Rami
Shafei
ad,
Philipp Jean
Strobel
c,
Peter J.
Schmidt
c,
Dimitrios
Maganas
*a,
Wolfgang
Schnick
*b and
Frank
Neese
*a
aMax-Planck-Institut für Kohlenforschung, Kaiser-Wilhelm-Platz 1, 45470 Mülheim an der Ruhr, Germany. E-mail: neese@kofo.mpg.de
bDepartment of Chemistry, University of Munich (LMU), Butenandtstraße 5-13, 81377 München, Germany
cLumileds Phosphor Center Aachen, Lumileds Germany GmbH, Philipsstraße 8, 52068 Aachen, Germany
dDepartment of Chemistry, Faculty of Science, Beni-Suef University, Salah Salem Str., 62511 Beni-Suef, Egypt
First published on 18th January 2024
We have previously presented a computational protocol that is based on an embedded cluster model and operates in the framework of TD-DFT in conjunction with the excited state dynamics (ESD) approach. The protocol is able to predict the experimental absorption and emission spectral shapes of Eu2+-doped phosphors. In this work, the applicability domain of the above protocol is expanded to Eu2+-doped phosphors bearing multiple candidate Eu doping centers. It will be demonstrated that this protocol provides full control of the parameter space that describes the emission process. The stability of Eu doping at various centers is explored through local energy decomposition (LED) analysis of DLPNO-CCSD(T) energies. This enables further development of the understanding of the electronic structure of the targeted phosphors, the diverse interactions between Eu and the local environment, and their impact on Eu doping probability, and control of the emission properties. Hence, it can be employed to systematically improve deficiencies of existing phosphor materials, defined by the presence of various intensity emission bands at undesired frequencies, towards classes of candidate Eu2+-doped phosphors with desired narrow band red emission. For this purpose, the chosen study set consists of three UCr4C4-based narrow-band phosphors, namely the known alkali lithosilicates RbNa[Li3SiO4]2:Eu2+ (RNLSO2), RbNa3[Li3SiO4]4:Eu2+ (RNLSO) and their isotypic nitridolithoaluminate phosphors consisting of CaBa[LiAl3N4]2:Eu2+ (CBLA2) and the proposed Ca3Ba[LiAl3N4]4:Eu2+ (CBLA), respectively. The theoretical analysis presented in this work led us to propose a modification of the CBLA2 phosphor that should have improved and unprecedented narrow band red emission properties. Finally, we believe that the analysis presented here is important for the future rational design of novel Eu2+-doped phosphor materials, with a wide range of applications in science and technology.
Despite this progress, achieving luminescence tunability in many promising phosphor materials remains a challenging task, especially for narrow band emitting phosphors with rigid structures coupled with limited geometrical flexibility of the activator site, e.g., in solid solution phosphors. In addition, one of the main difficulties lies in the observation of multiple emission signals, which adversely affect their brightness, efficiency, and applicability.14,32–36,38 This is in particular the case with an increasing number of recently synthesized red emitting phosphors, bearing Eu2,3+, Ce3+ and Mn4+ doping ions in a variety of host structures.38–40 In this concept, successful applications are mainly based on empirical observations and trial and error implying the urgent need for gaining electronic structure knowledge of these kind of systems.
In general, activated phosphors show systematic geometric and electronic structural properties.4,21,24,25,41–45 In this framework, we have recently shown the importance of constructing carefully calibrated theoretical spectroscopy protocols.1 In fact, protocols that are constructed on a systematic basis by combining methods that belong to the density functional theory (DFT) and wavefunction theory (WFT) arsenals have been proven instrumental in defining general descriptors that are able to connect (1) the band gap energy of the Eu2+-doped phosphor and (2) the covalency of the Eu-5d donor orbital involved in the emission process, with the color and the linewidth of the emission band. The availability of such descriptors is of paramount importance as they can be applied as a predictive tool of photoluminescence properties of novel phosphors or to cross-correlate and further validate a large amount of available data that are based on DFT computations,21,24,25,42,43,46–49 machine learning data analysis20,50 or empirical correlations50 towards a systematic design of novel phosphor materials with tailored photoluminescence properties.
To control and optimize the emission properties of Eu2+-doped phosphors, precise management of crystal and ligand field effects within the local environment of the doping center is essential. Various strategies have been proposed, including altering the central metal ions. This approach has demonstrated notable advancements in red-emitting phosphors, such as the transition from the Ca[LiAl3N4]:Eu2+,51 (CLA:Eu2+) to Sr[LiAl3N4]:Eu2+,23 (SLA:Eu2+) structures in lithoaluminate phosphors. However, it can also introduce drawbacks, as observed with the outlier Ba[Mg3SiN4]Eu2+,22 (BMS:Eu2+) compared to Sr[Mg3SiN4]Eu2+,26 (SMS:Eu2+) in magnesosilicate phosphors.
