LONGITUDINAL BEAM DYNAMICS

Size: px
Start display at page:

Download "LONGITUDINAL BEAM DYNAMICS"

Transcription

1 LONGITUDINAL BEAM DYNAMICS Frank Tecker CERN, BE-OP Basics of Accelerator Science and Technology at CERN Chavannes de Bogis, 4-8 November November 013 1

2 Summary of the 3 lectures: Acceleration methods Accelerating structures Phase Stability + Energy-Phase oscillations (Linac) Circular accelerators: Cyclotron / Synchrotron Dispersion Effects in Synchrotron Longitudinal Phase Space Motion Stationary Bucket Injection Matching Two more related lectures: Linacs Maurizio Vretanar RF Systems - Erk Jensen CAS@CERN, 4-8 November 013

3 Main Characteristics of an Accelerator Newton-Lorentz Force on a charged particle: ACCELERATION is the main job of an accelerator. It provides kinetic energy to charged particles, hence increasing their momentum. In order to do so, it is necessary to have an electric field E preferably along the direction of the initial momentum (z). dp dt = ee z BENDING is generated by a magnetic field perpendicular to the plane of the particle trajectory. The bending radius ρ obeys to the relation : p = Bρ e F = d p dt = e E + v B ( ) in practical units: nd term always perpendicular to motion => no acceleration B ρ [Tm] p [GeV/c] 0.3 FOCUSING is a second way of using a magnetic field, in which the bending effect is used to bring the particles trajectory closer to the axis, hence to increase the beam density. CAS@CERN, 4-8 November 013 3

4 Basics of Acceleration Today s accelerators and future projects work/aim at the TeV energy range. LHC: 7 TeV -> 14 TeV CLIC: 3 TeV HE/VHE-LHC: 33/100 TeV In fact, this energy unit comes from acceleration: 1 ev (electron Volt) is the energy that 1 elementary charge e (like one electron or proton) gains when it is accelerated in a potential (voltage) difference of 1 Volt. Basic Unit: ev (electron Volt) kev = 1000 ev = 10 3 ev MeV = 10 6 ev GeV = 10 9 ev TeV = 10 1 ev LHC = ~450 Million km of batteries!!! 3x distance Earth-Sun CAS@CERN, 4-8 November 013 4

5 Electrostatic Acceleration source E ΔV vacuum envelope Electrostatic Field: Force: F = d p dt = e E Energy gain: W = e ΔV used for first stage of acceleration: particle sources, electron guns, x-ray tubes Limitation: isolation problems maximum high voltage (~ 10 MV) 750 kv Cockroft-Walton generator at Fermilab (Proton source) CAS@CERN, 4-8 November 013 5

6 Methods of Acceleration: Time varying fields The electrostatic field is limited by insulation, the magnetic field does not accelerate. From Maxwell s Equations: E = φ A t B = µ H = A The electric field is derived from a scalar potential φ and a vector potential A The time variation of the magnetic field H generates an electric field E or E = B t The solution: => time varying electric fields - Induction - RF frequency fields CAS@CERN, 4-8 November 013 6

7 Acceleration by Induction: The Betatron It is based on the principle of a transformer: - primary side: large electromagnet - secondary side: electron beam. The ramping magnetic field is used to guide particles on a circular trajectory as well as for acceleration. Limited by saturation in iron (~300 MeV e-) Used in industry and medicine, as they are compact accelerators for electrons vacuum pipe side view beam B f iron yoke coil time top view R E beam Donald Kerst with the first betatron, invented at the University of Illinois in 1940 CAS@CERN, 4-8 November B f B

8 Radio-Frequency (RF) Acceleration Electrostatic acceleration limited by isolation possibilities => use RF fields Wideröe-type structure Cylindrical electrodes (drift tubes) separated by gaps and fed by a RF generator, as shown above, lead to an alternating electric field polarity Synchronism condition L = v T/ v = particle velocity T = RF period Similar for standing wave cavity as shown (with v c) D.Schulte CAS@CERN, 4-8 November 013 8

9 RF acceleration: Alvarez Structure g Used for protons, ions (50 00 MeV, f ~ 00 MHz) L 1 L L 3 L 4 L 5 Synchronism condition L ( g << L) = v T = β λ s RF s RF RF generator LINAC 1 (CERN) ω = π RF v s L CAS@CERN, 4-8 November 013 9

10 Resonant RF Cavities - Considering RF acceleration, it is obvious that when particles get high velocities the drift spaces get longer and one looses on the efficiency. => The solution consists of using a higher operating frequency. - The power lost by radiation, due to circulating currents on the electrodes, is proportional to the RF frequency. => The solution consists of enclosing the system in a cavity which resonant frequency matches the RF generator frequency. - The electromagnetic power is now constrained in the resonant volume - Each such cavity can be independently powered from the RF generator - Note however that joule losses will occur in the cavity walls (unless made of superconducting materials) CAS@CERN, 4-8 November

11 E z H θ The Pill Box Cavity From Maxwell s equations one can derive the wave equations: A A ε 0 µ 0 = 0 (A = E or H ) t Solutions for E and H are oscillating modes, at discrete frequencies, of types TM xyz (transverse magnetic) or TE xyz (transverse electric). Indices linked to the number of field knots in polar co-ordinates φ, r and z. For l<a the most simple mode, TM 010, has the lowest frequency, and has only two field components: E z = J 0 (kr) e iωt H θ = i Z 0 J 1 (kr) e iωt k = π λ = ω c λ =.6a Z 0 = 377Ω CAS@CERN, 4-8 November

12 The Pill Box Cavity () The design of a pill-box cavity can be sophisticated in order to improve its performances: - A nose cone can be introduced in order to concentrate the electric field around the axis - Round shaping of the corners allows a better distribution of the magnetic field on the surface and a reduction of the Joule losses. It also prevents from multipactoring effects. A good cavity is a cavity which efficiently transforms the RF power into accelerating voltage. CAS@CERN, 4-8 November 013 1

13 Some RF Cavity Examples L = vt/ (π mode) L = vt (π mode) Single Gap Multi-Gap CAS@CERN, 4-8 November

14 Transit time factor The accelerating field varies during the passage of the particle => particle does not always see maximum field => effective acceleration smaller Transit time factor defined as: T a = energy gain of particle with v = βc maximum energy gain (particle with v ) In the general case, the transit time factor is: for E(s,r,t) = E 1 (s,r) E (t) T a = + " E 1 (s,r) cos ω # $ RF + E 1 (s,r) ds s % v& ' ds Simple model uniform field: VRF E1 ( s, r) = = g const. follows: T a = sin ω RFg v ω RF g v 0 < T a < 1 T a 1 for g 0, smaller ω RF Important for low velocities (ions) CAS@CERN, 4-8 November

15 Disc loaded traveling wave structures -When particles gets ultra-relativistic (v~c) the drift tubes become very long unless the operating frequency is increased. Late 40 s the development of radar led to high power transmitters (klystrons) at very high frequencies (3 GHz). -Next came the idea of suppressing the drift tubes using traveling waves. However to get a continuous acceleration the phase velocity of the wave needs to be adjusted to the particle velocity. CLIC Accelerating Structures (30 & 11 GHz) solution: slow wave guide with irises ==> iris loaded structure CAS@CERN, 4-8 November

16 The Traveling Wave Case E z = E 0 cos( ω RF t kz) k = ω RF v ϕ z = v(t t 0 ) wave number The particle travels along with the wave, and k represents the wave propagation factor. " E z = E 0 cos $ ω RF t ω RF # v φ = phase velocity v = particle velocity v v ϕ t φ 0 % ' & If synchronism satisfied: v = v φ and E z = E 0 cosφ 0 where Φ 0 is the RF phase seen by the particle. CAS@CERN, 4-8 November

17 Energy Gain In relativistic dynamics, total energy E and momentum p are linked by E = E 0 + p c (E = E 0 +W ) W kinetic energy Hence: de =vdp The rate of energy gain per unit length of acceleration (along z) is then: and the kinetic energy gained from the field along the z path is: where V is just a potential. de dz =v dp dz = dp dt =ee z dw =de =ee z dz W =e E z dz = ev CAS@CERN, 4-8 November

18 Velocity, Energy and Momentum 1 normalized velocity v β = c = 1 1 γ Beta 0.5 electrons normalized velocity => electrons almost reach the speed of light very quickly (few MeV range) protons E_kinetic (MeV) total energy rest energy γ = E E Momentum = m m = E = γm 0 c 1 = v 1 c 1 β p = mv = E c βc = β E c = βγm 0 c Gamma total energy rest energy electrons protons E_kinetic (MeV) CAS@CERN, 4-8 November

