2008
DOI: 10.1088/1748-0221/3/08/s08001
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LHC Machine

Abstract: 2008 JINST 3 S08001 9.3.1 The VME and PC Front End Computers 9.3.2 The PLCs 9.3.3 The supported fieldbuses 9.3.4 The WorldFIP fieldbus 9.3.5 The Profibus fieldbus 9.4 Servers and operator consoles 9.5 Machine timing and UTC 9.5.1 Central beam and cycle management 9.5.2 Timing generation, transmission and reception 9.5.3 UTC for LHC time stamping 9.5.4 UTC generation, transmission and reception 9.5.5 NTP time protocol 9.6 Data management 9.6.1 Offline and online data repositories 9.6.2 Electrical circuits 9.6.3… Show more

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Cited by 1,820 publications
(1,478 citation statements)
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References 26 publications
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“…The cosmic trigger configuration during this run period consisted of L1 triggers from the muon spectrometer 3 (both the Resistive Plate Chamber (RPC) and the Thin Gap Chambers (TGC)), the L1 calorimeter trigger and the MBTS. For much of the cosmic ray analysis discussed in Sect.…”
Section: Detector and Data Taking Overviewmentioning
confidence: 99%
“…The cosmic trigger configuration during this run period consisted of L1 triggers from the muon spectrometer 3 (both the Resistive Plate Chamber (RPC) and the Thin Gap Chambers (TGC)), the L1 calorimeter trigger and the MBTS. For much of the cosmic ray analysis discussed in Sect.…”
Section: Detector and Data Taking Overviewmentioning
confidence: 99%
“…The electromagnetic calorimeter (ECAL) of the Compact Muon Solenoid (CMS) experiment [1] is a high-resolution, hermetic, homogeneous and compact detector made of 75848 lead tungstate (PbWO 4 ) scintillating crystals arranged in a cylindrical structure around the LHC [2] interaction point. The lead tungstate crystals are radiation tolerant, have fast scintillation (∼ 75% in 25 ns), density ρ = 8.28 g/cm 3 , short radiation length (X 0 = 0.89 cm) and small Moliere radius (R M = 2.2 cm).…”
Section: Introductionmentioning
confidence: 99%
“…In such framework, dimension six operators are suppressed by a factor M 2 (M being the mass of heavy fermions integrated out) and the dark matter sector, charged under U(1) X , couples with the weak or coloured sector of the Standard Model. An interaction with the weak SM sector was shown to have possible astrophysical signatures [48,49], while a coupling to the coloured SM sector was constrained [11] using mono-jets events at the LHC [52], as well as indirect detection constraints arising from astrophysical measurements. Such couplings had been studied, together with couplings to the top quarks in [53] but only in the context JHEP03(2016)006 Figure 1.…”
Section: Introductionmentioning
confidence: 99%