1 code implementation • 5 Nov 2013 • E. Castorina, E. Sefusatti, R. K. Sheth, F. Villaescusa-Navarro, M. Viel
We show that using the variance of the cold dark matter rather than the total mass field, i. e., $\sigma^2_{cdm}(M, z)$ rather than $\sigma^2_{m}(M, z)$, yields more universal results.
Cosmology and Nongalactic Astrophysics