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CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1 1 LHCb : what to do with the first month of data taking

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1 1 LHCb : what to do with the first month of data taking

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CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

1

LHCb : what to do with the

first month of data taking

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

2

Premessa

LHCb plans to set up a detailedstrategy for the detector and trigger startup over the coming years.My report summarizes the current ideas being discussed with some detector

and trigger experts and must be taken as a starting point

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

3

Outline

• detector and trigger general structure

• subsystems and calibration requirements

• trigger description and startup• a first look at physics

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

4

LHCb detector

p p

~ 200 mrad~ 300 mrad (horizontal)

10 mrad

Inner acceptance 10 mrad from conical beryllium beam pipe

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

5

LHCb vertex region

VErtex LOcator around the interaction region, verticesreconstruction

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

6

LHCb tracking

Tracking system and dipole magnet: to measure angles and momenta (together with VeLo)

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

7

LHCb P-ID

Two RICH detectors for charged hadron identification

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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LHCb calorimeters

Calorimeter system to identify electrons,hadrons and neutralsand used in the L0 trigger

e

h

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

9

LHCb muon detection

Muon system to identify muons and used in L0 trigger

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Trigger strategy 40 MHz

HLT:Final state

reconstruction

CalorimeterMuon system

Pile-up system

VErtex LOcatorTrigger TrackerLevel 0 objects

(Muon)

Full detectorinformation

Level-0:Level-0:ppTT of of

, e, h, , e, h,

Level-1:Impact parameterRough pT: (p)/p~ 20%

200Hz

1MHz

40kHz

•Level-0 : Use large B mass signaturehardware system with fixed latency (4s)

•Level-1 : use B mass and lifetime signatureSoftware analysis on reduced data from only few detectors. Run on a PC farm in common with HLT(~ 1800 CPU total)

•High Level Trigger (HLT):Software.The complete event is reconstructed with almost final accuracySelection of interesting physics decays

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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VertexLocator

- Silicon detector - 21 stations with

alternated R-segmentation

- sensitive area starts at 8mm from the beam

- retractable to 3cm during refill (the two halves open along the horizontal axis)

- used in L1 trigger: initiate tracking to compute IP and Pt

2 Pile-Up layers (only r sensors)to veto multiple interactions at L0

Interaction point z=5.3cm

~ 1m

~10cm

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Top view of the VeLo system

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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VeLo structure: R- sensors

Pitch 40-103m

Stereo angle 10 ° -20 ° 45° sector

Pitch 35-97m

R:

yx

yx

• angular coverage of each half disc = 182o

• total # channel ~170.000 • analogue readout

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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VeLo alignment figures

- Silicon strips are positioned on disc halves with <5m

- relative position of disc halves, within a half VeLo, surveyed before installation at x), y~ 5m, z)~ 20m precision in air and at room temperature.

to be checked on beam with tracks since vacuum and cooling may affect it

Goal is an hardware alignment of x), y~ 20m for L1 trigger to work- since VeLo retracts at each machine refill the two parts are re-positioned with a precision of <~100m , this can be checked with a few seconds of data taking thanks to small overlapping surfaces- final transverse software alignment precision for

event reconstruction ~ 5m

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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VeLo test beam activity before installation

A complete Half VeLo module should be tested on 120 Gev beam

- measure, and physically correct, misalignment among half discs

- full test of vertex reconstruction capability (target placed in front of the velo to simulate interactions),including software

- this is very important for its own survival: at LHC startup beam position can be estimated by VeLo itself reconstructing primary vertices at its retracted position before getting close to it

(VeLo can also determine the beam position before collisions with beam-gas interactions)

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Tracking system

• 1 station upstream the magnet and 3 downstream

• dipolar magnet: Bl=4Tm(*)

• each station is composed of 4 layers : x,+5o,-5o,x

• TT: silicon technology • T1-T3 mixed technology

(according to occupancy) Inner Tracker: silicon strips Outer Tracker: straw tubes

(*) installed&switched on successfully

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Tracking system: TT Station

• four layers: distance between 2 layers 30cm • total silicon area 4x2m2

• 183m pitch• Build with sensors each 9.6x9.4cm2 bonded to form strips 10cm–40cm long • 143,000 FE channels• used in L1

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Tracking system: T1-T3

IT

• silicon sensor: area 11x8cm2

• strip pitch 198m

• Max occupancy 1,5% • 130,000 channels

OT

45 0

• Two straw tubes (5mm Ø) layers staggered by 5.25mm for no dead space • 56,000 channels