19 Particle types and acceleration Accelerating system will depend upon the evolution of the particle velocity along the system electrons reach a constant velocity at relatively low energy heavy particles reach a constant velocity only at very high energy» may need different types of resonators, optimized for different velocities Particle rest mass: electron MeV proton 938 MeV 39 U ~0000MeV CAS@CERN, 4-8 November

20 Summary: Relativity + Energy Gain Newton-Lorentz Force F = d p dt = e ( E + v B ) nd term always perpendicular to motion => no acceleration Relativistics Dynamics v β = = c 1 1 γ γ = E E 0 = m m 0 = p = mv = E c βc = β E c = βγ m 0 c 1 1 β RF Acceleration E z =Êz sinω RFt=Êz sinφ ( t ) Ê z dz = ˆ V E de dz = E0 p c de =vdp + =v dp dz = dp dt =ee z de =dw =ee z dz W =e E z dz W =evˆsinφ (neglecting transit time factor) The field will change during the passage of the particle through the cavity => effective energy gain is lower CAS@CERN, 4-8 November 013 0

21 Common Phase Conventions 1. For circular accelerators, the origin of time is taken at the zero crossing of the RF voltage with positive slope. For linear accelerators, the origin of time is taken at the positive crest of the RF voltage Time t= 0 chosen such that: 1 E 1 E φ =ω RF t φ =ω RF t φ 1 φ E 1 (t) = E 0 sin( ω RF t) E (t) = E 0 cos( ω RF t) 3. I will stick to convention 1 in the following to avoid confusion CAS@CERN, 4-8 November 013 1

22 Principle of Phase Stability (Linac) Let s consider a succession of accelerating gaps, operating in the π mode, for which the synchronism condition is fulfilled for a phase Φs. ev s = e ˆ V sin Φ s is the energy gain in one gap for the particle to reach the next gap with the same RF phase: P 1,P, are fixed points. For a π mode, the electric field is the same in all gaps at any given time. If an energy increase is transferred into a velocity increase => M 1 & N 1 will move towards P 1 => stable M & N will go away from P => unstable (Highly relativistic particles have no significant velocity change) CAS@CERN, 4-8 November 013

23 A Consequence of Phase Stability Transverse focusing fields at the entrance and defocusing at the exit of the cavity. Electrostatic case: Energy gain inside the cavity leads to focusing RF case: Field increases during passage => transverse defocusing! Longitudinal phase stability means : V t > E z 0 < z 0 defocusing RF force The divergence of the field is x z x zero according to Maxwell :. E = 0 + = 0 > 0 E x E z E x External focusing (solenoid, quadrupole) is then necessary CAS@CERN, 4-8 November 013 3

24 - Rate of energy gain for the synchronous particle: dw dz = ee w = W Ws = E E s ϕ = φ s [ ( φ + ϕ) sinφ ] ee cosφ ϕ ( small ϕ ) 0 sin s s 0 s. - Rate of change of the phase with respect to the synchronous one: dϕ dz dt dt 1 1 ω RF = ωrf RF dz dz = ω v v s s vs v v Energy-phase Oscillations (1) = c de s dz = dp s dt β β c β φ ( v v ) Since: ( ) ( ) s s s 3 = ee 0 sinϕ s - Rate of energy gain for a non-synchronous particle, expressed in reduced variables, and : s β β w m vγ 0 s s s CAS@CERN, 4-8 November 013 4

25 Energy-phase Oscillations () one gets: dϕ = dz ω m v RF sγ s w Combining the two 1 st order equations into a nd order equation gives the equation of a harmonic oscillator: d ϕ dz + Ωsϕ = 0 with ee cos 0ω φs Ωs = m v γ RF 3 0 s Stable harmonic oscillations imply: Ω s > 0 and real hence: cos φ s > 0 And since acceleration also means: sin φ s > 0 You finally get the result for the stable phase range: 0 φ < acceleration CAS@CERN, 4-8 November s cos (φ s ) π V RF π π φ < π s 3

26 Longitudinal phase space The energy phase oscillations can be drawn in phase space: ΔΕ, Δp/p acceleration ΔΕ, Δp/p move forward move backward reference deceleration φ φ The particle trajectory in the phase space (Δp/p, φ) describes its longitudinal motion. Emittance: phase space area including all the particles NB: if the emittance contour correspond to a possible orbit in phase space, its shape does not change with time (matched beam) CAS@CERN, 4-8 November 013 6

27 Summary up to here Acceleration by electric fields, static fields limited => time-varying fields Synchronous condition needs to be fulfilled for acceleration Particles perform oscillation around synchronous phase visualize oscillations in phase space Electrons are quickly relativistic, speed does not change use traveling wave structures for acceleration Protons and ions need changing structure geometry 4-8 November 013 7

28 Circular accelerators Cyclotron Synchrotron 4-8 November 013 8

29 Circular accelerators: Cyclotron Used for protons, ions B = constant ω RF = constant B g RF generator, ω RF Synchronism condition π ω = ω s ρ = v s RF T RF Ion source Cyclotron frequency ω = q m 0 B γ Ions trajectory Extraction electrode 1. γ increases with the energy no exact synchronism. if v << c γ 1 CAS@CERN, 4-8 November 013 9

30 Cyclotron / Synchrocyclotron TRIUMF 50 MeV cyclotron Vancouver - Canada CERN 600 MeV synchrocyclotron Synchrocyclotron: Same as cyclotron, except a modulation of ω RF B = constant γ ω RF = constant ω RF decreases with time The condition: ω ( t) = ω ( t) = s RF q B m 0 γ ( t) Allows to go beyond the non-relativistic energies CAS@CERN, 4-8 November

31 Circular accelerators: The Synchrotron B R 1. Constant orbit during acceleration. To keep particles on the closed orbit, B should increase with time E 3. ω and ω RF increase with energy RF cavity RF generator RF frequency can be multiple of revolution frequency ω RF = hω r Synchronism condition s T s π R v = = h T h T RF RF h integer, harmonic number: number of RF cycles per revolution CAS@CERN, 4-8 November

32 Circular accelerators: The Synchrotron LEAR (CERN) Low Energy Antiproton Ring EPA (CERN) Electron Positron Accumulator CERN Geneva CERN Geneva Examples of different proton and electron synchrotrons at CERN + LHC (of course!) PS (CERN) Proton Synchrotron CAS@CERN, 4-8 November 013 CERN Geneva 3

33 The Synchrotron The synchrotron is a synchronous accelerator since there is a synchronous RF phase for which the energy gain fits the increase of the magnetic field at each turn. That implies the following operating conditions: B E ^ ev sin Φ Energy gain per turn Bending magnet Φ = Φ s = cte Synchronous particle R=C/π injection extraction ω RF = hω r RF synchronism (h - harmonic number) ρ bending radius ρ = cte R = cte Constant orbit Bρ = P e B Variable magnetic field If v c, ω r hence ω RF remain constant (ultra-relativistic e- ) CAS@CERN, 4-8 November

34 The Synchrotron Energy ramping Energy ramping is simply obtained by varying the B field (frequency follows v): p = ebρ dp = eρ B (Δp) turn = eρ BT r = π eρ R B dt v Since: E = E 0 + p c ΔE = vδp ( ΔE) = ( ΔW ) =π eρrb=e V ˆ sinφ s turn s Stable phase φ s changes during energy ramping sinφ = s π ρ R B V ˆ RF B φ = s arcsin π ρ R V ˆ RF The number of stable synchronous particles is equal to the harmonic number h. They are equally spaced along the circumference. Each synchronous particle satisfies the relation p=ebρ. They have the nominal energy and follow the nominal trajectory. CAS@CERN, 4-8 November

35 The Synchrotron Frequency change During the energy ramping, the RF frequency increases to follow the increase of the revolution frequency : ω r = ω RF h = ω(b, R s) f RF (t) = v(t) = 1 ec h π R s π E s (t) Hence: ( using ) E = (m 0 c ) + p c Since the RF frequency must follow the variation of the B field with the law f RF (t) h This asymptotically tends towards compared to m 0 c / (ecρ) which corresponds to = ρ B(t) p(t) = eb(t)ρ, E = mc R s c! B(t) " π R s #(m 0 c / ecρ) + B(t) v c f r c π R s 1 $ % & when B becomes large CAS@CERN, 4-8 November

36 cavity Dispersion Effects in a Synchrotron Circumference E+δE πr α = E If a particle is slightly shifted in momentum it will have a different orbit and the orbit length is different. The momentum compaction factor is defined as: dl L dp p α = p L dl dp p=particle momentum R=synchrotron physical radius f r =revolution frequency If the particle is shifted in momentum it will have also a different velocity. As a result of both effects the revolution frequency changes: η = d f r fr d p p η = p f r dfr dp CAS@CERN, 4-8 November

