Journal of Luminescence 175 (2016) 260–266Contents lists available at ScienceDirectJournal of Luminescencehttp://d 0022-23 n Corr E-mjournal homepage: www.elsevier.com/locate/jluminFull Length ArticleStokes and anti‐Stokes luminescence from cubic elpasolite Cs2NaYF6 crystals doped with Er3þand Yb3þ ions P.A. Loiko a,n, N.M. Khaidukov b, J. Méndez-Ramos c, E.V. Vilejshikova a, N.A. Skoptsov a, K.V. Yumashev a a Center for Optical Materials and Technologies (COMT), Belarusian National Technical University, 65/17 Nezavisimosti Ave., Minsk 220013, Belarus b N.S. Kurnakov Institute of General and Inorganic Chemistry, 31 Leninskii Prospekt, Moscow 119991, Russia c Departamento de Física, Universidad de La Laguna, Tenerife, 38206 La Laguna, Spaina r t i c l e i n f o Article history: Received 29 October 2015 Received in revised form 31 January 2016 Accepted 22 February 2016 Available online 15 March 2016 Keywords: Elpasolite crystals Erbium Ytterbium Luminescence Up-conversionx.doi.org/10.1016/j.jlumin.2016.02.025 13/& 2016 Elsevier B.V. All rights reserved. esponding author. ail address: kinetic@tut.by (P.A. Loiko).a b s t r a c t Er3þ and Yb3þ doped cubic elpasolite Cs2NaYF6 crystals including stoichiometric compositions Cs2NaErF6 and Cs2NaYbF6 have been synthesized under hydrothermal conditions. Absorption, stimulated-emission and gain cross-sections spectra have been determined for the 2F5/2- 2F7/2 (Yb 3þ) and 4I13/2-4I15/2 (Er3þ) transitions at room-temperature. The maximum σSE values are 1.81021 cm2 at 993 nm (Yb3þ) and 3.81021 cm2 at 1535 nm (Er3þ). Elpasolite crystals provide exceptionally long radiative lifetimes of the excited-states for both ions, namely τ(2F5/2)¼6.3 ms and τ(4I13/2) 32 ms for 10 at% Yb3þ:Cs2NaYF6 and 10 at% Er3þ:Cs2NaYF6 which can be used in high pulse energy Q-switched lasers. Up-conversion luminescence has been studied for Er3þ doped and Er3þ , Yb3þ codoped Cs2NaYF6 crystals. & 2016 Elsevier B.V. All rights reserved.1. Introduction Halide compounds having the elpasolite structure can be described by a general formula A2BMX6 where A and B are monovalent alkali ions provided that the ionic radius of A is greater than that of B, M stands for trivalent metal ions, which can be Al, Sc, transition elements and rare earth elements, and X is a halogen [1]. The elpasolite compounds crystallize in the face- centered cubic space group Fm3m [2] and can be described as double perovskites. In the structure the A alkali cations are located in the cuboctahedral sites whereas the B alkali cations and the M trivalent metal ions regularly alternate along the unit cell axes in octahedral sites. Accordingly, the MX6 octahedra are perfectly cubic with Oh site symmetry for trivalent metal ions, while the MX6 octahedra do not share halide ions with each other, i.e. the elpasolite structure is characterized by the isolated MX6 octahedra. In addition, as all the halide compounds, elpasolites are materials with low-phonon energy. The above mentioned peculiarities of elpasolite hosts lead to a significant reduction of the multiphonon relaxation rates for optically active rare earth (RE) ion dopants, which allows for an increased lifetime of some excited levels that can relax radiativelyor can store energy for further up-conversion and cross-relaxation as well as provide relatively low concentration quenching of luminescence, which allows obtaining efficient luminescence in A2BMX6 containing high trivalent RE ion concentrations up to 100 at%. To date, some spectroscopy data for several RE ions (Er3þ , Yb3þ , Tm3þ , Eu3þ) doped into the Cs2NaYF6 compound have been published; however, characterization of these materials is far from completeness mainly due to the difficulty of synthesizing optical quality crystals of elpasolites in general and Cs2NaYF6 in particular. For example, VUV 5d–4f luminescence of Er3þ ions, including a stoichiometric Cs2NaErF6 compound, has been studied followed by crystal field calculations for Er3þ ions [3,4]. Near-IR (2.7 μm) emission of Er3þ ions in Cs2NaYF6 has been also investigated and the lifetime of the 4I11/2 excited-state has been detected to be as long as 1 ms at room-temperature for highly-doped (410 at%) samples [5]. Absorption and emission as well as crystal field analysis for Yb3þ ions in Cs2NaYbF6 has been reported [6–8]. In particular, very long lifetime of the Yb3þ excited-state, τ(2F5/2)¼ 5.63 ms, at room-temperature is observed for Cs2NaYbF6. Some spectroscopic peculiarities of Tm3þ ions in Cs2NaYF6 have been also studied [3,6,9] and crystal field calculations for a Tm:Cs2NaYF6 crystal have been performed [10]. The spectroscopic properties of Eu3þ and Tb3þ ions doped into Cs2NaYF6 have been investigated as well [11–13]. P.A. Loiko et al. / Journal of Luminescence 175 (2016) 260–266 261The fluoride cubic elpasolite Cs2NaYF6 is isostructural with the chloride elpasolite Cs2NaYCl6, that has been extensively studied as an low phonon energy host for optically active ions of 3d, 4f and 5f elements, for example Er3þ [14,15]. In particular, Cs2NaYCl6 crystals doubly doped with Er3þ and Yb3þ have been studied as the near- IR-to-visible frequency converters [16,17] based on photon upcon- version processes [18]. As a result of upconversion mechanisms, Er3þ–Yb3þ ion pairs can convert near-IR (1 μm) emission of InGaAs laser diodes to green and red light. On the other hand, Cs2NaYF6 is harder and less moisture-sensitive than Cs2NaYCl6. Thus, the study of visible emissions in Er3þ and Yb3þ ions doped Cs2NaYF6 crystals is of practical interest for developing photon upconverters. High efficiency of up-conversion in the cubic elpa- solite Cs2NaYF6 can be achieved due to the low value of the max- imum phonon frequency which is 468 cm1 [11]. This value is higher than that for Cs2NaYCl6 (285 cm1) [19] but it is acceptable for energy storage on excited levels. In addition, long lifetimes of the first excited-states of Er3þ and Yb3þ ions observed for highly- doped Cs2NaYF6 crystals indicate their potential for generation of high pulse energies in passively Q-switched near-IR lasers. In the present paper, the data on optical absorption, near-IR and visible f–f emissions of Cs2NaYF6 crystals doped with Er3þ and Yb3þ ions as well as Cs2NaErF6 and Cs2NaYbF6 are reported.Fig. 1. X-ray diffraction patterns for Cs2NaYF6, Cs2NaErF6 and Cs2NaYbF6 crystals; numbers on the graph represent the Miller indices, (hkl). Table 1 Lattice parameter (а), unit cell volume (V), calculated density (ρ) and absolute concentration of rare earth ions (N) for cubic elpasolites (space group: Fm3m, Z¼4). Composition а, Å V, Å3 ρ, g/cm3 N, at/cm3 Cs2NaYF6 9.057 742.9 4.42 5.381021 Cs2NaErF6 9.045 740.0 5.15 5.411021 Cs2NaYbF6 9.016 732.9 5.24 5.4610212. Experimental Crystals of cubic elpasolite Cs2NaYF6 doped with Er3þ and Yb3þ ions as well as Cs2NaErF6 and Cs2NaYbF6 were grown under hydrothermal conditions. For hydrothermal experiments, copper- insert lined autoclaves with a volume of 40 cm3 were utilized, and the inserts were separated by perforated diaphragms into synthesis and crystallization zones. The fluoride crystals were synthesized by a direct temperature-gradient method as a result of the reaction of the aqueous solutions containing 35–40 mol% CsF and 8–10 mol% NaF with oxide mixtures (1x)Y2O3– xLn2O3 (Ln¼Er and Yb) at a temperature of 750 K in the synthesis zone, a temperature gradient along the reactor body of up to 3 K/cm, and a pressure of 100 MPa. Under these conditions, spontaneously nucleated crystals of up to 0.5 cm3 were grown in the upper crystallization zone of the autoclave for 200 h. The purities of the utilized rare earth oxides were 99.99%. The structure type and phase purity of synthesized samples were characterized with conventional powder X-ray diffraction (XRD) technique and powder XRD patterns were obtained by using a Bruker D8 Advance X-Ray powder diffractometer with Cu Kα radiation. Absorption spectrum was measured for 10 at% Er3þ and 10 at% Yb3þ doped Cs2NaYF6 crystals with a Varian CARY 5000 spectro- photometer (the spectral bandwidth, SBW, was 0.1 nm). Thin polished platelets (1 mm) of crystals were used. Luminescence spectra were measured with a lock-in amplifier, a monochromator MDR-23 (SBW 0.1 nm) and Hamamatsu G5851 and C5460-01 photodetectors. The spectral sensitivity of the set-up was accurately determined with a halogen lamp with calibrated spectral power density. Near-IR