accelerator physics and ion optics summary longitudinal optics

Transcription

1 accelerator physics and ion optics summary longitudinal optics Sytze Brandenburg sb/accphys003_5/1

2 feedback energy difference acceleration phase stability when accelerating on slope of sine low energy: rising slope high energy (above transition): falling slope stable region depends on phase reference particle sb/accphys003_5/

3 concept longitudinal optics same as transverse motion transverse: quadrupole longitudinal: buncher phase difference energy difference at time focus phase difference strongly reduced initial energy spread blurs time focus sb/accphys003_5/3

4 accelerator physics and ion optics distortion and resonances Sytze Brandenburg sb/accphys003_5/4

5 dipole error induced by dipole magnet different strength different length dipole kick ( ) quadrupole magnet BL = BL+ B L y y y positioning error x and/or y B y (x) = gx; B x (y) = -gy ( BL) y dipole kick = g xl sb/accphys003_5/5

6 dipole error single error along circumference angle kick x = (B y L)/Bρ largest effect when close to F-quadrupole minimum divergence, maximum beamsize smallest effect when close to D-quadrupole maximum divergence, minimum beamsize sb/accphys003_5/6

7 dipole error at F-quadrupole sb/accphys003_5/7

8 dipole error at F-quadrupole sb/accphys003_5/7

9 dipole error at F-quadrupole sb/accphys003_5/7

10 dipole error at F-quadrupole sb/accphys003_5/7

11 dipole error at F-quadrupole sb/accphys003_5/7

12 dipole error at F-quadrupole sb/accphys003_5/7

13 error at D-quadrupole sb/accphys003_5/8

14 error at D-quadrupole sb/accphys003_5/8

15 error at D-quadrupole sb/accphys003_5/8

16 error at D-quadrupole sb/accphys003_5/8

17 error at D-quadrupole sb/accphys003_5/8

18 error at D-quadrupole sb/accphys003_5/8

19 error at D-quadrupole sb/accphys003_5/8

20 error at D-quadrupole sb/accphys003_5/8

21 closed orbit distortion δ-function kick ( BL) ( ) y q BL y x' = = Bρ requirement for closed orbit: after one turn x x = R, R matrix for full turn ' ' ' x x x p sb/accphys003_5/9

22 solution in space coordinates R cosπ Q +α sinπq β sinπq 0 0 = γ0 sinπq cos πq α0 sin πq α 0, β 0 and γ 0 depend on location field error ( ) ( ) x cosπ Q+α sinπq 1 + x' β sinπ Q= x γ sinπ Q+ x' cosπq α sinπq 1 = x' solution x 0 = β 0 x' tan π Q x' α0 x' 0 = 1 tanπq Q integer amplitude explodes resonance sb/accphys003_5/10

23 solution in Floquet coordinates Floquet coordinate transformation (see also lecture 3) ( ) ( s) s x s 1 d σ η( s) ψ ( s) = β Q βσ ψ changes by π per turn 0 ( ) field perturbations along orbit given by ( ) Fs = B y Bρ ( s) equation of motion of η 3 d η Q s Q F s + η=β dψ ( ) ( ) sb/accphys003_5/11

24 δ-function perturbation equation inhomogeneous in one point except at perturbation homogeneous solution ( ) ( ) ( ) η s =η cosq ψ s ψ π =η cosφ K K K c phase at perturbation -Qπ decreasing φ c from zero: approaching from above Qπ increasing φ c from zero: approaching from below sb/accphys003_5/1

25 at perturbation dη KQsin c 0Qsin( Q ) 0QsinQ d = η φ = η π =η π ψ + dη = ηkqsinφ c = η0qsinqπ d ψ dx relate to real kick ds dψ 1 dx dη 1 dη = = β K = ds Qβ ds ds Q β dψ sb/accphys003_5/13 K ( BL) y x' dx = = = K π Bρ ds η = K β K sinqπ ( BL) y Bρ η β K sinq K

