luminosity measurement and calibration at the lhc
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LUMINOSITY MEASUREMENT AND CALIBRATION AT THE LHC W. Kozanecki, - PowerPoint PPT Presentation

LUMINOSITY MEASUREMENT AND CALIBRATION AT THE LHC W. Kozanecki, CEA-IRFU-SPP LAL-Orsay, 28 April 2017 Outline 2 ! Introduction: the basics ! Relative-luminosity monitoring strategies ! Absolute-luminosity calibration strategies & their


  1. LUMINOSITY MEASUREMENT AND CALIBRATION AT THE LHC W. Kozanecki, CEA-IRFU-SPP LAL-Orsay, 28 April 2017

  2. Outline 2 ! Introduction: the basics ! Relative-luminosity monitoring strategies ! Absolute-luminosity calibration strategies – & their challenges ! Instrumental systematics in the high- L environment ! Achieved precision on L - and why it matters ! Summary ! Selected bibliography W. Kozanecki 28 Apr 2017

  3. Luminosity: definition 3 The key parameter for the experiments is the event rate R [events/s]. For a physics process with cross-section σ , R is proportional to the luminosity L L : R = σ L unit of L : 1/(surface × time) Population n 1 Population n 2 area A n 1 × n 2 Collision rate ∝ σ × × encounters/second A L (goal: ± 1–2 %)

  4. Basics of L measurement: Rate = σ * L 4 µ = number of inelastic pp collisions per bunch crossing n b = number of colliding bunch pairs f r = LHC revolution frequency (11245 Hz) σ inel = total inelastic pp cross-section (~80 mb at 13 TeV) ε = acceptance x efficiency of luminosity detector µ eff = # visible (= detected) collisions per bunch crossing σ eff = effective cross-section = luminosity calibration constant W. Kozanecki 28 Apr 2017

  5. The experimental environment 5 LHC fill 5451: 2208 bunches, 25 ns apart 10 34 L -calibration sessions W. Kozanecki 13 June 2016 & other special runs

  6. A key issue: the pile-up [ SppS; Tevatron; LHC] - 6 n VTX = 9 " µ ~ 18 inelastic interactions • all occuring within ±0.25 ns! • cannot be time-resolved by L detectors W. Kozanecki 28 Apr 2017

  7. Pile-up: a more typical event 7 n VTX = 17 µ ~ 34 W. Kozanecki 28 Apr 2017

  8. Handling the pile-up: principle 8 ! Event- (or zero-) counting: bunch-by-bunch (bbb) ! an “event” is a bunch crossing (BX) where a given condition is satisfied, e.g.: # EventOR = at least 1 hit in either the A arm of a luminometer, or the C arm, or both # EventAND (aka A.C) = at least 1 hit in the A-arm AND at least 1 hit in the C arm ! count the fraction of BX with zero events " µ from Poisson probability # If µ is the average number of inelastic pp collisions/BX, and N OR (N AND ) is the total number of OR (AND) “events” over N orbits , then (for 1 colliding bunch pair) the Poisson probability P to detect an “event”/BX is L ~ µ = = - ln(1 – P OR ) / ε OR ~ P OR / ε OR only when µ << 1 ! examples: V0 A.C (ALICE), LUCID_Bi_ORA (ATLAS), ≥ 2 VELO tracks (LHCb) W. Kozanecki 28 Apr 2017

  9. Pile-up! L -monitoring algorithms: rate = σ eff * L ? 9 ! Event- (or zero-) counting algorithms: bunch-by-bunch (bbb) ! count the fraction of BX with zero “events” " µ from Poisson probability # L is a monotonic (but non-linear) function of the “event” rate ! if µ gets too large, no empty events " “zero starvation” or “saturation” ! Hit-counting algorithms (bbb) Now: ATLAS: # LUCID hits. CMS: # pixel clusters . ! count the fraction of channels hit in a given BX # Poisson formalism, very similar to that of event counting # linearity vs. µ depends on technology, granularity, thresholds, ... ! Track- (& vertex-) counting algorithms: bbb, but TDAQ-limited ! conceptually similar to hit-counting. Examples: ATLAS, LHCb ! Flux-counting algorithms (summed over all bunches) ! example: current in ATLAS hadronic-calorimeter photomultipliers (PMTs) W. Kozanecki 28 Apr 2017