luminescence and up- conversion luminescence (UCL) of Er3þ and Yb3þ ions was excited by InGaAs laser diode emitting at 960 nm (excitation to the Er3þ4I11/2 state or Yb3þ2F5/2 state). Excitation light was focused on a sample in a 100 μm spot; the maximum power density was 40 kW/cm2. Luminescence was also excited at 355 and 520 nm (excitation to the 2G9/2 and 2H11/2 states of Er3þ , respectively) and a ns optical parametric oscillator (OPO) Lotis TII LT-2214 was used. CIE chromaticity coordinates of phosphors were calculated by using the photoluminescence data.For the studies of luminescence decay of Yb3þ ions, OPO with the pulse duration of 20 ns was tuned to 960 nm. Luminescence was collected by a wide-aperture lens and re-imaged to the input slit of a monochromator MDR-12 (tuned to 1020 nm, SBW 1 nm); then it was detected with a fast Hamamatsu G5851 photodetector (response time,o100 ns) and a 500 MHz Textronix TDS-3052B digital oscilloscope. To avoid the reabsorption loss, studied crystals were finely powdered and immersed in glycerin (5 wt% powder content). All spectroscopic studies were performed at room temperature.3. Results and discussion The X-ray phase analysis has confirmed that all the synthesized compounds are single-phase samples containing only the cubic elpasolite phases, space group Fm3m, Z¼4 (ICDD PDF Cards: 00- 020-1214; 00-021-0221; 00-021-0224) [1]. X-ray diffraction pat- terns of Cs2NaYF6, Cs2NaErF6 and Cs2NaYbF6 are showed in Fig. 1 and they can be indexed with a cubic cell with the lattice para- meter, a¼9.057 Å, 9.045 Å and 9.016 Å, respectively. Lattice para- meter (a), volume of the unit cell (V), density (ρ) and concentra- tion (N) of the Y3þ , Er3þ and Yb3þ ions which have been obtained from the X-ray diffraction studies for these compounds are sum- marized in Table 1. One can see that there is a marginal change in cell parameters due to differences in rare earth ionic radii and it should be also noted that the unite cell parameters determined in this study are notably less than those tabulated in [1]. An absorption spectrum measured for a 10 at% Er3þ:Cs2NaYF6 crystal is shown in Fig. 2. For the 4I15/2-4I11/2 transition, the peak absorption cross-section is σabs¼0.071021 cm2 at 963 nm. The full width at half maximum (FWHM) for this band is 24 nm. Such low absorption determines low efficiency for the excitation of Er3þ ions by using InGaAs diodes. Indeed, for the stoichiometric Cs2NaErF6 crystal, the corresponding peak absorption coefficient is α 0.37 cm1, which means that the absorption of diode emission is not complete even for a few mm-thick crystal. For the 4I15/2-4I13/2 transition that is typically used for the in-band excitation of Fig. 2. Absorption cross-section spectra for a 10 at% Er3þ:Cs2NaYF6 crystal. Fig. 3. Near-IR emission spectra of Cs2NaErF6 (a) and Cs2NaYbF6 (b) crystals; excitation wavelength is denoted by arrow (960 nm). Table 2 Energies of Stark sub-levels for the ground-states and the first excited-states of Er3þ and Yb3þ in Cs2NaYF6 crystals [4,8]. Multiplet (Yb3þ) Sub-levels, cm1 Multiplet (Er3þ) Sub-levels, cm1 2F7/2 3 4I15/2 0 324 25 656 57 259 287 2F5/2 10,389 4I13/2 6492 11,109 6517 6532 6682 6686 Fig. 4. (a) Stimulated-emission cross-sections spectra calculated with the reci- procity and F-L methods for a 10 at% Er3þ:Cs2NaYF6 crystal, (b) gain cross-sections [σg¼βσSE–(1–β)σabs] spectra, β¼N2/N is the inversion ratio. P.A. Loiko et al. / Journal of Luminescence 175 (2016) 260–266262Er3þ ions, the absorption is much stronger, σabs¼4.61021 cm2 at 1532.2 nm. The FWHM of this band is 5.4 nm. Near-IR emissions of Er3þ ions have been studied under 960 nm excitation by using a stoichiometric Cs2NaErF6 crystal. The luminescence band related to the Er3þ4I13/2-4I15/2 transition spans from 1.4 to 1.68 μm, see Fig. 3(a). The band in the 920–1060 nm spectral range is attributed to the 4I11/2-4I15/2 transition of Er3þ ions. Emission of Er3þ ions at 1.5 μm is eye-safe and interesting for laser operation. To calculate the corresponding stimulated- emission cross-sections σSE spectra, two methods can be used. The first one is the reciprocity method [20]: σSEðλÞ ¼ σabsðλÞ Z1 Z2 exp hc=λEZL kT   ; ð1Þwhere Z1 and Z2 