Download presentation
Presentation is loading. Please wait.
Published byBeatrice Lee Modified over 9 years ago
1
Fast and Precise Luminosity Measurement at the ILC Ch.Grah LCWS 2006 Bangalore
2
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 2 Overview The forward region Luminosity measurement using LumiCal Requirements Systematics Physics background Fast luminosity monitor – BeamCal Using the pair background signal Beam parameter reconstruction Summary and outlook
3
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 3 Forward Region – New Geometry 20mrad geometry (LDC)
4
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 4 Forward Region - Tasks LumiCal (26 (43) mrad < θ < 153 mrad) Detection of low p T em interacting particles Measure bhahba particles with high precision BeamCal (5.6 mrad < θ < 28 (46) mrad) Detection of low p T em interacting particles Measure and analyse the deposition from pairs originating from beamstrahlung. LHCal (new idea) Low angle hadron calorimeter PhotoCal (not drawn on this picture) Analyse beamstrahlung photons in the range of ~100μrad Minimize background from backscattering from pairs. 20mrad 2mrad
5
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 5 Backgrounds (Old 20mrad Geometry) 20mrad DID backscattering from pairs hitting the LumiCal edge (K.Büsser) Sketch of old BeamCal geometry. Projection of LumiCal‘s inner radius. Energy deposited in LumiCal from pairs.
6
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 6 LumiCal Requirements: Events θ (rad) Bhabha scattering Energy (GeV) Events BHWIDE generated events precision by:
7
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 7 Detector Performance Detector performance can be included into MC. How well we have to know? R.Ingbir
8
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 8 Systematic Effects Changing the detector position without Including bias & resolution Headon, 14,20 mrad X-angle outgoing beam 14 mrad X-angle detector axis 20 mrad X-angle detector axis
9
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 9 Compensating Systematic Effects by MC X (cm) Y (cm) 20mrad X-angle Detector axis Before correction after correction ΔL/L~10 -2 ΔL/L~10 -3 This is assuming knowing in perfect precision many parameters ! So far these effects are all considered individually, so be careful!
10
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 10 Physics Background Four-lepton processes are the main source of physics background for luminosity measurement Simulation of e + e - -> e + e - l + l - (l=e, μ, τ) background with WHIZARD and Bhabha signal with BHLUMI detector simulation BARBIE for track hitting detector frontface (generated track information was used) M.Pandurović/I. Božović-Jelisavčić Energy [Gev] [deg] Energy and polar angle of background ≈10 -3 tracks/BX LUMICAL BEAMCAL LUMICAL BEAMCAL
11
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 11 Background Suppression background can be effectively surpressed x [cm] y [cm] signal/background before (top) and after applying the selection cuts (bottom)
12
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 12 BeamCal BeamCal: 4 < θ < 28 mrad (headon) 15000 e + e - per BX => 10 – 20 TeV ~ 10 MGy per year “fast” => O(μs) Direct photons for θ < 400 μrad (PhotoCal) e + e - pairs from beamstrahlung are deflected into the BeamCal e+e+ e-e- Deposited energy from pairs at z = +365 (no B-field)
13
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 13 New Geometry 20mrad DID (R i (LumiCal) = 10.0cm at z=2270mm) (R o (BeamCal) = 16.5cm) 20mrad AntiDID (14mrad seems necessary for AntiDID) An AntiDID configuration is close to the headon/2mrad design. BUT better be prepared for both possibilities.
14
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 14 Fast Luminosity Monitoring Why we need a fast signal from the BeamCal? We can significantly improve L! e.g. include number of pairs hitting BeamCal in the feedback system Luminosity development during first 600 bunches of a bunch-train. L total = L(1-600) + L(550600)*(2820-600)/50 G.White QMUL/SLAC RHUL & Snowmass presentation position and angle scan Improves L by more than 12% (500GeV)!
15
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 15 Beamstrahlung Pair Analysis A lot of information is stored in the energy distribution of beamstrahlung pairs hitting BeamCal. Observables (examples): total energy first radial moment thrust value angular spread E(ring ≥ 4) / Etot E / N l/r, u/d, f/b asymmetries detector: realistic segmentation, ideal resolution, bunch by bunch resolution Beam parameters σ x, σ y, σ z and Δσ x, Δσ y, Δσ z x offset y offset Δx offset Δy offset x-waist shift y-waist shift Bunch rotation N particles/bunch (Banana shape)
16
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 16 Analysis Concept Observables Δ BeamPar Taylor Matrix nom = + * Beam Parameters determine collision creation of beamstr. creation of e + e - pairsguinea-pig(D.Schulte) Observables characterize energy distributions in detectorsFORTRAN analysis program (A.Stahl) and/orGEANT4 1 st order Taylor- Exp. Solve by matrix inversion (Moore-Penrose Inverse)
17
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 17 Coefficients of the Taylor-Matrix beam parameter i [au] observable j [au] parametrization (polynomial) 1 point = 1 bunch crossing by guinea-pig slope at nom. value taylor coefficient i,j
18
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 18 Analysis for nominal ILC Parameters ILCNOM, 20mrad DID Quantity Nominal Value Precision oldnew xx 553 nm4.82.9 xx 3.97.4 yy 5.0 nm0.10.2 yy 0.10.4 zz 300 m8.5 zz 6.76.3 yy 02.00.6 single parameter analysis
19
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 19 2mrad and 20mrad Analysis Quantity Nominal Value Precision 2mrad20mrad20mrad (2par) xx 553 nm3.12.92.8 xx 5.27.47.6 yy 5.0 nm0.30.2 yy 0.30.4 zz 300 m4.88.511.1 zz 3.76.37.4 εyεy 40x10 -9 mrad1.72.95.2 εyεy 04.24.14.7 xx 17.79.310 yy 00.50.6 N2x10 10 0.01 NN 0 0.020.03...
20
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 20 BeamCal Geant4 Simulation Need precise simulation for showering/realistic bfield map. Includes: flexible geometry (beam crossing angle, layer thickness, variable segmentation, calorimeter tilt) simplified DiD/antiDiD magnetic field input – GP generated e+e- pairs output – root tree with energy distribution in segments 1 BX ~ 200min @ 2.4 GHz CPU Shower visualization Energy/Layer distribution A.Sapronov
21
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 21 G4 Simulation with simplified B-field σ z, μm 20mrad DID 20mrad AntiDID Deposited energy in sensor layer all layers layer8
22
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 22 Using Bfield Map All layers Layer 8 Energy deposited in the sensors of the forward BeamCal.
23
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 23 Summary Redesign of the forward region has been done to cope with 20mrad DID (worst case). LumiCal Investigated physics and selection cuts to effectively reduce background. Investigated systematic effects (displacement, resolution, bias....)...and recommend LumiCal to be centered around outgoing beam. A luminosity measurement of ΔL/L ≈ 10 -4 is feasible so far. BeamCal Intratrain feedback of BeamCal has the potential to increase the luminosity significantly. A fast beamdiagnostics has potential to access many beam parameters (intratrain). This is also feasible for 20mrad. Have set up a G4 simulation of BeamCal for realistic shower development and for realistic b-field map.
24
LCWS2006, Bangalore Ch.Grah: Luminosity Measurement 24 Outlook LumiCal: extend background study by detector simulation, crossing angle LumiCal Geant4 simulation for both design, pad and strip version, are in work Use the BeamCal G4 simulation for the beamdiagnostics Choose a subset of the detector information for the analysis Detector & Readout R&D => talk by W.Wierba (DAQ session) Find more details at: http://www.ifh.de/ILC/fcalhttp://www.ifh.de/ILC/fcal
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.