PPT-Atmospheric Muon Lifetime, Standard Model of Particles and

Cioli Barazandeh Angel Gutarraleon and Walerian Majewski Mentor Walerian Majewski Department of Physics Northern Virginia Community College Annandale VA Experiments Hello and welcome to my Presentation. with . climate variability and change . Seminar in Atmospheric Science, EESC G9910. Diagnosing ENSO from atmospheric composition (ozone measured from space). Ziemke. et al. ., 2010; . Oman et al. ., 2011. 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. Hyperons. Classification of the Elementary Particles. Elementary particles are classified into groups according to their mass and spin properties. These are, referring to their masses: . (1) the photon with zero rest mass and spin 1. It is a massless boson. . Atoms in magnetic field. orbiting electron behaves like current loop . .  magnetic moment . μ. = current x area . interaction energy = . μ. ·B. (both vectors!) = . μ. ·B. . loop current = -. 負電荷の. ミューオンの物質中での寿命. July 1. st. , 2014. Suguru. . Tamamushi. List of Contents. Purpose. Decay of Positive and Negative Muons. Experimental Procedure and Setup. Results. Nick Barlow. (University of Cambridge). on behalf of the ATLAS collaboration. Contents. Motivation . for searching for long-lived particles.. Very. quick look at a couple of . signal models. .. The ATLAS detector and the 2011 dataset.. for the GOCI. Jae Hyun . Ahn. *. Joo-Hyung. . Ryu. *. Young Jae Park*. Yu-Hwan . Ahn. *. Im. Sang Oh**. Korea Ocean Research & Development Institute. Seoul National University. I n d e x _. Introduction . S. Tarem, S. . Bressler. , S. . Vallecorsa. , E. . Kajomovitz. , S. . Trboush. A. . Soffer. , . Nimrod. What is RPVLL?. We work within the RPVLL subgroup of SUSY. It includes everything that does not rely on MET. QuarkNet. Student Investigations. DAQ Detector e-Lab. Mark Adams. Fermilab. DAQ Detector e-Lab. Global Cosmic Ray Effort. Outline. QuarkNet. Corrections. Atmospheric Effects on EMR. Kodiak Island, AK – Volcanic ash and clouds (MODIS image). Learning Objectives. What are the main ways that the atmosphere affects light traveling through it?. How did . the universe come to be the way that it . is?. Democritus (~2500 years ago). Recall the four fundamental forces:. GRAVITY: . All particles are influenced.. Relative strength: . WEAK: . All particles are influenced.. Atmospheric Correction Algorithm for the GOCI Jae Hyun Ahn * Joo-Hyung Ryu * Young Jae Park* Yu-Hwan Ahn * Im Sang Oh** Korea Ocean Research & Development Institute Seoul National University Cao Hoang Nam. Phenikaa. . University. Based on . arXiv. : 2007.xxx. ICISE - . Quy. Nhon, July 2020. Plan of the talk. GR+SM . and . m. otivations for beyond. Flipped . U(1) extended Standard Model and Majorana dark matter. Why study the anomalous magnetic moment of the muon?. Because, is one of the most precisely measured quantities in particle physics.. It put severe limits in deviations from the Standard Model and opens a window .