Description |
The conceptually simplest scenario for dark matter (DM) is that it is a stable thermal relic from standard Big Bang cosmology. In many SUSY models, it is the lightest neutralino. The relic density determination selects special regions in SUSY model parameter space with concomitant implications for collider physics, dark matter searches and low energy measurements. We point out some relatively robust implications for LHC and DM searches and conclude with an outlook for the future. |
Organised by | Dr. Vikram Tripathi |