Open Access Article
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Dual-emission center ratiometric optical thermometer based on Bi3+ and Mn4+ co-doped SrGd2Al2O7 phosphor

Yi Yu *ab, Kai Shaoab, Chonghui Niuab, Mingjie Danab, Yingying Wanga, Xiourong Zhuabc, Xianke Zhanga and Yeqing Wang*d
aSchool of Physics and Electronic Information, Gannan Normal University, Ganzhou 341000, China. E-mail: yuyignnu@163.com
bAdvanced Energy Storage & Photoelectric Materials Research Center, Gannan Normal University, Ganzhou 341000, China
cShanghai Key Laboratory of Special Artificial Microstructure Materials & Technology, Department of Physics, Tongji University, Shanghai 200092, China
dDepartment of Applied Physics, East China Jiaotong University, Nanchang, 330013, Jiangxi, China. E-mail: jxdxmeng@126.com

Received 2nd September 2023 , Accepted 19th October 2023

First published on 30th October 2023


Abstract

In recent years, more and more attention has been paid to optical temperature sensing, and how to improve its accuracy is the most important issue. Herein, a new temperature sensing material, SrGd2Al2O7:Bi3+,Mn4+, based on fluorescence intensity ratio was designed in this work. It has both blue-purple and red luminescence under 300 nm excitation, and the dual-emitting centers with distinct colors, the different thermal sensitivities of Bi3+ and Mn4+, and the energy transfer between Bi3+ and Mn4+ give it excellent signal resolution and accurate temperature detection. The Sa of SrGd2Al2O7:0.04Bi3+,0.003Mn4+ phosphor reaches a maximum value of 8.573% K−1 at 473 K, and the corresponding Sr is 1.927% K−1, both of which are significantly better than those of most other reported optical temperature sensing materials. Taking all the results into account, the SrGd2Al2O7:0.04Bi3+,0.003Mn4+ phosphor can be regarded as a prominent FIR-type temperature sensing material.


1. Introduction

Temperature is a physical quantity that shows how hot or cold something is. It is a fundamental and important physical quantity in daily life, industrial applications, scientific research, etc. Currently, thermometers can be divided mainly into contact type and non-contact type. The working principle of the contact type is based mainly on the thermocouple characteristics or the Seebeck effect, the latter relying on temperature-dependent optical properties.1

Traditional contact thermometers have limitations in application to biological tissue, or in a corrosive or strongly magnetic environment. For example, in the outbreak of the novel coronavirus pneumonia from December 2019, the virus is highly contagious, and the use of contact temperature measuring instruments greatly increases the risk of virus transmission, so non-contact measurement is an ideal choice to resolve this problem. Even in a variety of other fields, non-contact temperature measurement is still preferred. However, although many kinds of non-contact temperature sensors are emerging in the market at present, most of them are greatly affected by the environment, resulting in low measurement accuracy and large error, which makes the test results less repeatable. An optical temperature sensor can not only easily realize non-contact measurement, but also maintain high measurement accuracy in a special measurement environment. It also has incomparable advantages over traditional contact temperature sensors in terms of volume, response speed and sensitivity. Therefore, research on optical temperature sensors has attracted more and more attention.2

