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© 2021 MJH Life Sciences^{™} and Spectroscopy Online. All rights reserved.

November 5, 2020

Xiang Geng , Li Li , Chen Qian , Saiyu Luo**Special Issues**, Special Issues-10-01-2020, Volume 35, Issue S5

Xiang Geng

Li Li

Chen Qian

Saiyu Luo

Page Number: 39–45

A Judd-Ofelt analysis, quantifying the optical intensities of the rare-earth ions’ 4*f*-4*f* manifolds, is conducted in detail, based on the absorption spectrum from the visible to infrared spectral range for a Pr:YLF crystal. The values of key parameters, such as radiation lifetime, radiation transition probability, and branching ratio, are obtained accordingly. Additionally, the emission spectra are measured with precaution against reabsorption, and the emission cross sections are calculated using the Füchtbauer-Ladenburg formula, applied frequently in precise emission spectrum analysis, with the radiation lifetime derived from the Judd-Ofelt model. The results obtained regarding the orange and deep red spectral range are higher than those from previous reports, providing further insights into the lasing mechanism at the concerned wavelengths.

Highly-efficient visible lasers have attracted substantial research interest in recent years (1–5). Praseodymium (Pr), thanks to its energy structure (providing a direct down-conversion mechanism pumped by the booming blue diodes coming out recently) has become the most promising laser gain ion in the visible range (6). As for the host material, yttrium lithium fluoride (YLF), a positive uniaxial with tetragonal structure of scheelite type (7), is well-known for its superior physical and optical properties. The Mohs hardness of YLF is 4~5 (8), with a relatively high thermal conductivity (6 W·m^{-1}·K^{-1 }[8]) and expansivity (13×10^{-6} K^{-1} for *a*-axis, and 8×10^{-6} K^{-1} for *c*-axis [8]), facilitating its wide application in high-power lasers (9,10) and the Kerr lens mode-locking technique (11). In particular, Pr-doped YLF (Pr:YLF), as a fluoride crystal, is characterized by its low phonon energy (460 cm^{-1}), compared with its oxide counter- parts ( 550 cm^{-1 }for praseodymium-doped yttrium aluminum perovskite (Pr:YAP) with the formula Pr:AlYO_{3}, leading to a weaker non-radiative multi-phonon relaxation, and thus better lasing performance.

The spectroscopic characteristics of the crystal used in a laser being critical to laser performance, and involve both the absorption and emission spectra, respectively. The former can be derived through a Judd-Ofelt analysis, and the latter by employing the Füchtbauer-Ladenburg formula (14), both of which are analytical calculation procedures. Judd-Ofelt theory, which was proposed independently by B. R. Judd (12) and G. S. Ofelt (13) in 1962, describes the possibilities of radiative emissions in the 4f^{N} configuration, and is extensively adopted to determine the radiative lifetime and branching ratio of each emitting level for trivalent rare-earth-doped laser materials (15–24). On the other hand, the Füchtbauer-Ladenburg formula was derived from the fluorescence analysis correlated with an electronic transition (25), and has gained wide application in the determination of emission cross sections of laser gain media (22–24). To optimize the analytical procedure for characterizing Pr:YLF crystal, various improvements have been made in both theory and experiment. For example, Dunina and associates modified the Judd-Ofelt theory by considering the finite 4*f*-5*d* energy (26), Kornienko and colleagues introduced third order perturbation theory into the line intensity calculation (27,28), Goldner and associates adopted a normalized least-squares method in the fitting process to obtain a stable output (29), and Quimby and colleagues used the experimental branching ratios, other than theoretical ones, in deriving emission cross sections (30).

In this paper, the spectroscopic properties of a Pr:YLF laser crystal (31) were studied by analyzing the polarization-dependent absorption and emission spectra, accordingly. Radiation transition probabilities, theoretical branching ratios, and intrinsic radiation lifetimes were obtained from the absorption spectrum analysis. Experimental branching ratios were demonstrated by emission spectrum analysis. In addition, by introducing the intrinsic radiation lifetimes derived from Judd-Ofelt analysis and experimental branching ratios into the Füchtbauer-Ladenburg formula, emission cross sections are also reported.

**Experiment and Analysis**

**Absorption Spectrum**

For the absorption spectrum measurement, to reduce the absorption effect of the crystals, a relatively low doping concentration of 0.3 atomic percent (at.%) was adopted. The absorption spectrum was measured using a Lambda 1050 spectrophotometer (PerkinElmer). The data sampling interval was set at 0.05 nm. Polarizing prisms were placed in the sample path and the reference path, to measure absorption spectra in both polarizations.

The absorption coefficients for different wavelengths (*a*) were calculated from the absorption spectrum using equation 1:

where *L* is the length of the sample, and I_{ε} and I_{0} are the light intensities of the sample light path and the reference light path, respectively. The crystal absorption cross sections can then be calculated by equation 2:

where *N* = 4.2 × 10^{19 }cm^{-3 }is the lattice concentration of Pr^{3+} in the crystal. The calculated absorption cross sections are shown in Figure 1.

