Patentable Subject [Anti]Matter
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Confinement of Antihydrogen for 1000 Seconds
Confinement of antihydrogen for 1000 seconds G.B. Andresen1, M.D. Ashkezari2, M. Baquero-Ruiz3, W. Bertsche4, E. Butler5, C.L. Cesar6, A. Deller4, S. Eriksson4, J. Fajans3#, T. Friesen7, M.C. Fujiwara8,7, D.R. Gill8, A. Gutierrez9, J.S. Hangst1, W.N. Hardy9, R.S. Hayano10, M.E. Hayden2, A.J. Humphries4, R. Hydomako7, S. Jonsell11, S. Kemp5§, L. Kurchaninov8, N. Madsen4, S. Menary12, P. Nolan13, K. Olchanski8, A. Olin8&, P. Pusa13, C.Ø. Rasmussen1, F. Robicheaux14, E. Sarid15, D.M. Silveira16, C. So3, J.W. Storey8$, R.I. Thompson7, D.P. van der Werf4, J.S. Wurtele3#, Y. Yamazaki16¶. 1Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark. 2Department of Physics, Simon Fraser University, Burnaby BC, V5A 1S6, Canada 3Department of Physics, University of California, Berkeley, CA 94720-7300, USA 4Department of Physics, Swansea University, Swansea SA2 8PP, United Kingdom 5Physics Department, CERN, CH-1211, Geneva 23, Switzerland 6Instituto de Fısica, Universidade Federal do Rio de Janeiro, Rio de Janeiro 21941-972, Brazil 7Department of Physics and Astronomy, University of Calgary, Calgary AB, T2N 1N4, Canada 8TRIUMF, 4004 Wesbrook Mall, Vancouver BC, V6T 2A3, Canada 9Department of Physics and Astronomy, University of British Columbia, Vancouver BC, V6T 1Z1, Canada 10Department of Physics, University of Tokyo, Tokyo 113-0033, Japan 11 Department of Physics, Stockholm University, SE-10691, Stockholm, Sweden 12Department of Physics and Astronomy, York University, Toronto, ON, M3J 1P3, Canada 13Department of Physics, -
Analysis and Instrumentation for a Xenon-Doped Liquid Argon System
Analysis and instrumentation for a xenon-doped liquid argon system Ryan Gibbons Work completed under the advisement of Professor Michael Gold Department of Physics and Astronomy The University of New Mexico May 27, 2020 1 Abstract Liquid argon is a scintillator frequently used in neutrino and dark matter exper- iments. In particular, is the upcoming LEGEND experiment, a neutrinoless double beta decay search, which will utilize liquid argon as an active veto system. Neutri- noless double beta decay is a theorized lepton number violating process that is only possible if neutrinos are Majorana in nature. To achieve the LEGEND background goal, the liquid argon veto must be more efficient. Past studies have shown the ad- dition of xenon in quantities of parts-per-million in liquid argon improves the light yield, and therefore efficiency, of such a system. Further work, however, is needed to fully understand the effects of this xenon doping. I present a physical model for the light intensity of xenon-doped liquid argon. This model is fitted to data from various xenon concentrations from BACoN, a liquid argon test stand. Additionally, I present preliminary work on the instrumentation of silicon photomultipliers for BACoN. 2 Contents 1 Introduction 4 1.1 Neutrinos and double beta decay . 4 1.2 LEGEND and BACoN . 5 1.3 Liquid argon . 6 2 Physical modeling of xenon-doped liquid argon 8 2.1 Model . 8 2.2 Fits to BACoN Data . 9 2.3 Analysis of Rate Constant . 12 3 Instrumentation of SiPMs 12 4 Conclusions and Future Work 13 3 1 Introduction 1.1 Neutrinos and double beta decay Neutrinos are neutral leptons that come in three flavors: electron, muon, and tao. -
Antimatter Weapons (1946-1986): from Fermi and Teller's
Antimatter weapons (1946-1986): From Fermi and Teller’s speculations to the first open scientific publications ∗ Andre Gsponer and Jean-Pierre Hurni Independent Scientific Research Institute Box 30, CH-1211 Geneva-12, Switzerland e-mail: [email protected] Version ISRI-86-10.3 June 4, 2018 Abstract We recall the early theoretical speculations on the possible explosive uses of antimatter, from 1946 to the first production of antiprotons, at Berkeley in 1955, and until the first capture of cold antiprotons, at CERN on July 17–18, 1986, as well as the circumstances of the first presentation at a scientific conference of the correct physical processes leading to the ignition of a large scale thermonuclear explosion using less than a few micrograms of antimatter as trigger, at Madrid on June 30th – July 4th, 1986. Preliminary remark This paper will be followed by by Antimatter weapons (1986-2006): From the capture of the first antiprotons to the production of cold antimatter, to appear in 2006. 