Owing to their abundant and complex energy levels and temperature-sensitive optical behavior, lanthanide-ion-based fluorescence intensity ratio (FIR)-type temperature measurement materials are taking a leading role in the field of temperature sensing materials. However, their band gaps are often relatively narrow, leading to problems, including overlap of two transmitted signals, large detection deviation and poor resolution. These drawbacks in turn limit their ability to measure temperature with high accuracy.3,4 In order to overcome these shortcomings, temperature sensing materials based on multiple emission centers with different thermal sensitivities, such as rare earth/rare earth (Re/Re) or transition metal/rare earth (Tr/Re) ion co-doped materials, have been designed in recent years. Among these co-doped materials, Eu3+/Tb3+, Eu3+/Bi3+, and Eu3+/Dy3+ groups have revealed excellent temperature sensing ability.5–7 However, there are few reports on temperature sensing materials doped by double transition group metal elements. The luminescence properties of Bi3+ ions are easily affected by the crystal field environment where the ions reside. Based on their adjustable luminescence, Bi3+ ions are often selected as efficient sensitizers for activator ions. For instance, a lot of studies about enhancing the luminescent properties of Eu3+, Pr3+, and Tb3+ by means of co-doping Bi3+ ions as a sensitizer have been reported.6,8,9 On the other hand, Bi3+ itself can usually emit blue-purple light and its intensity depends on temperature, which makes it suitable for temperature sensing by measuring the fluorescent intensity at different temperatures. But this mono-band method for temperature sensing often suffers drawbacks, such as relatively low accuracy, low signal resolution and larger error. Compared to this method, the dual-emission center ratiometric method is advantageous. Hence, apart from the blue-purple emission band from Bi3+, another ion should be selected to offer a different emission band. Because of its preeminent optical properties, Mn4+-based red-emitting phosphors were regarded as promising fluorescent materials. More and more Mn4+-doped phosphors have gained a lot of attention recently. The good match between the 4T2g state of Mn4+ and the 3P1 state of Bi3+ provides a strategy for designing a temperature sensing material based on the fluorescent intensity ratio of the blue-purple emission to red emission. Therefore, we designed a new type of thermometer based on energy transfer between Bi3+ and Mn4+ using SrGd2Al2O7 (SGAO) as a matrix. The physical and chemical properties of SGAO are stable, and the Gd(Sr) atoms are distributed at two different sites, forming nine- and twelve-fold coordinated polyhedrons, which provides a good crystal field environment for Bi3+ ion substitution. In addition, the [AlO6] octahedron is very suitable for Mn4+ ion substitution and far-red emission (Fig. 1). Therefore, the emission of Bi3+ ions and Mn4+ ions is very easy to distinguish, and it can be predicted that this temperature sensing material should have good signal detection ability. Moreover, because of the energy transfer from sensitizer Bi3+ ions to activator Mn4+ ions, it is more suitable for design as an FIR-based dual-emission center temperature sensing material.


image file: d3ra05988j-f1.tif
Fig. 1 Structure framework of SGAO compound and Gd(Sr)–O, Al–O polyhedrons.

2. Experimental

2.1 Synthesis

A series of SGAO:xBi3+,yMn4+ (0.01 ≤ x ≤ 0.075; 0 ≤ y ≤ 0.01) phosphors were prepared by a high-temperature solid-state reaction. Raw materials SrCO3 (99.5%), Gd2O3 (99.99%), Al2O3 (99.99%), MnCO3 (99.99%), Al2O3 (99.99%), Bi2(CO3)3 (99.99%) were all purchased from Aladdin Reagents. They were stoichiometrically weighted according to the chemical equation:
 
SrCO3 + (1 − x)Gd2O3 + (1 − y)Al2O3 + 2yMnCO3 + xBi2(CO3)3 → SrGd(2−2x)Bi2xAl(2−2y)Mn2yO7 (1)
where x and y represent the doping concentrations of Bi3+ ions and Mn4+ ions, respectively. The mixtures were thoroughly ground for about 40 minutes and then transferred into a corundum crucible for calcining. A muffle furnace was adopted and the temperature was increased to 1550 °C at a heating rate of 3 °C min−1 in air. The temperature was kept constant for 10 hours. After natural cooling to room temperature, the products were ultimately obtained.

2.2 Properties measurements

XRD diffraction measurement was conducted on a high-resolution X-ray powder diffractometer (Rigaku Ultima-IV) with Cu Kα radiation as the radiative source to analyze the phase of the SGAO:xBi3+,yMn4+ (0.01 ≤ x ≤ 0.075; 0 ≤ y ≤ 0.01) phosphors. The signals were recorded in the range of 20–65° at a rate of 2° min−1. A scanning electron microscope (JSM-6700F) was used to obtain the surface morphology information for the samples. To measure the PL and PLE spectra, a fluorescence spectrometer (Hitachi-2500) equipped with a 150 W xenon lamp as the light source was adopted. The measurement of temperature-dependent emission spectra and decay curves were implemented on an Edinburgh FLS 980 spectrometer. The temperature fluctuated from 303 K to 473 K.

