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Improved resonant energy transfer and light emission from SnO2 nanocrystals and Er3+ embedded in silica films via Yb3+ co-doping

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Abstract

SiO2-SnO2:Er3+ thin films co-doped with Yb3+ ions have been prepared by the sol-gel method. By controlling the Yb3+ concentration, the enhanced Er3+-related near infrared (NIR) emission is achieved under 325 nm excitation. The energy transfer efficiency (ETE) from SnO2 to rare earth is investigated by photoluminescence decay curves. It is found that with the increase of Yb3+ ion concentration to 15 mol%, the ETE gradually increases to ∼68.7%. The comprehensive spectroscopic analysis results demonstrate that both improved ETE and a new energy transfer channel from SnO2 nanocrystals to Er3+ ions via the Yb3+ intermediate state contribute to the Er3+-related NIR emission enhancement.

© 2022 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement

1. Introduction

Silicon-based light sources with 1.55 µm near infrared (NIR) emission are mandatory for Si-based monolithic optoelectronic integrations [1,2]. Erbium ions doped Si-based materials have aroused great interest because the electronic transition 4I13/24I15/2 of Er3+ ions around ∼1.55 µm [35]. Co-doping semiconductor nanocrystals (NCs) and exploiting the resonance energy transfer mechanism between semiconductor NCs and Er3+ ions have been proven as an effective way to improve luminescence efficiency [68]. However, Er3+ ions have abundant meta-stable levels, which are suitable not only for NIR emission but also for visible light emissions. Therefore, it would be very interesting to study regulate energy transfer processes, for reducing the transfer probability of visible light emission bands and mainly enhance the NIR emission at 1.55 µm of Er3+ ions.

Silica materials have been proved to be good host materials for optical interconnection, for their specialty on high rare earth (Re) solubility, transparency and compatibility with Si-integrated technology [9]. Tin dioxide is a unique semiconductor with a wide band gap of 3.59 eV at 300 K and high ultraviolet light absorption coefficient [10]. In addition, it has been shown that the emission spectrum of SnO2 defect states in SiO2-SnO2 thin films overlaps well with the excitation spectra of Er3+ ions. The matching of SnO2 NCs defect states and the 2H11/2/4S3/2 levels of Er3+ ions can provide efficient energy transfer [11]. Yb3+ ion has a two-level structure and is often used as sensitizer in up-conversion fluorescent materials due to its large absorption cross-section near 980 nm, as well as its energy level matching with the low excited state levels of other Re3+ ions [12]. Co-doping Yb3+ ions in SiO2-SnO2:Er3+ would introduce a new energy transfer channel from SnO2 NCs to Er3+ via Yb3+ intermediate state. Recently, Dung et al. prepared Er3+/Yb3+ co-doped SiO2-SnO2 glass ceramics and obtained enhanced Er3+ emission at 1.54 µm [13,14]. In SiO2-SnO2:Er3+/Yb3+ nanomaterials, the energy transfer efficiency from SnO2 NCs to Re3+ is an important parameter. However, to our knowledge, there were few literature studies on it. In this work, we prepared Yb3+ ions co-doped SiO2-SnO2:Er3+ thin films by using sol-gel method. The effects of Yb3+ doping concentration on the photoluminescence (PL) characteristics under 325 nm excitation are investigated. By controlling the Yb3+ ions doping concentration, the increased energy transfer efficiency from SnO2 NCs to Re3+ ions and the enhanced NIR emission of Er3+ ions are achieved.

2. Experimental section

Yb3+ ions co-doped SnO2-SiO2;Er3+ thin films were prepared by sol-gel method. In brief, tetraethyl orthosilicate (1 mL), deionized water (1 mL) and ethanol (2 mL) were mixed together via stirring, to form a transparent silica sol. As a catalyst, HCl was dropped into the precursor to adjust the pH valve close to 2.0. Subsequently, SnCl4·5H2O, Er(NO3)3·5H2O and Yb(NO3)3·5H2O were accurately weighted and dissolved in the precursor solution. The effects of Sn and Er3+ concentrations on fluorescence emission have been investigated in our previous work, and the optimal Sn and Er3+ concentrations are 20 mol% and 5 mol%, respectively [11]. Therefore, in this case, the amount of Sn and Er3+ were fixed at 20 mol% and 5 mol% of SiO2 amount, while Yb3+ ratio was changed from 0 to 15 mol%. The mixed solution was sealed and vigorously stirred at 60 °C for 4 hours and aged at room temperature for 24 hours. Then, 30 µL of as-prepared gel was extracted and spin-coated onto clean Si substrates with a speed of 4000 rpm for 30 seconds to form silica thin films. After drying at 100 °C for 1 hour, the obtained thin films were annealed at 1000 °C in an air ambient to form SnO2-SiO2:Yb3+;Er3+ thin films.

