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Sridhara Dasu (Wisconsin) @ CMS101 1 18 June 2008 Introduction to CMS Trigger Sridhara Dasu, University of Wisconsin, CMS Collaboration

Introduction to CMS Trigger

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Introduction to CMS Trigger. Sridhara Dasu, University of Wisconsin, CMS Collaboration. The Large Hadron Collider. Low P T g , e, m. Low P T leptons. Low P T B, t jets. Missing E T. Multiple low P T objects. ~ give up to dedicated experiment, LHCB. High P T leptons and photons - PowerPoint PPT Presentation

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Page 1: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 118 June 2008

Introduction to CMS TriggerSridhara Dasu, University of Wisconsin, CMS Collaboration

Page 2: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 218 June 2008

The Large Hadron Collider

Page 3: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 318 June 2008

Physics in LHC Era

• Electroweak Symmetry Breaking Scale– Higgs discovery and higgs sector characterization– Quark, lepton Yukawa couplings to higgs

• New physics at TeV scale to stabilize higgs sector– Spectroscopy of new resonances (SUSY or otherwise)– Find dark matter candidate

• Multi-TeV scale physics (loop effects)– Indirect effects on flavor physics (mixing, FCNC, etc.)

• Bs mixing and rare B decays– Lepton flavor violation

• Rare Z and higgs decays• Planck scale physics

– Large extra dimensions to bring it closer to experiment– New heavy bosons– Blackhole production

Trigger ChallengeLow PT , e,

Low PT B, jets

Multiple low PT objects

Missing ET

Low PT leptons

High PT leptons and photons

Multi particle and jet events

~ give up to dedicated experiment, LHCB

Low 40 GeV

Page 4: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 418 June 2008

The LHC Trigger Challenge

• Physics at EWSB scale– 115 < Mhiggs < 250 GeV– Decays to , WW*, ZZ*

• 2- PT~20 GeV, Lepton PT ~ 40 GeV

• TeV scale supersymmetry• Multiple leptons, jets and LSPs

(missing PT), HT ~ 300 GeV• QCD Background

– Jet ET ~ 250 GeV, rate = 1 kHz– Jet fluctuations electron BG– Decays of , k, B muon BG

• Technical challenges– 40 MHz input fast processing– 100 Hz output physics selection– 109 events per year ≤102 higgs events

Page 5: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 518 June 2008

Multi Level Trigger Strategy

Level 1

•Coarse object identification

•Limited isolation

Page 6: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 618 June 2008

L1T Algorithms: tracking

– Link local track segments (in CSC) into distinct 3D tracks (FPGA logic)• Reconstruction in suppresses accelerator muons

– Measure pT, , and of the muon candidates in the non-uniform fringe field in the endcap iron (SRAM LUTs)

• Require 25% pT resolution for sufficient rate reduction– Send highest quality candidates for combination with other detectors (similar

algorithm for DT in barrel) and make final L1 trigger decision with pT cut

Page 7: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 718 June 2008

Calorimeter Trigger Geometry

EB, EE, HB, HE map to 18 RCT crates

Provide e/ and jet, ET triggers

Trigger towers: = = 0.087

HCAL

ECAL

HF

Page 8: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 818 June 2008

L1T Algorithms: e/

Triggers are mostly due to energetic 0s in em-rich jets

Page 9: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 918 June 2008

L1T: / Jet AlgorithmJets are real - however, difficult to get low pT jets

-jets are mostly fake

Page 10: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 1018 June 2008

Missing / Total ET Algorithm

20o

0o

40o

360o

……

-5 50

ET18 Ex

18

Ey18

ET2 Ex

2

Ey2

ET1 Ex

1

Ey1

ET MET

Strip ET sum over all LUT

For sums ET scale LSB (quantization) ~ 1 GeV is used

= 20o used instead of HCAL tower size: = 5o

L1 MET is easily spoiled by instrumental problems

Page 11: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 1118 June 2008

L1 Trigger System Production

BSCANASICs

PHASEASICs

MLUs

SORTASICs

EISO

EISO

SortASICs

BSCANASICs

PhaseASIC

RCT Receiver card RCT Jet/Summary card

RCT Electron isolation card• Custom ASICs

• Large FPGAs

• SRAM

• Gbit/s Optical links

• Dense boards

Optical links SRAM

FPGA

CSC Track-Finder

All L1 Trigger Hardware is installed

and is being commissioned

Page 12: Introduction to CMS Trigger

I. Mikulec: CRUZET1/CRUZET2 12

L1 DT trigger efficiencyCRUZET 1

same bx ±1 bx

[deg] [deg]

Bottom sectors seem to have lower efficiency due to cosmic rays stopped in the calo material

Runs 43439,43553

Page 13: Introduction to CMS Trigger

I. Mikulec: CRUZET1/CRUZET2 13

L1 DT trigger efficiencyCRUZET 2

same bx ±1 bx

[deg] [deg]

Internal DT trigger synchronization much better in CRUZET 2 as expectedSector 10, wheel -1 missing