Table I lists the peak wavelengths, absorption cross sections, and line widths of major transitions in the visible spectral range. There are three absorption bands in the blue spectral range, corresponding to transitions ^{3}H_{4}→^{3}P_{J} (J = 0,1,2). Transition ^{3}H_{4}→^{3}P_{0}, peaking at 479.2 nm, possesses the largest absorption cross section (2.16 × 10-19 cm2) with the narrowest line width (0.5 nm). Transition ^{3}H_{4}→^{3}P_{2} (443.9 nm) has a relatively large absorption cross section (9.0 × 10^{-20} cm^{2}) and line width (1.8 nm). In addition, there are four major absorption bands in the infrared spectral region, ^{3}H_{4}→ ^{1}G_{4} at approximately 1 μm, ^{3}H_{4}→^{3}F_{3}+^{1}F_{4} at 1.5 μm and ^{3}H_{4}→^{3}F_{2} at 1.9 μm, and ^{3}H_{4}→^{3}H_{6} at 2.3 μm, respectively. From the calculation results ranging from the visible to the infrared regime, it can be concluded that the absorption cross sections in π polarization are generally larger than their σ counterparts.

According to the Judd-Ofelt theory (12,13), the experimental line intensity can be expressed as:

where *J* and *J’* are the total angular momentum quantum numbers of the initial and final energy levels, respectively, *c* is the speed of light in a vacuum, *h* is Planck’s constant, *n* is the refractive index, and Γ_{(J→J’)} is the ›integral absorption cross sections. The values of the polarization-dependent line intensities are listed in Table II, in which λ is the average of measured wavelength weighted by the accordance absorption cross sections.

The mean experimental line intensity is defined as

then the intensity parameters Ω_{2,4,6} can be achieved using the least squares fitting, performed as

where *U ^{t}* are doubly reduced matrix elements in accordance with specific rare-earth ions. In our case, we use matrix elements evaluated and given by Weber for Pr

The experimental and calculated values of line intensities, and doubly reduced matrix elements of absorption transitions, are shown in Table III.

To verify the calculation accuracy, the root-mean-square (RMS) error is calculated, and its expression is given by:

where *q* is the number of required parameters and *p* is the number of spectral bands to be analyzed. Combined with our calculation, where *p* = 7 and *q* = 3, the calculated Δ*S*_{rms}= 0.47×10^{-20} cm^{2}, the experimental line intensity RMS Δ*S* = 3.78×10^{-20} cm^{2}, and Δ*S*_{rms}/Δ*S* = 12%, which is within the normal scope (5%~25%) (35).

Using S_{calc} (*J*→*J’*), the radiation probability of different transitions *A*(*J*→*J’*) can be obtained by:

For transitions from the same excited state, the theoretical branching ratios β_{calc} can be obtained by:

The *intrinsic radiation lifetime* is defined as the reciprocal of the sum of all radiation transition probabilities from the same energy level, shown as equation 10. The radiation transition probabilities, theoretical branching ratios, and intrinsic radiation lifetimes of 3P0, 3P1, and 1I6 level are listed in Table IV.

Because electrons residing in ^{3}P_{0}, ^{3}P_{1}, and ^{1}I_{6} levels obey the Boltzmann distribution, the radiation lifetimes of those levels must be considered simultaneously. The effective radiation lifetime of the upper level is the average of the intrinsic radiation lifetimes of ^{3}P_{0}, ^{3}P_{1}, and ^{1}I_{6} level, according to the distribution of the number of electrons (36,37), given by

where *g*_{k} (k = ^{3}P_{0}, ^{3}P_{1}, and ^{1}I_{6}) is the degeneracy of corresponding energy level, being 1, 13, and 3, respectively, and Δ*E* is the energy difference between the ^{1}I_{6}+^{3}P_{1} level and the ^{3}P_{0} level.

By substituting the radiation transition rates listed in Table IV into equation 11, the effective radiation life- time of the upper energy level was calculated to be 49 μs, with a derivation of ±10%, derived from the error of Judd-Ofelt theory. The effective radiation lifetime of the upper level τ_{rad} and fluorescence radiation lifetime τ_{flu} is related by

where W_{nonrad} is the non-radiative transition rate, including multi-phonon transition (^{3}P_{J} →^{1}D_{2}), up-conversion, cross relaxation (^{3}P_{0}→^{1}G_{4} and ^{3}H_{4}→^{1}G_{4}, ^{3}P_{0}→^{1}D_{2} and ^{3}H_{4}→^{3}H_{6} [38,39]), and so on. It could be deduced that τ_{flu} decreases with the increasing of W_{nonrad}, which could be reduced by lowering the doping concentration of rare earth ions.

**Emission Spectrum**

In terms of the emission spectrum, the measurement device is shown in Figure 2. Using an InGaN laser diode (LD) with a wavelength of 444 nm as the pump source, the driving current was set at 100 mA, and the corresponding output power was about 30 mW. The pump light is focused into the sample, whose emitting spectrum was converged into the slit of the monochromator through a lens with large aperture and long focal length. A photo-multiplier (PMT, Hamamatsu R3896) was employed. The phase-locked amplification technique, implemented with a chopper, was utilized to extract the small signal in the noise. A Mercury vapor lamp (color temperature 2900 K) was used for wavelength correction and calculation of spectrometer transfer function. The experiments were conducted at room temperature.

