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proposal2007_draft09.. - Henry A. Rowland Department of Physics ...

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data but needs the same database infrastructure that must be developed for the standard algorithm.<br />

The template algorithm is based upon the premise that the Pixelav simulation/electric field model<br />

can be tuned to accurately describe the pixel sensors as they are gradually damaged by exposure to<br />

the large LHC radiation field. This premise rests upon the demonstrated success in the modeling<br />

<strong>of</strong> charge collection pr<strong>of</strong>iles measured with test sensors irradiated to several fluences. The actual<br />

calibration procedure is to repeat the beam test measurements in-situ in CMS. This requires that<br />

samples <strong>of</strong> large-η tracks and pixel clusters be recorded at a series <strong>of</strong> pixel bias voltages. It has<br />

already been shown that, due to displaced primary vertices, it is possible to acquire such samples<br />

even in the central barrel modules. We are planning to develop a suite <strong>of</strong> CMSSW s<strong>of</strong>tware packages<br />

to facilitate this. The template calibration will be a continuing responsibility <strong>of</strong> the JHU group<br />

after LHC operation begins.<br />

Pixel Hit Validation The template-based reconstruction technique performs chisquare fits<br />

<strong>of</strong> the projected cluster shapes to simulated shapes. Goodness-<strong>of</strong>-fit information is generated and<br />

can be used to determine the consistency <strong>of</strong> the measured projections with the expected shapes.<br />

There are two distinct uses for this information. The first is to validate that the cluster is likely to<br />

have been produced by the transit <strong>of</strong> primary charged particle. In the region 2.25 < |η| < 2.5, about<br />

20% <strong>of</strong> all clusters are caused by secondaries and after track finding, about 8% <strong>of</strong> all muon tracks<br />

contain a hit generated by a secondary particle. These are entirely eliminated by the application<br />

<strong>of</strong> template probability cuts <strong>of</strong> 10 −3 . A second use <strong>of</strong> the goodness-<strong>of</strong>-fit information is to test<br />

angle hypotheses during track seed generation. Pixel track seeds contain two or three pixel hits<br />

and define track angles at each detector element. The template probabilities can be used to test<br />

the consistency <strong>of</strong> these angles with the observed clusters. The elimination <strong>of</strong> inconsistent seeds<br />

before the very cpu-intensive track-finding algorithm is invoked has the potential to significantly<br />

reduce the computing resources needed for track reconstruction.<br />

Fehling has recently begun to study the application <strong>of</strong> the template probabilities to seed-finding.<br />

This has the advantage that it eliminates pixel hits due to secondary particles at the earliest stage <strong>of</strong><br />

track finding in addition to reducing the computing resources needed for track reconstruction. His<br />

initial finding suggests that this procedure can reduce the total seed count by a factor <strong>of</strong> three with<br />

an efficiency larger than 98.2% (it’s possible that the lost tracks are “fakes”). Careful study and<br />

optimization are needed before the scheme can be used in the default CMS track reconstruction.<br />

Higher Level Trigger The second-level or Higher-Level Trigger (HLT) uses pixel triplets<br />

as primitives in the definition <strong>of</strong> various triggers. Pixel tracks are a crucial part <strong>of</strong> HLT triggers<br />

that identify τ-leptons and b-quarks in the final state. New postdoc Rappoccio is taking over<br />

maintenance <strong>of</strong> the trigger path designed to find two-τ final states from Z bosons and from neutral<br />

Higgs-boson-like states. This trigger is also a natural place to test the influence <strong>of</strong> the template algorithm<br />

which has already been shown to improve the impact parameter resolution <strong>of</strong> reconstructed<br />

tracks [301].<br />

Template-Based Pixel Simulation We know that the performance <strong>of</strong> the pixel tracker will<br />

be significantly degraded by radiation damage for much <strong>of</strong> its useful lifetime. This will adversely<br />

affect many physics analyses and it will be essential that the CMSSW simulation reflect the degraded<br />

pixel performance. We have established that the Pixelav simulation can simulate irradiated sensors<br />

but it requires approximately 1.5 s per cluster on a 2.5 GHz G5 processor and more than 3 s per<br />

cluster on a 2.8 GHz Xeon processor (due to an inferior vector processing architecture). The <strong>of</strong>ficial<br />

CMSSW pixel simulation adequately models unirradiated sensors with a simplified charge drift<br />

model and requires only about 12 ms per cluster on the 2.8 GHz Xeon processor. In order to retain<br />

the speed <strong>of</strong> the CMSSW simulation and achieve the accuracy <strong>of</strong> the Pixelav simulation, Swartz<br />

9

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