From Radium to Antihydrogen
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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, -
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. -
Download Report 2010-12
RESEARCH REPORt 2010—2012 MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science Cover: Aurora borealis paintings by William Crowder, National Geographic (1947). The International Geophysical Year (1957–8) transformed research on the aurora, one of nature’s most elusive and intensely beautiful phenomena. Aurorae became the center of interest for the big science of powerful rockets, complex satellites and large group efforts to understand the magnetic and charged particle environment of the earth. The auroral visoplot displayed here provided guidance for recording observations in a standardized form, translating the sublime aesthetics of pictorial depictions of aurorae into the mechanical aesthetics of numbers and symbols. Most of the portait photographs were taken by Skúli Sigurdsson RESEARCH REPORT 2010—2012 MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science Introduction The Max Planck Institute for the History of Science (MPIWG) is made up of three Departments, each administered by a Director, and several Independent Research Groups, each led for five years by an outstanding junior scholar. Since its foundation in 1994 the MPIWG has investigated fundamental questions of the history of knowl- edge from the Neolithic to the present. The focus has been on the history of the natu- ral sciences, but recent projects have also integrated the history of technology and the history of the human sciences into a more panoramic view of the history of knowl- edge. Of central interest is the emergence of basic categories of scientific thinking and practice as well as their transformation over time: examples include experiment, ob- servation, normalcy, space, evidence, biodiversity or force. -
Chapter 1 the Biography of a Trafficking Material
Trafficking Materials and Maria Rentetzi Gendered Experimental Practices Chapter 1 The Biography of a Trafficking Material In 1904, an article titled "Radium and Radioactivity" appeared in Century 1 Magazine, a monthly popular magazine published from 1881 to 1930. The article presents Marie Curie's personal account of the discovery of radium and radioactivity. In the article, Curie discusses in depth her arduous attempts to study the radiation of the compounds of uranium and that of known chemical elements, hoping to discover more which are endowed with atomic radioactivity. She revels that it was the chemists who supplied her with the materials she needed. "As I desired to make a very thorough investigation, I had resource to different chemists, who put at my disposal specimens—in some cases the only ones in existence—containing very rare elements." Her next step was to examine different minerals, especially the oxide of uranium 2 ore (pitchblende). To her great surprise, this specimen was found to be four times more active than oxide of uranium itself. The explanation was more than obvious. "The ore must contain a substance more radioactive than uranium and thorium, and this substance must necessarily be a chemical element as yet unknown."1 Her attempts to isolate the new element would lead Marie and Pierre Curie, who joined her research shortly after, to the discovery of both polonium and radium, to the Nobel Prize in Physics in 1903, and to a second Nobel Prize in 1911, this time in chemistry. This chapter attempts to present a cultural -
What Is the Use of the History of Geology to a Practicing Geologist? the Propaedeutical Case of Stratigraphy
What Is the Use of the History of Geology to a Practicing Geologist? The Propaedeutical Case of Stratigraphy A. M. Celâl Şengör* İstanbul Teknik Üniversitesi (İTÜ) Maden Fakültesi ve Avrasya Yerbilimleri Enstitüsü, Ayazağa 34810, Istanbul, Turkey ABSTRACT A practicing geologist can benefit from the history of geology professionally in two main ways: by learning about past mistakes so as not to repeat them and by finding out about different ways to discovery. In this article, I discuss some aspects of the history of stratigraphy and point out that the concept of a stratum has shoehorned geologists into thinking time and rock equivalent, which has led to some serious misinterpretations of geological phenomena, such as the timing of orogenic events and the charting of sea level changes. I call this the “tyranny of strata.” The very name of stratigraphy comes from strata, but what it does is simply deduce temporal relations from spatial relations of rock bodies, including fossils, by making certain assumptions about processes, that is, invoking inevitably a hypo- thetical step. What we have learned from looking at the history of geology is that empirical stratal correlation, even when well controlled by index fossils, can never yield perfect temporal correlation, and any assumption that it does is doomed to failure. Geology progresses in a direction that it may soon be possible to date every package of rock in a way to know what process is being dated and where exactly. We can correlate only processes in time hypothetically, not rock bodies empirically. This is the most important lesson a stratigrapher ought to have learned from the history of his or her subject. -
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 -
Kerne, Kooperation Und Konkurrenz. Kernforschung In
Wissenschaft, Macht und Kultur in der modernen Geschichte Herausgegeben von Mitchell G. Ash und Carola Sachse Band 3 Silke Fengler Kerne, Kooperation und Konkurrenz Kernforschung in Österreich im internationalen Kontext (1900–1950) 2014 Böhlau Verlag Wien Köln Weimar The research was funded by the Austrian Science Fund (FWF) : P 19557-G08 Bibliografische Information der Deutschen Nationalbibliothek: Die Deutsche Nationalbibliothek verzeichnet diese Publikation in der Deutschen Nationalbibliografie; detaillierte bibliografische Datensind im Internet über http://dnb.d-nb.de abrufbar. Umschlagabbildung: Zusammentreffen in Hohenholte bei Münster am 18. Mai 1932 anlässlich der 37. Hauptversammlung der deutschen Bunsengesellschaft für angewandte physikalische Chemie in Münster (16. bis 19. Mai 1932). Von links nach rechts: James Chadwick, Georg von Hevesy, Hans Geiger, Lili Geiger, Lise Meitner, Ernest Rutherford, Otto Hahn, Stefan Meyer, Karl Przibram. © Österreichische Zentralbibliothek für Physik, Wien © 2014 by Böhlau Verlag Ges.m.b.H & Co. KG, Wien Köln Weimar Wiesingerstraße 1, A-1010 Wien, www.boehlau-verlag.com Alle Rechte vorbehalten. Dieses Werk ist urheberrechtlich geschützt. Jede Verwertung außerhalb der engen Grenzen des Urheberrechtsgesetzes ist unzulässig. Lektorat: Ina Heumann Korrektorat: Michael Supanz Umschlaggestaltung: Michael Haderer, Wien Satz: Michael Rauscher, Wien Druck und Bindung: Prime Rate kft., Budapest Gedruckt auf chlor- und säurefrei gebleichtem Papier Printed in Hungary ISBN 978-3-205-79512-4 Inhalt 1. Kernforschung in Österreich im Spannungsfeld von internationaler Kooperation und Konkurrenz ....................... 