are the lower and upper manifold partition functions, respectively, EZL is the energy corresponding to the zero phonon line, h is the Planck constant, c is the speed of light, λ is the light wavelength, k is the Boltzmann constant and T is the crystal temperature (room-temperature). Partition functions are deter- mined as: Zm ¼ X k gmk expðEmk =kTÞ; ð2Þ where m¼1, 2; gmk is the degeneration of the sublevel having the number k and the energy Emk measured from the lower sublevel of the corresponding multiplet. The set of Emk values for the 4I15/2 and 4I13/2 states of Er3þ ions in the Cs2NaYF6 crystal [4] is listed in Table 2. Calculation of σSE with the reciprocity method is beneficial as it does not require the information about the radiative lifetime τrad of the emitting state as well as direct measurement of the emis- sion spectrum which can be changed as a result of the reabsorp- tion loss. The obtained results are shown in Fig. 4(a). The max- imum σSE value is 3.81021 cm2 at 1532.2 nm. This value is lower than the typical peak σSE values for the Er3þ4I13/2-4I15/2 transition in widespread oxide and fluoride laser hosts, 0.5– 11020 cm2 [21]. In the spectral range where laser operation is expected, the maximum σSE value is 1.51021 cm2 at 1574.1 nm. Radiative lifetime of the Er3þ emitting state (4I13/2) can be P.A. Loiko et al. / Journal of Luminescence 175 (2016) 260–266 263estimated from the so-called modified reciprocity method (n is the crystal refractive index) [22]: τrad ¼ 1 8πn2c Z2 Z1 expðEZL=kTÞR λ4σabsðλÞexpðhc=ðkTλÞÞdλ : ð3Þ For Er3þ:Cs2NaYF6 crystal, τrad(4I13/2) has been determined to be 3272 ms. Previously, lifetime of this state was measured for 1 at% Er3þ:Cs2NaYF6 crystal only at cryogenic temperature (4 K), τ (4I13/2) 100 ms [5] and this value can be considered as a radiative one at low temperatures, as the reabsorption for such crystal doping is nearly vanishing. Such long values are inherent for all the elpasolite crystals [14]. In particular, τ(4I13/2)¼22 ms for a cubic Cs2NaErCl6 crystal [23]. Independent estimation of the τrad for Er3þ:Cs2NaYF6 crystal can be done with the Judd–Ofelt mod- eling that will be performed in a separate study. Using the measured emission spectrum W(λ), Fig. 3(a), and the determined radiative lifetime τrad(4I13/2), it is possible to calculate a stimulated-emission cross-sections spectrum for the 4I11/2-4I15/2 transition with the Füchtbauer–Ladenburg (F–L) equation [24]: σSEðλÞ ¼ λ5 8πn2τradc WðλÞR λWðλÞdλ: ð4Þ The obtained results are shown in Fig. 4(a) and they are in good agreement with the ones from the reciprocity method, considering strong reabsorption at short wavelengths. For assessing the prospects of elpasolite crystals to lasers, a useful parameter is the gain cross-section, σg: σgðλÞ ¼ βσSEðλÞð1βÞσabsðλÞ; ð5Þ where β is the inversion ratio, β¼N2/N0 where N2 and N0 are the numbers of ions in the upper laser level and the overall number of ions, respectively. Gain spectra for a 10 at% Er3þ:Cs2NaYF6 crystal are shown in Fig. 4(b). For these calculations, we used stimulated- emission cross-sections spectra obtained with the reciprocity method. For low inversion ratios (βo0.4), laser operation is expected at several wavelength, 1624, 1658 or 1694 nm. For high inversion ratios, the peak centered at 1574 nm dominates in the spectrum. An absorption spectrum measured for a 10 at% Yb3þ:Cs2NaYF6 crystal is shown in Fig. 5(a) representing the 2F5/2-2F7/2 transition of Yb3þ ions. The peak absorption cross-section is σabs¼1.31021 cm2Fig. 5. (a) Absorption and stimulated-emission cross-sections spectra for a 10 at% Yb3þ:Cs2NaYF6 crystal, (b) gain cross-sections [σg¼βσSE–(1–β)σabs] spectra, β¼N2/N is the inversion ratio.at 962.0 nm. Thus, Cs2NaYF6 crystals containing both Er3þ and Yb3þ ions provide significant improvement of the excitation efficiency under using InGaAs laser diodes. In particular, the peak absorption coefficient for the stoichiometric Cs2NaYbF6 crystal, α¼6.9 cm1 and FWHM for this band is 5.2 nm. The stimulated-emission cross-sections spectrum for a 10 at% Yb3þ: Cs2NaYF6 crystal has been calculated with the reciprocity method, Eq. (1). The spectrum is shown in Fig. 5(a) and the energies of