The neutron irradiation experiments of the test samples were carried out at THOR, which is a 2-MW light-water nuclear reactor for research in Taiwan. The test samples were irradiated at the vertical tube, namely VT-4, of THOR. The vertical tube is located at the edge of the reactor core, corresponding to approximate thermal and fast neutron with a ratio of thermal-to-fast neutron around 3~5 [
11]. Details on the conditions of the neutron irradiation by the THOR neutron source are listed in
Table 1. The fast and thermal neutron fluences were determined according to the gold foil activation experiments, as reported in ref. [
11]. Test sample #0 and #0A, as reference, were not irradiated.
Since the irradiation experiments were performed near the fission reactor core, accompanying the emission of gamma rays from fission products with the neutron irradiation is expected. According to a calibration experiment in which a thermoluminescence dosimeter was used, the dose rate of gamma rays near the THOR irradiation tube was found to be about 0.04 Gy/s. We used the 60Co gamma-ray source to independently irradiate samples #1 and #4 to obtain gamma-only results. The accumulated gamma-ray dose was controlled to be the same as that being irradiated in the nuclear reactor for 2 h. Using the current 60Co source, it took 350 h to reach the same gamma-ray dose.
It is known that the irradiation of neutrons and gamma rays would change the refractive index of LiNbO
3 [
9,
10], so as to alter the phase-matching condition of the nonlinear optical process within it. It is also necessary to know the change in optical transmission after neutron and gamma-ray irradiation, since the nonlinear optical performance is strongly affected by the intensities of interacting waves. Samples #0, #1, #2, and #3 are x-cut LiNbO
3 crystals for measuring transmission spectra. The transmission spectra of the irradiated samples were measured by a Shimadzu grating spectrophotometer (UV-3101PC). The measurable wavelength range is from 190 nm to 3200 nm. The light sources are switched automatically in conjunction with wavelength scanning. To efficiently measure the full wavelength range, we initialized the configuration to have a scanning speed of 100 nm/min with a 2 nm sampling interval. Some unexpected spikes near the 850 nm wavelength in the measured transmission spectra during the switching of light sources occurred and were neglected for the broad range measurement.
2.1. Gamma Energy Spectrum of Neutron Activation Products
In order to see neutron-activated products in neutron-irradiated LiNbO
3, sample #3 was sent to a gamma energy spectrum analyzer after irradiation. After 24 h of cooling, the sample was measured using a high-purity germanium detector (GC3020, Canberra Industries, Inc., Meriden, CT, USA) coupled with a multichannel analyzer and a software package (Genie 2000, Canberra Industries, Inc., Meriden, CT, USA). The measured gamma-ray spectrum of the chip irradiated by neutrons is shown in
Figure 1. The prominent gamma rays (935 keV) were emitted from
92mNb (half-life 10.15 d), which is produced through
93Nb (n,2n)
92mNb reaction. The measured activity of
92mNb was about 2000 Bq. Some interfering gamma rays emitted from
24Na,
82Br,
122Sb, etc. were also observed. Those nuclides were formed by neutron capture reactions with impurities in the sample. The LiNbO
3 sample is optical-grade and contains a very small number of impurities. The remaining activity was insignificant after cooling. The radiation dose rate on the sample surface after 24 h of cooling was only 0.5 µSv/h, which mean that it was not necessary to use a lead container for radiation shielding while retrieving the sample from the neutron irradiation facility. Seven days after the first gamma spectrum measurement, the sample was measured again. It was found that most of the short-lived radio nuclides had decayed.
92mNb can still be measured, but the activity is significantly reduced in accordance with its 10.15-day half-life. In-crystal gamma emission should not affect the following experiments.
