Fundamental Concepts of Particle Accelerators III : High-Energy Beam Dynamics (2) Koji TAKATA KEK. Accelerator Course, Sokendai. Second Term, JFY2012

Similar documents
Accelerator Physics NMI and Synchrotron Radiation. G. A. Krafft Old Dominion University Jefferson Lab Lecture 16

CERN Accelerator School. RF Cavities. Erk Jensen CERN BE-RF

Low Emittance Machines

Fundamental Concepts of Particle Accelerators I : Dawn of Particle Accelerator Technology. Koji TAKATA KEK. Accelerator Course, Sokendai

Fundamental Concepts of Particle Accelerators V : Future of the High Energy Accelerators. Koji TAKATA KEK. Accelerator Course, Sokendai

Low Emittance Machines

CERN Accelerator School. Intermediate Accelerator Physics Course Chios, Greece, September Low Emittance Rings

Koji TAKATA KEK. Accelerator Course, Sokendai. Second Term, JFY2011. Oct.

Fundamental Concepts of Particle Accelerators. Koji TAKATA KEK. Accelerator Course, Sokendai, Second Term, JFY2010

Introduction to Accelerators. Scientific Tools for High Energy Physics and Synchrotron Radiation Research

Contents. LC : Linear Collider. µ-µ Collider. Laser-Plasma Wave Accelerator. Livingston Chart 6 References

Fundamental Concepts of Particle Accelerators V: Future of the High Energy Accelerators VI: References. Koji TAKATA KEK. Accelerator Course, Sokendai

1. (16) A point charge e moves with velocity v(t) on a trajectory r(t), where t is the time in some lab frame.

Synchrotron radiation

Graduate Accelerator Physics. G. A. Krafft Jefferson Lab Old Dominion University Lecture 1

Accelerator Physics Final Exam pts.

3. Synchrotrons. Synchrotron Basics

Longitudinal dynamics Yannis PAPAPHILIPPOU CERN

Single Particle Motion

D. Brandt, CERN. CAS Frascati 2008 Accelerators for Newcomers D. Brandt 1

Lorentz Force. Acceleration of electrons due to the magnetic field gives rise to synchrotron radiation Lorentz force.

Transverse dynamics Selected topics. Erik Adli, University of Oslo, August 2016, v2.21

Longitudinal Dynamics

Lectures on accelerator physics

Linac JUAS lecture summary

Appendix A2. Particle Accelerators and Detectors The Large Hadron Collider (LHC) in Geneva, Switzerland on the Border of France.

Vectors in Special Relativity

Suppression of Radiation Excitation in Focusing Environment * Abstract

Problems of Chapter 1: Introduction

2. X-ray Sources 2.1 Electron Impact X-ray Sources - Types of X-ray Source - Bremsstrahlung Emission - Characteristic Emission

Superconducting RF Accelerators: Why all the interest?

Accelerators Ideal Case

!"#$%$!&'()$"('*+,-')'+-$#..+/+,0)&,$%.1&&/$ LONGITUDINAL BEAM DYNAMICS

Tools of Particle Physics I Accelerators

Electron Linear Accelerators & Free-Electron Lasers

Physics 214 Final Exam Solutions Winter 2017

Compton Scattering I. 1 Introduction

Electrodynamics of Radiation Processes

Radiative Processes in Astrophysics

Short Introduction to CLIC and CTF3, Technologies for Future Linear Colliders

r,t r R Z j ³ 0 1 4π² 0 r,t) = 4π

Introduction to particle accelerators

ELECTRON DYNAMICS WITH SYNCHROTRON RADIATION

Physics 610. Adv Particle Physics. April 7, 2014

Summary of lecture 1 and 2: Main ingredients in LHC success

Fundamentals of Accelerators

RF LINACS. Alessandra Lombardi BE/ ABP CERN

Particles and Universe: Particle accelerators

Phase Space Study of the Synchrotron Oscillation and Radiation Damping of the Longitudinal and Transverse Oscillations

Particle physics experiments

Introduction to Longitudinal Beam Dynamics

Introduction to Particle Accelerators & CESR-C

Acceleration to higher energies

Direct-Current Accelerator

Engines of Discovery

Lecture 1 Introduction to RF for Accelerators. Dr G Burt Lancaster University Engineering

Introduction to Elementary Particle Physics I

Lecture 21 April 15, 2010

Impedance & Instabilities

Why do we accelerate particles?