9 1.1 Internationalisierungsprozesse in der Radioaktivitäts- und Kernforschung : Eine Skizze ...................... 9 1.2 Begriffsklärung und Fragestellungen ................. 10 1.2.2 Ressourcenausstattung und Ressourcenverteilung ......... 12 1.2.3 Zentrum und Peripherie ..................... 14 1.3 Forschungsstand ........................... 16 1.4 Quellenlage ............................. -
The Historical Background
01 orestes part 1 10/24/01 3:40 PM Page 1 Part I The Historical Background The idea that continents move was first seriously considered in the early 20th century, but it took scientists 40 years to decide that it was true. Part I describes the historical background to this question: how scientists first pondered the question of crustal mobility, why they rejected the idea the first time around, and how they ultimately came back to it with new evidence, new ideas, and a global model of how it works. 01 orestes part 1 10/24/01 3:40 PM Page 2 01 orestes part 1 10/24/01 3:40 PM Page 3 Chapter 1 From Continental Drift to Plate Tectonics Naomi Oreskes Since the 16th century, cartographers have noticed the jigsaw-puzzle fit of the continental edges.1 Since the 19th century, geol- ogists have known that some fossil plants and animals are extraordinar- ily similar across the globe, and some sequences of rock formations in distant continents are also strikingly alike. At the turn of the 20th cen- tury, Austrian geologist Eduard Suess proposed the theory of Gond- wanaland to account for these similarities: that a giant supercontinent had once covered much or all of Earth’s surface before breaking apart to form continents and ocean basins. A few years later, German meteo- rologist Alfred Wegener suggested an alternative explanation: conti- nental drift. The paleontological patterns and jigsaw-puzzle fit could be explained if the continents had migrated across the earth’s surface, sometimes joining together, sometimes breaking apart. -
![Patentable Subject [Anti]Matter](https://docslib.b-cdn.net/cover/7169/patentable-subject-anti-matter-1657169.webp)
Patentable Subject [Anti]Matter
PATENTABLE SUBJECT [ANTI]MATTER Whether antihydrogen qualifies as patentable subject matter for the purposes of the United States patent law is not an easy question. In general, man-made inventions and new compositions of matter are proper subjects of patent protection, while products of nature are not. Antihydrogen, a newly created element made entirely of antimatter, has qualities of both a newly created composition of matter and a product of nature. As a result, antihydrogen approaches the theoretical boundaries of the product of nature doctrine because mankind finally has the opportunity to create for the very first time an element that has probably never existed before in the entire universe. This iBrief will begin by briefly explaining antimatter and antihydrogen. Then, a distinction will be drawn between a man-made invention and a product of nature by analyzing relevant case law. Finally, antihydrogen will be analyzed as hypothetical subject matter under the United States patent laws without considering the further requirements of novelty and non-obviousness. An Overview of Antimatter and Antihydrogen Antimatter In 1930, the theoretical physicist Paul Dirac predicted that for every particle of matter, there exists an equivalent particle of antimatter.1 The existence of antimatter was confirmed in 1933 with the discovery of the positron, the antimatter pair of the electron.2 The theory does not mean to say that every proton in the universe must have a ghostly antiproton pair; rather it simply means that matter in the universe can be made of “real” matter, like protons and electrons, or it can be made of antimatter, like antiprotons and positrons. -
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. -
Antihydrogen Synthesis Via Magnetobound States of Protonium Within Proton-Positron-Antiproton Plasmas
43rd EPS Conference on Plasma Physics P4.112 Antihydrogen Synthesis Via Magnetobound States of Protonium Within Proton-Positron-Antiproton Plasmas M. Hermosillo, C. A. Ordonez University of North Texas, Denton, Texas, USA Through classical trajectory simulation, the possibility that antihydrogen can be synthesized via three body recombination involving magnetobound protonium is studied. It has been previ- ously reported that proton-antiproton collisions can result in a correlated drift of the particles perpendicular to a magnetic field. While the two particles are in their correlated drift, they are referred to as a magnetobound protonium system. Possible three body recombination resulting in bound state antihydrogen is studied when a magnetobound protonium system encounters a positron. The simulation incorporates a uniform magnetic field. A visual search and an energy analysis was done in an attempt to find parameters for which the positron is captured into a bound state with an antiproton, resulting in the formation of antihydrogen. Recently, simulations have shown that within a low temperature plasma containing protons and antiprotons, binary collisons invloving proton-antiproton pairs can cause them to become bound temporarily and experience giant cross-magnetic field drifts [1, 2]. These particle pairs have been referred to as being in a magnetobound state, which could serve as a useful intermedi- ate step in the production of neutral antimatter. Magnetobound states occur in low temperatures and strong magnetic fields such as those found inside Penning traps that produce antihydrogen. The possibility of three body recombination resulting in bound state antihydrogen is studied when a magnetobound protonium system encounters a positron. The interactions between particles throughout the simulation are treated classically.