2.2. Change in Absorption after Irradiation
Figure 2 shows the absorption coefficient change for neutron and gamma-irradiated LiNbO
3 as a function of wavelength. The absorption coefficient change, Δ
α, is the relative change in absorption coefficient with respect to that of sample #0 and is defined by
where
L is the thickness of the sample,
T#0 is the original transmission of sample #0, and
T#1,2,3 are the original transmission of samples #1,2,3. The change in absorption coefficient for the gamma-irradiated sample (#1) is very small, showing that congruent LiNbO
3 is less susceptible to gamma irradiation in optical transmission during the measured wavelength region. However, the neutron-irradiated samples (#2 and #3) showed a significant change in optical absorption, especially during the visible region. From the actual photo of the four samples, the neutron-irradiated samples are apparently “brown”, demonstrating the increased absorption in the shorter visible region. This broad band absorption in the visible region is primarily due to the oxygen vacancies induced by radiation, as the displacement damage is related to the oxygen vacancies and their corresponding interstitials trapped within the lattice [
12,
13,
14]. The radiation-induced change in absorption was not smoothly changed with the wavelength in
Figure 2. This was due to changes in the light sources in the spectrophotometer and the etalon effect of the 1-mm-thick sample. Since sharply decreased transmission occurs in the cut-off wavelength region (200~300 nm), the deduced radiation-induced changes in absorption during that region was very sensitive to tiny measurement instabilities and could be ignored.
Figure 3 shows the room-temperature dark change in absorption (for sample #3) as a function of days after neutron irradiation for four specific wavelengths (532 nm, 1064 nm, 1550 nm, and 3200 nm). At room temperature, the absorption continuously increased from day 2 to day 7 after irradiation, and then slightly decreased from day 7 to day 9, ending stationary after day 13. The change in absorption after neutron irradiation was more significant for the 532 nm wavelength and was much smaller for the 1064 nm, 1550 nm, and 3200 nm wavelengths. The dark change in absorption was not obvious for 1550 nm.
Thermal neutrons produce displacement damage mostly through (n, γ) reactions, while fast neutrons produce displacement damage through elastic collisions due to the recoil induced by the emission of the gamma photons [
15,
16]. The
6Li (n, α)
3H nuclear reaction also needs to be considered for LiNbO
3 since α and
3H also produce displacement damage [
17]. In fact, the
6Li (n, α)
3H reaction is the main source of damage, since the thermal cross section for this reaction is larger than the absorption cross sections of all other constituents. In addition, the damage production due to the charged MeV reaction products is high [
17]. The displacement damage alters the optical characteristics of LiNbO
3 and continuously relocates after neutron irradiation under room temperature until the whole structure becomes stable several days after irradiation.
2.3. QPM SHG Performance after Irradiation
After radiation-induced absorption was confirmed, we conducted a third-order QPM SHG experiment for radiation-irradiated PPLN samples to examine their nonlinear optical performance. The schematic experimental setup is shown in
Figure 4. A pulsed laser was used as the fundamental source. It is a 1064 nm passively Q-switched Nd:YAG laser, generating 1-ns pulses with a pulse energy of 9 µJ and a 3.76-kHz repetition rate. The peak power is 9 kW and the average power is 34 mW. An attenuator-isolator set, consisting of a Faraday rotator following a half-wave plate, controls the pump energy and eliminates the optical feedback. The focusing mirror focuses the pump laser beam to the PPLN crystal. The oven, containing the PPLN crystal, maintains the temperature at the SHG phase-matching temperature. The SHG temperature tuning curve acts as a sinc function and can be measured by recording the SHG power while tuning the PPLN temperature. The phase-mismatch caused by neutron irradiation can thus be determined in terms of the changes in the phase-matching temperature.
Due to radiation-induced absorption, it was expected that the SHG conversion efficiency would be decreased, as would the effective nonlinear coefficient after irradiation. However, the high-peak power of the fundamental laser would still result in high-efficiency SHG, even if significant radiation-induced absorption exists. Thus, the focusing condition was intentionally not optimized and the conversion efficiency was less than 10% to avoid running into a highly depleted regime. The SHG power at 532 nm was measured by a calibrated thermal detector. The response time of the thermal detector eliminated the effect of the ~10% Q-switch energy jitter and precisely measured the average SHG power.
