atlas data challenges the physics point of view ucl, september 5th 2001 fabiola gianotti (cern)

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ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

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Page 1: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

ATLAS Data ChallengesThe Physics point of view

UCL, September 5th 2001

Fabiola Gianotti (CERN)

Page 2: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

Three data challenges are foreseen: -- DC0 : end 2001 -- DC1 : first half 2002 -- DC2 : first half 2003 Computing TDR Goals : validate our computing model and our software Important physics content : provide data samples for physics studies and

hopefully many physics results How ?

Start with data which looks like real data need MC generators, G3/G4 simulation, event model, detailed detector

response (e.g. noise, cross-talk, etc.), pile-up Run the filtering/trigger and reconstruction chainStore the output data into the databaseRun the analysisProduce physics results

Page 3: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

DC0: November - December 2001

In principle should be a test of the WHOLE software chain : a kind of “rehearsal” for DC1 (check that everything works for DC1)

Issue is therefore not massive production of huge data samples

but few 100k events able to test the whole software chain Chosen physics sample : few 100 k Z+jet events, with Z

. -- allows tests of ALL sub-detectors (including b-tagging since 6% of jets are b-jets) -- idea is to produced several samples with the 3 general-purpose generators (PYTHIA, Isajet, Herwig) If you want to participate in DC1, you are (strongly)

encouraged to participate in DC0 as well.

Page 4: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

DC1: February - July 2002

Scope : stress-test the system with large-scale production, reconstruction and analysis Several samples of up to 107 events 10% data collected

at LHC in one year. Crucial issues :

-- simulation will be done mainly with G3 but it is important to perform smaller-scale production with G4 -- comparison G3/G4 (with same geometry, to be meaningful

…) -- learn about event model and detector description -- I/O performances : N events with different technologies -- pile-up treatment -- understand bottle necks -- understand distributed computing model / GRID (not

discussed here)

Page 5: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

DC1: Physics samples107 jets for e/jet separation studies in view of

Trigger/DAQ TDR (due end of 2002). ~ 10 times more statistics than “old jet production”. Study performance of ATHENA and HLT algorithms. Useful also for other physics studies (e.g. optimisation of jet energy reconstruction algorithm)

Any other CPU-consuming physics sample considered useful for physics studies. Mainly SM “background processes” : examples:

-- inclusive muon sample (for B-physics and muon performance studies), Zbb and Wbb samples (backgrounds to many searches), WW/ZZ samples

-- Z for tau-lifetime studies -- several samples with different generators to understand the physics of various MC

Physics groups and Combined Performance groups asked to prepare list of wishes first discussions at Physics Coordination in Lund and at October ATLAS week. Everybody is encouraged to make

suggestions

Page 6: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

DC2 : January - September 2003

Scope/precise goals: depend on the outcomes of DC0/1 Present goals: -- 108 events ( data collected in 1 LHC year) -- Geant4 should play a major role -- full test of calibration/alignement procedures and condition

database -- question : do we want to add part or all of DAQ, LVl1, LVL2,

Event filter ? Physics content: -- demonstrate capability of extracting and interpreting a signal from New Physics -- generate various SM samples and “hide” in each one a

different New Physics process (e.g. SUSY for one mSUGRA point, excited leptons, etc.). -- people will be asked to understand the nature and all possible features of the signal (without knowing a priori what it is)

Page 7: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

DC production : CPU and data size

~ 20 TB ~107~ 107DC1

~ 0.2 TB~105~ 105DC0

Total sizeTime hours SI95

Number of events

DC2~ 108 ~108 ~ 200 TB

Page 8: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

“Physics readiness document” (kind of Physics TDR prime … ) : LHC t0-1year

Content (examples): Work done with MC generators, the ATLAS MC library,

status/strategy for MC production Strategy for using different levels of simulation (full,

parametrisations, fast) for different processes Comparisons G4/test-beam data, FLUKA/test beam-data

systematics from full simulation Main figures of Physics TDR redone with new/final software Specialised packages needed for various physics studies

(e.g. MSSM scan packages for Higgs and SUSY with up-to-date theoretical calculations, etc.) etc.

