2011
DOI: 10.1103/physrevlett.106.170402
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Temperature Dependence of the Universal Contact Parameter in a Unitary Fermi Gas

Abstract: The contact I, introduced by Tan, has emerged as a key parameter characterizing universal properties of strongly interacting Fermi gases. For ultracold Fermi gases near a Feshbach resonance, the contact depends upon two quantities: the interaction parameter 1/(kF a), where kF is the Fermi wave-vector and a is the s-wave scattering length, and the temperature T /TF , where TF is the Fermi temperature. We present the first measurements of the temperature dependence of the contact in a unitary Fermi gas using Bra… Show more

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Cited by 87 publications
(119 citation statements)
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“…In order to appreciate the sensitivity of the slope to the choice of the values of ξ and ζ, in Fig.2, we also show the predictions [green (light gray) line] for the frequency shifts using the values ξ = 0.41 and ζ = 0.74, yielding the smaller value I/N k 0 F ≃ 2.7 for the contact. This value is closer to the measurement of the contact carried out in [5] and [9] at slightly higher values of temperature. The resulting slope δω/ω ∼ 0.09/(k 0 F a) provides a worse description of the experimental data for the collective frequencies.…”
Section: Collective Frequencies and Sound Velocity Shifts Near Usupporting
confidence: 83%
See 1 more Smart Citation
“…In order to appreciate the sensitivity of the slope to the choice of the values of ξ and ζ, in Fig.2, we also show the predictions [green (light gray) line] for the frequency shifts using the values ξ = 0.41 and ζ = 0.74, yielding the smaller value I/N k 0 F ≃ 2.7 for the contact. This value is closer to the measurement of the contact carried out in [5] and [9] at slightly higher values of temperature. The resulting slope δω/ω ∼ 0.09/(k 0 F a) provides a worse description of the experimental data for the collective frequencies.…”
Section: Collective Frequencies and Sound Velocity Shifts Near Usupporting
confidence: 83%
“…where with the index ± referring to the higher (+) and lower (−) frequencies of (9). In the second equality of (15), we have used relation (7) for the contact parameter calculated for an harmonically trapped atomic cloud and we have expressed the Fermi momentum k F in terms of the ideal Fermi gas wave vector k…”
Section: Collective Frequencies and Sound Velocity Shifts Near Umentioning
confidence: 99%
“…As is clear from its definition, C is also proportional to the local interaction energy. Although contact has been shown to relate various thermodynamic and many-body properties of a short-range interacting gas, it has so far been studied only in equilibrium and only with an unmagnetized gas [25,[30][31][32][33]. Figure 3A shows that after a short hold time the spectrum exhibits only the single-particle peak, whereas after a longer hold time, the spectrum develops a high-frequency tail.…”
Section: Fig 1 Magnetization Dynamicsmentioning
confidence: 99%
“…Some of the complications that naturally occur in experiments are then numerically investigated: a Bogoliubov theory is used to assess the conditions to be imposed to the geometry and the temporal duration of the pulse; a classical field model is used to assess the conditions on the amplitude of the gauge field for the linear response theory to be valid. A main difficulty appears to be the relatively small amount of energy that can be deposited in the gas before nonlinear couplings become difficult to extrapolate out: the resulting figure is on the order of 1% of the total energy of the gas, which is however not far from the sensitivity of state-of-the-art thermodynamic measurements of the energy [21][22][23][24][25].…”
Section: Introduction and Summary Of Main Resultsmentioning
confidence: 99%
“…Our scheme however requires a measurement of an energy change, not an absolute measurement of the energy, giving hope for a better precision. Recent experiments have actually measured the change of the momentum [24] and of the energy [25] of a gas to determine its structure factor with good precision, not for a gauge field excitation as proposed here, but for a…”
mentioning
confidence: 99%