# Pressure-dependent Semiconductor to Semimetal and Lifshitz transitions   in 2H-MoTe$_2$: Raman and First-principles studies

**Authors:** Achintya Bera, Anjali Singh, D V S Muthu, U V Waghmare, A K Sood

arXiv: 1702.00357 · 2017-03-08

## TL;DR

This study combines Raman spectroscopy and first-principles calculations to investigate pressure-induced phase transitions in 2H-MoTe$_2$, revealing a semiconductor to semimetal transition and a Lifshitz transition with changes in Fermi surface topology.

## Contribution

It provides the first detailed analysis of pressure-induced electronic and structural transitions in 2H-MoTe$_2$ using combined experimental and theoretical approaches.

## Key findings

- Identified phase transitions at ~6 GPa and ~16.5 GPa.
- Demonstrated a semiconductor to semimetal transition at 6 GPa.
- Revealed a Lifshitz transition at ~20 GPa with Fermi surface topology change.

## Abstract

High pressure Raman spectroscopy of bulk 2H-MoTe$_2$ upto $\sim$ 29 GPa is shown to reveal two phase transitions (at $\sim$ 6 and 16.5 GPa), which are analyzed using first-principles density functional theoretical calculations. The transition at 6 GPa is marked by changes in the pressure coefficients of A$_{1g}$ and E$^{1}_{2g}$ Raman mode frequencies as well as in their relative intensity. Our calculations show that this is an isostructural semiconductor to a semimetal transition. The transition at $\sim$ 16.5 GPa is identified with the changes in linewidths of the Raman modes as well as in the pressure coefficients of their frequencies. Our theoretical analysis clearly shows that the structure remains the same upto 30 GPa. However, the topology of the Fermi-surface evolves as a function of pressure, and abrupt appearance of electron and hole pockets at P $\sim$ 20 GPa marks a Lifshitz transition.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1702.00357/full.md

## References

49 references — full list in the complete paper: https://tomesphere.com/paper/1702.00357/full.md

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Source: https://tomesphere.com/paper/1702.00357