Stark sub-levels for the 2F5/2 and 2F7/2 states of Yb3þ ions used for calculations are listed in Table 2 [8]. The maximum σSE value is 1.81021 cm2 at 992.4 nm. Emission of Yb3þ ions spans from 920 to 1080 nm. Thus, the tuning range wider than 100 nm is expected under using this crystal as a laser gain med- ium. This is in agreement with the near-IR emission spectrum of the Cs2NaYbF6 crystal measured directly under 960 nm excitation and shown in Fig. 3(b). The radiative lifetime of the 2F5/2 state of Yb3þ ions in the Cs2NaYF6 crystal determined from the modified reciprocity method, Eq. (3), is τrad(4I13/2)¼6.4 ms. This value is in close agreement with the decay time of Yb3þ emission measured directly for a powdered 10 at% Yb3þ:Cs2NaYF6 composition, τ¼6.3 ms. The corresponding decay curve is shown in Fig. 6 and it is clearly single-exponential. For a stoichiometric Cs2NaYbF6 crystal, similar measurement yields τ¼5.7 ms, which is close to the previously reported value [6], τ¼5.63 ms. Thus, the anom- alously weak concentration quenching is observed for Yb3þ: Cs2NaYF6 crystals. Determined lifetimes are at least two times longer than those for typical Yb3þ-doped fluoride laser hosts with τ ranging typically from 1.5 to 3 ms. This indicates the potential of highly-doped Yb3þ:Cs2NaYF6 crystals (up to 100 at%) for genera- tion of high pulse energies in the Q-switched operation mode. Gain cross-sections spectra for a 10 at% Yb3þ:Cs2NaYF6 crystal are shown in Fig. 5(b). For low inversion ratios (βo0.1), the gain spec- trum is flat and it spans from 1000 to 1080 nm, so the multi-peak spectral behavior is expected. For high inversion, two intense local peaks centered at 992 nm and 1009 nm are observed. This indicates the possibility of dual-wavelength laser operation for this crystal. The lifetimes of the Yb3þ2F5/2 excited-state and the 4I13/2 and 4I11/2 excited-states for Er3þ ions are presented in Table 3. In this context, it is worth mentioning that even for a stoichiometric Cs2NaErF6 crystal, the value of τ(4I11/2) is as long as 0.7 ms at room- temperature [5], which indicates that it can be promising medium for 3 μm laser operation on the 4I11/2-4I13/2 transition [25]. UCL spectra of Er3þ:Cs2NaYF6 crystals under the excitation at 960 nm to the Er3þ4I11/2 state are shown in Fig. 7(a). For a 10 at% Er3þdoped crystal, the green emission band spanning from 510 to 580 nm and related to the transitions from the closely located and thermalized state 2H11/2 and 4S3/2 to the ground state 4I15/2Fig. 6. Luminescence decay curve for a 10 at% Yb3þ:Cs2NaYF6 crystal: λexc¼960 nm; luminescence is detected at 1020 nm. Fig. 7. Up-conversion luminescence (UCL) spectra for (a) 10 at% Er3þ:Cs2NaYF6 and Cs2NaErF6, (b) 1 at% Er3þ , 10 at% Yb3þ:Cs2NaYF6 and (c) Cs2NaYbF6 crystals; λexc¼960 nm; insets show images of the excited samples (a), (b) and details of blue emission from the Cs2NaYbF6 crystal (c): 1-measured UCL spectrum, 2-calculated spectrum of cooperative emission, Eq. (6). Table 4 CIE 1931 color coordinates x, y, dominant wavelength λd and color purity p for luminescence from Er3þdoped elpasolite crystals. Crystal x y λd, nm p Color Exc. 960 nm 10 at% Er3þ:Cs2NaYF6 0.385 0.603 562 98% Yellow–green Cs2NaErF6 0.343 0.656 556 99% Yellowish–green 1 at% Er3þ , 10 at% Yb3þ: Cs2NaYF6 0.340 0.660 555 99% Yellowish–green Exc. 355 nm 10 at% Er3þ:Cs2NaYF6 0.333 0.650 555 99% Yellowish–green Cs2NaErF6 0.325 0.586 553 75% Yellowish–green Table 3 Lifetimes of the excited-states of Er3þ and Yb3þ ions in Cs2NaYF6 crystals*. Ion Yb3þ ion Er3þ ion Er3þ ion concentration τ(2F5/2), ms τ(4I13/2), ms τ(4I11/2), ms This work/ RT [6]/RT This work/ RT [5]/4 K [5]/RT [5]/4 K 1 at% – – – 100 12 21 10 at% 6.3; 6.4rec – 32rec – 1.1 1.4 100 at% 5.7 5.63 – – 0.7 1.1 * RT - room temperature, REC - estimated with the reciprocity method. P.A. Loiko et al. / Journal of Luminescence 175 (2016) 260–266264dominates in the spectrum. Four intense peaks at 540, 551, 557 and 566 nm are observed within this emission band. The red emission in the range 630–700 nm related to the transition 4F9/2- 4I15/2 is much weaker than the green one. The ratio for integrated intensities of these bands (R/G ratio) is 0.27 which is