Speaker
Prof.
Teruki Kamon
(Texas A&M University)
Description
Recently, it is shown that the modifications of the Boltzmann equation
describing the evolution of relic abundances due to dilaton dissipative-source
and non-critical-string terms change the cosmologically allowed parameter
space of SUSY model. In this talk, we will investigate the allowed parameter
space in the context of minimal SUGRA boundary condition at the LHC.
We will characterize the experimental final states to distinguish the new
scenario from the standard scenario. We will also discuss the impact of the
new scenario in dark matter detection rates.
Work done in collaboration with: B. Dutta, A. Krislock and D. Nanopoulos
Primary author
Prof.
Teruki Kamon
(Texas A&M University)
Co-authors
Mr
Abram Krislock
(Texas A&M University)
Prof.
Bhaskar Dutta
(Texas A&M University)
Prof.
Dimitri Nanopoulos
(Texas A&M University)
