Spin Accumulation and Longitudinal Spin Diffusion of Magnets
Abstract
We extend to the longitudinal component of the magnetization the spintronics idea that a magnet near equilibrium can be described by two magnetic variables. One is the usual magnetization M. The other is the non-equilibrium quantity m, called the spin accumulation, by which the non-equilibrium spin current can be transported. M represents a correlated distribution of a very large number of degrees of freedom, as expressed in some equilibrium distribution function for the excitations; we therefore forbid M to diffuse, but we permit M to decay. On the other hand, we permit m, due to spin excitations, to both diffuse and decay. For this physical picture, diffusion from a given region occurs by decay of M to m, then by diffusion of m, and finally by decay of m to M in another region. This somewhat slows down the diffusion process. Restricting ourselves to the longitudinal variables M and m with equilibrium properties Meq=M0+MH and meq=0, we argue that the effective energy density must include a new, thermodynamically required exchange constant λM=-1/M. We then develop the macroscopic equations by applying Onsager's irreversible thermodynamics, and use the resulting equations to study the space and time response. At fixed real frequency ω there is, as usual, a single pair of complex wavevectors k but with an unusual dependence on ω. At fixed real wavevector, there are two decay constants, as opposed to one in the usual case. Extending the idea that non-equilibrium diffusion in other ordered systems involves a non-equilibrium quantity, this work suggests that in a superconductor the order parameter can decay but not diffuse, but a non-equilibrium gap-like δ, due to pair excitations, can both decay and diffuse.
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