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Investigation of physical characteristics for Al2O3:C dosimeter using LM-OSL

  • Kim, Myung-Jin (Archaeological Science Institute, RADPION Inc.) ;
  • Lee, Young-Ju (Radiation Technology Institute, Neosiskorea Co. Ltd.) ;
  • Kim, Ki-Bum (Institute of Liberal Education, Kangwon National University) ;
  • Hong, Duk-Geun (Dept. of Physics, Kangwon National University)
  • Received : 2019.05.11
  • Accepted : 2019.06.28
  • Published : 2019.08.25

Abstract

This paper reports results on the physical properties of a powder type of $Al_2O_3:C$ commonly used as a luminescence dosimeter using the LM-OSL technique. On the analysis with the general order kinetics model, the LM-OSL signal measured appeared to be composed of three components (fast, medium, slow) showing the largest area in the medium component. The photoionization cross sections of three components were distributed between $10^{-19}{\sim}10^{-21}cm^2$. The values of the thermal assistance energy were evaluated the largest in slow component and the smallest in fast component, which indicates the electrons trapped in defects attributed to slow component should be the most sensitive to thermal vibration among three components. In illumination to blue light, the fast component showed a rapid linear decay and completely disappeared after light exposure time of about 5 s. The medium component decayed with two exponential elements but the slow component did not observed any noticeable change until light exposure time of 40 s. In a dose response study, all components exhibited a linear behaviour up to approximately 10 Gy.

Keywords

1. Introduction

Al2O8:C is a compound, whose F center and F+ centerrelate to luminescence emission exhibiting a very high intensity peak (dosimetric trap) near 200 °C ontypical thermoluminescence (TL) glow curve, which was introduced in the 1990s for the purpose of developing a radiation dosimeter using TL1. The compound is highly sensitive to radiation to such anextent that it can degrade ~1 μGy of radiation, and thus, the compound has attracted attention for its potential in measuring environmental radiation, whichrequires low dosimetry. However, the compound has limitations in its thermal quenching effect, which shows a correlation between abnormal levels of radiation and luminescence intensity at high temperatures.2 Recently, amethod for radiation dosimetry using optically stimulated luminescence (OSL) that can overcome the thermal quenching phenomenon of Al2O8:C has been proposed and various research findings related to the compound have been reported.3,4

OSL that observes the luminescence emitted from the sample stimulated with light is classified according to the method of stimulation as follows. Continuous-wave OSL (CW-OSL) measures luminescence by continuously stimulating the sample with a constantoutput of light, linear modulation OSL (LM-OSL) measures luminescence while linearly increasing the output of the light, and pulsed OSL (POSL) measuresluminescence after applying a short pulse of optical stimulus to the sample. The intensity of CW-OSL mainly used for radiation dosimetry is proportional to the radiation dose and decreases with measurementtime. However, the luminescence signal measured using LM-OSL shows peak formation depending on the magnitude of the optical stimulation, where thesepeaks are related to the photoionization cross-section of the lattice defect (trap) present in the sample.5.6Additionally, POSL is commonly used to calculate the lifetime, indicating the duration time required for free electrons emitted from lattice defects due tooptical stimulation combining with the recombinationcenter and releasing the luminescence.7

In this study, the LM-OSL signal of Al2O3:C sample was measured, and then the photoionization cross-section of each component was calculated by decomposing the signal, which in turn was used tocalculate thermal assistance energy that affects the energy distribution function of the lattice defects associated with each component. In addition, the photosensitivity and the response to radiation of each component were investigated for radiation-dosimetry using the LM-OSL signal.

 

2. Theory

In general, LM-OSL can be explained by energy band theory. Assuming a first-order kinetic model with no probability of lattice defects re-trappingelectrons emitted by external stimuli in a samplecomposed of a single lattice defect and a singlerecombination center;8 given that the output of thestimulus light source increased at a constant rate with time, the de-trapping rate of the electrons trapped in the lattice defect is expressed by the following equation.

\(\frac{d n(t)}{d t}=-\sigma \gamma t n(t)\)       (1)

In this equation, γ = I0/T is the rate at which the output of the stimulus light source constantly increases with time and T is the total luminescence measurementtime. As the flux of the stimulus light source is represented by Φ(t) = γt, the signal of LM-OSL appears as follows.

\(L(t)=\frac{d n(t)}{d t}=n_{0} \gamma t \exp \left(-\frac{1}{2} \sigma \gamma{t}^{2}\right)\)       (2)

Here, n0 is the initial number of electrons trapped in the lattice defect and σ is the photoionizationcross-section of the lattice defect. Also, the maximumpeak point (Lmax) of the LM-OSL signal and the time (t< sub>max) at the maximum peak point can be obtained using Eq. (2) as follows.

