PPT-Direct Dark Matter (WIMPs) Searches and the XMASS Experiment

S earches and the XMASS Experiment Y Suzuki Kamioka Observatory Institute for Cosmic Ray Research ICRR the University of Tokyo a nd Kamioka Satellite Institute for the Physics and Mathematic of the Universe IPMU the University of Tokyo. 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. :. Dark Matter & Dark Energy. WWK: Students will understand the theories of Dark Matter & Dark Energy and how they’re thought to affect the Universe. .. Dark Matter. Dark Matter . - . matter that influences the evolution of the universe . 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 . Giorgio Busoni. 1. Based. on. : . arXiv:1409.2893 (and 1307.2253, 1402.1275, . 1405.3101. , 1402.2285) . Oxford, 27 September 2014. Outline. Problems with EFT approach in Mono-X searches. From EFT to Simplified models. Ron-Chou Hsieh. CYCU. Outline. It seems to have something there!. What are they?. Link with physics beyond the SM.. DM searches.. Constructing a DM model. Summary. It seems to have something there!. Galactic rotation curves:. direct dark matter detection. S. Moriyama . Institute for Cosmic Ray Research, University of Tokyo. Oct. 8. th. , 2011 @ FPUA2011, Okayama, Japan. Principle of direct detection in Lab.. 001). The Final Exam is. . Thurs. day. ,. . December. 22, 8:. 0. 0 . – . 10:. 0. 0 . a. m. The Final Exam will be given . in. :. Willey 175. Don’t come to Anderson 210. No one will be there. No one.. Jing LIU. IPMU, Univ. of Tokyo. TAUP2011, Munich. XMASS collaboration:. Kamioka. Observatory, ICRR, Univ. of Tokyo. ：. Y. Suzuki, M. . Nakahata. , S. Moriyama, M. Yamashita, Y. . Kishimoto. ,. Y. . 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. Cosmic Visions: New Ideas in Dark Matter. Maryland, March 24, 2017. Jing Liu. University of South Dakota. Supported by. NSF PHY-1506036. JSPS Grant-in-Aid(B) 26800122. DAMA. March 24, 2017. Cosmic Visions: New Ideas in Dark Matter, Maryland. Heavy. and . Light. Species. Annika Peter. Center for Cosmology and . AstroParticle. Physics (CCAPP). The Ohio State University. @. HowWeScience. on Instagram and Twitter. Whoooo. are you…ooh ooh…ooh ooh. I. MAGING . A. TMOSPHERIC . C. HERENKOV . T. ELESCOPES. J-F. . Glicenstein. IRFU, CEA-. Saclay. Outline. Imaging Atmospheric Cherenkov Telescopes. Indirect dark matter searches with IACT. Results on the Galactic Halo (H.E.S.S).