2006
DOI: 10.1103/physrevb.74.214409
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Hyperfine interaction ofEr3+ions inY2SiO5

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Cited by 89 publications
(107 citation statements)
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“…The main drawback of Pr is the small hyperfine separation (of order a few MHz), which limits the possible pulse bandwidth and thus N , since by definition N ≤ L0 c∆t = L0γ 6c . Neodymium and Erbium have hyperfine separations of hundreds of MHz [24,25]. Nd also has strong absorption, e.g.…”
mentioning
confidence: 99%
“…The main drawback of Pr is the small hyperfine separation (of order a few MHz), which limits the possible pulse bandwidth and thus N , since by definition N ≤ L0 c∆t = L0γ 6c . Neodymium and Erbium have hyperfine separations of hundreds of MHz [24,25]. Nd also has strong absorption, e.g.…”
mentioning
confidence: 99%
“…Each site also contains two magnetic inequivalent subclasses related by C 2 rotation. However, in our experiment the two subclasses should be equivalent, which is the case when B 0 is parallel to D 1 -D 2 plane or b axis of the crystal [36,37].…”
mentioning
confidence: 80%
“…The Stark coefficient is about 20 kHz/(V· cm −1 ) in Er:YAlO3 [10], and 25 kHz/(V· cm −1 ) in Er:LiNbO3 [11]. The ground state hyperfine splitting for Er ions is much wider than that of Pr ions [12,13], a spectral hole of 575 MHz can be prepared in Er:Y 2 SiO 5 according to the hyperfine splittings provided in Ref. [14].…”
Section: Introductionmentioning
confidence: 99%