PPT-Dark matter searches by charged cosmic rays detection in sp

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 . 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 . 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.. & Large scale structure. Tarun Souradeep. I.U.C.A.A. .. Cosmology . IUCAA . VSP program. (. May 18-22, . 2012). Lec. . 2:. Cosmic Content. Perturbed Universe . Simple. … yet, an . exotic. The Future of Cosmic Ray Research. .. 8 The Future of Cosmic Ray Research . As we have seen, a few cosmic rays can be detected with energies somewhat . greater . than 10. 20. . eV. . . These high energies must be due to particle accelerations . AMS Discoveries Affecting Cosmic-Ray SIG Priorities. Eun-Suk. . Seo. Inst. for Phys. Sci. & Tech. and . Department of Physics. University of Maryland. AAS HEAD meeting, Chicago, IL, 19 August 2014. AY 17. 10/19/2011. Outline. What is Multi-messenger astronomy?. Photons. Cosmic Rays. Neutrinos. Gravity-Waves. Sample-Return. Outline. What is Multi-messenger astronomy?. Photons. Cosmic Rays. Neutrinos. 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 . 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. 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: . Eun-Suk. . Seo. Inst. for Phys. Sci. & Tech. and . Department of Physics. University of Maryland. AAS HEAD meeting, Chicago, IL, 19 August 2014. w. ith edits & voice from . Angela V. Olinto. X Rays. Are electromagnetic radiations having wavelength of order of 1. Are highly energetic radiations which are emitted when energetic electrons are made to incident on a metallic target.. Were discovered by German Physicist W.C. Roentgen in1895..