1. Introduction
Hermite–Gaussian (HG
mn) laser beams, with specific intensity and phase distribution, have potential applications in many cutting-edge scientific scenarios [
1,
2,
3,
4,
5]. The typical methods for generating HG
mn laser beams are off-axis diode-end-pumping gain modules [
6,
7,
8] or inserting specific optical components such as a spiral phase plate [
9] and spatial light modulator [
10] in the laser cavity. Generally, the output power of most HG
mn laser beams is only one watt level or less. For example, a 265 mW average power and 1.7 kW peak power HG
mn laser beam was obtained using a passively Q-switched Nd:YVO
4 microchip laser based on off-axis pumping [
11]. In another work, an average power of less than 1.3 W with nanosecond (ns) pulse width and ~4 kW peak power has been achieved in a decentered Gaussian beam pumped Q-switched Nd:YAG microchip laser for different high-order transverse modes [
12].
A one-dimensional high-order HG
0n laser beam is a typical HG
mn laser beam, where
m = 0. This means no dark bars are crossing the pattern in the x-direction, while the number of dark bars in the y-direction is
n, so the HG
0n laser beams display as strip shape. Due to the fact that HG
0n laser beams can be easily converted into vortex Laguerre–Gaussian (LG
pl) beams carrying orbital angular momentum (OAM) by adopting the Astigmatic Mode Converter (AMC), the applications of HG
mn laser beams have been further expanded [
13,
14,
15], and the HG
0n laser beams with both high average power and high peak power are expected to be obtained.
As is well known, for the most commonly used off-axis pumping method, the radius of the pump beam with about a one-hundred-micrometer level is much smaller than the spot of the one-dimensional high-order HG0n mode beams, then the intensity of the HG0n mode beams inside and outside the pumping region is different. Consequently, the purity of the HG0n laser beams should be significantly reduced. On the other hand, in order to obtain HG0n laser beams with higher power, higher pump power is required, which will lead to significant thermal lens effects and thus affect the mode of the laser. Therefore, the development of a new method for obtaining high-average-power and high-peak-power, high-purity HG0n modes has become a hot research field.
Slabs with large aspect ratios have been widely used in laser systems because of their large gain volume, great pump uniformity, and favorable thermal management [
16,
17,
18]. Since the zig-zag optical path in the slab averages the thermal gradient, there is almost no first-order thermal lens effect, making it a promising method for extracting higher power while simultaneously maintaining good beam quality. In this letter, an alternative method for generating a high-purity, one-dimensional HG
0n laser beam has been proposed and demonstrated. Different from traditional approaches, a Nd:YAG slab with a large aspect ratio of 7.5 is selected as the gain medium. By adjusting the pump intensity, the size of the aperture pair in thickness and width directions of the slab, and the tilt angle of the output coupler (OC), the intracavity mode is controlled, and high-purity, ns one-dimensional HG
0n laser beams with orders 1 to 9 (HG
01 to HG
09) are obtained from the slab oscillator in Q-switched operation. The beam quality factors
M2 are in reasonable agreement with the theoretical values. Because the large aspect ratio slab provides an ideal amplifier for the strip-shaped HG
0n laser beam, further power scaling is realized. The seed beam from the oscillator is directly injected into the other identical slab as the amplifier. For the highest order HG
09 mode beam, the average power is amplified from 289 mW to 4.73 W with a pulse width of 294 ns, corresponding to a peak power of 32 kW.
2. Theoretical Analysis
According to the mode theory of the optical resonator, the self-reproducing field pattern of a square aperture flat–concave resonator can be expressed in rectangular coordinates as [
19]
where
is the beam radius on the axial position
z;
is the radius of curvature of the wavefront that intersects the axis at
z;
Cmn is the normalization constant;
w0 is the radius of the fundamental mode Gaussian beam at
z = 0, which can be calculated by the propagation matrix;
zR =
πw02/λ is the Rayleigh range of the mode; and
Hm and
Hn are the
mth- and
nth-order Hermite polynomial, respectively. In the transverse field distribution, the number of nodes with zero intensity in the x- and y-directions are
m and
n, respectively, so that for the one-dimensional HG
mn beams mentioned in this letter,
m = 0. The relationship between the radius of HG
0n mode and HG
00 mode can be obtained from Equation (1) [
20]:
Combined with the ABCD propagation matrix, the beam radius of HG0n mode at any position in the resonator can be calculated. Considering the ratio of the diameter of the one-dimensional HG0n beam in the x- and y-directions, the slab is selected as the gain medium due to the inherent advantage of its large aspect ratio.
