Time Projection Chambers
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Optimizing Tracking Software for a Time Projection Chamber Wilson H
Journal of the Arkansas Academy of Science Volume 49 Article 18 1995 Optimizing Tracking Software for a Time Projection Chamber Wilson H. Howe University of Arkansas at Little Rock Christine A. Byrd University of Arkansas at Little Rock Amber D. Climer University of Arkansas at Little Rock Wilfred J. Braithwaite University of Arkansas at Little Rock Jeffrey T. Mitchell Brookhaven National Laboratory Follow this and additional works at: http://scholarworks.uark.edu/jaas Part of the Nuclear Commons Recommended Citation Howe, Wilson H.; Byrd, Christine A.; Climer, Amber D.; Braithwaite, Wilfred J.; and Mitchell, Jeffrey T. (1995) "Optimizing Tracking Software for a Time Projection Chamber," Journal of the Arkansas Academy of Science: Vol. 49 , Article 18. Available at: http://scholarworks.uark.edu/jaas/vol49/iss1/18 This article is available for use under the Creative Commons license: Attribution-NoDerivatives 4.0 International (CC BY-ND 4.0). Users are able to read, download, copy, print, distribute, search, link to the full texts of these articles, or use them for any other lawful purpose, without asking prior permission from the publisher or the author. This Article is brought to you for free and open access by ScholarWorks@UARK. It has been accepted for inclusion in Journal of the Arkansas Academy of Science by an authorized editor of ScholarWorks@UARK. For more information, please contact [email protected], [email protected]. Journal of the Arkansas Academy of Science, Vol. 49 [1995], Art. 18 a Time Projection Chamber Wilson H. Howe, Christine A.Byrd, Amber D. Climer, W.J. Braithwaite Department of Physics and Astronomy University of Arkansas at Little Rock LittleRock, Ar 72204 Jeffrey T.Mitchell Brookhaven National Laboratory Upton, NY11973 Abstract International research collaborations willbe using accelerators in the U.S. -
Development of a Liquid Xenon Time Projection Chamber for the XENON Dark Matter Search
Development of a Liquid Xenon Time Projection Chamber for the XENON Dark Matter Search Kaixuan Ni Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Graduate School of Arts and Sciences COLUMBIA UNIVERSITY 2006 c 2006 Kaixuan Ni All rights reserved Development of a Liquid Xenon Time Projection Chamber for the XENON Dark Matter Search Kaixuan Ni Advisor: Professor Elena Aprile Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Graduate School of Arts and Sciences COLUMBIA UNIVERSITY 2006 c 2006 Kaixuan Ni All rights reserved ABSTRACT Development of a Liquid Xenon Time Projection Chamber for the XENON Dark Matter Search Kaixuan Ni This thesis describes the research conducted for the XENON dark matter direct detection experiment. The tiny energy and small cross-section, from the interaction of dark matter particle on the target, requires a low threshold and sufficient background rejection capability of the detector. The XENON experiment uses dual phase technology to detect scintillation and ionization simultaneously from an event in liquid xenon (LXe). The distinct ratio, be- tween scintillation and ionization, for nuclear recoil and electron recoil events provides excellent background rejection potential. The XENON detector is designed to have 3D position sensitivity down to mm scale, which provides additional event information for background rejection. Started in 2002, the XENON project made steady progress in the R&D phase during the past few years. Those include developing sensitive photon detectors in LXe, improving the energy resolution and LXe purity for detect- ing very low energy events. -
Physique Nucléaire Et De L'instrumentation Associée Introduction
