Ian Ross Rose-Hulman Institute of Technology Mentor: Dr. Richard Teuscher University of Toronto ATLAS Group ATLAS Calorimetery: Cosmic Ray Commissioning.

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Presentation transcript:

Ian Ross Rose-Hulman Institute of Technology Mentor: Dr. Richard Teuscher University of Toronto ATLAS Group ATLAS Calorimetery: Cosmic Ray Commissioning

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 2 Overview Cosmics in ATLAS Analysis: What to Look For and How to Find It –Example Runs and Events Cosmics as a Background –Spectrum of high energy hits and missing transverse energy Travel Acknowledgements

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 3 Cosmics in ATLAS: Why? Analysis of cosmic ray events provides valuable information about the status of detector modules and triggering mechanisms –Identify and tag malfunctioning cells –Ensure proper calibration and function of reconstruction software Determine frequency and impact of significant cosmic events as a background to beam collision events

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 4 Cosmics in ATLAS: A Superficial Explanation Data collection: Detector is left on, typically overnight Trigger: coincidence of high energy on both top and bottom of detector At best, there are 12 Φ modules on top and 12 Φ modules on bottom that can be used as triggers.

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 5 What Can Happen: Case 1 (Minimum Ionization)

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 6 What Can Happen: Case 2 (Hard Brem)

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 7 What Can Happen: Case 3 (Air Shower)

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 8 Analysis - The Basic Process Data is stored in raw format, then converted to more amiable ntuple (through Athena) Distribution of energy across detector is examined to find and cut malfunctioning cells Use ROOT to find and characterize high- energy events Events are reconstructed for further examination (through Atlantis or other event displays)

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 9 Example: Run Plot displays how many times during the run a cell reported an energy of >400 MeV Cells in lower left are malfunctioning: way too many high-energy events LBC41 – Known problem cell that has since been fixed

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 10 Picking out the Cosmics Malfunctioning cells are removed, and a histogram holding every cell’s energy for every event is constructed. Outlying events often indicate cosmic ray hits. Mostly brem hits, but also fireworks (cosmic air showers) Cosmics still exist lower at lower energies, but sometimes hide among noise and must be combed out. (MeV)

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 11 Ex. Hard Brem – Event 776 from Run Bad cell (LBC41) Bremsstrahlung hit Liquid Argon pulse Tile Calorimeter pulse Cosmic ray strikes detector and slows down, radiating energy as it does so

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 12 Ex. Fireworks – Event 3481 from Run Air shower event Cosmic ray collides with air particle, causing a cascade of energetic particles to shower over the detector Much rarer than Brem hits. 773 GeV spread across entire active detector Largest single hit was 73 GeV

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 13 PMT Saturation – Event 1630 Run Tile LBC41: known to be malfunctioning during the run Enormous amount of energy in this cell! PMTs are saturating! LBC15 B5 TILE cell: id = 5/1/-1/14/4/1/0/0 E Max = GeV ET Max = GeV ET Sum = GeV η = ±.1000 Φ = 81.6 ± 5.6°

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 14 Saturation Event Saturation occurs at 1023 ADC counts Calibration fits pulse, de-weighting the saturated samples by assigning them with a very large error in the fit

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 15 Pulse shape of neighbors indicates real physics hit 1.13 GeV GeV 0.58 GeV 0.43 GeV 2.87 GeV 0.79 GeV

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 16 More Neighbor Evidence LBC15 B6 TILE cell: id = 5/1/-1/14/5/1/0/0 E Max = GeV ET Max = GeV ET Sum = GeV η = ±.1000 Φ = 81.6 ± 5.6° The next cell (in Eta) also recorded a significant pulse for this event

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 17 Cosmics as a Background We would like to know how often high energy cosmics will appear as a background in ATLAS events of interest. More specifically, we would like to know what kind of effects these cosmics may have on the transverse energy balance. Sam Posen and I have constructed a spectrum to get an idea of how frequently cosmics could potentially disrupt ATLAS

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 18 Why ETransMiss? Barring any new physics, events in the LHC run should have balancing transverse energy and momentum. –Missing transverse energy can imply exotic new physics (like SUSY!) Cosmic rays can disrupt this balance, potentially leading to ‘fake’ ETMiss signals. Cataloging all significant cosmic events can give insight into this effect.

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 19 ETransMiss – Making the Catalog Every cell has an geometric address in standard ATLAS coordinates (Φ,η). The energy of each cell is ‘projected’ into E x (i), E y (i). Summing over all of the properly functioning cells yields a total E x and E y. The total missing transverse energy is: x y z Φ θ

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 20 Current Spectrum

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 21 Travel!

8 August 2007 Ian Ross - ATLAS Calorimeter: Cosmic Ray Commisioning University of Toronto Group 22 Acknowledgements Richard Teuscher, Adam Gibson, Sam Posen, and the University of Toronto Group Prof. Jean Krisch, Prof. Homer Neal, Dr. Steve Goldfarb, and Jeremy Herr The NSF and University of Michigan Questions?