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85033904074
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note
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All electrodynamical relations are given in SI units.
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10
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85033918427
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Diploma thesis, University of Nijmegen
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Groot Koerkamp, M., Diploma thesis, University of Nijmegen, 1995.
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Groot Koerkamp, M.1
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85033928493
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note
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An equivalent solution of equation (1) is given by Groot Koerkamp [10] with , /2Re(«)\ *=5arctanT-1-FJ. The solution of equation (1) for
yields an unphysical halving of the definition range to [-Tr/4, Tr/4], which is compensated by the angle
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12
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85033933970
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note
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Note, these conditions differ from the discussion of equation (4) in [3]. Koopmans et al. discussed a ±90° Kerr rotation for the case of s-polarized input light for normal incidence and a magnetiza-tion perpendicular to the photon polarization. Note, we define the Kerr rotation as the relative change of polarization directions of reflected to incident photons. Thus, K = E.,(ui)IEs(ui) and this yields the expected result of = O for the transversal Kerr geometry (polarization perpendicular to the in-plane magnetization).
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13
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85033907228
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note
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Note, in magneto-optics the observation of A/ = ±1 for dipole transitions is not required due to the addition of spin-orbit interaction. Furthermore, due to hybridization the discussed bands contain beside the p character also some /-electron character.
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14
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0026938282
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Kwon, Y.S.1
Suzuki, T.2
Kasuya, T.3
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15
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85033934285
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note
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Note, these conditions change when transitions for both majority and minority spin bands have to be considered.
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16
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0010394192
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Feil, H. and Haas, C., Phys. Rev. Lett., 58, 1987, 65.
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85033908723
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note
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Note the differences between CeSb and CeBi regarding the ellipticity and the off-diagonal conductivity a., s. Pittini et al. Note, CeBi exhibits less structure in at., and a, and a different frequency dependence suggesting different role of important electric dipole transitions.
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19
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0028409259
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