# Frustrated orbital Feshbach resonances in a Fermi gas

**Authors:** E. K. Laird, Z.-Y. Shi, M. M. Parish, J. Levinsen

arXiv: 1908.04495 · 2020-02-25

## TL;DR

This paper explores how frustration in orbital Feshbach resonances affects interaction tuning in fermionic gases, revealing suppressed binding energies and weaker pairing, with implications for superconductivity and superfluidity.

## Contribution

It provides a theoretical analysis of frustration effects in orbital Feshbach resonances in a $^{173}$Yb system, highlighting their impact on two-body and many-body interactions.

## Key findings

- Suppressed ground state binding energy due to closed-channel atom addition.
- Weaker fermion pairing when a closed-channel Fermi sea is introduced.
- Potential relevance to unconventional superfluidity and superconductivity.

## Abstract

The orbital Feshbach resonance (OFR) is a novel scheme for magnetically tuning the interactions in closed-shell fermionic atoms. Remarkably, unlike the Feshbach resonances in alkali atoms, the open and closed channels of the OFR are only very weakly detuned in energy. This leads to a unique effect whereby a medium in the closed channel can Pauli block, or frustrate, the two-body scattering processes. Here, we theoretically investigate the impact of frustration in the few- and many-body limits of the experimentally accessible three-dimensional $^{173}$Yb system. We find that by adding a closed-channel atom to the two-body problem, the binding energy of the ground state is significantly suppressed, and by introducing a closed-channel Fermi sea to the many-body problem, we can drive the system towards weaker fermion pairing. These results are potentially relevant to superconductivity in solid-state multiband materials, as well as to the current and continuing exploration of unconventional Fermi-gas superfluids near the OFR.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1908.04495/full.md

## References

68 references — full list in the complete paper: https://tomesphere.com/paper/1908.04495/full.md

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Source: https://tomesphere.com/paper/1908.04495