• Resolution ~ 200m with drift-time measurement • Occupancy max < 7%

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Trackers alignment Silicon trackers• strips positioned with ~5m• positioning precision of detector boxes at

survey~1mm • relative precision needed at L1 for VeLo-TT

~<200m, to be done with first tracks• final software alignment aims at about 10m for

complete event reconstruction

Straw tubes• installation precision at survey ~1mm• working without drift time information at the beginning (m),more ghosts but pattern recognition with reasonable efficiency possible.Found tracks used for alignment and r-t calibration

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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RICH system

2 Rich with 3 Cherenkov radiators

Need of PID in large p range 3-100 GeV

P threshold (GeV)

Aerogel C4F10 CF4

0.6 2.6 4.4

K 2.0 9.3 15.6

RICH1 RICH2

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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RICH mirrors alignment(1)

• RICH system is used in the offline analysis (its use in HLT is under development)

• Rich1 has 4 spherical+ 16 flat mirror segments• Rich2 has 58 spherical and 40 flat mirror segments

Mirror tilts can affect the resolution on the Cherenkov angle

Software corrections are possible with a precision of 0.1 mrad provided a mechanical precision of 1 mrad

is obtained during mounting (attainable with laser alignment). This limits the fraction of photons which cannot be attributed unambiguously to one mirror

(for which no correction possible) avoiding the

deterioration of PID performance. Alignment is much more critical for Rich2

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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RICH mirrors alignment(2)

Need for a working tracking, ~1k well reconstructed tracks/mirror needed,<~100Kevents

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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ScintillatingPadDetector&PreShower : two 15 mm scintillating pad

layers + 2.5X0 lead in between

Electromagnetic calorimeter: “shashlik” 2mm lead + 4mm scintillator , 25Xo

(E)/E=10%/√E 1.5%

Hadronic calorimeter.: iron-scintillator plates , 5.6

(E)/E=80%/√E 10%

Calorimeter system(1)

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Calorimeter system(2)

5952 ch

4 cm

12 cm

6 cm26 cm

13 cm

1468 ch

SPD : multiplicity, e/separationPreShower: e/h separationECAL: e, E,Et) measurement

}HCAL: hadrons (E,Et)

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Calorimeter calibration

• Ecal modules pre-equalized with cosmics• Hcal modules pre-equalized with 137Ce• a sub-sample is energy-calibrated on

test-beam, calibration transported on the whole detector with momentum well reconstructed tracks

• PM gain stability monitored with pulsed LED ( checked with photodiodes). This serves also as signal time synchronization

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Muon system(1)

• 5 Stations + 4 iron filters

• 1380 chambers: 1368 MWPC + 12

GEM => 435m2 • trigger imposes high

efficiency/station since 5 stations/5 are required

(>99%) 4 (2 in M1) gas gap ORed (each gap has >~95%),

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Muon system (2)

• Large (10x8x7 m3) system• 120K FE channels ORed to form 26k logical channels sent to L0/DAQ• Up to max 48 physical channels make up a logical channel • Granularity: Min 6.3x31.3 mm2 (M2R1) Max 250x310 mm2(M5R4)

One quadrant of Station 2

A high precision space alignment is not needed for the muon system but……

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Muon system time alignment(1)

.... an accurate time alignment is mandatory to ensure high L0 muon trigger efficiency

MWPC time spectrum of one physical channel (OR of 2 gaps) with cosmics.

25 ns

If not well centered significant losses are

possible

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Muon system time alignment(2)

Muon electronics is designed to providesynchronization tools:

ASD chip(Carioca)

DIALOG(*) chip

FE board

SYNC chip

ODE boardThe SYNC chip accumulates hits from the FE - in BX bins (25ns) - inside the BX with a 1.5ns resolution TDCWith SYNC histogramming facilities the total signal shift can be determined as M*25ns+K*1.5ns- M is corrected on the SYNC itself while K is corrected with an adjustable delay present on the DIALOG chip

(*) DIALOG performs the logic OR to form logical channels

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Muon system time alignment(3)Coarse alignment: hits in 16BX around the beginning of a full bunch crossing sequence whose timing is given by the accelerator (16 entries/LHC orbit) 16 cycles

BX identifiedResidual misalignment

BX number

Before FTO correction

BCn+2 BCn+3 BCn+2 BCn+3

Phasemeasurement(25 ns gate)

