Precision Physics with Low-Energy Antiprotons — from Antiproton Decelerator to Flair∗
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Few Electron Paramagnetic Resonances Detection On
FEW ELECTRON PARAMAGNETIC RESONANCES DETECTION TECHNIQUES ON THE RUBY SURFACE By Xiying Li Submitted in partial fulfillment of the requirements For the degree of Doctor of Philosophy Dissertation Adviser: Dr. Massood Tabib-Azar Co-Adviser: Dr. J. Adin Mann, Jr. Department of Electrical Engineering and Computer Science CASE WESTERN RESERVE UNIVERSITY August, 2005 CASE WESTERN RESERVE UNIVERSITY SCHOOL OF GRADUATE STUDIES We hereby approve the dissertation of ______________________________________________________ candidate for the Ph.D. degree *. (signed)_______________________________________________ (chair of the committee) ________________________________________________ ________________________________________________ ________________________________________________ ________________________________________________ ________________________________________________ (date) _______________________ *We also certify that written approval has been obtained for any proprietary material contained therein. Table of Contents TABLE OF CONTENTS ................................................................................................................................. II LIST OF FIGURES ...................................................................................................................................... IV ABSTRACT............................................................................................................................................... VII CHAPTER 1 INTRODUCTION .................................................................................................................1 -
Sp0103 32-36 Gaughan
Atomic Unique Atomic Spectroscopy Aims at Answering a Universal Question Richard Gaughan There is far more matter cover the detailed properties of the than antimatter in our antiproton. In 1930 Paul Dirac theoretically pre- universe, but scientists dicted the existence of these antimatter don’t know enough particles, which are the exact opposite of about the properties of common particles. The positron was ex- perimentally verified in 1932, while the antimatter to understand _ antiproton (p) was not observed until why. By spectroscopically 1955. Why did it take so long to experi- analyzing atoms created mentally identify the antiproton? One reason is that it is essentially nonexistent when antiprotons collide in our earthly environment, and it can with helium, physicists only be produced in particle accelerators at CERN are measuring more powerful than those required to produce positrons. the properties of The absence of antimatter was not a antimatter with subject of much concern until physicists unprecedented accuracy. began to improve our understanding of the origin of the universe. The early uni- verse, filled with dense energy, almost instantaneously expanded to the point where matter condensed from the initial PHOTODISC INCORPORATED PHOTODISC sea of energy. So where is the problem? e live in a universe con- The problem is that our current un- structed from atoms com- derstanding predicts that as the universe posed of light, negatively cooled, both matter and antimatter charged electrons orbiting should have been produced in roughly Wpositively charged protons and un- equivalent quantities. Something has to charged neutrons (both heavy). We account for the observed matter pre- know now that our universe could have dominance in today’s universe, and sci- been predominantly composed of anti- entists around the world are searching matter — atoms with light, positively for possibilities. -
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. -
B1.4 Microwave and Terahertz Spectroscopy
