PPT-QCD Effects on Direct Detection of Wino Dark Matter
Author : marina-yarberry | Published Date : 2017-10-31
Natsumi Nagata Based on J Hisano K Ishiwata N Nagata 150400915 May 4th 2015 Phenomenology 2015 University of Minnesota Kavli IPMU SUSY SM Supersymmetric
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QCD Effects on Direct Detection of Wino Dark Matter: Transcript
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. Roberta Sparvoli. Rome . “. Tor Vergata. ”. . University. and . INFN, ITALY. PCC 2011 - CERN. SIGNALS . from. RELIC . WIMPs. Direct . searches. :. . elastic. . scattering. of a WIMP off detector . CoEPP. , University . of Melbourne. June . 26 2014. Explaining galactic structure and direct detection experiments with mirror dark matter. 1. For further details see review:. See this review for detailed references to the literature. 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. Martti Raidal . NICPB, . Tallinn, Estonia. 07.01.2015. NORDITA Winer School 2015. 1. 07.01.2015. NORDITA Winer School 2015. 2. We are experiencing very interesting period in . f. undamental physics . and Large-Scale Structure. 1. Cora Dvorkin. IAS (Princeton) Harvard (Hubble fellow) . COSMO 2014. August 2014, Chicago. Outline. Dark Matter overview.. Effect of . WIMP Dark Matter . Pre-SUSY Summer School. Melbourne, June 29-July 1, 2016 . An . Introduction. to. Particle. Dark . Matter. Santa Cruz Institute for Particle Physics. University of California, Santa Cruz. Thank you. @. Baryons2013, Glasgow . Motoi Tachibana (Saga Univ.). Dark matter . capture . in . n. eutron . stars . with exotic . phases. A modern physics perspective. . “. UROBOROS” = unity of matters & universe. 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. DARK MATTER &DARK ENERGY. We know about only normal matter which is only 5% of the composition of universe and the rest is . DARK MATTER & DARK ENERGY. DARK MATTER. Susan Cartwright. University of Sheffield. 1. Dark Matter. Astrophysical Evidence. Candidates. Detection. 2. The Astrophysical Evidence. Rotation curves of spiral galaxies. flat at large radii: if mass traced light we would expect them to be . Dr. Simona . Murgia. (UC, Irvine). Dr. Will Dawson (Lawrence Livermore National Laboratory). Carolyn Slivinski (STScI). Facilitator: Dr. Emma Marcucci (STScI). Science Briefing. October . 5. , 2017. wino dark matter from an effective field theory approach EVAN JOHNSON* IN COLLABORATION WITH ERIC BRAATEN * AND HONG ZHANG † *THE OHIO STATE UNIVERSITY † PHYSIK DEPARTMENT T31, TECHNISCHE UNI LAPTh. IRN . Terascale. meeting . May 21. st. , 2019. Annecy. w. / . G. Bélanger. , . T. M. a. , . Y. Soreq. work. in . progress. 2. Dark Matter. c. ompelling. o. bservational. . evidence. . through . 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) .
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