Effective Theory of Interacting Dark Energy

To this purpose we use halo catalogs from N-body simulations of dynamical DE models and DM scenarios which are statistically indistinguishable from the standard Cold Dark Matter

Let us consider a spherical concentration of dark substance with a density in 1/r 2 (that we defined in previous sections) moving in the space. We could expect that its velocity

D’une part, sur le plan thématique, Allemagne année zéro est empreint d’un pessimisme évident qui contredit l’esprit des œuvres précédentes ; d’autre part, au niveau

We use the spherical collapse model of structure formation to investigate the separation in the collapse of uncoupled matter (essentially baryons) and coupled dark matter in

Let us consider a spherical concentration of dark substance with a density in 1/r 2 (that we defined in previous sections) moving in the space. We could expect that its velocity

Analyse méthodologique de la modélisation numérique des équations de la physique des milieux continus à l’aide de la méthode des éléments finis : flux-expert, un système

(Expérience III).. Pour les champs thermiques au sol, nous pouvons remar- quer une similitude générale dans la répartition des maxima et minima de la

Results Although the reduction of Sb(V) to Sb(III) under increased waterlogging time decreased Sb solubility, it increased Sb uptake by L. lanatus), implying preferential uptake