IOTA Integrable Optics Test Accelerator at Fermilab. Sergei Nagaitsev May 21, 2012 IPAC 2012, New Orleans

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IOTA Integrable Optics Test Accelerator at Fermilab Sergei Nagaitsev May 1, 01 IPAC 01, New Orleans

Collaborative effort Fermilab: S. Nagaitsev, A. Valishev SNS: V. Danilov Budker INP: D. Shatilov BNL: H. Witte JAI (Oxford) Tech X Special thanks to E. Forest List of posters at IPAC01: TUPPC090 Beam Physics of Integrable Optics Test Accelerator at Fermilab TUEPPB003 Motion Stability in D Nonlinear Accelerator Lattice Integrable in Polar Coordinates WEPPR01 Simulating High-Intensity Proton Beams in Nonlinear Lattices with PyORBIT

Strong Focusing our standard method since 195 Christofilos (1949); Courant, Livingston and Snyder (195) x + K x ( s) x = 0 y + K y ( s) y = 0 K x, y ( s + C) = K x, y ( s) s is time -- piecewise constant alternating-sign functions Particle undergoes betatron oscillations 3 3

Strong focusing Specifics of accelerator focusing: Focusing fields must satisfy Maxwell equations in vacuum For stationary fields: focusing in one plane while defocusing in another quadrupole: Δ ϕ ( x, y, z) = 0 ϕ( xy, ) x y However, alternating quadrupoles results in effective focusing in both planes 4

5 Courant-Snyder invariant y x z z s K z or 0, ) ( " = = + Equation of motion for betatron oscillations ( ) 3 1 ) ( where β β β = + s K + = ) ( ) ( ) ( 1 z s z s z s I β β β Invariant (integral) of motion, a conserved qty.

Linear oscillations Normalized variables In this variables the motion is a linear oscillator Thus, betatron oscillations are linear; all particles oscillate with the same frequency! 6, ) ( ) ( ) (, ) ( s z s s p p s z z N N β β β β = = 1 () s ψ β = -- new time variable 0 n n d z z d ω ψ + = y y x x I I H ω = ω + 1 n n I pdz π =

Our goal Our goal is to create a practical nonlinear focusing system with a large frequency spread and stable particle motion. Benefits: Increased Landau damping Improved stability to perturbations Resonance detuning 7

Octupoles and tune spread In all machines there is a trade-off between Landau damping and dynamic aperture (resonances). Typical phase space portrait: 1. Regular orbits at small amplitudes. Resonant islands + chaos at larger amplitudes; 8

Linear vs nonlinear Accelerators are linear systems by design (freq. is independent of amplitude). In accelerators, nonlinearities are unavoidable (SC, beam-beam) and some are useful (Landau damping). All nonlinearities (in present rings) lead to resonances and dynamic aperture limits. Are there magic nonlinearities that create large spread and zero resonance strength? The answer is yes (we call them integrable ) 3D: VEPP000 kν x + lν y = m H = F( J1, J, J3) 9

Ideal Penning trap The ideal Penning trap is a LINEAR integrable and system It is a linear 3-d oscillator H = ω J + ω J + ω J 1 1 3 3 10

Kepler problem nonlinear integrable system Kepler problem: k V = r In spherical coordinates: H = ( J + J + J ) r mk θ φ Example of this system: the Solar system 11

Nonlinear systems can be more stable! 1D systems: non-linear oscillations can remain stable under the influence of periodic external force perturbation. Example: + z ω 0 sin( z) = a sin( ω0t) D: The resonant conditions kω ( J, J ) + lω ( J, J ) = m 1 1 1 are valid only for certain amplitudes. Nekhoroshev s condition guaranties detuning from resonance and, thus, stability. 1

Suppose that Example of a good nonlinear system d zn 3 ω z 0, where is or n αzn zn xn yn dψ + + = This would be a nonlinear equivalent to strong focusing We do NOT know how realize this particular example in practice! 13

On the way to integrability 1) Colliding beams: a) Round beam angular momentum conservation- 1D motion in r (Novosibirsk, 80 s, realized at VEPP000, tune shift around 0.15 achieved); b) Crab waist - decoupling x and y motion (P. Raimondi (006), tune shift 0.1 achieved at DΑΦΝΕ). ) Numerical methods to eliminate resonances (e.g. J. Cary and colleagues; D. Robin, W. Wan and colleagues); 3) Exact solutions for realization our goal. The list is presented in next slides Major limiting factor: fields must satisfy Maxwell eqtns. 14