Microwave and terahertz pectroscopy 1063 B1.4 Microwave and terahertz spectroscopy Geoffrey A Blake 8 1.4.1 Introduction Spectroscopy, or the study of the interaction of light with matter. has become one of the major tools of the natural and physical ciences during this century. As the wavelength of the radiation is varied across the electromagnetic spectrum, characteristic properties of atoms, molecule , liquid and solids are probed. In the optical and ultraviolet regions (A. ""' I J-Lm up to 100 nm) it is the electronic structure of the material that is investigated, while at infrared wavelengths (""' 1-30 J-Lm) the vibrational degrees of freedom dominate. Microwave spectroscopy began in 1934 with the observation of the "-'20 GHz absorption spectrum of ammonia by Cleeton and Williams. Here we will consider the mjcrowave region of the electromagnetic spectrum to cover the l to I 00 x I 09 Hz, or I to I 00 GHz (A. ""' 30 em down to 3 mm). range. While the ammonia mjcrowave spectrum probes the inversion motion of this unique pyramidal molecule, more typically microwave spectroscopy is associated with the pure rotational motion of gas phase species. The section of the electromagnetic spectrum extending roughly from 0.1 to I 0 x 10 12 Hz (0.1-1 0 THz, 3- 300 cm- 1) is commonly known as the far-infrared (FIR), submjllimetre or terahertz (THz) region, and therefore lies between the mjcrowave and infrared windows. Accordingly, THz spectroscopy shares both cientific and technological characteri tic with its longer- and shorter-wavelength neighbours. While rich in cientific information, the FIR or THz region of the spectrum has, until recently, been notoriously lacking in good radiation ources--earning the dubious nickname 'the gap in the electromagnetic spectrum'. -
Perspective: Local Ferromagnetic Resonance Measurement Techniques
REVIEW OF SCIENTIFIC INSTRUMENTS 79, 040901 ͑2008͒ Perspective: Local ferromagnetic resonance measurement techniques: “Invited Review Article: Microwave spectroscopy based on scanning thermal microscopy: Resolution in the nanometer range” †Rev. Sci. Instrum. 79, 041101 „2008…‡ Nan Mo and Carl E. Patton Department of Physics, Colorado State University, Fort Collins, Colorado 80523, USA ͑Received 17 March 2008; accepted 31 March 2008; published online 24 April 2008͒ According to Vonsovskii,1 ferromagnetic resonance original Frait/Soohoo schemes at different levels of sophisti- ͑FMR͒ was unknowingly discovered by Arkad’yev in 1911.2 cation. These approaches have never been able to achieve The standard citation for the experimental discovery of FMR spatial resolutions below about 10 m or so. is to Griffiths3 for his observation of the rather broad absorp- In 1988, a new approach to local FMR based on thermal tion profile and an “anomalous” electron paramagnetic reso- effects was introduced by Pelzl16 at Ruhr University, Bo- nance ͑EPR͒ field for in-plane magnetized electroplated fer- chum, Germany. This method has led to a highly sensitive 4,5 romagnetic films. One year later, Kittel explained the and very fine scale FMR measurement capability down to anomalous FMR fields by taking the dynamic demagnetizing 10 nm or so. This technique may be termed “scanning ther- fields into account. FMR is distinct from EPR because the mal FMR microscopy” ͑SThM͒. For the conventional near FMR field or frequency is shifted from the usual range of field local FMR methods introduced above, a single probe pure electron spin resonance values by substantial amounts plays a dual role in both the excitation and detection of the because of both static and dynamic demagnetizing field ef- magnetic response. -
Antiprotonic Helium and CPT Invariance
IOP PUBLISHING REPORTS ON PROGRESS IN PHYSICS Rep. Prog. Phys. 70 (2007) 1995–2065 doi:10.1088/0034-4885/70/12/R01 Antiprotonic helium and CPT invariance Ryugo S Hayano1, Masaki Hori1, Dezso˝ Horvath´ 2,4 and Eberhard Widmann3 1 Department of Physics, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan 2 KFKI Research Institute for Particle and Nuclear Physics, H-1525 Budapest, Hungary 3 Stefan Meyer Institute for Subatomic Physics, Boltzmanngasse 3, A-1090 Vienna, Austria E-mail: [email protected] Received 12 March 2007, in final form 31 July 2007 Published 1 November 2007 Online at stacks.iop.org/RoPP/70/1995 Abstract We review recent progress in the laser and microwave spectroscopy of antiprotonic helium