1 Introduction At CERN (the European Laboratory for Particle Physics), on the evening of the 17 to the 18 of July 1986, antimatter was captured in an electromagnetic trap for arXiv:physics/0507132v2 [physics.hist-ph] 28 Oct 2005 the first time in history. Due to the relatively precarious conditions of this first ∗Expanded version of a paper published in French in La Recherche 17 (Paris, 1986) 1440– 1443; in English in The World Scientist (New Delhi, India, 1987) 74–77, and in Bulletin of Peace Proposals 19 (Oslo,1988) 444–450; and in Finnish in Antimateria-aseet (Kanssainvalinen¨ rauhantutkimuslaitos, Helsinki, 1990, ISBN 951-9193-22-7) 7–18. -
ANTIMATTER a Review of Its Role in the Universe and Its Applications
A review of its role in the ANTIMATTER universe and its applications THE DISCOVERY OF NATURE’S SYMMETRIES ntimatter plays an intrinsic role in our Aunderstanding of the subatomic world THE UNIVERSE THROUGH THE LOOKING-GLASS C.D. Anderson, Anderson, Emilio VisualSegrè Archives C.D. The beginning of the 20th century or vice versa, it absorbed or emitted saw a cascade of brilliant insights into quanta of electromagnetic radiation the nature of matter and energy. The of definite energy, giving rise to a first was Max Planck’s realisation that characteristic spectrum of bright or energy (in the form of electromagnetic dark lines at specific wavelengths. radiation i.e. light) had discrete values The Austrian physicist, Erwin – it was quantised. The second was Schrödinger laid down a more precise that energy and mass were equivalent, mathematical formulation of this as described by Einstein’s special behaviour based on wave theory and theory of relativity and his iconic probability – quantum mechanics. The first image of a positron track found in cosmic rays equation, E = mc2, where c is the The Schrödinger wave equation could speed of light in a vacuum; the theory predict the spectrum of the simplest or positron; when an electron also predicted that objects behave atom, hydrogen, which consists of met a positron, they would annihilate somewhat differently when moving a single electron orbiting a positive according to Einstein’s equation, proton. However, the spectrum generating two gamma rays in the featured additional lines that were not process. The concept of antimatter explained. In 1928, the British physicist was born. -
Ten Years of PAMELA in Space
Ten Years of PAMELA in Space The PAMELA collaboration O. Adriani(1)(2), G. C. Barbarino(3)(4), G. A. Bazilevskaya(5), R. Bellotti(6)(7), M. Boezio(8), E. A. Bogomolov(9), M. Bongi(1)(2), V. Bonvicini(8), S. Bottai(2), A. Bruno(6)(7), F. Cafagna(7), D. Campana(4), P. Carlson(10), M. Casolino(11)(12), G. Castellini(13), C. De Santis(11), V. Di Felice(11)(14), A. M. Galper(15), A. V. Karelin(15), S. V. Koldashov(15), S. Koldobskiy(15), S. Y. Krutkov(9), A. N. Kvashnin(5), A. Leonov(15), V. Malakhov(15), L. Marcelli(11), M. Martucci(11)(16), A. G. Mayorov(15), W. Menn(17), M. Mergè(11)(16), V. V. Mikhailov(15), E. Mocchiutti(8), A. Monaco(6)(7), R. Munini(8), N. Mori(2), G. Osteria(4), B. Panico(4), P. Papini(2), M. Pearce(10), P. Picozza(11)(16), M. Ricci(18), S. B. Ricciarini(2)(13), M. Simon(17), R. Sparvoli(11)(16), P. Spillantini(1)(2), Y. I. Stozhkov(5), A. Vacchi(8)(19), E. Vannuccini(1), G. Vasilyev(9), S. A. Voronov(15), Y. T. Yurkin(15), G. Zampa(8) and N. Zampa(8) (1) University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence, Italy (2) INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy (3) University of Naples “Federico II”, Department of Physics, I-80126 Naples, Italy (4) INFN, Sezione di Naples, I-80126 Naples, Italy (5) Lebedev Physical Institute, RU-119991 Moscow, Russia (6) University of Bari, I-70126 Bari, Italy (7) INFN, Sezione di Bari, I-70126 Bari, Italy (8) INFN, Sezione di Trieste, I-34149 Trieste, Italy (9) Ioffe Physical Technical Institute, RU-194021 St. -
