Anomalous loss behavior in a single-component Fermi gas close to a p-wave Feshbach resonance

We theoretically investigate three-body losses in a single-component Fermi gas near a p-wave Feshbach resonance in the interacting, nonunitary regime. We extend the cascade model introduced by Waseem et al. [M. Waseem, J. Yoshida, T. Saito, and T. Mukaiyama, Phys. Rev. A 99, 052704 (2019)] to descri...

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Hauptverfasser: Welz, Kilian (VerfasserIn) , Gerken, Manuel (VerfasserIn) , Zhu, B. (VerfasserIn) , Lippi, Eleonora (VerfasserIn) , Rautenberg, Michael (VerfasserIn) , Chomaz, Lauriane (VerfasserIn) , Weidemüller, Matthias (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 11 May 2023
In: Physical review
Year: 2023, Jahrgang: 107, Heft: 5, Pages: 1-8
ISSN:2469-9934
DOI:10.1103/PhysRevA.107.053310
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1103/PhysRevA.107.053310
Verlag, lizenzpflichtig, Volltext: https://link.aps.org/doi/10.1103/PhysRevA.107.053310
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Verfasserangaben:K. Welz, M. Gerken, B. Zhu, E. Lippi, M. Rautenberg, L. Chomaz, and M. Weidemüller
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Zusammenfassung:We theoretically investigate three-body losses in a single-component Fermi gas near a p-wave Feshbach resonance in the interacting, nonunitary regime. We extend the cascade model introduced by Waseem et al. [M. Waseem, J. Yoshida, T. Saito, and T. Mukaiyama, Phys. Rev. A 99, 052704 (2019)] to describe the elastic and inelastic collision processes. We find that the loss behavior exhibits a n3 and an anomalous n2 density dependence for a ratio of elastic-to-inelastic collision rate larger and smaller than 1, respectively. The corresponding evolutions of the energy distribution show collisional cooling or evolution toward low-energetic nonthermalized steady states, respectively. These findings are particularly relevant for understanding atom loss and the energetic evolution of ultracold gases of fermionic lithium atoms in their ground state.
Beschreibung:Gesehen am 28.06.2023
Beschreibung:Online Resource
ISSN:2469-9934
DOI:10.1103/PhysRevA.107.053310