Besides the local electronic structure nature of the emissive center, the role of the rigidity of the host environment in terms of its availability for doping, the imposed coordination environment around the doped emissive centers, and the way this influences the phosphor's photoluminescence properties have recently attracted attention. Hence, another versatile approach involves utilizing hosts with multiple doping centers, which offers enhanced diversity and improved control over the structural and electronic properties.38,52–54 This approach opens new avenues for investigating and optimizing the emission properties of Eu-doped phosphors, ultimately leading to improved performance. In systems with multiple potential doping centers, aspects like the volume of the doping coordination region,3 the probability of doping and the vibronic coupling of the rigid host structure55–58 have been successfully employed to interpret the studied phosphor emission properties. In particular, they have been employed to provide insight over the nature of the emission band in room and low temperature spectra of RbNa[Li3SiO4]2:Eu2+55 and Sr[LiAl3N4]:Eu2+
58 or to understand the relationship of the host environment to the heat induced blue shift (HIB) phenomenon in Eu2+-doped phosphors.59
With all these considerations in mind, in this work, we aim to present a systematic computational protocol that is strongly intertwined with experimental data and leads our experimental efforts towards the design of novel phosphor materials with desired photoluminescence properties. In particular, we will present the key chemical steps that are required to improve the photoluminescence properties of the well-known CaBa[LiAl3N4]2:Eu2+ (CBLA2)38 red phosphor towards the structural prediction of the yet unknown, Ca3Ba[LiAl3N4]4:Eu2+ (CBLA), Eu2+-doped phosphor that computationally exhibits unprecedented narrow-band red emission properties. For this purpose, we will expand the family of chemical systems that can be treated with the above-described protocol by including a set of phosphors bearing multiple candidate centers for Eu2+ doping. Hence besides the known CBLA2 and the target CBLA phosphor, the chosen study set consists of UCr4C4-based narrow-band phosphors, namely the alkali lithosilicates RbNa3[Li3SiO4]4:Eu2+ (RNLSO)52 and RbNa[Li3SiO4]2:Eu2+ (RNLSO2)53 as well as, the isotypical to RNLSO2, nitridolithoaluminate CaBa[LiAl3N4]2:Eu2+ (CBLA2).38 It is demonstrated that the electronic structure of the known CBLA2, RNLSO, and RNLSO2 is understood, and the isotypic to RNLSO, CBLA Eu2+-doped phosphor fulfils the requirements for narrow band red emission.
In Fig. 1, the probable cation sites for Eu2+ doping are highlighted. The selection of the doping sites is based on (1) the similarity of their ionic radii (r) to Eu2+60 and (2) their suitability for Eu2+ doping in a host environment that minimizes the steric effects.3 In fact, as seen in Table 1, Eu2+ doping with Ca2+ and Na+ is expected to form strained EuL8 (L is N3−/O2−) cuboids with rCa2+–Eu2+ = −0.19 Å and rNa+–Eu2+ = −0.07 Å and EuL8 cuboid volume that varies between 29.5 Å3 and 30.1 Å3. In contrast, Eu2+ doping at Ba2+ and Rb+ is expected to form rather relaxed EuL8 cuboids with rBa2+–Eu2+ = 0.10 Å and rRb+–Eu2+ = 0.36 Å and EuL8 cuboid volume that varies between 37.6 Å3 and 40.5 Å3. In particular, the Eu2+-doped CBLA2 phosphor has two candidate doping centers at Ca2+ and Ba2+ positions. RNLSO phosphor has three candidate doping centers at Na(1)+, Na(2)+ and Rb+ positions. Finally, RNLSO2 phosphor has two candidate doping centers at Na+ and Rb+ positions.
Phosphor | Doping site (Mm+) | Ionic radii (r) (Å)60 | ΔrMm+–Eu2+ (Å) | Average M–L bond distance (Å) | Volume of ML8 cuboid (Å3) | First shell cations | ΔEfd (eV) | ΔELF (eV) |
---|---|---|---|---|---|---|---|---|
CaBa[LiAl3N4]2:Eu2+ CBLA2 | Ba2+ | 1.35 | 0.10 | 2.90 | 37.60 | [Li4Al4]16+ | 3.08 | 2.17 |
Ca2+ | 1.06 | −0.19 | 2.70 | 29.50 | [Al8]24+ | 1.06 | 4.63 | |
RbNa3[Li3SiO4]4:Eu2+ RNLSO | Rb+ | 1.61 | 0.36 | 3.00 | 40.00 | [Li8]8+ | 4.16 | 1.60 |
Na(1)+ | 1.18 | −0.07 | 2.70 | 30.17 | [Li8]8+ | 2.94 | 3.06 | |
Na(2)+ | 1.18 | −0.07 | 2.60 | 30.61 | [Li4Si4]20+ | 2.42 | 3.60 | |
RbNa[Li3SiO4]2:Eu2+ RNLSO2 | Rb+ | 1.61 | 0.36 | 3.00 | 40.50 | [Li4Si4]20+ | 3.03 | 2.02 |
Na+ | 1.18 | −0.07 | 2.60 | 29.45 | [Li8]8+ | 2.38 | 3.68 |
As shown in Fig. 1, CBLA2 is isotypic to RNLSO2, hence Eu2+ doping at Ca2+ and Ba2+ centers form compressed and elongated EuN8 cuboids of C2h symmetry with average bonding or interatomic distances of (Ca/Eu)–N 2.65–2.75 Å and (Eu/Ca)–Ca 3.30 Å while (Eu/Ba)–N 2.83–2.96 Å and (Eu/Ba)–Ba is 3.31 Å. These cuboids deviatefrom the ‘ideal’ D4h symmetry by only 1–2%. In the case of RNLSO, Eu2+ doping at Na(1)+ or Rb+ centers forms compressed and elongated EuO8 cuboids with C2h symmetry, respectively, with an average bond distance of (Na(1)/Eu)–O ∼ 2.71 Å and (Rb/Eu)–O ∼ 3.01 Å. In contrast, Eu2+ doping at Na(2)+ centers forms compressed cuboids with D2d symmetry with (Na(2)/Eu)–O 2.45–2.75 Å. Similarly, in the case of RNLSO2 Eu2+ doping at Na(1)+ or Rb+ centers form compressed and elongated EuO8 cuboids of C2h symmetry, respectively, with an average bond distance of (Na/Eu)–O 2.55 Å and (Rb/Eu)–O 3.00 Å.
