A New look at Dark Matter in the Universe

          @misc{ scivideos_PIRSA:06060054,
            doi = {10.48660/06060054},
            url = {https://pirsa.org/06060054},
            author = {Kaplinghat, Manoj},
            keywords = {Cosmology},
            language = {en},
            title = {A New look at Dark Matter in the Universe},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2006},
            month = {jun},
            note = {PIRSA:06060054 see, \url{https://scivideos.org/pirsa/06060054}}
          }
          

Abstract

The best studied class of dark matter candidates in Supersymmetric theories is the WIMP, Weakly Interacting Massive Particles, which makes cold dark matter. There is a well-motivated alternative to the WIMP -- dark matter populated by decays of WIMPs. This dark matter from decays is closer in spirit to warm dark matter. They can be distinguished from cold dark matter by observations of structure on scales smaller than about a megaparsec, where cold dark matter models seem to face difficulty. Big Bang Nucleosynthesis predictions are also modified in interesting ways.