Accelerator Physics Third Edition

Total Page:16

File Type:pdf, Size:1020Kb

Accelerator Physics Third Edition Preface Accelerator science took off in the 20th century. Accelerator scientists invent many in- novative technologies to produce and manipulate high energy and high quality beams that are instrumental to progresses in natural sciences. Many kinds of accelerators serve the need of research in natural and biomedical sciences, and the demand of applications in industry. In the 21st century, accelerators will become even more important in applications that include industrial processing and imaging, biomedical research, nuclear medicine, medical imaging, cancer therapy, energy research, etc. Accelerator research aims to produce beams in high power, high energy, and high brilliance frontiers. These beams addresses the needs of fundamental science research in particle and nuclear physics, condensed matter and biomedical sciences. High power beams may ignite many applications in industrial processing, energy production, and national security. Accelerator Physics studies the interaction between the charged particles and elec- tromagnetic field. Research topics in accelerator science include generation of elec- tromagnetic fields, material science, plasma, ion source, secondary beam production, nonlinear dynamics, collective instabilities, beam cooling, beam instrumentation, de- tection and analysis, beam manipulation, etc. The textbook is intended for graduate students who have completed their graduate core-courses including classical mechanics, electrodynamics, quantum mechanics, and statistical mechanics. I have tried to emphasize the fundamental physics behind each innovative idea with least amount of mathematical complication. The textbook may also be used by advanced undergraduate seniors who have completed courses on classical mechanics and electromagnetism. For beginners in accelerator physics, one begins with Secs. 2.I–2.IV in Chapter 2, and follows by Secs. 3.I–3.II in Chapter 3 for the basic betatron and synchrotron motion. The study continues onto Secs. 2.V, 2.VIII, and 3.VII for chromatic aberration and collective beam instabilities. After these basic topics, the rf technology and basic physics of linac are covered in Secs. 3.V, 3.VI, 3.VIII in Chapter 3. The basic accelerator physics course ends with physics of electron storage rings in Chapter 4, and some advanced topics of free electron laser and beam-beam interaction in Chapter 5. For beginners, one should pay great attention to the Floquet transformation of Sec. 2.II that can be used to solve Hill’s equation with perturbations. Similarly, some scaling properties of bunch longitudinal distribution in Sec. 3.II are handy for beam vii viii PREFACE manipulation, data analysis, and machine design. The Hamiltonian formalism and canonical transformation, often used to solve particle motion in this book, can provide a better physics picture in beam dynamics. In this revised edition, I include some recently published information on beam ma- nipulation and detection methods, advanced data analysis. I revise some homework problems, and correct mis-prints in the second Edition. The homework is designed to solve a particular problem by providing step-by-step procedures to minimize frustra- tion. The answer is usually listed at the end of each homework problem so that the result can be used in practical design of accelerator systems. I take this opportunity to enhance the content of Sec. 2.VII. Your comments and criticisms to this revised edition are appreciated. S.Y. Lee Bloomington, Indiana, U.S.A. June 10, 2011 ix Preface to Second Edition Since the appearance of the first edition in 1999, this book has been used as a text- book or reference for graduate-level “Accelerator Physics” courses. I have benefited from questions, criticism and suggestions from colleagues and students. As a re- sponse to these suggestions, the revised edition is intended to provide easier learning explanations and illustrations. Accelerator Physics studies the interaction between the charged particles and elec- tromagnetic field. The applications of accelerators include all branches of sciences and technologies, medical treatment, and industrial processing. Accelerator scientists in- vent many innovative technologies to produce beams with qualities required for each application. This textbook