PDF-possible experimental manifestation of ultrahigh energy cosmic etaneut

Abstractspreading leptons created at interaction of neutrinos with nucleons of the Antarcticice This suggests the presence of a possible lepton decay as the origin of suchevent However such an interpr. Extensive air showers generated by cosmic rays produce muons and highenergy photons which can be detected by the CMOS sensors of smartphone cameras The small size and low e64259ciency of each sensor is compen sated by the large number of active phon 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. . . 4:. Current frontiers. Mildly Perturbed universe at z=1100. Present universe at z=0. 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. Indonesia has a long history of the sculptural arts. Megalithic images are found in archeological sites in Sumatra, Java to Sulawesi. The 8-10. th. century sculptures and reliefs found in Java and Bali of Hindu-Buddhist origins reveal foreign influences. Indigenous tribes developed their own distinct tribal styles created as ancestor, deity and animal memorial sculptures. . China’s Space Station. Shuang-Nan Zhang (. 张双南. ). zhangsn@ihep.ac.cn. Center . for Particle . Astrophysics. 粒子天体物理中心. . Institute . of High Energy Physics. Chinese Academy of Sciences. China’s Space Station. Shuang-Nan Zhang (. 张双南. ). zhangsn@ihep.ac.cn. Center . for Particle . Astrophysics. 粒子天体物理中心. . Institute . of High Energy Physics. Chinese Academy of Sciences. 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:. North Bengal University. TeV Neutrinos and Gamma rays from Pulsars/Magnetars. Introduction. The energy spectrum of cosmic rays extends to extremely high energies, values exceeding 10. 20. . eV. .. The origin of the cosmic rays and the mechanism responsible for acceleration of cosmic rays to such high energies . (LEP and LHC experiments). Arturo . Fernández. , Mario Rodriguez. Facultad. de . Ciencias. . Físico. . Matemáticas. Benemérita. Universidad Autonoma de Puebla. Manaus, Brazil Aug. 3. rd. 2015. Glenn . Sembroski. QuarkNet. Summer Workshop. July 24,2012. The Big Question. Which has become the Big Mystery. Where do Cosmic Rays come from?. A multi-part question. i.e. Lots of small mysteries. Different answers for different energy regimes. Plasma. . Astrophysics. Roger . Blandford. Paul Simeon. Yajie. Yuan. KIPAC. Stanford. 27 i 2012. AronsFest. 2. Describing Cosmic Plasma. Fluid description. P. , . . , . v. , B…. Magneto Fluid Dynamics . 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. 16 – 20 March 2015. Cosmic Rays: the current position -. from AMS to the Auger Observatory. 1. Alan Watson. University of Leeds. a.a.watson@leeds.ac.uk. Lecture 1:. Overview of the cosmic ray scene.