Making Muonium in Vacuum Atoms Indicate That 50 Per Cent Have Energies of Less Than 5 Kev and 95 Per Cent from C.J

Total Page:16

File Type:pdf, Size:1020Kb

Making Muonium in Vacuum Atoms Indicate That 50 Per Cent Have Energies of Less Than 5 Kev and 95 Per Cent from C.J Nature Vol. 295 11 February 1982 457 Estimates of the energies of the muonium Making muonium in vacuum atoms indicate that 50 per cent have energies of less than 5 keV and 95 per cent from C.J. Batty and G. Marshall of less than 20 ke V. There are two measurements in MuoNIUM is the name given to the simple general the muon will capture and lose an particular which would benefit from atomic state consisting of a positively electron many times before it reaches copious quantities of muonium in vacuum. charged muon and an electron. For atomic thermal energies, and if the likelihood for One is a sensitive search for the conversion and chemical purposes it is aptly described the capture process is large compared with of muonium to antimuonium (µ-e+) which as a light isotope of hydrogen with only that for electron loss as thermalization can be accommodated in some versions of about one-ninth the hydrogen mass. becomes complete, muonium will be the electroweak theory. The interaction of However the properties of its 'nucleus' formed. In most chemical and solid-state muonium with matter drastically reduces make muonium both interesting and useful applications the interaction of muonium the expected conversion rate, so that in physics and chemistry. Two recent with the target material is studied, but this current limits on the process are not papers describe a novel way of forming interaction can be a hindrance when particularly restrictive. The other is the muonium which will extend its use to studying certain other phenomena. It is Lamb shift in muonium, the energy measurements in vacuum. therefore of interest to develop an difference between the 2s ½ and 2p½ states The muon, identified in 1936 in cosmic alternative method of muonium pro­ of the n = 2 atomic level. Since both the ray studies, was one of the earliest of the duction so that measurements can be made muon and the electron are leptons and thus elementary particles to be discovered. But on the atom in vacuum. have no structure, quantum elec­ despite an enormous amount of study and A group working at the LAMPF ac­ trodynamics can predict the Lamb shift a considerable knowledge of its properties, celerator facility in New Mexico has very accurately, in contrast to the case for its existence remains an enigma. Like the recently reported the observation of fast atomic hydrogen. The fast muonium electron and the positron, negative and ("'10 keV) muonium in vacuum (P.R. emerging from the foil in the LAMPF positive muons are weakly interacting Bolton et al. Phys. Rev. Lett. 47, 1441; experiment should contain a 2s component point-like leptons and are not influenced 1981). The authors allowed an intense low­ of about one-eighth the total muonium by the strong interaction felt by hadrons. energy (4 MeV) muon beam to slow down intensity. The muon differs from the electron in a polyethylene degrader before it passed This component was also shown to exist essentially only in its mass, which is 207 through a thin foil target in vacuum. It is in another recent experiment performed by times that of the electron. predicted, on the basis of proton a group from the TRIUMF meson facility It is relatively simple to produce intense, measurements, that a significant fraction in Vancouver, Canada(C.J. Oram et al. J. high-quality muon beams from the decay of the muons emerging with energies less Phys. B14, L789; 1981) using a similar of pions obtained at some particle than 20 keV will be in the form of muon beam and thin foil target. Muonium accelerators. So it has been possible to muonium. produced in the skin of the foil emerged to make a thorough study of the properties of In order to separate the small neutral pass through two successive sets of parallel the muon, and then with this knowledge, to muonium component from the charged plates, used to produce high electric fields use the muon as a tool for measurements in remainder