37 Momentum Compaction Factor α = p L dl dp ds 0 = ρdθ ds = ( ρ + x)dθ The elementary path difference from the two orbits is: dl ds 0 = ds ds 0 ds 0 definition of dispersion D x = x ρ = D x ρ dp p s s 0 p + dp p ρ θ x dθ x leading to the total change in the circumference: dl = α = 1 L dl = x ds 0 = ρ C C D x (s) ρ(s) ds 0 D x ρ dp p ds 0 With ρ= in straight sections we get: α = Dx m R < > m means that the average is considered over the bending magnet only CAS@CERN, 4-8 November

38 Dispersion Effects Revolution Frequency There are two effects changing the revolution frequency: the orbit length and the velocity of the particle f r = βc π R df r f r = dβ β dr R = dβ β α dp p definition of momentum compaction factor p = mv = βγ E 0 c dp p = dβ β + d ( 1 β ) 1 df r ( 1 β ) 1 ( ) 1 = 1 β γ dβ β df f r r f r = η dp p dp = 1 α η = α γ p γ η=0 at the transition energy γ CAS@CERN, 4-8 November tr 1 = 1 α

39 Phase Stability in a Synchrotron From the definition of η it is clear that an increase in momentum gives - below transition (η > 0) a higher revolution frequency (increase in velocity dominates) while - above transition (η < 0) a lower revolution frequency (v c and longer path) where the momentum compaction (generally > 0) dominates. Stable synchr. Particle for η < 0 η > 0 above transition η 1 γ = α CAS@CERN, 4-8 November

40 Crossing Transition At transition, the velocity change and the path length change with momentum compensate each other. So the revolution frequency there is independent from the momentum deviation. Crossing transition during acceleration makes the previous stable synchronous phase unstable. The RF system needs to make a rapid change of the RF phase, a phase jump. CAS@CERN, 4-8 November

41 Dynamics: Synchrotron oscillations Simple case (no accel.): B = const., below transition φ 1 - The particle B is accelerated - Below transition, an increase in energy means an increase in revolution frequency - The particle arrives earlier tends toward φ 0 γ < γ tr The phase of the synchronous particle must therefore be φ 0 = 0. V RF B φ φ 0 φ 1 φ =ω RF t φ - The particle is decelerated - decrease in energy - decrease in revolution frequency - The particle arrives later tends toward φ 0 CAS@CERN, 4-8 November

42 Synchrotron oscillations A V B time 1 st revolution period CAS@CERN, 4-8 November 013 4

43 Synchrotron oscillations A V B time 100 th revolution period CAS@CERN, 4-8 November

44 Synchrotron oscillations A V B time 00 th revolution period CAS@CERN, 4-8 November

45 Synchrotron oscillations A V B time 400 th revolution period CAS@CERN, 4-8 November

46 Synchrotron oscillations A V B time 500 th revolution period CAS@CERN, 4-8 November

47 Synchrotron oscillations A V B time 600 th revolution period CAS@CERN, 4-8 November

48 Synchrotron oscillations A V B time 700 th revolution period CAS@CERN, 4-8 November

49 Synchrotron oscillations A V B time 800 th revolution period CAS@CERN, 4-8 November

50 Synchrotron oscillations A V B time 900 th revolution period CAS@CERN, 4-8 November

51 Synchrotron oscillations A V B time 900 th revolution period Particle B has made one full oscillation around particle A. The amplitude depends on the initial phase and energy. Exactly like the pendulum This oscillation is called: Synchrotron Oscillation CAS@CERN, 4-8 November

52 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November 013 5

53 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

54 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

55 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

56 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

57 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

58 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

59 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

60 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

61 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

62 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November 013 6

63 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

64 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

65 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

66 The Potential Well A Cavity voltage Potential B Potential well CAS@CERN, 4-8 November

67 Longitudinal Phase Space Motion (1) Particle B oscillates around particle A This is a synchrotron oscillation Plotting this motion in longitudinal phase space gives: ΔE higher energy early arrival late arrival Δt (or φ) lower energy CAS@CERN, 4-8 November

68 Longitudinal Phase Space Motion () Particle B oscillates around particle A This is a synchrotron oscillation Plotting this motion in longitudinal phase space gives: ΔE higher energy early arrival late arrival Δt (or φ) lower energy CAS@CERN, 4-8 November

69 Longitudinal Phase Space Motion (3) Particle B oscillates around particle A This is a synchrotron oscillation Plotting this motion in longitudinal phase space gives: ΔE higher energy early arrival late arrival Δt (or φ) lower energy CAS@CERN, 4-8 November

70 Longitudinal Phase Space Motion (4) Particle B oscillates around particle A This is a synchrotron oscillation Plotting this motion in longitudinal phase space gives: ΔE higher energy early arrival late arrival Δt (or φ) lower energy CAS@CERN, 4-8 November

71 Synchrotron oscillations V RF φ φ 0 φ t φ 1 Phase space picture Δp p stable region φ unstable region separatrix CAS@CERN, 4-8 November

72 Synchrotron oscillations (with acceleration) Case with acceleration B increasing γ < γ tr V RF 1 φ φ =ω RF t φ s Phase space picture Δp p φ < φ < π s φ s stable region unstable region separatrix φ The symmetry of the case B = const. is lost CAS@CERN, 4-8 November 013 7

73 Synchrotron motion in phase space ΔE-φ phase space of a stationary bucket Dynamics of a particle Non-linear, conservative oscillator e.g. pendulum Particle inside the separatrix: Particle at the unstable fix-point Bucket area: area enclosed by the separatrix The area covered by particles is the longitudinal emittance Particle outside the separatrix: CAS@CERN, 4-8 November

74 Synchrotron motion in phase space The restoring force is non-linear. speed of motion depends on position in phase-space (here shown for a stationary bucket) CAS@CERN, 4-8 November

75 (Stationary) Bunch & Bucket ΔE Bunch ΔE Bucket Δt (or φ) Δt Bucket area = longitudinal Acceptance [evs] Bunch area = longitudinal beam emittance = π.δe.δt/4 [evs] CAS@CERN, 4-8 November

76 RF Acceptance versus Synchronous Phase The areas of stable motion (closed trajectories) are called BUCKET. As the synchronous phase gets closer to 90º the buckets gets smaller. The number of circulating buckets is equal to h. The phase extension of the bucket is maximum for φ s =180º (or 0 ) which correspond to no acceleration. The RF acceptance increases with the RF voltage. CAS@CERN, 4-8 November

77 Longitudinal Dynamics in Synchrotrons It is also often called synchrotron motion. The RF acceleration process clearly emphasizes two coupled variables, the energy gained by the particle and the RF phase experienced by the same particle. Since there is a well defined synchronous particle which has always the same phase φ s, and the nominal energy E s, it is sufficient to follow other particles with respect to that particle. So let s introduce the following reduced variables: revolution frequency : Δf r = f r f rs particle RF phase : Δφ = φ - φ s particle momentum : Δp = p - p s particle energy : ΔE = E E s azimuth angle : Δθ = θ - θ s CAS@CERN, 4-8 November

78 First Energy-Phase Equation v Δθ θ s R f RF = h f r Δφ = h Δθ with θ = ω r dt For a given particle with respect to the reference one: Δω = r d dt particle ahead arrives earlier => smaller RF phase 1 h d dt ( Δθ ) = ( Δφ ) = 1 h dφ dt Since: η = p s ω rs # $ % dω r dp & ' ( s and p E = E 0 + c ΔE = v s Δp = ω rs R s Δp p ( ) srs d φ one gets: ΔE Δ ω rs = hηωrs dt = psrs hηω rs φ CAS@CERN, 4-8 November

79 Second Energy-Phase Equation The rate of energy gained by a particle is: de = evˆ sinφ ωr dt π The rate of relative energy gain with respect to the reference particle is then: $ π Δ& % E ω r ' ) ( = e ˆV(sinφ sinφ s ) Expanding the left-hand side to first order: Δ( ET ) r EΔT r + T rs Δ E = ΔE T r + T rs Δ E = d dt leads to the second energy-phase equation: ( T rs ΔE) π d dt $ % & ΔE ω rs ' ( ) = e ˆV sinφ sinφ s ( ) CAS@CERN, 4-8 November

80 Equations of Longitudinal Motion ΔE= ωrs psrs hηωrs d ( Δφ) dt = psrs hηω rs φ π d E evˆ dt Δ ω = rs ( sinφ sinφ s) deriving and combining d dt Rs ps hηωrs dφ ˆ + ev dt π ( sinφ sinφ ) s = 0 This second order equation is non linear. Moreover the parameters within the bracket are in general slowly varying with time. We will study some cases in the following CAS@CERN, 4-8 November

81 Small Amplitude Oscillations Let s assume constant parameters R s, p s, ω s and η: φ + s Ωs cosφ s ( sinφ sinφ ) = 0 with Ω s = hηωrsevˆcosφ s πrs ps Consider now small phase deviations from the reference particle: sinφ sinφ s = sin ( φ ) s+δφ sinφ s cosφ sδφ (for small Δφ) and the corresponding linearized motion reduces to a harmonic oscillation: φ + Ω s Δφ = 0 where Ω s is the synchrotron angular frequency CAS@CERN, 4-8 November