On-chip histogram

BCcycle

FTO determinationand correctionvia front-end

ProgrammableDelays

(DIALOG chip)

FT alignment

Statistics in ~1h

Statistics in <~1hFine alignment

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Muon system time alignment(4)

Peak position for 16 FE ch forming 1 logical channel

5 ns25 ns

It might be not true for logical channels formed by signals coming from different chambers

• no muon trigger needed (all hits are usable)• no DAQ needed, histogram analysis through ECS• alignment possible at the physical channel level (masking facility in DIALOG chip). In principle, in fact, each FE channel must be independently centered in 25ns. Cosmics test shows, however, that FE channels inside a logical channel are in time within < 5 ns

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Muon system time alignment(5)

After L0 has started (even with reduced efficiency)refinement can be done with offline analysis requiring channels with a muon hit (TDC information in DAQ)

All hits

Muon hitsMC

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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L0Trigger

>90% K decay

Nominal threshold

HCAL clusters

•Select local maxima in ECAL and HCAL towers•Use SPD and PS to separate e//h

MuonCalo

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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L0 Trigger(2)

HC

al dom

inate

s

Muon d

om

inate

s

EC

al dom

inate

s

ZB ZA

RB

RA

ZPV

2 silicon R-stations

Possible cut:retain >98% of single and reject ~60% of multipleGain of 30-40% of single bb-events at optimal luminosity

PileUp veto (to reject multiple interactions) L0 result.

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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L1 Trigger - track reconstruction in VELO

Velo 2D reconstructionPrimary vertex search

VELO sensor design optimized for fast track finding: B’s move predominantly along beam-line

impact parameter in RZ-view

1. Straight line search in R-Z view, forward and backward tracks

~ 58 (+ ~30 backward) tracks1. Vertexing, σZ ~ 60 μm, σX,Y ~ 25 μm2. Select tracks with high impact parameter, 0.15 to 3 mm

about 8.5 per event3. Full space tracking for those tracks4. Extrapolate 3-D VELO-tracks to TT, use fringe field for P

estimation dp/p=20-40% , (B-tracks)=94%

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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L1 Trigger–match large IP with L0 candidates

Match with high Pt L0 calo and muon tracksStudy ongoing to include muon information

Signal/background separation by

Pt and impact parameter

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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HLT Trigger

•Confirm Level-1 decision– Complete Velo 3D tracking– Primary vertex search– Select from the 3D Velo

the large IP tracks , measure accurately the momentum, confirm the decision (same variable)

• Extend Velo tracks across the magnet (p)/p ~ 0.6 %

• Gain a factor 2-3 without significant loss• Fraction of CPU time

budget

Input95% confirmed

• Physics selection (including lepton–ID but not Rich ,yet) It has been checked for a few representative channels that a loose exclusive selection brings the rates down to 10-20 Hz per channel

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Trigger startup(1)Assumptions:• the subsystems are commissioned prior to data taking with

the LHC beam ( noise, missing channels etc)• one circulating beam cannot be easily used since earlier

beam is most likely in the wrong direction but it can be helpful for VeLo

• something can be done with beam-gas interactions when the two beams circulate (alignment of the tracking elements).

• we have assumed we will use the first collisions

5

2

Ncoll/BX

R(MHz)

LHC scenario: L~1032cm-2s-1

75 ns bunch spacingE beam=6 TeV ~ 5-6 MHz with>=1 collisions 0 1 2 3 4 5

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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The transfer line with the right direction (TI2) will be installed in 2007

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Trigger startup(2)

• Muon system time is aligned as described • VeLo system is retracted • Calo system is operational• Set-up an interaction trigger with minimum energy released in HCAL and/or multiplicity in SPD. (SPD can be used also to select particularly “clean” events)Take minimum bias data O(106) and check of: - m.b. rate - measure beam position with VeLo retracted - check correct functioning of L0 triggers - measure Pt distributions at L0, rates.vs.Pt cut - when VeLo closed, pile-up veto efficiency can be checked - take data also with magnet off to perform relative of tracking elements : aim at an alignment sufficient to let L1 work

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Trigger startup(3)

L1 switched on• check IP distributions• check capability to match high Pt tracks• check L1 and HLT rates

A large fraction of the data processing during this startup

phase could be done by the L1/HLT CPU farm at the pit, assuming the ~full CPU power is available at t0

