Nicholas Christofilos and the Astron Project in America's Fusion Program
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論文 / 著書情報 Article / Book Information
論文 / 著書情報 Article / Book Information 題目(和文) 誘導加速シンクロトロンにおける広帯域加速と バリアバケツを用いた ビームハンドリング Title(English) Wide-band acceleration and barrier bucket beam handlings in the induction synchrotron 著者(和文) 由元崇 Author(English) Takashi Yoshimoto 出典(和文) 学位:博士(工学), 学位授与機関:東京工業大学, 報告番号:甲第10210号, 授与年月日:2016年3月26日, 学位の種別:課程博士, 審査員:高山 健,堀岡 一彦,小栗 慶之,長谷川 純,林崎 規託,菊池 崇志 Citation(English) Degree:, Conferring organization: Tokyo Institute of Technology, Report number:甲第10210号, Conferred date:2016/3/26, Degree Type:Course doctor, Examiner:,,,,, 学位種別(和文) 博士論文 Category(English) Doctoral Thesis 種別(和文) 要約 Type(English) Outline Powered by T2R2 (Tokyo Institute Research Repository) Summary “Wide-band acceleration and barrier bucket beam handlings in the induction synchrotron” Since the invention of accelerator at the beginning of the 20th century, so many accelerators has been built and dedicated to the progress in science and technology, especially on the cutting edges of modern particle physics. In the accelerator history, one of the most important inventions is the synchrotron independently invented by Vladimir Veksler and by Edwin McMillan in 1945. It is a circular machine that can produce high energy beams efficiently. The succeeding prominent invention is the principle of strong focusing which was conceived by Nicholas Christofilos in 1949 and found by Ernest Courant, M. Stanley Livingston, and H. Snyder at Brookhaven National Laboratory in 1952 without recognizing the work of Christofilos. The third one is that of separate-function strong-focusing invented by Toshio Kitagaki, which takes a crucial role to realize flexible accelerators such as various synchrotron radiation source or colliders. There are two streams in the frontier of modern synchrotron; one stream is the energy frontier such as Large Hadron Collider (LHC) in the European Organization for Nuclear Research (CERN) and the other is the intensity (or luminosity) frontier such as Japan Proton Accelerator Research Complex (J-PARC) or Super-KEKB in Japan. -
L-Shell and Energy Dependence of Magnetic Mirror Point of Charged
Soni et al. Earth, Planets and Space (2020) 72:129 https://doi.org/10.1186/s40623-020-01264-5 FULL PAPER Open Access L-shell and energy dependence of magnetic mirror point of charged particles trapped in Earth’s magnetosphere Pankaj K. Soni* , Bharati Kakad and Amar Kakad Abstract In the Earth’s inner magnetosphere, there exist regions like plasmasphere, ring current, and radiation belts, where the population of charged particles trapped along the magnetic feld lines is more. These particles keep performing gyration, bounce and drift motions until they enter the loss cone and get precipitated to the neutral atmosphere. Theoretically, the mirror point latitude of a particle performing bounce motion is decided only by its equatorial pitch angle. This theoretical manifestation is based on the conservation of the frst adiabatic invariant, which assumes that the magnetic feld varies slowly relative to the gyro-period and gyro-radius. However, the efects of gyro-motion can- not be neglected when gyro-period and gyro-radius are large. In such a scenario, the theoretically estimated mirror point latitudes of electrons are likely to be in agreement with the actual trajectories due to their small gyro-radius. Nevertheless, for protons and other heavier charged particles like oxygen, the gyro-radius is relatively large, and the actual latitude of the mirror point may not be the same as estimated from the theory. In this context, we have carried out test particle simulations and found that the L-shell, energy, and gyro-phase of the particles do afect their mirror points. Our simulations demonstrate that the existing theoretical expression sometimes overestimates or underesti- mates the magnetic mirror point latitude depending on the value of L-shell, energy and gyro-phase due to underlying guiding centre approximation. -
The Birth and Childhood of a Couple of Twin Brothers V
Proceedings of ICFA Mini-Workshop on Impedances and Beam Instabilities in Particle Accelerators, Benevento, Italy, 18-22 September 2017, CERN Yellow Reports: Conference Proceedings, Vol. 1/2018, CERN-2018-003-CP (CERN, Geneva, 2018) THE BIRTH AND CHILDHOOD OF A COUPLE OF TWIN BROTHERS V. G. Vaccaro, INFN Sezione di Napoli, Naples, Italy Abstract The context in which the concepts of Coupling Imped- Looking Far ance and Universal Stability Charts were born is de- scribed in this paper. The conclusion is that the simulta- Even before the successful achievements of PS and neous appearance of these two concepts was unavoidable. AGS, the scientific community was aware that another step forward was needed. Indeed, the impact of particles INTRODUCTION against fixed targets is very inefficient from the point of view of the energy actually available: for new experi- At beginning of 40’s, the interest around proton accel- ments, much more efficient could be the head on colli- erators seemed to quickly wear out: they were no longer sions between counter-rotating high-energy particles. able to respond to the demand of increasing energy and intensity for new investigations on particle physics. With increasing energy, the energy available in the Inertial Frame (IF) with fixed targets is incomparably Providentially important breakthrough innovations smaller than in the head-on collision (HC). If we want the were accomplished in accelerator science, which pro- same energy in IF using fixed targets, one should build duced leaps forward in the performances of particle ac- gigantic accelerators. In the fixed target case (FT), ac- celerators. cording to relativistic dynamics, an HC-equivalent beam should have the following energy. -
Cyclotrons: Old but Still New
Cyclotrons: Old but Still New The history of accelerators is a history of inventions William A. Barletta Director, US Particle Accelerator School Dept. of Physics, MIT Economics Faculty, University of Ljubljana US Particle Accelerator School ~ 650 cyclotrons operating round the world Radioisotope production >$600M annually Proton beam radiation therapy ~30 machines Nuclear physics research Nuclear structure, unstable isotopes,etc High-energy physics research? DAEδALUS Cyclotrons are big business US Particle Accelerator School Cyclotrons start with the ion linac (Wiederoe) Vrf Vrf Phase shift between tubes is 180o As the ions increase their velocity, drift tubes must get longer 1 v 1 "c 1 Ldrift = = = "# rf 2 f rf 2 f rf 2 Etot = Ngap•Vrf ==> High energy implies large size US Particle Accelerator School ! To make it smaller, Let’s curl up the Wiederoe linac… Bend the drift tubes Connect equipotentials Eliminate excess Cu Supply magnetic field to bend beam 1 2# mc $ 2# mc " rev = = % = const. frf eZion B eZion B Orbits are isochronous, independent of energy ! US Particle Accelerator School … and we have Lawrence’s* cyclotron The electrodes are excited at a fixed frequency (rf-voltage source) Particles remain in resonance throughout acceleration A new bunch can be accelerated on every rf-voltage peak: ===> “continuous-wave (cw) operation” Lawrence, E.O. and Sloan, D.: Proc. Nat. Ac. Sc., 17, 64 (1931) Lawrence, E.O. & Livingstone M.S.: Phys. Rev 37, 1707 (1931). * The first cyclotron patent (German) was filed in 1929 by Leó Szilard but never published in a journal US Particle Accelerator School Synchronism only requires that τrev = N/frf “Isochronous” particles take the same revolution time for each turn. -
Anl-7807 Anl-7807 Survey of Thermonuclear-Reactor
ANL-7807 ANL-7807 SURVEY OF THERMONUCLEAR-REACTOR PARAMETERS P. J. Persiani, W. C. Lipinski, and A. J. Hatcli U of C-AUA-USAECB ARGONNE NATIONAL LABORATORY, ARGONNE, ILLINOIS Prepared for the U.S. ATOMIC ENERGY COMMISSION under Contract W-31-109-Eng-38 The faciliUes of Argonne National Laboratory are owned by the "-'f •> S'^^f °°^^%'" ment. Under the terms of a contract (W-31-109-Eng-38) between the U. S. ""^^^^J^^'J/ Commission, Argonne Universities Association and The University of Chicago, the ""'J'"=">' employs the staff and operates the Laboratory in accordance with policies and programs formu- lated, approved and reviewed by the Association. MEMBERS OF ARGONNE UNIVERSITIES ASSOCIATION The Ohio State University The University of Arizona Kansas State University Carnegie-Mellon University The University of