is intended for graduate students who have completed their gradu- ate core-courses including classical mechanics, electrodynamics, quantum mechanics, and statistical mechanics. I have tried to emphasize the fundamental physics behind each innovative idea with least amount of mathematical complication. The textbook may also be used by undergraduate seniors who have completed courses on classical mechanics and electromagnetism. For beginners in accelerator physics, one begins with Secs. 2.1–2.4 in Chapter 2, and follows by Secs. 3.1–3.2 for the basic beta- tron and synchrotron motion. The study continues onto Secs. 2.5, 2.8, and 3.7 for chromatic aberration and collective beam instabilities. After these basic topics, the rf technology and basic physics of linac are covered in Secs. 3.5, 3.6, 3.8 in Chapter 3. The basic accelerator physics course ends with physics of electron storage rings in Chapter 4. I have chosen the Frenet-Serret coordinate-system of (ˆx, s,ˆ zˆ) for the transverse radially-outward, longitudinally-forward, and vertical unit base-vectors with the right- hand rule:z ˆ =x ˆ sˆ. I have also chosen positive-charge to derive the equations of betatron motion for× all sections of the Chapter 2, except a discussion of -signs in ± Eq. (2.22). The sign of some terms in Hill’s equation should be reversed if you solve the equation of motion for electrons in accelerators. The convention of the rf-phase differs in linac and synchrotron communities by φlinac = φsynchrotron (π/2). To be consistent with the synchrotron motion in Chapter 3, I have chosen the− rf-phase convention of the synchrotron community to describe the synchrotron equation of motion for linac in Sec. 3.8. x PREFACE TO SECOND EDITION In this revised edition, I include two special topics: free electron laser (FEL) and beam-beam interaction in Chapter 5. In 2000, several self-amplified spontaneous emission (SASE) FEL experiments have been successfully demonstrated. Many light source laboratories are proposing the fourth generation light source using high gain FEL based on the concept of SASE and high-gain harmonic generation (HGHG). Similarly, the success of high luminosity B-factories indicates that beam-beam in- teraction remains very important to the basic accelerator physics. These activities justify the addition of two introductory topics to the accelerator physics text. Finally, the homework is designed to solve a particular problem by providing step-by-step procedures to minimize frustrations. The answer is usually listed at the end of each homework problem so that the result can be used in practical design of accelerator systems. I would appreciate very much to receive comments and criticism to this revised edition. S.Y. Lee Bloomington, Indiana, U.S.A. November 2004 xi Preface to First Edition The development of high energy accelerators began in 1911 when Rutherford discov- ered the atomic nuclei inside the atom. Since then, high voltage DC and rf acceler- ators have been developed, high-field magnets with excellent field quality have been achieved, transverse and longitudinal beam focusing principles have been discovered, high power rf sources have been invented, high vacuum technology has been improved, high brightness (polarized/unpolarized) electron/ion sources have been attained, and beam dynamics and beam manipulation schemes such as beam injection, accumula- tion, slow and fast extraction, beam damping and beam cooling, instability feedback, etc. have been advanced. The impacts of the accelerator development are evidenced by many ground-breaking discoveries in particle and nuclear physics, atomic and molecular physics, condensed-matter physics, biomedical physics, medicine, biology, and industrial processing. Accelerator physics and technology is an evolving branch of science. As the tech- nology progresses, research in the physics of beams propels advancement in accelerator performance. The advancement in type II superconducting material led to the devel- opment of high-field magnets. The invention of the collider concept initiated research and development in single and multi-particle beam dynamics. Accelerator develop- ment has been impressive. High energy was measured in MeV’s in the 1930’s, GeV’s in the 1950’s, and multi-TeV’s in the 1990’s. In the coming decades, the center of mass energy will reach 10-100 TeV. High intensity was 109 particles per pulse in the 1950’s. Now, the AGS has achieved 6 1013 protons per pulse. We are looking for 1014 protons per bunch for many applications.