26 graphical representation complete turn - perturbation: φ c = πq orbit should be closed: φ c = πn η K = 0 (trivial solution, no kick) kick closes orbit φ K = π(n-q) φ = Qπ φ = Qπ dη/dψ η sb/accphys003_5/14

27 distorted orbit ( s) β ( BL) y β K x( s) = β( s) η ( s) = cosq ψ s ψ π sinqπ Bρ ( ( ) K ) distortions at locations s Ki, corresponding to ψ Ki sum contributions β ( BL) Ki y x( s) = β( s) cosq ψ( s) ψki π i sinqπ Bρ ( ) sb/accphys003_5/15

28 Fourier analysis of perturbations equation of motion of η 3 d η Q s Q F s + η=β dψ ( ) ( ) expand β 3/ F(s) in Fourier series (periodic system) d η + η=β = dψ 3 ( ) ikψ Q s Q F ( s) Q fke k= 1 π π 3 ik 1 1 ψ 1 ikψ( s) fk = β ( s) F( s) e dψ = β ( s) F( s) e ds π πq 0 0 dψ 1 = ds Q β K sb/accphys003_5/16

29 Fourier analysis of perturbations equation of motion of η 3 d η Q s Q F s + η=β dψ ( ) ( ) expand β 3/ F(s) in Fourier series (periodic system) d η + η=β = dψ 3 ( ) ikψ Q s Q F ( s) Q fke k= 1 π π 3 ik 1 1 ψ 1 ikψ( s) fk = β ( s) F( s) e dψ = β ( s) F( s) e ds π πq 0 0 solution η= Re k= 1 Q Q fk k e ikψ sb/accphys003_5/16

30 η= Re k= 1 Q Q fk k e ikψ amplitude very large for Q close to k resonance 100 Q / Q -k 10 sb/accphys003_5/ Q

31 η= Re k= 1 Q Q fk k e ikψ amplitude very large for Q close to k resonance 10 5 Q = 6.4 Q /(Q -k ) k sb/accphys003_5/17

32 closed orbit bumps correction of field perturbations displacement of closed orbit for injection and extraction ( ) BL y x( s) = β s βk sin φ φ Bρ ( ) ( ) simplest case: betatron phase advance π between two bumps K sb/accphys003_5/18

33 closed orbit bumps correction of field perturbations displacement of closed orbit for injection and extraction ( ) BL y x( s) = β s βk sin φ φ Bρ ( ) ( ) simplest case: betatron phase advance π between two bumps x' K δ1 δ x sb/accphys003_5/18

34 more general case: three field bumps: control x at specific location four field bumps: control x and x at specific location sb/accphys003_5/19

35 more general case: three field bumps: control x at specific location four field bumps: control x and x at specific location x' δ1 δ3 δ x sb/accphys003_5/19

36 general transfer matrix β ( cos φ+α1sin φ) ββ 1 sin φ x β1 x x' = 1 x' β1 ( α α ) cos φ+ ( 1+α α ) sin φ ( cos φ α sin φ) ββ β 1 x() related to x (1) ( ) =δ ββ sin( φ φ ) x x (3) related to x(): by going backward ( ) =δ ββ sin( φ φ ) x δ1 β 1 = sinφ δ β 3 3 sinφ 3 1 sb/accphys003_5/0

37 bump δ determined by change of x at x() dx dx dφ = ds d φ ds dx 1 β =δ ββ cos φ ϕ =δ φ ϕ ds 1 ( ) cos( ) β β + dx β =δ cos φ ϕ ds ( ) β + dx dx δ = ds + ds after some algebra δ1 β1 δ β δ β = = sinφ sinφ sinφ sb/accphys003_5/1

38 closed orbit correction profile monitors at each quadrupole sensitivity proportional to β horizontal at F-quadrupole vertical at D-quadrupole steering magnets at each quadrupole effect proportional to β horizontal at F-quadrupole vertical at D-quadrupole use magnets n-1, n and n+1 to correct error n linear problem N equations, N unknowns matrix inversion sb/accphys003_5/

