Non-abelian symmetries in tensor networks: a quantum symmetry space approach

TL;DR

This paper introduces a comprehensive framework called QSpace for implementing non-abelian symmetries in tensor networks, enhancing computational efficiency in methods like NRG and DMRG, with detailed applications to a spin-3/2 three-channel Anderson impurity model.

Contribution

The paper develops a unifying tensor-representation for non-abelian symmetry spaces, enabling efficient numerical algorithms for tensor networks with complex symmetries.

Findings

QSpace improves numerical efficiency in tensor network calculations.

Application to a spin-3/2 three-channel Anderson model demonstrates effectiveness.

Comparison of different symmetry scenarios shows significant computational gains.

Abstract

A general framework for non-abelian symmetries is presented for matrix-product and tensor-network states in the presence of orthonormal local as well as effective basis sets. The two crucial ingredients, the Clebsch-Gordan algebra for multiplet spaces as well as the Wigner-Eckart theorem for operators, are accounted for in a natural, well-organized, and computationally straightforward way. The unifying tensor-representation for quantum symmetry spaces, dubbed QSpace, is particularly suitable to deal with standard renormalization group algorithms such as the numerical renormalization group (NRG), the density matrix renormalization group (DMRG), or also more general tensor networks such as the multi-scale entanglement renormalization ansatz (MERA). In this paper, the focus is on the application of the non-abelian framework within the NRG. A detailed analysis is given for a fully screened spin-3/2 three-channel Anderson impurity model in the presence of conservation of total spin, particle-hole symmetry, and SU(3) channel symmetry. The same system is analyzed using several alternative symmetry scenarios. This includes the more traditional symmetry setting SU(2)^4, the larger symmetry SU(2)*U(1)*SU(3), and their much larger enveloping symplectic symmetry SU(2)*Sp(6). These are compared in detail, including their respective dramatic gain in numerical efficiency. In the appendix, finally, an extensive introduction to non-abelian symmetries is given for practical applications, together with simple self-contained numerical procedures to obtain Clebsch-Gordan coefficients and irreducible operators sets. The resulting QSpace tensors can deal with any set of abelian symmetries together with arbitrary non-abelian symmetries with compact, i.e. finite-dimensional, semi-simple Lie algebras.