FR0108546 # DEA-DAPNIA-RA-1997-98 A il. ..33/04 -DSM Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée Introduction Motivés par la curiosité pour les connaissances fondamentales et soutenus par des investissements impor- tants, les chercheurs du vingtième siècle ont fait des découvertes scientifiques considérables, sources de retombées économiques fructueuses. Une recherche ambitieuse doit se poursuivre. Organisé pour déve- lopper les grands programmes pour le nucléaire et par le nucléaire, le CEA est bien armé pour concevoir et mettre au point les instruments destinés à explorer, en coopération avec les autres organismes de recherche, les confins de l'infiniment petit et ceux de l'infinimenf grand. La recherche fondamentale évolue et par essence ne doit pas avoir de frontières. Le Département d'astrophysique, de physique des particules, de physique nucléaire et de l'instrumentation associée (Dapnia) a été créé pour abolir les cloisons entre la physique nucléaire, la physique des particules et l'as- trophysique, tout en resserrant les liens entre physiciens, ingénieurs et techniciens au sein de la Direction des sciences de la matière (DSM). Le Dapnia est unique par sa pluridisciplinarité. Ce regroupement a permis de lancer des expériences se situant aux frontières de ces disciplines tout en favorisant de nou- velles orientations et les choix vers les programmes les plus prometteurs. Tout en bénéficiant de l'expertise d'autres départements du CEA, la recherche au Dapnia se fait princi- palement au sein de collaborations nationales et internationales. Les équipes du Dapnia, de I'IN2P3 (Institut national de physique nucléaire et de physique des particules) et de l'Insu (Institut national des sciences de l'Univers) se retrouvent dans de nombreuses grandes collaborations internationales, chacun apportant ses compétences spécifiques afin de renforcer l'impact de nos contributions. -
Development and Evaluation of a Multiwire Proportional Chamber for a High Resolution Small Animal PET Scanner
Henning H¨unteler Development and Evaluation of a Multiwire Proportional Chamber for a High Resolution Small Animal PET Scanner — 2007 — Kernphysik Development and Evaluation of a Multiwire Proportional Chamber for a High Resolution Small Animal PET Scanner Diplomarbeit von Henning H¨unteler Westf¨alische Wilhelms-Universit¨at M¨unster Institut f¨ur Kernphysik — Februar 2007 — Contents 1 Introduction 7 2 Positron Emission Tomography 9 2.1 The β-Decay ............................... 10 2.1.1 Different Types of Radioactive Decay . 10 2.1.2 Different Types of β-Decays ................... 11 2.1.3 The β-Spectrum ......................... 13 2.2 Tracer ................................... 16 2.3 Mean Range and Annihilation of Positrons in Matter . .... 18 2.3.1 PositronRangeinMatter . 18 2.3.2 PositronAnnihilation. 22 2.4 Interactions ofGammaRadiationinMatter . .. 23 2.4.1 PhotoelectricEffect. 23 2.4.2 ComptonEffect.......................... 25 3 Multiwire Proportional Chambers 33 3.1 BasicsonProportionalCounters. 35 3.1.1 ProportionalCountersTubes . 35 3.1.2 GasAmplification. 36 3.1.3 FillGases ............................. 39 3.2 MultiwireProportionalChambers . 43 3.2.1 Geometry of Multiwire Proportional Chambers . 43 3.2.2 ReadoutMethods. .. .. 46 3 4 Contents 4 Motivation for an MWPC Small Animal PET 51 4.1 Reasons for the Construction of a Small Animal PET Detector.... 51 4.2 Motivation for the Development of an MWPC-based PET Detector . 54 4.2.1 Advantages of Scintillation Crystals . .. 54 4.2.2 Advantages of Multiwire Proportional Chambers . ... 55 4.2.3 Conclusions ............................ 56 5 Determination of the Optimal Converter Thickness 57 5.1 Theoretical Determination of the Optimal Converter Thickness . 58 5.2 Experimental Determination of the Optimal Converter Thickness . -
Using a Two-Phase Xenon Time Projection Chamber for Improved Background Rejection in Searches for Neutrinoless Double-Beta Decay
Using a two-phase xenon time projection chamber for improved background rejection in searches for neutrinoless double-beta decay by Callan Jessiman A thesis submitted to the Faculty of Graduate and Postdoctoral Affairs in partial fulfilment of the requirements for the degree of Master of Science in Physics Department of Physics Carleton University Ottawa, Ontario January 2020 c 2020 Callan⃝ Jessiman Abstract The nature of the neutrino masses is an important open question in particle physics; neutrinos were conceived and implemented into the Standard Model as massless, and their masses, now known to be nonzero, represent an area of new physics. Essential to the investigation of this area are mechanisms by which one might measure these masses, including the hypothetical neutrinoless double-beta decay, which has a lifetime related to the neutrino masses. Experiments searching for this rare decay, such as EXO, are impacted heavily by sources of background