Abstract
We clarify universal critical properties of delocalization-localization transitions in three-dimensional unitary and orthogonal classes with particle-hole and/or chiral symmetries (classes AIII, BDI, D, C, and CI). We first introduce tight-binding models on cubic lattice that belong to these five nonstandard symmetry classes, respectively. Unlike the Bogoliubov-de Gennes Hamiltonian for superconductors, all the five models have finite areas of Fermi surfaces in the momentum space in the clean limit. Thereby, the scaling theory of the Anderson transition guarantees the presence of the delocalization-localization transitions at finite disorder strength in these models. Based on this expectation, we carry out extensive transfer matrix calculations of the Lyapunov exponents for zero-energy eigenstates of the disordered tight-binding models with quasi-one-dimensional geometry. Near the Anderson transition point, the correlation length diverges with a universal critical exponent $\ensuremath{\nu}$. Using finite-size scaling analysis of the localization length, we determine the critical exponent of the transitions and scaling function of the (normalized) localization length in the three nonstandard unitary symmetry classes: ${\ensuremath{\nu}}_{\text{AIII}}=1.06\ifmmode\pm\else\textpm\fi{}0.02$, ${\ensuremath{\nu}}_{\text{D}}=0.87\ifmmode\pm\else\textpm\fi{}0.03$, and ${\ensuremath{\nu}}_{\text{C}}=0.996\ifmmode\pm\else\textpm\fi{}0.012$. Our result of the class C is consistent with a previous study of classical network model [M. Ortu\~no et al., Phys. Rev. Lett. 102, 070603 (2009)]. The critical exponents of the two nonstandard orthogonal classes are estimated as ${\ensuremath{\nu}}_{\text{CI}}=1.17\ifmmode\pm\else\textpm\fi{}0.02$ and ${\ensuremath{\nu}}_{\text{BDI}}=1.12\ifmmode\pm\else\textpm\fi{}0.06$. Our result of the class CI is consistent with another previous study of a lattice model, while the exponent of the class BDI is at variance with the previous evaluation of nodal Dirac ring model [X. Luo et al., Phys. Rev. B 101, 020202(R) (2020)].
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.