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 . 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 . Jon Coleman, Royal Society Research Fellow . To detect and measure effects of Dark Energy density or any dark contents of the vacuum (DCV) . 2. Many thanks to the support of the:. Liverpool Particle Physics Group. Guidance in Cross-Gender and . Transgender . Pat Searches . 2. Introductions. Instructor’s name here. Instructor agency or credentials. Insert bullets as needed. 3. Prison Rape Elimination Act (PREA). 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:. 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 . Paul McMillan. Surveys For All, 1st February 2016 . Why do we care?. On the biggest scales, the ΛCDM model works. Why do we care?. On the scale of individual galaxies, agreement is less obvious.. Things are more complicated, we have to consider the baryons. 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.. National Science Foundation • Division of Astronomical Sciences . Prepared by the . Association of Universities for Research in Astronomy . SCIENCE. . PEOPLE TECHNOLOGY. Scientists Discover Galaxy that is 99.99 Percent Dark Matter. John . Moffat. Perimeter Institute. Miami 2015 Conference. Fort Lauderdale, December 16, 2015. 2015-12-21. 1. 2. 2015-12-21. 3. https://angel.co/mog. 2015-12-21. Introduction. Observations of the dynamics of galaxies as well as the dynamics. 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. Perimeter Explorations 01. CERN HST2019 . Uniform Circular Motion. Predict. Observe. Explain. How are . mass. and . speed. connected in circular motion?. mass. speed. Uniform Circular Motion. Objective: . 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). arXiv:2307.02207. Taylor R. . Gray. a. In collaboration with Riccardo . Catena. a. a. Chalmers. University of Technology. Supported by a research grant from the Wallenberg foundation. TAUP Vienna 2023.