Accelerator Physics. G. A. Krafft Jefferson Lab Old Dominion University Lecture 2

Accelerator Physics. Tip World Scientific NEW JERSEY LONDON SINGAPORE BEIJING SHANGHAI HONG KONG TAIPEI BANGALORE. Second Edition. S. Y.

Introduction to electron and photon beam physics. Zhirong Huang SLAC and Stanford University

Introduction to accelerators for teachers (Korean program) Mariusz Sapiński CERN, Beams Department August 9 th, 2012

Accelerator Physics Weak Focusing. S. A. Bogacz, G. A. Krafft, S. DeSilva, R. Gamage Jefferson Lab Old Dominion University Lecture 2

Standard Model of Particle Physics SS 2013

Physics 598ACC Accelerators: Theory and Applications

Varying accelerating fields

Special Relativity. Christopher R. Prior. Accelerator Science and Technology Centre Rutherford Appleton Laboratory, U.K.

Accelerator. Physics of PEP-I1. Lecture #7. March 13,1998. Dr. John Seeman

PHYS General Physics for Engineering II FIRST MIDTERM

Columbia University Department of Physics QUALIFYING EXAMINATION

Electrodynamics Exam Solutions

Chapter 2 Radiation of an Accelerated Charge

- Synchrotron emission: A brief history. - Examples. - Cyclotron radiation. - Synchrotron radiation. - Synchrotron power from a single electron

Note. Performance limitations of circular colliders: head-on collisions

Part III. Interaction with Single Electrons - Plane Wave Orbits

Section 4 : Accelerators

Particles and Waves Particles Waves

Accelerator Physics Weak Focussing. A. Bogacz, G. A. Krafft, and T. Zolkin Jefferson Lab Colorado State University Lecture 2

Particle Accelerators. The Electrostatic Accelerators

Introduction to Synchrotron Radiation

ELECTRON DYNAMICS with SYNCHROTRON RADIATION

Bernhard Holzer, CERN-LHC

Introduction to Particle Accelerators Bernhard Holzer, DESY

Relativistic Aspects of the Centripetal Force M. Conte

Cavity basics. 1 Introduction. 2 From plane waves to cavities. E. Jensen CERN, Geneva, Switzerland

CEPC and FCCee parameters from the viewpoint of the beam-beam and electron cloud effects. K. Ohmi (KEK) IAS-HEP, HKUST, Hong Kong Jan.

FYS 3120: Classical Mechanics and Electrodynamics

Radiation by Moving Charges

PHYS 561 (GR) Homework 1 Solutions

Linear and circular accelerators

Physics 8.20 Special Relativity IAP 2008

PH 253 Exam I Solutions

Accelerator Physics and Technologies for Linear Colliders University of Chicago, Physics 575

Astrophysical Radiation Processes

CHARGED PARTICLE MOTION IN CONSTANT AND UNIFORM ELECTROMAGNETIC FIELDS

Historical developments. of particle acceleration

Penning Traps. Contents. Plasma Physics Penning Traps AJW August 16, Introduction. Clasical picture. Radiation Damping.

Emittance Growth and Tune Spectra at PETRA III

Transcription:

.... Fundamental Concepts of Particle Accelerators III : High-Energy Beam Dynamics (2) Koji TAKATA KEK koji.takata@kek.jp http://research.kek.jp/people/takata/home.html Accelerator Course, Sokendai Second Term, JFY2012 Oct. 25, 2012

Contents 1 Dawn of Particle Accelerator Technology 2 High-Energy Beam Dynamics (1) 3 High-Beam Dynamics (2) Beam-beam Collider RF Cavity and Beam Synchrotron Radiation 4 RF Technology 5 Future of the High Energy Accelerators 6 References Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 2 / 1