3. Results and discussion

3.1 Phase and morphology analysis

The XRD patterns of all SGAO:Bi3+ and SGAO:Bi3+,Mn4+ samples are shown in Fig. 2, accompanied by the standard pattern for the pure phase of SGAO compound (PDF# 76-0095). All the diffraction patterns are obviously very well matched with the standard PDF card for pure SGAO compound without the appearance of any additional diffraction peaks, indicating that all the samples obtained have the same phase as the SGAO compound. In order to determine the substitution position of dopant ions, the value of the percentage difference of radius (Dr) can be calculated with the following equation:10
 
image file: d3ra05988j-t1.tif(2)
where Rm and Rd are the radii of host ion and doping ion, respectively, and CN refers to the coordination number of the corresponding ions. The smaller the value of Dr, the easier it is to replace the host ions. According to eqn (2), the Dr values for the cases of a Bi3+ ion replacing a Gd3+ ion and an Al3+ ion are 2.70% and 111.11%, and the Dr values for the cases of an Mn4+ ion replacing a Gd3+ ion and an Al3+ ion are 52.25% and 1.85%, respectively. Therefore, it is rational to claim that Bi3+ ions replace Gd3+ ions and Mn4+ ions occupy the Al3+ sites.

image file: d3ra05988j-f2.tif
Fig. 2 XRD patterns of (a) SGAO:xBi3+ (0.01 ≤ x ≤ 0.075) and (b) SGAO:0.04Bi3+,yMn4+ (0.0005 ≤ y ≤ 0.0125).

Fig. 3(a) and (b) show the SEM images of the SGAO:0.04Bi3+,0.003Mn4+ phosphor taken at different magnification rates. It can be seen from the figures that the morphology of the samples is irregular and there is a certain degree of agglomeration, which is a common phenomenon for materials synthesized through a traditional high-temperature solid-state reaction. The size of phosphor is estimated to be about 1–5 μm.


image file: d3ra05988j-f3.tif
Fig. 3 SEM images of SGAO:0.04Bi3+,0.003Mn4+ phosphors at low (a) and high (b) magnification.

3.2 Photoluminescence properties

In order to investigate the photoluminescence characteristics of Bi3+ and Mn4+ ions in the SGAO host, the photoluminescence excitation (PLE) and photoluminescence (PL) spectra of SGAO:Bi3+ and SGAO:Mn4+ were performed and the results are shown in Fig. 4(a) and (b), respectively. The PLE spectrum of SGAO:Bi3+, in a wavelength range of 265–335 nm with the maximum peak at 300 nm is the typical electronic transition band of Bi3+, which corresponds to the transition from ground-state 1S0 to excited-state 3P1. Excited at 300 nm, the emission spectrum of SGAO:Bi3+ has only a single band with a wavelength range of 350–510 nm, and the peak is located at about 404 nm. This broad emission band is ascribed to the 3P11S0 transition of Bi3+.11 The PLE spectrum of SGAO:Mn4+ consists of two bands in the wavelength ranges of 270–440 nm and 440–550 nm, with their corresponding peaks of 340 nm and 487 nm. Under excitation at 340 nm, SGAO:Mn4+ shows a single emission band in the wavelength range of 670–760 nm, which corresponds to the 2Eg4A2g transition of an Mn4+ ion in an [AlO6] octahedral environment. Comparing the emission band of a Bi3+ ion and excitation band of an Mn4+ ion, it is intriguing to note that they overlap significantly with each other, as shown in Fig. 4(b), indicating a rational strategy in which the intensity of luminescence of Mn4+ ions can be enhanced by Bi3+ ions, which play the role of sensitization.10,12
image file: d3ra05988j-f4.tif
Fig. 4 Excitation (PLE) and emission spectra (PL) of (a) SGAO:Bi3+ and (b) SGAO:Mn4+.

