waynehu
Professor,
Department of Astronomy and Astrophysics
University of Chicago
Transfer Function
D.Eisenstein, W.Hu
We provide here accurate fitting forms for the matter transfer function
of adiabatic models, including high baryon and mixed dark matter
variants.
-
High baryon models (use if interested in baryon oscillations
significant for Ωb/Ωm >
Ωmh2+0.2
- Codes
- Animated Parameter Variation
- CDM Variants accurate for
Ωb/Ωm<0.3,
Ων/Ωm<0.3
-
Includes degenerate mass neutrinos, cosmological constant,
and spatial curvature.
- Transfer function codes
- Animated Parameter Variation
Based on: