Large-scale structure in superfluid Chaplygin gas cosmology

We investigate the growth of large-scale structure in the superfluid Chaplygin gas (SCG) model. Both linear and non-linear growth, such as $σ_8$ and the skewness $S_3$, are discussed. We find the growth factor of SCG reduces to the EdS case at early times while differs from the $Λ$CDM case in the large $a$ limit. We also find there will be much stricture growth on large scales in the SCG scenario than in $Λ$CDM and the variations of $σ_{8}$ and $S_3$ between SCG and $Λ$CDM can not be discriminated.

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