Fig. 5(a) shows the PL spectra of SGAO:xBi3+ (0.01 ≤ x ≤ 0.075) over a range of 350–510 nm. With the change in doped Bi3+ ion concentration, all the PL spectra keep the same shapes without obvious red shift or blue shift, and they are centered at 404 nm. However, the emission intensity fluctuates greatly with variation in the concentration of Bi3+ ions. The inset in Fig. 5(a) shows the variation in emission intensities at 404 nm with the increase in Bi3+ concentration. As one can see, the emission intensity of the SGAO:xBi3+ (0.01 ≤ x ≤ 0.075) phosphor first increases at lower doping concentration and then decreases at higher doping concentration. It reaches its maximum altitude when x = 0.04, indicating that the optimized concentration of Bi3+ ions should be 4 at%. To explore the quenching mechanism of the concentration of the SGAO:Bi3+ phosphor, the critical distance (Rc) can be calculated as follows:13

 
image file: d3ra05988j-t2.tif(3)
where V is the volume of a unit cell, N means the number of substitutable cations in the host matrix in a unit cell, and xc represents the critical concentration of activator ions. In the SGAO matrix, V = 271.56 Å3, xc = 0.04, N = 4. Thus, the value of Rc was calculated to be 14.8 Å, much greater than 5 Å. Therefore, it can be assumed that the quenching mechanism is the multipole interaction mechanism. For a further determination of the type of interaction mechanism between Bi3+ ions, the following formula based on Dexter's theory was adopted:14
 
image file: d3ra05988j-t3.tif(4)
where I is the emission intensity, x represents the doping concentration, A denotes a constant, and Q = 6, 8, and 10 correspond to dipole–dipole, dipole–quadrupole, and quadrupole–quadrupole interactions, respectively. Fig. 5(b) shows log(I/x)as a function of log(x). By the linear fitting method, the slope is determined to be −1.16. Further calculation shows that Q is 3.48, which is closer to 6, indicating that the dipole–dipole interaction between Bi3+ ions in the SGAO matrix is responsible for the concentration quenching.


image file: d3ra05988j-f5.tif
Fig. 5 (a) Emission spectra of SGAO:xBi3+ (0.01 ≤ x ≤ 0.075) phosphors; (b) log(I/x) dependence on log(x).

With the concentration of Bi3+ kept constant at 4 at%, samples with Mn4+ co-doped at different concentrations were fabricated and the effect of Mn4+ concentration on the luminescence properties was investigated. Fig. 6(a) shows the broad emission band of SGAO:0.04Bi3+, yMn4+ (0 ≤ y ≤ 0.01) phosphors corresponding to the 3P11S0 transition of Bi3+ measured in a 350–510 nm range,15 as well as the emission band in the 670–760 nm ascribed to the 2Eg4A2g transition of Mn4+.16 Fig. 6(b) depicts the luminescence intensity of Bi3+ and Mn4+ ions depending on the different concentrations of Mn4+ ions. With the increase in Mn4+ concentration, the emission intensity of Mn4+ ions increases first and then decreases. And when y = 0.003, it reaches the summit. In contrast, the emission intensity of Bi3+ ions decreases along with the rise in Mn4+ ion concentration, which is because of the existence of energy transfer process from Bi3+ ion to Mn4+ ion. The reason for the phenomenon that the emission intensity of Mn4+ ions increases first and then decreases can be ascribed to the integrative effects of energy transfer from Bi3+ to Mn4+ ions and the concentration quenching of the Mn4+ ion itself. Evidence for this hypothesis can be extracted from the fact that the optimized concentration of Mn4+ ions, namely 0.3 at%, rather than 0.1 at% which was reported in our very recent studies into the Mn4+-single doped SGAO phosphor.17 As such, this change in the optimum concentration of Mn4+ ions from 0.1 at% in SGAO to 0.3 at% in SGAO:0.04Bi3+,Mn4+ demonstrates that the procedure of energy transfer from Bi3+ to Mn4+ ions does occur in the Bi3+and Mn4+co-doped SGAO phosphor. Furthermore, when 0.001 ≤ y ≤ 0.003, the positive effect of energy transfer from Bi3+ to Mn4+ ions is stronger than the negative effect of Mn4+ ion concentration quenching. However, when y is larger than 0.003, the interaction between adjacent Mn4+ ions becomes much stronger, which gives the significant effect of emission weakness by concentration quenching the lead role in competition with the energy transfer process.


image file: d3ra05988j-f6.tif
Fig. 6 (a) Emission spectra of phosphors SGAO:0.04Bi3+,yMn4+ (0 ≤ y ≤ 0.01). (b) The luminescence intensity of Bi3+ and Mn4+ ions vary with the doping concentration of Mn4+ ions.