× The brilliance of synchrotron radiation was about 1012 [photons/s mm2 mrad2 0.1% (∆λ/λ)] from the first-generation light sources in the 1970’s. Now, it reaches 1021, and efforts are being made to reach a brilliance of 1029 1034 in many FEL research projects. − This textbook deals with basic accelerator physics. It is based on my lecture notes for the accelerator physics graduate course at Indiana University and two courses in the U.S. Particle Accelerator School. It has been used as preparatory course material for graduate accelerator physics students doing thesis research at Indiana University. The book has four chapters. The first describes historical accelerator development. The second deals with transverse betatron motion. The third chapter concerns
Recommended publications
  • Accelerator and Beam Physics Research Goals and Opportunities
    Accelerator and Beam Physics Research Goals and Opportunities Working group: S. Nagaitsev (Fermilab/U.Chicago) Chair, Z. Huang (SLAC/Stanford), J. Power (ANL), J.-L. Vay (LBNL), P. Piot (NIU/ANL), L. Spentzouris (IIT), and J. Rosenzweig (UCLA) Workshops conveners: Y. Cai (SLAC), S. Cousineau (ORNL/UT), M. Conde (ANL), M. Hogan (SLAC), A. Valishev (Fermilab), M. Minty (BNL), T. Zolkin (Fermilab), X. Huang (ANL), V. Shiltsev (Fermilab), J. Seeman (SLAC), J. Byrd (ANL), and Y. Hao (MSU/FRIB) Advisors: B. Dunham (SLAC), B. Carlsten (LANL), A. Seryi (JLab), and R. Patterson (Cornell) January 2021 Abbreviations and Acronyms 2D two-dimensional 3D three-dimensional 4D four-dimensional 6D six-dimensional AAC Advanced Accelerator Concepts ABP Accelerator and Beam Physics DOE Department of Energy FEL Free-Electron Laser GARD General Accelerator R&D GC Grand Challenge H- a negatively charged Hydrogen ion HEP High-Energy Physics HEPAP High-Energy Physics Advisory Panel HFM High-Field Magnets KV Kapchinsky-Vladimirsky (distribution) ML/AI Machine Learning/Artificial Intelligence NCRF Normal-Conducting Radio-Frequency NNSA National Nuclear Security Administration NSF National Science Foundation OHEP Office of High Energy Physics QED Quantum Electrodynamics rf radio-frequency RMS Root Mean Square SCRF Super-Conducting Radio-Frequency USPAS US Particle Accelerator School WG Working Group 1 Accelerator and Beam Physics 1. EXECUTIVE SUMMARY Accelerators are a key capability for enabling discoveries in many fields such as Elementary Particle Physics, Nuclear Physics, and Materials Sciences. While recognizing the past dramatic successes of accelerator-based particle physics research, the April 2015 report of the Accelerator Research and Development Subpanel of HEPAP [1] recommended the development of a long-term vision and a roadmap for accelerator science and technology to enable future DOE HEP capabilities.
    [Show full text]
  • Accelerator Physics and Modeling
    BNL-52379 CAP-94-93R ACCELERATOR PHYSICS AND MODELING ZOHREH PARSA, EDITOR PROCEEDINGS OF THE SYMPOSIUM ON ACCELERATOR PHYSICS AND MODELING Brookhaven National Laboratory UPTON, NEW YORK 11973 ASSOCIATED UNIVERSITIES, INC. UNDER CONTRACT NO. DE-AC02-76CH00016 WITH THE UNITED STATES DEPARTMENT OF ENERGY DISCLAIMER This report was prepared as an account of work sponsored by an agency of the Unite1 States Government Neither the United States Government nor any agency thereof, nor any of their employees, nor any of their contractors, subcontractors, 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. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, doea not necessarily constitute or imply its endorsement, recomm.ndation, or favoring by the UnitedStates Government or any agency, contractor or subcontractor thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency, contractor or subcontractor thereof- Printed in the United States of America Available from National Technical Information Service U.S. Department of Commerce 5285 Port Royal Road Springfieid, VA 22161 NTIS price codes: Am&mffi TABLE OF CONTENTS Topic, Author Page no. Forward, Z . Parsa, Brookhaven National Lab. i Physics of High Brightness Beams , 1 M. Reiser, University of Maryland . Radio Frequency Beam Conditioner For Fast-Wave 45 Free-Electron Generators of Coherent Radiation Li-Hua NSLS Dept., Brookhaven National Lab, and A.