To generate high-purity, one-dimensional HG0n laser beams, the fundamental mode in the slab’s thickness direction, i.e., the x-direction, needs to be determined first. A small aperture in the thickness direction of the slab provides an advantage for the fundamental mode output. On the other hand, an aperture that matches the diameter of the fundamental mode in the thickness direction of the slab can be inserted into the resonator to limit the transverse mode field in this direction; thus, only one-dimensional HG0n laser beams exist in the cavity.
Then, the high-order mode in the slab’s width (y-) direction must be ensured. Because the diameter of high-order modes is larger than that of the low-order mode, high-order modes can be suppressed using an intracavity aperture with proper width [
20]. The width of the aperture used for mode-limiting is adjusted according to the theoretical mode diameter of its position to ensure the highest order of the HG
0n mode that can exist in the cavity is
N. Due to the limitation of the aperture, only the HG
00 to HG
0N modes exist in the cavity. The width ratio of the two apertures in the width and thickness direction is just suitable due to the large aspect ratio of the slab.
Furthermore, to extract the high-purity HG
0N mode from the HG
00 to HG
0N modes, it is necessary to perform differential regulation on each order mode’s gain G
0n and loss L
0n. It can be seen from Equation (2) that the higher-order mode has a larger mode volume and a greater overlap with the gain region so that for slab configuration, the higher-order mode can occupy more population inversion; that is, the gain G
0n is larger. On the other hand, when the Fresnel number of the resonator is determined, the diffraction loss of the higher-order mode is higher than that of the lower-order mode [
21], so the threshold of the higher-order mode is generally higher than that of the low-order mode. But this can be changed by introducing OC tilt angles into the resonator. Previous studies have shown that for a given resonator, the misalignment of two cavity mirrors has less effect on higher-order modes [
22]. The introduction of the tilt leads to an increase in the total loss L
0n of each mode in the cavity, but the increase in the loss of the higher-order mode is less than that of the lower-order mode. For a given aperture, there is a suitable tilt angle that prevents the lower-order modes from oscillating, and the highest-order mode HG
0N wins in the mode competition. However, when the pump power is high, each order mode in the resonator can obtain sufficient gain, G
0n, which causes the simultaneous resonation of each mode in the cavity, producing a multimode laser output. Therefore, in order to achieve specific high-order mode output, the pump power needs to be controlled at a reasonable level. Thus, their output power is limited for a single oscillator.
The master oscillator power amplifier (MOPA) effectively scales the output power of high-purity HG0n laser beams. The slab with a large aspect ratio used in the amplifier provides an ideal condition for power scaling of strip-shaped HG0n laser beams without additional beam shaping. Another advantage of using a slab as an amplification gain medium is the simplicity of thermal management. Since the zig-zag optical path in the slab averages the thermal gradient, there is almost no first-order thermal lens effect, making it a promising method for scaling laser output to higher power while simultaneously maintaining good beam quality.
3. Generation of High-Purity, Nanosecond HG0n Laser Beams
The experimental setup of the oscillator for generating high-purity, nanosecond HG
0n laser beams is shown in
Figure 1. The laser oscillator includes a laser module, a pair of apertures A
x and A
y, a rear cavity mirror M1, an OC M2, and an acousto-optic (AO) Q-switch. The laser module contains a 0.6 at. % doped trapezoidal Nd:YAG slab crystal with dimensions of 139 mm × 30 mm × 4 mm (length × width × thick), having a large aspect ratio of 7.5. The cut angle of the two end facets of the slab is 56°, and both are coated with anti-reflective (AR) film at 1064 nm. The top surface of the slab is coated with an AR film for 808 nm, and the bottom surface of the slab is highly reflective (HR) at 808 nm for double-pass pumping. The top surface of the slab is edge-sealed with an O-ring, while the bottom surface is soldered on the oxygen-free copper heat sink with microchannels in order to maintain the temperature of the laser module at 20 °C (±0.2 °C) through a water cooler. The slab is face-pumped by six 808 nm quasi-continue-wave (QCW) microchannel-cooled laser diode arrays (LDA), with each array containing six bars. The temperature of cooling water for the LDA is tuned to 20 °C (±0.2 °C) to match the absorption spectrum of the crystal medium [
23]. A pump beam with a 300 μs pump pulse duration and 500 Hz pulse repetition rate (PRR) is normally incident on the top face of the slab via a quartz duct. The size of the pump region is 66 mm × 20 mm, so the effective aspect ratio in the pump region is 20 mm/4 mm = 5. The laser beam propagates along a zig-zag optical path in the slab, and the internal reflection angle between the optical path and the normal of the bottom face of the slab is 56.0°. The rear cavity mirror M1 is a concave mirror with curvature radius
R1 of 1600 mm coated with HR film at 1064 nm. The output coupler M2 with a transmittance (T) of 10% is placed on a mount with an adjustable tilt angle, while the tilt angle
θ in the y-o-z plane is the key to obtaining HG
0n laser beams. The AO Q-switch (SGQ27-1064-5QD, CETC) with a 5 mm × 5 mm active aperture is located in the front of the slab crystal. The arm lengths from the end facets of the slab to M
1 and A
y are
L1 = 110 mm and
L2 = 575 mm, respectively. Two apertures, A
x and A
y, with adjustable sizes in the thickness and width directions of the slab, are placed at
Lx = 20 mm and
Ly = 40 mm from M2, respectively. The total optical length of the resonator is 800 mm.