As the decay characteristic of the Bi3+ and Mn4+ ions is an effective way to reveal the mechanism of energy transfer between the two kinds of ions, the fluorescence lifetimes of Bi3+ in the series of SGAO:0.04Bi3+,yMn4+ (0 ≤ y ≤ 0.01) phosphors were measured. All the phosphors were excited at 300 nm and monitored at 404 nm and the decay curves are portrayed in Fig. 7. The decay curves were fitted with a double-exponential formula which can be expressed as follows:18,19

 
image file: d3ra05988j-t4.tif(5)
where It is the luminescence intensity changing with time, A1 and A2 are constants, τ1 and τ2 represent the decay coefficients, and τave means the average fluorescence lifetimes. Based on this equation, the lifetimes of Bi3+ ions in the SGAO co-doped with Mn4+ were obtained. As anticipated, they continuously decrease with an increase in Mn4+ ion concentration, from 325 ns to 67 ns as y goes up from 0 to 0.01. In addition, the shrinkage of the lifetimes of Bi3+ ions become faster with the increase in y values. The reason for this is mainly because the higher the concentration of Mn4+ ions, the shorter the distance between Bi3+ ions and Mn4+ ions, and as a consequence, the energy transfer of Bi3+ → Mn4+ was boosted with higher efficiency and this obviously leads to the shortened luminescence lifetimes of Bi3+ ions. The efficiency of energy transfer from Bi3+ to Mn4+ can be calculated with the following formula:20
 
image file: d3ra05988j-t5.tif(6)
where τ0 is the lifetime of Bi3+ ions when Mn4+ ions are absent, and τ is the lifetime when Mn4+ ions are co-doped with different concentrations. Therefore, the efficiencies for the SGAO:0.04Bi3+,yMn4+ (0.001 ≤ y ≤ 0.01) phosphors are 9.5%, 25.5%, 41.5%, 58.5%, and 79.4%, respectively. Interestingly, the efficiencies increase with a rise in Mn4+ ion concentration, and these results further demonstrate the aforementioned hypothesis.


image file: d3ra05988j-f7.tif
Fig. 7 Decay curve of SGAO:0.04Bi3+,yMn4+ (0 ≤ y ≤ 0.01) phosphors at room temperature.

According to the above results and analysis, the electron transition and energy transfer processes in the SGAO:0.04Bi3+,yMn4+ (0 ≤ y ≤ 0.01) phosphors are inferred, as shown in Fig. 8. When SGAO:0.04Bi3+,yMn4+ (0 ≤ y ≤ 0.01) phosphors are excited, a certain proportion of electrons from Bi3+ ions transfer from the 1S0 ground state to the 3P1, 3P2 and 1P1 excited states. Then they gradually relax from 1P1 to 3P2 and 3P1 states in a non-radiative process, resulting in energy consumption, which is regarded as an adverse effect. For the electrons in the 3P1 state, a proportion of them directly transit to the 1S0 ground state, accompanied by photon emission at the wavelength of 404 nm. Meanwhile, the rest of the electrons transfer their energy to the electrons in the 4T2g state of neighboring Mn4+ ions and successively relax to the 2Eg state. For the Mn4+ ions themselves, electrons in the excited states 4T1g, 2T2g and 4T2g will non-radiatively transit to the 2Eg state. Therefore, with the assistance of Bi3+ ions, the red emission of Mn4+ ions at 709 nm corresponding to the 2Eg4A2g transition can be achieved and the emission intensity is inevitably related to the concentration of Mn4+ ions.21


image file: d3ra05988j-f8.tif
Fig. 8 Electron transition and energy transfer of SGAO:Bi3+,Mn4+.

3.3 Temperature sensing behavior

Fig. 9(a) shows the emission spectra of SGAO:0.04Bi3+,0.003Mn4+ phosphors at different temperatures within 303–473 K. The sample was excited at 300 nm. With an increase in temperature, both the emissions originated from Bi3+ ions at 404 nm and from Mn4+ ions at 709 nm decrease in turn, but the rates of descent are different. As shown in Fig. 9(b), in the temperature range of 303–393 K, the emission intensity of Bi3+ ions decreases faster, while in the temperature range of 393–473 K, the emission intensity of Mn4+ ions decreases faster. Considering this characteristic, it is rational to design a new type of optical temperature sensor based on the fluorescence intensity ratio in these two temperature ranges.
image file: d3ra05988j-f9.tif
Fig. 9 (a) Temperature-dependent emission spectra of SGAO:0.04Bi3+,0.003Mn4+ phosphors. (b) The relationship between the emission intensity of Bi3+ (Mn4+) and temperature.