39 injection: transversal stacking displace closed orbit with injection magnets in ring inject one pulse reduce strength injection magnets inject next pulse etc. sb/accphys003_5/3

40 injection: transversal stacking displace closed orbit with injection magnets in ring inject one pulse reduce strength injection magnets inject next pulse etc. sb/accphys003_5/3

41 injection: transversal stacking displace closed orbit with injection magnets in ring inject one pulse reduce strength injection magnets inject next pulse etc. sb/accphys003_5/3

42 injection: transversal stacking displace closed orbit with injection magnets in ring inject one pulse reduce strength injection magnets inject next pulse etc. sb/accphys003_5/3

43 injection: transversal stacking displace closed orbit with injection magnets in ring inject one pulse reduce strength injection magnets inject next pulse etc. sb/accphys003_5/3

44 injection: transversal stacking displace closed orbit with injection magnets in ring inject one pulse reduce strength injection magnets inject next pulse etc. sb/accphys003_5/3

45 injection: transversal stacking displace closed orbit with injection magnets in ring inject one pulse reduce strength injection magnets inject next pulse etc. sb/accphys003_5/3

46 injection: transversal stacking displace closed orbit with injection magnets in ring inject one pulse reduce strength injection magnets inject next pulse etc. sb/accphys003_5/3

47 quadrupole error matrix of nominal quadrupole magnet (thin lense) 1 0 g MQ = By( x) = gx k = kl 1 Bρ matrix of perturbed quadrupole magnet M Q+ Q 1 0 ( k+ k) L 1 matrix one turn with perturbed quadrupole M= MQ+ QMQM0 = M0 kl 1 sb/accphys003_5/4

48 cosφ 0 +α0sinφ0 β0sinφ0 M = kl( cos 0 0sin 0) 0sin 0 kl 0sin 0 cos 0 0sin φ +α φ γ φ β φ + φ α φ0 α 0, β 0, γ 0 and φ 0 : betatron functions and phase at quadrupole Tr(M) = cos φ cosφ= cosφ klβ sinφ cosφ= φsinφ 0 = klβ0sinφ φ klβ0 Q = = π 4 π 0 sb/accphys003_5/5

49 second order resonance angle kick proportional to position ( ) dx s = x s kl = klη0 β s cosφ s ds ( ) ( ) ( ) in (η, φ)-coordinates dη = klη0βcosφ dφ dη dη dφ dη = =β dφ ds ds ds φ = π Q dη/dφ η sb/accphys003_5/6

50 second order resonance dη 1 η 0 = sin kl 0 cos sin kl 0 sin d φ= ηβ φ φ= ηβ φ φ 1 dη klβ φ= cosφ= klβcos φ= ( 1+ cosφ) η0 dφ φ klβ Q= = 1+ cosφ π 4π ( ) φ = π Q dη/dφ resonance for Q = N/ η sb/accphys003_5/7

51 width second order resonance dη 1 η 0 = sinφ= klηβ 0 cosφsinφ= klηβ 0 sinφ d φ per turn φ= πq resonance for φ = 4πQ= πn Q = N/ φ klβ Q = = ( 1+ cosφ) π 4π klβ Q oscillates in band with width Q = 4π if Q - N/ < Q locking in resonant condition at some moment in Q-oscillation Q = N/ sb/accphys003_5/8

52 why resonance for Q = N/ coordinates at passage of quadrupole x 0, x 0 kick (kl)x 0 after one turn for Q = N coordinates x 1 = x 0 + δx, x 1 = x 0 +(δx), kick (kl)x 1 after one turn for Q = M/ coordinates -x 1 = -(x 0 + δx), -x 1 = -(x 0 +(δx) ), kick - (kl)x 1 mirror symmetry kicks coherent for Q = N and Q = M/ sb/accphys003_5/9