    [Show full text]
  • Accelerator Physics Alid Engineering 3Rd Printing
    Handbook of Accelerator Physics alid Engineering 3rd Printing edited by Alexander Wu Chao Stanford Linear Accelerator Center Maury Tigner Carneil University World Scientific lbh NEW JERSEY • LONDON • SINGAPORE • BEIJING • SHANGHAI • HONG KONG • TAIPEI • CHENNAI Table of Contents Preface 1 INTRODUCTION 1 1.1 HOW TO USE THIS BOOK 1 1.2 NOMENCLATURE 1 1.3 FUNDAMENTAL CONSTANTS 3 1.4 UNITS AND CONVERSIONS 4 1.4.1 Units A. W. Chao 4 1.4.2 Conversions M. Tigner 4 1.5 FUNDAMENTAL FORMULAE A. W. Chao 5 1.5.1 Special Functions 5 1.5.2 Curvilinear Coordinate Systems 6 1.5.3 Electromagnetism 6 1.5.4 Kinematical Relations 7 1.5.5 Vector Analysis 8 1.5.6 Relativity 8 1.6 GLOSSARY OF ACCELERATOR TYPES 8 1.6.1 Antiproton Sources J. Peoples, J.P. Marriner 8 1.6.2 Betatron M. Tigner 10 1.6.3 Colliders J. Rees 11 1.6.4 Cyclotron H. Blosser 13 1.6.5 Electrostatic Accelerator J. Ferry 16 1.6.6 FFAG Accelerators M.K. Craddock 18 1.6.7 Free-Electron Lasers C. Pellegrini 21 1.6.8 High Voltage Electrodynamic Accelerators M. Cleland 25 1.6.9 Induction Linacs R. Bangerter 28 1.6.10 Industrial Applications of Electrostatic Accelerators G. Norton, J.L. Duggan 30 1.6.11 Linear Accelerators for Electron G.A. Loew 31 1.6.12 Linear Accelerators for Protons S. Henderson, A. Aleksandrov 34 1.6.13 Livingston Chart J. Rees 38 1.6.14 Medical Applications of Accelerators J. Alonso 38 1.6.14.1 Radiation therapy 38 1.6.14.2 Radioisotopes 40 1.6.15 Microtron P.H.
    [Show full text]
  • Accelerator Physics for Health Physicist by D. Cossairt
    Accelerator Physics for Health Physicists J. Donald Cossairt Ph.D., C.H.P. Applied Scientist III Fermi National Accelerator Laboratory 1 Introduction • Goal is to improve knowledge and appreciation of the art of particle accelerator physics • Accelerator health physicists should understand how the machines work. • Accelerators have unique operational characteristics of importance to radiation protection. – For their own understanding – To promote communication with accelerator physicists, operators, and experimenters • This course will not make you an accelerator PHYSICIST! – Limitations of both time and level prescript that. – For those who want to learn more, academic courses and the U. S. Particle Accelerator School provide much comprehensive opportunities. • Much of the material is found in several of the references. – Particularly clear or unique descriptions are cited among these. 2 A word about notation • Vector notation will be used extensively. – Vectors are printed in italic boldface (e.g., E) – Their corresponding magnitudes are shown in italics (e.g., E). • Variable names generally will follow the published literature. • Consistency has not been achieved. – This author cannot fix that by himself! – Chose to remain close to the literature – Watch the context! 3 Summary of relativistic relationships including Maxwell’s equations • Special theory of relativity is important. • Accelerators work because of Maxwell’s equations. •Therest energy of a particle Wo is connected to its rest mass mo by the speed of light c: 2 Wmcoo= (1) • Total energy W of a particle moving with velocity v is 2 22mco W 1 Wmc== =γ mco γ == , (2) 2 2 1− β , with Wo 1− β β = v/c, m is the relativistic mass, and γ is the relativistic parameter.
    [Show full text]
  • Sarah M. Cousineau
    Sarah M. Cousineau Section Head: Accelerator Science and Technology, Spallation Neutron Source Spallation Neutron Source Phone: +1 865 406 0294 PO Box 2008, MS 6461 [email protected] Oak Ridge, TN 37831-6461 Current Job Responsibilities: • Lead the Accelerator Science and Technology group at the Spallation Neutron Source (SNS) accelerator: § Lead the production, measurement, understanding and analysis of the SNS 1.4 MW H- linac and ring proton beams § Define and oversee a robust R&D program targeted at high intensity, high power beams § Define and oversee an effective mechanical engineering design program that supports both beam operations and accelerator R&D § Manage the beam study program aimed at identifying, understanding, and mitigating accelerator performance limitations § Guide and facilitate strategic plans for accelerator performance improvements, and software tools for efficient modeling and analysis of the beam § Manage the section budget and provide professional development opportunities for staff § Promote a strong culture of safety in all activities § Participate in outreach and professional community service roles Education: • 2003 Ph.D. (Accelerator Physics), Indiana University • 2000 M.S. (Accelerator Physics), Indiana University • 1998 B.S. (Physics, summa cum laude), University of North Dakota Research Interests: • Collective effects in high intensity beams, space charge and instabilities • Novel injection methods for proton drivers • Laser and ion beam interactions • Code development and simulation of high intensity beams • Novel beam diagnostics and measurement techniques • High power beam collimation • High current and duty factor H- ion sources Professional Experience: 07/2020 – present Section Head, Accelerator Science and Technology 01/2016 – 07/2020 Group Leader, Beam Science and Technology group, Spallation Neutron Source 02/2012 – 07/2020 Joint Faculty Professor, Department of Physics and Astronomy, University of Tennessee 1 Sarah M.
