CDM/baryon isocurvature perturbations in a sneutrino curvaton model
  Matter isocurvature perturbations are strictly constrained from cosmic microwave background observations. We study a sneutrino curvaton model where both cold dark matter (CDM)/baryon isocurvature perturbations are generated. In our model, total matter isocurvature perturbations are reduced since the CDM/baryon isocurvature perturbations compensate for each other. We show that this model can not only avoid the stringent observational constraints but also suppress temperature anisotropies on large scales, which leads to improved agreement with observations. 
Keisuke Harigaya, Taku Hayakawa, Masahiro Kawasaki, Shuichiro Yokoyama
hep-ph astro-ph.CO