Introduction

Persistent luminescence has been among the most popular subjects of investigations in the storage phosphors field since the late 1990s. Alkaline earth aluminates doped with the Eu2+ and R3+ ions (MAl2O4:Eu2+, R3+; M = Ca, Sr; R = Nd, Dy) have been introduced as new commercial persistent luminescence materials to replace ZnS:Cu, Co [13]. The luminescence properties of the aluminates are degraded when exposed to water and hence their use in luminous paints as a pigment is limited. Generally, in Eu2+ and Dy3+ co-doped systems, the Eu2+ is considered as an activator and the Dy3+ to produce some traps for electrons or holes [4, 5]. Recently, great attention has been paid to investigating the compounds of the melilite group. The melilites are a large group of compounds characterized by the general formula M2T1T 22 X7, where M is a large monovalent or divalent cation, T1 is a small divalent or trivalent cation in tetrahedral, T2 is also a small cation in the other tetrahedral, and X is an anion. Afterglow in melilite has already been well documented [69]. Currently, the ML phenomenon has attracted more attention because of its potential application for sensing structural damage, fractures, and deformation. Many efforts have been devoted for developing ML sensors due to their various applications such as visualization of stress, damage detection for airplanes or cars, and the study of human diseases in the near future. For these ML sensors, development of ML phosphors with various colors has much importance. At the same time, the high stabilities, such as resistance of water and thermal stability, are also very important for the application of ML [10, 11]. In order to search better silicate ML phosphors, we investigated the europium and dysprosium-doped M2MgSi2O7:Eu2+, Dy3+; M = Sr, Ca for different color and intensity [12]. The Sr2MgSi2O7:Eu2+,Dy3+ and Ca2MgSi2O7:Eu2+,Dy3+ phosphors were prepared by the high-temperature solid-state reaction method under a weak reducing atmosphere. This paper reports the structural characterization on the basis of XRD, EDX, and FTIR. The photoluminescence, mechanoluminescence, and afterglow properties were also studied.

Experimental

Sample preparation

The powder samples of Sr2MgSi2O7:Eu2+, Dy3+ (SMSED) and Ca2MgSi2O7:Eu2+, Dy3+ (CMSED) were prepared by solid-state reaction method. The raw materials are SrCO3 (99.90 %), CaCO3 (99.90 %), MgO (99.90 %), SiO2 (99.99 %), Eu2O3 (99.99 %), and Dy2O3 (99.99 %), all of analytical purity, were employed in this experiment. Boric acid [H3BO3 (99.90 %)] was added as a flux. Initially, the raw materials were weighed according to the nominal compositions of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+. Then the powders were mixed and milled thoroughly for 2 h using an agate mortar and pestle. The grinded sample was placed in an alumina crucible and subsequently fired at 1,050 °C for 3 h in a weak reducing atmosphere. The weak reducing atmosphere was generated with the help of activated charcoal.

Characterization

The XRD pattern was obtained from a Bruker D8 Advanced X-ray powder diffractometer using Cu-Kα radiation and the data were collected over the 2θ range 10–70° at room temperature. The phase structure of the sample was verified with the help of joint committee for powder diffraction studies (JCPDS) file (JCPDS: 75–1736, 87–0046). A Fourier transform infrared (FTIR) spectrum was recorded with the help of IR Prestige-21 by SHIMADZU for investigating the fingerprint region and functional groups on the surface of prepared phosphor. The FTIR spectra were collected in the middle infrared region (400–4,000 cm−1) by mixing the sample with potassium bromide (KBr). The excitation and emission spectra of sintered phosphors were recorded by spectrofluorophotometer (SHIMADZU, RF 5301 PC) using a xenon lamp as an excitation source. The decay curves were recorded with a time-resolved fluorescence spectrophotometer (TRFS). Samples were excited with 340-nm pulse nano LED light. Mechanoluminescence was observed by a homemade laboratory system. All measurements were carried out at room temperature.

Experimental setup for ML

The experimental set up used for the impulsive deformation of ML is shown in Fig. 1. The prepared phosphors were stressed by a dropping load of cylindrical shape (moving piston) of a mass of 400 g. To change the impact force, the load was dropped from different heights. The samples were wrapped in aluminum foil and kept in the dark until the ML studies were carried out. RCA 931A photomultiplier tube was positioned below the Lucite plate and the output was connected to the storage oscilloscope. In Fig. 1, 1-stand; 2-pulley; 3-metallic wire; 4-load; 5-guiding cylinder; 6-aluminium foil; 7-phosphors; 8-transparent Lucite plate; 9-wooden block; 10-photomultiplier tube (PMT); 11-oscilloscope; 12-iron base mounted on a table.