Fig. 10(a) shows the configuration coordinate diagram of Bi3+. At room temperature, electrons transition to excited states of 3P2 and 1P1 by absorbing energy, and then relax to the 3P1 state by non-radiative transition. Finally, electrons transition to the 1S0 ground state and release photons, and the correlation path is expressed as (O → A → B → C → D → O). But at higher temperatures, due to the fluctuation of the energy band, intersection between excited-state 3P1 and ground-state 1S0 usually occurs, denoted as point E in Fig. 10(a). Therefore, a proportion of electrons in the 3P1 excited state will non-radiatively relax to ground-state 1S0 through this intersection. The whole correlation path can be depicted as (O → A → B → C → D → E → O). In addition, the higher the temperature, the more frequently the electrons transit to the ground state through the non-radiative channel.22 Obviously, this side effect will give rise to a weakness in emission intensity. When it comes to the Mn4+ ions, the mechanism of thermal quenching is similar to that of Bi3+ ions discussed above, and the configuration coordinate diagram of Mn4+ is shown in Fig. 10(b).


image file: d3ra05988j-f10.tif
Fig. 10 Configuration coordinate diagrams of (a) Bi3+ and (b) Mn4+.

Based on Struck and Fonger theory, the relationship between photoluminescence intensity and temperature can be defined by the following formula:23

 
image file: d3ra05988j-t6.tif(7)
where IT represents the photoluminescence intensity at a specified temperature, I0 means the photoluminescence intensity at the initial temperature, T is the absolute temperature, A is a constant, kB is the Boltzmann constant, and ΔE is the activation energy of the hot quenching process. According to the above formula, the relationship between FIR and T can be deduced as follows:24–26
 
image file: d3ra05988j-t7.tif(8)
where B and D are related parameters. After the experimental data of FIR was fitted, a successive FIR curve could be obtained. Then the absolute sensitivity (Sa) that represents the change in FIR value when the temperature changes by 1 K can be calculated as follows:25
 
image file: d3ra05988j-t8.tif(9)

And the relative sensitivity (Sr) which represents the ratio of absolute sensitivity (Sa) to FIR can be calculated with the following formula:26

 
image file: d3ra05988j-t9.tif(10)

Fig. 11 depicts the scatter diagram for the FIR (IMn4+/IBi3+) of SGAO:0.04Bi3+,0.003Mn4+ phosphor as a function of temperature over the range 303–473 K and the corresponding range of the horizontal coordinate (1/T) is 0.0021–0.0033 K−1. From this figure, one can see that the value of FIR shows a trend of first increasing and then decreasing and the turning point appears at 393 K. Thus, the fitting analysis was separately carried out in the range of 393–473 K and 303–393 K. For the first section, namely in the range of 0.0021–0.0025 K−1, the fitting curve, as shown in Fig. 12(a), is highly matched with the experimental data, indicating the small error and high accuracy of the data. The absolute sensitivity Sa and relative sensitivity Sr were further derived and are portrayed in Fig. 12(b). Both Sa and Sr monotonically increase as the temperature increases from 393 K to 473 K. The maximum Sa and Sr at 473 K are 8.573% K−1 and 1.927% K−1, respectively. The relatively large Sa is superior to most other materials for the application of a temperature sensor. Table 1 lists the Sa values of several other temperature measuring materials for comparison. This result suggests that the SGAO:0.04Bi3+,0.003Mn4+ phosphor is a promising temperature measuring material, particularly in the 393–473 K range.


image file: d3ra05988j-f11.tif
Fig. 11 Scatter diagram for the change in FIR (IMn4+/IBi3+) versus temperature from 303 K to 473 K.