Observation of High-Energy Gamma-Rays with the Calorimetric
Louisiana State University LSU Digital Commons LSU Doctoral Dissertations Graduate School 10-22-2018 Observation of High-Energy Gamma-Rays with the Calorimetric Electron Telescope (CALET) On-board the International Space Station Nicholas Wade Cannady Louisiana State University and Agricultural and Mechanical College, [email protected] Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_dissertations Part of the Instrumentation Commons, and the Other Astrophysics and Astronomy Commons Recommended Citation Cannady, Nicholas Wade, "Observation of High-Energy Gamma-Rays with the Calorimetric Electron Telescope (CALET) On-board the International Space Station" (2018). LSU Doctoral Dissertations. 4736. https://digitalcommons.lsu.edu/gradschool_dissertations/4736 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Doctoral Dissertations by an authorized graduate school editor of LSU Digital Commons. For more information, please [email protected]. OBSERVATION OF HIGH-ENERGY GAMMA-RAYS WITH THE CALORIMETRIC ELECTRON TELESCOPE (CALET) ON-BOARD THE INTERNATIONAL SPACE STATION A Dissertation Submitted to the Graduate Faculty of the Louisiana State University and Agricultural and Mechanical College in partial fulfillment of the requirements for the degree of Doctor of Philosophy in The Department of Physics and Astronomy by Nicholas Wade Cannady B.S., Louisiana State University, 2011 December 2018 To Laura and Mom ii Acknowledgments First and foremost, I would like to thank my partner, Laura, for the constant and unconditional support that she has provided during the research described in this thesis and my studies in general. Without her, this undertaking would not have been possible. -
New Device Uses Biochemistry Techniques to Detect Rare Radioactive Decays 27 March 2018, by Louisa Kellie
New device uses biochemistry techniques to detect rare radioactive decays 27 March 2018, by Louisa Kellie UTA researchers are now taking advantage of a biochemistry technique that uses fluorescence to detect ions to identify the product of a radioactive decay called neutrinoless double-beta decay that would demonstrate that the neutrino is its own antiparticle. Radioactive decay is the breakdown of an atomic nucleus releasing energy and matter from the nucleus. Ordinary double-beta decay is an unusual mode of radioactivity in which a nucleus emits two electrons and two antineutrinos at the same time. However, if neutrinos and antineutrinos are identical, then the two antineutrinos can, in effect, cancel each other, resulting in a neutrinoless decay, with all of the energy given to the two Dr. Ben Jones, UTA assistant professor of physics, who electrons. is leading this research for the American branch of the Neutrino Experiment with Xenon TPC -- Time Projection Chamber or NEXT program. Credit: UTA To find this neutrinoless double-beta decay, scientists are looking at a very rare event that occurs about once a year, when a xenon atom decays and converts to barium. If a neutrinoless UTA researchers are leading an international team double-beta decay has occurred, you would expect developing a new device that could enable to find a barium ion in coincidence with two physicists to take the next step toward a greater electrons of the right total energy. UTA researchers' understanding of the neutrino, a subatomic particle proposed new detector precisely would permit that may offer an answer to the lingering mystery identifying this single barium ion accompanying of the universe's matter-antimatter imbalance. -
Antihydrogen and the Antiproton Magnetic Moment
