# Single spin resonance in a van der Waals embedded paramagnetic defect

**Authors:** Nathan Chejanovsky, Amlan Mukherjee, Youngwook Kim, Andrej Denisenko,, Amit Finkler, Takashi Taniguchi, Kenji Watanabe, Durga Bhaktavatsala Rao, Dasari, Jurgen H. Smet, J\"org Wrachtrup

arXiv: 1906.05903 · 2021-06-14

## TL;DR

This paper reports the discovery of a single paramagnetic spin defect in hexagonal boron nitride with optical magnetic resonance, revealing its electronic structure, spin properties, and potential for quantum applications.

## Contribution

It introduces a new single spin defect in h-BN with detailed optical and magnetic characterization, advancing quantum defect research in 2D materials.

## Key findings

- Isotropic g factor close to 2
- Zero field splitting ≤ 4 MHz
- Spin relaxation time around 17 μs

## Abstract

Spins constitute a group of quantum objects forming a key resource in modern quantum technology. Two-dimensional (2D) van der Waals materials are of fundamental interest for studying nanoscale magnetic phenomena. However, isolating singular paramagnetic spins in 2D systems is challenging. We report here on a quantum emitting source embedded within hexgonal boron nitride (h-BN) exhibiting optical magnetic resonance (ODMR). We extract an isotropic $g$ factor close to 2 and derive an upper bound for a zero field splitting (ZFS) ($\leq$ 4 MHz). Photoluminescence (PL) behavior under temperature cycling using different excitations is presented, assigning probable zero phonon lines (ZPLs) / phonon side band (PSBs) to emission peaks, compatible with h-BN's phonon density of states, indicating their intrinsic nature. Narrow and inhomogeneous broadened ODMR lines differ significantly from monoatomic vacancy defect lines known in literature. We derive a hyperfine coupling of around 10 MHz. Its angular dependence indicates an unpaired electron in an out-of-plane $\pi$-orbital, probably originating from an additional substitutional carbon impurity or other low mass atom. We determine the spin relaxation time $T_1$ to be around 17 $\mu$s.

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Source: https://tomesphere.com/paper/1906.05903