  10. ATLAS: redundancy " many L msmts! 10 Note: all luminometers are LUCID – Lu minosity measurement using a C herenkov I ntegrating D etector (bbb) independent of TDAQ " “ATLAS-preferred” (exc. trk-, vtx- & Z-counting) LUCID-2 for 13 TeV pp data + Z counting (relative- L checks) MPX/TPX + Vertex counting + Track counting (both bbb) " “ATLAS-preferred” for 7 & 8 TeV pp data BCM – B eam C onditions M onitor (bbb) W. Kozanecki 28 Apr 2017

  11. L -monitoring: instrumental strategies 11 Preferred offline ( " L phys ) Main addtn’l luminometers: luminometer offline corrections + systs. V0 (scintillator arrays): A.C ALICE T0 (Cherenkov arrays): A.C + Δ T cut AD (“diffractive” scint. arrays): A.C ZDC (had. cal): EventOR (Pb-Pb only) µ - & drift-corrected using: Si tracker: track counting LUCID-2 (quartz Cherenkov +PMTs): ATLAS EM/Fwd calorimeter: current in LAr gaps HitOR [hit counting, 2-arm inclusive] TILE hadronic calorimeter: PMT currents Pixel L telescope: evt cntg [3-fold AND] CMS / Muon Drift Tubes : track-segment cntg Si tracker: pixel-cluster counting (PCC) TOTEM Fwd calorimeter (HF): hit counting VELO tracker: vertex-based evt counting VELO tracker: track-based event LHCb PU & SPD arrays: hit counting counting Calorimeters (+ SPD): energy > E thresh W. Kozanecki 28 Apr 2017

  12. Absolute- L calibration: the initial plan 12 ! Optical theorem + pp $ pp (elastic) at low t ! dR el /dt + R inel ( R tot = R el + R inel ) [TOTEM + ALFA ] W. Kozanecki 28 Apr 2017

  13. Absolute- L calibration: the initial plan 13 ! Optical theorem + pp $ pp (elastic) at low t ! dR el /dt + R inel ( R tot = R el + R inel ) [TOTEM + ALFA ] ! dR el /dt in Coulomb-interference region [ALFA + TOTEM ] ! d σ el /dt, σ el msrd at √ s = 7+8 [+13] TeV (ALFA, TOTEM) ! but L -indep. method " only loose x-check (3.8 % so far) W. Kozanecki 28 Apr 2017

  14. Absolute- L calibration: actual strategy 14 Principle: σ eff = R collisions / L (beam parameters) ! van der Meer scans: L = f ( Σ x , Σ y , n 1 , n 2 ) Σ x ~ ( σ 1x 2 ) 1/2 2 + σ 2x ! Σ x,y from R vs. beam sep. ( δ x, δ y); n 1 , n 2 = bunch currents # + exploit luminous-region evolution in scan: ( δ x , δ y ) dependence of 3-d position, angles & width of luminous region (aka “beamspot”) ! Beam-gas imaging: L = f( σ x1 , σ y1 , σ x2 , σ y2 , σ z , φ c , n 1 , n 2 ) ! extract single-beam parameters from (x, y, z) distribution of reconstructed p-gas & pp evt vertices (stationary beams) ! Beam-beam imaging: L = f( σ x1 , σ y1 , σ x2 , σ y2 , ... , n 1 , n 2 ) ! scan B1 as a probe across B2 & v-v " single-beam parms # closely related to luminous-region evolution method in vdM scans W. Kozanecki 28 Apr 2017

