'Susy dark matter' presentation slideshows

Dark Matter Phenomenology of the GUT-less CMSSM

Dark Matter Phenomenology of the GUT-less CMSSM. Pearl Sandick University of Minnesota. Ellis, Olive & PS, Phys. Lett . B 642 (2006) 389 Ellis, Olive & PS, JHEP 06 (2007) 079. Dark Matter Candidate!. R-Parity conservation. Why we like SUSY. Solves the Naturalness Problem

325 views • 26 slides

Daniel Stolarski

369 views • 18 slides

Constrained MSSM

Constrained MSSM. Requirements:. Unification of the gauge couplings Radiative EW Symmetry Breaking Heavy quark and lepton masses Rare decays (b -> s ?, b-> ?? ) Anomalous magnetic moment of muon LSP is neutral Amount of the Dark Matter Experimental limits from direct search.

249 views • 16 slides

Measurement of the LSP Mass

Measurement of the LSP Mass. Dan Tovey University of Sheffield On Behalf of the ATLAS Collaboration. Contents. Motivation: Why measure the LSP mass? Will assume LSP ? lightest neutralino in this talk Natural in many SUSY models (constrained MSSM etc.)

256 views • 13 slides

Measurement of the LSP Mass

Measurement of the LSP Mass. Dan Tovey University of Sheffield On Behalf of the ATLAS Collaboration. Contents. Motivation: Why measure the LSP mass? Will assume LSP ? lightest neutralino in this talk Natural in many SUSY models (constrained MSSM etc.)

178 views • 13 slides

Welcome talk I DEA meeting, Prague, 20 .- 21 . 4 .200 6

208 views • 9 slides