    [Show full text]
  • Accelerator Physics of Colliders
    1 31. Accelerator Physics of Colliders 31. Accelerator Physics of Colliders Revised August 2019 by M.J. Syphers (Northern Illinois U.; FNAL) and F. Zimmermann (CERN). This article provides background for the High-Energy Collider Parameter Tables that follow and some additional information. 31.1 Luminosity The number of events, Nexp, is the product of the cross section of interest, σexp, and the time integral over the instantaneous luminosity, L: Z Nexp = σexp × L(t)dt. (31.1) Today’s colliders all employ bunched beams. If two bunches containing n1 and n2 particles collide head-on with average collision frequency fcoll, a basic expression for the luminosity is n1n2 L = fcoll ∗ ∗ F (31.2) 4πσxσy ∗ ∗ where σx and σy characterize the rms transverse beam sizes in the horizontal (bend) and vertical directions at the interaction point, and F is a factor of order 1, that takes into account geometric effects such as a crossing angle and finite bunch length, and dynamic effects, such as the mutual focusing of the two beam during the collision. For a circular collider, fcoll equals the number of bunches per beam times the revolution frequency. In 31.2, it is assumed that the bunches are identical in transverse profile, that the profiles are Gaussian and independent of position along the bunch, and the particle distributions are not altered during bunch crossing. Nonzero beam crossing angles θc in the horizontal plane and long bunches (rms bunch length σz) will reduce the luminosity, 2 1/2 ∗ e.g., by a factor F ≈ 1/(1 + φ ) , where the parameter φ ≡ θcσz/(2σx) is known as the Piwinski angle.
    [Show full text]
  • A Brief History and Review of Accelerators
    A BRIEF HISTORY AND REVIEW OF ACCELERATORS P.J. Bryant CERN, Geneva, Switzerland ABSTRACT The history of accelerators is traced from three separate roots, through a rapid development to the present day. The well-known Livingston chart is used to illustrate how spectacular this development has been with, on average, an increase of one and a half orders of magnitude in energy per decade, since the early thirties. Several present-day accelerators are reviewed along with plans and hopes for the future. 1 . INTRODUCTION High-energy physics research has always been the driving force behind the development of particle accelerators. They started life in physics research laboratories in glass envelopes sealed with varnish and putty with shining electrodes and frequent discharges, but they have long since outgrown this environment to become large-scale facilities offering services to large communities. Although the particle physics community is still the main group, they have been joined by others of whom the synchrotron light users are the largest and fastest growing. There is also an increasing interest in radiation therapy in the medical world and industry has been a long-time user of ion implantation and many other applications. Consequently accelerators now constitute a field of activity in their own right with professional physicists and engineers dedicated to their study, construction and operation. This paper will describe the early history of accelerators, review the important milestones in their development up to the present day and take a preview of future plans and hopes. 2 . HISTORICAL ROOTS The early history of accelerators can be traced from three separate roots.