82 Stability condition for ϕ s Stability is obtained when Ω s is real and so Ω s positive: Ω s = e ˆV RF η hω s cosφ s Ω s > 0 η cosφ s > 0 π R s p s cos (φ s ) V RF π π 3 π φ Stable in the region if γ < γ tr γ > γ tr γ > γ tr γ < γ tr η > 0 η < 0 η < 0 η > 0 acceleration deceleration CAS@CERN, 4-8 November 013 8

83 Large Amplitude Oscillations For larger phase (or energy) deviations from the reference the second order differential equation is non-linear: φ Ω s cosφ ( sinφ sinφ ) = 0 + s s Multiplying by φ Ω cos φ (Ω s as previously defined) and integrating gives an invariant of the motion: ( cosφ + φ sin φ ) I s s = φs which for small amplitudes reduces to: ( ) φ + Ω Δφ s = I$ (the variable is Δφ, and φ s is constant) Similar equations exist for the second variable : ΔE dφ/dt CAS@CERN, 4-8 November

84 Large Amplitude Oscillations () When φ reaches π-φ s the force goes to zero and beyond it becomes non restoring. Hence π-φ s is an extreme amplitude for a stable motion which in the φ phase space(, Δφ ) is shown as Ω s closed trajectories. Equation of the separatrix: φ Ω s cosφ s m s ( cosφ + φ sinφ ) = ( cos( π φ ) + ( π φ ) sinφ ) cosφ + φ sinφ = cos m s s Ω cosφ Second value φ m where the separatrix crosses the horizontal axis: s ( π φs ) + ( π φs ) sin s Area within this separatrix is called RF bucket. CAS@CERN, 4-8 November s φ s s

85 Energy Acceptance φ φ = φ From the equation of motion it is seen that φ = 0 when, hence corresponding to. reaches an extreme Introducing this value into the equation of the separatrix gives: s φ max = Ω s { + ( φ s π )tanφ } s That translates into an acceptance in energy: " # $ ΔE % E s & ' = β e ˆV π hηe G s max ( φ ) s G( φ s )= $% cosφ s + ( φ s π )sinφ s & ' This RF acceptance depends strongly on φ s and plays an important role for the capture at injection, and the stored beam lifetime. It s largest for φ s =0 and φ s =π (no acceleration, depending on η). CAS@CERN, 4-8 November

86 RF Acceptance versus Synchronous Phase The areas of stable motion (closed trajectories) are called BUCKET. As the synchronous phase gets closer to 90º the buckets gets smaller. The number of circulating buckets is equal to h. The phase extension of the bucket is maximum for φ s =180º (or 0 ) which correspond to no acceleration. The RF acceptance increases with the RF voltage. CAS@CERN, 4-8 November

87 Stationnary Bucket - Separatrix This is the case sinφ s =0 (no acceleration) which means φ s =0 or π. The equation of the separatrix for φ s = π (above transition) becomes: φ φ φ + Ωs cosφ =Ω = Ωssin s Replacing the phase derivative by the (canonical) variable W: W W bk 0 π π φ ps s W = π ΔE = π R ωrs hηω rs φ and introducing the expression for Ω s leads to the following equation for the separatrix: with C=πR s W = ± C c e ˆV E s π hη sinφ = ±W sinφ bk CAS@CERN, 4-8 November

88 Stationnary Bucket () Setting φ=π in the previous equation gives the height of the bucket: W = C c bk evˆ π h E s η This results in the maximum energy acceptance: ΔE max = ω rs π W bk = β s e ˆV RF E s πηh The area of the bucket is: π φ Since: sin dφ = one gets: 0 4 Abk A bk = 8W bk = 16 C c π 0 = W dφ e ˆV E s π hη W bk = A 8 bk CAS@CERN, 4-8 November

89 Effect of a Mismatch Injected bunch: short length and large energy spread after 1/4 synchrotron period: longer bunch with a smaller energy spread. W W φ φ For larger amplitudes, the angular phase space motion is slower (1/8 period shown below) => can lead to filamentation and emittance growth V RF W W ϕ φ φ restoring force is non-linear stationary bucket accelerating bucket W.Pirkl CAS@CERN, 4-8 November

90 Effect of a Mismatch () Evolution of an injected beam for the first 100 turns. For a matched transfer, the emittance does not grow (left). matched beam mismatched beam bunch length CAS@CERN, 4-8 November

91 Effect of a Mismatch (3) Evolution of an injected beam for the first 100 turns. For a mismatched transfer, the emittance increases (right). matched beam mismatched beam phase error CAS@CERN, 4-8 November

92 Bunch Rotation Phase space motion can be used to make short bunches. Start with a long bunch and extract or recapture when it s short. initial beam CAS@CERN, 4-8 November 013 9

93 The LHC5 (ns) cycle in the PS Inject 4+ bunches h = 7 γ tr h = 1 h = 84 Eject 7 bunches Triple splitting after nd injection Split in four at flat-top energy nd injection 1.4 GeV 6 GeV/c (sketched) Each bunch from the Booster divided by = 7 CAS@CERN, 4-8 November

94 Bunch Manipulation in the PS Two times double splitting and bunch rotation: 4-8 November

95 Capture of a Debunched Beam with Fast Turn-On CAS@CERN, 4-8 November

96 Capture of a Debunched Beam with Adiabatic Turn-On CAS@CERN, 4-8 November

97 Bunch Matching into a Stationnary Bucket A particle trajectory inside the separatrix is described by the equation: φ Ω cosφ s φs = s ( cosφ + φsin ) I W W bk W b 0 π π π ˆφ φ φ s = π φ +Ω φ + Ωs cosφ = I The points where the trajectory crosses the axis are symmetric with respect to φ s = π s cosφ =Ω s cosφ m ( cosφ cosφ ) φ = ±Ωs m φ m π-φ m ϕ W = ±W bk cos m cos ϕ cos(φ) = cos φ 1 CAS@CERN, 4-8 November

98 Bunch Matching into a Stationnary Bucket () Setting φ = π in the previous formula allows to calculate the bunch height: W b = W bk φ cos m = W bk sin ˆφ or: W b = A 8 bk cos φ m " # $ ΔE % & ' = E s b " # $ ΔE % φ E s & ' cos m = " ΔE % # $ RF E s & ' RF sin ˆφ This formula shows that for a given bunch energy spread the proper matching of a shorter bunch (φ m close to π, ˆφ small) will require a bigger RF acceptance, hence a higher voltage For small oscillation amplitudes the equation of the ellipse reduces to: W = A bk 16 ˆφ ( Δφ) " 16W % # $ ˆφ & ' + " Δφ % # $ ˆφ & ' =1 Abk Ellipse area is called longitudinal emittance A b = π 16 A ˆφ bk CAS@CERN, 4-8 November

99 Summary Cyclotrons/Synchrocylotrons for low energy Synchrotrons for high energies constant orbit, rising field and frequency Particles with higher energy have a longer orbit (normally) but a higher velocity at low energies (below transition) velocity increase dominates at high energies (above transition) velocity almost constant Particles perform oscillations around synchronous phase synchronous phase depending on acceleration below or above transition bucket is the region in phase space for stable oscillations matching the shape of the bunch to the bucket is important CAS@CERN, 4-8 November

100 Bibliography M. Conte, W.W. Mac Kay An Introduction to the Physics of particle Accelerators (World Scientific, 1991) P. J. Bryant and K. Johnsen The Principles of Circular Accelerators and Storage Rings (Cambridge University Press, 1993) D. A. Edwards, M. J. Syphers An Introduction to the Physics of High Energy Accelerators (J. Wiley & sons, Inc, 1993) H. Wiedemann Particle Accelerator Physics (Springer-Verlag, Berlin, 1993) M. Reiser Theory and Design of Charged Particles Beams (J. Wiley & sons, 1994) A. Chao, M. Tigner Handbook of Accelerator Physics and Engineering (World Scientific 1998) K. Wille The Physics of Particle Accelerators: An Introduction (Oxford University Press, 000) E.J.N. Wilson An introduction to Particle Accelerators (Oxford University Press, 001) And CERN Accelerator Schools (CAS) Proceedings 4-8 November

101 Acknowledgements I would like to thank everyone for the material that I have used. In particular (hope I don t forget anyone): - Joël Le Duff - Rende Steerenberg - Gerald Dugan - Heiko Damerau - Werner Pirkl - Genevieve Tulloue - Mike Syphers - Daniel Schulte - Roberto Corsini CAS@CERN, 4-8 November

