Chapter 5 EVENT RECONSTRUCTION 5.1 Jets
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ATLAS EXPERIMENT 15 3.1 the Large Hadron Collider
THE UNIVERSITY OF CHICAGO SEARCH FOR NEW PHENOMENA IN DIJET TOPOLOGIES FROM PROTON-PROTON COLLISIONS AT pS = 13 TEV A DISSERTATION SUBMITTED TO THE FACULTY OF THE DIVISION OF THE PHYSICAL SCIENCES IN CANDIDACY FOR THE DEGREE OF DOCTOR OF PHILOSOPHY DEPARTMENT OF PHYSICS BY JEFFREY ROGERS DANDOY CHICAGO, ILLINOIS SEPTEMBER 2016 For my family TABLE OF CONTENTS ABSTRACT xvii 1 INTRODUCTION 1 2 THE STANDARD MODEL 3 2.1 Quantum Chromodynamics . .4 2.1.1 Hard Scatter . .8 2.1.2 Parton Shower . 11 2.1.3 Hadronization . 11 2.2 Motivation for New Physics . 12 3 THE ATLAS EXPERIMENT 15 3.1 The Large Hadron Collider . 15 3.1.1 LHC Operation . 17 3.2 The ATLAS Detector . 20 3.2.1 Inner Detector . 20 3.2.2 Calorimetry . 25 3.2.3 Electromagnetic Calorimeters . 27 3.2.4 Hadronic Calorimeters . 29 3.2.5 Muon Spectrometer . 35 3.2.6 Data Acquisition . 37 4 EVENT SIMULATION 39 4.1 QCD Simulation . 40 4.1.1 The Pythia Generator . 40 4.1.2 Monte Carlo Production . 42 4.2 Signal Models . 44 4.2.1 Excited Quark . 44 4.2.2 Dark Matter Mediators . 44 4.2.3 Heavy Boson . 46 4.2.4 Quantum Black Holes . 47 4.3 Monte Carlo Uncertainties . 49 iii 5 JET RECONSTRUCTION AND PERFORMANCE 52 5.1 Jet Reconstruction . 52 5.1.1 Topo-clusters . 53 5.1.2 Jet-finding . 54 5.2 Jet Calibration . 57 5.2.1 In-situ Jet Calibration . 60 5.2.2 Single Particle Response . 62 5.2.3 Corrections for 2015 data . -
5.12. Ratio of the Inclusive B-Jet Measurement with the POWHEG+Pythia 6 Prediction
Two b or not two b-jets Measurements of inclusive and dijet b-jet differential cross-sections with the ATLAS detector Stephen Paul Bieniek Supervisor: Prof. Nikos Konstantinidis University College London Submitted to University College London in fulfilment of the requirements for the award of the degree of Doctor of Philosophy, 21st June 2013. I, Stephen Bieniek confirm that the work presented in this thesis is my own. Where information has been derived from other sources, I confirm that this has been indicated in the thesis. 1 2 Acknowledgements There are many people who I would like to thank for helping me get through my PhD and I don’t have the space to list all of them. I would first like to thank my supervisor, Nikos Konstantinidis [1], for providing me the support, motivation and direction for this project. I would like to thank Eric Jansen [2] for being there to answer my questions, show me the ropes while I was learning everything and always being there for bouncing ideas off. I would like to thank Lynn Marx [3] who provided the competition I needed to motivate me to produce my best during my time at CERN and Sarah Baker [4] for keeping me company when working late. I’d like to thank my fellow PhD students Erin Walters [5] and Bobby Xinyue [6] who allowed me to keep things in perspective when the work was hard. I would also like to thank Daniel Lattimer [7] for helping me ease back into London life after my time away. As a last note, I would like to dedicate this thesis to Francis Corry. -
Fast Calorimeter Punch-Through Simulation for the ATLAS Experiment
Fast Calorimeter Punch-Through Simulation for the ATLAS Experiment Diplomarbeit in der Studienrichtung Physik zur Erlangung des akademischen Grades Magister der Naturwissenschaft (Mag.rer.nat.) eingereicht an der Fakult¨atf¨urMathematik, Informatik und Physik der Universit¨atInnsbruck von Elmar Ritsch [email protected] CERN-THESIS-2011-112 28/09/2011 Betreuer der Diplomarbeit: Dr. Andreas Salzburger, CERN Ao.Univ.