Fig. 1
figure 1

Schematic diagram of the experimental setup for ML measurement

Results and discussion

XRD analysis

XRD patterns of the Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors are shown in Fig. 2a and b. The position and intensity of diffraction peaks of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ were found to be consistent with that of the JCPDS file (JCPDS: 75–1736) and (JCPDS: 87–0046) [1314]. The result revealed that the phase structure of the Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7: Eu2+, Dy3+ phosphors are of akermanite type, which belongs to the tetragonal crystallography with space group \( \hbox{P}\bar{42}_1 \hbox{m}\), this structure is a member of the melilite group and forms a layered compound. From the analysis of XRD, it was revealed that no impurity phase has been observed in the compositions, clearly implying that the little amount of doped rare earth ions have almost no effect on the XRD of the prepared phosphors.

Fig. 2
figure 2

a X-ray diffraction patterns of Sr2MgSi2O7: Eu2+, Dy3+ phosphor. b X-ray diffraction patterns of Ca2MgSi2O7: Eu2+, Dy3+ phosphor

Energy-dispersive X-ray spectroscopy (EDX)

The composition of the powder sample was measured using EDX. Table 1 shows the compositional elements of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+, which is compared with the standard element. Energy-dispersive X-ray spectroscopy (EDX) is a standard procedure for identifying and quantifying elemental composition of sample area as small as a few nanometers. The existence of europium (Eu) and dysprosium (Dy) in the phosphors is clear in their corresponding EDX spectra. There appeared no other emissions apart from Sr, Mg, Si, and O in Sr2MgSi2O7:Eu2+, Dy3+ and Ca, Mg, Si and O in Ca2MgSi2O7:Eu2+, Dy3+ the EDX spectra of the samples. In the spectrum, intense peaks are present that confirm the formation of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors in Fig. 3a and b, respectively.

Table 1 Composite element of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+
Fig. 3
figure 3

a EDX spectra of Sr2MgSi2O7: Eu2+, Dy3+ phosphor. b EDX spectra of Ca2MgSi2O7: Eu2+, Dy3+ phosphor

Fourier transform infrared spectra (FTIR)

Fourier transform infrared spectroscopy (FTIR) has been widely used for the identification of organic and inorganic compounds. The infrared spectrum of an inorganic compound represents its physical properties. Spectroscopically, the middle infrared region (400–4,000 cm−1) is extremely useful for the study of organic and inorganic compounds. Figure 4a and b shows the FTIR spectra of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors. The wave-number 3,429.43 cm−1 for Sr2MgSi2O7:Eu2+, Dy3+ and 3,444.87 cm−1 for CaMgSi2O7:Eu2+, Dy3+ arises due to the O–H stretching mode. The O–H group around the 3,400 cm−1 in Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors are might be due to the presence of moisture. The wave-number 1,762.94 cm−1 for Sr2MgSi2O7:Eu2+, Dy3+ and 1779.32 cm−1 for CaMgSi2O7:Eu2+, Dy3+ arises due to the stretching of CO3 2−. The CO3 2− modes (asymmetric stretching) around the 1,700 cm−1 in Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors are due to the presence of carbonate. In the experimental section, to prepare the Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors, we used the raw material (SrCO3, CaCO3) in carbonate form. The free CO3 2− ions have a D3 h symmetry (trigonal planar) and its spectrum is dominated by the band at 1,700 cm−1. The vibration bands around 1,643.35 and 1,485.19 cm−1 for Sr2MgSi2O7:Eu2+, Dy3+ are assigned due to the Mg2+ and Sr2+ and 1,631.78 and 852.54, 740.57 cm−1 for CaMgSi2O7:Eu2+, Dy3+ are assigned due to the Mg2+ and Ca2+. The wave-numbers 1,046.34, 991.41, 964.41, 925.83, and 844.82 cm−1 for Sr2MgSi2O7:Eu2+, Dy3+ and 1,016.32, 979.67, and 941.26 cm−1 for Ca2MgSi2O7:Eu2+, Dy3+ are due to the (Si–Ob–Si) and (Si–Onb) stretching modes. The wave-numbers 744.52, 705.95, 667.37, 621.08, and 567.07 cm−1 for Sr2MgSi2O7:Eu2+, Dy3+ and 684.80, 644.52 cm−1 for Ca2MgSi2O7:Eu2+, Dy3+ arises due to the (Si–O–Si) bending modes and the wave-number 470.63 cm−1 for Sr2MgSi2O7:Eu2+, Dy3+ and 482.20 cm−1 for Ca2MgSi2O7:Eu2+, Dy3+ are based on the (Si–O–Si) bending modes as well as the Mg–O modes. In Sr2MgSi2O7:Eu2+, Dy3+; and Ca2MgSi2O7:Eu2+, Dy3+; Mg2+ occupy the tetrahedral sites. FTIR spectra confirm the component of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors [1521].

