1 Introduction

Recently, MgAl2O4 spinel has received many attentions because of its stable structure, high thermal shock resistance, high resistance against chemical attacks and transparency in a wide spectral range, etc. MgAl2O4 spinel belongs to the A2+B23+O4 structure of the cubic space group Fd3m, and one cubic cell has eight MgAl2O4 units. The Mg2+ and O2− constituted the tetrahedral coordination with full Td symmetry (1/8 of the available site A); Al3+ has octahedral coordination with D3d symmetry (1/2 of the available site B). Such behaviors make it be considered as a good host of holding a great deal of divalent and trivalent cations in solid-state solution [1, 2]. The transition-metal ions doped in MgAl2O4 form a colorful group of phosphor materials [3], such as doped with Co2+ [4, 5], Cr3+ [6, 7], Ti4+ [8, 9] and Mn2+ [10, 11]. In recent years, Cr3+ doped in MgAl2O4 has been studied widely, and the reports revealed that MgAl2O4:Cr3+ is a new potential candidate as laser applications, scintillators, biomarkers for in vivo imaging and sensing [12,13,14,15].

The photoluminescence properties of Cr3+ are highly relative with the crystal field strength and may produce the emission either from the exited state 2E or 4T2 to ground state 4A2. There are two types of materials: one is due to the 4T24A2 spin-allowed transition in low-field materials and the other is assigned to the 2E–4A2 spin forbidden transition (R-line) in high-field materials [16]. Usually, its excitation spectrum is a broad band from 400 to 660 nm and composed of two excited bands derived from the transitions of Cr3+, the 4A24T1(~ 420 nm) and 4A24T2(~ 540 nm) transition [17,18,19]. Since spinels can be used for laser materials, scintillators and sensing, it is necessary to further to understand the effect of the crystal field on the photoluminescence behavior of Cr3+. In this work, MgAl2−xO4:xCr3+ (0 ≤ x ≤ 0.05) were synthesized through the Pechini-type sol–gel process, and their structure, morphology, photoluminescence and the crystal field parameters were investigated.

2 Experimental

2.1 Synthesis of MgAl2O4:Cr3+ nanopowders

All samples were synthesized through the Pechini-type sol–gel process. The starting materials were Mg(NO3)2·6H2O (AR, 99.5%), Al(NO3)3·9H2O (AR, 99.0%), Cr(NO3)3·9H2O (AR, 99.0%), citric acid (CA, AR, 98%) and ethylene glycol (EG). Stoichiometric ratio of the starting materials (Mg:Al:CA:EG = 1:2:3:6) was dissolved in ethanol and water. And the solution was adjusted to the pH of 4 with NH4OH. Then the solution was heated to 90–100 °C till forming the sol, and the whole process were accompanied by magnetic stirring. The sol was left in the air for about 1 day, and then was dried in an oven at 120 °C for 20 h. Finally, the dried gel was ground to powders and calcined at 600–1100 °C for 3 h.

2.2 Characterization

The XRD patterns were measured by Rigaku DMAX1400 X-ray diffractometer with Cu Kα (λ = 0.15406 nm) incident radiation. The morphologies were examined by Tescan MAIA3 ultra high-resolution FESEM. The FTIR spectra were carried out by Nicolet 5700 Fourier transformations infrared spectrometer with standard KBr disk technique. The diffuse reflection spectra were performed by Shimadzu Solidspec-3700 UV–VIS-NIR spectrophotometer. The excitation and emission spectra were examined by Perkin Elmer LS 55 fluorescence spectrophotometer.

3 Results and discussion

3.1 Structure

The XRD patterns were shown in Fig. 1. It confirmed that the single phase of MgAl2O4 were present until the temperature arrived at 700 °C. The intensity of diffraction peak improved evidently as the increasing of calcination temperatures, and this was caused by the growth of the crystallinity. The lattice parameters and crystallite size can be calculated through Bragg diffraction and Scherrer’s equation, and the calculation results were shown in Fig. 3f. It’s evident that the crystallite size grew slowly below 900 °C and increased obviously after that. And the result was similar to the previous report [13, 18].

Fig. 1
figure 1

XRD patterns of MgAl1.96O4:0.04Cr3+ calcined at different temperatures

The FTIR of MgAl1.96O4:0.04Cr3+ calcined at 700 °C to 1100 °C were shown in Fig. 2. The spectra exhibited four major transmittance bands of 548 cm−1, 707 cm−1, 1406 cm−1 and 1636 cm−1. The bands observed at 548 cm−1 and 707 cm−1 were corresponded to octahedral and tetrahedral Al–O bonds of the regular spinel structure [17, 20]. It’s clear that the bands shifted to lower wavenumbers and their boundary became clearer about the increase in calcination temperatures. This was identified with the results of Fig. 1. The band of 1407 cm−1 was due to the stretching vibration of CO32− [1, 20]. It revealed that some metal carbonates existed on the samples calcined at 800 °C and it became weak as the calcination temperatures increasing. The metal carbonates disappeared until the calcination temperatures arrived at 1100 °C. The transmittance bands at 1636 cm−1 corresponded to H–O–H bending vibrations. Besides, the spectra showed three weak bands of 1050 cm−1, 1083 cm−1 and 1517 cm−1. The C–O stretching vibration was at 1050 cm−1, and it disappeared above 1000 °C. The Mg–O–C bending resonated with 1083 cm−1 [20]. The band of 1517 cm−1 should be the N–O stretching of nitrate group [20], and it disappeared when calcination temperatures were above 700 °C.

