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Beam-induced and cosmic-ray backgrounds observed in the ATLAS detector during the LHC 2012 proton-proton running period

  • The ATLAS collaboration
  • Aix-Marseille Université
  • University of Oklahoma
  • University of Iowa
  • Azerbaijan National Academy of Sciences
  • IN2P3/CNRS
  • University of Amsterdam
  • Michigan State University
  • University of California at Santa Cruz
  • University of Sussex
  • Tel Aviv University
  • Technion-Israel Institute of Technology
  • University of Oregon
  • Stockholm University
  • Oskar Klein Centre
  • National Institute for Nuclear Physics
  • King's College London
  • Abdus Salam International Centre for Theoretical Physics
  • AGH University of Krakow
  • Brookhaven National Laboratory
  • Northern Illinois University
  • Ludwig Maximilian University of Munich
  • Rutherford Appleton Laboratory
  • University of Liverpool
  • University of Belgrade
  • University of Göttingen
  • Laboratório de Instrumentação e Física Experimental de Partículas
  • University of Granada
  • NOVA University Lisbon
  • Boston University
  • Joint Institute for Nuclear Research
  • University of Rome Tor Vergata
  • Lund University
  • P.N. Lebedev Physical Institute of the Russian Academy of Sciences
  • University of Bologna
  • University of Victoria BC
  • Université Grenoble Alpes
  • Instituto de Física La Plata
  • CERN
  • Transilvania University of Brasov
  • Horia Hulubei National Institute of Physics and Nuclear Engineering
  • National Technical University of Athens
  • University of Salento
  • The University of Chicago
  • Columbia University

Research output: Contribution to journalArticlepeer-review

21 Scopus citations

Abstract

This paper discusses various observations on beam-induced and cosmic-ray backgrounds in the ATLAS detector during the LHC 2012 proton-proton run. Building on published results based on 2011 data, the correlations between background and residual pressure of the beam vacuum are revisited. Ghost charge evolution over 2012 and its role for backgrounds are evaluated. New methods to monitor ghost charge with beam-gas rates are presented and observations of LHC abort gap population by ghost charge are discussed in detail. Fake jets from colliding bunches and from ghost charge are analysed with improved methods, showing that ghost charge in individual radio-frequency buckets of the LHC can be resolved. Some results of two short periods of dedicated cosmic-ray background data-taking are shown; in particular cosmic-ray muon induced fake jet rates are compared to Monte Carlo simulations and to the fake jet rates from beam background. A thorough analysis of a particular LHC fill, where abnormally high background was observed, is presented. Correlations between backgrounds and beam intensity losses in special fills with very high β are studied.

Original languageEnglish
Article numberP05013
JournalJournal of Instrumentation
Volume11
Issue number5
DOIs
StatePublished - May 20 2016

Keywords

  • Beam-intensity monitors
  • Beam-line instrumentation (beam position and profile monitors
  • Bunch length monitors)
  • Data analysis
  • Performance of high energy physics detectors

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