A New look at Dark Matter in the Universe
APA
Kaplinghat, M. (2006). A New look at Dark Matter in the Universe. Perimeter Institute. https://pirsa.org/06060054
MLA
Kaplinghat, Manoj. A New look at Dark Matter in the Universe. Perimeter Institute, Jun. 20, 2006, https://pirsa.org/06060054
BibTex
@misc{ pirsa_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}, year = {2006}, month = {jun}, note = {PIRSA:06060054 see, \url{https://pirsa.org}} }
University of California, Irvine
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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.