In particular, CBLA2:Eu2+, upon excitation with a 444 nm laser, exhibits an intense, narrow red emission band at 639–636 nm (15650–15
723 cm−1) with FWHM 48–57 nm (∼1095–1266 cm−1) and a weak broad infrared (IR) emission band at 790 nm (12
660 cm−1) and FWHM ∼89 nm (∼1430 cm−1). The intensity of the later band improves with increasing Eu2+ doping concentration. The two bands have been assigned to emission from Eu2+-doped centers at Ba2+ and Ca2+ positions, respectively.38 In contrast, RNLSO:Eu2+ upon excitation with a 400 nm laser exhibits a single narrow blue emission band at 471 nm (21
230 cm−1) with a FWHM of 22.5 nm (∼1015 cm−1).52 In the case of RNLSO2, two bands show up when a variety of excitation lasers in the 400 nm region is employed.53 A high intensity narrow green emission band appears at 523 nm (19
120 cm−1) with a FWHM of 40 nm (∼1465 cm−1). A second weaker intensity cyan emission band occurs at higher energies (472 nm, 21
185 cm−1). These bands have been ascribed to Eu2+-doped centers at Na+ and Rb+ positions, respectively, while it has been shown that their relative intensity varies with the Eu2+ doping concentration at the Na+ and Rb+ positions.52,55
As seen in Fig. 2, the study set of phosphors lies between the absorption and emission characteristics of two well-known narrow band phosphors, namely the red emitting nitride SLA:Eu2+23 and the blue emitting oxide SLBO:Eu2+
16 phosphors. While SLBO:Eu2+ contains a single doping site for Eu doping, in SLA:Eu2+, there are in principle two doping candidate sites. The two sites have a similar local geometric structure, but they are not identical. Hence while at room temperature within the experimental resolution, the two sites provide similar absorption spectra and emission spectra,1 it has been recently shown that at low temperature, they provide unique emission band signatures in the vibrationally resolved emission spectrum.58 These phosphors define the lower and upper boundaries of a range of Eu2+ doped phosphors in which the crystal field strength as well as the Eu/ML8 cuboid compression is increasing.1 It should be noted that the actual bottom boundary in the Eu2+-doped phosphors is defined by the narrow band red emitting Ca[LiAl3N4]:Eu2+ (CLA:Eu2+) phosphor.51 As seen, the CBLA2:Eu2+ emission spectrum is blue shifted by +300 cm−1 with respect to the SLA:Eu2+ one, showing a similar bandwidth range, FWHM ∼ 50 nm (1090 cm−1). Likewise, the RNLSO:Eu2+ emission spectrum is red shifted by 700 cm−1 with respect to the SLBO:Eu2+ one, showing again a similar bandwidth range in the ultranarrow band regime, FWHM ∼ 22–25 nm (1010–1220 cm−1). RNLSO2 lies in between the above described cases indicating that complex phosphors with multiple candidate doping centers might still show linear property characteristics like the single doping center phosphors.
To conclude this part, while RNLSO:Eu2+ show a unique blue emission band. RNLSO2:Eu2+ shows a predominant cyan emission band and a blue emission band with higher energy and weaker intensity, where the relative intensity of the bands is tunable by the chosen excitation wavelength (Fig. S9 and S10, ESI†). The isotypic to RNLSO2:Eu2+ and CBLA2:Eu2+ shows a broad IR band besides the main red emission band. In principle, the presence of a second or multiple bands besides the main emission band is undesirable in the novel phosphor design efforts as they may reduce effectively their brightness, performance and efficiency. While in the case of RNLSO2:Eu2+, the higher energy, second weaker intensity blue emission band is tunable by the choice of the laser excitation energy,53 the IR band in CBLA2:Eu2+ can only be suppressed at low Eu2+ doping concentrations.38 This emphasizes the urgent need for advancing the information content of the emission intensity mechanism in these materials.
The optical band gap of the host structures was calculated by the similarity transformed equation of motion domain-based local pair natural orbital coupled cluster singles and doubles (STEOM-DLPNO-CCSD)81,82 as well as TD-DFT83 methods. In the latter, a collection of DFT functionals were chosen, belonging to the GGA:PBE,84 hybrid:PBE0,85–87 range separated hybrid: CAM-B3LYP,88 double hybrid: B2PLYP,89 and range separated double hybrid: ωB2PLYP90 families. Similarly, TD-DFT and complete active space (SA-CASSCF)91,92 methods in conjunction with the second order N-electron valence state perturbation theory (NEVPT2)93,94 including spin–orbit coupling (SOC) were employed to compute the band gap energies of the Eu2+-doped structures. As briefly discussed in the computational considerations Section IV.3 and in detail in section SII of the ESI,† based on these results, the TD-DFT/PBE0 was chosen for the production calculations. Preliminary calculations for estimating the multi-root nature of the Eu2+-doped phosphor emission process and the effect of SOC and spin state energetics of the emission bands were performed employing SA-CASSCF(7,19)/NEVPT2/SOC. As discussed in section IV.3, the SOC interactions do not significantly influence the emission band energy positions, hence they were excluded from the production calculations. Eu2+ doping energies at different candidate sites were computed at DFT/PBE0 and DLPNO-CCSD(T) levels of theory.95–97 DLPNO-CCSD(T) doping energies were decomposed into chemically meaningful energies on the basis of local energy decomposition (LED) approach98,99 starting from quasi-restricted (QRO)100 Kohn Sham (KS) orbitals.