image file: d3ra05988j-f12.tif
Fig. 12 (a) FIR (IBi3+/IMn4+) fitting curves in the temperature range of 393–473 K. (b) Curves of Sa and Sr with respect to temperature in the same range. (c) FIR (IMn4+/IBi3+) fitting curve in the temperature range of 303–393 K. (d) Curves of Sa and Sr with respect to temperature in the same range.
Table 1 Sa and Sr of different temperature measuring materials
Phosphors Temperature range (K) Sa (K−1) Sr (K−1) PLE peak (nm) Ref.
LaAlO3:Er3+/Yb3+ 100–673 0.0048 0.0244 973 27
Sr4Al14O25:Eu2+ 293–423 0.004 0.00624 373 28
ZnAl2O4:Cr3+ 80–310 <0.003 0.0025 310 29
LiAl5(1−x)O8:xCr3+ 200–600 0.015 0.0025 443 30
Ca14Al10Zn6O35:Bi3+/Mn4+ 303–563 0.014 0.0121 340 31
Gd2ZnTiO6:Bi3+/Mn4+ 313–473 0.168 0.024 420 32
SrGd2Al2O7:Bi3+/Mn4+ 393–473 0.0857 0.01927 300 This work


In the temperature range of 303–393 K with the corresponding horizontal coordinate (1/T) range of 0.0025–0.0033 K−1, the FIR (IMn4+/IBi3+) fitting curve (Fig. 12(c)) also exhibits a monotonical decreasing trend. Fig. 12(d) shows the Sa and Sr in the corresponding range. The maximum Sa and Sr are 0.172% K−1 and 0.433% K−1 at 303 K, respectively. Obviously, the property in this range is depressingly not as good as that in the high-temperature range, which may have a certain adverse effect on its application.

4. Conclusion

In conclusion, a series of Bi3+ single-doped and Bi3+,Mn4+ co-doped SGAO phosphors were synthesized by the traditional high-temperature solid-phase method. The emission center of SGAO:Bi3+ is 404 nm. The optimal excitation wavelength and doping concentration are 300 nm and 4 at%, respectively. The concentration quenching effect is mainly caused by dipole–dipole interaction. With the concentration of Bi3+ kept constant at 4 at%, different contents of Mn4+ were co-doped and the optimized concentration was determined as 0.3 at%. Via the PL and EPL spectra, as well as the fluorescence lifetimes with different Mn4+ concentrations, the mechanism and efficiency of energy transfer between Bi3+ and Mn4+ were studied. The highest efficiency reaches 79.4%. To investigate the temperature sensing properties of the SGAO:0.04Bi3+,0.003Mn4+ phosphor, variational PL spectra were conducted in the temperature range of 303–473 K. The results show that SGAO:0.04Bi3+,0.003Mn4+ phosphor exhibits wide, completely non-overlapping blue-purple and red emission bands under 300 nm excitation, which corresponds to the 3P11S0 transition of Bi3+ and the 2Eg4A2g transition of Mn4+, respectively, providing beneficial conditions for the purpose of a temperature sensing application. Based on the comprehensive analysis, the SGAO:0.04Bi3+,0.003Mn4+ phosphor was demonstrated to possess high thermal detection sensitivity and good signal resolution, especially in the temperature range of 393–473 K. At 473 K, the Sa and Sr of the SGAO:0.04Bi3+,0.003Mn4+ phosphor are 8.573% K−1 and 1.927% K−1, respectively, much better than those of most other reported optical temperature sensing materials. With all the analyses combined, it is reasonable to assert that the SGAO:0.04Bi3+,0.003Mn4+ phosphor is a prominent temperature sensing material that possesses properties of excellent signal resolution and accurate temperature detection.

Conflicts of interest

On behalf of all authors, the corresponding author states that there is no conflict of interest which could have appeared to influence the work reported in this paper.

Acknowledgements

This work is supported by the National Natural Science Foundation of China (12264004, 12164004), the Natural Science Foundation of Jiangxi Province (20202ACBL214020, 20224BAB204029, 20202ACBL202003, 20224BAB204005), and the Opening Project of Shanghai Key Laboratory of Special Artifcial Microstructure Materials and Technology (Ammt2022B-2).

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Footnote

These authors contributed equally to this work.

This journal is © The Royal Society of Chemistry 2023