The emission spectrum, showing multiple transitions in the visible range, is shown in Figure 3. The main transitions of ^{3}P_{0}→ ^{3}H_{4}, ^{3}P_{1}→ ^{3}H_{5}, ^{3}P_{0}→ ^{3}H_{6}, ^{3}P_{0}→ ^{3}F_{2}, ^{3}P_{0}→^{3}F_{3}, and ^{3}P_{0}→^{3}F_{4} correspond to the peak wavelengths of 479.4, 522.6, 607.2, 639.5, 697.7, and 720.7 nm. Blue ^{3}P_{0}→^{3}H_{4} (479.4 nm), green ^{3}P_{1}→^{3}H_{5} (522.6 nm), and deep red ^{3}P_{0}→^{3}F_{3} (697.7 nm) and ^{3}P_{0}→^{3}F_{4} (720.7 nm) are mainly π-polarized, while red light ^{3}P_{0}→^{3}F_{2} (639.5 nm) is mainly σ-polarized.

A stimulated emission cross section is usually treated as a parameter for evaluating the gain performance of the laser material. The methods for calculating the stimulated emission cross section mainly include the reciprocity method (40), the Füchtbauer-Ladenburg formula (14), and the reverse of the laser performance (41). The first method is applicable to quasi-three-level transitions with clarified ground-state level distribution, the second method is suitable to either quasi-three-level or four- level transitions with a highly accurate emission spectrum, and the third method is strongly dependent to the measurements of laser experiments. Based on the emission measurement results in the 450–750 nm spectral range, the Füchtbauer-Ladenburg formula was employed to calculate the stimulated emission cross section.

For a uniaxial laser crystal with two polarization directions, the Füchtbauer-Ladenburg formula can be written as (42):

For the branching ratio *β* in equation 13, experimental value *β*_{exp} was employed, instead of the theoretical value calculated based on Judd-Ofelt theory, owing to the small energy differences between the 4*f* and 4*f*–5*d* configurations in Pr^{3+}. *β*_{exp} was expressed by:

where the denominator is an integral over the entire fluorescence spectrum. The calculation results are shown in Table V.

By substituting equation 14 into equation 13, the numerator of *β*_{exp} can be eliminated; therefore, equation 13 could be simplified to

The results are displayed in Figure 4, with the emission cross sections and line widths of the main transitions listed in Table VI.

Note that the emission cross sections in *π* polarization are generally larger than those in σ polarization. The σ-polarized 640 nm transition has the largest emission cross section, reaching 22.3 x 10^{-20} cm^{2}.

It should be noted that some results different from those of previous reports (43,44) were demonstrated. For the orange transition at 607 nm, a slightly larger value was achieved (1.57×10^{-19} cm^{2}, compared with 1.4×10^{-19}cm^{2} [43]), thanks to the precaution to avoid the ground-state reabsorption process ^{3}H_{4}→^{1}D_{2}. In terms of the transitions in the deep red spectral region, the emission cross sections of 698 and 721 nm were 1.07×10^{-19} cm^{2} and 1.78×10^{-19} cm^{2}, about 2x larger than those in (43) (0.5×10^{-19 }cm^{2} and 0.9×10^{-19 }cm^{2}). Because emission cross sections are proportional to the corresponding laser thresholds, further investigations in the deep red range laser thresholds can be used to verify the accuracy of the emission cross sections.

**Conclusion**

The spectroscopic properties of a Pr:YLF laser crystal were studied theoretically and experimentally. The polarization-dependent ab- sorption cross sections at room temperature from the visible to infrared spectral range were demonstrated. The maximum absorption of 21.7×10^{-20} cm^{2} peaked at 478 nm, with the narrowest line-width of 0.5 nm. In the framework of Judd-Ofelt theory, intensity parameters Ω_{2,4,6} were obtained when the hypersensitive transition ^{3}H_{4}→^{3}P_{2} was excluded from the fitting procedure. For the emission spectrum, the experimental branching ratio was introduced to calculate the emission cross section using the Füchtbauer-Ladenburg formula in the visible spectral range. Results different from those seen in previous reports were obtained in both the orange and deep red spectral regions. This investigation provides insight into the spectroscopic analysis of Pr:YLF crystals used in lasers.

**Acknowledgments**

This work is supported by NSAF (No. U1830123), the National Natural Science Foundation of China (No. 61627802), the Natural Science Foundation of Jiangsu Province (No. BK20180460), and the High-Level Educational Innovation Team Introduction Plan of Jiangsu, China.

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**Xiang Geng**, **Li Li**, **Chen Qian**, and **Saiyu Luo** are with the School of Electronic and Optical Engineering, at Nanjing University of Science and Technology, in Nanjing, The People’s Republic of China. Direct correspondence to: 905645238@qq.com

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