At different Eu2+ doping sites, absorption spectra were computed at TD-DFT/PBE0 employing the Tamm–Dancoff approximation (TDA)101 accompanied by the Natural Transition Orbital (NTO) analysis for the computed bands. Photoluminescence spectra were computed using TD-DFT/TDA/PBE0 employing the excited state dynamics (ESD) path integral protocol102–104 in which vibronic coupling is included within the Frank–Condon and Herzberg–Teller coupling schemes. In this framework, the ground state Hessian was calculated at the DFT/PBE0 level while the excited state geometry and Hessian obtained by approximating excited state PES through the vertical gradient (VGFC) model as discussed in the ESD module.104
A constant Gaussian broadening was used for all presented absorption and emission spectra which amounts to an FWHM of 1500 cm−1 and 500 cm−1, respectively. For better visual agreement with the experimental absorption spectra, a second Gaussian broadening with an FWHM of 3000 cm−1 was used in some of the computed absorption spectra.
As shown in Fig. S1 (ESI†), the series of the chosen cluster models consists of sequences of cuboidal structures ranging from monomers to pentamers. The low doping limit is considered so that Eu2+-doped structures contain only one Eu2+ ion replacing one (Ca2+, Ba2+, Na+, or Rb+) cation per cluster.60 In addition, no (Eu2+–Eu2+) interaction is expected, as well, no other cation substitution (e.g., Li+, Mg2+, Al3+, or Si4+) or occupation of interstitial sites is expected due to structural and steric reasons.1 Owing to the strong rigidity of the considered solid-state crystal structures, no further structural relaxation due to Eu2+ doping needs to be taken into account.
It should be noted that in RNLSO and RNLSO2, charge compensation for singly charged ion replacements (Na/Rb) is achieved through charge redistribution within the employed embedded cluster scheme. This allows for the electronic relaxation around the Eu2+ doped centers in terms of electrostatic and covalent Eu-host interactions. Details regarding the principles of this analysis are provided in Section SIII.1-2 of the ESI.† Focusing on CBLA2 as shown in Table 2 and Fig. 4, DLPNO-CCSD(T) results predict that Eu2+ doping at Ba2+ centers provides more stable structures with respect to Eu2+ doping at Ca2+ centers by 3 eV. Similarly, in RNLSO2 Eu2+, the doping at Rb+ centers provides more stable structures with respect to Eu2+ doping at Na+ centers by ∼2.5 eV. In contrast, in RNLSO, Eu2+ doping at (Rb+, Na(1)+) centers provides close DLPNO-CCSD(T) doping energies (−1.66, −1.32 eV) while Eu2+ doping at Na(2)+ provides rather less stable structures (−0.88 eV).
Phosphor | Doping site | Doping energy (eV) |
---|---|---|
CBLA2 | Ba2+ | −3.67 |
Ca2+ | −0.67 | |
RNLSO | Na(1)+ | −1.32 |
Na(2)+ | −0.88 | |
Rb+ | −1.66 | |
RNLSO2 | Na+ | −0.87 |
Rb+ | −3.34 |
DLPNO-CCSD(T) results are used as a basis for the quantitative analysis of the doping energy in terms of ionic and covalent interactions as they collectively describe the various interactions in the framework of the local energy decomposition (LED) analysis as presented for CBLA2:Eu2+ in Fig. 4 and in Section III.2 of the ESI.† As has been shown in several studies110,111 local energy decomposition (LED) enables the classification of interactions into different types of meaningful chemical and physical interactions, thereby facilitating a comprehensive exploration of the electronic structure and the ionic and covalent interactions surrounding the Eu ions in their respective environments.
As shown in Fig. 4 and Fig. S7 (ESI†), the least probable site for each system (CBLA:Eu2+ at Ca2+, RNLSO2:Eu2+ at Na+, and RNLSO:Eu2+ at Na(2)+, respectively) shows positive ionic interactions as they are expressed by EREFint = +1.8, +0.9 and +1.1 eV, respectively, indicating the unavailability of the host structure for Eu2+ doping due to the significant compression in the EuL8 cuboid. This is also accompanied by the shorter Eu–L ligand and strong repulsion with the first shell of cations, as shown in Table 1. In contrast, the most probable site for each system exhibits strong and negative electrostatic interactions (∼EREFint = −2.3, −3.0 and −1.4 eV) for CBLA2:Eu2+ at Ba2+, RNLSO2:Eu2+ at Rb+, and RNLSO:Eu2+ at Rb+, respectively.
The relevant covalent type interactions (ECnon-disp, ECdisp) result in rather fine tuning of the doping energy. In particular, dispersion corrections follow the difference in the ionic radii between the substituted cations and Eu2+ (Table 1). They are hence repulsive in the most probable and more relaxed EuL8 cuboids of CBLA2:Eu2+ at Ba2+, RNLSO2:Eu2+ at Rb+, and RNLSO:Eu2+ at Rb+, respectively. Similarly, as expected, stronger non-dispersion corrections are observed in the more covalent nitride (CBLA2) with respect to the oxide (RNLSO and RNLSO2) phosphors. Compressed versus elongated EuL8 cuboids show also larger non-dispersion interactions that are associated with stronger Eu–N/O covalent interactions and bond lengths according to Table 1. Finally, the most stable EuL8 cuboids also show the smallest triple corrections across the study set that are inverted proportional to the doping energy.
