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Est-ce que MOND peut résoudre les trois principauxprobì emes du ?CDM ? On peut penser que oui : (i) l'absence dematì ere noiré elimine les cuspides, (ii) tout le moment angulaire reste dans les disques des galaxies au cours de leur formation, (iii) si la persistance des petits satellites est liéè a la présence de cuspides dans les micro-halos dematì ere noire, les forces de marée MONDienne pourraient elles, ? etre suffisantes pour déchirer ces sous-structures... Cette vision très optimiste n'attend que d'? etre testée par des simulations cosmologiques ! Il ne va pas sans dire que d'autresprobì emes vont venir se greffer, en particulier la physique des neutrinosà neutrinosà l'´ echelle des amas de galaxies. Si MOND ne fonctionne pas, c'est l'histoire de la formation des grandes structures qui peut le montrer. Malgré tout, il resterà a comprendre pourquoì a petité echelle ,
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