1-D nonlinear optics 4 In 1967 E. McMillan published a paper p n, k 0 4 4 0 4 x n, k Final report in 1971. This is what later became known as the McMillan mapping : xi = pi 1 Bx + Dx f ( x) = p = x + f ( x ) Ax + Bx + C i i 1 i Ax p ( x p + xp ) + C( x + p ) + = const + B Dxp If A = B = 0 one obtains the Courant-Snyder invariant Generalizations (Danilov-Perevedentsev, 199-1995) 15

D case with realistic fields 1. The 1-D McMillan mapping was extended to -D round thin lens by R. McLachlan (1993) and by D-P (1995) Round lenses can be realized only with charge distributions: ar a) 1 or thin lenses with radial kicks f1( f)( r) = br + c1 ( c 1 r b) Time dependent potential U( ). β β. Approximate cases J. Cary & colleagues - decoupling of x-y motion and use of 1D solutions; 3. Stable integrable motion without space charge in Laplace fields the only known exact case is IOTA case (Danilov, Nagaitsev, PRSTAB 010); ) 16

Choice of nonlinear elements 1) For large beam size accumulators and boosters external fields can produce large frequency spread at beam size amplitudes; ) Small beam size colliders need nonlinearities on a beam-size scale. The ideal choice is colliding beam fields (like e-lens in Tevatron) The IOTA ring can test both variants of nonlinearities. 17

Advanced Superconductive Test Accelerator at Fermilab Photo injector ILC Cryomodules IOTA 18

Layout Beam from linac 19

IOTA schematic Injection, rf cavity Nonlinear inserts pc = 150 MeV, electrons (single bunch, 10^9) ~36 m circumference 50 quadrupoles, 8 dipoles, 50-mm diam vac chamber hor and vert kickers, 16 BPMs 0

Why electrons? Small size (~50 um), pencil beam Reasonable damping time (~1 sec) No space charge In all experiments the electron bunch is kicked transversely to sample nonlinearities. We intend to measure the turn-by-turn BPM positions as well as synch light to obtain information about phase space trajectories. 1

Proposed experiments We are proposing several experiments with nonlinear lenses Based on the electron (charge column) lens Based on electromagnets U 0 U = 0

Experiments with electron lens solenoid 150 MeV beam Example: Tevatron electron lens For IOTA ring, we would use a 5-kG, ~1-m long solenoid Electron beam: ~0.5 A, ~5 kev, ~1 mm radius 3

Experiment with a thin electron lens The system consists of a thin (L < β) nonlinear lens (electron beam) and a linear focusing ring Axially-symmetric thin McMillan lens: θ () r = kr ar + 1 Electron lens with a special density profile The ring has the following transfer matrix electron lens 0 β 0 0 1 0 0 0 ci si β si ci 0 0 0 β 1 0 0 0 β c = cos( φ) s = sin( φ) 1 0 I = 0 1 4

Electron lens (McMillan type) The system is integrable. Two integrals of motion (transverse): px i Angular momentum: xpy ypx = const McMillan-type integral, quadratic in momentum 4 0 py i 4 4 0 4 4 x i 4 0 4 0 4 For large amplitudes, the fractional tune is 0.5 For small amplitude, the electron (defocusing) lens can give a tune shift of ~-0.3 Potentially, can cross an integer resonance y i Electron lens current density: nr () I ( ar + 1) 5

0.5 Ideal McMillan round lens FMA fractional tunes ν y Linear tune Large amplitudes (0.3,0.) 0 Small amplitudes 0 0.5 ν x 6

Practical McMillan round lens e-lens (1 m long) is represented by 50 thin slises. Electron beam radius is 1 mm. The total lens strength (tune shift) is 0.3 FMA analysis All excited resonances have the form k (ν x + ν y ) = m They do not cross each other, so there are no stochastic layers and diffusion 7