The above quantitative analysis demonstrates the direct connection of the cuboid characteristics of a given host ion with its probability for Eu2+ doping. This indicates that relaxed host cuboids have in general a higher tendency for Eu2+ doping.
Entering the spectra computation section, as shown in Fig. 6, in the case of CBLA2, the main emission band arises from absorption band 2. The emission process involves a Eu2+ center doped at the Ba2+ site and takes place from a Eu 5dz2 based molecular orbital MO with a covalency factor a2 = 0.94. In contrast, the lower energy and weak intensity emission band arise from absorption band 1. The emission process involves a Eu2+ center doped at the Ca2+ site involving a Eu 5dx2−y2 based molecular orbital MO with a covalency factor a2 = 0.87. Absorption band 3 arises from a Eu2+ center doped at the Ca2+ site and involves a Eu 4fy(3x2−y2) → Eu 5dx2−y2 electron excitation showing no pronounced emission intensity. Likewise, the high energy absorption band 4 arises from a Eu2+ center doped at the Ba2+ site and involves an Eu 4fxyz → Eu 5dx2−y2 electron excitation showing a negligible emission intensity.
It should be noted that symmetry reduction towards C2h or S4 symmetric EuN8 cuboids could render the Eu 4fxyz ↔ Eu 5dx2−y2 electron decay a dipole allowed process. As shown in Fig. S8 (ESI†) this is in fact the case for both the isotypic to CBLA2, RNLSO2 but also RNLSO rendering in particular the Eu2+ doping at Na and Na(1) centers, respectively, a dipole allowed Eu 4fxyz ↔ Eu 5dx2−y2 emissive process. As discussed in detail in Section SIII.3 of the ESI,† these positions dominate the experimental spectra. In fact, in contrast to CBLA2 in the case of RNLSO2 (Fig. S9a, ESI†), the main emission band 1* arises from Eu2+ centers doped at the Na+ sites (in relation to Ca2+ sites in CBLA2) and takes place from the non-bonding Eu 5dx2− y2 based MO with a2 of 0.92. A weak blue shifted emission band 2* arises from Eu2+ centers doped at the Rb+ sites (in relation to Ba2+ sites in CBLA2) reached by absorption band 2 and takes place from the non-bonding Eu 5dz2 based MO with a2 = 0.97. As shown in Fig. S10 (ESI†) and according to the experiment, the intensity of this second band can be tuned by the excitation laser. In the case of RNLSO (Fig. S9b, ESI†), the main emission band arises from a Eu2+ center doped at the Na(1)+ site and takes place again from the non-bonding Eu 5dx2−y2 based MO with a2 of 0.95.
It should be emphasized that the emission bands arising from Eu2+ centers doped at Ca2+, Na+ and Na(1)+ sites in the case of CBLA2, RNLSO2 and RNLSO have the following characteristics (1) involve compressed EuN8 and EuO8 cuboids, (2) take place from non-bonding Eu 5dx2−y2 based MO and (3) the RNLSO band is blue shifted (FWHM = 1015 cm−1, 22.5 nm) with respect to the RNLSO2 (FWHM = 1465 cm−1, 40 nm) band by 2100 cm−1 with a narrower bandwidth by 450 cm−1, respectively. Hence, there is a clear relation between the geometric characteristics around the Eu2+ centers and their emission properties in these systems. This is consistent with the descriptor relationships discussed in Section S IV, Fig. S11, and Table S5 (ESI†).
Up to this point of analysis, it has been shown that owing to the very rigid nature of the emissive states in both Eu2+-doped phosphors bearing one or multiple doping centers, the TDDFT/PBE0 computed spectra provide satisfactory agreement to the experimentally observed absorption and emission spectral features allowing for a quantitative analysis. However, for the identification of the probable Eu2+-doping centers at the ground state and a comprehensive qualitative and quantitative description that connects the strength of electrostatic and covalent interactions between Eu2+ and the coordination environment provided by the phosphor host structure, the sensitivity provided by DLPNO-CCSD(T) computed energies and their respective LED analysis is required. These two successful approaches will be employed below towards an in silico investigation of new Eu2+ doped phosphor with tailored photoluminescence properties.
The results are summarized in Fig. 7, emphasizing the structural transformation from RNLSO2 to RNLSO, highlighting its profound impact on electronic structure and bonding, resulting in a significant enhancement in emission properties. It can be applied similarly to enhance CBLA2, toward CBLA thereby advancing its properties.