  15. L calibration: van der Meer scans 15 ! Measure visible interaction rate μ eff as a function of beam separation δ ! The measured reference luminosity is given by L = n b f r n 1 n 2 2 π Σ x Σ y Σ x with Σ x,y = integral under the scan curve / peak = RMS of scan curve (if Gaussian) Hor. beam separation δ x [mm] W. Kozanecki 28 Apr 2017

  16. L calibration: van der Meer scans 16 ! Measure visible interaction rate μ eff as a function of beam separation δ ! The measured reference luminosity is given by L = n b f r n 1 n 2 peak µ eff 2 π Σ x Σ y Σ x with Σ x,y = integral under the scan curve / peak ! This allows a direct calibration of the effective cross section σ vis for each luminosity detector/algorithm scan widths effective bunch cross-section Hor. beam separation δ x [mm] populations peak rate ! Key assumption: factorization of luminosity profile L ( δ x , δ y ) = f x ( δ x ) f y ( δ y ) W. Kozanecki 28 Apr 2017

  17. L calibration: beam-gas imaging (BGI) 17 ! Extract p -density distributions ρ 1,2 (x, y, z) from simultaneous fit to 3D distributions of B1-gas, B2-gas & pp collision vertices ! Each beam modelled by non-factorizable sum of 3D gaussians ! L = 2c f r n 1 n 2 cos φ /2 ∫ ρ 1 (x, y, z, t) ρ 2 (x, y, z, t) dx dy dz dt Most critical: vertexing resolution " LHCb only! Typical σ L W. Kozanecki 13 June 2016

  18. L calibration: lessons from LHC run 1 18 ! The central role of beam dynamics ! L calibs: widely-spaced low-I bunches, no high- µ trains! # injected-beam quality, parasitic beam-beam, µ -dependence ! orbit drifts can cost 2-3% of bias &/or systematics ! beam-beam deflections & dyn. β must be corrected for ! non-factorization: an often dominant uncertainty ! Luminosity instrumentation: redundancy essential! ! non-linear headaches: µ -dep., but also total- L dep.? ! the pains of aging: response drifts %" reproducibility ! Run 2 harder: 25 vs 50 ns, higher L / multiplicity / ∫ dose W. Kozanecki 28 Apr 2017

  19. Beam-beam corrections (1) 19 ! Two distinct beam-beam effects: beam-beam deflection and dynamic β ! bias σ vis if not corrected ! < 0.5% PbPb, 1 - 2% for 7/8/13 TeV pp and around 4% for 5 TeV pp ! The interaction of the two beams during a scan distorts the scan curve Beam-beam deflection Change in beam separation [ µ m] Luminosity [arb. units] ] -2 1 p) 11 (10 LHC fill: 2520 -1 (Size of effect 0.8 ) [BC s = 8TeV exaggerated 2 n 1 0.6 for /(n vis µ demonstration) 0.4 0.2 0 3 data-fit data δ [ µ m] Nominal vertical beam separation δ [ µ m] σ True beam separation larger than nominal separation δ W. Kozanecki 28 Apr 2017

  20. Beam-beam corrections (2) 20 ! Two distinct beam-beam effects: beam-beam deflection and dynamic β ! bias σ vis if not corrected ! < 0.5% PbPb, 1 - 2% for 7/8/13 TeV pp and around 4% for 5 TeV pp ! The interaction of the two beams during a scan distorts the scan curve Beam-beam deflection Dynamic- β ] ] -2 1 -2 1 p) p) 11 11 (10 (10 LHC fill: 2520 LHC fill: 2520 -1 0.8 -1 0.8 (Size of effect ) [BC ) [BC s = 8TeV s = 8TeV exaggerated 2 2 n n 1 0.6 1 0.6 /(n /(n for vis vis µ µ demonstration) 0.4 0.4 0.2 0.2 0 0 3 δ [ µ m] δ [ µ m] 3 data-fit data data-fit data σ σ True beam separation larger Beams focus/defocus each other by an than nominal separation δ amount that is a function of separation W. Kozanecki 28 Apr 2017

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