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Particle ID and baryon production asymmetries from LHCb Susanne Koblitz (CERN) on behalf of the LHCb collaboration 22 nd Rencontres de Blois 2010 15 th - 20 th July 2010

Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

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Page 1: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Particle ID and baryon production asymmetries from LHCb

Susanne Koblitz (CERN)on behalf of the LHCb collaboration

22nd Rencontres de Blois 201015th - 20th July 2010

Page 2: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 2 /21

VELO

collision point

Dipolemagnet

VELO

RICH2

RICH1

CALO

LHCb Detector Layout

Crucial for physics program:➢ excellent vertex resolution➢ PID: RICH for /K/p, calorimeters, muon system

A forward detector (2<η<5) for precision measurement of CP violation and rare B-decays: MUON

RICH2 CALO

Page 3: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 3 /21

C4F10 gas n=1.0014

Silica Aerogel n=1.03

CF4 gas n=1.0005

The RICH Detectors

RICH1: 25250 mrad vertical25 300 mrad horizontal

Angular AcceptancesRICH2: 150 mrad vertical15 120 mrad horizontal

Need good /K/p separation in momentum range between 1 and 100 GeV and good coverage of angular acceptance

2 Detectors, 3 Radiators!

Page 4: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 4 /21

RICH1 & RICH2: more details

RICH1 RICH2Detector Planes 2 (Horizontal) 2 (Vertical)

Photon Detectors 2×7×14 = 196 2×9×16 = 288

Flat Mirrors 16 40

Spherical Mirrors 4 56

➢ RICH2 rotated by 90°

➢ detectors planes outside tracking acceptance (flat mirrors)

Page 5: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 5 /21

RICH1 detector in action

Up Panel Photon Detectors

Down Panel Photon Detectors

Aerogel

C4F10 Gas Volume

Cosmic Track

Flat Mirrors

Spherical Mirrors

A charged track emits a cone of Cherenkov light on passing through the radiators (Aerogel & C4F10 Gas).

Mirrors focus these cones into rings on 2 banks of photon detectors positioned out of LHCb acceptance.

Cosmic event display

Page 6: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 6 /21

RICH 1LHCb data(preliminary)

Kaon ring

RICH 2LHCb data(preliminary)

Kaon ring

Nov/Dec 2009LHC beams √s = 900 GeV

RICH Event Display

RICH2LHCb data(preliminary)

Saturated Ring

RICH Event Display:Detected signals: Photon hits shown in yellow pointsInformation from reconstruction:Expected rings for given hypothesis and ray-traced photons shown in white lines and blue points

Page 7: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 7 /21

Particle Identification in the data

Φ KK !

with PID

LHCbPreliminary s=0.9 TeV Data

Φ KK ?

Without PID

LHCbPreliminary s=0.9 TeV Data

➢ for PID need to look at all tracks and photons at the same time

➢ maximize event likelihood for photon distribution by changing mass hypotheses for the tracks

➢ use mass hypotheses of best event likelihood

➢ to improve purity:require large change in the event likelihood for a change of mass hypothesis for a given track

Page 8: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 8 /21

Study of RICH performance

➢ preliminary calibration used in analysis

➢ loose PID selection➢ purity improved with

stricter cuts

➢ use known resonances to measure PID performance

➢ : , KS - decays➢ K:  decays with one

identified K➢ p: - decays

p mis-ID rate

Proton ID efficiency

Proton ID efficiency

p mis-ID rate

stricter PID

loose PID

LHCbPreliminarys=7 TeV Data

LHCbPreliminarys=7 TeV Data

Page 9: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 9 /21

Comparison with PID in MC

➢ only preliminary calibration and alignment used➢ very good agreement between data and MC

LHCbPreliminary s=7 TeV MC

Proton ID efficiency

p mis-ID rate

LHCbPreliminary s=7 TeV DATA

Proton ID efficiency

p mis-ID rate

Page 10: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 10 /21

Particle ID in calorimeters

➢ particle identification based on energy deposits in different calorimeters

➢ PID performance depends on energy resolution

➢ for electrons (E/p­cut):    90% efficiency and 5% mis­ID➢ very good agreement with MC

~ 7 MeV

Page 11: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 11 /21

The Muon System

➢ 5 tracking stations around hadron absorbers (~ 23

➢ Multi Wire Proportional Chambers (MWPCs) and Gas Electron Multipliers (GEMs)

➢ provides μ-ID with very high purity

Page 12: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 12 /21

-Identification

ε() = 97.3 ± 1.2 %

➢ extrapolate track to system and look for hits in -stations➢ a candidate needs several hits in region of track impact point➢ calculate probability based on hit distribution in -stations➢ performance studied with J/ for -ID ➢ use /K/p from decays to look at mis-ID rate