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

!#$%$!&'()$('*+,-')'+-$#..+/+,0)&,$%.1&&/$ LONGITUDINAL BEAM DYNAMICS LONGITUDINAL BEAM DYNAMICS Elias Métral BE Department CERN The present transparencies are inherited from Frank Tecker (CERN-BE), who gave this course last year and who inherited them from Roberto Corsini

More information

Longitudinal dynamics Yannis PAPAPHILIPPOU CERN

Longitudinal dynamics Yannis PAPAPHILIPPOU CERN Longitudinal dynamics Yannis PAPAPHILIPPOU CERN United States Particle Accelerator School, University of California - Santa-Cruz, Santa Rosa, CA 14 th 18 th January 2008 1 Outline Methods of acceleration

More information

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

!#$%$!&'()$('*+,-')'+-$#..+/+,0)&,$%.1&&/$ LONGITUDINAL BEAM DYNAMICS LONGITUDINAL BEAM DYNAMICS Elias Métral (CERN BE Department) The present transparencies are inherited from Frank Tecker (CERN-BE), who gave this course in 2010 (I already gave this course in 2011-12-13)

More information

LONGITUDINAL DYNAMICS RECAP

LONGITUDINAL DYNAMICS RECAP LONGITUDINAL DYNAMICS RECAP Frank Tecker CERN, BE-OP Advanced Accelerator Physics Course Egham, UK, 3-15/9/2017 Advanced CAS, Egham, September 2017 1 Summary of the 2 lectures: Acceleration methods Accelerating

More information

Introduction to Longitudinal Beam Dynamics

Introduction to Longitudinal Beam Dynamics Introduction to Longitudinal Beam Dynamics B.J. Holzer CERN, Geneva, Switzerland Abstract This chapter gives an overview of the longitudinal dynamics of the particles in an accelerator and, closely related

More information

Linac JUAS lecture summary

Linac JUAS lecture summary Linac JUAS lecture summary Part1: Introduction to Linacs Linac is the acronym for Linear accelerator, a device where charged particles acquire energy moving on a linear path. There are more than 20 000

More information

Physics 610. Adv Particle Physics. April 7, 2014

Physics 610. Adv Particle Physics. April 7, 2014 Physics 610 Adv Particle Physics April 7, 2014 Accelerators History Two Principles Electrostatic Cockcroft-Walton Van de Graaff and tandem Van de Graaff Transformers Cyclotron Betatron Linear Induction

More information

LONGITUDINAL BEAM DYNAMICS IN CIRCULAR ACCELERATORS

LONGITUDINAL BEAM DYNAMICS IN CIRCULAR ACCELERATORS LONGITUDINAL BEAM DYNAMICS IN CIRCULAR ACCELERATORS J. Le Duff Laboratoire de l'accélérateur Linéaire Université Paris-Sud, 91405 Orsay, France 1. ACCELERATION BY TIME VARYING FIELDS 1. 1 Time varying

More information

Longitudinal Beam Dynamics

Longitudinal Beam Dynamics Longitudinal Beam Dynamics Shahin Sanaye Hajari School of Particles and Accelerators, Institute For Research in Fundamental Science (IPM), Tehran, Iran IPM Linac workshop, Bahman 28-30, 1396 Contents 1.

More information

Synchrotron Motion. RF cavities. Charged particles gain and lose energy in electric field via

Synchrotron Motion. RF cavities. Charged particles gain and lose energy in electric field via 217 NSRRC FEL Longitudinal Motion (SYL) 1 Synchrotron Motion RF cavities Charged particles gain and lose energy in electric field via Δ. For DC accelerators such as the Cockcroft-Walton and Van-der- Graaff

More information

Longitudinal Dynamics

Longitudinal Dynamics Longitudinal Dynamics F = e (E + v x B) CAS Bruges 16-25 June 2009 Beam Dynamics D. Brandt 1 Acceleration The accelerator has to provide kinetic energy to the charged particles, i.e. increase the momentum

More information

PBL SCENARIO ON ACCELERATORS: SUMMARY

PBL SCENARIO ON ACCELERATORS: SUMMARY PBL SCENARIO ON ACCELERATORS: SUMMARY Elias Métral Elias.Metral@cern.ch Tel.: 72560 or 164809 CERN accelerators and CERN Control Centre Machine luminosity Transverse beam dynamics + space charge Longitudinal

More information

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

Phase Space Study of the Synchrotron Oscillation and Radiation Damping of the Longitudinal and Transverse Oscillations ScienceAsia 28 (2002 : 393-400 Phase Space Study of the Synchrotron Oscillation and Radiation Damping of the Longitudinal and Transverse Oscillations Balabhadrapatruni Harita*, Masumi Sugawara, Takehiko

More information

Introduction to Longitudinal Beam Dynamics

Introduction to Longitudinal Beam Dynamics Introduction to Longitudinal Beam Dynamics Andrea Latina (CERN) andrea.latina@cern.ch Credits: Elias Métral, Daniel Schulte (CERN) 1 st SLRI-CERN ASEAN Accelerator School August 28 - Setember 1, 2017 Table

More information

LONGITUDINAL DYNAMICS OF PARTICLES IN ACCELERATORS. Author: Urša Rojec Mentor: Simon Širca. Ljubljana, November 2012

LONGITUDINAL DYNAMICS OF PARTICLES IN ACCELERATORS. Author: Urša Rojec Mentor: Simon Širca. Ljubljana, November 2012 Seminar I a, četrti letnik, stari program LONGITUDINAL DYNAMICS OF PARTICLES IN ACCELERATORS Author: Urša Rojec Mentor: Simon Širca Ljubljana, November 2012 Abstract The seminar focuses on longitudinal

More information

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

CERN Accelerator School. Intermediate Accelerator Physics Course Chios, Greece, September Low Emittance Rings CERN Accelerator School Intermediate Accelerator Physics Course Chios, Greece, September 2011 Low Emittance Rings Part 1: Beam Dynamics with Synchrotron Radiation Andy Wolski The Cockcroft Institute, and

More information

Engines of Discovery

Engines of Discovery Engines of Discovery R.S. Orr Department of Physics University of Toronto Berkley 1930 1 MeV Geneva 20089 14 TeV Birth of Particle Physics and Accelerators 1909 Geiger/Marsden MeV a backscattering - Manchester

More information

RF LINACS. Alessandra Lombardi BE/ ABP CERN

RF LINACS. Alessandra Lombardi BE/ ABP CERN 1 RF LINACS Alessandra Lombardi BE/ ABP CERN Contents PART 1 (yesterday) : Introduction : why?,what?, how?, when? Building bloc I (1/) : Radio Frequency cavity From an RF cavity to an accelerator PART

More information

Accelerators Ideal Case

Accelerators Ideal Case Accelerators Ideal Case Goal of an accelerator: increase energy of CHARGED par:cles Increase energy ΔE = r 2 F dr = q ( E + v B)d r The par:cle trajectory direc:on dr parallel to v ΔE = increase of energy

More information

PBL (Problem-Based Learning) scenario for Accelerator Physics Mats Lindroos and E. Métral (CERN, Switzerland) Lund University, Sweden, March 19-23,

PBL (Problem-Based Learning) scenario for Accelerator Physics Mats Lindroos and E. Métral (CERN, Switzerland) Lund University, Sweden, March 19-23, PBL (Problem-Based Learning) scenario for Accelerator Physics Mats Lindroos and E. Métral (CERN, Switzerland) Lund University, Sweden, March 19-23, 2007 As each working day, since the beginning of the

More information

Theory English (Official)

Theory English (Official) Q3-1 Large Hadron Collider (10 points) Please read the general instructions in the separate envelope before you start this problem. In this task, the physics of the particle accelerator LHC (Large Hadron

More information

Low Emittance Machines

Low Emittance Machines Advanced Accelerator Physics Course RHUL, Egham, UK September 2017 Low Emittance Machines Part 1: Beam Dynamics with Synchrotron Radiation Andy Wolski The Cockcroft Institute, and the University of Liverpool,

More information

Particle physics experiments

Particle physics experiments Particle physics experiments Particle physics experiments: collide particles to produce new particles reveal their internal structure and laws of their interactions by observing regularities, measuring

More information

Low Emittance Machines

Low Emittance Machines CERN Accelerator School Advanced Accelerator Physics Course Trondheim, Norway, August 2013 Low Emittance Machines Part 1: Beam Dynamics with Synchrotron Radiation Andy Wolski The Cockcroft Institute, and

More information

Beam Dynamics in Synchrotrons with Space- Charge

Beam Dynamics in Synchrotrons with Space- Charge Beam Dynamics in Synchrotrons with Space- Charge 1 Basic Principles without space-charge RF resonant cavity providing accelerating voltage V (t). Often V = V 0 sin(φ s + ω rf t), where ω rf is the angular

More information

Medical Linac. Block diagram. Electron source. Bending magnet. Accelerating structure. Klystron or magnetron. Pulse modulator.

