Speaker
Prof.
Bumseok Kyae
(Pusan National University)
Description
The thermally produced LSP has long believed to be the best candidate
for dark matter in the Universe. However, recently reported PAMELA/Fermi's
observations on high energy cosmic positrons' excess seem to require
a new dark matter theory. It will be pointed out that they do not necessarily imply the presence of a new dark matter theory, and discussed how PAMELA/Fermi data can be explained, keeping the conventional scenario
of dark matter.
Author
Prof.
Bumseok Kyae
(Pusan National University)
