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Measurement and modeling of polarized specular neutron reflectivity in large magnetic fields

机译:大磁场中极化镜面中子反射率的测量和建模

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摘要

The presence of a large applied magnetic field removes the degeneracy of the vacuum energy states for spin-up and spin-down neutrons. For polarized neutron reflectometry, this must be included in the reference potential energy of the Schrödinger equation that is used to calculate the expected scattering from a magnetic layered structure. For samples with magnetization that is purely parallel or antiparallel to the applied field which defines the quantization axis, there is no mixing of the spin states (no spin-flip scattering) and so this additional potential is constant throughout the scattering region. When there is non-collinear magnetization in the sample, however, there will be significant scattering from one spin state into the other, and the reference potentials will differ between the incoming and outgoing wavefunctions, changing the angle and intensities of the scattering. The theory of the scattering and recommended experimental practices for this type of measurement are presented, as well as an example measurement.
机译:大施加磁场的存在消除了旋转中子和旋转中子的真空能态的退化。对于极化中子反射法,必须将其包括在Schrödinger方程的参考势能中,该参考势能用于计算磁性层状结构的预期散射。对于具有与定义量化轴的施加磁场完全平行或反平行的磁化强度的样品,自旋状态没有混合(无自旋翻转散射),因此,此附加电势在整个散射区域中都是恒定的。但是,当样品中存在非共线磁化强度时,从一种自旋态到另一种自旋态会产生明显的散射,并且入射电势和出射波函数之间的参考电势会有所不同,从而改变了散射的角度和强度。提出了散射理论和推荐的用于此类测量的实验方法,并提供了示例测量。

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