Fig. 2
figure 2

FTIR spectra of MgAl1.96O4:0.04Cr3+calcined at different temperatures

3.2 Morphology

The FESEM micrographs and particle sizes distribution histogram of MgAl1.96O4: 0.04Cr3+ samples were shown in Fig. 3 It’s clear that the powders calcined below 1000 °C were near-spherical and uniform. The average particle size was 20–30 nm below 900 °C and then increased evidently after 900 °C. It was in accordance with the results of the XRD spectra. The samples calcined at 1100 °C were spherical and the average particle size was 90 nm. Nam [21] reported that the spherical-spinel powder is helpful for high densification and smaller grain size of transparent MgAl2O4 ceramics. Accordingly, the MgAl2O4:Cr3+ nano powder obtained from the Pechini-type sol–gel process is suitable for the preparation of the transparent MgAl2O4:Cr3+ ceramics.

Fig. 3
figure 3

FESEM,particle sizes distribution histogram, crystallite size and lattice parameters of MgAl1.96O4:0.04Cr3+, a 700 °C; b 800 °C; c 900 °C; d 1000 °C; e 1100 °C; f crystallite size and lattice parameters

3.3 Photoluminescence properties

The excitation and emission spectra of MgAl1.96O4:0.04Cr3+ calcined at different temperatures were similar and the sample calcined at 1100 °C had the highest luminescent intensity. The excitation (λem = 522, 574 and 694 nm) and emission (λex = 250, 300 and 460 nm) spectra of MgAl1.96O4:0.04Cr3+ calcined at 1100 °C were shown in Fig. 4. The excitation spectrum (λem = 522 nm) was a broad excitation band centered around 236 nm, which could be attributed to the host and the charge transferred band of Cr3+–O2− [6, 13]. The excitation spectrum (λem = 574 nm) included a broad band centered around 236 nm, 250 nm and 300 nm. These excited bands were also due to the host and the charge transfer band of Cr3+–O2−. The excitation spectrum (λem = 690 nm) included a broad band centered around 250 nm and a narrow band of the maximum at 457 nm. The former was due to the host and the charge transferred band of Cr3+–O2−, and the latter was assigned to the spin-forbidden transition of 4A22T2 [15, 19].

Fig. 4
figure 4

Excitation (a) and emission (b) spectra of MgAl1.96O4:0.04Cr3+ calcined at 1100 °C, the inset in a: emission intensity (λex = 457 nm) as calcination temperatures and Cr3+ concentration, and the inset in b: chromaticity coordinates

The emission spectra (λex = 250 nm) included a broad band centered around 425 nm (23,529 cm−1), 461 nm (21,692 cm−1), 498 nm (20,080 cm−1), 522 nm (19,157 cm−1) and 690 nm (14,493 cm−1), and their attributions were also shown in Fig. 4. The emission bands of 425 nm (23,529 cm−1), 461 nm (21,692 cm−1) were assigned to the transition of 4T14A2 and 2T24A2, respectively. It’s known that the 4A24T2 transition was a broad band of 480–560 nm [17,18,19], and there existed an obvious splitting in Fig. 4b. Brik [16] reported that stronger crystal field implied larger splitting of the orbital triplets, especially for the 4T2 state. It can be concluded that Cr3+ was suited in a stronger crystal field and the emission bands centered around 488 nm, 498 nm, 508 nm, 522 nm, 537 nm and 548 nm were attributed to the transitions of the splitting 4T2 state to the ground state 4A2. The emission bands of 574 nm (17,421 cm−1), 597 nm (16,750 cm−1) and 622 nm (16,077 cm−1) were assigned to the transition 2T14A2. It also can be concluded that there existed an obviously splitting of the 2T1 states. The emission band of 690 nm was the characteristic zero phonon line (ZPL, R-line) ascribed to the 2E–4A2 transition of Cr3+, and the weak emission band around it were the multi phonon side of Cr3+ bands of either side of the ZPL [13,14,15]. It’s clear that the emission of the 4T24A2 and 2E–4A2 transitions became weaker and the emission of the 2T14A2 transition got stronger when the excitation wavelength was 300 nm. And excited at 457 nm, it only showed the 2E–4A2 transition with the FWHM about 8 nm. The chromaticity coordinates were shown in the inset of Fig. 4b.