radiation. Here, a prototype two-phase time projection chamber is described, having superior temporal resolution to the existing EXO architecture. A machine- learning analysis of data from this prototype is used for pulse-shape discrimination, which has the potential to significantly increase EXO's sensitivity; the preliminary efforts described here are able to reduce backgrounds by 94%, while rejecting only 21% of the signal. ii Acknowledgements First, and foremost, I express my gratitude towards my supervisor, David Sinclair, and my colleague Braeden Veenstra. The entire project was of David's devising, as was the leadership that saw it through. Meanwhile, getting the thing to actually work, and extracting results from it, was Braeden's task as much as it was mine. -
Parity Non-Conservation in Atoms L.M
INIJ. •®'82 Dl OF THE INTERNATIONAL CONFERENCE '82 14-19 JUNE, 1982 BALATONFURED, HUNGARY EDITORS A. FRENKEL LJENIK BUDAPEST, 1982 III. CONTENTS Volume I ! -4- OPENING ADDRESS NEUTRINO OSCILLATION SEARCH FOR NEUTRINO OSCILLATIONS - A PROGRESS REPORT R. L. Mös sbauer 1 SEARCH FOR NEUTRINO OSCILLATION F. Reines Suppl NEUTRINO OSCILLATION EXPERIMENTS ON AMERICAN ACCELERATORS C. Baltay , Suppl PAST AND FUTURE OSCILLATION EXPERIMENTS IN CERN NEUTRINO BEAMS H. Wachsmuth 13 DETECTION OF MATTER EFFECTS ON NEUTRINO OSCILLATIONS BY DUMAND R.J. Oakes 23 LARGE AMPLITUDE NEUTRINO OSCILLATIONS WITH MAJORANA MASS EIGENSTATES? B. Pontecorvo 35 TRULY NEUTRAL MICROOBJECTS AND OSCILLATIONS IN PARTICLE PHYSICS S.M. Bilenky 42 A POSSIBLE TEST OF CP INVARIANCE IN NEUTRINO OSCILLATIONS S.M. Bilenky 46 *Papers labelled "Suppl" are to be found in the Supplement to this Proceedings. Their titles as given here are provisional. IV. NEUTRINO MASS AN EXPERIMENT TO STUDV THE 3-DECAY OF FREE ATOMIC AND MOLECULAR TRITIUM R.G.H. Robertson 51 MEASUREMENT OF THE MASS OF THE ELECTRON NEUTRINO USING THE ELECTRON CAPTURE DECAY PROCESS OF THE NUCLEUS S. Yasumi 59 AN EXPERIMENT TO DETERMINE THE MASS OF THE ELECTRON ANTINEUTRINO R.N. Boyd 67 DETERMINATION OF AN UPPER LIMIT OF THE MASS OF THE MUONIC NEUTRINO FROM THE PION DECAY IN FLIGHT P. Le Coultre , 75 RADIATIVE DECAYS OF DIRAC AND MAJORANA NEUTRINOS (RECENT RESULTS) S.T. Petcov 82 BEAM DUMP PROMPT NEUTRINO OSCILLATION BY 4OO GeV PROTON INTERACTIONS R. J. Loveless 89 A STUDY OF THE FORWARD PRODUCTION OF CHARM STATES AND PROMPT MUONS IN 350 GeV p-Fe AND 278 GeV n~-Fe INTERACTIONS A. -
Particle Detectors
Particle Detectors Summer Student Lectures 2007 Werner Riegler, CERN, [email protected] History of Instrumentation ↔ History of Particle Physics The ‘Real’ World of Particles Interaction of Particles with Matter, Tracking detectors Photon Detection, Calorimeters, Particle Identification Detector Systems W. Riegler/CERN 1 Detectors based on Ionization Gas Detectors: • Transport of Electrons and Ions in Gases • Wire Chambers • Drift Chambers • Time Projection Chambers Solid State Detectors • Transport of Electrons and Holes in Solids • Si- Detectors • Diamond Detectors W. Riegler/CERN Gas Detectors 2 Gas Detectors with internal Electron Multiplication • Principle: At sufficiently high electric fields (100kV/cm) the electrons gain energy in excess of the ionization energy secondary ionzation etc. etc. • Elektron Multiplication: – dN = N α dx α…’first Townsend Coefficient’ – N(x) = N0 exp (αx) α= α(E), N/ N0 = A (Amplification, Gas Gain) – N(x)=N0 exp ( (E)dE ) – In addition the gas atoms are excited emmission of UV photons can ionize themselves photoelectrons – NAγ photoeletrons → NA2 γ electrons → NA2 γ2 photoelectrons → NA3 γ2 electrons – For finite gas gain: γ < A-1, γ … ‘second Townsend coefficient’ W. Riegler/CERN Gas Detectors 3 Wire Chamber: Electron Avalanche Wire with radius (10-25m) in a tube of radius b (1-3cm): Electric field close to a thin wire (100-300kV/cm). E.g. V0=1000V, a=10m, b=10mm, E(a)=150kV/cm Electric field is sufficient to accelerate electrons to energies which are sufficient to produce secondary ionization electron avalanche signal. b a b Wire W. Riegler/CERN Gas Detectors 4 Gas Detectors with internal Electron Multiplication From L. -
Design and Construction of the Spirit Tpc
