PPT-PRESENT AND FUTURE DARK MATTER SEARCHES WITH

I MAGING A TMOSPHERIC C HERENKOV T ELESCOPES JF Glicenstein IRFU CEA Saclay Outline Imaging Atmospheric Cherenkov Telescopes Indirect dark matter searches with IACT Results on the Galactic Halo HESS. 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 . This . powerpoint. will show you the basics of dark matter and dark energy . Their place in the universe . By Jordan . Ilori. . DARK MATTER. Dark matter is a type of matter hypothesized in astronomy and cosmology to account for a large part of the mass that appears to be missing from the universe. Dark matter cannot be seen directly with telescopes; evidently it neither emits nor absorbs light or other electromagnetic radiation at any significant level. Instead, the existence and properties of dark matter are inferred from its gravitational effects on visible matter, radiation, and the large-scale structure of the universe. According to the Planck mission team, and based on the standard model of cosmology, the total mass–energy of the known universe contains 4.9% ordinary matter, 26.8% dark matter and 68.3% dark energy. Thus, dark matter is estimated to constitute 84.5% of the total matter in the universe and 26.8% of the total content 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. 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 . 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. Cody . Carr. , Minh Nguyen. December 9. th. , 2014.. Agenda. Motivations (Cosmic & Atomic scales). Dark Matter categories. The Dark Matter Zoo. Neutrinos. Neutralinos. Kaluza. -Klein particles. Summary. 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. 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. 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. 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. 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 . 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) . 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.