As shown in Fig. 7a, in the case of RNLSO, the Na(1)+ sites form host cuboids (Na(1)+O8) that are tetragonally compressed with respect to the (Na+O8) cuboids in RNLSO2, owing to the formation of the Rb+–Na(1)+–Rb+ cuboid sequence. As discussed in the previous sections, these sites dominate the emission bands in the respective Eu2+-doped phosphors. In particular, Na(1)+ centers have a higher probability for Eu2+doping with respect to the Na+ sites in RNLSO2 while they result in emission bands that are blue shifted and narrower. The local energy decomposition (LED) analysis confirms that Eu2+ doping at the Na+ sites in RNLSO2 results in repulsive ionic interactions with the [O8Li4Si4Na2]6+ host environment that is only partially compensated by attractive covalent interactions leading to an overall low probability for Eu2+ doping in these centers. In contrast, Eu2+ doping at the Rb+–Na(1)+–Rb+ tetragonally compressed cuboid sequence in RNLSO shows almost neutral ionic interaction (+0.02 eV) with the [O8Li8Rb2]6− host coordination environment and slightly reduced covalent interactions. This is also reflected to the EuO8 cuboid volumes and Eu–O bond distances (29.3 Å3, 2.6 Å in RNLSO2 and 30.2 Å3, 2.7 Å in RNLSO). Overall, the analysis confirms the improvement in the doping probability at the Na(1)+ centers of RNLSO with respect to the Na+ centers in RNLSO2. While the EuO8 cuboid expansion and the covalency reduction along this direction are also consistent with the blue shifted and narrower bandwidth emission signal in RNLSO in comparison to RLNSO2 for these doped centers. We would like to emphasize that while within the local energy decomposition (LED) framework, the covalent interactions are probed in the ground state, it has been shown that the open Eu2+ 4f7 shell is only marginally involved in the bonding,112 and the important covalent interactions with the host environment are actually taking place in the Eu2+ 5d and 6s shells. In this concept, these interactions are probing indirectly the bonding characteristics of the excited emissive states of the 4f75d1 shell.
Na+ and Rb+ sites in RNLSO2 resemble the characteristics of the Ca2+ and Ba2+sites in CBLA2. As shown in Fig. S7 (ESI†), Eu2+ doping at the respective Rb+ and Ba2+ sites in RNLSO2 and CBLA2 leads to favorable doping situations. This is reflected in both the ionic and covalent interactions between the Eu2+ site and the host environment. Due to the negatively charged host environments, [O8Li8Na2]6− and [N8Al4Li4Ba2]4− the Eu2+ site – host environment ionic interactions are attractive (2.7 and 2.3 eV) while the EuO8 and EuN8 cuboid expansions (Eu–O ∼ 3.00 Å and 40.5 Å3 cuboid volume and Eu–N ∼ 2.93 A and 37.6 A3 cuboid volume, respectively) lead to weaker covalent interactions, hence to weaker vibronic coupling at these sites, which is also reflected in the reduction of the emission bandwidths in comparison to the emission spectra originating from the respective Eu2+-doped Na+ and Ca2+ sites.
Likewise to the Rb+ and Ba2+ sites, Eu2+ doping at Na+ and Ca2+ in RNLSO2 and CBLA2 phosphors not only results in compressed EuO8 and EuN8 cuboids with similar principle emission characteristics with respect to the non-bonding Eu 5dx2−y2 MO character of the emissive state but also in terms of their probabilities for Eu2+ doping (Fig. 7 and Table S4, ESI†). As shown in Fig. 7a and b, both the Na+ sites in RNLSO2 and the Ca2+ sites in CBLA2 are less favorable for Eu2+ doping showing significant repulsive ionic (+1.7 eV) interactions owning to the positive [N8Al8Ca2]4+ coordination environment opposing the rather covalent Eu2+-host interactions (−2.4 eV). Hence as in the case of RNLSO2, at the Eu2+-doped Na+ sites, in the case of CBLA2, the overall doping probability, for the Eu2+-doped Ca2+ sites is significantly reduced.
These results confirm the experimental and computational observations that for the RNLSO2:Eu2+ phosphor, the emission band characteristics can be improved by tuning the excitation laser to higher energies to basically probe the emission originating from Eu2+-doped Rb+ over Na+ sites. Alternatively one may resort to the RNLSO:Eu2+ phosphor to benefit from the improved doping probability of the Eu2+doped Na(1)+ sites towards a unique, narrow band blue shifted emission band in comparison to the Eu2+doped Na(1)+ sites of RNLSO2:Eu2+. In contrast in the case of CBLA2:Eu2+ phosphor, the only possibility to reduce the emission intensity losses into the IR is to in principle reduced the Eu2+ doping concentration to suppress the emission from the low probability for Eu2+ doping at Ca2+ centers at the cost of reducing the total light intensity and brightness of the phosphor. Hence, at this point, the question arises whether it is possible to alter the unfavorable emission characteristics of the CBLA2:Eu2+ phosphor by generating the hypothetical CBLA:Eu2+doped phosphor that is isotypic to the RNLSO:Eu2+ phosphor. The structural characteristics of the hypothetical CBLA:Eu2+ doped phosphor are provided in the ESI† (Fig. S16, Section SV).
As shown in Fig. 7a and b likewise to the Na(1)+ centers of RNLSO, the Ca(1)2+ centers in CBLA form tetragonally compressed (Ca2+N8) cuboids owing to the formation of the asymmetric Ba2+–Ca(1)2+–Ba2+ cuboid sequence. In contrast to the Eu2+-doped Ca2+ sites in CBLA2:Eu2+,Eu2+ doping at Ca(1)2+ centers becomes favorable. This is due to the attractive ionic interactions between Eu2+ and [N8Al8Ba2]4+ host environment and the reduced covalent interactions leading to an improved probability for Eu2+ doping at these sites. The Eu2+N8 expansion (Eu–N, volume) and the suppression of the Eu host covalent interactions could in fact lead to a blue shifted narrow band emission signal in comparison to the Ca2+ Eu2+-doped positions. However, as in fact shown in Table S4 and Fig. S7 (ESI†) in CBLA:Eu2+, the doping probability of both Ca(1)2+, Ca22+ and Ba2+ in comparison to the respective Ca2+ and Ba2+ Eu2+-doped centers in CBLA2:Eu2+, improves. The extent to which this could ultimately lead to a candidate phosphor with improved emission properties is investigated below.