referred to the domination of the excited-state absorption (ESA) over the cross-relaxation (CR) mechanism in generation of UCL, however, further time-resolved studies of UCL are required to support this [26]. In the blue region there is a weak emission band which is due to the transition from the higher-lying excited state 2H9/2 to the 4I15/2 ground-state. These features determine the yellow-green color of UCL from 10 at% Er3þ:Cs2NaYF6 with x¼0.385 and y¼0.603 in the 1931 CIE chromaticity coordinates as well as high color purity, p498%, caused by the dominant wavelength at 562 nm. Color purity p was calculated from the CIE 1931 chromaticity diagram with respect tothe CIE-E illuminant (uniform white, x¼0.333 and y¼0.333). It is defined as p¼a/b where a is the distance from the white point to the sample color point and b is the distance from the white point to the point on the spectral locus corresponding to the dominant wavelength. The color purity is a quantitative measure of the saturation of a particular color. For a stoichiometric Cs2NaErF6 crystal and a 1 at% Er3þ , 10 at% Yb3þ:Cs2NaYF6 crystals, very similar UCL spectra are observed, see Fig. 7. Color character- istics for UCL from the studied crystals are summarized in Table 4. In addition, UCL from a stoichiometric Cs2NaYbF6 crystal has been studied under the excitation at 960 nm to the Yb3þ2F5/2 state. The emission bands observed in Fig. 7(c) are due to ET from Yb3þ to impurity Tm3þ and Er3þ ions and UCL from Tm3þ dominates. Both Tm and Er are presented as trace impurities in ytterbium oxide, Yb2O3, reagent and thus their amount in stoi- chiometric crystal is enough to provide detectable UCL. The bands at 450–505, 640–680 and 750–820 nm are related to the transitions 1G4-3H6, 1G4-3F4 and 3H4-3H6 for Tm3þ , respectively, whereas weak green Er3þ emission from the 2H11/2 and 4S3/2 states to the 4I15/2 ground state is detected at 550 nm. The red Er3þ emission from the 4F9/2 state at 650 nm can overlap with the red Tm3þ one, so it is not discovered. Accordingly, UCL from the Cs2NaYbF6 crystal is blue–violet. In the previous study of a Cs2NaYbF6 crystal [6], the strong emission bad at 480 nm is at least partially attributed to coop- erative emission from Yb3þ–Yb3þ ion pairs [27]. This effect is known for materials with the strong clustering of Yb3þ ions [28]. In this case, a pair of closely located ions can form a virtual excited state with the energy 2E(2F5/2) 20,000 cm1. The emission from this state can be observed in the region 480–500 nm [29]. The emission spectrum can be calculated as the convolution of the near-IR emission spectrum of Yb3þ ions related to the 2F5/2-2F7/2 transition [27]: FcoopðEÞ ¼ Z FIRðE0ÞFIRðEE0ÞdE0: ð6Þ The result of this calculation is presented in the inset of Fig. 7(c). The cooperative emission should occur in the spectral range 475–510 nm with a maximum at 484 nm that is very close to the maximum of the 1G4-3H6 Tm3þ emission in the Cs2NaYF6 crystal [3]. Thus, it is difficult to distinguish these effects spectrally. In [6] it has been found that the decay time of blue emission from a Cs2NaYbF6 crystal is 2.73 ms, which is almost exactly half of τ(2F5/2) measured at 1 μm for Yb3þ ions. Such a correlation is expected for cooperative emission, τcoop¼τIR/2. Thus, blue UCL may be attributed to both Tm3þ impurity centers and cooperative emission. It should be also noticed that such intense UV up-conversion emissions can contribute to enhance the spectral response of photocatalytic semiconductor electrodes used in water-splitting processes for sustainable production of hydrogen, since they can help in bridging large bands gaps of efficient photocatalysts, like α-Fe2O3 (hematite), located at around 560 nm and eventually increase the efficiency of photoelectrochemical devices. Fig. 9. Luminescence of Cs2NaErF6 (a) and 1 at% Er3þ , 10 at% Yb3þ:Cs2NaYF6 (b) crystals after excitation into the 2G9/2 state at 355 nm and into the 2H11/2 state at 520 nm; the spectrum of Yb3þ emission from the Cs2NaYbF6 crystal is added in (b) for comparison. P.A. Loiko et al. / Journal of Luminescence 175 (2016) 260–266 265In Fig. 8(a), log–log plots for the UCL intensity (IUCL) versus the excitation