Kansas Ohio University Case Western Reserve University Loyola University The Pennsylvania State University The University of Chicago Marquette University Purdue University University o£ Cincinnati Michigan State University Saint Louis University Illinois Institute of Technology The University of Michigan Southern Illinois University University of Illinois University of Minnesota The University of Texas at Austin Indiana University University of Missouri Washington University Iowa State University Northwestern University Wayne State University The University of Iowa University of Notre Dame The University of Wisconsin NOTICE This report was prepared as an account of work sponsored by the United States Government. Neither the United States nor the United States Atomic Energy Commission, nor any of their employees, nor any of their contractors, subcontrac tors, or their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness or usefulness of any information, apparatus, product or process disclosed, or represents that its use would not infringe privately-owned rights. -
Accelerators, Colliders, and Snakes
P1: FDS October 14, 2003 15:16 Annual Reviews AR199-FM Ernest D. Courant 17 Sep 2003 18:1 AR AR199-NS53-01.tex AR199-NS53-01.sgm LaTeX2e(2002/01/18) P1: IKH 10.1146/annurev.nucl.53.041002.110450 Annu. Rev. Nucl. Part. Sci. 2003. 53:1–37 doi: 10.1146/annurev.nucl.53.041002.110450 Copyright c 2003 by Annual Reviews. All rights reserved ACCELERATORS, COLLIDERS, AND SNAKES Ernest D. Courant Brookhaven National Laboratory, Upton, New York 11973; email: [email protected] Key Words particle accelerators, storage ring, spin, polarized beams PACS Codes 01.60. q, 01.65. g + + ■ Abstract The author traces his involvement in the evolution of particle accelera- tors over the past 50 years. He participated in building the first billion-volt accelerator, the Brookhaven Cosmotron, which led to the introduction of the “strong-focusing” method that has in turn led to the very large accelerators and colliders of the present day. The problems of acceleration of spin-polarized protons are also addressed, with discussions of depolarizing resonances and “Siberian snakes” as a technique for miti- gating these resonances. CONTENTS 1. BEGINNINGS ...................................................... 2 1.1. Growing Up .................................................... 2 1.2. Rochester ...................................................... 4 1.3. Montreal ....................................................... 5 1.4. Cornell ........................................................ 6 2. BROOKHAVEN .................................................... 7 2.1. The Cosmotron -
Effect of Quaslconflned Particles and I= 2 Stellarator Fields on the Negative Mass Lnstablllty in a Modified Betatron G
TABLE II. Coefficients a and b + r of log(ac,) vs log[2/( p 1/p0 +Pel ACKNOWLEDGMENTS p,)J. We thank Jeanette Nelson for a careful reading of the log(ac1 ) =a+ b log(2/( pc/p1 + p 1/p0 ) l when a = 10 manuscript and G. Pollarolo for useful discussions about the NAG FORTRAN LIBRARY. The numerical computations were 0.1 <Pi <Po< 10 carried out on the Vax 11/780 ofINFN Sezione di Torino. M = 100 M=30 M =IO a; b; r 0.44; 0.06; 0.99 0.33; 0.06; 0.98 0.42; 0.04; 0.98 1 where r0 is the Lorentz factor and spans between 1 and 10. A. E. Gill, Phys. Fluids 8, 1428 (1965). The presence of a shear in cylindrical symmetry has not 2 A. Ferrari, B. Trusooni, and L. Zaninetti, Mon. Not. R. Astron. Soc. 196, yet been considered and will presumably produce a cutoff in !OSI (1981). 3H. Cohn, Astrophys. J. 269, 500 (1983). the instabilities where a> 21'Id, with d (in jet radius units) 4 D. G. Payne and H. Cohn, Astrophys. J. 287, 29S (1984). the length characterizing the thickness of the shear. ' A. M. Anile, J.C. Miller, and S. Motta, Phys. Fluids 26, 14SO (1983). Effect of quaslconflned particles and I= 2 stellarator fields on the negative mass lnstablllty in a modified betatron G. Roberts and N. Rostoker Department ofPhy sics, University ofCalifomia, Irvine. California 92717 (Received 5 February 1985; accepted 10 October 1985) A sufficient stability condition for the negative mass instability is derived. -
Los Alamos National Laboratory
