The condensation of ideal Bose gas in a gravitational field in the framework of Dunkl-statistic

In the framework of theory Dunkl-deformed bosons, Bose-Einstein condensation two and three-dimensional Dunkl-boson gases confined in one-dimensional gravitational field is investigated. Using semi-classical approximation method, we calculate expressions Dunkl-critical temperature $T_{c}^{D}$, ground state population $\frac{N_{0}^{D}}{N}$ Dunkl-mean energy Dunkl-specific heat functions. Further numerical calculation shows that ratio $\frac{T_{c}^{D}}{T_{c}^{B}}$ increases with increasing Wigner parameter.