power P are shown for a Cs2NaErF6 crystal. For the up- conversion process, IUCL is proportional to the nth power of P, i.e. IUCLPn [30] where n is the number of pump photons absorbed per up-converted photon emitted. A plot of log IUCL versus log P yields a straight line with slope n. For green emissions that occur from the 2H11/2 and 4S3/2 states, for the slope of this dependence n¼2.1 (524 nm) and 1.9 (557 nm), which means that two pump photons are required to populate the above mentioned states. There is the same situation for red emission from the 4F9/2 state at 660 nm where n¼2.1. Normally, excitation of Er3þ ions to the higher lying excited states is achieved in two steps, for example ground-state absorption (GSA) 4I15/2-4I11/2 followed by excited- state absorption (ESA) from the 4I11/2 or the 4I13/2 states. For Cs2NaErF6, cross-relaxation (CR) between the adjacent Er3þ ions, which can participate as an additional mechanism for the popu- lation of the 4F9/2 state, seems to be very weak. Indeed, the R/G ratio for UCL is not enhanced when the Er3þ concentration in Cs2NaYF6 increases from 10 to 100 at%, Fig. 7(a). This well corre- lates with the large distance between the isolated Y3þ sites in the Er3þ:Cs2NaYF6 crystal, so the probability of CR is not varied with the increase of the Er3þ concentration in the elpasolite hosts. No significant dependence of R/G ratio on the excitation power was detected. Similar slopes (n2) for the log–og plots of the UCL intensity vs. the excitation power are observed also for a 1 at% Er3þ , 10 at% Yb3þ: Cs2NaYF6 crystal, Fig. 8(b). In this case, the first step of the UCL mechanism is the excitation of Er3þ ions through the GSA 2F7/2-2F5/2 of Yb3þ ions and the energy-transfer from Yb3þ to Er3þ , 2F5/2(Yb3þ)-4I11/2(Er3þ). On the other hand, in any case, 2 pump infrared photons are required for the generation of one visible photon. More detailed discussion about the mechanisms of UCL in hosts containing Er3þ and Yb3þ can be found elsewhere [31]. In Fig. 8(a), the IUCL vs P plot for the blue UCL from a Cs2NaYbF6 crystal is also presented and the slope of this straight line is 2.4. This value is intermediate between the theoretical value of 2 for pure cooperative emission and 3 for pure Tm3þ1G4-3H6 emission. This supports our idea that the blue emission from the Cs2NaYbF6 crystal is due to the both processes. Under excitation into the 2G9/2 or the 2H11/2 states of Er3þ in Cs2NaYF6 at 355 nm or 520 nm, respectively, all the crystals singly doped with Er3þ ions demonstrate emission spectra similar to those obtained under near-IR excitation, Figs. 9(a), 3(a) and 7(a). The corresponding color coordinates can be found in Table 4. However, for a 1 at% Er3þ , 10 at% Yb3þ:Cs2NaYF6 crystal the spectra are different from those of Er3þ doped Cs2NaYF6 crystals. In particular, a broad emission band spanning from 940 to 1050 nm is detected. This band is clearly different from theFig. 8. Dependences of the UCL intensity on the excitation power in a log–log scale fo λexc¼960 nm; n is the number of pump photons absorbed per up-converted photon emluminescent band related to the 4I11/2-4I15/2 transition of Er3þ ions and has the spectral features of emission on the Yb3þ2F5/ 2- 2F7/2 transition. Excitation of Yb3þ ions is due to the so-called down-conversion (“quantum cutting”) process for the Er3þ–Yb3þ ion pairs [32,33]. It should be also noted that enhancement of the efficiency of the up- and down- conversion processes in cubic elpasolites is possible with the ytterbium compositions Cs2NaErxYb1xF6 con- taining relatively high Er3þconcentrations.4. Conclusions To conclude, we have studied absorption and luminescence of Er3þ and Yb3þ ions in cubic elpasolite Cs2NaYF6 crystals as well as in crystals of Cs2NaErF6 and Cs2NaYbF6 synthesized under hydro- thermal conditions. Stimulated-emission and gain cross-sections have been determined for the Yb3þ2F5/2-2F7/2 and the Er3þ4I13/2- 4I15/2 transitions in 10 at% Yb3þ:Cs2NaYF6 and 10 at% Er3þ: Cs2NaYF6 at room temperature. The maximum σSE values are 1.81021 cm2 at 993 nm (Yb3þ) and 3.81021 cm2 at 1535 nm (Er3þ). The possibility of dual-wavelength laser operation and wide tuning range exceeding 100 nm for