\(t_{\max }=\sqrt{\frac{1}{\sigma \gamma}}\)       (3)

\(L_{\max }=n_{0} \sqrt{\sigma \gamma} \exp \left(-\frac{1}{2}\right)=0.607 \frac{n_{0}}{t_{\max }}\)       (4)

However, in contrast to the previous assumption, assuming a general order kinetic model that considersthe probability that electrons emitted from the latticedefects are re-trapped in the lattice defects, the electronemission rate with increasing output of stimulus lightsource is given by Eq. (5).9

\(\frac{d n(t)}{d t}=-\alpha \gamma t n^{\beta}(t)\)​​​​​​​​​​​​​​       (5)

Here, \(\alpha=\sigma / n_{0}^{\beta-1}\)and β is a dimensionless coefficient that is neither 0 nor 1. The signal of the LM-OSL in this case is shown below.

\(L(t)=-\frac{d n(t)}{d t}=n_{0} \sigma \gamma{t}\left[(\beta-1) \frac{1}{2} \sigma \gamma{t}^{2}+1\right]^{\beta /(1-\beta)}\)​​​​​​​       (6)

Furthermore, the maximum peak point (Lmax) of LM-OSL and the time at the peak point (tmax) are as follows.

\(t_{\max }=\sqrt{\frac{2}{\sigma \gamma(\beta+1)}}\)​​​​​​​       (7)

\(L_{\max }=\frac{2 n_{0}}{\beta+1} \frac{1}{t_{\max }}\left(\frac{2 \beta}{\beta+1}\right)^{\beta /(1-\beta)}\)​​​​​​​       (8)

The LM-OSL signal can be de-convoluted into alinear combination of the first or general order kinetic model, since the maximum points of the peaks can beseparated according to the stimulation time, and thus, provide information on the number of electrons trapped in the lattice defects of each decomposed componentand the size of the photoionization cross-section.10

 

3. Samples and Experimental Equipment

This study used Al2O3:C powder (< 105 μm) manufactured by Landauer, USA as samples. The LM-OSL signal was measured with an automated Risø TL/OSL reader (Risø TL/OSL-DA-20) from the Risø laboratory in Denmark installed in the Central Laboratory of Kangwon National University.11A blue light emitting diode (Nichia type NSPB-500S, 470 ± 20 nm) was used as the stimulus lightsource and the maximum power output of the lightsource was 50 mW/cm2. The LM-OSL signal was detected by the photomultiplier tube (EMI 9635QA) attached a Hoya U-340 filter. The sample was irradiated from 90Sr/90Y beta source, and the radiation dose rate was approximately 0.08 Gy/s.

 

4. Results and Discussion

 

4.1. LM-OSL measurement and photoionization cross-section

While the CW-OSL signal that stimulates the sample with constant output from a stimulus lightsource exponentially decreases over time, the LM-OSL signal that stimulates the sample with linearly increasing output leads to peaks according to time. The LM-OSL signal in peak form can be represented by a mathematical linear combination of the selected kinetic model. It can be represented as Eq. (9) when the first order kinetic model has been selected, and Eq. (10) when the general order kinetic model has been selected.

\(L(t)=\sum_{i=1}^{N} L_{i}=\sum_{i=1}^{N} n_{0 i} \sigma_{i} \gamma{t} \exp \left(\frac{1}{2} \sigma_{i} \gamma{t}^{2}\right)\)​​​​​​​       (9)

\(L(t)=\sum_{i=1}^{N} L_{i}=\sum_{i=1}^{N} n_{0 i} \sigma_{i} \gamma{t}\left[(\beta-1) \frac{1}{2} \sigma_{i} \gamma{t}^{2}+1\right]^{\beta /(1-\beta)}\)​​​​​​​       (10)

It is very important to determine the kinetic order toseparate the exact components of the LM-OSL signal. In examining the previous studies on the kinetic order of Al2O3:C, Whitley and McKeever12 decomposed the LM-OSL signal into three components with the first-order kinetic model, while Dallas et al.9 approached the component decomposition of the LM-OSL signal using the general order kinetic model of three components. The kinetic order determination process performed in this study was intended to mathematically decomposethe LM-OSL signal by an optimal combination of variables through repeatedly substituting appropriateparameters into Eqs, (9) and (10). The suitability of the signal decomposition by the final combination of variables was determined by considering the figure of merit (\(F O M(\%)=\frac{\sum\left|I_{\mathrm{exp}}-I_{d e c}\right|}{\sum I_{\mathrm{exp}}} \times 100\)). The sequence was performed using the non-linear least squaresmethod applying the Levenberg-Marquardt algorithmemploying the Origin (version 6.1) program.