of the beam, a 5 kG magnetic at right angles to the direction of motion of other fields. Thus the spin and magnetic sweeping field is used immediately after the the atoms. The electric fields will introduce moment of the muon, together with the target foil. The neutral particles travel 160 through the Stark effect a 2p component to fact that its weak decay (with a mean cm from the target through the magnetic any 2s state which may be present. Decay lifetime of 2.2 µs) into an electron plus two field to a beam stop. The positrons can then proceed from the 2p to the 1 sstate neutrinos is asymmetric or parity violating, expected from the decay of the muon are by emission of UV light with a lifetime of have been used to give information on the detected in an array of scintillation about 3 ns. The light can be detected by a magnetic fields inside a variety of counters and a NaI detector. If the e+ are wavelength shifter and photomultiplier materials. This technique of muon spin from the decay ofµ + then they should have system mounted close to the second set of rotation, or µSR in analogy with NMR and a characteristic energy spectrum with an plates. A clock is started when a muon is ESR, is a subject of intense interest at endpoint energy of 53 MeV. incident on the thin foil and is stopped several laboratories throughout the world. This characteristic energy spectrum, when an event is recorded by the UV Another application involves the superimposed on a flat background of detection system. formation of muonic atoms, in which a events due to cosmic rays and dominated at If voltage is applied only to the second negative muon is captured in an atomic energies below 30 Me V by counts due to the set of plates the time spectrum should show orbital, effectively replacing one of the electron contamination in the incident three muon components: an exponential electrons. Measurements of the radiation beam, has been observed in the experiment decay due to muon-decay positrons emitted in the subsequent atomic cascade reported. The introduction of a few Torr of incident on the photomultiplier system; a can determine the distribution of charge in helium gas into the normally evacuated flat background due to uncorrelated the nucleus. (< 5 x 10-5 Torr) apparatus causes the events; and a foreground peak, about 150 The formation of muonium is fun­ muonium signal to disappear due to the ns wide, due to muonium in the 2s state damental to experiments with muons in ionizing collisions µ+ e- + He->-µ+ + e- + decaying in the region of high electric field. fields as diverse as quantum electro­ He; the µ+ are then swept away by the The foreground peak should largely dynamics, particle physics, solid-state and magnet, and the background spectrum can disappear when an electric field is applied surface physics, and chemistry. For most be measured. The results show that, for the to the first set of plates, as this would cause applications muonium can be formed by particular muon beam used, the pro­ the 2s state muonium atoms emerging from arresting a beam of energetic positive duction rate for muonium is about 3 x lo-4 the foil to decay rapidly to the ls ground muons in a suitable solid, liquid, or gas per incident µ+ regardless of which of state before they reach the second set of target, in the same way that hydrogen several target foils is used. The conclusions plates and photon detector system. atoms can be formed by stopping proton are consistent with proton beam data and Further experiments are planned to beams. Near the end of its range, the with models of the neutralization process. improve the production of muonium in positive particle loses energy by ionization, vacuum. In this way, the goals of an and in the low-velocity regime (cor­ accurate determination of the Lamb shift responding to less than about 20 keV for C.J. Batty and G. Marshall are at the and a sensitive search for the conversion of muons) there is a high probability that it Rutherford Appleton Laboratory, Chilton, muonium to antimuonium should be will form a neutral muonium atom. In Didcot, Oxfordshire OX11 OQX. achieved. D 0028-0836/ 82/0li0457• 01$01 .00 © 1981 Macmillan Journals Ltd .