The microstructures of the thin films were investigated by X-ray diffraction (XRD, Rigaku Ultima III) and transmission electron microscopy (TEM, Tecnai G2 F20). Steady state PL, PL decay curves were measured by a fluorescence spectrophotometer (Edinburgh Photonics, FLS980). A UV-Visible-Infrared spectrophotometry (UV3600) was employed to record absorption spectra.

3. Results and discussion

Figure 1(a) shows a typical TEM image of 2 mol% Yb3+ ions co-doped SiO2-SnO2: 5 mol% Er3+ thin film annealed at 1000 °C for 1 hour in an air ambient. It can be clearly seen that the spherical morphology SnO2 nanocrystals dispersed in amorphous SiO2 matrix with an average diameter of about 9 nm. The inset in Fig. 1(a) is a high resolution TEM image. The well-distinguished lattice fringes in the high resolution TEM corresponding to the (110) plane of the tetragonal rutile phase SnO2 with a d-spacing of 3.41 Å. The nanostructures are further confirmed by the XRD. Figure 1(b) displays the XRD patterns of SiO2-SnO2: 5 mol% Er3+ films without and with 2 mol% Yb3+ ions. The characteristic diffraction peaks at 26.6°, 33.9°, 37.9°, 51.8°, 54.8°, 58.1°, 61.9°, 64.8°, 65.9° can be assigned to the diffractions from (110), (101), (200), (211), (220), (002), (310), (112), and (301) crystal planes of the tetragonal rutile phase SnO2 (JCPDS 05-0467). The diffraction peak (110) is consistent with the high resolution TEM observation.

 figure: Fig. 1.

Fig. 1. (a) TEM images of SiO2-SnO2:5 mol% Er3+/2 mol% Yb3+ ions. (b) XRD patterns of the SiO2-SnO2:5 mol% Er3+ films without and with 2 mol% Yb3+ ions

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The UV-Visible absorption spectra of SiO2-SnO2:Er3+ thin films doped with different Yb3+ concentrations are shown in Fig. 2. The absorption peak of ultraviolet band (<350 nm) is attributed to the band-gap absorption of SnO2 [15]. It can also be found that the Yb3+/Er3+ doped thin films exhibit obvious blue shift, comparing to the un-doped thin film. The optical bandgap of the thin films can be estimated by Tauc equation:

$$\alpha \textrm{ = }\frac{{A{{(hv - {E_g})}^\textrm{n}}}}{{hv}}$$
Where α is the optical absorption coefficient, A is a constant, h is the Planck’s constant, ν is the frequency of light, Eg is the optical band gap, and n = 0.5 for direct band gap semiconductor [16,17]. The plots of (α)2 versus photon energy are shown in inset of Fig. 2 and the optical bandgap energy can be estimated by extrapolation of the lines to zero. The optical bandgap energies are calculated to be 4.37, 4.50 and 4.56 eV for SiO2-SnO2, SiO2-SnO2:5%Er/0%Yb and SiO2-SnO2:5%Er/2%Yb, respectively. One can find that the optical bandgap energy of SiO2-SnO2 thin film is larger than 3.6 eV of bulk SnO2, and further increases with the addition of Er3+/Yb3+ ions. According to the XRD results, the full width at half maximum of the diffraction peaks increases with the introduction of Yb3+ ions, suggesting that the crystallite size becomes smaller. The results suggest that the blue shift of the absorption spectra can be attributed to the quantum-sized confinement effect of the nanosized SnO2 NCs in amorphous SiO2 thin film [18,19].

 figure: Fig. 2.

Fig. 2. Absorption spectra of SiO2-SnO2:Er3+ thin films with varying Yb3+ concentrations.