Spotlight on National Labs Los Alamos National Laboratory Thom Mason, Director of Los Alamos National Laboratory Alan Carr, Historian of Los Alamos National Laboratory Leslie Sherrill, Group Leader, XTD-IDA (Integrated Design and Assessment) Alexis Trahan, Engineer, NEN-1 (Safeguards Science and Technology) Joetta Goda, Engineer, NEN-2 (Advanced Nuclear Technology) Dave Poston, Chief Reactor Designer, NEN-5 (Systems Design and Analysis) Moderator Nicholas Thompson, Engineer, NEN-2 (Advanced Nuclear Technology) May 6, 2020 ANS Spotlight on National Labs Los Alamos National Laboratory Thom Mason Director of LANL May 6, 2020 LA-UR-20-23309 75+ years serving the nation • In 1943, Los Alamos Laboratory was founded with a single, urgent purpose: build an atomic bomb • The future holds no shortage of national security threats, but there is no shortage of innovative ways to combat those threats • LANL leverages strategic nuclear deterrence to solve challenges to our nation’s security LANL’s national security focus means we are uniquely qualified to tackle big, novel problems such as COVID-19 Los Alamos National Laboratory 4/30/20 | 3 Our 12,866 employees rely on cutting-edge equipment and facilities to solve grand challenges on Earth and in space • 37.8 sq. mile campus (about the size of D.C.) • Flagship research facilities For plutonium, explosives, simulations, chemistry, and more, enabling work that’s impossible anywhere else • Much of our stockpile research is applied to complex challenges in: – Climate change – Vaccine development & epidemic -
Publ. Astron. Obs. Belgrade No. 99 (2020), 256 - 257 Invited Lecture
Publ. Astron. Obs. Belgrade No. 99 (2020), 256 - 257 Invited Lecture CHALLENGES AND PROGRESS ON THE PATH TOWARDS FUSION ELECTRICITY A. J. H. DONNÉ EUROfusion, Garching, Germany E-mail [email protected] Abstract. The European Roadmap to the Realisation of Fusion Energy1 breaks the quest for fusion energy into eight missions: 1. Plasma regimes of operation: Demonstrate plasma scenarios (based on the tokamak configuration) that increase the success margin of ITER and satisfy the requirements of DEMO. 2. Heat-exhaust systems: Demonstrate an integrated approach that can handle the large power leaving ITER and DEMO plasmas. 3. Neutron tolerant materials: Develop materials that withstand the large 14MeV neutron flux for long periods while retaining adequate physical properties. 4. Tritium self-sufficiency: Find an effective technological solution for the breeding blanket that also drives the generators. 5. Implementation of the intrinsic safety features of fusion: Ensure safety is integral to the design of DEMO using the experience gained with ITER. 6. Integrated DEMO design and system development: Bring together the plasma and all the systems coherently, resolving issues by targeted R&D activities 7. Competitive cost of electricity: Ensure the economic potential of fusion by minimising the DEMO capital and lifetime costs and developing long-term technologies to further reduce power plant costs. 8. Stellarator: Bring the stellarator line to maturity to determine the feasibility of a stellarator power plant. Now we are approaching the end of the 8th European Framework Programme (2014- 2020), it is a good moment to look back at the achievements since the establishment of EUROfusion in 2014, while at the same time have a peek into the future, to see which challenges lay ahead of us as well as the strategy to tackle them. -
Spitzer S 100Th: Founding PPPL & Pioneering Work in Fusion Energy
(1) Spitzer’s 100th: Founding PPPL & Pioneering Work in Fusion Energy Greg Hammett (2) Some Stories From Working with Spitzer In the Early Years Russell Kulsrud Princeton Plasma Physics Laboratory Colloquium Dec. 4, 2013 These are shorter versions of talks we gave at the 100th Birthday Celebration for Lyman Spitzer, October 19-20, 2013, Peyton Hall, Princeton University, http://www.princeton.edu/astro/news-events/public-events/spitzer-100/ https://www.princeton.edu/research/news/features/a/?id=11377 Video of a longer talk by Kulsrud, “My Early Years Spent Working with Lyman Spitzer“: https://mediacentral.princeton.edu/id/1_1kil7s0p Thanks for slides: Dale Meade, Rob Goldston, Eleanor Starkman and PPPL photo