PPT-Stochastic Particle Acceleration in High Energy Astrophysical Sources

Siming Liu University of Glasgow Collaborators Vahe Petrosian Yanwei Jiang Stanford University Zhonghui Fan Yunnan University Oct 2008 Krakow Poland Outline I Observations Distribution. introduction. Erik . Adli. , University . of . Oslo, . . August 2015, . Erik.Adli. @cern.ch. . , . v2.11. Video: the LHC accelerator. youtube: the LHC Accelerator. 3. 25 ns. Event rate in ATLAS : . Acceleration Mechanisms. 1. Acceleration Mechanisms. There is clear observational evidence that hadrons and electrons are accelerated to extreme energies by astrophysical objects. direct evidence: charged cosmic rays. Introduction: What is particle astrophysics?. 1. What is particle astrophysics?. Particle astrophysics is the use of particle physics techniques (experimental or theoretical) to address astrophysical questions.. (Fermi acceleration at shock: most standard, nice powerlaw, few free parameters). main . signatures to . be determined: . E. min . , . E. max. [. Ã. timescale . t. acc. (E. ) ], . spectral slope . 2. PH421: . Homework . 30%;. . Laboratory reports . 35%; . . Final 35%. . All . lab reports will be submitted in class.. ~ November 2015 ~ . Mon. Tue. Wed. Thu. Fri. 9. 10 . 11 . Civic Holiday. 12 . 2. PH424: . Homework 30%;. Laboratory reports 35%; . Final 35%. . Feb & March 2017 ~ . Mon. Tue. Wed. Thu. Fri. 13. Simple Harmonic Motion. - 4 representations. 14 . - Free motion of an oscillator . "QFT methods in stochastic nonlinear dynamics". ZIF, 18-19 March, 2015. D. Volchenkov. The analysis of stochastic problems sometimes might be easier than that of nonlinear dynamics – at least, we could sometimes guess upon the asymptotic solutions.. in a Developing Turbulence. . Shuichi M. ATSUKIYO. . ESST Kyushu Univ.. Collaborator : T. . Hada. Outline . Background. -- motivation. -- acceleration processes in turbulent plasmas. -- parametric instability (PI). . Spring 2018. Introductions. Overview of Particle . Accelerators. Todd Satogata (Jefferson . Lab and ODU) . / . satogata@jlab.org. http://www.toddsatogata.net/. 2018-ODU-AP. Happy Birthday to Nina Dobrev, Dave Matthews, Jimmy Page, Joan Baez, and Vladimir Steklov!. Excitations Nucléaires par Laser . Group. :. M.M. Aléonard, . M. Gerbaux. , F. Gobet, F. Hannachi, G. Malka, C. Plaisir, J.N. Scheurer, M. Tarisien.. CERN, CLIC meeting - October, 3. rd. 2008. In all the . 1. John Beacom, The Ohio State University. High Energy . Neutrino . Astronomy. Topic: Impossible. Requires. : sources that reach high energies. . sources that are luminous. . sources of different types. based on the course by. Joël . Le . Duff. Many Thanks!. CAS on Advanced Level Accelerator Physics Course . Trondheim, 18-29 August 2013. Summary of the 2 lectures:. Acceleration methods. Accelerating. Steven Jamison, . Lancaster University. & UK mm-wave acceleration steering group. S.P. . Jamison,. . High . Gradient . Accelerator . T. ownhall. , 31. st. May 2021. Lancaster University, University of . Erik . Adli, University of Oslo,. . September 2017, . Erik.Adli. @cern.ch. . , v2.30. Particle accelerator physics. Particle detectors. Data analysis. The study of relativistic charged particle beams in electromagnetic fields.