Owing to the dark recovery observation, we conducted the SHG experiments 13 days after irradiation (at the 14-th day).
Figure 5 shows the phase-matching temperature tuning curve obtained for the neutron-irradiated PPLN samples. Sample #0A was a reference PPLN crystal without any irradiation. Samples #5 and #6 were irradiated by THOR for 1 h and 2 h, respectively. The gamma-irradiated PPLN crystal (sample #4) had a similar temperature tuning curve as sample #0A and was not shown in
Figure 5 for a clearer presentation. Notice that the discrepancy between the measured phase-matching temperature and the theoretical value for sample #0A is due to the temperature gradient between the temperature sensor and the PPLN crystal and the possible fabrication error of the PPLN gratings.
The experimental results showed that gamma rays did not affect the optical absorption of LiNbO
3 with the radiation dose up to 288 Gy. The SHG phase-matching condition was also not altered. However, the irradiation of neutrons caused strong absorption during some specific wavelength regions, especially in the visible and the mid-infrared region. According to the Kramers–Krönig relations in nonlinear optics, the strong absorption should result in the dispersion of optical materials. Nonlinear optical processes in a neutron-irradiated LiNbO
3 crystal would have a different phase-matching condition.
Figure 5 demonstrates that the phase-matching temperature was down-shifted by ~1 °C and ~3 °C for the 1-h- and 2-h-neutron-irradiated PPLN samples, respectively. Additionally, as shown in
Figure 5, the SHG conversion efficiencies for the two neutron-irradiated PPLN samples were comparable to that of the non-irradiated one. It is known that the absorption loss of the interacting waves dramatically decreases the conversion efficiency of a second-order nonlinear process. In our experiment, the increased absorption coefficient (~0.55 cm
−1) for 532 nm corresponded to a ~50% transmission loss for the 1.5-cm-long PPLN crystal. For the neutron-irradiated PPLN crystals, we expected to obtain SHG efficiencies which are significantly lower than the non-irradiated one. However, we found that the SHG efficiencies are still comparable to the non-irradiated one. Even though the measured SHG efficiencies for the two irradiated samples seem to be only slightly smaller, the result still demonstrated that the nonlinearity of LiNbO
3 after irradiation would be increased. It is evident that neutron irradiation not only introduced optical absorption but also caused increased effective nonlinearity in LiNbO
3 crystals. Further investigation needs to be carried out for this observation.
Photorefractive distributed feedback (DFB) grating in PPLN is reported in our previous experiment, in which the preliminarily results of DFB optical parametric oscillation (DFB OPO) in PPLN were demonstrated [
18]. During the experiment in ref. [
18], we found that UV-induced infrared absorption (UVIIRA) is an issue for laser application. Investigations on UVIIRA have been conducted and reported [
19]. Ultra-long lifetime UVIIRA in congruent LiNbO
3 was observed, showing that absorption coefficient change in congruent LiNbO
3 is significant if UV light is used for creating photorefractive grating in a LiNbO
3 crystal. This makes UV photorefractive scheme inefficient for DFB OPO. Irradiation of gamma rays with a suitable dose would greatly introduce index change in bulk LiNbO
3 crystals [
9] without affecting optical absorption and nonlinearity. This could be an alternative way of producing DFB grating for DFB OPO if an appropriate method of spatially distribution of gamma rays is utilized; for example, the periodic deposition of lead upon the surface of PPLN. Neutrons could be also useful for creating non-volatile index changes in bulk LiNbO
3 crystals, despite the disadvantage of introducing optical absorption. According to our experimental results, the nonlinear optical performance in neutron-irradiated PPLN crystals for third-order QPM SHG was not susceptible after neutron irradiation. Irradiation of neutrons could also be useful for nonlinear optical applications that require non-volatile changes in the refractive index for phase adjusting or modulation.