PPT-QCD Effects on Direct Detection of Wino Dark Matter

Natsumi Nagata Based on J Hisano K Ishiwata N Nagata 150400915 May 4th 2015 Phenomenology 2015 University of Minnesota Kavli IPMU SUSY SM Supersymmetric SUSY Standard Model SM. THE . PAMELA POSITRON . EXCESS AS . WINOS?. Gordy Kane. January 2009. Ann Arbor. arXiv. 0812.4555, see also 0807.1509. Phill Grajek, Aaron Pierce, Dan Phalen, Scott Watson. LSP, WINO LSP, VERY WELL MOTIVATED FOR DARK MATTER. Axion Dark Matter. Georg G. . Raffelt. , Max-Planck-. Institut. f. ür Physik, . München. Physics Colloquium, University of Sydney, 3 March 2014. Axions. as Cold Dark Matter of the Universe. Dark . Craig Roberts. Physics Division. . Charting the interaction . between light-quarks. Recall Lecture IB …. Through QCD's Dyson-Schwinger equations (DSEs) the . pointwise. . behaviour. of the . β. Craig Roberts, Physics Division. . Collaborators: 2012-Present. Rocio. BERMUDEZ (U . Michoácan. ). ;. Shi CHAO. (. Nanjing U. ) ;. Ming-. hui. DING (. PKU. );. Fei. GAO (. PKU. ) ;. S. HERNÁNDEZ. Lisa Randall. Harvard University. @. lirarandall. . What do we know about dark matter?. It has gravitational interactions—of matter!. Gravitational . lensing. Rotation curves in galaxies. Detailed measurements of energy abundances—total and normal matter. in the continuum with. Dyson-Schwinger equations. Craig Roberts. Physics Division. . Published collaborations. ― 2010-Present. Rocio. BERMUDEZ (. U . Micho. á. can. ). ;. Chen . CHEN. (ANL, IIT, USTC);. Ton-scale detectors for direct detection experiments are expected to yield significantly improved sensitivities.. Direct Detection of . Dark Matter Degenerate with Colored Particle in Mass. . Natsumi. -Only SUSY Scenarios. Galileo Galilei Institute Week I. Collider Physics and the Cosmos. August 28-September 1, 2017. Bruce Schumm. UC Santa Cruz. Question to consider: In scenarios in which . gaunginos. Koichi Hattori. Fudan. University. “Strangeness and charm in hadrons and dense matter” @ YITP, May 15, 2017. Table of contents. “. QCD Kondo effect: . dense quark . matter . with . heavy-flavor . Cosmic Opportunities. . –. 45. th. SLAC Summer Institute. Jonathan . Feng. , UC Irvine. 16 August 2017. INTRODUCTION. We’ve learned a lot about the Universe. Dark . Matter: 23% . ± 4. %. Dark . Gravity . and Light. Black Holes. What is Dark Matter?. Recap. Midterm . Friday . 11/. 1: summary review sheet posted. Canvas homework : . due Wednesday. Lab this week. Using . gravity to measure . masses. Cao Hoang Nam. Phenikaa. . University. Based on . arXiv. : 2007.xxx. ICISE - . Quy. Nhon, July 2020. Plan of the talk. GR+SM . and . m. otivations for beyond. Flipped . U(1) extended Standard Model and Majorana dark matter. Niayesh Afshordi. Western University. Friday, April 13, 2012. “Friday . the 13th. . is a date considered to be bad luck in. . Western. . superstition. .” . -Wikipedia. . Outline. Introduction: Cold Dark Matter (CDM) . . Craig Roberts. Emergent Phenomena in the Standard Model. Existence of the Universe as we know it depends critically on the following empirical facts:. Proton is massive, . i.e. . the mass-scale for strong interactions is vastly different to that of electromagnetism.