Excitation Spectrum and Superfluid Gap of an Ultracold Fermi Gas
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A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä
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Date
2022-03-11
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en
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7
1-7
1-7
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Physical Review Letters, Volume 128, issue 10
Abstract
Ultracold atomic gases are a powerful tool to experimentally study strongly correlated quantum many-body systems. In particular, ultracold Fermi gases with tunable interactions have allowed to realize the famous BEC-BCS crossover from a Bose-Einstein condensate (BEC) of molecules to a Bardeen-Cooper-Schrieffer (BCS) superfluid of weakly bound Cooper pairs. However, large parts of the excitation spectrum of fermionic superfluids in the BEC-BCS crossover are still unexplored. In this work, we use Bragg spectroscopy to measure the full momentum-resolved low-energy excitation spectrum of strongly interacting ultracold Fermi gases. This enables us to directly observe the smooth transformation from a bosonic to a fermionic superfluid that takes place in the BEC-BCS crossover. We also use our spectra to determine the evolution of the superfluid gap and find excellent agreement with previous experiments and self-consistent T-matrix calculations both in the BEC and crossover regime. However, toward the BCS regime a calculation that includes the effects of particle-hole correlations shows better agreement with our data.Description
Funding Information: We thank R. Haussmann, L. Mathey, C. Vale, and W. Zwerger for helpful discussions and R. Haussmann, W. Zwerger, and P. Pieri for providing us with the results of their calculations. This work is supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) in the framework of SFB-925, Project No. 170620586, and the excellence cluster Advanced Imaging of Matter, EXC 2056, Project ID No. 390715994. Publisher Copyright: © 2022 American Physical Society.
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Biss, H, Sobirey, L, Luick, N, Bohlen, M, Kinnunen, J J, Bruun, G M, Lompe, T & Moritz, H 2022, ' Excitation Spectrum and Superfluid Gap of an Ultracold Fermi Gas ', Physical Review Letters, vol. 128, no. 10, 100401, pp. 1-7 . https://doi.org/10.1103/PhysRevLett.128.100401