Does a generalized Chaplygin gas correctly describe the cosmological dark sector? 

R.F. vom Marttens, LC, W. Zimdahl, W.S. Hipólito-Ricaldi & D.F. Mota

Phys.Dark Univ. 15, 114-124 (2017) [ads]

Generalized Chaplygin Gas Model. CMB temperature anisotropies (left), matter power spectrum (top right), and transfer function (bottom right).

Dark MaGICC: the effect of dark energy on disc galaxy formation. Cosmology does matter

C. Penzo, A. V. Macció, LC, G. S. Stinson & J. Wadsley

Mon. Not. Roy. Astron. Soc. 442, 176 (2014) [ads]

Zoomed hydro simulation in SUCDM model. Close view on gas (left),  large view on gas (top right), and close view on stars (bottom right).