Page 9: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

Status of the non-core software(my view, emphasis on “physics part”)

Main generators (PYTHIA, ISAJET, HERWIG) interfaced to HepMC (HERWIG being finalised …). Next : specialised generators (e.g. VECBOS, QQ) Simulation : -- G4 : physics validation not completed (lot of work done with EM

physics, hadronic physics being tested now); full ATLAS geometry

not yet in. -- DC0, DC1: use G3 plus smaller/restricted (e.g. to some detector parts) productions with G4 -- FLUKA : I am 100% sure with need it. I intitiated a pilot-project with Tilecal : G4 test-beam geometry input to FLUKA (first results in Lund). Then extend to other sub-detectors Intermediate simulation (e.g. shower/track parametrisation): I am 100%

sure we need it. Tried to find people over the last two years failed. Recently a couple of groups have shown some interest.

Page 10: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

ATLFAST OO (UK product): -- runs in ATHENA -- reads HepMC from Objectivity, writes output into Objectivity (and ntuples) -- first validation made. Further results in Lund (from “users-non- developers”) -- next steps: improve functionality (beyond ATLFAST fortran). E.g. : shower shapes ? Trigger simulation ? Parametrisation for B-physics ? C++/OO reconstruction: -- runs in ATHENA -- reads G3 hits/digis (Phyiscs TDR data) -- validation results in Lund

Less clear situation (to me ...) for : e.g. -- event data model -- detector description -- database , condition database, technology choice -- simulation framework vs ATHENA -- analysis tools (maybe premature today but one of the aims of DC’s should be validation of

analysis tools)

Page 11: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

Where could you contribute ?Lot of work to be done everywhere , of course ….

Examples: Improve understanding of ATLAS potential for physics (e.g. SUSY, Extra-dimensions, backgrounds) and detector performance (e.g. can we tag

charm-jets ?) by analysing data produced by DC’s. Improve reconstruction, algorithms, etc. (e.g. HLT, E-flow algorithm for jet reconstruction using ID+CALOs) Validation of MC generators: e.g. Which MC for which process ? For which processes do

we need more calculations and/or additional/specialised MC ? Validation of G4/FLUKA physics : comparisons with test-beam data (in particular nuclear

interactions) Validation of ATLFAST OO and new reconstruction against old/fortran ATLFAST and ATRECON Intermediate simulation (shower and track parametrisations) Detector response : hits digi (including noise, pile-up with correct time structure, efficiency, etc.)

Page 12: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

HLT-DC1 scenario

This has to be discussed with the HLT community but the basis could be similar to what has been done previously

Generation:Pt hard scattering > 17 Gev| | < 2.7 2 samples

1) e-candidate Et > 17 Gev, no , no • Grid 0.12 x 0.12

2) Jet-candidate Et > 40 Gev• Grid 1.0 x 1.0

A first selection is made at the level of the event generation

One keeps 14.5% of generated events • 14.4% for (1) and 2% for (2)

Page 13: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

HLT- DC1 scenario

SimulationThe remaining events are run through the full simulationThe Lvl1 trigger is applied at that level

One keeps 13.7% of the events• 97% for (1) and 10% for (2)

The pile-up is run for the remaining events means ~2% of the ‘generated’ sample

ReconstructionThen the events are run through Lvl2, Event Filter and offline reconstruction

Page 14: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

What next

Prepare a first list of goals & requirementswith

HLT, Physics community simulation, reconstruction, database communities people working on ‘infrastructure’ activities (bookkeeping)

to be discussed with A-team with CSG (July 24th meeting)

In order toprepare a list of tasks

• Some Physics oriented• But also like testing code, running production, …

define the priorities

Page 15: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

Then

Start the validation of the various components in the chain (putting dead lines for readiness)

SoftwareSimulation, pile-up, …

Infrastructure Database, bookkeeping, …

Estimate what it will be realistic (!) to doFor DC0For DC1

“And turn the key”

Page 16: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

The ATLAS Data Challenges Project Structure Organisation

ATLAS Data Challenges

CSG

DC Overview Board

DCExecution

Board

DCDefinition

Committee(DC2)

Work Plan Definition

WP

RTAG

WP WP WP WP

Reports

ReviewsNCB

Resource Matters

OtherComputing

GridProjects

DataGridProject TIERs

Page 17: ATLAS Data Challenges The Physics point of view UCL, September 5th 2001 Fabiola Gianotti (CERN)

Expression of interests

So far, after the NCB meeting of July 10th:Canada, France, Italy, Japan, Nordic Grid, Russia, Taiwan, UK

Proposition to help in DC0Proposition to participate to DC1Contact with HLT community

Contact with EU-Data-GRIDKit of ATLAS software