Recommended publications
  • The Lamb Shift Experiment in Muonic Hydrogen
    The Lamb Shift Experiment in Muonic Hydrogen Dissertation submitted to the Physics Faculty of the Ludwig{Maximilians{University Munich by Aldo Sady Antognini from Bellinzona, Switzerland Munich, November 2005 1st Referee : Prof. Dr. Theodor W. H¨ansch 2nd Referee : Prof. Dr. Dietrich Habs Date of the Oral Examination : December 21, 2005 Even if I don't think, I am. Itsuo Tsuda Je suis ou` je ne pense pas, je pense ou` je ne suis pas. Jacques Lacan A mia mamma e mio papa` con tanto amore Abstract The subject of this thesis is the muonic hydrogen (µ−p) Lamb shift experiment being performed at the Paul Scherrer Institute, Switzerland. Its goal is to measure the 2S 2P − energy difference in µp atoms by laser spectroscopy and to deduce the proton root{mean{ −3 square (rms) charge radius rp with 10 precision, an order of magnitude better than presently known. This would make it possible to test bound{state quantum electrody- namics (QED) in hydrogen at the relative accuracy level of 10−7, and will lead to an improvement in the determination of the Rydberg constant by more than a factor of seven. Moreover it will represent a benchmark for QCD theories. The experiment is based on the measurement of the energy difference between the F=1 F=2 2S1=2 and 2P3=2 levels in µp atoms to a precision of 30 ppm, using a pulsed laser tunable at wavelengths around 6 µm. Negative muons from a unique low{energy muon beam are −1 stopped at a rate of 70 s in 0.6 hPa of H2 gas.
    [Show full text]
  • Muonium-Antimuonium Conversion Abstract
    SciPost Phys. Proc. 5, 009 (2021) Muonium-antimuonium conversion Lorenz Willmann? and Klaus Jungmann Van Swinderen Institute, University of Groningen, 9747 AA, Groningen, The Netherlands ? [email protected] Review of Particle Physics at PSI doi:10.21468/SciPostPhysProc.5 Abstract The MACS experiment performed at PSI in the 1990s provided an yet unchallenged upper bound on the probability for a spontaneous conversion of the muonium atom, + + M =(µ e−), into its antiatom, antimuonium M =(µ−e ). It comprises the culmination of a series of measurements at various accelerator laboratories worldwide. The experimen- tal limits on the process have provided input and steering for the further development of a variety of theoretical models beyond the standard theory, in particular for mod- els which address lepton number violating processes and matter-antimatter oscillations. Several models beyond the standard theory could be strongly disfavored. There is inter- est in a new measurement and improved sensitivity could be reached by exploiting the time evolution of the conversion process, e.g., at intense pulsed muonium sources. Copyright L. Willmann and K. Jungmann. Received 16-02-2021 This work is licensed under the Creative Commons Accepted 28-04-2021 Check for Attribution 4.0 International License. Published 06-09-2021 updates Published by the SciPost Foundation. doi:10.21468/SciPostPhysProc.5.009 9.1 Introduction + The bound state of a positive muon (µ ) and an electron (e−) is an exotic atom which has been named muonium (M) by V.Telegdi. This exotic atom was first produced and observed by V.W. Hughes and collaborators in 1960 [1].
    [Show full text]
  • Muon Decay 1
    Muon Decay 1 LIFETIME OF THE MUON Introduction Muons are unstable particles; otherwise, they are rather like electrons but with much higher masses, approximately 105 MeV. Radioactive nuclear decays do not release enough energy to produce them; however, they are readily available in the laboratory as the dominant component of the cosmic ray flux at the earth’s surface. There are two types of muons, with opposite charge, and they decay into electrons or positrons and two neutrinos according to the rules + + µ → e νe ν¯µ − − µ → e ν¯e νµ . The muon decay is a radioactiveprocess which follows the usual exponential law for the probability of survival for a given time t. Be sure that you understand the basis for this law. The goal of the experiment is to measure the muon lifetime which is roughly 2 µs. With care you can make the measurement with an accuracy of a few percent or better. In order to achieve this goal in a conceptually simple way, we look only at those muons that happen to come to rest inside our detector. That is, we first capture a muon and then measure the elapsed time until it decays. Muons are rather penetrating particles, they can easily go through meters of concrete. Nevertheless, a small fraction of the muons will be slowed down and stopped in the detector. As shown in Figure 1, the apparatus consists of two types of detectors. There is a tank filled with liquid scintillator (a big metal box) viewed by two photomultiplier tubes (Left and Right) and two plastic scintillation counters (flat panels wrapped in black tape), each viewed by a photomul- tiplier tube (Top and Bottom).