The Idea of the Collider High-energy physics experiment had been done by colliding high energy beams against a target fixed on the accelerator, i.e. fixed target experiment. The particle reaction, however, depends not on the laboratory energy of the projectile particle, but on the center of mass energy of it and a target particle. The proposal of the colliding-beam machine (collider) by B. Touschek, Frascati Lab., Italy (1960). The first collider AdA (Frascati, 1961): 200 MeV e 200 MeV e + Hence-forward, the collider scheme has become the paradigm of high energy accelerators today. Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 3 / 1

Center of Mass Energy E CM Consider the collision of particles of the same rest mass m. In the rest frame: particle energy in the beam is γmc 2, while that in the target is mc 2. total energy of the two particles: E T = (1 + γ)mc 2. total momentum : p T = βγmc = γ 2 1 mc. Since E 2 c 2 p 2 T is a Lorentz invariant, the total energy in the center of mass frame is E CM (fixed target) = 2γ + 2 mc 2 2γ mc 2 Ḃut if we use a collider, it becomes E CM (collider) = 2γmc 2 E CM (fixed target). Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 4 / 1

Luminosity at Beam-Beam Collision In colliders, very thin beams collide each other. If we put the beam cross section as S and the reaction cross section as σ, the probability of reaction at a single collision is given by σ/s. When each beams comprise N + and N particles, respectively, and collide at a rate of f times per second, the number of reaction per second is f N + N σ S Coefficient of σ is called the luminosity L L = f N + N S In every collider, a great effort is continually paid to maximize the luminosity both at the design stage and at the beam commissioning stage. Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 5 / 1

RF Cavity and Beam (1) The first RF accelerator tried by Rolf Wideröe used electric fields in the gap between drift tubes which are in open space. But this simple scheme has a problem of the radiation loss of the RF power. The gap may be considered as a kind of oscillating electric dipole having a moment p = qd e jωt, where q is the charge induced on the drift tube surface and d the gap length. And the radiation power may be estimated like ω 4 12π µ 0 ε0 µ 0 p 2. It is therefore necessary to enclose the acceleration gap with a metal wall, when both RF field and frequency become ever higher. Acceleration by Cavity Resonator Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 6 / 1

RF Cavity and Beam (2) There are a great variety of RF cavities for the beam acceleration. But each one is a variation of the cylindrical cavity resonating with the lowest resonant mode TM 010. The cavity of this type is often called pillbox cavity. E z (r) J 0 (ξ 01 r/b) and H θ (r) J 1 (ξ 01 r/b), where b is the cavity radius, J n the Bessel function of n th order, and ξ 01 = 2.40483 the lowest zero of J 0. the resonant frequency is ω 01 = ξ 01 b/c. r=b Hθ 0 Ez 2b arbitrary scale 1 0.8 0.6 E z H θ 0.4 d 0.2 0 0.5 1 1.5 2 χ 01 r/b Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 7 / 1

RF Cavity and Beam (3) An example : single cell cavity at KEK Photon Factory 2.5 GeV Storage Ring modified pill-box cavity specification: f RF = 500 MHz, V peak = 0.7 MV r R10mm R234.69mm Ez (r=0) R50mm R91.375mm z 220mm R130mm 300mm Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 8 / 1

RF Cavity and Beam (4) Schematic diagram of accelerating cavity with beam and coupling hole to external RF circuits. RF power from/to external devices beam cavity Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 9 / 1

RF Cavity and Beam (5) Global behaviors of a cavity is represented by an equivalent circuit with three parameters L, C and R. Two equations are straightforward to obtain by using the observed/simulated resonant frequency and Q value: ω 0 = 1/ LC and Q = ω 0 RC. C R L one more equation is wanted to determine the 3 parameters. We must define the voltage. Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 10 / 1

RF Cavity and Beam (6) In order to define the voltage for the equivalent circuit, we add the beam I b = I b e jωt as an external current. In the cavity at a stationary state, the following energy conservation law J E dv + (E H) n ds = 0 V should be satisfied, where J is the current density of the beam, and E and H are EM fields excited by the beam. This equation means that the energy lost by the electric field on the beam orbit should be equal to the power loss on the cavity wall S. S Beam C R L ~ I b Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 11 / 1

RF Cavity and Beam (7) The first term of the equation in the previous page can be interpreted as the effective deceleration voltage V b times the beam current I b. Then the energy generated by the beam is represented as I b V b. This should be equal to the ohmic loss of the circuit: RIb 2. Thus we can define circuit resistance by the relation R = V b /I b with the aid of the voltage defined above and eventually can uniquely define L and C. The R thus defined is called shunt impedance of the accelerating cavity. Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 12 / 1