Finally, as soon as we have a reasonable trigger, we can

start taking useful data and first signal to look for is obviously J/

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Look for J/

J/ is selected with a dedicated dimuon trigger

2 VeLo tracks coming from a common vertex and connected to 2 L0muon candidates (Pt1+Pt2)>1.3GeV no IP cuts, Minv window around J/mass

We can have a ~70Hz of J/ signal after L0&L1&HLT(*) with B/S~2-3

(*) J/ HLT

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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J/• If we are lucky a J/ sample of ~3x107 could be

gathered in 2 weeks running with a J/trigger

• With it we can do a more precise tracks momentum calibration using J/mass and vertex

Once the detector is well aligned and calibrated we may

start to look at physics: (J/promptmb- a lot of b’s J/X Pythia gives: J/bJ/prompt~ 5% (CDF probably effect of cuts ~1.5Mevts b J/X

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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J/

• Dimuon Trigger: Pt > 1.5 GeV per • ~2 million psi• ~80% prompt ~20% B

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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bJ/Statistics of some interesting B decay channels assumingnominal detector performance

Channel J/ident Full ev.rec.

B0 J/Ks0

BRvis=1.9x10-5

15Kevts 5Kevts

B0 J/K*0 (K)BRvis=5.9x10-5

45Kevts 14Kevts

B+ J/K+

BRvis=6.8x10-552Kevts 37Kevts

B+ c J/+

BRvis <=6.8x10-4

<=1Kevts

<=500evt

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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B0 J/K*0 (K)• Control process, no CP violation• B oscillation could be seen (with some tagging efficiency, maybe only )

Stat.err. only, nominal tagging,no Bg (B/S=0.37)

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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B+ J/()K+

• Tagging check• Lifetime check (no IP bias in this

sample)

B+c J/+

•Very clean peak at 6.4 GeV•Never observed

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Conclusions

• A detailed startup procedure will be established in the coming years

• Trigger startup, sub-detectors calib. & align. (even if not final) feasible in the first month

of data provided a lot of work is done before, also on test-beams

• Part of this work can be done without offline analysis, while the rest implies data taking and full reconstruction

• Some “not really physics results but showing our capability of doing physics can be achieved”

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Backup

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Trigger: possible improvement

• There is an on-going study to increase to ~ 2kHz the events rate to DAQ.

• 200Hz as baseline strategy + ~2kHz of events with a muon with high impact parameter

• On muon ”highway” triggered events b content ~ 50%• Gain a sample of unbiased b (the companion of triggering b-

>)– useful for systematic study– Inclusion of b decay not easy to trigger on– Inclusion of b decay not of interest now but maybe in the

future…

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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VELO

Primary vertex resolution in bb events: and || to the beams

z=44mx-y=8m

IP=14+35/pT

Impact parameter resolution vs 1/PT

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Vertex Locator

Primary vertex resolution in bb events: and || to the beams

z=44mx-y=8m

IP=14+35/pT

Impact parameter resolution vs 1/PT

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Track finding strategy

VELO seeds

Long track (forward)

Long track (matched)

T seeds

Upstream track

Downstream track

T track

VELO track

Long tracks highest quality for physics (good IP & p resolution)Downstream tracks needed for efficient KS finding (good p resolution)Upstream tracks lower p, worse p resolution, but useful for RICH1 pattern recognition

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Tracking performance

Ghost rate < 4% Pt>0.5GeV

Eff=94%

P>10GeV

p/p = 0.35% – 0.55%

Momentum resolution

Ghost rate

Track finding efficiency

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Rich Particle IdentificationBs->KK decay

<(K->K)> = 88%

< (->K)> = 3%

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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KS reconstruction

DD =54%

LL =75%

LU =61%

Ks decays •inside Velo(25%) (LL+LU)•between Velo TT(50%)(DD)•behind TT (25%)

Only first 2 cases reconstructed

Low momentum track swept out by the magnet: (U type track) poor p resolution

When both tracks are reconstructed the selection is reasonably efficient

CSN1, 16 Novembre 2004 Roberta Santacesaria, INFN Roma1

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Flavour tagging

sources for wrong tags:Bd-Bd mixing (opposite side)b → c → l (lepton tag) conversions…

Tag Tag

(%) w (%)

eff (%)

Muon 11 35 1.0

Electron 5 36 0.4

Kaon 17 31 2.4

Vertex Charge

24 40 1.0

Frag. kaon (Bs)

18 33 2.1

Frag (B) 0.7

Combined B0 (decay dependent:Combined Bs trigger + select.)

~4.7

~6

effective efficiency:

eff = tag (1-2wtag )2