Fig. 4
figure 4

a FTIR spectra of Sr2MgSi2O7: Eu2+, Dy3+ phosphor. b FTIR spectra of Ca2MgSi2O7: Eu2+, Dy3+ phosphor

Photoluminescence (PL)

The excitation and emission spectra of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors are shown in Fig. 5a and b. The excitation spectra were observed in the range of 200–425 nm and emission spectra were recorded in the range of 400–650 nm. The results illustrate that both of them are broadband spectra.

Fig. 5
figure 5

a Excitation and emission spectra of Sr2MgSi2O7:Eu2+, Dy3+ phosphor. b Excitation and emission spectra of Ca2MgSi2O7:Eu2+, Dy3+ phosphor

The excitation broadband is due to transitions of (4f7) ground state to excited state (4f65d1) [4f7 → 4f65d1] and emission broadband is due to transitions of excited state (4f65d1) to ground state (4f7) [4f65d1 → 4f7]. In Fig. 5a, there are four excitation peaks found at 269, 278, 335, and 353 nm and corresponding to emission peaks that occurred at 465 nm, which emit blue color. Similarly, in Fig. 5b there are four excitation peaks found at 270, 279, 315, and 340 nm, and corresponding emission peaks were recorded at 535 nm, which emits green color.

In Fig. 5a and b, the main emission peak at 465 nm and 535 nm is ascribed to the 4f65d1 → 4f7 transition of Eu2+, but there is no special emission of Dy3+ and Eu3+ ions in the spectra, which implies that Eu3+ ions have been reduced to Eu2+ completely, and the co-doped Dy3+ did not emit any color and transferred the absorbed energy to Eu2+ ions in the Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ crystal lattice. The co-doped Dy3+ plays a role as a hole-trapped center at the hole trap levels, which capture the free electrons or holes when Eu2+ is excited and then release the free electrons to the conduction band. It is known that the blue emission that peaked at 465 nm corresponds to the transitions of 4F9/2 → 6H15/2, and 535 nm corresponds to the transitions of 4F9/2 → 6H13/2 this emission belongs to hypersensitive transition, which strongly depends on outside environments of Dy3+ ions.

Decay

Figure 6 shows the typical decay curves of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors. The initial afterglow intensity of both the material was high. The decay times of phosphors can be calculated by a curve-fitting technique, and the decay curves fitted by the sum of two exponential components have different decay times.

$$ I \, = \, A_{ 1} { \exp }\left( { - t/\tau_{ 1} } \right) \, + \, A_{ 2} { \exp }\left( { - t/\tau_{ 2} } \right), $$
(1)

where I is phosphorescence intensity, A 1 , A 2 are constants, t is time, τ 1, and τ 2 are decay times (in nanoseconds) for the exponential components. Decay curves are successfully fitted by Eq. (1) and the fitting curve results are shown in Table 2. Dy3+ ions have often been used as co-dopant in the previously developed long afterglow materials (e.g., SrAl2O4:Eu2+, Dy3+). Alkaline earth ion sites are a very probable source of electron trap [22]. In the alkaline earth silicate, most of the excitation energy will be transferred from the host (from Dy3+ → to Eu2+ → to host).

Fig. 6
figure 6

Decay curves of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors

Table 2 Fitting results of the decay curves

However, part of the excitation energy will be stored when some of the excited carriers drop into the traps, instead of returning to the ground states. Later, the traps created by Dy3+ are deeper than those created by Eu2+ and with thermal excitation at proper temperature; these carriers will be released from the traps and transferred via the host to the Dy3+ ions, followed by the characteristic Dy3+ emissions as long afterglow. Dy3+ in the silicates act as traps, meanwhile Dy3+ can also act as luminescent centers, thus the persistence time is prolonged [22].

