Galaxy formation from the IIB Superstring with Fluxes Tonatiuh Matos http:/www.fis.cinvestav.mx/~tmatos. Problems with the CDM Model. Dark Energy: Extreme fine tuning for Coincidence Dark Matter: Cuspy central density profiles Too much substructure Too late galaxy formation
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+ dV/d = 0
Scalar Field Fluctuation = HaloTonatiuh Matos and F. Siddhartha GuzmanClass. Q. Grav. 17(2000)L9; Tonatiuh Matos, F. Siddhartha Guzman and Dario Nuñez, Phys. Rev. D62(2000)061301(R);Tonatiuh Matos and F. Siddhartha Guzman,Class.Q. Grav. 18(2001)5055