# Understanding the temperature and pressure dependent electronic   properties of FeSi: DFT+DMFT study

**Authors:** Paromita Dutta, Sudhir K. Pandey

arXiv: 1907.10566 · 2021-02-03

## TL;DR

This study uses DFT+DMFT and KKR-CPA methods to analyze how pressure and temperature influence the electronic and magnetic properties of FeSi and Fe-rich FeSi, revealing pressure-induced band-gap widening, impurity states, and magnetic moment reduction.

## Contribution

It provides a comprehensive theoretical analysis of pressure and temperature effects on FeSi's electronic structure using advanced computational methods, highlighting impurity states and magnetic behavior.

## Key findings

- Band-gap widens with pressure, shifting insulator-metal transition to higher temperatures.
- Impurity states in the gap suggest half-metallic behavior in Fe-rich samples.
- Magnetic moments decrease with increasing pressure, aligning with experimental observations.

## Abstract

Electronic structures of FeSi and Fe$_{1.02}$Si$_{0.98}$ under pressure (achieved through volume compression) have been investigated by using DFT+DMFT and KKR-CPA methods, respectively. The widening of band-gap with increasing pressure suggests that the experimentally observed insulator to metal transition temperature should shift towards the higher temperature for FeSi. KKR-CPA calculations have shown the presence of impurity states in the gapped region which predicts the half-metallic nature. The closure of gap (in one spin channel) with pressure increment appears to be responsible for experimentally observed semiconductor to metal transition in Fe excess samples at a temperature below 50 K. Magnetic moments at Fe excess sites are found to be decreasing with increasing pressure from 2.4 $\mu_B$ per Fe atom (612 Bohr$^3$) to 1.2 $\mu_B$ per Fe atom (507 Bohr$^3$). Moreover, for FeSi the calculated local spin susceptibility has shown decreasing behavior with pressure rise similar to experimental result.

## Full text

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## Figures

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## References

68 references — full list in the complete paper: https://tomesphere.com/paper/1907.10566/full.md

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Source: https://tomesphere.com/paper/1907.10566