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1 Etat de l'art De nombreux algorithmes pour la construction d'arbre de fusion analytique ont ´ eté implémentés ,
Un bilan de l'ensemble de ces méthodes, ainsi qu'une nouvelle approche, est disponiblè a la référence suivante, Cole Tous ces algorithmes reconstruisent l'histoire des halos dematì ere noire en remontant le temps, 1993. ,
se base sur l'hypothèse de fusions binaires : deux progéniteurs donnent naissancè a un descendant La masse du premier progéniteur est tirée en lien avec la masse du halo descendent (connue) suivant la distribution conditionnelle de masse (Eq. 2.10) La masse du second n'est alors rien d'autre que la différence entre la masse du halo descendant (donnée initiale) et la masse du premier progéniteur, ont mis en exergue des incompatibilités entre les résultats de cet algorithme binaire et les distributions théoriques des modèles dit de Press et SchechterétenduSchechterétendu (EPS), incompatibilités toujours présentes même pour des pas de redshift faibles. Pour pallieràpallierà ces divergences, 1993. ,
) l'hypothèse de la fusion binaire est conservée En revanche Somerville & Kolatt (1999) construisent des arbres de fusion multi-branches (N-branch), dans lesquels un halo peut avoir plus de deux progéniteurs. Alors que ces premiers algorithmes Monté-Carlo se basaient sur les distributions théoriques des modèles EPS, par la suite, 2000. ,
´ evolution des galaxies présenté ici utilise les résultats plus récents de Même si ces derniers s'appuient sur une paramétrisation identique (Eq. 4.1) pour la fraction de baryon, l'expression de la masse de filtrage est différente. Celle-ci est déduite d'un ajustement de l'´ evolution avec le, 2008. ,
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