ELECTRON DYNAMICS with SYNCHROTRON RADIATION

Transcription

1 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 Physics September 5, 2014, Prague, Czech Republic

2 Useful books and references H. Wiedemann, Synchrotron Radiation Springer-Verlag Berlin Heidelberg 2003 H. Wiedemann, Particle Accelerator Physics I and II Springer Study Edition, 2003 A. Hofmann, The Physics of Synchrotron Radiation Cambridge University Press 2004 A. W. Chao, M. Tigner, Handbook of Accelerator Physics and Engineering, World Scientific 1999

3 CERN Accelerator School Proceedings Synchrotron Radiation and Free Electron Lasers Grenoble, France, April 1996 (A. Hofmann s lectures on synchrotron radiation) CERN Yellow Report Brunnen, Switzerland, 2 9 July 2003 CERN Yellow Report

4 Curved orbit of electrons in magnet field Accelerated charge Electromagnetic radiation

5 Crab Nebula 6000 light years away GE Synchrotron New York State First light observed 1054 AD First light observed 1947

6 GENERATION OF SYNCHROTRON RADIATION Swiss Light Source, Paul Scherrer Institute, Switzerland

7 Why do they radiate? Charge at rest: Coulomb field, no radiation Uniformly moving charge does not radiate But! Cerenkov! v = const. Accelerated charge

8 Bremsstrahlung or braking radiation

9 Transverse acceleration a v Radiation field quickly separates itself from the Coulomb field

10 Longitudinal acceleration a Radiation field cannot separate itself from the Coulomb field v

11 Fields of a moving charge E t = q 4 0 n 1 n r 2 ret + q 4 0 c n n 1 n r ret B t = 1 c n E

12 Moving Source of Waves

13 Time compression Electron with velocity emits a wave with period T emit while the observer sees a different period T obs because the electron was moving towards the observer n The wavelength is shortened by the same factor in ultra-relativistic case, looking along a tangent to the trajectory obs = emit since T ( 1nβ) obs T emit ( 1 cos ) obs emit 1 =

14 Radiation is emitted into a narrow cone e v ~ c = 1 e v << c vc

15 Sound waves (non-relativistic) Angular collimation = e v v s v s + v = v s v 1 s 1 + v v e v s v s v Doppler effect (moving source of sound) heard emitted 1 v v s

16 Synchrotron radiation power Power emitted is proportional to: P E 2 B 2 P cc E C = 4 3 r e 5 m e c 2 3 = m 10 GeV 3

17 P cc E The power is all too real! 2 4 2

18 Typical frequency of synchrotron light Due to extreme collimation of light observer sees only a small portion of electron trajectory (a few mm) l ~ 2 Pulse length: difference in times it takes an electron 1/ and a photon to ~ 1 t ~ 3 0 cover this distance t ~ l c l c = l c 1 t ~ c 1 2 2

19 Spectrum of synchrotron radiation Synchrotron light comes in a series of flashes every T 0 (revolution period) T 0 the spectrum consists of harmonics of 0 1 T 0 time flashes are extremely short: harmonics reach up to very high frequencies At high frequencies the individual harmonics overlap 3 typ 0 ~ 1 ~ 4000 continuous spectrum! ~ 10 MHz 0 typ 16 Hz!

20 Wavelength continuously tunable!

21 Synchrotron radiation power Power emitted is proportional to: P E 2 B 2 P 4 cc E 2 2 P 2 c C = 4 3 r e 5 m e c 2 3 = m 10 GeV 3 = Energy loss per turn: U 0 = C E 4 hc = 197 Mev fm U 0 = 4 3 hc 4

22 dp d = P tot c S c S x = x K5 5 3 x dx x 0 S x dx = 1 P tot = 2 3 hc2 4 2 c = 3 c ~ 2.1x 1 3 G 1 x = x K 5 3 x dx x c ev = 665E 2 GeV B T 50% ~ 1.3 xe x x = c

23 Flux [photons/s/mrad/0.1%bw] Synchrotron radiation flux for different electron energies LEP Dipole Flux I = 1 ma 100 GeV 50 GeV GeV Photon energy [ev]

24 Angular divergence of radiation The rms opening angle R at the critical frequency: = c R 0.54 well below «c R 1 c independent of! 1 3 well above» c R 0.6 c 1 2

25 Radiation effects in electron storage rings Average radiated power restored by RF Electron loses energy each turn RF cavities provide voltage to accelerate electrons back to the nominal energy Radiation damping Average rate of energy loss produces DAMPING of electron oscillations in all three degrees of freedom (if properly arranged!) Quantum fluctuations Statistical fluctuations in energy loss (from quantised emission of radiation) produce RANDOM EXCITATION of these oscillations Equilibrium distributions U of E 0 V RF > U 0 The balance between the damping and the excitation of the electron oscillations determines the equilibrium distribution of particles in the beam

