Higgs mode in a strongly interacting fermionic superfluid
Higgs mode in a strongly interacting fermionic superfluid
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DOI:
10.1038/s41567-018-0128-6
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发表时间:
2018-08-01
期刊:
影响因子:
19.6
通讯作者:
Koehl, M.
中科院分区:
文献类型:
--
作者:
Behrle, A.;Harrison, T.;Koehl, M.
Higgs and Goldstone modes are possible collective modes of an order parameter on spontaneously breaking a continuous symmetry. Whereas the low-energy Goldstone (phase) mode is always stable, additional symmetries are required to prevent the Higgs (amplitude) mode from rapidly decaying into low-energy excitations. In high-energy physics, where the Higgs boson(1) has been found after a decades-long search, the stability is ensured by Lorentz invariance. In the realm of condensed-matter physics, particle-hole symmetry can play this role(2) and a Higgs mode has been observed in weakly interacting superconductors(3-5). However, whether the Higgs mode is also stable for strongly correlated superconductors in which particle-hole symmetry is not precisely fulfilled or whether this mode becomes overdamped has been the subject of numerous discussions(6-11). Experimental evidence is still lacking, in particular owing to the difficulty of exciting the Higgs mode directly. Here, we observe the Higgs mode in a strongly interacting superfluid Fermi gas. By inducing a periodic modulation of the amplitude of the superconducting order parameter Delta, we observe an excitation resonance at the frequency 2 Delta/h. For strong coupling, the peak width broadens and eventually the mode disappears when the Cooper pairs turn into tightly bound dimers signalling the eventual instability of the Higgs mode.