As discussed in Section II, in the case of CBLA2 Eu doping at Ba2+ centers results in tetragonally elongated EuN8 cuboids with a volume of 37.5 Å3 surrounded by tetragonally elongated BaN8 cuboids of the same volume while doping at Ca2+ centers results in tetragonally compressed EuN8 cuboids with a volume of 29.5 Å3 surrounded by tetragonally compressed CaN8 cuboids of the same volume. Along the list of vibrational modes that influence the emission bands in CBLA2 according to their computed Huang–Rhys factors S,102,103 the eg group of vibrational modes, illustrated in Fig. S13 and S14a (ESI†), shows the most significant contributions. Not surprisingly, these group of modes represent the tetragonal distortion pathway of EuN8, BaN8 and CaN8 cuboids. The DLPNO-CCSD(T) potential energy surface (PES) was computed as well as the respective emission spectra along the tetragonal distortion pathway at both Ba2+ and Ca2+ doping centers. The results are summarized in Fig. 8a and b and Fig. S14 (ESI†).
As seen in Fig. S14 (ESI†), at the Ba doping centers, both the EuN8 cuboids at the doped Ba2+ center and the BaN8 cuboids of the undoped centers maintain practically similar cuboid volumes along the tetragonal distortion pathway (∼37 Å3 at Q = 0 and ∼33 Å3 at Q = 6). In contrast, at the Ca doping centers, the EuN8 cuboid compresses further (from 29.5 Å3 to 28.85 Å3) while the CaN8 ones expand (from 30.5 Å3 at Q = 0 to 37.3 Å3 at Q = 6). A similar trend is observed in the computed emission spectra shown in both Fig. S14 (ESI†) and Fig. 8b. In fact, along the compression pathway the emission arising from Eu2+-doped Ba2+centers, remains unaffected in terms of energy position and absolute intensity the respective emission band, arising from Eu2+-doped Ca2+ centers, becomes blue-shifted with increasing intensity. Along the tetragonal distortion pathway, at normal mode value Q = 3, this band actually overtakes the total intensity while Q = 6 dominates the emission signal providing a unique red emission band at ∼14300 cm−1. It becomes evident that structural modifications that could stabilize the Eu2+-doped centers around the Q = 6 magnitude of the axial compression pathway would potentially lead to an unprecedented narrow band red-emitting phosphor.
Hence in a next step at the trimer model CBLA2:Eu2 structures containing Ca2+ doping centers, we exchange the Ca2+ undoped centers with Ba2+ in order to better accommodate the MN8 (M = Ca2+, Ba2+) expansion along the EuN8 compression pathway. Likewise, at the trimer structures that contain Ba2+ doping centers, we exchange the bulky Ba2+ centers with the smaller Ca2+ centers in an effort to minimize any remaining geometric strain at the CaN8 cuboids along the EuN8 compression pathway. In this way, the host cuboid asymmetric sequences Ba2+–Ca2+–Ba2+ and Ca2+–Ba2+–Ca2+ that are actually present in CBLA are formed. This is shown in Fig. S15, ESI.† As expected, this structural modification creates an asymmetry at the doped Ca2+ and Ba2+ sites in both the doped EuN8 cuboids (35.8 Å3 at Ca2+ site, 43.7 Å3 at Ba2+ site) and undoped BaN8 cuboids (33.2 Å3 at Ca2+ site) and CaN8 cuboids (32.4 Å3 at Ba2+ site) at the formal CBLA2:Eu2+ equilibrium structure (Q ∼ 0). This further reduces the local cuboid symmetries from D4h to C2h and activates a combination of eg and t2g modes that lead the tetragonal distortion. Allowing the system to relax along the tetragonally compression pathway, we compute once again the relevant PES of the CBLA:Eu2+ model.
In order to be able to compare the energetics between the CBLA2:Eu2+ and CBLA:Eu2+ PESs, the CBLA:Eu2+ is constructed on the basis of the transformations at the Ca2+ and Ba2+ doping centers, respectively. As seen in Fig. 8a at the Ca2+, Eu2+-doped site, the CBLA:Eu2+ PES in comparison to the CBLA2:Eu2+ PES stabilizes at Q = 3 at about 12 kcal mol−1 indicating that along the tetragonal distortion pathway, the transformation of CBLA2:Eu2+ to CBLA:Eu2+ is energetically feasible. In contrast, no significant stabilization is observed of the CBLA:Eu2+ over the CBLA2:Eu2+ at the Eu2+-doped Ba2+ centers. The relevant computed emission spectra are provided at Fig. 8c and Fig. S15 (ESI†). Interestingly, the intensity overtake at the Eu2+-doped Ca2+ centers takes place already at Q = 2, in comparison to model CBLA2:Eu2+ (Q = 4), and at Q = 3, the emission is dominated by the Eu2+-doped Ca2+ centers showing a red emission band at 14
700 cm−1. The respective emission band corresponding to the Eu2+-doped Ba2+ centers is shifted to higher energies and loses practically its intensity at Q = 3.
