'Relic density' presentation slideshows

973 views • 78 slides

Dark Matters: WIMP and Beyond

Dark Matters: WIMP and Beyond. Shufang Su U. of Arizona SI 2005. Outline. -. Brief introduction of standard cosmology Dark matter evidence New physics and dark matter WIMP candidates: neutralino LSP in MSSM, lightest KK particle in UED

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Supersymmetric dark matter: implications for colliders and astroparticle

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A Solution to the Li Problem by the Long Lived Stau

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DARK MATTER AND THE LHC

DARK MATTER AND THE LHC. 24 April 2014 Technion Colloquium. UC Irvine Jonathan Feng. INTRODUCTION. The Higgs discovery at the LHC was a landmark achievement It capped a 50-year saga and completed the particle content of the Standard Model

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Relic Density at the LHC

Relic Density at the LHC. B. Dutta. In Collaboration With:. R. Arnowitt, A. Gurrola, T. Kamon, A. Krislock, D.Toback. Phys.Lett.B639:46,2006 , hep-ph/0608193 (Phys. Lett.B), To appear. SUSY in Early Stage at the LHC. The signal to look for: 4 jet + missing E T. Example Analysis.

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LHC PROSPECTS FOR COSMOLOGY

LHC PROSPECTS FOR COSMOLOGY. Jonathan Feng University of California, Irvine. COSMO 09, CERN 7 September 2009. LARGE HADRON COLLIDER. 7 Sep 09. Feng 2. LHC PHYSICS. Higgs Boson Particle Physics Beyond the Standard Model Supersymmetry Extra Dimensions

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Dark Matter in SUGRA Models with Universal and Nonuniversal Gaugino Masses

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Relic density in SUGRA models

Relic density in SUGRA models. Relic density in mSUGRA models Uncertainties from SUSY spectrum Implications for LHC Non universal models Remarks on direct detection. Introduction. Supersymmetric models with R parity conservation have a good darkmatter candidate: neutralino LSP

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Supersymmetric Dark Matter

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DARK MATTER: THEORY

DARK MATTER: THEORY. Jonathan Feng, UC Irvine SUSY11 Fermilab, University of Chicago. OUTLINE. Note: This is not an overview. Why? See talks of Aaron Pierce, Dan McKinsey, Simona Murgia Sentimentality for when people talked about what they were excited about

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Mia Schelke , Ph.D. Student The University of Stockholm, Sweden

Mia Schelke , Ph.D. Student The University of Stockholm, Sweden. Supersymmetric Dark Matter & coannihilations. Cosmo 03. SUSY DM phenomenology highlights What are coannihilations Why can coannihilations control the relic neutralino density When are coannihilations important

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THE DARK UNIVERSE

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The LC and the Cosmos: Connections in Supersymmetry

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Uncertainties in the relic density calculations in mSUGRA

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Uncertainties in the relic density calculations in mSUGRA

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Constraints on the very early universe from thermal WIMP Dark Matter

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Probing 23% of the Universe at the Large Hadron Collider

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Uncertainties in the relic density calculations in mSUGRA

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