DESIGN AND CONSTRUCTION OF THE SPIRIT TPC By Suwat Tangwancharoen A DISSERTATION Submitted to Michigan State University in partial fulfillment of the requirements for the degree of Physics-Doctor of Philosophy 2016 ABSTRACT DESIGN AND CONSTRUCTION OF THE SPIRIT TPC By Suwat Tangwancharoen The nuclear symmetry energy, the density dependent term of the nuclear equation of state (EOS), governs important properties of neutron stars and dense nuclear matter. At present, it is largely unconstrained in the supra-saturation density region. This dissertation concerns the design and construction of the SπRIT Time Projection Chamber (SπRIT TPC) at Michigan State University as part of an international collaborations to constrain the symmetry energy at supra-saturation density. The SπRIT TPC has been constructed during the dissertation and transported to Radioactive Isotope Beam Factory (RIBF) at RIKEN, Japan where it will be used in conjunction with the SAMURAI Spectrometer. The detector will measure yield ratios for pions and other light charged particles produced in central collisions of neutron-rich heavy ions such as 132Sn + 124Sn. The dissertation describes the design and solutions to the problem presented by the measurement. This also compares some of the initial fast measurement of the TPC to calculation of the performance characteristics. ACKNOWLEDGMENTS The design and construction of the SAMURAI Pion-Reconstruction and Ion Tracker Time Projection Chamber (SπRIT TPC) involved an international collaboration to study and constrain the symmetry energy term in the nuclear equation of state (EOS) at twice supra- saturation density. The TPC design and construction as well as many additional aspects of the project were supported financially by the U.S. -
3 Detector Gas 25 3.1 Gas Properties
DISSERTATION Titel der Dissertation A GEM based Time Projection Chamber prototype for the PANDA¯ experiment - Gas system development and forward tracking studies Verfasser Mag. rer. nat. Philipp Müllner angestrebter akademischer Grad Doktor der Naturwissenschaften (Dr. rer. nat.) Wien, 2012 Studienkennzahl lt. Studienblatt: A 091 411 Dissertationsgebiet lt. Studienblatt: Physik Betreuer: Doz. Dr. Johann Zmeskal 2 Abstract The PANDA¯ collaboration is building a state-of-the-art universal detector for strong interaction studies at the High Energy Storage Ring (HESR) at the new Facility for Antiproton and Ion Research (FAIR) at Darmstadt, Germany. The facility will provide a high intensity, cooled antiproton beam. Together with the advanced particle identification system of the PANDA¯ detector a wide experimental program ranging from QCD studies to funda- mental symmetry tests will be accessible. One of two options for the PANDA¯ central tracker was a Gas Electron Multiplier (GEM) based Time Projection Chamber (TPC). The low ma- terial budget GEM based TPC is an ideal device for 3-dimensional space tracking, which features fulfill the PANDA¯ tracking system requirements, e.g. high rate capability, continuous operation, high momentum resolution, high spatial resolution and full solid coverage. In the course of the detector developments for PANDA,¯ a large GEM- TPC prototype was build and tested at GSI (Darmstadt, Germany) by the GEM-TPC collaboration. Within the framework of this work, an overview of the prototype general design will be given. The main task of my thesis was the development of a closed gas supply system for the large GEM-TPC prototype. The detector requirements made it necessary to build it as closed circulation system with infrastructures for O2 and H2O measurement and purification as well as for precise pressure controlling inside the gas system. -
Time Projection Chamber the LUX Experiment LZ @ SLAC National
Time Projection Chamber LZ is a liquid-xenon TPC that collects two scintillation signals for each The LZ experiment scattering event. S1 is from the de-excitation of short-lived xenon molecules, or dimers. S2 is from electrons liberated at the event site that The LUX-ZEPLIN search for WIMP dark matter are extracted into the gas phase where they undergo electroluminescence. The S2 hit pattern give the lateral position and the S2-S1 time difference gives the depth. The localization allows for An Inventory of the Universe selection of WIMP candidates only in the detector interior, where wternal In 1933, Fritz Zwicky’s observation and virial radioactive backgrounds do not readily penetrate. analysis of the Coma Cluster of galaxies led to his discovery that most of its