Micromegas-Based Detectors for Time-Of-Flight Measurements Of
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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. -
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. -
Current Status and Future Developments of Micromegas Detectors for Physics and Applications
applied sciences Review Current Status and Future Developments of Micromegas Detectors for Physics and Applications David Attié , Stephan Aune, Eric Berthoumieux , Francesco Bossù , Paul Colas, Alain Delbart, Emmeric Dupont, Esther Ferrer Ribas , Ioannis Giomataris , Aude Glaenzer , Hector Gómez , Frank Gunsing, Fanny Jambon, Fabien Jeanneau , Marion Lehuraux, Damien Neyret, Thomas Papaevangelou * , Emanuel Pollacco , Sébastien Procureur , Maxence Revolle , Philippe Schune, Laura Segui , Lukas Sohl * , Maxence Vandenbroucke and Zhibo Wu † CEA, Institut de Recherche sur les Lois Fondamentales de l’Univers, Université Paris-Saclay, 91191 Gif-sur-Yvette, France; [email protected] (D.A.); [email protected] (S.A.); [email protected] (E.B.); [email protected] (F.B.); [email protected] (P.C.); [email protected] (A.D.); [email protected] (E.D.); [email protected] (E.F.R.); [email protected] (I.G.); [email protected] (A.G.); [email protected] (H.G.); [email protected] (F.G.); [email protected] (F.J.); [email protected] (F.J.); [email protected] (M.L.); [email protected] (D.N.); [email protected] (E.P.); [email protected] (S.P.); [email protected] (M.R.); [email protected] (P.S.); [email protected] (L.S.); [email protected] (M.V.); [email protected] (Z.W.) * Correspondence: [email protected] (T.P.); [email protected] (L.S.) † Also: Department of Modern Physics, University of Science and Technology of China, Hefei 230026, China. Abstract: Micromegas (MICRO-MEsh GAseous Structure) detectors have found common use in Citation: Attié, D.; Aune, S.; different applications since their development in 1996 by the group of I. -
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. -
Effect of Mesh Geometry on Resistive Micromegas for the ATLAS
Micro-Pattern Gaseous Detectors Conference 2019 IOP Publishing Journal of Physics: Conference Series 1498 (2020) 012031 doi:10.1088/1742-6596/1498/1/012031 Effect of mesh geometry on resistive Micromegas for the ATLAS experiment Ourania Sidiropoulou on behalf of the ATLAS Muon Collaboration CERN, Esplanade des Particules 1, 1211 Meyrin, Switzerland E-mail: [email protected] Abstract. The ATLAS Experiment will use resistive Micromegas detectors for the upgrade of the forward Muon System (NSW, for New Small Wheel). With the test of the first production modules, instabilities in the detector operation have been observed, leading to a systematic revision of the selected construction components and working parameters. In particular, the effect of the mesh geometry with respect to the discharge behaviour was studied using a special Micromegas detector designed and built by the ATLAS CERN group in 2014. The detector has a Micromegas structure similar to the one later on adopted by the NSW project; moreover it provides the possibility to easily replace the mesh. The test procedure consisted in measuring current, gain and counting rate from a 55Fe X-ray source, as a function of the amplification voltage up to the discharge limit. The systematic analysis of the data allowed us to draw conclusions on the stability interval of six different types of mesh, including the one chosen to be used for the NSW, consistent with the expectations. Results suggested that the mesh selected for the NSW (among the few available in the requested big size), was not optimal for operation with a safe plateau at high gain before discharges start to occur. -
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. -
MICROMEGAS Chambers for Hadronic Calorimetry, Search for New Physics in the Field of the Top Quark Ambroise Espargilière
MICROMEGAS Chambers for Hadronic Calorimetry, Search for New Physics in the Field of the Top Quark Ambroise Espargilière To cite this version: Ambroise Espargilière. MICROMEGAS Chambers for Hadronic Calorimetry, Search for New Physics in the Field of the Top Quark. High Energy Physics - Experiment [hep-ex]. Université de Grenoble, 2011. English. tel-00657129v1 HAL Id: tel-00657129 https://tel.archives-ouvertes.fr/tel-00657129v1 Submitted on 5 Jan 2012 (v1), last revised 17 Mar 2012 (v2) HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. THESE` Pour obtenir le diplomeˆ de DOCTEUR DE L’UNIVERSITE´ DE GRENOBLE Specialit´ e´ : Physique/Physique Subatomique & Astroparticules Arretˆ e´ ministerial´ : 7 aoutˆ 2006 Present´ ee´ par AMBROISE ESPARGILIERE` These` dirigee´ par Catherine ADLOFF et codirigee´ par Yannis KARYOTAKIS prepar´ ee´ au Laboratoire d'Annecy-le-vieux de Physique des Particules et de l’Ecole´ Doctorale de Physique de Grenoble Chambres MICROMEGAS pour la Calorimetrie´ Hadronique, Recherche d’une Nouvelle Physique dans le Domaine du Quark Top R&D pour un futur collisionneur lineaire´ These` soutenue publiquement le 21 septembre 2011, devant le jury compose´ de : Dr. Jean-Jacques BLAISING Directeur de Recherche au LAPP, Annecy-le-Vieux, President´ Dr. -
35. Particle Detectors at Accelerators
1 35. Particle Detectors at Accelerators 35. Particle Detectors at Accelerators Revised 2019. See the various sections for authors. 35.1 Introduction ....................................... 2 35.2 Photon detectors..................................... 3 35.2.1 Vacuum photodetectors .............................. 4 35.2.2 Gaseous photon detectors............................. 6 35.2.3 Solid-state photon detectors............................ 7 35.3 Organic scintillators................................... 8 35.3.1 Scintillation mechanism.............................. 9 35.3.2 Caveats and cautions................................ 10 35.3.3 Scintillating and wavelength-shifting fibers.................... 11 35.4 Inorganic scintillators .................................. 11 35.5 Cherenkov detectors................................... 16 35.6 Gaseous detectors .................................... 21 35.6.1 Energy loss and charge transport in gases.................... 21 35.6.2 Multi-Wire Proportional and Drift Chambers.................. 27 35.6.3 High Rate Effects.................................. 29 35.6.4 Micro-Pattern Gas Detectors ........................... 30 35.6.5 Time-projection chambers............................. 34 35.6.6 Transition radiation detectors (TRD’s)...................... 39 35.6.7 Resistive-plate chambers.............................. 42 35.7 Semiconductor detectors................................. 45 35.7.1 Materials Requirements .............................. 45 35.7.2 Detector Configurations.............................. 46 -
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 .................................................................................................................