Gabrielse ATRAP: Context and Status Antihydrogen and the Antiproton Magnetic Moment Gerald Gabrielse Spokesperson for TRAP and ATRAP at CERN Levere tt Pro fesso r o f Phys ics, Har var d Uni ver sit y Gabrielse Context CERN Pursues Fundamental Particle Physics at WWeveegySceseesghatever Energy Scale is Interesting A Long and Noble CERN Tradition 1981 – traveled to Fermilab “TEV or bust” 1985 – different response at CERN wh en I went th ere to try to get access to LEAR antiprotons for qqyg/m measurements and cold antihydrogen It is exciting that there is now • a dedicated storaggge ring for antih ygpydrogen experiments • four international collaborations • too few antiprotons for the demand Gabrielse Pursuing Fundamental Particle Physics atWhtt Whatever Energy Sca le is In teres ting A Long and Noble CERN Tradition 1986 – First trapped antiprotons (TRAP) 1989 – First electron-cooling of trapped antiprotons (TRAP) 1 cm magnetic field 21 MeV antiprotons slow in matter degrader _ + _ CERN’s AD, plus these cold methods make antihydrogen possible Gabrielse Pursuing Fundamental Particle Physics atWhtt Whatever Energy Sca le is In teres ting A Long and Noble CERN Tradition 1981 – traveled to Fermilab “TEV or bust” 1985 – different response at CERN when I went there to try to get access to LEAR antiprotons for q/m measurements and cold antihydrogen LHC: 7 TeV + 7 TeV AD: 5 MeV 100 times 5 x 1016 More trapped ELENA upgrade: 0.1 MeV antiprotons ATRAP: 0.3 milli-eV Gabrielse Physics With Low Energy Antiprotons First Physics: Compare q/m for antiproton -
APS News January 2019, Vol. 28, No. 1
January 2019 • Vol. 28, No. 1 A PUBLICATION OF THE AMERICAN PHYSICAL SOCIETY Plasma physics and plants APS.ORG/APSNEWS Page 3 Highlights from 2018 Blending Paint with Physics The editors of Physics (physics. The experiments sparked a series By Leah Poffenberger aps.org) look back at their favorite of theoretical studies, each attempt- 2018 APS Division of Fluid stories of 2018, from groundbreak- ing to explain this unconventional Dynamics Meeting, Atlanta— ing research to a poem inspired by behavior (see physics.aps.org/ Five years ago, Roberto Zenit, a quantum physics. articles/v11/84). One prediction physics professor at the National Graphene: A New indicates that twisted graphene’s Autonomous University of Mexico, superconductivity might also be Superconductor later reported the first observation was studying biological flows when topological, a desirable property 2018’s splashiest condensed- of the Higgs boson decaying into art historian Sandra Zetina enlisted for quantum computation. matter-physics result came bottom quarks (see physics.aps.org/ him for a project: using fluid from two sheets of graphene. The Higgs Shows up with the articles/v11/91). This decay is the dynamics to uncover the secret Researchers in the USA and Japan Heaviest Quarks most likely fate of the Higgs boson, behind modern art techniques. reported finding superconductiv- After detecting the Higgs boson but it was extremely difficult to At this year’s Division of Fluid ity in stacked graphene bilayers in 2012, the next order of business see above the heavy background Dynamics meeting—his 20th— ids, a person who has developed in which one layer is twisted with was testing whether it behaves as of bottom quarks generated in a Zenit, an APS Fellow and member certain knowledge about the way respect to the other. -
Pursuit of Dark Matter Progresses At
New results from the Alpha Magnetic Spectrometer experiment show that a possible sign of dark matter is within scientists’ reach. Dark matter is a form of matter that neither emits nor absorbs light. Scientists think it is about five times as prevalent as regular matter, but so far have observed it only indirectly. The AMS experiment, which is secured to the side of the International Space Station 250 miles above Earth, studies cosmic rays, high-energy particles in space. A small fraction of these particles may have their origin in the collisions of dark matter particles that permeate our galaxy. Thus it may be possible that dark matter can be detected through measurements of cosmic rays. AMS scientists—based at the AMS control center at CERN research center in Europe and at collaborating institutions worldwide—compare the amount of matter and antimatter cosmic rays