atoms (pHe¯ + ≡ e− − p¯ − He++) carried out at CERN’s Antiproton Decelerator facility (AD). Laser transitions were here induced between Rydberg states (n, ) and (n ± 1, − 1) of pHe¯ + (n ∼ 40 and n − 1 being the principal and orbital angular momentum quantum numbers of the antiproton orbit). Successive refinements in the experimental techniques improved the fractional precision on the pHe¯ + frequencies from 3 parts in 106 to ∼1 part in 108. These included a radiofrequency quadrupole decelerator, which reduced the energy of the antiprotons from 5.3 MeV (the energy of the beam emerging from AD) to ∼100 keV. This enabled the production of pHe¯ + in ultra-low density targets, where collisional effects with other helium atoms are negligible. A continuous wave pulse-amplified dye laser, stabilized against a femtosecond optical frequency comb, was then used to measure the pHe¯ + frequencies with ppb-scale precision. -
Nodal Quasiparticle Dynamics in the Heavy Fermion Superconductor Cecoin5 Revealed by Precision Microwave Spectroscopy
ARTICLE Received 18 Oct 2012 | Accepted 21 Aug 2013 | Published 20 Sep 2013 DOI: 10.1038/ncomms3477 Nodal quasiparticle dynamics in the heavy fermion superconductor CeCoIn5 revealed by precision microwave spectroscopy C.J.S. Truncik1, W.A. Huttema1, P.J. Turner1,S.O¨ zcan2, N.C. Murphy1, P.R. Carrie`re1, E. Thewalt1, K.J. Morse1, A.J. Koenig1, J.L. Sarrao3 & D.M. Broun1 CeCoIn5 is a heavy fermion superconductor with strong similarities to the high-Tc cuprates, including quasi-two-dimensionality, proximity to antiferromagnetism and probable d-wave pairing arising from a non-Fermi-liquid normal state. Experiments allowing detailed com- parisons of their electronic properties are of particular interest, but in most cases are difficult to realize, due to their very different transition temperatures. Here we use low-temperature microwave spectroscopy to study the charge dynamics of the CeCoIn5 superconducting state. The similarities to cuprates, in particular to ultra-clean YBa2Cu3Oy, are striking: the frequency and temperature dependence of the quasiparticle conductivity are instantly recognizable, a consequence of rapid suppression of quasiparticle scattering below Tc; and penetration-depth data, when properly treated, reveal a clean, linear temperature dependence of the quasi- particle contribution to superfluid density. The measurements also expose key differences, including prominent multiband effects and a temperature-dependent renormalization of the quasiparticle mass. 1 Department of Physics, Simon Fraser University, Burnaby, British Columbia, Canada V5A 1S6. 2 Cavendish Laboratory, Madingley Road, Cambridge CB3 0HE, UK. 3 Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA. Correspondence and requests for materials should be addressed to D.M.B. -
Energies and Relativistic Corrections for the Metastable States of Antiprotonic Helium Atoms
VOLUME 79, NUMBER 18 PHYSICAL REVIEW LETTERS 3NOVEMBER 1997 Energies and Relativistic Corrections for the Metastable States of Antiprotonic Helium Atoms V. I. Korobov Joint Institute for Nuclear Research, 141980, Dubna, Russia D. D. Bakalov Institute for Nuclear Research and Nuclear Energy, Tsarigradsko chaussée 72, Sofia 1784, Bulgaria (Received 16 April 1997) We present accurate results for the energy levels of antiprotonic helium atoms with the relativistic and QED corrections of order a4mc2 taken into account. These results reduce the discrepancy between theory and experiment to about 5–10 ppm and rigorously confirm Condo’s model of metastability for the long-lived fraction of antiprotonic helium. The present level of precision enables the unambiguous ascription of quantum numbers to all of the transition lines observed so far. [S0031-9007(97)04162-8] PACS numbers: 36.10.