Mechanoluminescence (ML)

Figure 7a and b shows the characteristic curve between ML intensity versus time for different heights on Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors. The experiment was carried out for a fixed mass (400 g). The quantity of the sample was kept the same for all the cases. The figure A, B, C, and D shows ML curves dropped from different heights 20, 30, 40, and 50 cm, respectively. These figures showed that the ML intensity increases linearly with increases in the falling height of the moving piston; that is, the ML intensity depending upon the impact velocity. The maximum ML intensity has been obtained for the 50-cm dropping height (for both Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+). The synthesized phosphors were not irradiated by any of the excitation source such as ultra-violet, laser, X-ray, β-rays, or γ-rays.

Fig. 7
figure 7

a ML intensity versus time of Sr2MgSi2O7:Eu2+, Dy3+ phosphor. b ML intensity versus time of Ca2MgSi2O7:Eu2+, Dy3+ phosphor

Figure 8a and b shows the characteristics curve between peak ML intensity versus impact velocity of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors. The strait line found implies that the ML intensity increases linearly with the increasing impact velocity [\( \sqrt {2gh} \) {where h is the different heights of moving piston (20, 30, 40, 50 cm)}]. It can also be said that ML intensity increases with increasing mechanical stress. When the moving piston hits the prepared sample, it produces a piezoelectric field in the prepared phosphors as they are non-centrosymmetric. The piezoelectric field near certain defect centers may be high due to the change in the local structure. The piezoelectric field reduces the trap depth of the carriers. The decrease in trap depth causes a transfer of electrons from electron traps to the conduction band. Subsequently, the moving electrons in the conduction band are captured in the excited state, located at the bottom of the conduction band, whereby excited ions are produced. The subsequent recombination of electrons with the hole centers gives rise to the light emission [23, 24]. It was found that ML emission was observed even when the height of the moving piston was comparatively low (10 cm).

Fig. 8
figure 8

a Peak ML intensity versus impact velocity of Sr2MgSi2O7:Eu2+, Dy3+ phosphor. b Peak ML intensity versus impact velocity of Ca2MgSi2O7:Eu2+, Dy3+ phosphor

Figure 9a and b shows the ML spectrum of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors. The spectrum consists of a broad emission band peaking at 460 and 530 nm, which is similar to the spectra of PL spectrum of Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors. The small difference of the peak location between the ML (460 nm for Sr2MgSi2O7:Eu2+, Dy3+ and 530 nm for Ca2MgSi2O7:Eu2+, Dy3+) and PL (465 and 535 nm) can be ascribed to the different measurement devices. This implies that ML is emitted from the same emitting center of Eu2+ ions as PL, which is also produced by the transition of Eu2+ ions between the (4f65d1) excited state to (4f7) ground state. Furthermore, both prepared phosphors have a tetragonal structure with space group \( \hbox{P}\bar{42}_1 \hbox{m}\)m; previous research has revealed that the crystal with these structure possesses piezo-electrification. When a mechanical stress, such as compress, friction, and striking, and so on, was applied on the (for both Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+) phosphor, a piezoelectric field can be produced. The strain energy impels the filled shallow trap to release holes to the valence band. Then, free holes excite Eu+ to produce Eu2+, which returns to the (4f7) ground state by emitting light. Based on the above analysis, these phosphors can be used as sensors to detect the stress on an object [2529].

Fig. 9
figure 9

a ML spectra of Sr2MgSi2O7:Eu2+, Dy3+ phosphor. b ML Spectra of Ca2MgSi2O7:Eu2+, Dy3+ phosphor

Conclusions

Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors with a long afterglow were synthesized by the high-temperature solid-state reaction method under weak reducing atmospheres. The radius of Eu2+ (1.12 Å) and Dy3+ (0.99 Å) is very close to that of Sr2+ (about 1.12 Å), Ca2+ (about 1.12 Å) rather than Mg2+ (0.65 Å) and Si4+ (0.41 Å) nm). Therefore, the Eu2+ and Dy3+ ions are expected to occupy the Sr2+ sites in Sr2MgSi2O7 and Ca2+ sites in Ca2MgSi2O7 host. The EDX and FTIR spectra confirm the present elements in Sr2MgSi2O7:Eu2+, Dy3+ and Ca2MgSi2O7:Eu2+, Dy3+ phosphors. The emission peaks of Ca2MgSi2O7:Eu2+, Dy3+ phosphor, when compared with that of Sr2MgSi2O7:Eu2+, Dy3+ phosphor, shift towards the longer wavelength direction, which can be explained by the slight difference in the crystal structure. The mechanoluminescence intensity increases linearly with the load and linear relationship has been obtained with the impact velocity, which suggests that both prepared phosphors can be used as sensors to detect the stress on an object.