Structure of the Hilbert-space of the infinite-dimensional Hubbard model
C. Gros, W. Wenzel

TL;DR
This paper develops an iterative method to explicitly construct the symmetry-adapted subspace of the ground state in the infinite-dimensional Hubbard model, connecting it to impurity problems and providing highly accurate estimates.
Contribution
It introduces a novel iterative procedure based on symmetrized transition operators for analyzing the Hubbard model's ground state in infinite dimensions.
Findings
Constructed the nontrivial symmetry-adapted subspace explicitly.
Linked the transition operators to the impurity model mapping.
Achieved estimates for the Hubbard model with 0.1% accuracy.
Abstract
An iterative procedure for the explicit construction of the nontrivial subspace of all symmetry-adapted configurations with non-zero weight in the ground-state of the infinite-dimensional Hubbard model is developed on the basis of a symmetrized representation of the transition operators on a sequence of Bethe-Lattices of finite depth. The relation ship between these operators and the well known mapping of the infinite-dimensional Hubbard model onto an effective impurity problem coupled to a (self-consistent) bath on non-interacting electrons is given. As an application we calculate the properties of various Hubbard stars and give estimates for the half-filled Hubbard model with up to 0.1% accuracy.
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