroform (c = 1.2 × 10−6 M) showing the region of interest. (b) Perylene–R6G emission profiles in chloroform (c = 1.2 × 10−6 M) obtained at various excitation wavelengths (347–367 nm, 2 nm intervals) and (c) the corresponding CIE diagram showing the measured (●) and predicted (○) CIE coordinates. Relative excitation intensities of perylene and R6G were calculated using the intensities shown in Table S6, ESI.† | ||
By treating the ideal WLE coordinates as a barycenter, we calculated the normalized contributions of perylene (a1 = 0.34), C6 (a2 = 0.28), and NR (a3 = 0.38) that are required to achieve WLE (Fig. S34; eqn (S3)–(S7), ESI†). Subsequently, an excitation wavelength was chosen wherein each PL component had comparatively high intensities (λex = 274 nm; Iex,perylene = 99
590 cps, Iex,C6 = 130
500 cps, and Iex,NR = 137
900 cps; Fig. S35, ESI†). However, it should be noted that any excitation wavelength in which each PL component has a non-zero intensity could have been chosen. Next, we determined the necessary mole fractions of perylene (χperylene = 0.41), C6 (χC6 = 0.26), and NR (χNR = 0.33) by selecting an arbitrary concentration of perylene and calculating the corresponding concentrations of C6 and NR needed to satisfy their contribution requirements (p. S28, ESI†). We then acquired the emission spectrum of a mixture of perylene–C6–NR (0.41
:
0.26
:
0.33) in chloroform, and as expected, the mixture's emission spectrum spanned the entire visible region and consisted of each emitter's characteristic emission profile (Fig. 5a). Moreover, the CIE coordinate (0.33,0.34) resulting from exciting the mixture at 274 nm was exceptionally close (<0.01 au) to the ideal WLE coordinate (0.33,0.33) that was targeted (Fig. 5b).
![]() | ||
Fig. 5 (a) The emission spectrum (λex = 274 nm) of the perylene–C6–NR mixture (χperylene : χC6 : χNR = 0.41 : 0.26 : 0.33) in chloroform (c = 1.2 × 10−6 M) and (b) the corresponding CIE diagram showing the measured (●) and targeted (○) CIE coordinates. The inset showing the WLE produced by the perylene–C6–NR mixture was irradiated at 365 nm using a TLC lamp.27 | ||
Footnote |
| † Electronic supplementary information (ESI) available. See DOI: 10.1039/d1sc03447b |
| This journal is © The Royal Society of Chemistry 2021 |