# Accelerating spin-space sampling by auxiliary spin-dynamics and   temperature-dependent spin-cluster expansion

**Authors:** Ning Wang, Thomas Hammerschmidt, Jutta Rogal, Ralf Drautz

arXiv: 1902.02116 · 2019-03-27

## TL;DR

This paper introduces a Hamiltonian Monte Carlo method utilizing auxiliary spin-dynamics and a temperature-dependent spin-cluster expansion to efficiently sample high-dimensional spin spaces in magnetic material simulations, compatible with electronic-structure methods.

## Contribution

The authors develop a novel sampling framework that combines auxiliary spin-dynamics with a flexible, temperature-dependent spin-cluster expansion, improving efficiency in magnetic simulations.

## Key findings

- Fast warm-up observed in classical Heisenberg model
- Small dynamical critical exponent indicating efficiency
-  Successful application to magnetic phase transition in bcc iron

## Abstract

Atomistic simulations of thermodynamic properties of magnetic materials rely on an accurate modelling of magnetic interactions and an efficient sampling of the high-dimensional spin space. Recent years have seen significant progress with a clear trend from model systems to material specific simulations that are usually based on electronic-structure methods. Here we develop a Hamiltonian Monte Carlo framework that makes use of auxiliary spin-dynamics and an auxiliary effective model, the temperature-dependent spin-cluster expansion, in order to efficiently sample the spin space. Our method does not require a specific form of the model and is suitable for simulations based on electronic-structure methods. We demonstrate fast warm-up and a reasonably small dynamical critical exponent of our sampler for the classical Heisenberg model. We further present an application of our method to the magnetic phase transition in bcc iron using magnetic bond-order potentials.

## Full text

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## Figures

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## References

61 references — full list in the complete paper: https://tomesphere.com/paper/1902.02116/full.md

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Source: https://tomesphere.com/paper/1902.02116