A claimed stable BEC star solution in f(R,T) gravity based on the Durgapal-Fuloria metric, but the derivation is opaque and internally inconsistent.
Dynamics of trapped Bose gases at finite temperatures
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abstract
Starting from an approximate microscopic model of a trapped Bose-condensed gas at finite temperatures, we derive an equation of motion for the condensate wavefunction and a quantum kinetic equation for the distribution function for the excited atoms. The kinetic equation includes collisions between the condensate and non-condensate atoms ($C_{12}$), in addition to collisions between the excited atoms as described by the Uehling-Uhlenbeck ($C_{22}$) collision integral. Assuming that the $C_{22}$ collision rate is sufficiently rapid to produce a local equilibrium Bose distribution, the kinetic equation can be used to derive hydrodynamic equations for the non-condensate. These equations include a description of the equilibration of the local chemical potentials of the condensate and non-condensate components which gives rise to a new relaxational mode associated with the exchange of atoms between the two components. We show how the Landau two-fluid equations emerge in the frequency domain $\omega \tau_\mu \ll 1$, where $\tau_\mu$ is a characteristic relaxation time of the equilibration process. This process provides an additional source of damping of the collective modes (first and second sound in the case of a uniform system). Our equations are consistent with the generalized Kohn theorem. Finally, a variational solution of the equations is developed which is used to determine some of the monopole, dipole and quadrupole normal modes of a trapped Bose gas in an isotropic trap.
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Durgapal-Fuloria Bose-Einstein condensate stars within $ f(R,T) $ gravity theory
A claimed stable BEC star solution in f(R,T) gravity based on the Durgapal-Fuloria metric, but the derivation is opaque and internally inconsistent.