–k, 31.15.Ar Over the past few years a new experimental program The antiprotonic helium atom consists of three particles: has been launched [1] following the discovery that a a helium nucleus, an electron, and an antiproton which sub- fraction of the antiprotons stopped in a helium target stitutes the second electron of the helium atom. The non- survive for a surprisingly long time (tens of microseconds) relativistic Hamiltonian (in atomic units e hÅ me [2]. As suggested by Condo [3] more than 20 years ago, 1) can be written in Jacobian coordinates as the longevity of antiprotons in helium is explained by the 1 1 2 1 2 existence of metastable states of the exotic atom He1pÅ . H 2 DR 2 Dr 2 1 2 , (1) 2M 2m rHe rpÅ R In these states the antiproton, after having substituted one 21 21 21 21 21 of the electrons of the neutral helium atom, settles in where M MHe 1 MpÅ and m me 1 sMHe 1 21 a nearly circular orbit sn, ld with the principal quantum MpÅ d , r is the position vector of the electron with respect number n close to the value MyMe ø 38, where M to the center of mass of the heavy particles, rHe and rpÅ are is the reduced mass of pÅ . -
Spectroscopy of High Rydberg States of Highly Charged Ions and Antiprotonic Helium Atoms
RIKEN Review No. 31 (November, 2000): Focused on Production of Ultra Slow Highly-Charged Ions and Its Application Spectroscopy of high Rydberg states of highly charged ions and antiprotonic helium atoms Hiroyuki A. Torii,∗1 Y. Morishita,∗2 Y. Yamazaki,∗1,∗2 K. Komaki,∗1 K. Kuroki,∗1 R. Hutton,∗3 K. Ishii,∗4 K. Ando,∗2 H. Masuda,∗5 M. Sekiguchi,∗6 M. Hori,∗7 E. Widmann,∗7 and R. S. Hayano∗7 ∗1 Institute of Physics, University of Tokyo, Komaba Campus ∗2 Atomic Physics Laboratory, RIKEN ∗3 Department of Physics, University of Lund, Sweden ∗4 Department of Engineering Science, Kyoto University ∗5 Department of Industrial Chemistry, Tokyo Metropolitan University ∗6 Center for Nuclear Study, University of Tokyo, RIKEN Campus ∗7 Department of Physics, University of Tokyo, Hongo Campus We have performed fluorescence spectroscopy of high Rydberg states of highly charged ions (HCIs) extracted in vacuum using a microcapillary foil target. We identified photons emitted from ions with one electron in a high n Q + Rydberg state, for ∆n = 1 transitions from Q 1 3 states in the VUV-visible-NIR light range. Time- resolved measurements clearly showed radiative cascade, and the initial population was deduced for the first time n Q + by our analysis which revealed that the electrons are preferentially transferred to states around 1, in good agreement with the classical over-barrier model. Also, laser spectroscopy of antiprotonic helium atom is introduced in the latter section to give a hint to the similar time-variant method for the aim of mapping the initial population, which gives an important information of atomic capture process of antiprotons. -
(BRP) COURSE SPECTROSCOPY a by Prof. Dr. Rosari Saleh
TEACHING INSTRUCTIONAL DESIGN (BRP) COURSE SPECTROSCOPY A by Prof. Dr. Rosari Saleh Undergraduate Program in Physics Faculty of Mathematics and Natural Sciences Universitas Indonesia Depok 2020 PREFACE The Learning Design Book (BRP) for the Spectroscopy A course contains a lesson plan for one semester and is compiled as a learning reference for the Spectroscopy A course in the Undergraduate Program at the Department of Physics, Faculty of Mathematics and Natural Sciences UI. The Spectroscopy A course is a compulsory subject for students of the Bachelor of Physics program who major in Condensed Matter Physics. The requirements needed by students to be able to take this course are already taking Basic Physics 3 and Modern Physics courses. The Spectroscopy A lecture which is held in one semester is designed to provide students with a deeper description of the theory of several spectroscopic techniques and their applications. The first unit is an introduction to the characteristics of electromagnetic radiation and the types of interactions that occur between matter and electromagnetic radiation as well as techniques and instrumentation in spectroscopy. The microwave spectroscopy used to identify the rotational characteristics of the molecules is contained in the second unit. The third and fourth units contain techniques and instrumentation in infrared spectroscopy and Raman spectroscopy to identify the structure of matter through the characteristics of vibrations and rotational vibrations of the molecules that make up the material as well as the harmonic oscillator approach. The basic theory, techniques and instrumentation for luminescence spectroscopy are contained in the fifth unit. The sixth unit contains the basic theory, techniques and instrumentation of electron spectroscopy for atoms and molecules. -
