PPT-Radiation Backgrounds for Future High Energy Electron Positron Colliders

Radiation Backgrounds for Future High Energy Electron Positron Colliders Hongbo Zhu IHEP Beijing On behalf of the CEPC Study Group Workshop on the Circular Electron Positron Collider EU edition 24 26 May Rome. TED 121 Educational Technology. Dr. Steve Broskoske. This exercise will afford you an opportunity to create artistic backgrounds to enhance the topic presented on a slide, making them more meaningful and instructionally effective.. Tzu-Cheng, Chuang. . (. 莊子承. ). Exchange student from. National Tsing-Hua University (Taiwan). (. 國立清華大學. , . 台灣. ). Where?. Russia. China. Japan. Taiwan. Zoom in. China. Hong Kong. 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 . collapses. In . collaboration. . with. . Wen-Biao. Han, & Remo . Ruffini. . ICRANet. & . Physics. . Department. , . University. . of. . Rome. She-Sheng. . Xue. MG13, Stockholm, July 5. Tim Wiser. Splash P2506. 3 Nov 2012. Plan . Standard Model of Particle Physics. Particles, interactions, and the Higgs field. Drawing Feynman diagrams. These simple pictures are actually . calculational. CEPC and past CLIC studies. Armen Apyan. Northwestern University. Evanston, IL, US. 26/05/2014. FCC-ee Accelerator meeting #6. 1. Outline. __________________. Polarized Positron Production Methods. CLIC Main . Chemistry. ________________ involve changes with electrons. . ________________ involve changes in atomic nuclei. . Spontaneously-changing nuclei emit ________ and. are said to be _________. . Chemical reactions. R.CHEHAB (IPNL). On behalf of . I.Chaikovska. (LAL), . H.Guler. (LAL), . P.Bambade. (LAL), . O.Bianco. (LAL), . F.Plassard. (LAL), . X.Artru. (IPNL), . M.Chevallier. (IPNL), . J.Gao. (IHEP), . throughout the radiation belts. Sarah . Glauert. British . Antarctic Survey, Cambridge, UK. SPACECAST . stakeholders . meeting, . BAS, . 7 February 2014. Electron Radiation Belts. High energy electrons (E>500 keV) are trapped by Earth’s magnetic field. M.I. . Bryzgunov. , V.V. . Parkhomchuk. , V.B. . Reva. Budker Institute of Nuclear Physics, Novosibirsk, Russia. NICA project. The NICA (. Nuclotron. -based Ion Collider . fA. с. ility. ) . complex . 1 Identify and describe the process of Recognize the implications of the various interaction processes in imaging, radiation shielding, and Identify and describe the process of Recognize the implicati A person working with radioisotopes wears protective clothing and gloves and stands behind a shield.. 2. Radioactive Isotopes. A . radioactive isotope . has an unstable nucleus. emits radiation to become more stable. beta decay. . They are designated by beta (β). There are two forms of beta decay, . β. −.  and . β. +. , which respectively give rise to the electron and the positron.. . The generalized atomic equation for beta decay is as follows. Lightsource. (SSRL) . Michael Toney . Synchrotron . Materials Sciences . Division, SSRL. SLAC National Accelerator Laboratory. http://. www-ssrl.slac.stanford.edu/toneygroup. Outline. 2. SSRL & Synchrotron Radiation.