laser emission arer (a) Cs2NaErF6, Cs2NaYbF6 and (b) 1 at% Er3þ , 10 at% Yb3þ:Cs2NaYF6 (b) crystals; itted. P.A. Loiko et al. / Journal of Luminescence 175 (2016) 260–266266expected for Yb3þ:Cs2NaYF6 crystals. Due to their structure peculiarities, elpasolite crystals provide exceptionally long radia- tive lifetimes of the excited-states for both Yb3þand Er3þ ions, τ (2F5/2)¼6.3 ms and τ(4I13/2) 32 ms, respectively, together with relatively weak UCL, which makes them attractive for high pulse energy Q-switched lasers. Under excitation at 960 nm, Cs2NaErF6 crystals provide yellowish–green UCL with CIE coordinates x¼0.353, y¼0.656. Down-conversion is detected for Er3þ ,Yb3þ: Cs2NaYF6 crystals.Acknowledgments This research was partially supported by the Russian Founda- tion for Basic Research (Research Project no. 15-03-02507a); Fundación CajaCanarias (AYE06) within the Project MAGEC (Materials for Advanced Generation of Energy at Canary Islands) and the Spanish Ministry of Economy and Competitiveness (Pro- ject ENE2013-47826-C4-4-R).References [1] G. Meyer, Prog. Sol. St. Chem. 14 (1982) 141. [2] L.R. Moras, J. Inorg. Nucl. Chem. 36 (1974) 3876. [3] V.N. Makhov, N.M. Khaidukov, D. Lo, J.C. Krupa, M. Kirm, E. Negodin, Opt. Mater. 27 (2005) 1131. [4] X. Zhou, P.A. Tanner, M.D. Faucher, J. Phys. Chem. C 111 (2007) 683. [5] H. Vrielinck, I. Izeddin, V.Y. Ivanov, T. Gregorkiewicz, F. Callens, D.S. Lee, A.J. Steckl, N.M. Khaidukov, Mater. Res. Soc. Symp. 866 (2005) V381. [6] D.S. Pytalev, A. Jaffres, P. Aschehoug, P.A. Ryabochkina, A.V. Malov, N.M. Khaidukov, M.N. Popova, J. Lumin. 153 (2014) 125. [7] M.L. Falina, K.I. Gerasimova, A.M. Leushin, N.M. Khaidukov, J. Lumin. 128 (2008) 1103. [8] X. Zhou, M.F. Reid, M.D. Faucher, P.A. Tanner, J. Phys. Chem. B 110 (2006) 14939.[9] B.Z. Malkin, D.S. Pytalev, M.N. Popova, E.I. Baibekov, M.L. Falin, K.I. Gerasimov, N.M. Khaidukov, Phys. Rev. B 86 (2012) 134110. [10] P.A. Tanner, M.D. Faucher, Chem. Phys. Lett. 445 (2007) 183. [11] P.A. Tanner, Y.L. Liu, N. Edelstein, K. Murdoch, N.M. Khaidukov, J. Phys. : Condens. Matter 9 (1997) 7817. [12] J.R.G. Thorne, M. Jones, C.S. McCaw, K.M. Murdoch, R.G. Denning, N.M. Khaidukov, J. Phys. : Condens. Matter 11 (1999) 7851. [13] A.J. Berry, I.D. Morrison, R.G. Denning, Mol. Phys. 93 (1998) 1. [14] W. Ryba-Romanowski, Z. Mazurak, B. Jezowska-Trzebiatowska, J. Lumin. 27 (1982) 177. [15] P.A. Tanner, C.S.K. Mak, W.-M. Kwok, D.L. Phillips, M.D. Faucher, Phys. Rev. B 66 (2002) 165203. [16] Z. Mazurak, E. Lujowiak, B. Jezowska-Trzebiatowska, W. Ryba-Romanowski, J. Lumin. 29 (1984) 47. [17] Z. Mazurak, E. Lujowiak, B. Jezowska-Trzebiatowska, J. Lumin. 33 (1985) 159. [18] F. Auzel, Chem. Rev. 104 (2004) 139. [19] G.N. Papatheodorou, J. Chem. Phys. 66 (1977) 2893. [20] S.A. Payne, L.L. Chase, L.K. Smith, W.L. Kway, W.F. Krupke, IEEE J. Quant. Electron. 28 (1992) 2619. [21] P.A. Loiko, E.A. Arbabzadah, M.J. Damzen, X. Mateos, E.B. Dunina, A.A. Kornienko, A.S. Yasukevich, N.A. Skoptsov, K.V. Yumashev, J. Lumin. 171 (2016) 226. [22] A.S. Yasyukevich, V.G. Shcherbitskii, V.E. Kisel, A.V. Mandrik, N.V. Kuleshov, J. Appl. Spectr. 71 (2004) 202. [23] P.A. Tanner, Mol. Phys. 63 (1988) 365. [24] B.F. Aull, H.P. Jenssen, IEEE J. Quantum Electron. 18 (1982) 925. [25] B.J. Dinerman, P.F. Moulton, Opt. Lett. 19 (1994) 1143. [26] J. Mendez-Ramos, V. Lavin, I.R. Martin, U.R. Rodriguez-Mendoza, J.A. Gonzalez- Almeida, V.D. Rodriguez, A.D. Lozano-Gorrin, P. Nunez, J. Alloy. Compd. 323– 324 (2001) 753. [27] Ph Goldner, F. Pelle, D. Meichenin, F. Auzel, J. Lumin. 71 (1997) 137. [28] F. Auzel, D. Meichenin, F. Pellé, P. Goldner, Opt. Mater. 4 (1994) 35. [29] P.A. Loiko, G.E. Rachkovskaya, G.B. Zakharevich, A.A. Kornienko, E.B. Dunina, A.S. Yasukevich, K.V. Yumashev, J. Non-Cryst. Solids 392–393 (2014) 39. [30] M. Pollnau, D.R. Gamelin, S.R. Luthi, H.U. Gudel, Phys. Rev. B 61 (2000) 3337. [31] P.A. Loiko, N.M. Khaidukov, J. Méndez-Ramos, E.V. Vilejshikova, N.A. Skoptsov, K.V. Yumashev, J. Lumin. 170 (2015) 1. [32] L. Aarts, B.M. van der Ende, A. Meijerink, J. Appl. Phys. 106 (2009) 023522. [33] J.J. Eilers, D. Biner, J.T. van Wijngaarden, K. Krämer, H.-U. Güdel, A. Meijerink, Appl. Phys. Lett. 96 (2010) 151106.