To summarize, the structural modifications that are necessary to transform CBLA2:Eu2+ phosphor to a unique narrow band red emitting phosphor require the presence of a hypothetical host with (1) containing an asymmetric sequence of cuboids around the Ca and Ba doping centers. For example, sequences of cuboids with Ba2+–Ca2+–Ba2+ and Ca2+–Ba2+–Ca2+ building units and (2) formation of EuN8 cuboids so that the Eu 4fxyz ↔ Eu 5dx2−y2 electron decay represents dipole allowed processes.
Looking into the structural characteristics of the isotypic CBLA2, RNLSO2 and RNLSO, we demonstrated in the previous sections that formation of the Ca3Ba[LiAl3N4]4:Eu2+, CBLA host structure that is isotypic to RNLSO adopting the tetragonal (I4/m) space group fulfils the above structural requirements (Fig. S16, ESI†).
In fact as seen in Fig. S17a (ESI†), in the hypothetical CBLA:Eu2+ compound, Ca2+ and Ba2+ are alternating in the same channel forming cuboid sequences with Ca(1)2+–Ba2+–Ca(1)2+–Ba2+ with elongated and compressed central cation BaN8 and Ca(1)N8 cuboids as well as Ca(2)2+–Ca(2)2+–Ca(2)2+ ones with elongated Ca(2)N8 cuboids. As shown in Table S4 (ESI†), all these doping positions are in principle available for Eu doping. As expected, the computed absorption spectrum shows distinct energy separation (∼0.5 eV) between local (4f–5d) and metal to ligand charge transfer (MLCT) bands resulting in a potentially thermally stable Eu doped phosphor. According to the NTO analysis at the Eu2+-doped Ca(1)2+centers, emission from the C2h symmetric (distorted D4h) compressed EuN8 cuboid is dominated by allowed Eu 4fxyz ↔ Eu 5dx2−y2 electron decays, while at Ba and Ca(2) doped centers, emission from elongated EuN8 cuboid (of approximately D4h symmetry) emission is dominated by forbidden Eu 4fxyz ↔ Eu 5dz2 electron decays.
Collectively, as seen in (Fig. 8d, e and Fig. S17c, ESI†) and according to the expectations from the descriptor relationships (Fig. S11 and Table S5, ESI†), the computed emission spectrum of the hypothetical CBLA:Eu2+ is characterized by a single narrow red band with FWHM 1170 cm−1 (56 nm) at 14800 cm−1 originating by the Eu2+-doped Ca(1)2+ centers. In this concept, CBLA:Eu2+ can be seen as a candidate derivative of CBLA2:Eu2+ with considerably improved photoluminescence properties. However, all the above require confirmation from the actual synthesis of CBLA:Eu2+ phosphors. We believe that the present study serves as an example of how systematic computational chemistry can be used to aid the synthetic efforts towards novel phosphor materials.
In particular, it was shown that the most probable doping centers are those enabling the formation of relaxed EuL8 cuboids dictating the Ba2+ and Rb+ positions as the most probable positions for Eu2+-doping in the case of CBLA2, and (RNLSO and RNLSO2) phosphors. In this concept, the absorption and luminescence spectra of the chosen study set of phosphors were computed, on the basis of the defined doping and symmetry selection rules, showing very good agreement with the experimental results. Once again,1 it was shown that the suppression of the Eu–O/N covalent interactions, as well as the steric effects imposed by the second coordination sphere, is the origin of the desired narrow band emission across the most probable centers for Eu2+doping.
This analysis led us to realize that the Na+ and Rb+ sites in RNLSO2 resemble the geometric and electronic structure characteristics of the Ca2+ and Ba2+sites in CBLA2. Most importantly, it was shown that Eu2+-doping of the Na(1)+ sites in RNLSO is more favorable than the Eu2+ doping of the Na+ sites in RNLSO2 leading to improved emission characteristics as the origin of the blue shifted, single narrow band emission spectrum in the former.52,53
This inspired us to synthesize, in silico, the respective CBLA phosphor with an ultimate goal to improve the emission characteristics of the Ca2+ sites in CBLA2. It was indeed demonstrated that the geometric transformation of CBLA2 to CBLA follows a tetragonal cuboid compression pathway along the most important coupling vibrational modes dominating the emission bands in CBLA2. The resulted CBLA phosphor host environment that is involved in the Eu2+-doping process is more feasible energetically. It creates a host environment which renders the emission from the relevant Ca(1)2+ Eu2+ doped sites a favorable process leading to a blue shifted narrow band red emission signal in comparison to the Ca2+ Eu2+-doped sites in CBLA2. At the same time, emission from the Ca(2)2+ and Ba2+ Eu2+-doped sites is negligible due to symmetry reasons. Overall, this resulted in a single narrow band red emission, that is computationally predicted at around 14800 cm−1 and FWHM 1170 cm−1, introducing the CBLA as a candidate phosphor with potentially unprecedented emission properties for pc-LEDs applications.
We believe that the results presented herein are important in the design of novel narrow band phosphors with tunable emission properties and for further improving the quality and the energy efficiency of phosphor converted LEDs. In this direction, research is ongoing in our laboratories to validate the concept of the computational predictions by synthesizing candidate phosphors of the novel CBLA phosphor family, for predicting the potential photoluminescence properties of other yet unknown promising phosphor materials, as well as for a general and in depth understanding of the narrow band emission mechanisms.
Footnote |
† Electronic supplementary information (ESI) available: Tables containing detailed information regarding the different embedded clusters as well as figures containing complementary information regarding the electronic structure, band gap calculations and the computed absorption and emission spectra of the study set of the Eu2+-doped phosphors are provided. See DOI: https://doi.org/10.1039/d3cp06039j |
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