    [Show full text]
  • Hadronic Light-By-Light Contribution to $(G-2) \Mu $ from Lattice QCD: A
    MITP/21-019 CERN-TH-2021-047 Hadronic light-by-light contribution to (g − 2)µ from lattice QCD: a complete calculation En-Hung Chao,1 Renwick J. Hudspith,1 Antoine G´erardin,2 Jeremy R. Green,3 Harvey B. Meyer,1, 4, 5 and Konstantin Ottnad1 1PRISMA+ Cluster of Excellence & Institut f¨urKernphysik, Johannes Gutenberg-Universit¨atMainz, D-55099 Mainz, Germany 2Aix Marseille Univ, Universit´ede Toulon, CNRS, CPT, Marseille, France 3Theoretical Physics Department, CERN, 1211 Geneva 23, Switzerland 4Helmholtz Institut Mainz, Staudingerweg 18, D-55128 Mainz, Germany 5GSI Helmholtzzentrum f¨urSchwerionenforschung, Darmstadt, Germany (Dated: April 7, 2021) We compute the hadronic light-by-light scattering contribution to the muon g 2 − from the up, down, and strange-quark sector directly using lattice QCD. Our calcu- lation features evaluations of all possible Wick-contractions of the relevant hadronic four-point function and incorporates several different pion masses, volumes, and lattice-spacings. We obtain a value of aHlbl = 106:8(14:7) 10−11 (adding statistical µ × and systematic errors in quadrature), which is consistent with current phenomenolog- ical estimates and a previous lattice determination. It now appears conclusive that the hadronic light-by-light contribution cannot explain the current tension between theory and experiment for the muon g 2. − I. INTRODUCTION The anomalous magnetic moment of the muon, aµ (g 2)µ=2, is one of the most precisely measured quantities of the Standard Model (SM)≡ of− particle physics. Its value is of considerable interest to the physics community as, currently, there exists a 3:7σ tension between the experimental determination of Ref.
    [Show full text]
  • Muon Neutrino Mass Without Oscillations
    The Distant Possibility of Using a High-Luminosity Muon Source to Measure the Mass of the Neutrino Independent of Flavor Oscillations By John Michael Williams [email protected] Markanix Co. P. O. Box 2697 Redwood City, CA 94064 2001 February 19 (v. 1.02) Abstract: Short-baseline calculations reveal that if the neutrino were massive, it would show a beautifully structured spectrum in the energy difference between storage ring and detector; however, this spectrum seems beyond current experimental reach. An interval-timing paradigm would not seem feasible in a short-baseline experiment; however, interval timing on an Earth-Moon long baseline experiment might be able to improve current upper limits on the neutrino mass. Introduction After the Kamiokande and IMB proton-decay detectors unexpectedly recorded neutrinos (probably electron antineutrinos) arriving from the 1987A supernova, a plethora of papers issued on how to use this happy event to estimate the mass of the neutrino. Many of the estimates based on these data put an upper limit on the mass of the electron neutrino of perhaps 10 eV c2 [1]. When Super-Kamiokande and other instruments confirmed the apparent deficit in electron neutrinos from the Sun, and when a deficit in atmospheric muon- neutrinos likewise was observed, this prompted the extension of the kaon-oscillation theory to neutrinos, culminating in a flavor-oscillation theory based by analogy on the CKM quark mixing matrix. The oscillation theory was sensitive enough to provide evidence of a neutrino mass, even given the low statistics available at the largest instruments. J. M. Williams Neutrino Mass Without Oscillations (2001-02-19) 2 However, there is reason to doubt that the CKM analysis validly can be applied physically over the long, nonvirtual propagation distances of neutrinos [2].