the matter Anatomy of LZ was dark. This finding launched a decades Scintillator Detector Feedthroughs long mystery as astronomers since have reinforced his findings time and again. The now Standard Cosmology based on Water independent observations of clusters, the Shield cosmic microwave background and distant Science reach type-1a supernovae converge on a consistent The 2013 Snowmass Community Summer Study’s set of cosmological parameters shown below. Anode & Electron Time Extraction Grids Cosmic Frontier working group on WIMP Dark Matter Big Bang Nucleosynthesis indicates that only Projection Detection (CF1) made a survey of the field, producing 20% of the mass density is composed of Chamber this summary plot, including the world leading LUX ordinary matter. A leading hypothesis is that result and the LZ projection for a 1000-day run. dark matter is composed of Weakly Interacting Massive Particles, or WIMPs. -
Oral Program As of May 27, 2008
Oral Program as of May 27, 2008 We invite you to Berkeley for the first West Coast meeting of the Symposium on Radiation Measurements and Applications. SORMA West 2008 is hosted jointly by the University of California, Berkeley and the Lawrence Berkeley and Lawrence Livermore National Laboratories. It is made possible by the generosity of our agency sponsors and private-sector supporters. We gratefully acknowledge the cooperation and advice of the original SORMA, now SORMA East, hosted by the University of Michigan and next scheduled for 2010. Note: the Monday opening plenaries (in International House) and Thursday summary or rapporteur plenaries are described in a different document. Monday's plenaries will be held at International House, which is also the location of the poster session and reception. The parallel oral sessions Tuesday through Thursday, and the closing plenary, will be in Stanley Hall (rooms 105 and 106) and Bechtel Engineering Center (Sibley Auditorium). Table of Contents Monday, June 2............................................................................................................................................. 1 Tuesday, June 3 ............................................................................................................................................ 1 New Scintillators........................................................................................................................................ 2 Tuesday AM I: Stanley 105 ................................................................................................................. -
Two-Phase Xenon Time Projection Chambers for WIMP Searches and Other Applications
Two-Phase Xenon Time Projection Chambers for WIMP Searches and Other Applications Nicole A. Larsen Yale University Department of Physics Advisor: Daniel McKinsey Thesis Prospectus May 24, 2012 Abstract Astronomical evidence indicates that 23 % of the energy density in the universe is comprised of some form of non-standard, non-baryonic matter that has yet to be observed. One of the predominant theories is that dark matter consists of WIMPs (Weakly Interacting Massive Particles), so named be- cause they do not interact electromagnetically or through the strong nuclear force. In direct dark matter detection experiments the goal is to look for evidence of collisions between WIMPs and other particles such as heavy nuclei. Here, the challenge is to measure exceedingly rare interactions with very high precision. In recent years xenon has risen as a medium for particle detection, exhibiting a number of desirable qualities that make it well-suited for direct WIMP searches. The LUX (Large Underground Xenon) experiment is a 350-kg xenon-based direct dark matter detection experiment currently deployed at the Homestake Mine in Lead, South Dakota, consisting of a two-phase (liq- uid/gas) xenon time projection chamber with a 100-kg fiducial mass. Its projected sensitivity for 300 days of underground data acquisition is a cross-section of 7 × 10-46 cm2 for a WIMP mass of 100 GeV, representing an improvement of nearly an order of magnitude over previous WIMP-nucleon scattering cross-section limits. Furthermore, two-phase xenon-based technologies are useful in many other applications, in- cluding other fundamental physics searches, imaging of special nuclear materials, and medical imaging.