1995
DOI: 10.1209/0295-5075/32/3/012
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Magnetic X-Ray Dichroism Study of the Nearest-Neighbor Spin-Spin Correlation Function and Long-Range Magnetic Order Parameter in Antiferromagnetic NiO

Abstract: A new effect on the X-ray absorption line shape is described which is proportional to the nearest-neighbor spin-spin correlation function. We present theory and demonstrate the use of linear polarized X-ray absorption spectroscopy to study the temperature dependence of the long-range order parameter and the nearest-neighbor spin-spin correlation function in antiferromagnetic NiO.

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Cited by 63 publications
(52 citation statements)
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“…Although quite small, this effect is however highly reproducible and is at least an order of magnitude larger than the noise. The effect can thus be trusted and, following earlier work on NiO thin films on MgO [5,20] can be associated with the occurrence of antiferromagnetic order. By plotting the intensity ratio between the two peaks at 867.7 and 868.9 eV (L 2 ratio) as a function of temperature, as done in the top panel of Fig.…”
mentioning
confidence: 73%
“…Although quite small, this effect is however highly reproducible and is at least an order of magnitude larger than the noise. The effect can thus be trusted and, following earlier work on NiO thin films on MgO [5,20] can be associated with the occurrence of antiferromagnetic order. By plotting the intensity ratio between the two peaks at 867.7 and 868.9 eV (L 2 ratio) as a function of temperature, as done in the top panel of Fig.…”
mentioning
confidence: 73%
“…The intensity of the XMLD signal in a single cycloidal magnetic domain, obtained by a spatial average of the collinear antiferromagnetic case [35], is proportional to M 2 3/2 cos 2 (k ·Ê) + 3/2 cos 2 (ẑ ·Ê) − 1 , where M 2 is the square of the local magnetic moment, whilek andẑ are the directions of the propagation vector and of the surface normal, respectively, andÊ is the polarisation vector of the light. The signal is maximum (∝ +M 2 /2) forÊ along the propagation vector, in which case the signal from the other two domains is ∝ −5M 2 /8.…”
mentioning
confidence: 99%
“…The XMCD signal is proportional to the atomic magnetic moments in ferromagnetically ordered samples [13]. On the contrary XLD can be due to an orbital or magnetic uniaxial anisotropy (or both), and the magnetic part (XMLD, x-ray magnetic linear dichroism) is sensitive to both FM and AFM ordering [14]. To disentangle the magnetic from the orbital part of XLD we have performed measurements at different temperatures T : above the magnetic ordering temperature only the orbital contribution survives, so in our samples XLD at high T (room T for n = 1 and 200K for n = 5, 8) have orbital character only.…”
mentioning
confidence: 99%