Run 47011

Page 14: Introduction to CMS Trigger

L1 Calorimeter Triggers

HCALRCTGCTGT (tower > threshold)– Tested in CRUZET-II

Sridhara Dasu (Wisconsin) @ CMS101 1418 June 2008

Stuck bits

Noise Run

Page 15: Introduction to CMS Trigger

L1 Calorimeter Triggers

HCALRCTGCTGT (tower > threshold)– Tested in CRUZET-II

Sridhara Dasu (Wisconsin) @ CMS101 1518 June 2008

Noise Run

Page 16: Introduction to CMS Trigger

Calorimeter Triggers

HCALRCTGCTGT (tower > threshold)– Tested in CRUZET-II

Sridhara Dasu (Wisconsin) @ CMS101 1618 June 2008

Cosmics Run

Page 17: Introduction to CMS Trigger

Trigger Rates

Trigger rate during one of the CRUZET-II runs

Not all cosmics – lots of noise!

Muon (DT) trigger commissioning is farther along than calorimeters

Studying correlations between DT/RPC/CSC now

HCAL dominated by noise – but may still be acceptable for running

Detailed studies of MET etc. begin

ECAL also tried but not used in CRUZET-II

Sridhara Dasu (Wisconsin) @ CMS101 1718 June 2008

Total

Hcal

DT

CSCRPC

Page 18: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 1818 June 2008

The High-Level Triggers

In CMS all trigger decisions beyond Level-1 are performed in a Filter Farm running ~normal CMS reconstruction software on “PCs”

The filter algorithms are setup in several steps

HLT does partial event reconstruction “on demand” seeded by the L1 objects found, using full detector resolution

Algorithms are essentially offline quality but optimized for fast performance

Page 19: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 1918 June 2008

HLT Executable Structure

1 0 1 1 0 0 1 1 0 0 1 0 0 1 1 0 0 1 0 0 1 0 0

Step 1

Step 2

Step 3

Step 4

Step 5

Step 6

Step 1

Step 2

Step 3

Step 4

Step 1

Step 2

Step 3

Step 4

Step 5

Step 1

Step 2

Step 3

Step 4

Step 5

Step 6

0 10 0

128-bit L1 Word

HLT Bits…H

LT

Alg

orith

m S

teps

Pat

h st

ops

whe

n a

sele

ctio

n st

ep f

ails

e/

2 e/

ME

T

1-Je

t2-

Jet

e+Je

t

HT

Page 20: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 2018 June 2008

HLT e/ Selection• Initial steps using calorimeter (“Level-2 e/”):

– Search for matching Level-1 e/ object• Use 1-tower margin around 4x4-tower trigger region

– Bremsstrahlung recovery “super-clustering”– Select highest ET cluster

• Bremsstrahlung recovery:– Road along — in narrow -window around seed– Collect all sub-clusters in road “super-cluster”

basic cluster

super-cluster

Page 21: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 2118 June 2008

HLT -jet tagging

Final steps in HLT paths involve tracking which is more time consuming

Reconstruct tracks only in the region of interest around “Level-2” tagged objects

Page 22: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 2218 June 2008

HLT algorithm design

“Global” vs. “Regional”: All algorithms (except for Jets) regional by now

o Seeded by previous levels (L1, L2, L2.5)

Can benefit significantly by doing regional data-unpacking and local reconstruction across HLT

Have implemented regional ECAL unpacking/RecHit for Egamma and Muon trigger paths

Started planning (& development) of regional unpacking across rest of detectors, HLT paths

L1 seeds

L2 unpacking (MUON/ECAL/HCAL)

Local Reco (RecHit)

L2 Algorithm

Filter

L2.5 unpacking (Pixels)

L2.5 Algorithm

Local Reco (RecHit)

“Local”: using one sub-detector only“Regional”: using small (η, φ) region

HLT Framework Design & Implementation: Martin Gruenewald

Page 23: Introduction to CMS Trigger

Getting Ready for LHC

Sridhara Dasu (Wisconsin) @ CMS101 2318 June 2008

Parameters Beam levels Rates in 1 and 5

kb N * IP1,5(m)

Ibeam

proton

Ebeam

(MJ)

Lumi

(cm-2s-1)

Events/

crossing

Min bias rates

1 1010 11 1 1010 10-2 1.6 1027 << 1 90 Hz in ~104 Xing

43 1010 11 4.3 1011 0.5 7.0 1028 << 1 4 KHz in 5 105 Xing

43 4 1010 11 1.7 1012 2 1.1 1030 << 1 23 KHz in 5 105 Xing

43 4 1010 2 1.7 1012 2 6.1 1030 0.76 200 KHz in 5 105 Xing

156 4 1010 2 6.2 1012 7 2.2 1031 0.76 800 KHz in 107 Xing

156 9 1010 2 1.4 1013 16 1.1 1032 3.9 4 MHz in 107 Xing

Goal: be prepared for luminosities up to 1E32 Using two reference values (2E30, 2E31) for CSA08 exercise At lower luminosities take lots of minimum bias and some zero bias for detector debugging using towers over threshold in calorimeter