53 sextupole error second order effect angle kick proportional to x ( ) dx s db L db L x s 0 s cos s ds = dx Bρ = dx Bρ η β φ y y ( ) ( ) ( ) analysis analogous to quadrupole error in (η, φ)-coordinates dby L 0 cos 3 dη d = β η φ φ dx Bρ dη dφ dη dφ = =β ds ds dη ds sb/accphys003_5/30

54 third order resonance 3 dη dby L η 0 = sin 0cos sin d φ = β η φ φ φ dx Bρ 3 1 dη db y L 3 φ= cosφ= β η 0 cos φ η0 dφ dx Bρ dby 3 L = β η0 φ+ φ dx 8Bρ 3 dby ( cos3 3cos ) φ β L Q= = η0 cos3φ+ 3cosφ π 16π dx Bρ ( ) Q close to N/3 resonance second term averages out in three turns sb/accphys003_5/31

55 width third order resonance 3 dby β L Q= η0 cos3φ+ 3cosφ 16π dx Bρ ( ) β dby L Q moves in band Q Q < η 16π dx Bρ amplitude changes given by dby L a =β a sin3 dx 8Bρ φ Q = N/3 amplitude grows quadratically no locking because Q amplitude dependent amplitude growth faster than change in Q beam losses sb/accphys003_5/3

56 third order resonant extraction Q= dby β L a 16π dx Bρ Q = N/3 - Q: particles will not hit resonance for a < 16πBρ Q dby βl dx stable area reduce Q with quadrupoles particles pushed into unstable area can be extracted from ring sb/accphys003_5/33

57 third order resonant extraction stable area particles on closed orbit Q periods per turn unstable area jump from one trajectory to another Q = p/3 step π/3 Q = p/3 step 4π/3 Q = p step π sb/accphys003_5/34

58 Fourier analysis Fourier expansion of perturbation around ring P ( ψ ) = k p coskψ response on single perturbation n = quadrupole; n = 3 sextupole 1 Q = βpcosnqψ π overall response π 1 Q= βp( ψ) cosnqψdψ π 0 π 1 = βpk cosnqψcoskψdψ π 0 large for nq = k driven by single harmonic of distribution sb/accphys003_5/35

59 resonance zoo simple resonance mq x = p; nq y = p coupling resonances drive e.g. rotated quad mq x ± nq y = p + sign: beamloss - sign exchange of amplitude sb/accphys003_5/36

60 chromaticity tune on momentum (second order) Q = Q p/p 0 caused by momentum dependence focussing 1 db k = y k p = B ρ dx k p 0 treatment analogous to quadrupole error π π 1 1 p Q = β( s) k( s) ds= β( s) k( s) ds 4π 4π p typical value Q 1.3 Q; Q 5 p/p 0 = x 10-3 ; Q 0.15 too large to escape resonances sb/accphys003_5/37

61 chromaticity tune on momentum (second order) Q = Q p/p 0 caused by momentum dependence focussing 1 db k = y k p = B ρ dx k p 0 treatment analogous to quadrupole error π π 1 1 p Q = β( s) k( s) ds= β( s) k( s) ds 4π 4π p typical value Q 1.3 Q; Q 5 p/p 0 = x 10-3 ; Q 0.15 too large to escape resonances momentum dependent additional focussing needed sb/accphys003_5/37

62 dispersion function: radius depends on momentum magnet with radial dependent gradient = sextupole locations with large dispersionfunction h By x,y = x y Bx x,y = hxy sextupole ( ) ( ) ( ) sb/accphys003_5/38

63 focussing strength hd k = B ρ p p ( ) ( ) π π 1 1 p hsds Q = β( s) k( s) ds= β( s) ds 4π 4π p Bρ separate correction for Q x and Q y two sets of sextupoles width third order resonance amplitude dependent constraints on useful acceptance sb/accphys003_5/39

64 next lecture damping and cooling reading material Wilson: chapter 8 Electrons Wilson: chapter 1 Cooling CERN Accelerator School 199, CERN report Chapter 18 Synchrotron radiation Chapter 4 Cooling techniques presentations and excercises available in PDF-format on sb/accphys003_5/40