English

Charge density wave and spin $1/2$ insulating state in single layer 1T-NbS$_2$

Strongly Correlated Electrons 2019-05-27 v1

Abstract

In bulk samples and few layer flakes, the transition metal dichalcogenides NbS2_2 and NbSe2_2 assume the H polytype structure with trigonal prismatic coordination of the Nb atom. Recently, however, single and few layers of 1T-NbSe2_2 with octahedral coordination around the transition metal ion were synthesized. Motivated by these experiments and by using first-principles calculations, we investigate the structural, electronic and dynamical properties of single layer 1T-NbS2_2. We find that single-layer 1T-NbS2_2 undergoes a 13×13\sqrt{13}\times\sqrt{13} star-of-David charge density wave. Within the generalized gradient approximation, the weak interaction between the stars leads to an ultraflat band at the Fermi level isolated from all other bands. The spin-polarized generalized gradient approximation stabilizes a total spin 1/21/2 magnetic state with opening of a 0.150.15 eV band gap and a 0.21μB0.21\mu_B magnetic moment localized on the central Nb in the star. Within GGA+U, the magnetic moment on the central Nb is enhanced to 0.41μB0.41\mu_{B} and a larger gap occurs. Most important, this approximation gives a small energy difference between the 1T and 1H polytypes (only +0.5+0.5 mRy/Nb), suggesting that the 1T-polytype can be synthesized in a similar way as done for single layer 1T-NbSe2_2. Finally we compute first and second nearest neighbors magnetic inter-star exchange interactions finding J1J_1=9.5~K and J2J_2=0.4~K ferromagnetic coupling constants.

Keywords

Cite

@article{arxiv.1902.00234,
  title  = {Charge density wave and spin $1/2$ insulating state in single layer 1T-NbS$_2$},
  author = {Cesare Tresca and Matteo Calandra},
  journal= {arXiv preprint arXiv:1902.00234},
  year   = {2019}
}
R2 v1 2026-06-23T07:29:09.295Z