1998
DOI: 10.1103/physrevb.58.5173
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Magnetic x-ray scattering at relativistic energies

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Cited by 2 publications
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“…͑2.1͒ for energies larger than 100 keV has been demonstrated experimentally 1 and later confirmed theoretically. 12 Hence, to a first approximation, no orbital contribution to the magnetic signal exists with this method. For neutrons, on the other hand, the diffracted intensity is proportional to the linear combination L ជ (Q ជ )ϩ2S ជ (Q ជ ) of the Fourier transforms of the orbital and spin angular momenta.…”
Section: High-energy X-ray Diffractionmentioning
confidence: 95%
“…͑2.1͒ for energies larger than 100 keV has been demonstrated experimentally 1 and later confirmed theoretically. 12 Hence, to a first approximation, no orbital contribution to the magnetic signal exists with this method. For neutrons, on the other hand, the diffracted intensity is proportional to the linear combination L ជ (Q ជ )ϩ2S ជ (Q ជ ) of the Fourier transforms of the orbital and spin angular momenta.…”
Section: High-energy X-ray Diffractionmentioning
confidence: 95%
“…The validity of Eq. (1) for energies larger than 100 keV has been demonstrated experimentally [15] and later confirmed theoretically [17]. Hence, 3152 0031-9007͞01͞86(14)͞3152(4)$15.00…”
mentioning
confidence: 86%