A Constraint on Antigravity of Antimatter from Precision Spectroscopy of Simple Atoms*
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Springer - Publisher Connector ISSN 1063-7737, Astronomy Letters, 2009, Vol. 35, No. 10, pp. 663–669. c Pleiades Publishing, Inc., 2009. Published in Russian in Pis’ma v Astronomicheski˘ı Zhurnal, 2009, Vol. 35, No. 10, pp. 736–744. A Constraint on Antigravity of Antimatter from Precision Spectroscopy of Simple Atoms* S. G. Karshenboim** Max-Planck-Institut fur¨ Quantenoptik, Garching, 85748 Germany Mendeleev Institute for Metrology, St. Petersburg, 190005 Russia Received November 28, 2008 Abstract—Consideration of antigravity for antiparticles is an attractive target for various experimental projects. There are a number of theoretical arguments against it but it is not quite clear what kind of experimental data and theoretical suggestions are involved. In this paper we present straightforward arguments against a possibility of antigravity based on a few simple theoretical suggestions and some experimental data. The data are: astrophysical data on rotation of the Solar System in respect to the center of our galaxy and precision spectroscopy data on hydrogen and positronium. The theoretical suggestions for the case of absence of the gravitational field are: equality of electron and positron mass and equality of proton and positron charge. We also assume that QED is correct at the level of accuracy where it is clearly confirmed experimentally. PACS num b e r s : 04.80.Cc; 11.30.Er; 12.20.Fv DOI: 10.1134/S1063773709100028 Key words: Equivalence principle, CPT symmetry, Galactic gravitational field, quantum electrody- namics, precision spectroscopy. INTRODUCTION dominates over any general relativity effects), have the same absolute values for particles and antiparticles; After producing cold antihydrogen atoms via the (iii) the particle–particle and antipartic-le–anti- recombination of positrons and antiprotons [1, 2] a particle gravitational interaction is attractive, while number of possibilities to experimentally test CPT in- the particle–antiparticle one is repulsive. -
Single-Photon Laser Spectroscopy of Cold Antiprotonic Helium
Hyperfine Interaction (2018) 239:44 https://doi.org/10.1007/s10751-018-1518-y Single-photon laser spectroscopy of cold antiprotonic helium Masaki Hori1 © The Author(s) 2018 Abstract Some laser spectroscopy experiments carried out by the Atomic Spectroscopy and Col- lisions Using Slow Antiprotons (ASACUSA) collaboration to measure the single-photon transition frequencies of antiprotonic helium (pHe+ ≡ p+He2+ +e−) atoms are reviewed. The pHe+ were cooled to temperature T = 1.5–1.7 K by buffer-gas cooling in a cryogenic gas target, thus reducing the thermal Doppler width in the single-photon resonance lines. The antiproton-to-electron mass ratio was determined as Mp/me = 1836.1526734(15) by comparisons with the results of three-body quantum electrodynamics calculations. This agreed with the known proton-to-electron mass ratio. Keywords Antiprotonic helium · CPT symmetry · Exotic atoms 1 Introduction Metastable antiprotonic helium (pHe+ ≡ p + He2+ + e−) is a three-body atom composed of a helium nucleus, an electron in the ground state, and an antiproton occupying a Ryd- berg state of principal and orbital angular momentum quantum numbers n ∼ − 1 ∼ 38 [1–3]. By measuring its transition frequencies by laser spectroscopy [4–7], and comparing the values with the results of three-body quantum electrodynamics (QED) calculations, the antiproton-to-electron mass ratio Mp/me can in principle be determined with a relative pre- cision of < 10−11. This corresponds to the best determinations of the proton-to-electron + mass ratio Mp/me from Penning trap experiments [8–12], or laser spectroscopy of HD molecular ions [13–15].