PPT-Gamma rays from dark matter in the Galactic center and IN

Dan Hooper Fermilab University of Chicago University of Michigan Dark Matter Workshop April 1 5 th 2013 Dark Matter in The Galactic Center The volume surrounding the Galactic Center is complex backgrounds present are not necessarily well understood . 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 . Susan Cartwright. University of Sheffield. Neutrinos and the Universe. Discovering neutrinos. Detecting neutrinos. Neutrinos and the Sun. Neutrinos and Supernovae. Neutrinos and Dark Matter. Neutrinos and the Universe. 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:. Wavelength the size of an atom. Frequencies above UV. Uses of X-rays. Used in airports to examine luggage for the presence of dangerous weapons or bombs or for illegal transit of goods. . used to detect structural deficits or cracks in metal objects such as bridges and aircraft that are likely to be missed by the human eye. as . the target of . hadronic. gamma rays.  . Yasuo. . Fukui. Nagoya University. Southern Observatories .  . CTA meeting. April 16-17, 2015, Adelaide. 1. ISM. I. nterstellar . medium ISM . between stars. A ‘finger’ of the Universe’s dark-matter skeleton, which ultimately dictates where galaxies form, has been observed for the first time. Researchers have directly detected a slim bridge of dark matter joining two clusters of galaxies, using a technique that could eventually help astrophysicists to understand the structure of the Universe and identify what makes up the mysterious invisible substance known as . :. . the need for cross section data. Fiorenza Donato. Torino University and INFN. Compass Analysis Meeting. CERN, 16.04.2015. Plan of my talk. What are cosmic rays (CRs). Searches for dark matter in CRs. 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. H. . Herrmann (LANL. ). e. -. Next . Steps. Cherenkov detectors . Energy . thresholded. Gas limited to >2.5 . MeV. Solid limited to <~0.2 . MeV. Aerogel. might span the gap. Real . g. -ray spectroscopy (Energy resolved) . Giant Shocks in the Fermi Bubbles and the Origin of the Microwave Haze. Roland Crocker. ARC Future Fellow. Australian National University. image credit: NASA. Geoff Bicknell, RSAA. Ettore Carretti, Cagliari Observatory. Liz Hays . (. NASA Goddard Space Flight Center). The Origin of Cosmic Rays. Credit S. . Swordy. Victor Hess and his . “Flight . Ops . Team”, . 1912. From protons. Pion decay. Accelerated protons (p) interact with matter. 1. Julie . McEnery. (NASA/GSFC) on behalf of the AMEGO team.. Active . Galactic . Nuclei. Pulsars. Black Hole Binaries. Sun. Dark Matter. Novae. Gamma-ray Bursts. Diffuse galactic lines. AMEGO Collaboration. Vikram . Dwarkadas. . (U Chicago). Matthieu. Renaud, . Alexandre. . Marcowith. . (LUPM, U Montpellier). Vincent . Tatischeff. . (. Univ. Paris-. Sud. ). August 11 2017. TevPA 2017 : VVD. 1. We acknowledge support from the FACCTS program at . Schedule Notes. Program web page: . https://confluence.slac.stanford.edu/x/No-cDg. Hashtag #. FermiSchool. . Let’s Begin!. Intro to the Fermi Summer School. Liz Hays. NASA GSFC. May 28, 2019. What makes gamma-ray observations distinctive?.