The emission intensities (λex = 457 nm) as calcination temperatures and the concentration of Cr3+ were displayed in the inset of Fig. 4a. It’s expected that the emission intensity increased as calcination temperatures, which was owned to the crystallization of the sample. It’s also evident that the quenching concentration of Cr3+ was x = 0.04. In this work, a higher quenching concentration was obtained comparing with the previous reports [13, 19], which could be attributed to the better molecular homogeneity and monodisperse nanoparticles obtained from the Pechini-type sol–gel process.

Brik et al. [16] presented that the emissions of Cr3+ ions depended on the strength of the crystal field: the low-field materials (4T24A2 spin-allowed transition) and the high-field materials (2E–4A2 spin forbidden transition). But in this work (λex = 457 nm), the 4T24A2 and 2E–4A2 transitions appeared simultaneously. And the obvious 2T14A2 transition was observed at λex = 300 nm. It seemed that Cr3+ was suited in complicated surroundings. The diffuse reflectance spectra of MgAl2−xO4:xCr3+ (0 ≤ x ≤ 0.05) were also measured and shown in Fig. 5. The diffuse reflectance spectra were composed of three broad bands centered around 270 nm, 369 nm and 543 nm. The band of 270 nm was ascribed to the MgAl2O4 host; meanwhile the charge transfer band of Cr3+–O2− was also in this region [12]. The band of 369 nm (27,100 cm−1) was assigned to 4A22A1 transitions of Cr3+, and its shoulder band included the 4A24T1 and 4A22T2 transitions [16, 22]. The absorption band centered on 543 nm (18,416 cm−1) was due to the 4A24T2 transitions of Cr3+. The relative weak band appeared at 667 nm (14993 cm−1) was originated from 4A22T1 transitions of Cr3+. According to the excitation, emission spectra and the diffuse reflectance spectra, the energy level diagram of Cr3+ in nano-MgAl2O4 powders can be obtained and shown in the inset of Fig. 5. Meanwhile, basing on Tanabe–Sugano theory, the experienced crystal field parameters Dq, the Racah parameters B and C can be calculated by the energies of these transitions [23,24,25]. The energies of 4A24T2, 4A24T1 and 2E–4A2 transitions were ν1 (543 nm, 18,416 cm−1), ν2 (425 nm, 23,529 cm−1) and ν (690 nm, 14,493 cm−1) respectively. Dq, B and C can be calculated by the following formula:

Fig. 5
figure 5

Diffuse reflectance spectra of MgAl2-xO4: xCr3+ (0 ≤ x ≤ 0.05) calcined at 1100 °C, the inset was the energy level diagram of Cr3+

$$10D_{q} = v_{1}$$
(1)
$$B = \frac{{(2v_{1} - v_{2} )(v_{2} - v_{1} )}}{{(27v_{1} - 15v_{2} )}}$$
(2)
$$9B + 3C = v$$
(3)

Consequently, Dq was about 1842 cm−1, B was about 471 cm−1 and C was about 3418 cm−1. The value of Dq/B was 3.9. It’s higher than the previous reported to be 3–3.5 [12, 13, 17]. And it is accordance with the results of the emission spectra, the obvious energy level splitting of 4T2 and 2T1 state. Comparing with the previous reports [16,17,18,19], the well-known excited bands derived from the 4A24T1(~ 420 nm) and 4A24T2(~ 540 nm) transition of Cr3+ were not detected in this work. Brik [16] also reported that the energy excitation band (4A24T1 transition) is explained by a well-known effect of “intensity borrowing”, when the 4T1 and 2T2 state are mixed by spin–orbit coupling. But in Fig. 4b, the 4T14A2 and 2T24A2 transitions were separated evidently, which meant that the coupling between the 4T1 and 2T2 state were weak. It’s also because that in this work Cr3+ ion was situated in a stronger crystal field.

4 Conclusion

Cr3+ doped MgAl2O4 nano powders were successfully synthesized through the Pechini-type sol–gel process. The results showed the MgAl2O4 spinel phase appeared when the temperature arrived at 700 °C, and the particle sizes were grown as calcinations temperatures increased. The results were accordance with the results of FESEM. The FESEM images also showed that the powders calcined at 1100 °C were spherical and the average particle size was about 90 nm. The study on the optical performance revealed that in the obtained MgAl2O4:Cr3+ nano powders, Cr3+ was suited in a high crystal field with the value of Dq/B = 3.9. The strong crystal field caused an obvious splitting of the 4T2 and 2T1 state, and the weak coupling between the 4T1 and 2T2 state. The MgAl2O4:Cr3+ nano powders showed different emissions at different excitations, broad band emission centered at 522 nm (4T24A2, λex = 457 nm), broad band emission centered at 574 nm (2T14A2, λex = 300 nm) and R-line emission centered at 690 nm (2E–4A2, λex = 457 nm). Comparing with previous reports, Cr3+ suited in a stronger crystal field and had a higher quenching concentration. The higher crystal field and the quenching concentration could be attributed to the better molecular homogeneity and monodisperse nanoparticles obtained from the Pechini-type sol–gel process.