Interacting Dark Energy
arXiv:hep-ph/0410292
Abstract
In this paper I discuss some of the phenomenologies of models of the dark energy interacting with the ordinary matter. After a very brief review about the current constraint on the equation of the state of the dark energy from the SN and a new scenario of dark energy {\it the Quintom}, I present models of Quintessential Baryo(Lepto)genesis, Quintessino dark matter and mass varying neutrinos in details.
Plenary talk at "SUSY2004", Tsukuba, Japan, June 2004: LaTeX with pdproc.sty (included), 13pages