    [Show full text]
  • Muons: Particles of the Moment
    FEATURES Measurements of the anomalous magnetic moment of the muon provide strong hints that the Standard Model of particle physics might be incomplete Muons: particles of the moment David W Hertzog WHEN asked what the most important strange, bottom and top; and six leptons, issue in particle physics is today, my ABORATORY namely the electron, muon and tau- colleagues offer three burning ques- L lepton plus their associated neutrinos. ATIONAL tions: What is the origin of mass? Why N A different set of particles is respon- is the universe made of matter and not sible for the interactions between these equal parts of matter and antimatter? ROOKHAVEN matter particles in the model. The elec- And is there any physics beyond the B tromagnetic interaction that binds elec- Standard Model? trons to nuclei results from the exchange The first question is being addressed of photons, whereas the strong force by a feverish quest to find the Higgs that binds quarks together inside neut- boson, which is believed to be respon- rons, protons and other hadrons is car- sible for the mass of fundamental par- ried by particles called gluons. The ticles. The Tevatron at Fermilab, which third force in the Standard Model – the is currently running, or the Large Had- weak nuclear interaction, which is re- ron Collider at CERN, which is due sponsible for radioactive decay – is car- to start experiments in 2007, should OWMAN ried by the W and Z bosons. B IPP eventually provide the answer to this R Physicists love the Standard Model, question by detecting the Higgs and but they do not like it.
    [Show full text]
  • Angular Distribution Measurement of Beam-Foil Muonium Part II: Muon Injection Simulation for a New Muon G-2 Experiment
    LAr-12380-T DE93 002178 Part I: Angular Distribution Measurement of Beam-Foil Muonium Part II: Muon Injection Simulation for a New Muon g-2 Experiment Hyo Eun Ahn* 'Guest Scientist at Los Alamos. Department of Physics, Yale University, New Haven, CT 06511-8167. DISTFUDUTiCN Of-' TH5S DOCUMENT 16 f7\\C^ /A\ fl^ir?Trr)/?^i(^ Los A|amos National Laboratoryy L ^© ZAiUaiLI LJ U\VJ& LoL s Alamos.NeAlN w MexicMi o 8754875455 Acknowledgement s I thank my advisor, Vernon Hughes, for his support and guidance throughout the last five years and for providing me an opportunity to work on both muonium experiments at LAMPF and the simulation study on muon g—2 experiment at BNL. I am grateful to Walter Lysenko for introducing me to the simulation study of muon injection and the availability of his help whenever I need. I also like to thank my collaborators for the angular distribution experiment. They are Frank Chmely, Ver- non Hughes, Steve Kittell, Yunan Kuang, Bjorn Matthias, Hans-Jurgen Mundinger, Benwen Ni, Gisbert zu Putlitz, Reiner Schaefer, and Kim Woodle. This experiment would not have been possible without the effort and commitment of these co-workers. Special thanks goes to Bjorn Matthias ior many helpful remarks and discussion from the first stage of data analysis to reading this manuscript. Technical support from LAMPF staff was marvelous. Thanks goes to Jov Ivie, Chandra Pillai, Richard Werbeck, and the LAMPF staff. I appreciate the help of the staff at the data analysis center (DAC) of LAMPF; they are Art Chavez, John Faucett, Elvira Martinez, and Mike Oothoudt.
