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Journal of Applied Physics

Persistent spectral hole burning studies of europium-doped sodium germanate glass

Rajamohan R. Kalluru, Chandra R. Pulluru, Bommareddi Rami Reddy

Published Sep 27, 2004• 8 citations
Publisher

Abstract

Persistent spectral hole burning has been observed in europium-doped sodium germanate glass. Hole-burning efficiency increased by 85% when the glasses were made in a reduced atmosphere, and hole burning was detected even at room temperature. There is evidence for photochemical as well as photophysical hole-burning mechanisms.
DOI
10.1063/1.1787908

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Persistent spectral hole burning has been observed at 77 K, 180 K, and room temperature for Eu(3+) in sodium aluminosilicate glass melted under a reducing atmosphere. In particular, room-temperature persistent spectral hole burning is reported for the first time to our knowledge in Eu(3+) -doped materials. The persistent hole is accompanied by no antiholes and lasts for 1 h at least. The thermal stability of the hole is greater than that of a persistent hole burned for Eu(3+) in sodium aluminosilicate glass melted in air.
We reported the first observation of room-temperature persistent spectral hole burning in Sm2+-doped fluoride glass in the last conference [1]. Room-temperature hole burning had been also observed in Sm2+-doped crystals [2]. We found considerable differences in the hole-burning characteristics between Sm2+-doped glasses and Sm2+-doped crystals: The burning-laser-intensity dependence is approximately linear, and no antihole is observed around the hole burned in Sm2+-doped glasses [3]. More detailed experimental studies are needed to clarify the mechanism of the hole burning in this glass and to explore more efficient hole-burning systems. In this paper, we report several experimental results related to wavelength dependence of the hole burning process.
Persistent spectral hole burning is observed in Sm(2+)-doped glasses at room temperature. The holes are burned in the (7)F(0) ? (5)D(0), (5)D(1) lines of the Sm(2+) ions in three kinds of fluoride glass. The dependence of the burning efficiency on the sample and on the burning intensity is measured. The intensity dependence is approximately linear, and no antihole is observed around the burned hole. The hole-burning mechanism is discussed. The temperature dependence of the homogeneous width is also measured.
Persistent and time-resolved transient holes were burnt into the 1D2^{1}\mathrm{D}_{2}1D2​${\ensuremath{\leftarrow}}^{3}$H4{\mathrm{H}}_{4}H4​ transition of Pr3+{\mathrm{Pr}}^{3+}Pr3+ and the 5D0^{5}\mathrm{D}_{0}5D0​${\ensuremath{\leftarrow}}^{7}$F0{\mathrm{F}}_{0}F0​ transition of Eu3+{\mathrm{Eu}}^{3+}Eu3+ in silicate glasses. The holewidths were studied as a function of burning-fluence density, wavelength, and temperature between 0.4 and 12 K. Transient holes arising from optical pumping of ground-state nuclear hyperfine levels were found for both ions at T3 K. Their lifetime decreases with increasing temperature. They are accompanied by symmetrically placed antiholes. For Eu3+{\mathrm{Eu}}^{3+}Eu3+, two pairs of antiholes were found which are attributed to the two europium isotopes, 151Eu^{151}\mathrm{Eu}151Eu and 153Eu^{153}\mathrm{Eu}153Eu. For Pr3+{\mathrm{Pr}}^{3+}Pr3+, an additional mechanism leading to persistent hole burning dominates above 3 K. The holewidth follows a ${\mathit{T}}^{(1.3\ifmmode\pm\else\textpm\fi{}0.1)}$ dependence for Pr3+{\mathrm{Pr}}^{3+}Pr3+ and a ${\mathit{T}}^{(1.0\ifmmode\pm\else\textpm\fi{}0.1)}$ dependence for Eu3+{\mathrm{Eu}}^{3+}Eu3+. The temperature dependence is the same as that of the contribution of the two-level systems to the specific heat measured on the same samples and in the same temperature range. The quadrupole splittings of the 7F0^{7}\mathrm{F}_{0}7F0​ ground state and the crystal-field splittings of the 7F1^{7}\mathrm{F}_{1}7F1​ and 7F2^{7}\mathrm{F}_{2}7F2​ levels of Eu3+{\mathrm{Eu}}^{3+}Eu3+ as a function of excitation wavelength indicate that the strength of the noncubic component of the crystal field varies monotonically for excitation across the 5D0^{5}\mathrm{D}_{0}5D0​${\ensuremath{\leftarrow}}^{7}$F0{\mathrm{F}}_{0}F0​ absorption band, falling to zero at the long-wavelength edge. The hole width shows a similar variation with excitation frequency. No influence of the experimental time scale on the hole width was detected for either sample between ${10}^{\mathrm{\ensuremath{-}}2}$ and 102{10}^{2}102 s.