# Vacancy in graphene: insight on magnetic properties from theoretical   modeling

**Authors:** A. M. Valencia, M. J. Caldas

arXiv: 1704.01906 · 2017-10-11

## TL;DR

This study uses advanced ab initio methods to clarify the magnetic properties of vacancies in graphene, demonstrating the importance of exchange-correlation effects and revealing potential for spin interactions in defect arrays.

## Contribution

It provides a comprehensive theoretical analysis with multiple simulation protocols and DFT functionals, resolving previous discrepancies in magnetic moment predictions for graphene vacancies.

## Key findings

- Inclusion of exchange-correlation is crucial for accurate magnetic moment prediction.
- Predicted magnetic moment for a single vacancy is 2 μB.
- Periodic vacancy arrays may exhibit interesting spin interactions.

## Abstract

Magnetic properties of a single vacancy in graphene is a relevant and still unsolved problem. The experimental results point to a clearly detectable magnetic defect state at the Fermi energy, while several calculations based on density functional theory (DFT) yield widely varying results for the magnetic moment, in the range of $\mu=1.04-2.0$ $\mu_{B}$. We present a multi-tool \textit{ab initio} theoretical study of the same defect, using two simulation protocols for a defect in a crystal (cluster and periodic boundary conditions) and different DFT functionals - bare and hybrid DFT, mixing a fraction of exact Hartree-Fock exchange (XC). Our main conclusions are two-fold: First, we find that due to the $\pi$-character of the Fermi-energy states of graphene, inclusion of XC is crucial and for a single isolated vacancy we can predict an integer magnetic moment $\mu=2\mu_{B}$. Second, we find that due to the specific symmetry of the graphene lattice, periodic arrays of single vacancies may provide interesting diffuse spin-spin interactions.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1704.01906/full.md

## References

35 references — full list in the complete paper: https://tomesphere.com/paper/1704.01906/full.md

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Source: https://tomesphere.com/paper/1704.01906