26 Radiation is emitted into a narrow cone of only a few mrads opening angle

27 Synchrotron radiation power Power emitted is proportional to: P E 2 B 2 P 4 cc E 2 2 P 2 c C = 4 3 r e 5 m e c 2 3 = m 10 GeV 3 = Energy loss per turn: U 0 = C E 4 hc = 197 Mev fm U 0 = 4 3 hc 4

28 RADIATION DAMPING TRANSVERSE OSCILLATIONS

29 Average energy loss and gain per turn Every turn electron radiates small amount of energy E 1 = E 0 U 0 = E 0 1 U 0 E 0 only the amplitude of the momentum changes P 1 = P 0 U 0 c = P 0 1 U 0 E 0 Only the longitudinal component of the momentum is increased in the RF cavity Energy of betatron oscillation E A 2 A 1 2 = A U 0 E 0 or A 1 A 0 1 U 0 2E 0

30 Damping of vertical oscillations But this is just the exponential decay law! A A = U 0 2E The oscillations are exponentially damped with the damping time (milliseconds!) 2ET U 0 0 In terms of radiation power 2E P AA e t 0 the time it would take particle to lose all of its energy 4 and since P E E 3 1

31 Adiabatic damping in linear accelerators In a linear accelerator: p p In a storage ring beam passes many times through same RF cavity x = p p decreases E 1 p p Clean loss of energy every turn (no change in x ) Every turn is re-accelerated by RF (x is reduced) Particle energy on average remains constant

32 Emittance damping in linacs: W W 4 W 4 1 or 4 const.

33 RADIATION DAMPING LONGITUDINAL OSCILLATIONS

34 Longitudinal motion: compensating radiation loss U 0 RF cavity provides accelerating field with frequency h harmonic number V RF f RF h f 0 The energy gain: U 0 URF ev RF Synchronous particle: has design energy gains from the RF on the average as much as it loses per turn U 0

35 Longitudinal motion: phase stability U 0 V RF Particle ahead of synchronous one gets too much energy from the RF goes on a longer orbit (not enough B) >> takes longer to go around comes back to the RF cavity closer to synchronous part. Particle behind the synchronous one gets too little energy from the RF goes on a shorter orbit (too much B) catches-up with the synchronous particle

36 Longitudinal motion: energy-time oscillations energy deviation from the design energy, or the energy of the synchronous particle longitudinal coordinate measured from the position of the synchronous electron

37 Orbit Length Length element depends on x dl = 1 + x ds dl x ds Horizontal displacement has two parts: x = x + x To first order x does not change L x has the same sign around the ring Length of the off-energy orbit L = dl = 1 + x ds = L 0 +L L = D s s ds where = p p = E E L L =

38 Something funny happens on the way around the ring... Revolution time changes with energy T T = L L Particle goes faster (not much!) while the orbit length increases (more!) Ring is above transition energy isochronous ring: T 0 = L 0 c d = 1 2 dp p The slip factor since >> 1 2 T = 1 T 2 dp p = dp p = 0 or = tr 1 2 tr (relativity) L = dp L p

39 Not only accelerators work above transition Dante Aligieri Divine Comedy

40 RF Voltage V RF U 0 V Vˆ sin h 0 s here the synchronous phase s U arcsin 0 evˆ

41 Momentum compaction factor 1 L Like the tunes Q x, Q y - depends on the whole optics D s s ds A quick estimate for separated function guide field: = 1 L 0 0 mag D s ds L mag = 2 0 = 1 L 0 0 D L mag But = D R Since dispersion is approximately D R Q 2 1 typically < 1% 2 Q and the orbit change for ~ 1% energy deviation L = L 2 Q = 0 in dipoles = elsewhere

42 Energy balance Energy gain from the RF system: U RF = ev RF = U 0 + ev RF synchronous particle () will get exactly the energy loss per turn we consider only linear oscillations Each turn electron gets energy from RF and loses energy to radiation within one revolution time T 0 = U 0 + ev RF U 0 + U V RF = dv RF d = 0 d dt = 1 T 0 ev RF U An electron with an energy deviation will arrive after one turn at a different time with respect to the synchronous particle d dt = E 0

43 Synchrotron oscillations: damped harmonic oscillator Combining the two equations where the oscillation frequency the damping is slow: the solution is then: t = 0 e t cos Wt + d 2 dt d dt + W2 = 0 W 2 ev RF T 0 E 0 U 2T 0 typically <<W similarly, we can get for the time delay: t = 0 e t cos Wt +

