In a slowly rotating ideal Bose gas, the BEC critical temperature scales as (density x angular velocity)^{2/5} in the nonrelativistic limit, and the heat capacity acquires a jump at the transition.
III A, we compute the pressure P for a ro- tating Bose gas in NR and UR limits in terms of the corresponding fugacities [see ( III.12) and ( III.26)]
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Bose-Einstein condensation in a rigidly rotating relativistic boson gas
In a slowly rotating ideal Bose gas, the BEC critical temperature scales as (density x angular velocity)^{2/5} in the nonrelativistic limit, and the heat capacity acquires a jump at the transition.