Medical Linac. Block diagram. Electron source. Bending magnet. Accelerating structure. Klystron or magnetron. Pulse modulator. Block diagram Medical Linac Electron source Bending magnet Accelerating structure Pulse modulator Klystron or magnetron Treatment head 1 Medical Linac 2 Treatment Head 3 Important Accessories Wedges Dynamic

More information

Lectures on accelerator physics

Lectures on accelerator physics Lectures on accelerator physics Lecture 3 and 4: Examples Examples of accelerators 1 Rutherford s Scattering (1909) Particle Beam Target Detector 2 Results 3 Did Rutherford get the Nobel Prize for this?

More information

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

D. Brandt, CERN. CAS Frascati 2008 Accelerators for Newcomers D. Brandt 1 Accelerators for Newcomers D. Brandt, CERN D. Brandt 1 Why this Introduction? During this school, you will learn about beam dynamics in a rigorous way but some of you are completely new to the field of

More information

Why do we accelerate particles?

Why do we accelerate particles? Why do we accelerate particles? (1) To take existing objects apart 1803 J. Dalton s indivisible atom atoms of one element can combine with atoms of other element to make compounds, e.g. water is made of

More information

Physics 663. Particle Physics Phenomenology. April 9, Physics 663, lecture 2 1

Physics 663. Particle Physics Phenomenology. April 9, Physics 663, lecture 2 1 Physics 663 Particle Physics Phenomenology April 9, 2002 Physics 663, lecture 2 1 History Two Principles Electrostatic Cockcroft-Walton Accelerators Van de Graaff and tandem Van de Graaff Transformers

More information

Synchrotron Motion with Space-Charge

Synchrotron Motion with Space-Charge Synchrotron Motion with Space-Charge Basic Principles without space-charge RF resonant cavity providing accelerating voltage V (t). Often V = V 0 sin(φ s + ω rf t), where ω rf is the angular frequency

More information

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

Transverse dynamics Selected topics. Erik Adli, University of Oslo, August 2016, v2.21 Transverse dynamics Selected topics Erik Adli, University of Oslo, August 2016, Erik.Adli@fys.uio.no, v2.21 Dispersion So far, we have studied particles with reference momentum p = p 0. A dipole field

More information

Historical developments. of particle acceleration

Historical developments. of particle acceleration Historical developments of particle acceleration Y.Papaphilippou N. Catalan-Lasheras USPAS, Cornell University, Ithaca, NY 20 th June 1 st July 2005 1 Outline Principles of Linear Acceleration Electrostatic

More information

E. Wilson - CERN. Components of a synchrotron. Dipole Bending Magnet. Magnetic rigidity. Bending Magnet. Weak focusing - gutter. Transverse ellipse

E. Wilson - CERN. Components of a synchrotron. Dipole Bending Magnet. Magnetic rigidity. Bending Magnet. Weak focusing - gutter. Transverse ellipse Transverse Dynamics E. Wilson - CERN Components of a synchrotron Dipole Bending Magnet Magnetic rigidity Bending Magnet Weak focusing - gutter Transverse ellipse Fields and force in a quadrupole Strong

More information

Basic Mathematics and Units

Basic Mathematics and Units Basic Mathematics and Units Rende Steerenberg BE/OP Contents Vectors & Matrices Differential Equations Some Units we use 3 Vectors & Matrices Differential Equations Some Units we use 4 Scalars & Vectors

More information

Introduction to Elementary Particle Physics I

Introduction to Elementary Particle Physics I Physics 56400 Introduction to Elementary Particle Physics I Lecture 9 Fall 2018 Semester Prof. Matthew Jones Particle Accelerators In general, we only need classical electrodynamics to discuss particle

More information

ACCELERATION, DECELERATION AND BUNCHING OF STORED AND COOLED ION BEAMS AT THE TSR, HEIDELBERG

ACCELERATION, DECELERATION AND BUNCHING OF STORED AND COOLED ION BEAMS AT THE TSR, HEIDELBERG ACCELERATION, DECELERATION AND BUNCHING OF STORED AND COOLED ION BEAMS AT THE TSR, HEIDELBERG M. Grieser, R. Bastert, K. Blaum, H. Buhr, R. von Hahn, M. B. Mendes, R. Repnow, A. Wolf Max-Planck-Institut

More information

ELECTRON DYNAMICS WITH SYNCHROTRON RADIATION

ELECTRON DYNAMICS WITH SYNCHROTRON RADIATION ELECTRON DYNAMICS WITH SYNCHROTRON RADIATION Lenny Rivkin Ecole Polythechnique Federale de Lausanne (EPFL) and Paul Scherrer Institute (PSI), Switzerland CERN Accelerator School: Introduction to Accelerator

More information

Beam Dynamics. D. Brandt, CERN. CAS Bruges June 2009 Beam Dynamics D. Brandt 1

Beam Dynamics. D. Brandt, CERN. CAS Bruges June 2009 Beam Dynamics D. Brandt 1 Beam Dynamics D. Brandt, CERN D. Brandt 1 Some generalities D. Brandt 2 Units: the electronvolt (ev) The electronvolt (ev)) is the energy gained by an electron travelling, in vacuum, between two points

More information

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

Introduction to Accelerators. Scientific Tools for High Energy Physics and Synchrotron Radiation Research Introduction to Accelerators. Scientific Tools for High Energy Physics and Synchrotron Radiation Research Pedro Castro Introduction to Particle Accelerators DESY, July 2010 What you will see Pedro Castro

More information

Particles and Universe: Particle accelerators

Particles and Universe: Particle accelerators Particles and Universe: Particle accelerators Maria Krawczyk, Aleksander Filip Żarnecki March 24, 2015 M.Krawczyk, A.F.Żarnecki Particles and Universe 4 March 24, 2015 1 / 37 Lecture 4 1 Introduction 2

More information

LONGITUDINAL beam DYNAMICS in circular accelerators

LONGITUDINAL beam DYNAMICS in circular accelerators LONGITUDINAL beam DYNAMICS in circular accelerator Frank Tecker CERN, BE-OP Introduction to Accelerator Phyic Budapet, -14/10/016 Introductory CAS, Budapet, October 016 1 Summary of the lecture: Introduction

More information

Accelerators. W. Udo Schröder, 2004

Accelerators. W. Udo Schröder, 2004 1 Accelerators Overview Electrostatic Accelerators Cascade Van de Graaff V.d.G. Tandem generator Accelerator 2-3 stages steady (DC) beam, high quality focusing, energy, currents; but low energies Accelerators

More information

Section 4 : Accelerators

Section 4 : Accelerators Section 4 : Accelerators In addition to their critical role in the evolution of nuclear science, nuclear particle accelerators have become an essential tool in both industry and medicine. Table 4.1 summarizes

More information

Bernhard Holzer, CERN-LHC

Bernhard Holzer, CERN-LHC Bernhard Holzer, CERN-LHC * Bernhard Holzer, CERN CAS Prague 2014 x Liouville: in reasonable storage rings area in phase space is constant. A = π*ε=const x ε beam emittance = woozilycity of the particle

More information

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

Introduction to accelerators for teachers (Korean program) Mariusz Sapiński CERN, Beams Department August 9 th, 2012 Introduction to accelerators for teachers (Korean program) Mariusz Sapiński (mariusz.sapinski@cern.ch) CERN, Beams Department August 9 th, 2012 Definition (Britannica) Particle accelerator: A device producing

More information

Accelerators. There are some accelerators around the world Nearly all are for industrial (20 000) or clinical use (10 000)

Accelerators. There are some accelerators around the world Nearly all are for industrial (20 000) or clinical use (10 000) Accelerators There are some 30 000 accelerators around the world Nearly all are for industrial (20 000) or clinical use (10 000) Scientific research community (~ 100) Synchrotron light sources Ion beam

More information

10 GeV Synchrotron Longitudinal Dynamics

10 GeV Synchrotron Longitudinal Dynamics 0 GeV Synchrotron Longitudinal Dynamics G. Dugan Laboratory of Nuclear Studies Cornell University Ithaca, NY 483 In this note, I provide some estimates of the parameters of longitudinal dynamics in the

More information

An Introduction to Particle Accelerators. v short

An Introduction to Particle Accelerators. v short An Introduction to Particle Accelerators v1.42 - short LHC FIRST BEAM 10-sep-2008 Introduction Part 1 Particle accelerators for HEP LHC: the world biggest accelerator, both in energy and size (as big as

More information

Varying accelerating fields

Varying accelerating fields Varying accelerating fields Two approaches for accelerating with time-varying fields Linear Accelerators Circular Accelerators Use many accelerating cavities through which the particle beam passes once.

