A modified version of the spin-wave (s.w.) approximation is devised to calculate the zero-point and finite-temperature contributions to the spin correlation functions (SCF) and small wavevector neutron scattering structure factors (SF), longitudinal and transverse to a magnetic field, H, for random magnetic anisotropy (RMA) magnets, in the quasi-saturated regime. All possible origins for spin deviations are considered, and several contributions to the SF have been identified. For the transverse structure factor (TSF), the zero-point static spin deviations due to the RMA give rise to a squared Lorentzian ( L 2). The s.w. scattering off the RMA disorder leads to a new TSF in form of a power L 1 2 . The s.w. scattering leads to a renormalization of the s.w. spectrum and to a negative shift of the magnon gap. The inclusion of 1 S -order operator expansions for magnon interactions yields L 2 as well, although weaker than the above L 2. In all situations the magnetic correlation length (MCL) has been determined for both H=0 and H≠0, identifying several magnetic regimes. The finite-temperature s.w. excitation leads to: a Lorentzian ( L), and to a new TSF of the form L 3 2 , due to RMA s.w. scattering. All of the above results apply without structural correlations (SCs). The presence of SCs keeps the TSF as L 2, although they substantially enlarge the MCL at both H=0 and H≠0. For the longitudinal spin correlation (LSCF), an important result is that, at 0 K, the RMA does not destroy the long-range ferromagnetic order (LRFO) induced by the magnetic field, although the LSCF is weaker than for a good ferromagnet and the longitudinal SF becomes L 2. The LRFO only appears above a threshold magnetic field. The comparison of these results and small-angle neutron scattering observed in rare earth intermetallics is discussed. We should stress that the main aim of this work is to provide a comprehensive microscopic background to the phenomenological, continuous spin and mean field theories for RMA magnets.
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