| Literature DB >> 34031382 |
Ying-Ming Xie1, Xue-Jian Gao1, Xiao Yan Xu2, Cheng-Ping Zhang1, Jin-Xin Hu1, Jason Z Gao1, K T Law3.
Abstract
Recently, it was pointed out that all chiral crystals with spin-orbit coupling (SOC) can be Kramers Weyl semimetals (KWSs) which possess Weyl points pinned at time-reversal invariant momenta. In this work, we show that all achiral non-centrosymmetric materials with SOC can be a new class of topological materials, which we term Kramers nodal line metals (KNLMs). In KNLMs, there are doubly degenerate lines, which we call Kramers nodal lines (KNLs), connecting time-reversal invariant momenta. The KNLs create two types of Fermi surfaces, namely, the spindle torus type and the octdong type. Interestingly, all the electrons on octdong Fermi surfaces are described by two-dimensional massless Dirac Hamiltonians. These materials support quantized optical conductance in thin films. We further show that KNLMs can be regarded as parent states of KWSs. Therefore, we conclude that all non-centrosymmetric metals with SOC are topological, as they can be either KWSs or KNLMs.Entities:
Year: 2021 PMID: 34031382 PMCID: PMC8144424 DOI: 10.1038/s41467-021-22903-9
Source DB: PubMed Journal: Nat Commun ISSN: 2041-1723 Impact factor: 14.919
Fig. 1Schematic plot of Fermi surfaces of KWSs and KNLMs.
a The Fermi surface of a KWS where two Fermi pockets enclose one TRIM. b Spindle torus-type Fermi surface in a KNLM induced by a KNL (the dashed black line). c The Fermi surface of a KWS where each pocket encloses a different TRIM. d Octdong-type Fermi surface in KNLMs induced by a KNL. The gray dots in a–d indicate the position of TRIMs Γ1, Γ2. The touching points of the Fermi surfaces are circled by red dashed lines.
Kramers nodal line metals (KNLMs) with symmorphic space groupsa.
| Type | SG no. | Point group | KNLs | KW points | Material |
|---|---|---|---|---|---|
| Type I | 6, | (Γ, B, Y, A, Z, C, D, E)b | – | CsIO3 | |
| 8, | (Γ, Y, A, M) | – | BiPd2Pb | ||
| 25, | Γ–Z, Y–T, X–U, S–R | – | CdTe, Bi4Te2Br2O9 | ||
| 38, | Γ–Y, T–Z | – | NbS2 | ||
| 42, | Γ–Z, Y–T | – | – | ||
| 99, | Γ–Z, X–R, A–M | – | PbCsCl3 | ||
| 107, | Γ–M, X–X, (N) | – | In2Te3 | ||
| 115, | Γ–Z, M–A, X–R | – | PbF2O | ||
| 156, | Γ–A, (M, L) | – | BiTeI | ||
| 157, | Γ–A, (M, L) | – | Bi2Pt | ||
| 160, | Γ–T, (L, FA) | – | Bi2Te3 | ||
| 174, | Γ–A, (M, L) | – | – | ||
| 183, | Γ–A, M–L | – | AuCN | ||
| 187, | Γ–M, A–L, Γ–A | – | GeI2, TaN | ||
| 189, | Γ–K–M, A–H–L, Γ–A | – | Sn5(BIr3)2 | ||
| 215, | Γ–X, Γ–R, R–M | – | Cu3TaTe4 | ||
| 216, | Γ–L, Γ–X | – | HgSe, HgTe | ||
| 217, | Γ–H | – | TaTl3Se4 | ||
| Type II | 35, | Γ–Z, Y–T | S, R | MnCs2V2Br2O6 | |
| 44, | Γ–X, (S, R) | T | AgNO2 | ||
| 81, | Γ–Z, M–A | X, R | GeSe2 | ||
| 82, | Γ–M | N, X | CdGa2Te4, Cr2AgBiO8 | ||
| 111, | Γ–Z, M–A | X, R | Ag2HgI4 | ||
| 119, | Γ–M, (N) | X | TlAgTe2 | ||
| 121, | Γ–M, X–X | N | Cu3SbS4 |
aHere, we enumerate symmetry allowed KNLs in symmorphic space groups. The definitions of TRIMs follow the conventions given in Bilbao Crystallographic Server[73]. Some of the representative materials hosting KNLs are identified with the assistance of the Materials Project[90] and the Topological Material Database[58].
bThe TRIMs in the parentheses are connected by the KNLs that are not along the high symmetry lines, such as (Γ, A), (Y, M) in SG no. 8 (Pm) and (M, L) in SG no. 156 (P3m1).