ε(mis) = 2.38 ± 0.02 % for

LHCbPreliminarys=7 TeV Data

DATA KSMC KS

LHCbPreliminarys=7 TeV Data

DATAMC

effi

cien

cy (

%)

p (MeV/c)

Page 13: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 13 /21

Baryon asymmetries

http://home.fnal.gov/~skands/leshouches-plots/

➢ Study of baryon number transport in pp-collisions➢ expectation for p & similar➢ baryon: sea-quark contribution➢ existing models tuned to lower energies

Page 14: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 14 /21

Event Selection

➢ at least 1 primary vertex in interaction region➢ select only good quality long tracks ➢ selection: p

➢ prompt pointing to primary vertex➢ selected by the Armenteros-Podolansky variable➢ RICH PID not used➢ combinatorial background in s reduced with cuts

on ratio of impact paratmeters (IPp·IP/IP) and on decay angle

➢ 2 data sets: s=0.9 TeV: 0.31nb-1 ➢ : 9224 and 6802

➢ s=7 TeV: 1nb-1

➢ : 45605 vs 41192

Page 15: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 15 /21

anti-Λ

Invariant Mass Distributions

Eve

nts

(0.3

5MeV

/c2 )

Eve

nts

(0.3

5MeV

/c2 )

Eve

nts

(0.3

5MeV

/c2 )

mp(MeV/c2)

Eve

nts

(0.3

5MeV

/c2 )

mp(MeV/c2)

mp(MeV/c2)

mp(MeV/c2)

LHCbPreliminarys=7 TeV Data

LHCbPreliminarys=0.9 TeV Data

LHCbPreliminarys=7 TeV Data

LHCbPreliminarys=0.9 TeV Data

Λ

Λ

Page 16: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 16 /21

Λ

Looking at - kinematics

LHCbPreliminarys=7 TeV Data

LHCbPreliminarys=0.9 TeV Data

LHCbPreliminarys=7 TeV Data

LHCbPreliminarys=0.9 TeV Data

● data

● data

● data

MC

● data

MC MC

MC

Page 17: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 17 /21

Measuring Baryon Asymmetries

➢ Determine raw asymmetries from number of observed particles and anti-particles in a given bin➢ use sideband subtraction to correct for background

➢ Correct raw asymmetries for:➢ Detector acceptance effects: efficiencies, material

interactions and more (from detector simulation)➢ Look at corrected asymmetries in bins of y and pT

➢ Main contributions to systematic errors:➢ Uncertainty in acceptance corrections taken from

Monte Carlo (material interactions)➢ Possible contribution from non-prompt and diffractive

baryon production (below percent level)

Page 18: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 18 /21

MC models:Perugia tunes do not include diffractionLHCb tune include diffraction (<1% after selection cuts)

Results for

➢ high energy data good agreement to MC

➢ low energy data significantly below MC

look at y(beam) - y()

--- LHCb MC

--- Pythia – perugia0 tune

● LHCb data

● LHCb data

--- LHCb MC

LHCbPreliminarys=7 TeV Data

LHCbPreliminarys=0.9 TeV Data

Page 19: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 19 /21

● STAR data – 0.2 TeV

● LHCb data – 0.9 TeV

● LHCb data – 7 TeV

Results for

n(

)/

n(

)

y=yBEAM – y

yBEAM=8.345 for 7 TeV   yBEAM=6.556 for 0.9 TeV 

y

Page 20: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 20 /21

Proton production asymmetry➢ use PID information from the RICH detectors to select 

protons cuts tuned to obtain purity>90% in acceptance➢ parallel analysis for /K and p➢ correct raw p and p rates for PID efficiency and purity

obtained from analysis of control channels➢ need to correct raw asymmetries for acceptance effects, in

particular material interaction➢ study contribution from diffractive

and non-prompt interaction➢ analysis being finalised,

full results at ICHEP

Page 21: Particle ID and baryon production asymmetries from LHCb · RICH1 detector in action Up Panel Photon Detectors Down Panel Photon Detectors Aerogel C4F10 Gas Volume Cosmic Track Flat

Susanne Koblitz, Talk given at the 22nd Rencontres de Blois, July 18th 2010 p. 21 /21

➢ Particle ID in LHCb is in very good shape➢ all systems show good performances in agreement

with expectations from Monte Carlo simulation

➢ measurement of baryon asymmetry for prompt production shown

➢ results for s=0.9 TeV show larger asymmetry than expected from MC predictions

➢ agreement of s=7 TeV data with MC is better

➢ measurement of baryon asymmetry for prompt p production being finalised

Conclusion