More information

Transverse Dynamics II

Transverse Dynamics II Transverse Dynamics II JAI Accelerator Physics Course Michaelmas Term 217 Dr. Suzie Sheehy Royal Society University Research Fellow University of Oxford Acknowledgements These lectures have been produced

More information

Small Synchrotrons. Michael Benedikt. CERN, AB-Department. CAS, Zeegse, 30/05/05 Small Synchrotrons M. Benedikt 1

Small Synchrotrons. Michael Benedikt. CERN, AB-Department. CAS, Zeegse, 30/05/05 Small Synchrotrons M. Benedikt 1 Small Synchrotrons Michael Benedikt CERN, AB-Department CAS, Zeegse, 30/05/05 Small Synchrotrons M. Benedikt 1 Contents Introduction Synchrotron linac - cyclotron Main elements of the synchrotron Accelerator

More information

Tools of Particle Physics I Accelerators

Tools of Particle Physics I Accelerators Tools of Particle Physics I Accelerators W.S. Graves July, 2011 MIT W.S. Graves July, 2011 1.Introduction to Accelerator Physics 2.Three Big Machines Large Hadron Collider (LHC) International Linear Collider

More information

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

Accelerator Physics Weak Focussing. A. Bogacz, G. A. Krafft, and T. Zolkin Jefferson Lab Colorado State University Lecture 2 Accelerator Physics Weak Focussing A. Bogacz, G. A. Krafft, and T. Zolkin Jefferson Lab Colorado State University Lecture 2 Betatrons 25 MeV electron accelerator with its inventor: Don Kerst. The earliest

More information

Acceleration to higher energies

Acceleration to higher energies Acceleration to higher energies While terminal voltages of 20 MV provide sufficient beam energy for nuclear structure research, most applications nowadays require beam energies > 1 GeV How do we attain

More information

A Proposal of Harmonictron

A Proposal of Harmonictron Memoirs of the Faculty of Engineering, Kyushu University, Vol.77, No.2, December 2017 A Proposal of Harmonictron by Yoshiharu MORI *, Yujiro YONEMURA ** and Hidehiko ARIMA *** (Received November 17, 2017)

More information

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

Accelerator Physics Weak Focusing. S. A. Bogacz, G. A. Krafft, S. DeSilva, R. Gamage Jefferson Lab Old Dominion University Lecture 2 Accelerator Physics Weak Focusing S. A. Bogacz, G. A. Krafft, S. DeSilva, R. Gamage Jefferson Lab Old Dominion University Lecture 2 Betatrons 25 MeV electron accelerator with its inventor: Don Kerst. The

More information

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

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

More information

Introduction to Accelerators

Introduction to Accelerators Introduction to Accelerators D. Brandt, CERN CAS Platja d Aro 2006 Introduction to Accelerators D. Brandt 1 Why an Introduction? The time where each accelerator sector was working alone in its corner is

More information

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

CERN Accelerator School. RF Cavities. Erk Jensen CERN BE-RF CERN Accelerator School RF Cavities Erk Jensen CERN BE-RF CERN Accelerator School, Varna 010 - "Introduction to Accelerator Physics" What is a cavity? 3-Sept-010 CAS Varna/Bulgaria 010- RF Cavities Lorentz

More information

ELECTRON DYNAMICS with SYNCHROTRON RADIATION

ELECTRON DYNAMICS with SYNCHROTRON RADIATION ELECTRON DYNAMICS with SYNCHROTRON RADIATION Lenny Rivkin École Polythechnique Fédérale de Lausanne (EPFL) and Paul Scherrer Institute (PSI), Switzerland CERN Accelerator School: Introduction to Accelerator

More information

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

Accelerator Physics. Tip World Scientific NEW JERSEY LONDON SINGAPORE BEIJING SHANGHAI HONG KONG TAIPEI BANGALORE. Second Edition. S. Y. Accelerator Physics Second Edition S. Y. Lee Department of Physics, Indiana University Tip World Scientific NEW JERSEY LONDON SINGAPORE BEIJING SHANGHAI HONG KONG TAIPEI BANGALORE Contents Preface Preface

More information

EP228 Particle Physics

EP228 Particle Physics EP8 Particle Physics Topic 3 Department of Engineering Physics University of Gaziantep Course web page www.gantep.edu.tr/~bingul/ep8 Dec 01 Page 1 Outline 1. Introduction. Electrostatic (DC) Accelerators

More information

Bernhard Holzer, CERN-LHC

Bernhard Holzer, CERN-LHC Bernhard Holzer, CERN-LHC * 1 ... in the end and after all it should be a kind of circular machine need transverse deflecting force Lorentz force typical velocity in high energy machines: old greek dictum

More information

The FAIR Accelerator Facility

The FAIR Accelerator Facility The FAIR Accelerator Facility SIS300 existing GSI proton linac SIS18 UNILAC SIS100 HESR pbar target SuperFRS goals: higher intensity (low charge states) higher energy (high charge states) production of

More information

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

Short Introduction to CLIC and CTF3, Technologies for Future Linear Colliders Short Introduction to CLIC and CTF3, Technologies for Future Linear Colliders Explanation of the Basic Principles and Goals Visit to the CTF3 Installation Roger Ruber Collider History p p hadron collider

More information

Physics 417/517 Introduction to Particle Accelerator Physics. G. A. Krafft Jefferson Lab Jefferson Lab Professor of Physics Old Dominion University

Physics 417/517 Introduction to Particle Accelerator Physics. G. A. Krafft Jefferson Lab Jefferson Lab Professor of Physics Old Dominion University Physics 417/517 Introduction to Particle Accelerator Physics G. A. Krafft Jefferson Lab Jefferson Lab Professor of Physics Old Dominion University Methods of Acceleration Acceleration by Static Electric

More information

TUNE SPREAD STUDIES AT INJECTION ENERGIES FOR THE CERN PROTON SYNCHROTRON BOOSTER

TUNE SPREAD STUDIES AT INJECTION ENERGIES FOR THE CERN PROTON SYNCHROTRON BOOSTER TUNE SPREAD STUDIES AT INJECTION ENERGIES FOR THE CERN PROTON SYNCHROTRON BOOSTER B. Mikulec, A. Findlay, V. Raginel, G. Rumolo, G. Sterbini, CERN, Geneva, Switzerland Abstract In the near future, a new

More information

Accelerator Physics Final Exam pts.

Accelerator Physics Final Exam pts. Accelerator Physics Final Exam - 170 pts. S. M. Lund and Y. Hao Graders: C. Richard and C. Y. Wong June 14, 2018 Problem 1 P052 Emittance Evolution 40 pts. a) 5 pts: Consider a coasting beam composed of

More information

Introduction to Transverse Beam Dynamics

Introduction to Transverse Beam Dynamics Introduction to Transverse Beam Dynamics B.J. Holzer CERN, Geneva, Switzerland Abstract In this chapter we give an introduction to the transverse dynamics of the particles in a synchrotron or storage ring.

More information

Physics 598ACC Accelerators: Theory and Applications

Physics 598ACC Accelerators: Theory and Applications Physics 598ACC Accelerators: Theory and Instructors: Fred Mills, Deborah Errede Lecture 6: Collective Effects 1 Summary A. Transverse space charge defocusing effects B. Longitudinal space charge effects

More information

CERN EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH CTF3 DRIVE BEAM INJECTOR OPTIMISATION

CERN EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH CTF3 DRIVE BEAM INJECTOR OPTIMISATION CERN EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH CLIC Note 1060 CTF3 DRIVE BEAM INJECTOR OPTIMISATION - 1 Sh. Sanaye Hajari 1, 2, * H. Shaker 1, 2 and S. Doebert 2 Institute for Research in Fundamental

More information

3. Particle accelerators

3. Particle accelerators 3. Particle accelerators 3.1 Relativistic particles 3.2 Electrostatic accelerators 3.3 Ring accelerators Betatron // Cyclotron // Synchrotron 3.4 Linear accelerators 3.5 Collider Van-de-Graaf accelerator

More information

Physics at Accelerators

Physics at Accelerators Physics at Accelerators Course outline: The first 4 lectures covers the physics principles of accelerators. Preliminary plan: Lecture 1: Accelerators, an introduction. Acceleration principles. Lecture

More information

COMBINER RING LATTICE

COMBINER RING LATTICE CTFF3 TECHNICAL NOTE INFN - LNF, Accelerator Division Frascati, April 4, 21 Note: CTFF3-2 COMBINER RING LATTICE C. Biscari 1. Introduction The 3 rd CLIC test facility, CTF3, is foreseen to check the feasibility

More information

Extraction from cyclotrons. P. Heikkinen

Extraction from cyclotrons. P. Heikkinen Extraction from cyclotrons P. Heikkinen Classification of extraction schemes Linear accelerators Circular accelerators No extraction problem Constant orbit radius (sychrotrons, betatrons) Increasing orbit

