PPT-Cosmic rays, antimatter, dark matter

the need for cross section data Fiorenza Donato Torino University and INFN Compass Analysis Meeting CERN 16042015 Plan of my talk What are cosmic rays CRs Searches for dark matter in CRs. 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 . (for the STAR Collaboration) . . Heavy and Exotic Antimatter . . What has RHIC discovered?. . and signal (for . discovery. ). How . Anti-Helium-4. was discovered. What can we do with the discovery?. & 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. 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 . 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 . 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. & 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. 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. Objectives. What is antimatter?. Antiparticles. Annihilation. Artificial production. Applications. CONTENTS. To understand the basics of antimatter technology.. OBJECTIVES. Antimatter is exactly what you might think it is -- the opposite of normal matter, of which the majority of our universe is made. These anti-particles are, literally, mirror images of normal matter. Each anti-particle has the same mass as its corresponding particle, but the electrical charges are reversed.. 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. antimatter. ?. Susan Cartwright. The Standard Model of particle . physics contains 12 fundamental . particles. 9 of these have electric charge. It turns out that each of these particles has a corresponding antiparticle. Research physicist. CERN. 2. The story line of .... Detective story about a . secret society which .... ... steals 1 g of antimatter from a physicist . at the ‘LHC’ in a place called “CERN” .... via QFT Effects from. Parallel Electric and Magnetic Fields. 22 April 2016. Gerald B. Cleaver. Head, Early Universe Cosmology & Strings Division. Center for Astrophysics, Space Physics, & Engineering Research. What is antimatter?. Antiparticles. Annihilation. Artificial production. Applications. CONTENTS. To understand the basics of antimatter technology.. OBJECTIVES. Antimatter is exactly what you might think it is -- the opposite of normal matter, of which the majority of our universe is made. These anti-particles are, literally, mirror images of normal matter. Each anti-particle has the same mass as its corresponding particle, but the electrical charges are reversed..