Orateur
M.
Manoj Kaplinghat
(UC Irvine)
Description
I will discuss superWIMP dark matter models and differentiate their
predictions from that of WIMP dark matter, focusing on the differences
in the BBN era and for small-scale structure formation. I will draw
some generic lessons for the connection between the particle
properties of dark matter and structure of dark matter on sub-galactic
scales and discuss present status and future observations that aim to
discern this structure.
Author
M.
Manoj Kaplinghat
(UC Irvine)