The sizes of apertures A
x and A
y in the thickness and width direction of the slab denote D
x and D
y, respectively. As mentioned above, D
x and D
y should be selected based on the resonator shown in
Figure 1. Since the zig-zag optical path averages the thermal gradient, the first-order thermal lens effect is almost ignored. The diameter of the beam at the position of A
y can be calculated by the ABCD propagation matrix, which is given by
where
is the optical path length in the slab;
L is the length of the Nd:YAG slab;
n is the refractive index of Nd:YAG, which is 1.82;
α is the angle between the laser path and the bottom surface of the slab;
LQ is the length of the AO Q-switch, which is 50 mm;
nq is the refractive index of the AO Q-switch, which is 1.45; and
R2 is the curvature radius of OC, which is taken as positive infinity in calculation. With the laser oscillator presented in
Figure 1, the beam diameter, under the assumption of the fundamental mode, can be expressed by
where
λ is the wavelength of the oscillating laser. Based on the beam diameter ratio between the HG
0n mode and the fundamental mode described in Equation (2), for a calculated 1.04 mm diameter fundamental mode at the position of A
y, the corresponding beam diameters of the HG
01 to HG
09 modes are about 1.80 mm, 2.33 mm, 2.76 mm, 3.13 mm, 3.45 mm, 3.76 mm, 4.04 mm, 4.30 mm, and 4.54 mm, respectively. Therefore, considering the 5 mm active aperture of the AO Q-switch, for the width direction of the slab, the width D
y of aperture A
y is adjusted to 2.0 mm, 2.4 mm, 3.0 mm, 3.4 mm, 3.8 mm, 4.0 mm, 4.3 mm, 4.5 mm, and 4.8 mm, respectively. A similar calculation is used to select the diameter D
x of the aperture A
x; in order to obtain the fundamental mode in the thickness direction of the slab, D
x is selected to be 1.3 mm.
A CMOS sensor (Beamage-4M, Gentec Inc., St-Jean-Baptiste, QC, CA) is used to record the intensity distribution of the output laser beams. The laser beams are focused by a lens with a 300 mm focal length. The tilt angle
θ of OC M2 in the y-o-z plane is adjusted carefully, and then the beam intensity profile changes can be observed. When the HG
0n mode spatial profile with the strongest contrast is displayed on the CMOS at a given tilt angle
θ, as shown in
Table 1, the corresponding intensity distribution is recorded.
A beam quality analyzer (Beamage-M2, Gentec Inc., St-Jean-Baptiste, QC, CA) measures the beam quality factors
M2 of the output laser beams at different apertures A
y and M2 tilt angles.
Figure 2 shows the typical beam quality factors of the highest order HG
09 mode in the x- and y-directions, which are
Mx2 = 1.15 (blue) and
My2 = 19.96 (red), respectively. The inset of
Figure 2 displays the corresponding three-dimensional (3D) beam spatial intensity distribution at the far field, indicating nine intensity peaks.
Figure 3 shows the measured beam quality factors
Mx2 (blue triangle) and
My2 (red circle) of the HG
01 to HG
09 modes in the x- and y-directions, respectively. In
Figure 3, it can be seen that the beam quality factors (
Mx2,
My2) of the HG
01 to HG
09 modes are (1.19, 3.44), (1.20, 5.58), (1.14, 7.09), (1.15, 9.98), (1.17, 11.20), (1.26, 13.39), (1.22, 15.79), (1.25, 17.10), and (1.15, 19.96), respectively. Considering the theoretical beam quality factor
Mx2 = 1 for the ideal fundamental mode in the x-direction and the beam quality factor
My2 = 2
n + 1 for the ideal HG
0n mode in the y-direction [
24], the measured data are in reasonable agreement with the theoretical values. The corresponding two-dimensional (2D) intensity distribution is also shown in the insets of
Figure 3, which exhibits high-purity HG
0n modes for orders 1 to 9. These results verify the feasibility of obtaining high-purity HG
0n laser beams by using a large aspect ratio Nd:YAG slab.
The output power of the HG
01 to HG
09 modes is measured with a power meter (30A-BB-18, Ophir Inc., Jerusalem, Israel), and the results are shown in
Table 1. It can be seen that the power is approximately 330 mW and fluctuates with the order, but for the highest order HG
09 mode laser, the average power is about 289 mW. This is partly due to the larger tilt angle of the OC M2 in the y-o-z plane.
