1 Thursday Week 1 Lecture Jeff Eldred Nonlinear

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1 Thursday Week 1 Lecture Jeff Eldred Nonlinear Sextupole Resonance

1 Thursday Week 1 Lecture Jeff Eldred Nonlinear Sextupole Resonance

2 Overview Nonlinear Sextupole Resonance: 1. Linear Betatron motion in Action-Angle 2. CT to

2 Overview Nonlinear Sextupole Resonance: 1. Linear Betatron motion in Action-Angle 2. CT to orbital angle frame 3. Addition of sextupole perturbation 4. Fourier analysis of sextupole perturbation 5. CT to resonance-rotating frame 6. Motion of sextupole-driven nonlinear beam 7. Application to slow extraction

3 Action-Angle to Orbital Angle Frame

3 Action-Angle to Orbital Angle Frame

4 Linear Action-Angle Coordinates Shown in Gregg’s “Lecture 8” yesterday:

4 Linear Action-Angle Coordinates Shown in Gregg’s “Lecture 8” yesterday:

5 CT to Orbital-Angle Coordinate

5 CT to Orbital-Angle Coordinate

6 What is the Orbital-Angle Coord. ?

6 What is the Orbital-Angle Coord. ?

7 Nonlinear Sextupole Resoance

7 Nonlinear Sextupole Resoance

8 Sextupole Perturbation We add a term corresponding to a sextupole: We transform to

8 Sextupole Perturbation We add a term corresponding to a sextupole: We transform to the Action-Angle Orbital-Angle Frame:

9 3 rd-Order Nonlinear Resonance Near a 3 nu = l resonance we can

9 3 rd-Order Nonlinear Resonance Near a 3 nu = l resonance we can focus on: Integrating over s we obtain the Fourier coefficient:

10 Fourier coefficient Evaluated only at sextupoles, which may add up constructively or destructively.

10 Fourier coefficient Evaluated only at sextupoles, which may add up constructively or destructively. Super-periodicity of accelerator rings cause the resonances to cancel out naturally. Families of sextupoles are also used to change chromaticity without driving resonances. Credit: USPAS Wolski & Newton

11 Nonlinear Motion

11 Nonlinear Motion

12 Resonance-Rotating Frame With a given Fourier coefficient:

12 Resonance-Rotating Frame With a given Fourier coefficient:

13 Nonlinear Equations of Motion

13 Nonlinear Equations of Motion

14 Nonlinear Motion

14 Nonlinear Motion

15 Nonlinear Motion

15 Nonlinear Motion

16 Nonlinear Motion X, P x, x’

16 Nonlinear Motion X, P x, x’

17 3 rd-Order Resonance Slow-Extraction

17 3 rd-Order Resonance Slow-Extraction

18 Slow Extraction All diagrams taken from Marco Pullia thesis Chapter 3. Adiabatically increasing

18 Slow Extraction All diagrams taken from Marco Pullia thesis Chapter 3. Adiabatically increasing the sextupole strength deforms the linear circular trajectory into a triangular trajectory surrounded by the separatrix.

19 Two Septa to Extraction Line The ES is thin and delivers a kick

19 Two Septa to Extraction Line The ES is thin and delivers a kick to provide a large enough gap that the MS can fully extract. The phase advance between the two septa determines the rotation of the separatrix.

20 Steinbach Diagrams Steinbach diagrams are useful for determining the uniformity of the spill

20 Steinbach Diagrams Steinbach diagrams are useful for determining the uniformity of the spill and the momentum spread of the spill. Chromaticity relates the particle momenta to the tune.

21 Method 1: Move the Tune

21 Method 1: Move the Tune

22 Method 2: Move the Beam

22 Method 2: Move the Beam

23 Method 3: Excite the Beam Operation experience shows this is the method that

23 Method 3: Excite the Beam Operation experience shows this is the method that provides the most fine-control of the spill uniformity. Method 4: Change the Sextupoles This method is not recommended, because the spill is very non-uniform and not all particles may be removed.

24 Hardt Condition The line of unstable particle trajectories should coincide for particles of

24 Hardt Condition The line of unstable particle trajectories should coincide for particles of different momenta. Hardt Condition relates dispersion, phase-advance, chromaticity, and sextupole strength.

25 Septa Locations The Hardt condition, the rotation of the separatrix, and the aperture

25 Septa Locations The Hardt condition, the rotation of the separatrix, and the aperture constraints determine the septa locations.