Published June 1, 2023 | Version v1
Dataset Open

Hyperfine interactions in open-shell planar sp2-carbon nanostructures

Description

ORCA data files for the publication:

S. Sengupta, T. Frederiksen, and G. Giedke
Hyperfine interactions in open-shell planar sp2-carbon nanostructures
Phys. Rev. B 107, 224433 (2023) [arXiv:2303.11422]

We investigate hyperfine interaction (HFI) using density-functional theory for several open-shell planar sp2-carbon nanostructures displaying π magnetism. Our prototype structures include both benzenoid ([n]triangulenes and a graphene nanoribbon) as well as nonbenzenoid (indene, fluorene, and indene[2,1-b]fluorene) molecules. Our results obtained with orca indicate that isotropic Fermi contact and anisotropic dipolar terms contribute in comparable strength, rendering the HFI markedly anisotropic. We find that the magnitude of HFI in these molecules can reach more than 100 MHz, thereby opening up the possibility of experimental detection via methods such as electron spin resonance-scanning tunneling microscopy (ESR-STM). Using these results, we obtain empirical models based on π-spin polarizations at carbon sites. These are defined by generic sp2 HFI fit parameters which are derived by matching the computed HFI couplings to π-spin polarizations computed with methods such as Orca, Siesta, or mean-field Hubbard (MFH) models. This approach successfully describes the Fermi contact and dipolar contributions for 13C and 1H nuclei. These fit parameters allow to obtain hyperfine tensors for large systems where existing methodology is not suitable or computationally too expensive. As an example, we show how HFI scales with system size in [n]triangulenes for large n using MFH. We also discuss some implications of HFI for electron-spin decoherence and for coherent nuclear dynamics.

Notes

We acknowledge funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 863098 (FET-Open project "SPRING")

Files

Files (2.0 MB)

Name Size Download all
md5:83b98d098e49888f0059f10f46e4b2d9
2.0 MB Download

Additional details

Related works

Documents
Journal article: 10.1103/PhysRevB.107.224433 (DOI)
Preprint: arXiv:2303.11422 (arXiv)