Mahlik S, Lazarowska A, Grinberg M, Wells J-P R, Reid M F
Institute of Experimental Physics, University of Gdańsk, Wita Stwosza 57, 80-952 Gdańsk, Poland.
J Phys Condens Matter. 2015 Aug 5;27(30):305501. doi: 10.1088/0953-8984/27/30/305501. Epub 2015 Jul 14.
We present a detailed spectroscopic investigation of CaF2 doped with Yb(2+) performed at high hydrostatic pressure which is applied in a diamond anvil cell. At ambient pressure and at temperatures lower than 175 K, the luminescence consists of a single broad band peaked at 18 500 cm(-1), attributed to the recombination of impurity-trapped excitons. Increasing pressure causes the luminescence to be observable at higher temperature. At a pressure of 72 kbar luminescence can be observed up to 275 K. The emission lineshape does not strongly depend on pressure below 85 kbar. However, at 85 kbar it is blue shifted to 21 630 cm(-1). This is attributed to the known phase transition of the CaF2 crystal from cubic to the orthorhombic phase. The absolute energy of the ground and 4f(13)5d states of Yb(2+) as well as the energy of the impurity-trapped exciton with respect to valence and conduction bands have been estimated. The results, are discussed in comparison with the pressure dependences observed for the luminescence of BaF2 : Eu(2+) and CaF2 : Eu(2+). The difference between the spectral properties of Eu(2+) and Yb(2+) is attributable to the fact that the ground and 4f(6)5d states of Eu(2+) are placed deeper in the CaF2 bandgap than the ground and excited 4f(13)5d states of Yb(2+), whereas the energies of the impurity-trapped exciton states for Yb(2+) and Eu(2+) with respect to the conduction band are approximately the same.
我们展示了在金刚石对顶砧池中施加的高静水压力下对掺Yb(2+)的CaF2进行的详细光谱研究。在环境压力和低于175 K的温度下,发光由一个在18500 cm(-1)处达到峰值的单一宽带组成,这归因于杂质捕获激子的复合。压力增加导致在更高温度下可观察到发光。在72 kbar的压力下,高达275 K时都能观察到发光。在85 kbar以下,发射线形状对压力的依赖性不强。然而,在85 kbar时,它蓝移至21630 cm(-1)。这归因于CaF2晶体从立方相到正交相的已知相变。已经估计了Yb(2+)的基态和4f(13)5d态的绝对能量以及杂质捕获激子相对于价带和导带的能量。将结果与在BaF2:Eu(2+)和CaF2:Eu(2+)发光中观察到的压力依赖性进行了比较讨论。Eu(2+)和Yb(2+)光谱特性的差异归因于这样一个事实,即Eu(2+)的基态和4f(6)5d态在CaF2带隙中的位置比Yb(2+)的基态和激发态4f(13)5d态更深,而Yb(2+)和Eu(2+)的杂质捕获激子态相对于导带的能量大致相同。