-Prof. Dr. Emmerich Kneringer, Institut f¨ur Astro- und Teilchenphysik Innsbruck, September 2011 Abstract This work discusses the parametrization, implementation and validation of a tuneable fast simulation of hadronic leakage in the ATLAS detector. It is dedicated to simulate calorimeter punch-through and decay in flight processes inside the ATLAS calorime- ter. Both effects can cause systematic errors in muon reconstruction and identification. Therefore a correct description of these effects is crucial for many physics studies in- volving muons. The parameterized punch-through simulation is integrated into the fast ATLAS detector simulations Fatras and AtlfastII, respectively. The Fatras based simu- lation of single pions shows a good agreement with results obtained by the full Geant4 detector simulation { especially in the context of a fast simulation. It is shown that for high energy multi jet events, simulated with the AtlfastII implementation, the muon reconstruction rates show a good agreement with the Geant4 simulated reference. i Acknowledgements { Danksagung Beginnen m¨ochte ich meine Danksagung bei meinen Betreuern Dr. Andreas Salzburger und Prof. Dr. Emmerich Kneringer. Ihr habt mich seit meinen Anf¨angenin der Teilchen- physik engagiert unterst¨utzt.Gemeinsam haben wir unz¨ahligeDiskussionen gef¨uhrt,die mir sowohl bei meiner Arbeit von großer Hilfe waren, als auch, mich weit ¨uber die Physik hinaus inspiriert haben. -
The Search for B S → Μτ At
ETHZ-IPP Internal Report 2008-10 August 2008 0 ! The Search for Bs ¹¿ at CMS DIPLOMA THESIS presented by Michel De Cian under the supervision of Prof. Dr. Urs Langenegger ETH Zürich, Switzerland Abstract Using the technique called neutrino reconstruction, a method is presented to analyze the decay 0 ! ! Bs ¹¿, where ¿ ¼¼¼º¿ , in the environment of the CMS detector at the LHC at CERN. Several models with physics beyond the Standard Model are discussed for a motivation of Lepton Flavor Violation within reach of current detectors. The actual event chain from the data production with Monte Carlo simulations to the final cut-based analysis is exposed in detail, considering some alternative approaches concerning the reconstruction procedure as well. Finally, a short overview of the calculation of the upper limit of the branching fraction and the value itself is given. Contents Preface: The Burden of Negative Knowledge 7 1 Towards a New Era at CERN 9 1.1 Fifty Years of Accelerated Physics . 9 1.2 The Large Hadron Collider . 10 1.3 The Compact Muon Solenoid . 11 2 Theoretical Motivation 13 3 Neutrino Reconstruction 17 3.1 Decay Topology ................................... 17 3.2 Illustrative Understanding . 18 3.3 Full Calculation . 18 0 3.4 Reconstruction of the Bs .............................. 19 4 Data Production 21 4.1 CMSSW, Pythia, EvtGen and FAMOS . 21 4.1.1 CMSSW ................................... 21 4.1.2 Pythia .................................... 21 4.1.3 EvtGen ................................... 22 4.1.4 FAMOS ................................... 22 4.2 The Signal Sample . 22 4.3 The Background Sample ............................... 22 4.4 Candidate Reconstruction . 23 4.5 Efficiencies of the Signal Sample . -
Search for New Physics in Dijet Resonant Signatures and Recent Results from Run 2 with the CMS Experiment
138 Proceedings of the LHCP2015 Conference, St. Petersburg, Russia, August 31 - September 5, 2015 Editors: V.T. Kim and D.E. Sosnov Search for new physics in dijet resonant signatures and recent results from Run 2 with the CMS experiment GIULIA D’IMPERIO Universit`aLa Sapienza and INFN Roma On behalf of the CMS Collaboration Abstract. A search for narrow resonances in proton-proton collisions at a center-of-mass energy of √s = 13 TeV is presented. The dijet invariant mass distribution of the two leading jets is measured with the CMS detector using early data from Run 2 of the Large Hadron Collider. The dataset presented here was collected in July 2015 and corresponds to an integrated luminosity of 42 1 pb− . The highest observed dijet mass is 5.4 TeV. The spectrum is well described by a smooth parameterization and no evidence for new particle production is observed. Upper limits at a 95% confidence level are set on