Electron spin dynamics in Ce3+ : YAG crystals: Hyperfine interaction of 4f and 5d electrons
Source abstract
Abstract
The electron spin dynamics of $\mathrm{C}{\mathrm{e}}3+$ ions in YAG crystals is studied by time-resolved photoluminescence spectroscopy with an alternating left and right circularly polarized continuous-wave laser modulation technique. The electron spin relaxation due to hyperfine interaction with randomly oriented nuclear spins can be efficiently suppressed by a weak external longitudinal magnetic field. The suppression of the hyperfine-induced spin relaxation makes the electron spin polarization increase from 0.001 to 0.016 for the lowest $4f$ state, and from 0.08 to 0.32 for the lowest $5d$ state. The suppression magnetic fields for the $4f$ electrons are several times weaker than that for the $5d$ electrons, dependent on the crystal orientation. The dispersion of the local hyperfine field distribution $\mathrm{\ensuremath{\Delta}}B$ is isotropic and equal to 4.0 mT for the $5d$ electrons, and anisotropic for the $4f$ electrons with $\mathrm{\ensuremath{\Delta}}{B}[001]=0.8\phantom{\rule{0.16em}{0ex}}\mathrm{mT},\mathrm{\ensuremath{\Delta}}{B}[110]=1.1\phantom{\rule{0.16em}{0ex}}\mathrm{mT},\mathrm{\ensuremath{\Delta}}{B}_{[1\overline{1}0]}=2.4\phantom{\rule{0.16em}{0ex}}\mathrm{mT}$. The hyperfine coupling strength for the $4f$ electrons is \ensuremath{\sim}4 times weaker than that for the $5d$ electrons.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Quantum optics and atomic interactions · Atomic and Subatomic Physics Research · Photorefractive and Nonlinear Optics
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References (24)
Show source-provided references
1. 10.1103/PhysRevA.57.12010.1103/PhysRevA.57.120 ↗
2. 10.1103/PhysRevLett.83.420410.1103/PhysRevLett.83.4204 ↗
3. 10.1038/s41467-018-04359-610.1038/s41467-018-04359-6 ↗
4. 10.1038/nphoton.2015.5810.1038/nphoton.2015.58 ↗
5. 10.1063/1.369606910.1063/1.3696069 ↗
6. 10.1103/PhysRevB.65.20530910.1103/PhysRevB.65.205309 ↗
7. 10.1103/PhysRevB.67.19532910.1103/PhysRevB.67.195329 ↗
8. 10.1103/PhysRevLett.88.18680210.1103/PhysRevLett.88.186802 ↗
9. 10.1103/PhysRevLett.94.11660110.1103/PhysRevLett.94.116601 ↗
10. 10.1103/PhysRevB.93.12530210.1103/PhysRevB.93.125302 ↗
11. 10.1063/1.170824710.1063/1.1708247 ↗
12. 10.1016/0168-9002(94)90500-210.1016/0168-9002(94)90500-2 ↗
13. 10.1088/0957-0233/17/4/R0110.1088/0957-0233/17/4/R01 ↗
14. 10.1103/PhysRevLett.111.12050210.1103/PhysRevLett.111.120502 ↗
15. 10.1038/ncomms489510.1038/ncomms4895 ↗
16. 10.1103/PhysRevB.96.07516010.1103/PhysRevB.96.075160 ↗
17. 10.1063/1.498423210.1063/1.4984232 ↗
18. 10.1134/S106378341406003110.1134/S1063783414060031 ↗
19. 10.1063/1.500788610.1063/1.5007886 ↗
20. 10.1002/pssb.20160063110.1002/pssb.201600631 ↗
21. 10.1103/PhysRevLett.97.05660210.1103/PhysRevLett.97.056602 ↗
22. 10.1103/PhysRevLett.99.03660410.1103/PhysRevLett.99.036604 ↗
23. 10.1063/1.502086110.1063/1.5020861 ↗
24. 10.1103/PhysRevA.76.04383110.1103/PhysRevA.76.043831 ↗