PPT-fsPHENIX Detector Overview

Joe Seele RBRC for the fsPHENIX Study Group sPHENIX Workfest Japan Outline Physics Program Review Measurement Needs and Design Parameters fsPHENIX Detector Overview 1 Plugging the holes in . 山下智弘. JST CREST/. 神戸大学. Borrowing especially from presentations of M. . Asai. (SLAC). Geant4 Tutorial @ Japan 2007. 17-19 Oct, 2007 @ RCNS, based on Geant4 9.0.p01. 1. Outline. Introduction. Matthew Mendonca. Woodside High . School. Mentor. : Dr. . Doug Higinbotham and Lawrence . Selvy. Abstract. The particles that make up the nucleus of an atom are so infinitesimally small that it takes a detector of large magnitude in order to predict where protons and neutrons are located. This certain device requires the construction and utilization of one-meter-long rectangular plastic bars called scintillators. Attached to the left and right ends of each bar are Photomultiplier Tubes (PMTs) and bases with outlets for high voltage and signal wires. In experiments, there is a thick wall of lead positioned in front of the detector which excludes nearly all charged particles and permits primarily neutrons to enter and react with the nuclei inside the bars. When charged particles do pass through the scintillators, photons are released and bounce around until they reach a light guide and are collected by the PMTs. Within these there is liberation of electrons which in turn provide an analog signal to the electronics. A data acquisition system (DAQ) comprised of ADCs (Analog-to-Digital Converters) and TDCs (Time-to-Digital Converters) then store the data into files for later replay and analysis. By doing so, we can better measure the type of particle detected, it’s trajectory, and the amount of energy that it deposits. To ensure that these complex apparatuses are working at an acceptable level, scientists manipulate the constant flux (100 particles/m. of Plastic Scintillator. Oct. 2, 2009. IP-BSM Group. 1. Schematic . Drawing . of. new Gamma Detector. 2. sandwich type calorimeter. SUS and plastic scintillation plate. wavelength-shifting fiber (WLSF) for light transmission. 2012/3/2. Y.Sugimoto. Background. Request for more space from DESY team. Several installation works in parallel. Depends on total allowed construction perio. d . Design of common cryogenic system. ILD, . Philip Anderson. National Sales Manager. System Sensor Canada. A hospital is like a city. Living areas. Machinery, high technology. Food prep/service. Retail, public spaces. Open spaces, parking. Wide range of application challenges. Brian . Kross. – mechanical design and construction / gas systems. Seungjoon. Lee – advanced image recon algorithms / mechanical / detectors. John . McKisson. – software / data acquisition / electronics. Mark Stewart. Materials Characterisation. Workshop on low gain fast silicon detectors for EM and synchrotron applications Nov 25th. Welcome to the National Physical Laboratory. Workshop on low gain fast silicon detectors for EM and synchrotron applications. side. Wago. 2002-1201 . Wago. 2002-3203 . Door open. 800x600x200 mm. 0.93x60 cm. 10 cm. 4.9 cm. 4.9 cm. GSM cable. Gas pipes. ~25cm. ~25cm. NSYS3D8620. Inputs. Outputs. 600. 8. 00. 200. 60cm. 90 ˚ turn. Jin Huang (BNL). for the PHENIX collaboration. 2014 RHIC & AGS Annual Users' Meeting - Workshop on Nucleon Structure. RHIC/AGS AUM 2014. Jin Huang <jhuang@bnl.gov>. 2. Overview. ~2000. 2017→2020. MicroTCA. platform with embedded sub-ns WR synchronization. G. .. Kasprowicz (WUT). 2. Outline. NICA . collider. & . Cosmic Ray Detector – Goals. SIPM AFE. SIPM readout chain based on Open Source HW. FCC week Washington. 23. -27 March . 2015. W. . Riegler. D. . Denisov. , H. . ten. Kate, L. . Lienssen. , F. . Lanni. , M. . Abbrescia. , R. Richter, Y. . Onel. , W. Smith, S. . C. hekanov. Exploration + Higgs as a tool for . results during isotopic analysis Traditionally it was recodetector with a full width half-maximum FWHMHowever in many cases when using large detectors or when using a short amplifier time constant thi Innovative silicon sensors for future trackers. N. . Cartiglia. M. . Mandurrino. INFN - Italy. Part II: Principles of operation of RSD. Single point precision and charge sharing. Signal formation. Charge sharing: RSD master formula. IceCube. Justin Vandenbroucke, June 9, 2021. IceCube. Bootcamp, WIPAC, UW–Madison. Outline. Neutrino interactions and cross sections. Muon lifetime. Charged particles losing energy in matter. Ionization.