RF Cavity and Beam (8) The actual cavity system is provided with the external RF generator as shown below. Ig I b External RF Generator ~ Beam C R L ~ The cavity voltage is a phasor sum of voltages generated by I b and I g. Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 13 / 1

Synchrotron Radiation: Theory Synchrotron radiation (SR) is an electric-dipole radiation due to the point charge s transverse acceleration by bending magnetic fields. Radiation power by a charge that is instantaneously at rest is given by Larmor s formula: q 2 ( ) dv 2 P = 6πε 0 mc 3. dt For an electron, in particular, it is written as P = 2r em e 3c ( ) dv 2, dt where r e is the classical electron radius: e 2 r e 4πε 0 m e c 2 = 2.82 10 15 m. Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 14 / 1

Electric-dipole Radiation (1) #1 Radiation pattern in #2 the rest frame of an electric dipole oscillating in #3 the z direction at a frequency ω : #4 the pattern is rotationally #5 symmetric with the z axis #6 λ = 2πc/ω x/xz/λ 0 x e/x 0 x /k 4 η (m) s = 0 s = 0 + nl 2 s = L 2 s = L 4 s = 0 + + nl s = 0 + 0 s = 0 + s = L + nl = 0 + (n + 1)L s/l-2 s (m) f = 1.6L ρ = 50 m -4 L = 2 m 0 1 2 3 4 5 r/λ Fig: Contours of electric field lines Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 15 / 1

Electric-dipole Radiation (2) Let us transform the Larmor s formula P = 2r ( em e dv 3c dt ) 2 = 2r e 3m e c ( ) dp 2. dt to that for the laboratory frame. P is the radiated energy E during a time span t, but energy and time transform in the same manner under the Lorentz transformation. Thus P should have a Lorentz invariant form. For this end, we must find an invariant form for the right-hand side of the above equation. This is achieved through replacing (dp/dt) 2 by (dp/dτ) 2 (de/dτ) 2 /c 2, where dτ is the differential of proper time dτ = dt 2 (dx 2 + dy 2 + dz 2 ) /c 2 = dt/γ. Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 16 / 1

Electric-dipole Radiation (3) Formula in the laboratory frame is then given as follows: Instantaneous radiation power of a single electron: { [d P = 2r ] 2 em e (γv) γ 2 3c dt [ ] } 2 d (γc). dt Radiated energy E per turn of a circular orbit with the radius ρ: E m e c 2 = 4π 3 r e ρ β3 γ 4. Expression in practical units for an electron energy of E e (GeV): E(keV) 88.5 [E e (GeV)] 4 /ρ(m). Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 17 / 1

Electric-dipole Radiation (4) Radiation from a relativistic electron on the circular orbit relativistic electron 1 γ 1 γ 1 γ 1 γ Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 18 / 1

Electric-dipole Radiation (5) Radiation profile in the laboratory frame Radiation profile in the electron s rest frame x, y, z, ct dp/dω sin 2 θ, with Ω being the solid angle and θ the angle from the z axis. Coordinates in laboratory frame are: x = x, y = y, z = γ (z vt), ct = γ (ct vz/c). Projection angle of the x axis and y axis to the z axis: 1/γ. Power radiated in the forward direction is concentrated in the cone with a full angle of 2/γ. An observer can see the light emission only during the period when the electron is running on the arc whose length is 2ρ/γ. Wavelengths for the observer are shortened due to the doppler effect by a factor of (1 v/c) 1 2γ 2. Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 19 / 1

Electric-dipole Radiation (6) Critical Frequency ω c and Wavelength λ c = 2πc/ω c : Power spectrum increases as ω up to around ω c, wherefrom it sharply drops to zero. The critical frequency is given by ω c = 3 2 after Schwinger-Jackson s definition. cγ 3 ρ The radiation is wave-like up to ω c, wherefrom it becomes photon-like (quantum regime). (from wikipedia: synchrotron radiation) Koji Takata (KEK) Fund. Conc. Part. Acc. 3 Acc. Course, Oct. 2012 20 / 1