In this study, the beta dose of 0.1 Gy was irradiated to the sample as the first step to calculate the photoionization cross-section of Al2O3:C sample from the LM-OSL signal. The LM-OSL signal was measured by linearly increasing the intensity of thestimulus light source from 0 to 90 % for 3600 seconds while keeping the sample constant at 120 °C, in order to remove the interference caused by unstable latticedefect (see Fig. 1). The results of the decomposition of the measured LM-OSL signal showed that the LM-OSL signal was decomposed into three components and in this case, the FOM values of the first-orderkinetic model and the general order dynamic model were 11.2 % and 1.5 %, respectively. This implies that in the case of Al2O3:C samples used in this study, the approach using the general order kinetic model may be more reliable than the first-orderkinetic model.

Fig. 1 shows an example of decomposing the measured LM-OSL signal using the general-orderkinetic model of Eq. (10). The decomposed components were named as fast (F), medium (M) and slow (S) components, respectively, depending on the magnitude of the photoionization cross-section, and the dataimply that the intensity of the medium component is the highest. The photoionization cross-section of each component of the Al2O3:C sample calculated from the LM-OSL signal decomposition was 10−19 ~10− 21 cm2, and the results are summarized in Table 1.

 

BGHHBN_2019_v32n4_131_f0001.png 이미지Fig. 1. An example of LM-OSL signal measured from Al2O3:C dosimeter and peak deconvolution using the general order kinetics.

 

Table 1. Physical characteristics evaluated from the LM-OSL measurements of Al2O3:C dosimeter

BGHHBN_2019_v32n4_131_t0001.png 이미지

 

4.2. Thermal assistance energy

The electron-phonon coupling phenomenon ininorganic crystals widens the energy distribution function of lattice defects and changes photoionizationcharacteristics by photons. In other words, electronscan be released from lattice defects by somewhat lower photon energy due to the increase in phononenergy from the heat. This thermal dependence iscalled thermal assistance,13 and in the case of LM-OSL it can be calculated from the thermal dependence of the photoionization cross-section.14,15

\(\sigma=\sigma_{\infty} \exp \left(\frac{E^{*}}{k_{B} T}\right), E^{*}=\phi\left(E_{0}-h v\right)\)​​​​​​​       (11)

In the equation above, σ is the magnitude of the photoionization cross-section when is T = ∞, E0 is the energy gap, hν is the photon energy of light source for optical pumping, and kB is the Boltzmann constant.

In this study, Al2O3:C samples were irradiated with 0.1 Gy beta radiation to observe the thermal assistance of Al2O3:C samples and each LM-OSL signal was measured for 3600 seconds while sequentially increasing the measurement temperature to 20, 50, 75, 100, 120, and 140 °C. As shown in Fig. 2(a), the LM-OSL intensity of Al2O3:C samples also increased as the measurement temperature increased. This suggests that there exists a thermal assistance phenomenonin the Al2O3: C sample.

 

BGHHBN_2019_v32n4_131_f0002.png 이미지Fig. 2. (a) LM-OSL signal according to measuring temperature (b) ln(LM-OSL) versus 1/T to obtain value of thermal assistance energy

In general, when the LM-OSL signal can berepresented as a linear combination of the first-orderkinetic model as shown in Eq. (9), the LM-OSL signalintensity and the photoionization cross-section aredirectly correlated. Therefore, the thermal assistance energy E* can be easily calculated from the change in the LM-OSL signal intensity according to the measured temperature. However, the LM-OSL signal of the Al2O3:C sample measured in this study is decomposed into the general order kinetic component of Eq. (10), which makes it difficult to calculate the direct thermalassistance energy. Therefore, the thermal assistance energy value calculated using the general orderkinetic model in this study was used as the data tocompare the relative sizes of electron-phonon bond samong the components.

To observe in detail the thermal assistance of Al2O3:C samples based on these assumptions, the LM-OSL signal obtained at each measurement temperature was decomposed by three (fast, medium, slow) general-order kinetic components. The results showed that the intensity of each component increased with the measured temperature. If this was expressed as a function of ln(LM-OSL) and 1/T as shown in Fig. 2(b), the intensity of each LM-OSL componentappears linear with the measured temperature. Therefore, the thermal assistance energy E* of each component was directly calculated using Eq. (12).