4. Power Scaling in MOPA System Using Cascaded Slab Module
The feasibility of power scaling is the inherited advantage of selecting a large aspect ratio slab module. A cascaded slab gain module is used for laser amplification. This amplification module is the same as the laser module mentioned earlier in the article, which includes a 0.6 at. % Nd
3+ doped 139 mm × 45 mm × 4 mm (length × width × thick) trapezoidal Nd:YAG slab, a 6 × 6 LDA with 808 nm pump wavelength, 300 μs pump pulse duration and 500 Hz PRR, and a quartz duct. The temperature of the amplification module is also maintained at 20 °C (±0.2 °C). The experimental configuration scheme of the amplifier is shown in
Figure 4a, and the picture illustrating the real system is also shown in
Figure 4b. The seed pulse output from the oscillator is injected into the slab amplification module. To achieve higher energy extraction, a double-pass amplification geometry is adopted. The internal reflection angles between the two optical paths and the normal of the bottom face of the plate are 56.0° and 68.9°, respectively. The change in the optical path is due to the use of flat mirrors M3 and M4 coated with 35°~45° HR film at 1064 nm. After passing through the amplifier, the beam is divided into two parts by a beam splitter. The main part enters the power meter for the power measurement, and the leaking part is incident on CMOS to record the beam intensity distribution.
Figure 5 shows the amplified two-dimensional (2D) intensity distribution of HG
01 to HG
09 beam modes. Meanwhile, the normalized intensity curves (red) in the y-direction are shown in
Figure 5, and the corresponding theoretical normalized intensity curves (blue) are also shown in
Figure 5. In general, the experimental results are in reasonable agreement with the numerical simulation. Compared to the theoretical model, the slight intensity deviation of the beam in the experiment may be caused by the residual lower-order HG
0n modes.
The purity of the mode is described by using the Pearson correlation coefficient
ρ:
where
Ii is the measured normalized intensity of each pixel,
is the average value of normalized intensities of all pixels,
Ii* is the normalized intensity obtained by the theoretical calculation, and
is the corresponding average value. The correlation coefficient of the highest order HG
09 mode is calculated as
ρ09 = 0.944, while the correlation coefficient of other modes
ρ0n > 0.93. It can be observed that the measured laser beams all have longer tails in the edge region of the x-direction. The diffraction effect of the intracavity aperture and the beam diffusion caused by the off-axis aberration of the cavity mirror are the reasons for the insufficient sharpness of the edge reduction.
Figure 6a shows the amplified output power of typical mode HG
09 (blue) versus the LD pump power. From
Figure 6a, it can be seen the output power shows a monotonic increase with the incident pump power, amplifying from 289 mW to 4.73 W. The increase of output power is faster with the increase of the incident pump power and does not show any saturation effect up to around 850 W pump power. The amplified output powers of the HG
01 to HG
09 modes are also shown in
Figure 6b, and it can be seen from
Figure 6b that each output power from the HG
01 to HG
08 modes is higher than 5 W.
The pulse temporal characteristic of the amplified highest order HG
09 mode is monitored by a photodiode detector (DET10N/M, Thorlabs Inc., Newton, NJ, USA) connected to a 200 MHz bandwidth digital oscilloscope (SDS1204X-E, SIGLENT Inc., Shenzhen, Guangdong, China), as shown in
Figure 7 (red line). It was found that the pulse interval of the output pulse was 2 ms, indicating that the laser operated at a PRR of 500 Hz. The pulse-to-pulse amplitude fluctuation is less than 1.2% (Standard Deviation). The upper right inset of
Figure 7 expresses an expanded single pulse profile (blue line), showing a pulse width of 295 ns, so the peak power corresponds to 32 kW.
To expand the application, the following aspects, such as higher-order number
n of the HG
0n mode, narrow pulse width, and the conversion to vortex LG
pl modes, will be the focus of our future work. In this paper, the 5 mm × 5 mm active aperture of the AO Q-switch limits the upper boundary of order number
n, but with the use of the customized Q-switch with a larger aspect ratio aperture, HG
0n modes with order number
n higher than 9 will be generated. Meanwhile, by replacing the AO Q-switch with a saturable absorber, the mode-locking can be obtained, and the pulse width can be reduced to several hundred picoseconds. Although previous studies have shown that ultrafast high-power HG
mn laser beams are affected by other parameters like self-phase modulation and bandwidth [
25,
26], the relatively large dimensions of the gain medium, such as a slab with a large aspect ratio, will reduce the effect. Further conversion to vortex LG
pl modes can be achieved by using AMC composed of cylindrical lenses, which will be widely used in optical communication, material processing, and many other fields [
27,
28,
29].