    [Show full text]
  • Arxiv:1512.01765V2 [Physics.Atom-Ph]
    August12,2016 1:27 WSPCProceedings-9.75inx6.5in Antognini˙ICOLS˙3 page 1 1 Muonic atoms and the nuclear structure A. Antognini∗ for the CREMA collaboration Institute for Particle Physics, ETH, 8093 Zurich, Switzerland Laboratory for Particle Physics, Paul Scherrer Institute, 5232 Villigen-PSI, Switzerland ∗E-mail: [email protected] High-precision laser spectroscopy of atomic energy levels enables the measurement of nu- clear properties. Sensitivity to these properties is particularly enhanced in muonic atoms which are bound systems of a muon and a nucleus. Exemplary is the measurement of the proton charge radius from muonic hydrogen performed by the CREMA collaboration which resulted in an order of magnitude more precise charge radius as extracted from other methods but at a variance of 7 standard deviations. Here, we summarize the role of muonic atoms for the extraction of nuclear charge radii, we present the status of the so called “proton charge radius puzzle”, and we sketch how muonic atoms can be used to infer also the magnetic nuclear radii, demonstrating again an interesting interplay between atomic and particle/nuclear physics. Keywords: Proton radius; Muon; Laser spectroscopy, Muonic atoms; Charge and mag- netic radii; Hydrogen; Electron-proton scattering; Hyperfine splitting; Nuclear models. 1. What atomic physics can do for nuclear physics The theory of the energy levels for few electrons systems, which is based on bound- state QED, has an exceptional predictive power that can be systematically improved due to the perturbative nature of the theory itself [1, 2]. On the other side, laser spectroscopy yields spacing between energy levels in these atomic systems so pre- cisely, that even tiny effects related with the nuclear structure already influence several significant digits of these measurements.
    [Show full text]
  • Experimental Limits for the Electron-Proton Charge Difference and for the Neutron Charge
    790 Session P 1 (II and III) polarized muons were stopped in argon Our recent measurements of the asymmetry para­ at different magnetic fields and for case I pions were meter, a, for various gases at high pressure, done in stopped. The solid curves were obtained from the a free muon precession experiment3), give : analysis of the data and represent the per cent am­ plitude of A compared to the total counting rate. The dashed curves are theoretical line shapes centered in each case at the muonium precession frequency predicted from the measured value of the magnetic field. Resonances are clearly seen in cases II and Since depolarization in this experiment is a necessary III and indicate abundant formation of muonium condition for muonium formation, it can be conclu­ in pure argon. ded that no more than one half of the muons stopping The general conditions required to form muonium in SF6 and 02 form muonium, whereas all of the and to retain its polarization are not well understood. muons may form muonium in A, N2, and N20. From our experiments alone it is not determined In view of the abundant formation of muonium in whether the high purity of the argon gas is required, pure argon, it should be possible to measure the although if they are combined with unpublished hyperfine structure, Av, of muonium with high preci­ negative results of others2) it appears that the purity sion. Comparison of a precise experimental value is essential. If this is indeed true, it seems quite for Av with the theoretical value would provide a likely that free muonium is lost in a chemical reac­ critical test of electrodynamics involving the muon tion in impure argon.
    [Show full text]
  • Explaining Muon G − 2 Data in the Μνssm Arxiv:1912.04163V3 [Hep-Ph]
    Explaining muon g 2 data in the µνSSM − Essodjolo Kpatcha∗a,b, Iñaki Lara†c, Daniel E. López-Fogliani‡d,e, Carlos Muñoz§a,b, and Natsumi Nagata¶f aDepartamento de Física Teórica, Universidad Autónoma de Madrid (UAM), Campus de Cantoblanco, 28049 Madrid, Spain bInstituto de Física Teórica (IFT) UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain cFaculty of Physics, University of Warsaw, Pasteura 5, 02-093 Warsaw, Poland dInstituto de Física de Buenos Aires UBA & CONICET, Departamento de Física, Facultad de Ciencia Exactas y Naturales, Universidad de Buenos Aires, 1428 Buenos Aires, Argentina e Pontificia Universidad Católica Argentina, 1107 Buenos Aires, Argentina fDepartment of Physics, University of Tokyo, Tokyo 113-0033, Japan Abstract We analyze the anomalous magnetic moment of the muon g 2 in the µνSSM. − This R-parity violating model solves the µ problem reproducing simultaneously neu- trino data, only with the addition of right-handed neutrinos. In the framework of the µνSSM, light left muon-sneutrino and wino masses can be naturally obtained driven by neutrino physics. This produces an increase of the dominant chargino-sneutrino loop contribution to muon g 2, solving the gap between the theoretical computation − and the experimental data. To analyze the parameter space, we sample the µνSSM using a likelihood data-driven method, paying special attention to reproduce the cur- rent experimental data on neutrino and Higgs physics, as well as flavor observables such as B and µ decays. We then apply the constraints from LHC searches for events with multi-leptons + MET on the viable regions found. They can probe these regions through chargino-chargino, chargino-neutralino and neutralino-neutralino pair pro- duction.