\(\ln (L)=\ln \left(L_{\infty}\right)-\frac{E^{*}}{k_{B}} \cdot \frac{1}{T}\)​​​​​​​       (12)

Table 1 summarizes the thermal assistance energy of each component of Al2O3:C calculated by linearregression analysis using the linear function of Eq. (12). As a result, the thermal assistance energy of the fast component was the smallest, followed by the medium component, and then, the slow component. This suggests that the electron-phonon bonds of fastand medium components, which are mainly used for the calculation of the radiation dose, are relatively weak, and thus, the electrons trapped in these latticedefects are less sensitive to the lattice vibration caused from heat. Therefore, to overcome the thermal quenching phenomenon of Al2O3:C materials and to improve the accuracy of the dosimetry, the use of OSL with heat stability is required.

 

4.3. Reduction of LM-OSL due to light exposure

To investigate the sensitivity of the LM-OSL signal to light on the Al2O3:C sample, Al2O3:C samplesirradiated with 0.1 Gy beta radiation were prepared. Before the measurement of LM-OSL, the samples were exposed to light using a blue light emitting diode by sequentially increasing irradiation time for 1, 3, 5, 10, 20, and 40 seconds, and measured for LM-OSL signals for 3600 seconds at a measurementtemperature of 120 oC. As shown in Fig. 3(a), the LM-OSL signal intensity of the Al2O3:C samplerapidly decreased as light exposure time increased.

 

BGHHBN_2019_v32n4_131_f0003.png 이미지Fig. 3. (a) LM-OSL signal according to light exposure time (b) LM-OSL intensity against light exposure time for each LM-OSL component.

To analyze the photosensitivity of Al2O3:C samples in detail, the LM-OSL signals measured from the samples with different light exposure times were decomposed into three (fast, medium, slow) generalorder kinetic components. As a result, as shown in Fig. 3(b), the fast component with the largest photoionization cross-section disappeared as the LM-OSL signal decreased linearly within 5 seconds of light exposure, and the LM-OSL signal of the medium component declined exponentially. However, no significant change was observed in LM-OSL signal intensity of the slow component in up to 40 seconds of light exposure. This shows that thesensitivity of the Al2O3:C luminescent signal to light is directly related to the photoionization cross-section obtained as a result of this study. In the case of the exponentially decreasing medium component LM-OSL signal, curve fitting using linear combinations of two exponential functions was performed as shown in Eq. (13).

\(L_{\text {medium}}=\sum_{i=1}^{2} a_{i} \exp \left(b_{i} t\right)\)​​​​​​​       ​​​​​​​(13)

The phenomenon of two exponential decays of the medium component is considered to be due to the phototransfer phenomenon (a phenomenon in whichelectrons in a lattice defect by light irradiation do not directly move to a recombination center after being transferred to a conduction band, but are re-trapped in a lattice defect and are then moved to arecombination center via a conduction band by continuous light irradiation to emit luminescence)18in the luminescence process.

 

4.4. Radiation response of LM-OSL signal

To observe the radiation reactivity of the LM-OSL signal to Al2O3:C samples, LM-OSL signals weremeasured for 3600 seconds at 120 oC in samplesirradiated with 0.24, 0.48, 0.96, 4.8, and 9.6 Gy. As shown in Fig. 4(a), the LM-OSL signal intensity of the Al2O3:C sample also increased with an increase in the radiation dose. This means that the radiation response of the LM-OSL signal to the Al2O3:C sample is excellent.

To thoroughly investigate the radiation reactivity of Al2O3:C samples, the LM-OSL signal obtained from each dose was decomposed into three (fast, medium, slow) general order kinetic components, which was made as a function of radiation dose and LM-OSL signal intensity. As shown in Fig. 4(b), the dose response curve of the LM-OSL signal linearly increased to more than 8 Gy of lethal dose (LD100 / < sub>60 )for all components. In particular, the dose response was 2.29 × 107 counts/Gy in the case of the medium component occupying the largest area of the LM-OSL signal (see Fig. 1), which is more than 7 timeshigher than that of the fast component of 3.20 × 10 6counts/Gy.

 

BGHHBN_2019_v32n4_131_f0004.png 이미지Fig. 4. (a) LM-OSL signal after the various radiation doses (b) Dose response curves of each LM-OSL component.

