2016
DOI: 10.1016/j.jallcom.2016.07.048
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Spectroscopic properties and laser performances of Yb:LGSB nonlinear optical crystal

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Cited by 12 publications
(8 citation statements)
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“…The absorption cross-section, a at 980 nm for σ-polarization is about 0.6×10 −20 cm 2 with a bandwidth (FWHM definition) of 33 nm, being 1.65 times larger than that of Yb:YAB crystal [2]. In the case of π-polarization, the highest a was determined to be 0.37×10 −20 cm 2 at 904 nm, being close to the value reported for Yb:LGSB crystal [3]. Furthermore, spectroscopic studies revealed an intrinsic disorder due to the presence of Yb 3+ ions in the trigonal prismatic sites occupied by La 3+ and Y 3+ ions and also in the octahedral sites occupied by Sc 3+ ions.…”
supporting
confidence: 74%
“…The absorption cross-section, a at 980 nm for σ-polarization is about 0.6×10 −20 cm 2 with a bandwidth (FWHM definition) of 33 nm, being 1.65 times larger than that of Yb:YAB crystal [2]. In the case of π-polarization, the highest a was determined to be 0.37×10 −20 cm 2 at 904 nm, being close to the value reported for Yb:LGSB crystal [3]. Furthermore, spectroscopic studies revealed an intrinsic disorder due to the presence of Yb 3+ ions in the trigonal prismatic sites occupied by La 3+ and Y 3+ ions and also in the octahedral sites occupied by Sc 3+ ions.…”
supporting
confidence: 74%
“…On the other hand, the absorption cross-section at 980 nm was higher for σ-polarization, having a maximum value of σ abs = 0.6 × 10 −20 cm 2 with an associated FWHM of 33 nm. Compared to other huntite-type crystals, the value of σ abs at 980 nm was smaller than that of the well-known YAB:Yb crystal (σ abs = 3.4 × 10 −20 cm 2 ) [45] and close to the value for the LGSB:Yb crystal (σ abs = 0.47 × 10 −20 cm 2 ) [46]. However, the FWHM bandwidth was larger, with a factor of 1.65, than the corresponding value for the YAB:Yb crystal (FWHM of 20 nm at 975 nm) [45], thus being advantageous for laser diode pumping.…”
Section: Spectroscopic Propertiescontrasting
confidence: 55%
“…Taking into account that Yb 3+ ions may substitute both RE 3+ (RE = La, Y) and Sc 3+ ions, we can attribute this shift to the modification of the contents of RE and Sc cations in the LYSB host matrix induced by doping with Yb 3+ ions. Compared to the isostructural LGSB:Yb crystal [46], LYSB:Yb had a higher transmission and also showed no absorption lines in the UV spectral range specific to Gd 3+ ions, thus being more advantageous for NLO applications, particularly in the UV domain. The room-temperature (300 K) and low-temperature (10 K) absorption and emission spectra of the LYSB:Yb (4 at.%) crystal were recorded in polarized light on a 0.93 mm thick crystal sample oriented perpendicular to the a-axis direction (a-cut).…”
Section: Spectroscopic Propertiesmentioning
confidence: 99%
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“…The advantage of the LGSB crystal is that it can be grown to a large size and with a high quality by the Czochralski method. In the same year, Khaled et al achieved efficient laser emission from a Czochralski grown 12.9-at.% Yb:LGSB nonlinear optical crystal, reporting 0.94 W CW output power at 1070 nm, for a P abs = 2.8 W at 972 nm, with 44% slope efficiency [29].…”
Section: Introductionmentioning
confidence: 99%