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  Dynamical quasicondensation in the weakly interacting Fermi-Hubbard model

Březinová, I., Stimpfle, M., Donsa, S., & Rubio, A. (2024). Dynamical quasicondensation in the weakly interacting Fermi-Hubbard model. Physical Review B, 109(17): 174308. doi:10.1103/PhysRevB.109.174308.

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https://doi.org/10.1103/PhysRevB.109.174308 (Publisher version)
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 Creators:
Březinová, I.1, Author
Stimpfle, M.1, Author
Donsa, S.1, Author
Rubio, A.2, 3, Author           
Affiliations:
1Institute for Theoretical Physics, Vienna University of Technology, ou_persistent22              
2Theory Group, Theory Department, Max Planck Institute for the Structure and Dynamics of Matter, Max Planck Society, ou_2266715              
3Center for Computational Quantum Physics (CCQ), Flatiron Institute, ou_persistent22              

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 Abstract: We study dynamical (quasi)condensation in the Fermi-Hubbard model starting from a completely uncorrelated initial state of adjacent doubly occupied sites. We show that upon expansion of the system in one dimension, dynamical (quasi)condensation occurs not only for large interactions via the condensation of doublons, but also for small interactions. The behavior of the system is distinctly different in the two parameter regimes, underlining a different mechanism at work. We address the question of whether the dynamical (quasi)condensation effect persists in the thermodynamic limit. For this purpose, we use the time-dependent two-particle reduced density matrix method, which allows the extension to large system sizes, long propagation times, and two-dimensional (2D) systems. Our results indicate that the effect vanishes in the thermodynamic limit. However, especially in 2D, further investigation beyond numerically tractable system sizes calls for the use of quantum simulators, for which we show that the described effect can be investigated by probing density fluctuations.

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Language(s): eng - English
 Dates: 2024-04-222024-02-202024-04-232024-05-152024-05-01
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: arXiv: 2402.16604
DOI: 10.1103/PhysRevB.109.174308
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Project name : We thank Marie Eder, Salvatore R. Manmana, Florian Libisch, and Joseph Tindall for helpful discussions and hints on literature. I.B. thanks the Simons Foundation for the great hospitality and support during her research visit at the CCQ of the Flatiron Institute, where parts of this research were conducted. The Flatiron Institute is a division of the Simons Foundation. We acknowledge support from the Max Planck–New York City Center for Non-Equilibrium Quantum Phenomena, Cluster of Excellence ‘CUI: Advanced Imaging of Matter'–EXC 2056–project ID. This research was funded by the Austrian Science Fund (FWF) Grant No. P 35539-N, as well as by the FWF Grant No. 10.55776/COE1. Calculations were performed on the Vienna Scientific Cluster (VSC4).
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Title: Physical Review B
  Abbreviation : Phys. Rev. B
Source Genre: Journal
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Publ. Info: Woodbury, NY : American Physical Society
Pages: - Volume / Issue: 109 (17) Sequence Number: 174308 Start / End Page: - Identifier: ISSN: 1098-0121
CoNE: https://pure.mpg.de/cone/journals/resource/954925225008