44 Synchrotron (time - energy) oscillations The ratio of amplitudes at any instant Oscillations are 90 degrees out of phase = WE 0 = + 2 The motion can be viewed in the phase space of conjugate variables, ˆ E 0, W E 0 ˆ W

45 V Vo sin s s Stable regime U Separatrix d( ) dt Longitudinal Phase Space

46 Longitudinal motion: damping of synchrotron oscillations During one period of synchrotron oscillation: when the particle is in the upper half-plane, it loses more energy per turn, its energy gradually reduces U > U 0 U < U 0 when the particle is in the lower half-plane, it loses less energy per turn, but receives U 0 on the average, so its energy deviation gradually reduces The synchrotron motion is damped 2 B 2 the phase space trajectory is spiraling towards the origin P E

47 Robinson theorem: Damping partition numbers Transverse betatron oscillations are damped with Synchrotron oscillations are damped twice as fast x z 2ET U ET U The total amount of damping (Robinson theorem) depends only on energy and loss per turn 1 x + 1 y + 1 = 2U 0 ET 0 = U 0 2ET 0 J x + J y + J the sum of the partition numbers J x + J z + J = 4

48 Radiation loss P E 2 B 2 Displaced off the design orbit particle sees fields that are different from design values energy deviation different energy: P different magnetic field B particle moves on a different orbit, defined by the off-energy or dispersion function D x γ E 2 both contribute to linear term in P γ betatron oscillations: zero on average

49 Radiation loss To first order in U rad = U 0 + U P E 2 B 2 electron energy changes slowly, at any instant it is moving on an orbit defined by D x after some algebra one can write U = U D E 0 U du rad de E0 D 0 only when k 0

50 Damping partition numbers J x + J z + J = 4 Typically we build rings with no vertical dispersion J 1 J 3 z Horizontal and energy partition numbers can be modified via D : J x J x 1D J 2 D Use of combined function magnets Shift the equilibrium orbit in quads with RF frequency

51 EQUILIBRIUM BEAM SIZES

52 Radiation effects in electron storage rings Average radiated power restored by RF Electron loses energy each turn RF cavities provide voltage to accelerate electrons back to the nominal energy Radiation damping Average rate of energy loss produces DAMPING of electron oscillations in all three degrees of freedom (if properly arranged!) Quantum fluctuations Statistical fluctuations in energy loss (from quantised emission of radiation) produce RANDOM EXCITATION of these oscillations Equilibrium distributions U of E 0 V RF > U 0 The balance between the damping and the excitation of the electron oscillations determines the equilibrium distribution of particles in the beam

53 Quantum nature of synchrotron radiation Damping only If damping was the whole story, the beam emittance (size) would shrink to microscopic dimensions!* Lots of problems! (e.g. coherent radiation) How small? On the order of electron wavelength E =mc 2 = h = hc e = 1 mc h = C e C = m Compton wavelength Diffraction limited electron emittance

54 Quantum nature of synchrotron radiation Quantum fluctuations Because the radiation is emitted in quanta, radiation itself takes care of the problem! It is sufficient to use quasi-classical picture:» Emission time is very short» Emission times are statistically independent (each emission - only a small change in electron energy) Purely stochastic (Poisson) process

55 Visible quantum effects I have always been somewhat amazed that a purely quantum effect can have gross macroscopic effects in large machines; and, even more, that Planck s constant has just the right magnitude needed to make practical the construction of large electron storage rings. A significantly larger or smaller value of would have posed serious -- perhaps insurmountable -- problems for the realization of large rings. Mathew Sands

56 Quantum excitation of energy oscillations Photons are emitted with typical energy at the rate (photons/second) Fluctuations in this rate excite oscillations During a small interval t electron emits photons u ph h typ = hc 3 N = P u ph N = N t losing energy of Actually, because of fluctuations, the number is resulting in spread in energy loss N u ph N N N u ph For large time intervals RF compensates the energy loss, providing damping towards the design energy E 0 Steady state: typical deviations from E 0 typical fluctuations in energy during a damping time

57 Equilibrium energy spread: rough estimate We then expect the rms energy spread to be and since E 0 P and P N u ph N u ph E 0 u ph geometric mean of the electron and photon energies! Relative energy spread can be written then as: e E e = m h 0 e c m it is roughly constant for all rings typically E 2 E 0 ~ const ~ 10 3

58 Equilibrium energy spread More detailed calculations give for the case of an isomagnetic lattice s = 0 in dipoles elsewhere E 2 = C q E 2 J 0 with C q = hc = m 10 m e c GeV 2 It is difficult to obtain energy spread < 0.1% limit on undulator brightness!