    [Show full text]
  • Physics of Muonium and Muonium Oscillations
    Physics of muonium and muonium oscillations Alexey A. Petrov1 1Department of Physics and Astronomy Wayne State University, Detroit, MI 48201, USA Precision studies of a muonium, the bound state of a muon and an electron, provide access to physics beyond the Standard Model. We propose that extensive theoretical and experimental studies of atomic physics of a muonium, its decays and muonium-antimuonium oscillations could provide an impact on indirect searches for new physics. An especially clean system to study BSM effects in in the Standard Model at tree level, New Physics degrees lepton sector is muonium Mµ, a QED bound state of a of freedom can effectively compete with the SM parti- positively-charged muon and a negatively-charged elec- cles running in the loop graphs, making their discovery + − tron, jMµi ≡ jµ e i. The main decay channel of the possible. This is, of course, only true provided beyond state is driven by the weak decay of the muon. The av- the Standard Model (BSM) constructions include flavor- erage lifetime of a muonium state τMµ is thus expected violating interactions. In order to probe those we con- to be the same as that of the muon, τµ = (2:1969811 ± sider muonium decays and oscillations. −6 0:0000022) × 10 s [1], apart from the tiny effect due to Denoting the \muon quantum number" by Lµ, FCNC 2 2 2 −10 time dilation, (τMµ −τµ)/τµ = α me=(2mµ) = 6×10 . decays of a muonium would probe ∆Lµ = 1 interactions. Such a lifetime, in principle, is rather long to allow for The effective Lagrangian, L∆Lµ=1, can then be divided precision measurements of muonium's atomic and parti- eff into the dipole part, LD, and a part that involves four- cle physics properties [2].
    [Show full text]
  • RCED-85-96 DOE's Physics Accelerators
    DOE’s Physics Accelerators: Their Costs And Benefits This report provides an inventory of the Department of Energy’s existing and planned high-energy physics and nuclear physics accelerator facilities, identifies their as- sociated costs, and presents information on the benefits being derived from their construction and operation. These facilities are the primary tools used by high-energy and nuclear physicists to learn more about what energy and matter consist of and how their component parts or particles are influenced by the most basic natural forces. Of DOE’s $728 million budget for high-energy physics and nuclear physics during fiscal year 1985, about $372.1 million is earmarked for operating 14 DOE-supported accelerator facilities coast-to-coast. DOE’s investment in these facilities amounts to about $1.2 billion. If DOE’s current plans for adding new facilities are carried out, this investment could grow by about $4.3 billion through fiscal year 1994. Annual facility operating costs wilt also grow by about $230 million, or an increase of about 60 percent over current costs. The primary benefits gained from DOE’s investment in these facilities are new scientific knowledge and the education and training of future physicists. Accor- ding to DOE and accelerator facility officials, accelerator particle beams are also used in other scientific applications and have some medical and industrial applications. GAOIRCED-85-96 B APRIL 1,198s 031763 UNITED STATES GENERAL ACCOUNTING OFFICE WASHINGTON, D.C. 20548 RESOURCES, COMMUNlfY, \ND ECONOMIC DEVELOPMENT DIV ISlON B-217863 The Honorable J. Bennett Johnston Ranking Minority Member Subcommittee on Energy and Water Development Committee on Appropriations United States Senate Dear Senator Johnston: This report responds to your request dated November 25, 1984.
    [Show full text]