the cross section of narrow resonances with masses above 1.3 TeV. When interpreted in the context of specific models the limits exclude: string resonances with masses below 5.1 TeV; scalar diquarks below 2.7 TeV; axigluons and colorons below 2.7 TeV; excited quarks below 2.7 TeV; and color octet scalars below 2.3 TeV. Introduction Deep inelastic proton-proton (pp) collisions often produce two or more energetic jets when the constituent partons are scattered with large transverse momenta (pT ). The invariant mass of the two jets with the largest pT in the event (the dijet) has a spectrum that is predicted by quantum chromodynamics (QCD) to fall steeply and smoothly with increasing dijet mass (m jj) [1]. -
Generative Models for Particle Shower Simulation in Fundamental Physics
Published as a workshop paper at ICLR 2021 SimDL Workshop GENERATIVE MODELS FOR PARTICLE SHOWER SIMULATION IN FUNDAMENTAL PHYSICS Erik Buhmann, Sascha Diefenbacher, Daniel Hundhausen, Gregor Kasieczka & William Korcari Institut fur¨ Experimentalphysik Universitat¨ Hamburg Luruper Chaussee 149, 22761 Hamburg, Germany [email protected] Engin Eren, Frank Gaede, Katja Kruger,¨ Peter McKeown & Lennart Rustige Deutsches Elektronen-Synchrotron Notkestraße 85, 22607 Hamburg Anatolii Korol Taras Shevchenko National University Volodymyrska St, 60, Kyiv, Ukraine ABSTRACT Simulations in fundamental physics connect underlying first-principle theories and empirical descriptions of detectors with experimentally observed data. They are indispensable, e.g., in particle physics, where they underpin statistical infer- ence tasks and experiment design. However, these Monte-Carlo-based simulations are computationally costly. Growing data volumes produced by upcoming experi- ments exacerbate this problem and need to be matched by a commensurate growth in simulated statistics for precision measurements. Generative machine learning models offer a potential way to leverage the effectiveness of classical simulation via amplification. This contribution presents state-of-the-art performance for sim- ulating the interaction of two different types of elementary particles with different characteristics — photons and pions — with high granularity detectors of 27k and 8k read-out channels, respectively. 1 INTRODUCTION Fundamental physics probes the physical laws of Nature at length scales of 10−18 meters by inves- tigating the interactions of high-energy particles at collider experiments. There, beams of particles (e.g. protons or electrons) close to the speed of light are brought into collision. These interactions produce sprays of secondary particles that are eventually measured in complex and highly-granular detectors. -
THE DIJET CROSS SECTION MEASUREMENT in PROTON-PROTON COLLISIONS at a CENTER of MASS ENERGY of 500 GEV at STAR Grant D
University of Kentucky UKnowledge Theses and Dissertations--Physics and Astronomy Physics and Astronomy 2014 THE DIJET CROSS SECTION MEASUREMENT IN PROTON-PROTON COLLISIONS AT A CENTER OF MASS ENERGY OF 500 GEV AT STAR Grant D. Webb University of Kentucky, [email protected] Recommended Citation Webb, Grant D., "THE DIJET CROSS SECTION MEASUREMENT IN PROTON-PROTON COLLISIONS AT A CENTER OF MASS ENERGY OF 500 GEV AT STAR" (2014). Theses and Dissertations--Physics and Astronomy. Paper 20. http://uknowledge.uky.edu/physastron_etds/20 This Doctoral Dissertation is brought to you for free and open access by the Physics and Astronomy at UKnowledge. It has been accepted for inclusion in Theses and Dissertations--Physics and Astronomy by an authorized administrator of UKnowledge. For more information, please contact [email protected]. STUDENT AGREEMENT: I represent that my thesis or dissertation and abstract are my original work. Proper attribution has been given to all outside sources. I understand that I am solely responsible for obtaining any needed copyright permissions. I have obtained and attached hereto needed written permission statement(s) from the owner(s) of each third-party copyrighted matter to be included in my work, allowing electronic distribution (if such use is not permitted by the fair use doctrine). I hereby grant to The nivU ersity of Kentucky and its agents the irrevocable, non-exclusive, and royalty- free license to archive and make accessible my work in whole or in part in all forms of media, now or hereafter known. I agree that the document mentioned above may be made available immediately for worldwide access unless a preapproved embargo applies. -
