Holographic Cosmology Inflation and Entropy


Banks, T. (2011). Holographic Cosmology Inflation and Entropy. Perimeter Institute. https://pirsa.org/11070007


Banks, Tom. Holographic Cosmology Inflation and Entropy. Perimeter Institute, Jul. 15, 2011, https://pirsa.org/11070007


          @misc{ pirsa_11070007,
            doi = {},
            url = {https://pirsa.org/11070007},
            author = {Banks, Tom},
            keywords = {Cosmology},
            language = {en},
            title = {Holographic Cosmology Inflation and Entropy},
            publisher = {Perimeter Institute},
            year = {2011},
            month = {jul},
            note = {PIRSA:11070007 see, \url{https://pirsa.org}}


I provide a mathematical model of holographic cosmology whose coarse grained description is that of a homogeneous isotropic, flat universe, which makes a transitions from an FRW to an eternal de Sitter regime. Based on this model, I suggest some heuristic ideas which explain the low initial entropy of the universe and may provide a description of an inflationary era with small fluctuations.