59 Equilibrium bunch length Bunch length is related to the energy spread Energy deviation and time of arrival (or position along the bunch) are conjugate variables (synchrotron oscillations) recall that W s V RF = W s E = W s E Two ways to obtain short bunches: RF voltage (power!) 1 V VRF RF Momentum compaction factor in the limit of = 0 isochronous ring: particle position along the bunch is frozen

60 Excitation of betatron oscillations x x x 0 x x x x x x E D x E D x E D x Courant Snyder invariant E D DD D x x x x

61 Excitation of betatron oscillations Electron emitting a photon at a place with non-zero dispersion starts a betatron oscillation around a new reference orbit x D E

62 Horizontal oscillations: equilibrium Emission of photons is a random process Again we have random walk, now in x. How far particle will wander away is limited by the radiation damping The balance is achieved on the time scale of the damping time x = 2 x N x D 2 E Typical horizontal beam size ~ 1 mm Quantum effect visible to the naked eye! Vertical size - determined by coupling D E

63 Beam emittance Betatron oscillations Particles in the beam execute betatron oscillations with different amplitudes. x Transverse beam distribution Gaussian (electrons) Typical particle: 1 - ellipse (in a place where = = 0) Emittance x 2 Units of x = x = / m rad Area = x x x = x x = x x

64 Equilibrium horizontal emittance Detailed calculations for isomagnetic lattice 2 x x0 = C qe 2 J x H mag where H = D 2 + 2DD + D 2 = 1 D 2 + D + D 2 and H mag is average value in the bending magnets

65 2-D Gaussian distribution Electron rings emittance definition 1 - ellipse x x n x dx = 1 2 e x 2 / 2 2 dx x x Area = x Probability to be inside 1- ellipse P 1 = 1 e 1 2 = 0.39 Probability to be inside n- ellipse P n = 1 e n 2 2

66 FODO cell lattice

67 Emittance FODO lattice emittance 100 H ~ D 2 ~ R Q 3 10 x0 C qe 2 J x R 1 Q 3 E2 J x 3 F FODO Phase advance per cell [degrees] 180

68 Ionization cooling p p absorber E acceleration similar to radiation damping, but there is multiple scattering in the absorber that blows up the emittance = MS 0 >> MS to minimize the blow up due to multiple scattering in the absorber we can focus the beam

69 Minimum emittance lattices C E 2 q 3 x0 θ Flatt J x F min =

70 Quantum limit on emittance Electron in a storage ring s dipole fields is accelerated, interacts with vacuum fluctuations: «accelerated thermometers show increased temperature» synchrotron radiation opening angle is ~ 1/-> a lower limit on equilibrium vertical emittance independent of energy G(s) =curvature, C q = pm in case of SLS: 0.2 pm isomagnetic lattice y 0.09 pm y Mag

71 Polarisation Synchrotron radiation observed in the plane of the particle orbit is horizontally polarized, i.e. the electric field vector is horizontal Observed out of the horizontal plane, the radiation is elliptically polarized E E

72 Polarisation: spectral distribution x S x S P x S P d dp c tot c tot x S S 8 7 S S 8 1 3:1

73 Angular divergence of radiation at the critical frequency well below 0. 2 c well above 2 c

74 Seeing the electron beam (SLS) Making an image of the electron beam using the vertically polarised synchrotron light

75 Seeing the electron beam (SLS) X rays visible light, vertically polarised x ~ 55m

76 Vertical emittance record Beam size m Emittance pm SLS beam cross section compared to a human hair: 80 m 4 m

77 Summary of radiation integrals Momentum compaction factor I 1 = D ds = I 1 2R Energy loss per turn U 0 = 1 2 C E 4 I 2 I 2 = I 3 = ds 2 ds 3 I 4 = D 2k ds I 5 = H 3 ds C = 4 3 r e 5 m e c 2 3 = m 10 GeV 3

78 Summary of radiation integrals (2) Damping parameter Damping times, partition numbers Equilibrium emittance x0 = 2 x =C qe 2 I 5 J x D = I 4 I 2 J = 2 + D, J x = 1 D, J y = 1 0 = 2ET 0 i = 0 J i Equilibrium energy spread 2 C = q E 2 I 3 E J I 2 I 2 U 0 C q = I 1 = I 2 = I 3 = D ds ds 2 ds 3 I 4 = D 2k ds I 5 = H 3 hc = m 10 m e c H = D 2 + 2DD + D 2 ds GeV 2

79 Damping wigglers Increase the radiation loss per turn U 0 with WIGGLERS reduce damping time emittance control P E P wig wigglers at high dispersion: blow-up emittance e.g. storage ring colliders for high energy physics wigglers at zero dispersion: decrease emittance e.g. damping rings for linear colliders e.g. synchrotron light sources (PETRAIII, 1 nm.rad)

80 END