Introduction to Calorimeters
STFC RAL Introduction to Calorimeters David Cockerill Southampton Lecture 4 May 2016 D Cockerill, RAL, STFC, UK Introduction to Calorimeters 4 May 2016 1 STFC RAL Overview • Introduction • Electromagnetic Calorimetry • Hadron Calorimetry • Jets and Particle Flow • Future directions in Calorimetry • Summary D Cockerill, RAL, STFC, UK Introduction to Calorimeters 4 May 2016 2 STFC RAL Introduction Calorimetry One of the most important and powerful detector techniques in experimental particle physics Two main categories of Calorimeter: Electromagnetic calorimeters for the detection of e and neutral particles Hadron calorimeters for the detection of 0 , p , K and neutral particles n, K L usually traverse the calorimeters losing small amounts of energy by ionisation The 13 particle types above completely dominate the particles from high energy collisions reaching and interacting with the calorimeters All other particles decay ~instantly, or in flight, usually within a few hundred microns from the collision, into one or more of the particles above Neutrinos, and neutralinos, χo, undetected but with hermetic calorimetry can be inferred from measurements of missing transverse energy in collider experiments D Cockerill, RAL, STFC, UK Introduction to Calorimeters 4 May 2016 3 STFC RAL Introduction Calorimeters Calorimeters designed to stop and fully contain their respective particles ‘End of the road’ for the incoming particle Measure - energy of incoming particle(s) by total absorption in the calorimeter - spatial location of the energy -
Spallation Backgrounds in Super-Kamiokande Are Made in Muon-Induced Showers
Spallation backgrounds in Super-Kamiokande are made in muon-induced showers Shirley Weishi Li1, 2 and John F. Beacom1, 2, 3 1Center for Cosmology and AstroParticle Physics (CCAPP), Ohio State University, Columbus, OH 43210 2Department of Physics, Ohio State University, Columbus, OH 43210 3Department of Astronomy, Ohio State University, Columbus, OH 43210 [email protected],[email protected] (Dated: April 28, 2015) Crucial questions about solar and supernova neutrinos remain unanswered. Super-Kamiokande has the exposure needed for progress, but detector backgrounds are a limiting factor. A leading component is the beta decays of isotopes produced by cosmic-ray muons and their secondaries, which initiate nuclear spallation reactions. Cuts of events after and surrounding muon tracks reduce this spallation decay background by ' 90% (at a cost of ' 20% deadtime), but its rate at 6{18 MeV is still dominant. A better way to cut this background was suggested in a Super-Kamiokande paper [Bays et al., Phys. Rev. D 85, 052007 (2012)] on a search for the diffuse supernova neutrino background. They found that spallation decays above 16 MeV were preceded near the same location by a peak in the apparent Cherenkov light profile from the muon; a more aggressive cut was applied to a limited section of the muon track, leading to decreased background without increased deadtime. We put their empirical discovery on a firm theoretical foundation. We show that almost all spallation decay isotopes are produced by muon-induced showers and that these showers are rare enough and energetic enough to be identifiable. This is the first such demonstration for any detector. -
How We Detect Particles?