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Room temperature PL spectra of SiO2-SnO2:Er3+ thin films co-doped with different Yb3+ concentrations are recorded by a fluorescence spectrophotometer under the excitation wavelength of 325 nm. As shown in Fig. 3(a), for the SiO2-SnO2 thin film with Re3+-free, a broad visible emission band centered at 530 nm can be observed, which is originated from the radiative recombination of the defect-states of SnO2 nanocrystals [20]. It is very clear that co-doping with 5 mol% Er3+ ions attenuates the SnO2 NCs signal and produces Er3+-related green emissions (525 nm, 549 nm and 565 nm), red emission (662 nm and 682 nm) and NIR emission (1532 nm) corresponding to the 2H11/2/4S3/24I15/2, 4F9/24I15/2 and 4I13/24I15/2 transitions of Er3+ ions, respectively. The result indicates that there is an efficient energy transfer process between SnO2 NCs and Er3+ ions [11,21]. In addition, when Yb3+ ions are introduced into the thin films, a NIR emission band at 970 nm can be observed, which is assigned to the 2F5/22F7/2 transition of Yb3+ ions. It can be found that with the increase of Yb3+ concentration, the intensity of visible emission band gradually decreases, while the 1532 nm NIR emission of Er3+ ions increases first and then decreases. The integrated intensity of visible and 1532 nm NIR emissions are calculated respectively, and the data are plotted in Fig. 3(b). When co-doping with Yb3+ ions, the reduction in visible fluorescence can be attributed to the following factors. Co-doping Yb3+ ions into SiO2-SnO2:Er3+ thin films can introduce a new energy transfer channel from SnO2 NCs to 2F5/2 level of Yb3+ ions, so that part of the energy of SnO2 NCs is transferred to Yb3+ ions, resulting in weakened visible light emissions [13]. Furthermore, increasing Yb3+ content will promote cross-relaxation (CR) process between Yb3+ and Er3+ ions: 2F7/2(Yb3+)+4S3/2(Er3+)→2F5/2(Yb3+)+4I13/2(Er3+), which can depopulate the 4S3/2 levels of Er3+ ions and in turn attenuate the visible light emission of Er3+ ions. Concentration quenching effect at high Yb3+ content is also one of the reasons. For NIR emission of Er3+ ions, the intensity reaches its maximum when the Yb3+ ion concentration is about 2 mol%, and then gradually decreases. Yb3+ ion usually acts as a sensitizer, due to its simple energy levels structure, large absorption cross-section and efficient energy transfer to Re3+ ions. In Yb3+-Er3+ system, the 2F5/2 level of Yb3+ matches well with the 4I11/2 level of Er3+. As mentioned above, the establishment of energy transfer channel from SnO2 NCs will populate 2F5/2 level of Yb3+ and promote the efficient ET process from 2F5/2 level of Yb3+ to 4I11/2 level of Er3+, resulting in the enhancement of NIR emission of Er3+ ions. When the Yb3+ concentration increased higher than 2 mol%, the NIR emission of Er3+ ions gradually weakens, which can be attributed to the concentration quenching effect caused by high Yb3+ concentration.

 figure: Fig. 3.

Fig. 3. (a) PL spectra of SiO2-SnO2:Er3+ thin films with varying Yb3+ concentrations. (b) The normalized PL intensity versus the Yb3+ concentration. (c) Diagram of the energy levels in SiO2-SnO2:Er3+/Yb3+ thin film under 325 nm excitation.

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In order to investigate the energy transfer processes from the defect-states of SnO2 nanocrystals to Re3+ ions, the PL decay curves of SnO2 nanocrystals emission at 530 nm for SiO2-SnO2 thin films doped with different concentrations of Er3+/Yb3+ ions are measured by using a 375 nm picosecond laser (see Fig. 4(a)). It is clear that 530 nm emission from SiO2-SnO2:Er3+/Yb3+ decays faster than that of SiO2-SnO2:Er3+ thin film, and the lifetime of 530 nm emission of SnO2 nanocrystals becomes shorter with the increase of Yb3+ concentration. The gradually declined lifetime can be attributed to the energy transfer process from SnO2 nanocrystals to Yb3+ ions, which contributes to the increase of the nonradiative decay rate of SnO2-related emission. The result indicates that introduction of Yb3+ ions does establish a new energy transfer channel from SnO2 nanocrystals to Yb3+ ions. The average lifetime of the emission at 530 nm can be estimated by the following equation [11]:

$${\tau _{\textrm{average}}}\textrm{ = }\int {\frac{{I(t)}}{{{I_{\textrm{max}}}}}} dt$$
Where I(t) is the time-dependent PL intensity at 530 nm, Imax is the maximal PL intensity at the initial time. The calculated average lifetime values of SnO2 emission are 5.11 ns, 2.60 ns, 2.39 ns, 2.23 ns, 2.22 ns, 1.89 ns for Re3+-free sample, 5 mol%Er3+/x mol%Yb3+(x = 0, 2, 5, 7 and 10) samples, respectively. The energy transfer efficiency from SnO2 NCs to Re3+ ions can be defined as the ratio of defect-states of SnO2 NCs, which are depopulated by energy transfer to Re3+ ions over the total number of defect-states of SnO2 NCs [22]. The energy transfer efficiency can be expressed as:
$${\eta _{\mathrm{5\%Er/x\%Yb}}} = 1 - \frac{{{\tau _{\mathrm{5\%Er/x\%Yb}}}}}{{{\tau _{\mathrm{0\%Er/0\%Yb}}}}}$$
where τ is average lifetime, x%Yb stands for the Yb3+ concentration. The energy transfer efficiency from SnO2 nanocrystals to Er3+/Yb3+ ions is calculated and plotted as a function of Yb3+ concentration, as shown in Fig. 4(b). As the Yb3+ concentration increases from 0 mol% to 10 mol%, the energy transfer efficiency enhances from 49.12% to 63.01%. We also prepared 15 mol% Yb3+ co-doped SiO2-SnO2:Er3+ thin film. Under a 325 nm laser excitation, the visible and NIR emissions are further weakened, which can be attributed to the concentration quenching at high Yb3+ ions concentration. The corresponding NIR emission spectrum is shown in the inset in Fig. 4(c). Furthermore, the energy transfer efficiency of 15 mol% Yb3+ co-doped thin film is also investigated. According to the PL decay curve of 15 mol% Yb3+ co-doped thin film in Fig. 4(c), the mean life time is estimated to be 1.60 ns. Then, it can be calculated that the energy transfer efficiency is about 68.7%. The results suggest that the concentration quenching effect plays a dominant role in the photoluminescence at high Yb3+ ions concentration.

 figure: Fig. 4.

Fig. 4. (a) PL decay curves of SnO2 emission at 530 nm for the thin films with different Yb3+ concentrations. (b) Lifetime of SnO2 emission and energy transfer efficiency as a function of Yb3+ concentration. (c) PL decay curve of SnO2 emission for 15 mol% Yb3+ co-doped SiO2-SnO2:Er3+ thin film; the inset is the corresponding NIR PL spectrum.

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4. Conclusion

In summary, Yb3+ ions co-doped SiO2-SnO2:Er3+ thin films have been prepared by employing a sol-gel method with spin-coating technique. The introduction of Yb3+ ions can establish a new energy transfer channel from SnO2 NCs to Er3+ ions via Yb3+ intermediate state, resulting in weakened visible light emission and enhanced Er3+-related NIR emission. By controlling Yb3+ ions concentration, the Er3+-related NIR emission can be increased by about 1.5-fold. The results of PL decay curves of SnO2 NCs emission indicate that the ETE of SnO2 NCs to Re3+ ions is increased gradually with the increase of Yb3+ concentration. For the thin film with 15 mol% Yb3+ ions, the estimated ETE is about 68.7%. The SiO2-SnO2:Er3+/Yb3+ thin films would be a definitely promising candidate for the electroluminescence devices.

Funding

National Key Research and Development Program of China (2018YFB2200101); National Natural Science Foundation of China (61735008, 62004078, 61921005); University Natural Science Research Project of Anhui Province (KJ2021A1087); Natural Science Foundation of Jiangsu Province (BK20201073); Natural Science Research of Jiangsu Higher Education Institutions of China (20KJB510017).

Disclosures

The authors declare no conflicts of interest.

Data Availability

Data underlying the results presented in this paper are not publicly available at this time but may be obtained from the authors upon reasonable request.

References

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Data Availability

Data underlying the results presented in this paper are not publicly available at this time but may be obtained from the authors upon reasonable request.

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Figures (4)

Fig. 1.
Fig. 1. (a) TEM images of SiO2-SnO2:5 mol% Er3+/2 mol% Yb3+ ions. (b) XRD patterns of the SiO2-SnO2:5 mol% Er3+ films without and with 2 mol% Yb3+ ions
Fig. 2.
Fig. 2. Absorption spectra of SiO2-SnO2:Er3+ thin films with varying Yb3+ concentrations.
Fig. 3.
Fig. 3. (a) PL spectra of SiO2-SnO2:Er3+ thin films with varying Yb3+ concentrations. (b) The normalized PL intensity versus the Yb3+ concentration. (c) Diagram of the energy levels in SiO2-SnO2:Er3+/Yb3+ thin film under 325 nm excitation.
Fig. 4.
Fig. 4. (a) PL decay curves of SnO2 emission at 530 nm for the thin films with different Yb3+ concentrations. (b) Lifetime of SnO2 emission and energy transfer efficiency as a function of Yb3+ concentration. (c) PL decay curve of SnO2 emission for 15 mol% Yb3+ co-doped SiO2-SnO2:Er3+ thin film; the inset is the corresponding NIR PL spectrum.

Equations (3)

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α  =  A ( h v E g ) n h v
τ average  =  I ( t ) I max d t
η 5 % E r / x % Y b = 1 τ 5 % E r / x % Y b τ 0 % E r / 0 % Y b
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