PDF-COSMIC RAY MUONS

Anthony Tatum xF076 What Is a Muon xF076 Cosmic Origin and Interactions xF076 Muon Production and Path xF076 Effects in The Atmosphere xF076 Using Muons to Test Beam Profile Monitor . 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. By Jacob Ritz. Kelly Clark. Zach Beckman . Setup. Box of magnets. Detector D. Detector B. Detector A. Magnetic field ~0.42 . mT. Muon. A Graphs. C. O. U. N. T. S. P. E. R. S. E. C. Voltage. A Singles Rate. J. Brunner. 20/02/2013. Relativistic Monopoles. Analysis for 2007/2008 published. N. Picot, S. Escoffier. New people needed for full analysis 2007/2012. We can still beat . IceCube. !!. Nuclearites. 2015/07/03. COSMIC RAY-BANS. Image source: http://. ssg.sheffield.ac.uk. The Standard Model and Muons. First, a brief (re) introduction to the standard model.. -- Here it is. Fundamental particles.. Quarks make up hadrons, e.g. protons, neutrons etc.. James . C. ostlow. , Ryan . Wilken. , and . Arnav. Joshi. Capstone B7. Project overview. with this mentorship we will be collecting data from the Cosmic Ray . Muon. Detector(CRMD). The data we will be collecting is the number of . cryo. needs. Mary . Convery. Muon Campus Review. 1/23/13. 2. The . anomolous. magnetic . moment and . g-2. g. . 2 but higher-order corrections. QED, EW, . hadronic. , new physics?. 3. proposed exp. precision. Puri. , . Y. Uchida, Y. . Yap, Imperial College London, . UK. R. B. Appleby, S. . Tygier. , The University of Manchester and the Cockcroft Institute, . UK. R. D’Arcy, A. . . Edmonds, M. Lancaster, M. Wing, . in condensed matter research. . Tom Lancaster. Durham University, UK. Condensed matter physics in a nutshell. Lev Landau (1908-1968). T>T. C. T<T. C. T>T. C. T<T. C. What can we do with . 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. Cioli Barazandeh, Angel . Gutarra-leon. and Walerian Majewski. Mentor: . Walerian. . Majewski. , Department of Physics . Northern Virginia Community College, Annandale, VA . Experiments. Hello, and welcome to my Presentation!. (MCORD) . for . MPD . detector. by . Polish consortium NICA-PL. 23.X.2019 NICA Days 2019. 23.X.2019 NICA Days 2019. Design, modeling . proposition. Motivation. T. rigger during commissioning. Muons detection – . Z( mumu ) & Z( mumug ) Prof. Goshaw Duke University Cuts Stage Number of Events passing cut Cut Percentage from total (%) Percentage from last cut (%) Total Events: 10001 - 100.00 - Vertex Cut: 999 (LEP and LHC experiments). Arturo . Fernández. , Mario Rodriguez. Facultad. de . Ciencias. . Físico. . Matemáticas. Benemérita. Universidad Autonoma de Puebla. Manaus, Brazil Aug. 3. rd. 2015. 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.