Abstract

Spin defects in wide-bandgap semiconductors provide a promising platform to create qubits for quantum technologies. Their synthesis, however, presents considerable challenges, and the mechanisms responsible for their generation or annihilation are poorly understood. Here, we elucidate spin defect formation processes in a binary crystal for a key qubit candidate—the divacancy complex (VV) in silicon carbide (SiC). Using atomistic models, enhanced sampling simulations, and density functional theory calculations, we find that VV formation is a thermally activated process that competes with the conversion of silicon (VSi) to carbon monovacancies (VC), and that VV reorientation can occur without dissociation. We also find that increasing the concentration of VSi relative to VC favors the formation of divacancies. Moreover, we identify pathways to create spin defects consisting of antisite-double vacancy complexes and determine their electronic properties. The detailed view of the mechanisms that underpin the formation and dynamics of spin defects presented here may facilitate the realization of qubits in an industrially relevant material.

Highlights

  • Spin defects in wide-bandgap semiconductors provide a promising platform to create qubits for quantum technologies

  • Our results reveal that a divacancy is a thermodynamically stable state, while VSi represents a kinetically trapped state that readily transforms into an intermediate carbon antisite-vacancy (CSiVC) defect

  • Before conducting firstprinciples molecular dynamics (FPMD) simulations coupled to enhanced sampling techniques, we explored the dynamics of vacancy defects in silicon carbide (SiC) using an empirical force field[39], based on a widely used Tersoff-type bond-order formalism[40,41]

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Summary

Introduction

Spin defects in wide-bandgap semiconductors provide a promising platform to create qubits for quantum technologies. The optical and electronic properties of spin defects in SiC, including the silicon vacancy (VSi)[10,11], NV centers[12,13], and carbon antisite-vacancy complexes (CSiVC)[14], have been characterized using a variety of techniques. These include densityfunctional theory (DFT) calculations, electron paramagnetic resonance spectroscopy (EPR), deep-level transient spectroscopy (DLTS), and photoluminescence spectroscopy (PL)[15,16,17,18,19,20,21]. Recent kinetic Monte Carlo simulations considered the dynamics of vacancies in SiC34, but they did so by invoking a priori mechanisms for defect mobilization

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