    [Show full text]
  • Relativity, EM Forces - Historical Introduction
    Accelerator Physics Alex Bogacz (Jefferson Lab) / [email protected] Geoff Krafft (Jefferson Lab/ODU) / [email protected] Timofey Zolkin (U. Chicago/Fermilab) / [email protected] Thomas Jefferson National Accelerator Facility Lecture 1Accelerator− Relativity, Physics EM Forces, Intro Operated by JSA for the U.S. Department of Energy USPAS, Fort Collins, CO, June 10-21, 2013 1 Introductions and Outline Syllabus Week 1 Week 2 Introduction Course logistics, Homework, Exam: http://casa/publications/USPAS_Summer_2013.shtml Relativistic mechanics review Relativistic E&M review, Cyclotrons Survey of accelerators and accelerator concepts Thomas Jefferson National Accelerator Facility Lecture 1Accelerator− Relativity, Physics EM Forces, Intro Operated by JSA for the U.S. Department of Energy 2 Syllabus – week 1 Mon 10 June 0900-1200 Lecture 1 ‘Relativity, EM Forces - Historical Introduction Mon 10 June 1330-1630 Lecture 2 ‘Weak focusing and Transverse Stability’ Tue 11 June 0900-1200 Lecture 3 ‘Linear Optics’ Tue 11 June 1330-1630 Lecture 4 ‘Phase Stability, Synchrotron Motion’ Wed 12 June 0900-1200 Lecture 5 ‘Magnetic Multipoles, Magnet Design’ Wed 12 June 1330-1630 Lecture 6 ‘Particle Acceleration’ Thu 13 June 0900-1200 Lecture 7 ‘Coupled Betatron Motion I’ Thu 13 June 1330-1630 Lecture 8 ‘Synchrotron Radiation’ Fri 14 June 0900-1200 Lecture 9 ‘Coupled Betatron Motion II’ Fri 14 June 1330-1530 Lecture 10 ‘Radiation Distributions’ Thomas Jefferson National Accelerator Facility Lecture 1Accelerator− Relativity, Physics EM Forces, Intro Operated
    [Show full text]
  • PHY 564 Advanced Accelerator Physics
    1 PHY 564 Advanced Accelerator Physics Vladimir N. Litvinenko Yichao Jing Gang Wang Department of Physics & Astronomy, Stony Brook University Collider-Accelerator Department, Brookhaven National Laboratory PHY 564 Fall 2015 Lecture 1 2 Plan to teach you about: • The fundamental physics and in depth exploration of advanced methods of modern particle accelerators • Theoretical concept related to the above • Principle of least actions, relativistic mechanics and E&D, 4D notations • N-dimensional phase space, Canonical transformations, simplecticity and invariants of motion • Relativistic beams, Reference orbit and Accelerator Hamiltonian • Parameterization of linear motion in accelerators, Transport matrices, matrix functions, Sylvester's formula, stability of the motion • Invariants of motion, Canonical transforms to the action and phase variables, emittance of the beam, perturbation methods. Poincare diagrams • Standard problems in accelerators: closed orbit, excitation of oscillations, radiation damping and quantum excitation, natural emittance • Non-linear effects, Lie algebras and symplectic maps • Vlasov and Fokker-Plank equations, collective instabilities & Landau Damping • Spin motion in accelerators • Types and Components of Accelerators PHY 564 Fall 2015 Lecture 1 3 Learning goals • Have full understanding of transverse and longitudinal particles dynamics in accelerators • Being capable of solving problems arising in modern accelerator theory • Understand modern methods in accelerator physics • Being capable to fully understand modern accelerator literature PHY 564 Fall 2015 Lecture 1 4 Materials • Lecture notes presented after each class should be used as the main text. Presently there is no textbook, which covers the material of this course. • Some material can be found in my note which summarizes USPAS lectures: http://www0.bnl.gov/isd/documents/74289.pdf Optional: • H.
    [Show full text]
  • Engineering for Particle Accelerators
    Engineering for Particle Accelerators Vyacheslav Yakovlev U.S. Particle Accelerator School (USPAS) Education in Beam Physics and Accelerator Technology 19 June 2017 Engineering for Particle Accelerators Instructors: Vyacheslav Yakovlev, Timergali Khabiboulline, Thomas Nicol and Vladimir Kashikhin, Fermilab, Batavia One-week course at USPAS 2017, Lisle, Il June 19-23, 2017 Purpose and Audience: The purpose of this course is to give an engineering foundation to the development of modern particle accelerators. This course is suitable for graduate students, senior undergraduate students, and engineers interested in particle accelerator design and development. The course will focus on large-scale proton superconducting linear particle accelerators. Prerequisites Undergraduate-level electromagnetism, classical mechanics, RF and mechanical engineering courses. It is the responsibility of the student to ensure that he or she meets the course prerequisites or has equivalent experience. 2 6/19/2017 V. Yakovlev | Engineering in Particle Accelerators Engineering for Particle Accelerators Objectives Students will learn basic principles of the engineering design of large- scale proton superconducting linear particle accelerators. Upon completing this course, students will be familiar with the principles, approach, and basic technique of the design of the main components in superconducting linear accelerators, and be able to perform basic analysis on their performance. Instructional Method The course will consist of lectures and daily homework assignments on the fundamentals of engineering of superconducting linear particle accelerators. 3 6/19/2017 V. Yakovlev | Engineering in Particle Accelerators Engineering for Particle Accelerators Course Content * The course will cover the fundamentals of accelerator engineering and provide examples and exercises in the practical design of the main accelerator components.
