1 Dynamic aperture of non-scaling FFAG with sextupole Shinji Machida CCLRC/RAL/ASTeC 21 July, 2006 ffag/machida_20060721.ppt.

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Presentation transcript:

1 Dynamic aperture of non-scaling FFAG with sextupole Shinji Machida CCLRC/RAL/ASTeC 21 July, ffag/machida_ ppt & pdf

2 Non-scaling FFAG with sextupole new optics by Scott Berg Berg made a new optics which does not cross 3rd order resonance. See if this new optics has any improvements in dynamic aperture. Different colors show different setting of chromaticity correction: 0, 5, 10, …, 50%. 10 GeV 20 GeV

3 Non-scaling FFAG with sextupole Berg’s optics vs. S-code modeling Tune diagram Time of flight (0, 20, 30, 40, 50% only)

4 Non-scaling FFAG with sextupole dynamic aperture With more than 40% of sextupole, dynamic aperture becomes less than 30 pi mm. 50% 40% 30% 20% dynamic aperture [pi m]

5 Non-scaling FFAG with sextupole with constant energy gain 30 pi mm 0 pi mm 30 pi mm 0 pi mm 19 pi mm 11 pi mm 0 %20 %30 % 50 %40 % Time of flight variation can be corrected with chromaticity correction. (constant energy gain) ?

6 Non-scaling FFAG with sextupole accelerate out of bucket 50 %40 % 0 %20 %30 % 30 pi mm 0 pi mm 30 pi mm 0 pi mm 24 pi mm 0 pi mm 11 pi mm Time of flight variation can be corrected with chromaticity correction. (acceleration out of bucket) ?

7 Non-scaling FFAG with sextupole with constant energy gain 0 % 20 % Initially x!=0, y!=0 Initially x!=0, y=0 Initially x=0, y!=0 Slight reduction of phase slip with 20% sextupole except when both x and y are not zero initially.

8 Non-scaling FFAG with sextupole with constant energy gain 0 % 20 % Horizontal phase space of 30 pi mm Vertical phase space of 30 pi mm Larger phase slip of 20% sextupole is caused by transverse emittance growth.

9 Summary Problem of path length variation with finite transverse amplitude can be corrected with sextupole. However, with more sextupole strength, dynamic aperture becomes less. Need to find compromise between them. Dynamic aperture is suffered also locally with resonances. For example, a dip on dynamic aperture may be due to nx=0.25 and ny=0.25.

10 Non-scaling FFAG with sextupole (previous) tune excursion Sextupole strength: Red 0% Green 10% Blue 25% Magenta50% Both SF and SD sextupoles are installed at QF and QD*. Strength are relative to the one required for full chromaticity correction in a SAD (MAD) model. *Although SF is more effective than SD as pointed out by Koscielniak(tridn pdf), SF only makes vertical tune unstable at high momentum. 10 GeV 20 GeV

11 Non-scaling FFAG with sextupole (previous) dynamic aperture at injection Sudden decrease of dynamic aperture with sextupole. Gradual increase with stronger sextupole.

12 Non-scaling FFAG with sextupole (previous) time of flight variation sext=0% sext=50% 24 pi mm 0 pi mm Path length variation is reduced with (Hor. ) chromaticity correction. sext=0% 24 pi mm 0 pi mm sext=50% 24 pi mm 0 pi mm with constant energy gain Accelerate outside of bucket