Unrestricted Binary Tree State for the Fermionic Hubbard Model
Abstract
Binary tree states have been introduced as compact correlated pair wave functions that improve upon the antisymmetrized geminal power by adding variational flexibility. Here, we extend the binary tree state to the fermionic half-filled Hubbard model using restricted and unrestricted orbitals. Although the ansatz is seniority zero in its optimized pairing basis, its expansion in the original Hubbard site basis can contain nonzero site- seniority character, while unrestricted orbital optimization provides additional flexibility through independent spin-up and spin-down orbitals. This provides a mechanism for a paired ansatz to describe the singly occupied configurations that dominate the repulsive Hubbard model at large U/t. We find that unrestricted BTS closely approaches optimized DOCI in the repulsive regime, substantially improves upon AGP, and reproduces DOCI density correlations more accurately than pCCD
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BibTeX
@misc{hazaveh2026unrestricted,
title = {{Unrestricted Binary Tree State for the Fermionic Hubbard Model}},
author = {Mahroo Mirabdolhagh Hazaveh and Armin Khamoshi and Fei Gao and Thomas M. Henderson and Gustavo E. Scuseria},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.30399},
eprint = {2610.30399},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.30399},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Unrestricted Binary Tree State for the Fermionic Hubbard Model
AU - Mahroo Mirabdolhagh Hazaveh
AU - Armin Khamoshi
AU - Fei Gao
AU - Thomas M. Henderson
AU - Gustavo E. Scuseria
PY - 2026
DA - 2026/10/21
PB - arXiv
DO - 10.48550/arxiv.2610.30399
UR - https://arxiv.org/abs/2610.30399
AB - Binary tree states have been introduced as compact correlated pair wave functions that improve upon the antisymmetrized geminal power by adding variational flexibility. Here, we extend the binary tree state to the fermionic half-filled Hubbard model using restricted and unrestricted orbitals. Although the ansatz is seniority zero in its optimized pairing basis, its expansion in the original Hubbard site basis can contain nonzero site- seniority character, while unrestricted orbital optimization provides additional flexibility through independent spin-up and spin-down orbitals. This provides a mechanism for a paired ansatz to describe the singly occupied configurations that dominate the repulsive Hubbard model at large U/t. We find that unrestricted BTS closely approaches optimized DOCI in the repulsive regime, substantially improves upon AGP, and reproduces DOCI density correlations more accurately than pCCD
ER -