Introduction to CosmologyII. Modeling the Universe

Marek DemianskiMarek DemianskiInstitute of Theoretical Physics

University of Warsaw

Fig. 16-27a, p.331

iPossible dark matter particlesparticles

neutralino, mN ~ 50 GeV,

gravitino,

axions,

other WIMPs

Dark energy

cosmological constant,

vacuum energy,

quintessence (potential q (penergy of some scalar field)

????