Fig. 2Representative materials with KNLs.
a–j The crystal structure, the first Brillouin zone, and KNLs of BiTeI (SG no. 156, P3m1), Cr2AgBiO8 (SG no. 82, ), and BiPd2Pb (SG no. 8, Cm). c, g The band structures of BiTeI and Cr2AgBiO8, respectively, where the KNLs are highlighted as blue lines, and the crossing points within the red circles of f are KW points. These KNLs are also marked out by solid blue lines in the 3D first Brillouin zone. d, j The DFT-calculated energy difference of two selected SOC-split bands ∣E1(k) − E2(k)∣ (in units of eV) on a mirror-invariant k plane for BiTeI and BiPd2Pb, respectively. The dark green lines that connect two TRIMs (dashed circles) are KNLs on this mirror plane.
Fig. 3Spindle torus and octdong Fermi surfaces.
a The Fermi surface of BiTeI with Fermi energy EF = 0.2 eV, which cuts through the KNL Γ–A. The inner (orange) and outer (purple) Fermi pockets (FP) together form a spindle torus. The energy dispersion at a fixed k indicated by the dashed line is shown in b. b The Rashba-like energy dispersion for a fixed k. c The Fermi surface of Bi4Te2Br2O9 (SG no. 25, Pmm2) with Fermi energy EF = 0.05 eV, which cuts through the KNL Γ–Z. The labeled hole and the electron Fermi pockets together form an octdong-type Fermi surface. d The Fermi surface from the two-band tight-binding model with m = 0.05t, m = 0.05t, m = 0.5t, v = t, v = t, EF = 0, and t = 1 as the unit of the hybridization energy. The positions of TRIMs depicted are all connected by four KNLs in the k-direction. e The energy dispersion for a fixed k = 0 (purple) and k = π (red) in d. f Schematic plot of optical excitations that contribute to the optical conductivity for the hole-type (electron-type) Dirac fermions with onset frequency ω1 (ω2). The horizontal dashed line denotes the position of Fermi energy. g The optical conductivity σ (left axis) and estimated optical conductivity NDσ0/4 (right axis) versus frequency ω for a three-layer slab, where the number of Dirac points with θ as the Heaviside step function, n as band index, and Γ labeling four TRIMs. The inset figure in g shows the band structure of this trilayer slab. h The bulk optical conductivity for the model material with octdong Fermi surface at EF = 0, 0.2t with η = 0.002t and temperature T = 0.01t. Here, cm−1 with Å and a as the lattice constant. i The bulk optical conductivity for Bi4Te2Br2O9 with η = 1 meV and temperature T = 10 K. The slight deviation from linear dependence (red dashed line) for Bi4Te2Br2O9 is due to the presence of the extra trivial pockets (blue pockets in c).
Fig. 4Strain-induced Kramers Weyl fermions.
a Schematic plot of a KNL (solid line) carrying Berry flux π. b The Berry flux emerges from TRIMs when the degeneracy of the KNL is lifted. The total flux through a sphere (in green) that enclose the TRIM is 2π. c–e The splitting along Γ–A with 1%, 3%, and 5% strain strengths, respectively. f The chiral charge versus light frequency ω, calculated at four different strain strengths: no strain (in black), 1% strain (in blue), 3% strain (in red), and 5% strain (in purple).
The k ⋅ p Hamiltonians at TRIMs with non-centrosymmetric achiral little groups.
| Point group | IR coreps[ | k ⋅ p Hamiltonian | Directions of KNLs | |
|---|---|---|---|---|
| 2 | ∈ | |||
| 2 | ||||
| 2 | ( | |||
| 2 | ||||
| 2 | ||||
| 2 | ∈ | |||
| 2 | ||||
| 2 | ||||
| 2 | ∈ | |||
| 2 | ||||
| 2 | ||||
| 2 | ||||
| 2 | ||||
| 2 | ||||
| 4 |
The point group symmetry, the corresponding abstract group (AG) symbols together with time-reversal invariant irreducible corepresentations (IR coreps) are listed. The general form of the Hamiltonians and the direction of the KNLs are listed. In general, the KNLs lie along some high symmetry directions such as the z-direction. For points groups C1v, C3, and C3, the KNLs lie within the mirror planes that is denoted as ∈ m. Here, k± = k ± ik, the Pauli matrices σ operate on the spinor basis with J = ±1/2 or J = ±3/2, and are the angular momentum operators with J = 3/2.