More information

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

Graduate Accelerator Physics. G. A. Krafft Jefferson Lab Old Dominion University Lecture 1 Graduate Accelerator Physics G. A. Krafft Jefferson Lab Old Dominion University Lecture 1 Course Outline Course Content Introduction to Accelerators and Short Historical Overview Basic Units and Definitions

More information

The Relativistic Stern-Gerlach Interaction as a Tool for Attaining the Spin Separation

The Relativistic Stern-Gerlach Interaction as a Tool for Attaining the Spin Separation The Relativistic Stern-Gerlach Interaction as a Tool for Attaining the Spin Separation P. Cameron, M. Conte, A. U. Luccio, W. W. MacKay, M. Palazzi and M. Pusterla Brookhaven National Laboratory, Upton,

More information

Physics 736. Experimental Methods in Nuclear-, Particle-, and Astrophysics. - Accelerator Techniques: Introduction and History -

Physics 736. Experimental Methods in Nuclear-, Particle-, and Astrophysics. - Accelerator Techniques: Introduction and History - Physics 736 Experimental Methods in Nuclear-, Particle-, and Astrophysics - Accelerator Techniques: Introduction and History - Karsten Heeger heeger@wisc.edu Homework #8 Karsten Heeger, Univ. of Wisconsin

More information

S1: Particle Equations of Motion S1A: Introduction: The Lorentz Force Equation

S1: Particle Equations of Motion S1A: Introduction: The Lorentz Force Equation S1: Particle Equations of Motion S1A: Introduction: The Lorentz Force Equation The Lorentz force equation of a charged particle is given by (MKS Units):... particle mass, charge... particle coordinate...

More information

arxiv: v1 [physics.acc-ph] 22 Aug 2014

arxiv: v1 [physics.acc-ph] 22 Aug 2014 THE SYNCHROTRON MOTION SIMULATOR FOR ADIABATIC CAPTURE STUDY IN THE TLS BOOSTER Cheng-Chin Chiang Taipei Taiwan arxiv:.7v [physics.acc-ph] Aug Abstract The synchrotron motion simulator is invented to simulate

More information

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

Accelerator Physics and Technologies for Linear Colliders University of Chicago, Physics 575 Accelerator Physics and Technologies for Linear Colliders University of Chicago, Physics 575 Lecture 1: S. D. Holmes, An Introduction to Accelerators for High Energy Physics I. Introduction to the Course

More information

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

Penning Traps. Contents. Plasma Physics Penning Traps AJW August 16, Introduction. Clasical picture. Radiation Damping. Penning Traps Contents Introduction Clasical picture Radiation Damping Number density B and E fields used to increase time that an electron remains within a discharge: Penning, 936. Can now trap a particle

More information

Beam Diagnostics Lecture 3. Measuring Complex Accelerator Parameters Uli Raich CERN AB-BI

Beam Diagnostics Lecture 3. Measuring Complex Accelerator Parameters Uli Raich CERN AB-BI Beam Diagnostics Lecture 3 Measuring Complex Accelerator Parameters Uli Raich CERN AB-BI Contents of lecture 3 Some examples of measurements done with the instruments explained during the last 2 lectures

More information

Accelerator Basics. Abhishek Rai IUAC

Accelerator Basics. Abhishek Rai IUAC Accelerator Basics Abhishek Rai IUAC School on Accelerator Science and Technology May 7-18, 2018 Some basics Charge on an electron(e) = 1.6 10-19 Coulomb (1 unit of charge) 1 Atomic mass unit (amu) = 1.66

More information

3. Synchrotrons. Synchrotron Basics

3. Synchrotrons. Synchrotron Basics 1 3. Synchrotrons Synchrotron Basics What you will learn about 2 Overview of a Synchrotron Source Losing & Replenishing Electrons Storage Ring and Magnetic Lattice Synchrotron Radiation Flux, Brilliance

More information

Compressor Lattice Design for SPL Beam

Compressor Lattice Design for SPL Beam EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH CERN A&B DIVISION AB-Note-27-34 BI CERN-NUFACT-Note-153 Compressor Lattice Design for SPL Beam M. Aiba Abstract A compressor ring providing very short proton

More information

Introduction and Overview of Accelerators

Introduction and Overview of Accelerators Introduction and Overview of Accelerators Fanglei Lin Center for Advanced Studies of Accelerators, Jefferson Lab 29th Annual Hampton University Graduate Studies Program HUGS 2014, Jefferson Lab, June 2-20,

More information

Transverse dynamics. Transverse dynamics: degrees of freedom orthogonal to the reference trajectory

Transverse dynamics. Transverse dynamics: degrees of freedom orthogonal to the reference trajectory Transverse dynamics Transverse dynamics: degrees of freedom orthogonal to the reference trajectory x : the horizontal plane y : the vertical plane Erik Adli, University of Oslo, August 2016, Erik.Adli@fys.uio.no,

More information

Introduction to particle accelerators

Introduction to particle accelerators Introduction to particle accelerators Walter Scandale CERN - AT department Lecce, 17 June 2006 Introductory remarks Particle accelerators are black boxes producing either flux of particles impinging on

More information

Direct-Current Accelerator

Direct-Current Accelerator Nuclear Science A Teacher s Guide to the Nuclear Science Wall Chart 1998 Contemporary Physics Education Project (CPEP) Chapter 11 Accelerators One of the most important tools of nuclear science is the

More information

First propositions of a lattice for the future upgrade of SOLEIL. A. Nadji On behalf of the Accelerators and Engineering Division

First propositions of a lattice for the future upgrade of SOLEIL. A. Nadji On behalf of the Accelerators and Engineering Division First propositions of a lattice for the future upgrade of SOLEIL A. Nadji On behalf of the Accelerators and Engineering Division 1 SOLEIL : A 3 rd generation synchrotron light source 29 beamlines operational

More information

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

Summary of lecture 1 and 2: Main ingredients in LHC success Summary of lecture 1 and 2: Main ingredients in LHC success LHC LHC Tevatron Tevatron s=1.8tev Energy 10 times higher cross section than Tevatron and integrated luminosity already ½ at end of 2011! 1 Lectures

More information

Accelerator Physics. Elena Wildner. Transverse motion. Benasque. Acknowldements to Simon Baird, Rende Steerenberg, Mats Lindroos, for course material

Accelerator Physics. Elena Wildner. Transverse motion. Benasque. Acknowldements to Simon Baird, Rende Steerenberg, Mats Lindroos, for course material Accelerator Physics Transverse motion Elena Wildner Acknowldements to Simon Baird, Rende Steerenberg, Mats Lindroos, for course material E.Wildner NUFACT08 School Accelerator co-ordinates Horizontal Longitudinal

More information

50 MeV 1.4 GeV 25GeV 450 GeV 8 TeV. Sources of emittance growth CAS 07 Liverpool. Sept D. Möhl, slide 1

50 MeV 1.4 GeV 25GeV 450 GeV 8 TeV. Sources of emittance growth CAS 07 Liverpool. Sept D. Möhl, slide 1 * 5 KeV 750 KeV 50 MeV 1.4 GeV 5GeV 450 GeV 8 TeV Sources of emittance growth CAS 07 Liverpool. Sept. 007 D. Möhl, slide 1 Sources of Emittance Growth Dieter Möhl Menu Overview Definition of emittance,

More information

Linear and circular accelerators

Linear and circular accelerators Linear and circular accelerators Ion Accelerator Physics and Technology Oliver Boine-Frankenheim, Gesellschaft für Schwerionenforschung (GSI), Darmstadt Tel. 06159 712408, O.Boine-Frankenheim@gsi.de o

More information

Advanced Design of the FAIR Storage Ring Complex

Advanced Design of the FAIR Storage Ring Complex Advanced Design of the FAIR Storage Ring Complex M. Steck for the FAIR Technical Division and the Accelerator Division of GSI The FAIR Accelerator Facility SIS300 existing GSI proton linac SIS18 UNILAC

More information

APPLICATIONS OF ADVANCED SCALING FFAG ACCELERATOR

APPLICATIONS OF ADVANCED SCALING FFAG ACCELERATOR APPLICATIONS OF ADVANCED SCALING FFAG ACCELERATOR JB. Lagrange ), T. Planche ), E. Yamakawa ), Y. Ishi ), Y. Kuriyama ), Y. Mori ), K. Okabe ), T. Uesugi ), ) Graduate School of Engineering, Kyoto University,

More information

Weak focusing I. mv r. Only on the reference orbit is zero

Weak focusing I. mv r. Only on the reference orbit is zero Weak focusing I y x F x mv r 2 evb y Only on the reference orbit is zero r R x R(1 x/ R) B y R By x By B0y x B0y 1 x B0 y x R Weak focusing (II) Field index F x mv R 2 x R 1 n Betatron frequency 2 Fx mx

More information

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

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 koji.takata@kek.jp http://research.kek.jp/people/takata/home.html Accelerator

More information