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Birkhäuser-Verlag eBooks

The Dilute Bose Gas in 3D

Published Dec 22, 2005• 0 citations
Publisher
DOI
10.1007/3-7643-7337-7_2

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We measure the ground-state occupation and energy of a dilute Bose gas of ${}^{87}\mathrm{Rb}$ atoms as a function of temperature. The ground-state fraction shows good agreement with the predictions for an ideal Bose gas in a 3D harmonic potential. The measured transition temperature is $0.94(5){T}_{o}$, where ${T}_{o}$ is the value for a noninteracting gas in the thermodynamic limit. We determine the energy from a model-independent analysis of the velocity distribution, after ballistic expansion, of the atom cloud. We observe a distinct change in slope of the energy-temperature curve near the transition, which indicates a sharp feature in the specific heat.

Physical Review Letters•Dec 16, 1996•318 citations
We study equilibrium properties of a cold two-component Fermi gas confined in a quasi-one-dimensional trap of the transverse size ${l}_{\ensuremath{\perp}}$. In the dilute limit ($n{l}_{\ensuremath{\perp}}\ensuremath{\ll}1$, where nnn is the 1D density) the problem is exactly solvable for an arbitrary 3D fermionic scattering length aF{a}_{F}aF​. When ${l}_{\ensuremath{\perp}}/{a}_{F}$ goes from $\ensuremath{-}\ensuremath{\infty}$ to $+\ensuremath{\infty}$, the system successively passes three regimes: weakly interacting Fermi gas, hard core Bose gas, and weakly coupled Bose gas. The regimes are separated by two crossovers at ${a}_{F}\ensuremath{\sim}\ifmmode\pm\else\textpm\fi{}n{l}_{\ensuremath{\perp}}^{2}$. In conclusion, we discuss experimental implications of these results.
We measure the ground-state occupation and energy of a dilute Bose gas of 87Rb{}^{87}\mathrm{Rb}87Rb atoms as a function of temperature. The ground-state fraction shows good agreement with the predictions for an ideal Bose gas in a 3D harmonic potential. The measured transition temperature is 0.94(5)To0.94(5){T}_{o}0.94(5)To​, where To{T}_{o}To​ is the value for a noninteracting gas in the thermodynamic limit. We determine the energy from a model-independent analysis of the velocity distribution, after ballistic expansion, of the atom cloud. We observe a distinct change in slope of the energy-temperature curve near the transition, which indicates a sharp feature in the specific heat.