of different energies their detector picks up in space. AMS has collected information about 54 billion cosmic ray events, of which scientists have analyzed 41 billion. Theorists predict that at higher and higher energies, the proportion of antimatter particles called positrons should drop in comparison to the proportion of electrons. AMS found this to be true. However, in 2013 it also found that beyond a certain energy—8 billion electronvolts—the proportion of positrons begins to climb steeply. “This means there’s something new there,” says AMS leader and Nobel Laureate Sam Ting of the Massachusetts Institute of Technology and CERN. “It’s totally unexpected.” The excess was a clear sign of an additional source of positrons. -
Theory of Dual Horizonradius of Spacetime Curvature
Preprints (www.preprints.org) | NOT PEER-REVIEWED | Posted: 15 May 2020 doi:10.20944/preprints202005.0250.v1 Theory of Dual Horizon Radius of Spacetime Curvature Mohammed. B. Al Fadhli1* 1College of Science, University of Lincoln, Lincoln, LN6 7TS, UK. Abstract The necessity of the dark energy and dark matter in the present universe could be a consequence of the antimatter elimination assumption in the early universe. In this research, I derive a new model to obtain the potential cosmic topology and the horizon radius of spacetime curvature 푅ℎ(휂) utilising a new construal of the geometry of space inspired by large-angle correlations of the cosmic microwave background (CMB). I utilise the Big Bounce theory to tune the initial conditions of the curvature density, and to avoid the Big Bang singularity and inflationary constraints. The mathematical derivation of a positively curved universe governed by only gravity revealed ∓ horizon solutions. Although the positive horizon is conventionally associated with the evolution of the matter universe, the negative horizon solution could imply additional evolution in the opposite direction. This possibly suggests that the matter and antimatter could be evolving in opposite directions as distinct sides of the universe, such as visualised Sloan Digital Sky Survey Data. Using this model, we found a decelerated stage of expansion during the first ~10 Gyr, which is followed by a second stage of accelerated expansion; potentially matching the tension in Hubble parameter measurements. In addition, the model predicts a final time-reversal stage of spatial contraction leading to the Big Crunch of a cyclic universe. The predicted density is Ω0 = ~1.14 > 1. -
Trapped Antihydrogen in Its Ground State
Trapped Antihydrogen in Its Ground State The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Richerme, Philip. 2012. Trapped Antihydrogen in Its Ground State. Doctoral dissertation, Harvard University. Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:10058466 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Other Posted Material, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#LAA ©2012 - Philip John Richerme All rights reserved. Thesis advisor Author Gerald Gabrielse Philip John Richerme Trapped Antihydrogen in Its Ground State Abstract Antihydrogen atoms (H) are confined in a magnetic quadrupole trap for 15 to 1000 s - long enough to ensure that they reach their ground state. This milestone brings us closer to the long-term goal of precise spectroscopic comparisons of H and H for tests of CPT and Lorentz invariance. Realizing trapped H requires charac- terization and control of the number, geometry, and temperature of the antiproton (p) and positron (e+) plasmas from which H is formed. An improved apparatus and implementation of plasma measurement and control techniques make available 107 p and 4 × 109 e+ for H experiments - an increase of over an order of magnitude. For the first time, p are observed to be centrifugally separated from the electrons that cool them, indicating a low-temperature, high-density p plasma. Determination of the p temperature is achieved through measurement of the p evaporation rate as their con- fining well is reduced, with corrections given by a particle-in-cell plasma simulation.