Collider Phenomenology. SWIMP Dark Matter. no signals in direct / indirect dark matter searches ... Rich collider phenomenology (no direct/indirect DM signal) ...
Cosmology and Collider Physics - Focus on Neutralino Dark Matter - Masahiro ... Cosmology in ... Interesting interplay between cosmology and collider physics ...
Early Universe dense and hot; WIMPs in thermal equilibrium ... Need precise predictions within models of SUSY breaking. WHEPP-9 Bhubaneswar. 44. S. Kraml ...
Prospects depend on both the characteristics of the dark matter particle and its ... (Draco, Sagittarius, etc.) Little is known for certain about the halo ...
Problem 2: Halo substructure. N-body simulations show more than 10 ... find very dense dark halo with profile r-1.2, with very stringent constraints to core. ...
Michael Turner: 'Accelerators, Astrophysics and Funding' Very much an overview here - we have three ... Feng, Murayama, Peskin, Tata (1995) LC500. B.~ H.~ B ...
... Dec 2006. The Quest for SUSY : issues for collider physics and cosmology ... The cosmology connection. Dark matter. EW phase transition and baryon ... cosmology ...
As a result of the thermal freeze-out process, a relic density of WIMPs is left behind: ... LHC Relic Density. Studying SUSY with the LHC and Astrophysics ...
Involving ETmiss, jet production, lepton ID, etc Relevant to Dark Matter, ... by space- based detectors such as EGRET/GLAST with thresholds as low as 100's ...
Less dependent on understanding of halo profile, diffusion parameters ... (Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such ...
... and every ordinary particle, a SUSY partner is present compensating each other. ... are already capable to sample the SUSY models at a level compatible with ...
The LHC and its multi-purpose detectors, for high pt physics (and forward physics? ... by space- based detectors such as EGRET or GLAST with thresholds as low as ...
(Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such objects ... Halo profile (inhomogeneities?) Boundary conditions ...