How we detect particles? Dr. Chayanit Asawatangtrakuldee (Aj Nan) Chulalongkorn University The Beginning of Everything C. Asawatangtrakuldee ([email protected]) Credit : https://youtu.be/wNDGgL73ihY 2 Credit : https://www.flickr.com/photos/arselectronica/5996559603 How a Detector works “Just as hunters can identify animals from tracks in mud or snow, physicists identify subatomic particles from the traces they leave in detectors” C. Asawatangtrakuldee ([email protected]) 4 A Chronology Particle Physics Instrumentation C. Asawatangtrakuldee ([email protected]) 5 A Chronology < 1950s : Cloud Chambers, Nuclear Emulsions + 1960-1985 : Geiger- Muller tubes dominated peak time for Bubble Chambers, > 1970 : Wire Chambers and > 1980 : Drift Chambers solid state Detectors start to dominate become a common use C. Asawatangtrakuldee ([email protected]) 6 Spinthariscope (1903) ★ The spinthariscope, invented and beautifully named by William Crookes in 1903, is a device for seeing individual atoms or at least, seeing the death of individual atoms ★ Consist of a small screen coated with zinc sulfide affixed to the end of a tube, with a tiny amount of radium salt suspended a short distance from the screen and a lens on the other end of the tube for viewing the screen. Crookes named his device after the Greek word 'spintharis', meaning "a spark” C. Asawatangtrakuldee ([email protected]) Credit : https://blog.wolfram.com/2007/10/30/a-thousand-points-of-light/ 7 Cloud Chamber (1911) ★ Originally developed to study formation of rain clouds ★ Passage of charge particle would condense the vapour into tiny droplets, making the particle’s path → their number being proportional to dE/dx ★ The discoveries of positron in 1932 and muon in 1936, both by Carl Anderson (awarded a Nobel Prize in Physics in 1936), used cloud chambers Charles Thomson Rees Wilson (1869–1959) Nobel Prize in 1927 C. -
Angular Distribution of Prompt Photons Using the Compact Muon
Florida International University FIU Digital Commons FIU Electronic Theses and Dissertations University Graduate School 9-14-2012 Angular Distribution of Prompt Photons Using the Compact Muon Solenoid Detector at √S =7 TeV Vanessa Gaultney Werner Florida International University, [email protected] DOI: 10.25148/etd.FI12111303 Follow this and additional works at: https://digitalcommons.fiu.edu/etd Recommended Citation Werner, Vanessa Gaultney, "Angular Distribution of Prompt Photons Using the Compact Muon Solenoid Detector at √S =7 TeV" (2012). FIU Electronic Theses and Dissertations. 727. https://digitalcommons.fiu.edu/etd/727 This work is brought to you for free and open access by the University Graduate School at FIU Digital Commons. It has been accepted for inclusion in FIU Electronic Theses and Dissertations by an authorized administrator of FIU Digital Commons. For more information, please contact [email protected]. FLORIDA INTERNATIONAL UNIVERSITY Miami, Florida ANGULAR DISTRIBUTION OF PROMPT PHOTONS USING THE COMPACT p MUON SOLENOID DETECTOR AT S = 7 TEV A dissertation submitted in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY in PHYSICS by Vanessa Gaultney Werner 2012 To: Dean Kenneth Furton College of Arts and Sciences This dissertation, written by Vanessa Gaultney Werner, and entitled Angularp Distri- bution of Prompt Photons Using The Compact Muon Solenoid Detector at S = 7 TeV, having been approved in respect to style and intellectual content, is referred to you for judgment. We have read this dissertation and recommend that it be approved. Stephan Linn Jorge Rodriguez Joerg Reinhold Eric Brewe Pete Markowitz, Major Professor Date of Defense: September 14, 2012 The dissertation of Vanessa Gaultney Werner is approved. -
An Introduction to Jet Substructure and Boosted-Object Phenomenology
Looking inside jets: an introduction to jet substructure and boosted-object phenomenology Simone Marzani1, Gregory Soyez2, and Michael Spannowsky3 1Dipartimento di Fisica, Universit`adi Genova and INFN, Sezione di Genova, Via Dodecaneso 33, 16146, Italy 2IPhT, CNRS, CEA Saclay, Universit´eParis-Saclay, F-91191 Gif-sur-Yvette, France 3Institute of Particle Physics Phenomenology, Physics Department, Durham University, Durham DH1 3LE, UK arXiv:1901.10342v3 [hep-ph] 17 Feb 2020 Preface The study of the internal structure of hadronic jets has become in recent years a very active area of research in particle physics. Jet substructure techniques are increasingly used in experimental analyses by the Large Hadron Collider collaborations, both in the context of searching for new physics and for Standard Model measurements. On the theory side, the quest for a deeper understanding of jet substructure algorithms has contributed to a renewed interest in all-order calculations in Quantum Chromodynamics (QCD). This has resulted in new ideas about how to design better observables and how to provide a solid theoretical description for them. In the last years, jet substructure has seen its scope extended, for example, with an increasing impact in the study of heavy-ion collisions, or with the exploration of deep-learning techniques. Furthermore, jet physics is an area in which experimental and theoretical approaches meet together, where cross-pollination and collaboration between the two communities often bear the fruits of innovative techniques. The vivacity of the field is testified, for instance, by the very successful series of BOOST conferences together with their workshop reports, which constitute a valuable picture of the status of the field at any given time.