Judd-Ofelt analysis, frequency upconversion, and infrared photoluminescence of Ho3+ -doped and Ho3+/ Yb3+ -codoped lead bismuth gallate oxide glasses

Research output: Journal Publications and ReviewsRGC 21 - Publication in refereed journalpeer-review

124 Scopus Citations
View graph of relations

Author(s)

Related Research Unit(s)

Detail(s)

Original languageEnglish
Article number103105
Journal / PublicationJournal of Applied Physics
Volume106
Issue number10
Publication statusPublished - 2009

Abstract

Ho3+ -doped and Ho3+/ Yb3+ -codoped lead bismuth gallate (PBG) oxide glasses were prepared and their spectroscopic properties were investigated. The derived Judd-Ofelt intensity parameters ( 2 =6.81× 10-20 cm2, ω4 =2.31× 10-20 cm2, and ω6 =0.67× 10-20 cm2) indicate a higher asymmetry and stronger covalent environment for Ho3+ sites in PBG glass compared with those in tellurite, fluoride (ZBLAN), and some other lead-contained glasses. Intense frequency upconversion emissions peaking at 547, 662, and 756 nm as well as infrared emissions at 1.20 and 2.05 μm in Ho3+ / Yb3+ -codoped PBG glass were observed, confirming that energy transfer between Yb3+ and Ho3+ takes place, and a two-phonon-assisted energy transfer from Yb3+ to Ho3+ ions was determined by the calculation using phonon sideband theory. The 1.20 μm emission observed was primarily due to the weak multiphonon deexcitation originated from the small phonon energy of PBG glass (∼535 cm-1). A large product of emission cross-section and measured lifetime (9.93× 10-25 cm2 s) was obtained for the 1.20 μm emission and the gain coefficient dependence on wavelength with population inversion rate (P) was performed. The peak emission cross-section for 2.05 μm emission was calculated to be 4.75× 10-21 cm2. The relative mechanism of Ho3+ -doped and Ho3+ / Yb3+ -codoped PBG glasses on their spectroscopic properties was also discussed. Our results suggest that Ho 3+ / Yb3+ -doped PBG glasses are a good potential candidate for the frequency upconversion devices and infrared amplifiers/lasers. © 2009 American Institute of Physics.

Citation Format(s)