PPT-Cosmic rays, antimatter, dark matter
Author : briana-ranney | Published Date : 2018-01-20
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
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Cosmic rays, antimatter, dark matter: Transcript
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 . & 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 . & 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 Discovery of Antimatter!. In 1932 Carl Anderson studied cosmic rays using a “cloud . chamber”. . Charged particles produced in cosmic rays would enter the chamber and leave “tracks”. The tracks would bend in circles because the chamber was placed in a strong magnetic field. Theoretical Motivation. Cosmological Role. Experimental Searches. Georg Raffelt. Max Planck Institute for Physics. Munich. xions. Axion Physics in a Nut Shell. CP conservation in QCD by. Peccei-Quinn mechanism. 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.. 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” .... The universe is the sum of all energy, matter, space and time.. But there. ’. s a difference between the universe we see (the observable universe) . and the universe as it really exists.. This gets complicated….. 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.. Cosmological Role. Experimental Searches. Georg Raffelt. Max Planck Institute for Physics. Munich. xions. Axion Physics in a Nut Shell. CP conservation in QCD by. Peccei-Quinn mechanism. For f. a. . 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. Dynamics. of. FRWL Universes. . Dynamics. FRW Universe. Friedmann-Robertson-Walker-Lemaitre Universe. . Cosmic Constituents:. Evolving Energy Density . . FRW Energy Equation. To infer the evolving energy density .
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