Our system is currently under heavy load due to increased usage. We're actively working on upgrades to improve performance. Thank you for your patience.
2022
DOI: 10.1103/physrevmaterials.6.014005
|View full text |Cite
|
Sign up to set email alerts
|

Thermodynamics of carbon point defects in hexagonal boron nitride

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

2
24
0

Year Published

2022
2022
2024
2024

Publication Types

Select...
7

Relationship

0
7

Authors

Journals

citations
Cited by 25 publications
(33 citation statements)
references
References 50 publications
2
24
0
Order By: Relevance
“…After Bourrellier et al. reported the first quantum emission at near 300 nm (4.09 eV) using CL (Figure 9b), theoretical calculations also revealed that C B C N , [ 132 ] C B , [ 133 ] and other carbon‐related defects [ 131,134 ] are origins of the single‐photon emissions near 300 nm (≈4.1 eV). The wavelengths of single‐photon emissions from exfoliated h‐BN (flake) or grown h‐BN with corresponding proposed defect origins are summarized in Figure 9 and Table 3 .…”
Section: H‐bn For Next‐generation Photonicsmentioning
confidence: 97%
“…After Bourrellier et al. reported the first quantum emission at near 300 nm (4.09 eV) using CL (Figure 9b), theoretical calculations also revealed that C B C N , [ 132 ] C B , [ 133 ] and other carbon‐related defects [ 131,134 ] are origins of the single‐photon emissions near 300 nm (≈4.1 eV). The wavelengths of single‐photon emissions from exfoliated h‐BN (flake) or grown h‐BN with corresponding proposed defect origins are summarized in Figure 9 and Table 3 .…”
Section: H‐bn For Next‐generation Photonicsmentioning
confidence: 97%
“…Carbon interstitials have been excluded due to their high formation energies and low diffusion barriers . Nonetheless, the number of possibilities is large, as it includes numerous nearest-neighbor and next-nearest-neighbor permutations of the point defects, as well as larger clusters. , Many of these defects are thermodynamically stable under various growth conditions, can occur in multiple charge states, and have calculated ZPL energies that correlate with SPEs observed experimentally (Figure ). The resulting diversity makes it challenging to assign conclusively the simulated atomic structures to SPEs based on ZPL wavelengths observed in experiments .…”
Section: Atomic Structurementioning
confidence: 99%
“…Overall, none of the above defect structure assignments are conclusive, despite an emerging consensus about the significant role of carbon in hBN SPEs. For example, even the simplest monatomic substitutional carbon defects (C B and C N , Figure ) have been both proposed , and dismissed as potential SPEs in recent computational studies. At the opposite extreme of clusters, various complexes other than the carbon dimers/trimers have calculated optical properties that are consistent with UV and visible SPEs.…”
Section: Atomic Structurementioning
confidence: 99%
“…Theoretical calculations found the formation energy of the C B C N defect to be about 2 eV (ref. 25, 26 and 30) (the energy is positive since the original B B N N pair has a lower energy than the C B C N pair) and it is independent of nitrogen flux.…”
Section: Resultsmentioning
confidence: 99%