2016
DOI: 10.1103/physrevlett.117.213001
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Comparison of Spectral Linewidths for Quantum Degenerate Bosons and Fermions

Abstract: We observe a dramatic difference in optical line shapes of a 4 He Bose-Einstein condensate and a 3 He degenerate Fermi gas by measuring the 1557-nm 2 3 S − 2 1 S magnetic dipole transition (8 Hz natural linewidth) in an optical dipole trap. The 15 kHz FWHM condensate line shape is only broadened by mean field interactions, whereas the degenerate Fermi gas line shape is broadened to 75 kHz FWHM due to the effect of Pauli exclusion on the spatial and momentum distributions. The asymmetric optical line shapes are… Show more

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Cited by 17 publications
(33 citation statements)
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“…By rewriting equation 1 we can express the unknown triplet-singlet scattering length in units of the very well known triplet-triplet scattering length, a tt = +7.512(5) nm = +142.0(1) a 0 [45]. We find a ts = +82.5(5.2) a 0 , which is in agreement with our previous result of a ts = +50(10) stat (43) syst a 0 [42].…”
Section: Resultssupporting
confidence: 90%
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“…By rewriting equation 1 we can express the unknown triplet-singlet scattering length in units of the very well known triplet-triplet scattering length, a tt = +7.512(5) nm = +142.0(1) a 0 [45]. We find a ts = +82.5(5.2) a 0 , which is in agreement with our previous result of a ts = +50(10) stat (43) syst a 0 [42].…”
Section: Resultssupporting
confidence: 90%
“…At the maximum density used in the experiments (peak density n(0) ≈ 4.5 × 10 13 cm −3 or equivalently µ ≈ k B × 0.5 µK), a full width δν max ≈ 4.4 kHz is expected (see supplementary material). The additional ac-Stark shift contribution to the width [42] is negligible for the range of ODT laser wavelengths used in the final measurement campaign. Possible line-pulling effects due to the asymmetric lineshape were investigated by fitting Gaussians to simulations of the broadened lineshape but were not found to affect the fitted frequencies.…”
Section: Resultsmentioning
confidence: 94%
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“…There are many experiments on the the cold and ultracold 3 He gases [19,20]. Consider a 3 He gas with the density n ≃ 1 × 10 18 m −3 [38][39][40]. The lower limit on the temperature, by the above estimation, is about 0.25µK.…”
Section: /6mentioning
confidence: 99%