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MultiComponent Dark Matter Da Huang Physics Department NTHU Fo Guang Shan 1 Talk Fo Guang Shan PRD89 0550212014 arXiv 13120366 amp Invited Paper for the S pecial Issue of Indirect Dark Matter Searches. This Statement of Excesses sets out the amount of resources that the Northern Ireland Assembly is asked to grant in Excess Votes for two departments Department of Culture Arts and Leisure and Department for Social Development in respect of the 20101 M. Bhuyan. 1. , V.M. Datar. 2. , S.D. Kalmani. 1. , S.M. Lahamge. 1. , N.K. Mondal. 1. , . P. Nagaraj. 1. , S. Pal. 1. , L.V. Reddy, A. Redij. 1. , D. Samuel. 1. , M.N. Saraf. 1. , . B. Satyanarayana. 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. . . 4:. Current frontiers. Mildly Perturbed universe at z=1100. Present universe at z=0. and Other . Applications. Neutron Monitor Community Workshop—Honolulu, Hawaii . October . 24-25, 2015. Physicist. National Urban Security Technology Laboratory . Science and Technology Directorate. 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. Bruce Reynolds, November 2015. 1. Outline. Cosmic Definition. Functional Size Measurement. Functional User Requirements. Non-Functional Requirements. COSMIC Approach. In-Class Exercise. COSMIC—a Real World example. Dave Ector. COSMIC PM for OSD. 4 November 10. COSMIC 2. 2. Requirements. GNSSRO Level . 1 . Requirements Documents (L1RD) . status. L1RD Completed and signed 5 May 2010. L1RD assessment underway. Initial budget/partnerships for COSMIC-2 do not fully support all L1RD requirements. What is Cosmic Education?. Cosmic education, one of Dr. Montessori’s fundamental principles, provides the students with opportunities for exploration and appreciation of the world around them. “When the child goes out, it is the world itself that offers itself to him. Let us take the child out to show him real things instead of making objects which represent ideas and closing them in cupboards”. (Montessori, 1994) . Heino Falcke . Radboud University, Nijmegen. ASTRON, . Dwingeloo. What we (don’t) know about UHECRs . We know:. their energies (up to 10. 20. eV).. their overall energy spectrum. We don’t know:. :. . 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. FM 2. FM 3. FM 4. FM5. FM6. 2016.214. 2016.215. 2016.216. 2016.217. 2016.218. 2016.219. 2016.220. FM . 1. TOTAL. 279. 377. 489. 240. 514. 617. 304. 383. 376. 327. 315. 174. 235. 22. 198. 242. USING DATA ON EXTRAGALACTIC DIFFUSE . GAMMA-RAY EMISSION. . A. . Uryson. Lebedev. Physical Institute RAS, . Moscow. INTRODUCTION. UHECR data are obtained by Pierre Auger Observatory (PAO) and Telescope Array (TA):. (LEP and LHC experiments). Arturo . Fernández. , Mario Rodriguez. Facultad. de . Ciencias. . Físico. . Matemáticas. Benemérita. Universidad Autonoma de Puebla. Manaus, Brazil Aug. 3. rd. 2015.