Spectral hole burning of Eu2+ in CaF2

被引:19
作者
Boye, DM
Macfarlane, RM
Sun, Y
Meltzer, RS
机构
[1] IBM CORP,ALMADEN RES CTR,SAN JOSE,CA 95120
[2] UNIV GEORGIA,DEPT PHYS & ASTRON,ATHENS,GA 30602
来源
PHYSICAL REVIEW B | 1996年 / 54卷 / 09期
关键词
D O I
10.1103/PhysRevB.54.6263
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
Spectral hole burning on the 4f(7)(S-8(7/2))-->4f(6)5d transition of Eu2+ is observed to occur by two mechanisms in CaF2:Eu2+. At zero magnetic field, persistent spectral hole burning occurs by two-step photoionization where the hole burning survives cycling to room temperature. The observed hole spectrum is compared with a calculation which considers the small Eu2+ ground-state splitting and both the ground- and excited-state hyperfine interactions. In a magnetic field above 1 T, transient spectral hole burning occurs by population redistribution among the ground-state hyperfine levels. Long-lived (minutes) holes are observed for a half integral spin system. The resulting hole spectrum consists of holes, antiholes, and a nuclear spin-flip sideband and can be explained from the hyperfine interactions in the ground and excited states. The dominant hole decay occurs by phonon-induced transitions among hyperfine levels of the M(S) = -7/2 and M(S) = -5/2 electron-spin sublevels. Central hole linewidths of 200 MHz are observed at zero magnetic field. Hole linewidths at high magnetic fields are as narrow as 40 MHz but these are inhomogenously broadened by superhyperfine interactions with the F nuclear spins. Estimates of hole-burning quantum efficiency are also obtained.
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页码:6263 / 6271
页数:9
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