Fork Tensor-Product States: Efficient Multiorbital Real-Time DMFT Solver

We present a tensor network especially suited for multi-orbital Anderson impurity models and as an impurity solver for multi-orbital dynamical mean-field theory (DMFT). The solver works directly on the real-frequency axis and yields high spectral resolution at all frequencies. We use a large number...

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Main Authors: Daniel Bauernfeind, Manuel Zingl, Robert Triebl, Markus Aichhorn, Hans Gerd Evertz
Format: Article
Language:English
Published: American Physical Society 2017-07-01
Series:Physical Review X
Online Access:http://doi.org/10.1103/PhysRevX.7.031013
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spelling doaj-1af0b42bf6d14c2dba4c561b74a50b502020-11-24T21:57:53ZengAmerican Physical SocietyPhysical Review X2160-33082017-07-017303101310.1103/PhysRevX.7.031013Fork Tensor-Product States: Efficient Multiorbital Real-Time DMFT SolverDaniel BauernfeindManuel ZinglRobert TrieblMarkus AichhornHans Gerd EvertzWe present a tensor network especially suited for multi-orbital Anderson impurity models and as an impurity solver for multi-orbital dynamical mean-field theory (DMFT). The solver works directly on the real-frequency axis and yields high spectral resolution at all frequencies. We use a large number (O(100)) of bath sites and therefore achieve an accurate representation of the bath. The solver can treat full rotationally invariant interactions with reasonable numerical effort. We show the efficiency and accuracy of the method by a benchmark for the three-orbital test-bed material SrVO_{3}. There we observe multiplet structures in the high-energy spectrum, which are almost impossible to resolve by other multi-orbital methods. The resulting structure of the Hubbard bands can be described as a broadened atomic spectrum with rescaled interaction parameters. Additional features emerge when U is increased. Finally, we show that our solver can be applied even to models with five orbitals. This impurity solver offers a new route to the calculation of precise real-frequency spectral functions of correlated materials.http://doi.org/10.1103/PhysRevX.7.031013
collection DOAJ
language English
format Article
sources DOAJ
author Daniel Bauernfeind
Manuel Zingl
Robert Triebl
Markus Aichhorn
Hans Gerd Evertz
spellingShingle Daniel Bauernfeind
Manuel Zingl
Robert Triebl
Markus Aichhorn
Hans Gerd Evertz
Fork Tensor-Product States: Efficient Multiorbital Real-Time DMFT Solver
Physical Review X
author_facet Daniel Bauernfeind
Manuel Zingl
Robert Triebl
Markus Aichhorn
Hans Gerd Evertz
author_sort Daniel Bauernfeind
title Fork Tensor-Product States: Efficient Multiorbital Real-Time DMFT Solver
title_short Fork Tensor-Product States: Efficient Multiorbital Real-Time DMFT Solver
title_full Fork Tensor-Product States: Efficient Multiorbital Real-Time DMFT Solver
title_fullStr Fork Tensor-Product States: Efficient Multiorbital Real-Time DMFT Solver
title_full_unstemmed Fork Tensor-Product States: Efficient Multiorbital Real-Time DMFT Solver
title_sort fork tensor-product states: efficient multiorbital real-time dmft solver
publisher American Physical Society
series Physical Review X
issn 2160-3308
publishDate 2017-07-01
description We present a tensor network especially suited for multi-orbital Anderson impurity models and as an impurity solver for multi-orbital dynamical mean-field theory (DMFT). The solver works directly on the real-frequency axis and yields high spectral resolution at all frequencies. We use a large number (O(100)) of bath sites and therefore achieve an accurate representation of the bath. The solver can treat full rotationally invariant interactions with reasonable numerical effort. We show the efficiency and accuracy of the method by a benchmark for the three-orbital test-bed material SrVO_{3}. There we observe multiplet structures in the high-energy spectrum, which are almost impossible to resolve by other multi-orbital methods. The resulting structure of the Hubbard bands can be described as a broadened atomic spectrum with rescaled interaction parameters. Additional features emerge when U is increased. Finally, we show that our solver can be applied even to models with five orbitals. This impurity solver offers a new route to the calculation of precise real-frequency spectral functions of correlated materials.
url http://doi.org/10.1103/PhysRevX.7.031013
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