Page 24: Introduction to CMS Trigger

First Look at HLT for 4 1029

Trigger object L1 Seed HLT thresh [GeV] Prescale HLT Rate

[Hz]

Jet(MET)

L1_SingleJet15

L1_SingleJet30

L1_ETM30

30

60

30

10

1

1

15

55

15

Electron L1_SingleEG5 5 1 5

Photon L1_SingleEG5 10 1 33

Muon OR of All MuSeeds none 1 34

ALL 140

Large minimum bias and zero bias trigger events for debugging

Page 25: Introduction to CMS Trigger

2E30 / 2E31 Trigger Menu• Muons:

Single-muons above 5 GeV (11 GeV) Double-muons above 3 GeV (effective kinematic limit)

• Egamma: Single-relaxed electrons above 8 GeV (12 GeV) Double-relaxed electrons above 5 GeV (10 GeV) Single-relaxed photons above 15 GeV (25 GeV) Single-photons above 10 GeV with tracker-isolation (20 GeV)

• JetMET: Single-jets above 110 GeV (180 GeV) MET above 50 GeV (65 GeV)

• Plus: Prescaled triggers for lower energies/momenta (all flavors) Few Hz of minimum bias

Lowest-threshold unprescaled triggers

Page 26: Introduction to CMS Trigger

HLT CPU performance: 1E32

Average CPU-time to run all HLT paths: 44 ms

Overall:• No surprises• Additional speed-up improvements since last summer consumed by introduction of new triggers (60 → 110)• With new Filter Farm nodes we should be able to deal w/ L1 rate of 50 kHz even if HLT takes 100 ms/evt

Page 27: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 2718 June 2008

2007 HLT Exercise

HLT Timing is influenced by– Trigger menu (L1T & HLT)

• Determined by physics priorities• Instantaneous luminosity

– Chose to make a menu for 1032 cm-2 s-1

– Maximum luminosity in 2008

– Input L1Trigger rate• Parameters of various L1T algorithms, e.g., H/E• Limited by bandwidth safety factor to 17 kHz

– HLTrigger algorithms• Standard trigger paths at HLT seeded by L1 trigger bits• Order of modules and filters in a path• Parameters of the modules and filters

We settled on one setting for the 2007 HLT Exercise

Page 28: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 2818 June 2008

L1T Menu: Single + Double

L1TEmulator Developers +Werner Sun, SD, Pedram Bargassa

Page 29: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 2918 June 2008

L1T Menu : Mixed

L1T Menu– Optimized to fit in the budget and e/ thresholds yield

good W, Z efficiencies, but not – Jet thresholds low enough to

cover Tevatron range well– MET only L1T used at HLT in

combination with jets– Double and mixed triggers for

specific physics channels addedL1TEmulator Developers +Werner Sun, SD, Pedram Bargassa

Page 30: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 3018 June 2008

HLT Menu : + X

Rates: Pedram Bargassa

Juan Alcaraz Maestre, Adam Everett,Muriel Vander Donckt, …

Lotte Wilke

Meenakshi Narain, …

Vuko Briglevic

Greg Landsberg, Duong Nguyen,Len Christofek, Muriel Vander Donckt,Sylvia Goy Lopez

Page 31: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 3118 June 2008

HLT Menu: Jet MET

Len Apanasavich

Rates: Pedram Bargassa

Page 32: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 3218 June 2008

HLT Menu: e, , + X

Monica Vazquez Acosta,Marco Pieri,Alessio Ghezzi, …

Ian Tomalin

Greg Landsberg, Duong Nguyen,Len Christofek, Nadia Eram

Simone Gennai

Rates: Pedram Bargassa

Marta Felcini

Page 33: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 3318 June 2008

HLT Timing Table

Times: Tulika Bose

Page 34: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 3418 June 2008

HLT Times: Minbias

Time Plot: Tulika & Simone

Page 35: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 3518 June 2008

HLT Times: QCD + EWK + X

Time Plot: Tulika & Simone

Page 36: Introduction to CMS Trigger

Sridhara Dasu (Wisconsin) @ CMS101 3618 June 2008

SummaryLHC Trigger is Challenging

– The choice of physics studied is already made at level-1 trigger• Choices made with calorimeter and muon systems only

– Complete object reconstruction at higher level trigger• Optimum resolution online with calibration and alignment• Includes b/ tagging in high level trigger farms

– CMS has designed trigger systems for golden discovery modes (lepton, diphoton, muti-jets…)

• Startup triggers setup to restablish the Standard Model• Pickup searches for new particles where left off by Tevatron• Definitive exploration of higgs sector is assured

– Innovative designs may allow more measurements• Topological selection starting from level-1• Low mass higgs & some MSSM higgs decays to invisible higgs

Commissioning is underway– Steady progress in both L1 and HLT worlds– Configuration plans for luminosities evolution from startup to design-level