Experiments with nonlinear magnets See: Phys. Rev. ST Accel. Beams 13, 08400 (010) Start with a round axially-symmetric LINEAR focusing lattice (FOFO) Add special non-linear potential V(x,y,s) such that ΔV ( x, y, s) ΔV ( x, y) = 0 Sun Apr 5 0:48:31 010 OptiM - MAIN: - C:\Documents and Settings\nsergei\My Documents\Papers\Invariants\Round 0 5 βx = βy BETA_X&Y[m] V(x,y,s) V(x,y,s) V(x,y,s) V(x,y,s) V(x,y,s) DISP_X&Y[m] 0 0 BETA_X BETA_Y DISP_X DISP_Y 40 0 8

Fake thin lens inserts Example only! Tue Feb 14:40:15 011 OptiM - MAIN: - C:\Users\nsergei\Documents\Papers\Invariants\Round lens\quad line1.opt BETA_X&Y[m] DISP_X&Y[m] 00 5 1 0 0 0 k 1 0 0 0 0 1 0 0 0 k 1 0 1 0 0 0 k 1 0 0 0 0 1 0 0 0 k 1 1 0 0 0 k 1 0 0 0 0 1 0 0 0 k 1 V(x,y,s) V(x,y,s) V(x,y,s) 1 0 0 0 k 1 0 0 0 0 1 0 0 0 k 1 0 BETA_X BETA_Y DISP_X DISP_Y 110.04 0 9

4-Magnet Lattice (Exp. 3-4) Equal beta-functions, Qx=5.0+0.3 4, Qy=4.0+0.3 4 Dispersion=0 in the Nonlinear Magnet Maximum Vertical amplitude in the NM=11 mm α=0.015 βx=βy, Q=0.5 Q=0.5 30

Main ideas 1. Start with a time-dependent Hamiltonian: pxn + p yn xn + y N H N = + + β ( ψ ) V xn β ( ψ ), y N β ( ψ ), s( ψ ). Chose the potential to be time-independent in new variables pxn + p yn xn + y N H N = + + U ( x ( ) 3. Find potentials U(x, y) with the second integral of motion and such that ΔU(x, y) = 0 N, y N ) 31

Nonlinear integrable lens H px + py x + y = + + U( x, y) This potential has two adjustable parameters: t strength and c location of singularities Multipole expansion : t 4 8 6 16 8 For z < c U( x, y) Im ( ) ( ) ( ) ( )... x+ iy + x+ iy + x+ iy + x+ iy + 4 6 c 3c 15c 35c For c = 1 t < 0.5 to provide linear stability for small amplitudes For t > 0 adds focusing in x Small-amplitude tune s: ν ν 1 = = 1+ t 1 t 3

Transverse forces Focusing in x Defocusing in y 300 00 Fx 50 40 30 Fy 100 0 10 0-1 -0.8-0.6-0.4-0. 0 0. 0.4 0.6 0.8 1-100 -00 x 0 - -1.5-1 -0.5 0 0.5 1 1.5-10 -0-30 y -40-300 -50 33

Nonlinear Magnet Practical design approximate continuously-varying potential with constant cross-section short magnets Quadrupole component of nonlinear field c 14 Distance to pole c Magnet cross section V.Kashikhin 8 34

-m long magnet 35

Examples of trajectories 36

Ideal nonlinear lens A single -m long nonlinear lens creates a tune spread of ~0.5. 1.0 FMA, fractional tunes Large amplitudes ν y 0.5 Small amplitudes (0.91, 0.59) 0.5 1.0 ν x 37

Experimental goals with nonlinear lenses Overall goal is to demonstrate the possibility of implementing nonlinear integrable optics in a realistic accelerator design Demonstrate a large tune shift of ~1 (with 4 lenses) without degradation of dynamic aperture minimum 0.5 Quantify effects of a non-ideal lens Develop a practical lens design. 38

Summary We have found first (practical) examples of completely integrable non-linear optics. We have explored these ideas with modeling and tracking simulations. The Integrable Optics Test Accelerator (IOTA) ring is now under construction. Completion expected in 014. Poster:TUPPC090 Beam Physics of Integrable Optics Test Accelerator at Fermilab The ring can also accommodate other Advanced Accelerator R&D experiments and/or users Current design accommodates Optical Stochastic Cooling 39