 

5. Conclusions

In this study, the LM-OSL signal of the Al2O3:Csample was measured, and the photoionization cross-section of each component was calculated by decomposing the signal, which in turn was used tocalculate the thermal assistance energy of each component. The photosensitivity and the reactivity toradiation of the decomposed components were also investigated. As a result of LM-OSL measurement, the Al2O3:C sample was decomposed into three general-order kinetic components (fast, medium, slow). The medium area was the largest and the photo-ionization cross-section of each component was distributed in the range of 10−19 ~ 10−21 cm2. The thermal assistance energy of these components was the lowest in the fast component, followed by the medium component, and then the slow component. This suggests that electrons trapped in these latticedefects are less sensitive to lattice vibrations due to heat, since the electron-phonon bonds of fast and medium components, mainly used for calculatingradiation dose, are relatively weak. From the photo-sensitivity of the Al2O3:C sample, the fast component with the greatest photoionization cross-section arealinearly decreased within approximately 5 seconds of light exposure time and disappeared. In addition, the LM-OSL signal of the medium component was reduced exponentially in the two components, and the LM-OSL signal intensity of the slow component was not significantly changed until the light exposuretime reached 40 seconds. Finally, results of the investigation on the radiation reactivity of the LM-OSL signal showed that the dose response curve of the LM-OSL signal linearly increased for all the components up to approximately 10 Gy irradiation and the dose response of the medium component, which occupied the largest area of the LM-OSL signal, was excellent at 2.29 × 107 counts/Gy. The photoionization cross-section, thermal assistance energy, photosensitivity and radiation reactivity of each component of LM-OSL for the Al2O3:C sampleevaluated in this study can be used as the fundamentalinformation for calculation of radiation dose using OSL signal of Al2O3:C.

 

Acknowledgements

This research was supported by 2017 Research Grant from Kangwon National University (No.520170484) and Basic Science Research Program through the National Research Foundation of Korea(NRF) funded by the Ministry of Education, Science and Technology (NRF-2017R1D1A1B03029608).

References

  1. M. S. Akselrod, N. Agersnap Larsen, V. Whitley and S. W. S. Mckeever, J. Appl. Phys., 84(6), 3364-3373 (2012). https://doi.org/10.1063/1.368450
  2. M. S. Akselrod, V. S. Kortov, D. J. Kravetsky and V. I. Gotlib, Radiat. Prot. Dosim., 33(1), 119-122 (1990). https://doi.org/10.1093/rpd/33.1-4.119
  3. S. W. S. Mckeever, Nucl. Instr. Methods Phys. B, 184, 29-54 (2011). https://doi.org/10.1016/S0168-583X(01)00588-2
  4. J. M. Edmund and C. E. Andersen, Radiat. Meas., 42, 177-189 (2007). https://doi.org/10.1016/j.radmeas.2006.11.006
  5. E. Bulur, Radiat. Meas., 26(5), 701-709 (1996). https://doi.org/10.1016/S1350-4487(97)82884-3
  6. E. Bulur, L. Botter-Jensen ,and A. S. Murray, Radiat. Meas., 33, 715-719 (2001). https://doi.org/10.1016/S1350-4487(01)00089-0
  7. M. L. Chithambo, J. Phys. D: Appl. Phys., 40. 1874-1879 (2007). https://doi.org/10.1088/0022-3727/40/7/006
  8. R. Chen and S. W. S. Mckeever, 'Theory of thermoluminescence and related phenomena', World Scientific Publishing, 1997.
  9. G. I. Dallas, G. S. Polymeris, E. C. Stefanaki, D. Afouxenidis, N. C. Tsirliganis, and G. Kitis, Radiat. Meas., 43, 335-340 (2008). https://doi.org/10.1016/j.radmeas.2007.10.018
  10. E. Bulur, L. Botter-Jensen, and A. S. Murray, Radiat. Meas., 32, 407-411 (2000). https://doi.org/10.1016/S1350-4487(00)00115-3
  11. L. Botter-Jenson, E. Bulur, G. A. T. Duller, and A. S. Murray, Radiat. Meas., 32, 523-528 (2000). https://doi.org/10.1016/S1350-4487(00)00039-1
  12. V. H. Whitley and S. W. S. Mckeever, Radiat. Prot. Dosim., 100(1-4), 61-66 (2002). https://doi.org/10.1093/oxfordjournals.rpd.a005936
  13. N. A. Spooner, Radiat. Meas., 23, 593-600 (1994). https://doi.org/10.1016/1350-4487(94)90105-8
  14. F. Urbach, Phys. Rev., 92, 1324 (1953). https://doi.org/10.1103/PhysRev.92.1324
  15. M. J. Kim, K. W. Song, and D. G. Hong, SAEMULLI, 53, 171-177 (2006).
  16. M. L. Chithambo, C. Seneza, and J. M. Kalita, Radiat. Meas., 105, 7-16 (2017). https://doi.org/10.1016/j.radmeas.2017.08.009