Longitudinal integration measure in classical spin space and its application to first-principle based simulations of the high temperature magnetism of Fe and Ni
Sergii Khmelevskyi

TL;DR
This paper derives a new integration measure for classical spin space that improves the modeling of temperature-dependent magnetism in Fe and Ni, incorporating longitudinal spin fluctuations from first-principles calculations.
Contribution
It introduces a fundamental derivation of the integration measure in classical spin space considering quantum limits, enhancing the accuracy of finite-temperature magnetic simulations.
Findings
The derived measure accounts for the proportionality of quantum states to spin amplitude.
Application to Fe and Ni yields more accurate Curie temperature predictions.
Comparison shows the new measure outperforms previous scalar and vector measures.
Abstract
The classical Heisenberg type spin Hamiltonian is widely used for simulations of finite temperature properties of magnetic metals often using parameters derived from first principles calculations. In itinerant electron systems, however, the atomic magnetic moments vary their amplitude with temperature and the spin Hamiltonian should thus be extended to incorporate the effects of longitudinal spin fluctuations (LSF). Although the simple phenomenological spin Hamiltonians describing LSF can be efficiently parameterized in the framework of the constrained Local Spin Density Approximation (LSDA) and its extensions, the fundamental problem concerning the integration in classical spin space remains. It is generally unknown how to integrate over the spin amplitude. Two intuitive choices of integration measure have been used up to date; the Murata-Doniach scalar measure and the simple three…
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