    [Show full text]
  • Tune and Chromaticity Diagnostics
    Tune and chromaticity diagnostics R. J. Steinhagen CERN, Geneva, Switzerland Abstract Tune and chromaticity, the oscillation frequency of the transverse motion and its dependence on the particle's momentum, are important observables that are used to estimate, measure, and control beam stability in circular accelerators. They are also the first, low-order, non-trivial beam parameters that cannot be directly derived by a single beam instrument. This contribution summarizes diagnostics methods to estimate tune and chromaticity and aims to highlight less obvious key experimental aspects. 1 Introduction The beam particle's tune, defined as the frequency of the transverse oscillation, and chromaticity as its dependence on particle momentum, require precise control as they may drive self-amplified instabilities leading to an increase in beam size, chaotic particle motion, and therefore, particle loss. Furthermore, since tune and chromaticity can be measured with great precision and small systematic errors, they provide valuable diagnostics for a variety of higher-order beam physics processes such as measurement of beam optics, effects related to machine impedance, beam–beam, electron-cloud, and other collective effects. The concept of tune and chromaticity in particle accelerators finds analogies in other physics do- mains such as acoustics (e.g., musical string vibration) or light (e.g., refraction and decomposition of light according to its wavelength in prisms and lenses). Similar to the refraction index n that defines the bending angle of light on its wavelength (or equivalently its photon energy), in accelerators chromaticity describes the dependence of the tune on momentum. The range of tunes providing stable beam condi- tions is typically limited.
    [Show full text]
  • Computational Methods in Accelerator Physics
    Computational Methods in Accelerator Physics Robert D. Ryne c Draft date June 22, 2009 ! Contents Contents i Preface 1 1 Single Particle Dynamics and Numerical Integration 3 1.1 Lagrangian and Hamiltonian Dynamics . 3 1.1.1 Coordinate as an Independent Variable . 6 1.1.2 Canonical Transformations . 7 1.2 Numerical Integration . 8 1.3 Runge-Kutta Algorithms . 10 1.4 Adams Schemes . 15 1.5 Symplectic Integration . 16 1.5.1 2nd Order Leap-Frog . 17 1.5.2 Split-Operator Symplectic Integration . 18 1.5.3 The Method of Yoshida . 18 2 Linear Magnetic Optics 23 i ii CONTENTS 2.1 Equations for the Linear Map . 23 2.2 Rectilinear Magnetostatic Elements . 26 2.2.1 Drift Space . 28 2.2.2 Magnetic Quadrupole . 29 2.2.3 Magnetic Solenoid . 32 2.3 Bending Magnets . 34 2.3.1 Ideal Sector Bend . 35 2.4 Accelerating Gap . 37 2.5 Courant-Snyder Theory . 41 2.5.1 Invariant of Motion . 42 2.5.2 Solution of the Equations of Motion . 43 3 Lie Algebraic Methods 47 3.1 Symplectic Matrices and Symplectic Mappings . 47 3.2 Symplectic Mappings and Hamiltonian Dynamics . 49 3.3 Lie Algebraic Tools . 53 3.4 Successive Lie Transformations . 56 3.5 Representation of Transfer Maps . 58 3.6 Computation of Lie Algebraic Maps . 60 4 Multiparticle Dynamics 63 4.1 The Vlasov Equation . 63 4.2 The KV Distribution . 64 4.3 RMS Equations . 70 CONTENTS iii 4.3.1 Overview . 70 4.3.2 Derivation of RMS Equations . 72 4.4 3D RMS Equations .
    [Show full text]