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Using a cosmological galactic evolutionary approach to model the Milky Way,we calculate the star formation history (SFH) of the solar neighborhood. Thegood agreement we obtain with the observational inferences suggests that ourphysical model describes accurately the long term/large spatial trends of thelocal and global Milky Way SFH. In this model, star formation is triggered bydisk gravitational instabilities and self-regulated by an energy balance in theISM. The drivers of the SFH are the cosmological gas infall rate and the gassurface density determined by the primordial spin parameter. A LambdaCDMcosmology was used throughout.Comment: 8 pages, uses kluwer.cls. Invited talk, to appear in "New Quests in  Stellar Astrophysics: The link between Stars and Cosmology", eds. M. Chavez,  A. Bressan, A. Buzzoni & D. Mayya, Kluwer Academic Publisher

Star Formation History in the Solar Neighborhood: The Link Between Stars and Cosmology