archives, ... PPPL Historical Photos: https://www.dropbox.com/sh/tjv8lbx2844fxoa/FtubOdFWU2 June 19, 2014: added historical info. Jul 9, 2015: pointer to updated figure Lyman Spitzer Jr.’s 100th: Founding PPPL & Pioneering Work in Fusion Energy Outline: • Pictorial tour: from Spitzer’s early days, the Model-C stellarator (1960’s), to TFTR’s 10 megawatts of fusion & the Hubble Space Telescope (Dec. 9-10, 1993) • Russell Kulsrud: A few personal reflections on early days working with Lyman Spitzer. • The road ahead for fusion: – Interesting ideas being pursued in fusion, to improve confinement & reduce the cost of power plants I never officially met Prof. Spitzer, though I saw him at a few seminars. Heard many stories from Tom Stix, Russell Kulsrud, & others, learned from the insights in his book and his ideas in other books. 2 2 Lyman Spitzer, Jr. 1914-1997 Photo by Orren Jack Turner, from Biographical Memoirs V. -
Signature Redacted %
EXAMINATION OF THE UNITED STATES DOMESTIC FUSION PROGRAM ARCHW.$ By MASS ACHUSETTS INSTITUTE Lauren A. Merriman I OF IECHNOLOLGY MAY U6 2015 SUBMITTED TO THE DEPARTMENT OF NUCLEAR SCIENCE AND ENGINEERING I LIBR ARIES IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF BACHELOR OF SCIENCE IN NUCLEAR SCIENCE AND ENGINEERING AT THE MASSACHUSETTS INSTITUTE OF TECHNOLOGY FEBRUARY 2015 Lauren A. Merriman. All Rights Reserved. - The author hereby grants to MIT permission to reproduce and to distribute publicly Paper and electronic copies of this thesis document in whole or in part. Signature of Author:_ Signature redacted %. Lauren A. Merriman Department of Nuclear Science and Engineering May 22, 2014 Signature redacted Certified by:. Dennis Whyte Professor of Nuclear Science and Engineering I'l f 'A Thesis Supervisor Signature redacted Accepted by: Richard K. Lester Professor and Head of the Department of Nuclear Science and Engineering 1 EXAMINATION OF THE UNITED STATES DOMESTIC FUSION PROGRAM By Lauren A. Merriman Submitted to the Department of Nuclear Science and Engineering on May 22, 2014 In Partial Fulfillment of the Requirements for the Degree of Bachelor of Science in Nuclear Science and Engineering ABSTRACT Fusion has been "forty years away", that is, forty years to implementation, ever since the idea of harnessing energy from a fusion reactor was conceived in the 1950s. In reality, however, it has yet to become a viable energy source. Fusion's promise and failure are both investigated by reviewing the history of the United States domestic fusion program and comparing technological forecasting by fusion scientists, fusion program budget plans, and fusion program budget history. -
Observation of Nuclear Fusion Driven by a Pyroelectric Crystal
letters to nature 1900þ14. I. An interpretive study of BeppoSAX and Ulysses observations. Astrophys. J. 549, electrostatic field of the crystal is used to generate and accelerate 1021–1038 (2001). a deuteron beam (>100 keV and >4 nA), which, upon striking a 10. Gaensler, B. M. et al. Second-epoch VLA observations of SGR 1806220. GRB Circ. Network 2933 (2005). deuterated target, produces a neutron flux over 400 times the 11. Corbel, S. & Eikenberry, S. S. The connection between W31, SGR 1806220, and LBV 1806220: background level. The presence of neutrons from the reaction Distance, extinction, and structure. Astron. Astrophys. 419, 191–201 (2004). D 1 D ! 3He (820 keV) 1 n (2.45 MeV) within the target is 12. Kolpak, M. A., Jackson, J. M., Bania, T. M. & Dickey, J. M. The radial distribution of cold atomic hydrogen in the galaxy. Astrophys. J. 578, 868–876 (2002). confirmed by pulse shape analysis and proton recoil spectro- 13. Corbel, S. et al. The distance of the soft gamma repeater SGR 1806220. Astrophys. J. 478, 624–630 scopy. As further evidence for this fusion reaction, we use a novel (1997). time-of-flight technique to demonstrate the delayed coincidence 14. Hartmann, D. & Burton, W. B. Atlas of Galactic Neutral Hydrogen. Ch. 4, 169 (Cambridge Univ. Press, between the outgoing a-particle and the neutron. Although the Cambridge, 1997). 15. Garwood, R. W. & Dickey, J. M. Cold atomic gas in the inner Galaxy. Astrophys. J. 338, 841–861 (1989). reported fusion is not useful in the power-producing sense, we 16. Figer, D.