introduction to cosmology ii. modeling the universe
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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)
????
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