Compensation of Detector Solenoids

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Presentation transcript:

Compensation of Detector Solenoids G.H. Wei, V.S. Morozov, Fanglei Lin JLEIC Meeting, JLab, March 24, 2016 F. Lin

Contents Detector solenoids Effect Compensation Options JLEIC Considerations & a Solution Summary

Detector Solenoid Effect Coherent orbit distortion Transverse betatron coupling Dynamic effect Coupling resonances Rotates beam planes at the IP Breaks Horizontal and vertical dispersion free Perturbation on lattice tune & W function of the first order chromaticity compensation Spin effect Breaks figure 8 symmetry Crab crossing Complicates the design if crab cavities are installed in a coupled region

JLEIC and Detector Solenoids Length 4 m Strength < 3 T Crossing Angle 50 mrad

Vertical and horizontal orbit oscillations Detector Solenoid 1 T: Closed orbit V: ~170 mm, H: ~30 mm Detector Solenoid > 2 T: No closed orbit

Coupling of X and Y betatron motion Coupling beta ~ 5 % of nominal beta

Break of H & V dispersion-free Left: detector solenoid off Right: detector solenoid on

Perturbation on lattice tune & W function Detector solenoid status: Left: off; Right: on

V. Garczynsky, RHIC-Notes/AD-AP-37 Compensation Options Detector Solenoid + Drift + Anti-Solenoid (a RHIC design) Pro: dynamically is the best Con: there seems to be no space in the IR of JLEIC Detector Solenoid + + same-field-integral solenoid Cons: long locally coupled section, crab cavity issue, spin effect is not compensated Detector Solenoid + + Anti-Solenoid Cons: long locally coupled section, crab cavity issue V. Garczynsky, RHIC-Notes/AD-AP-37

V. Garczynsky, RHIC-Notes/AD-AP-38 Compensation Options Distributed skew quadrupole compensation Pro: less complicated optics than in options 2 & 3 Cons: long locally coupled section, crab cavity issue, spin effect is not compensated a RHIC design, PEP-II 3 ~ 6 skew quads on each side of IP V. Garczynsky, RHIC-Notes/AD-AP-38

Compensation Options Super KEKB & DAFNE Solenoid + tilt Quads + Anti-Solenoid Pros: coupling is localized, no crab cavity problem, spin effect is compensated Con: more complicated final focus design Super KEKB & DAFNE

JLEIC Considerations & a Solution Compensation constraints for both electron and ion rings Optics fixed and uncoupled at IP due to variety of solenoid fields and energies Coupling compensated locally and independently on each side of IP Optics fixed at the entrance into and exit from IR No coupling elements (for now) dispersive regions Cancel spin effect to keep figure 8 symmetry 12

JLEIC Considerations & a Solution A solution: Solenoid + Quads(normal+skew) + Anti-Solenoid Quads(normal+skew): a normal quad with an additional winding or a skew quad next to the normal quad 13

Coupling of X and Y betatron motion Coupling compensated locally and independently on each side of IP

Vertical and horizontal orbit oscillations Detector Solenoid 1 T: Closed orbit V: ~170 mm, H: ~30 mm Detector Solenoid > 2 T: No closed orbit

Restoration of H & V dispersion Left: before restoration Right: after restoration

Summary Detector solenoid gives effects of orbit distortion, transverse betatron coupling, Rotates beam planes at the IP, Breaks Horizontal and vertical dispersion free, Perturbation on lattice tune & W function of the first order chromaticity compensation, Spin effect to Break figure 8 symmetry. A solution of ‘Solenoid + Quads(normal+skew) + Anti-Solenoid’ is used to compensate detector solenoid effects. Results are acceptable. More study should be done on W function restoration.

Thank you F. Lin

Perturbation on lattice tune & W function Left: uncorrected; Right: corrected

Perturbation on beam size at IP Left: detector solenoid off Right: detector solenoid on

Perturbation on beam size at IP Left: detector solenoid off Right: detector solenoid on

Detector Solenoids in LHC Old LHC HL-LHC Length 5.3 m Strength 2 T Crossing Angle 285 rad 590 rad

Detector Solenoids in RHIC Length 6.2 m Strength 0.5 T Crossing Angle <1.7 mrad

Simulation setup & method Multipoles Normal: Systematic + Random Skew: Systematic + Random

Simulation setup & method Single Multipole: Normal Systematic Combined result: Normal Systematic Normal + Skew Systematic Single Multipole: Skew Systematic Combined result: Skew Systematic

Cases x/y Rref DA_sm DA_cm an,bn Non-liner drive to 6 FFQ 1 0.35/0.07 43 mm 20 10 not same 2 15  18 same 3 LHC/HI-LHC N/A 4 1.2/1.2 20 mm 5 12  6 8  ? 7 Physical Aperture / 3 ?

Discussion Multipole dependent on reference point, emittance, constraint in physical aperture Emittance and physics aperture should be confirmed before multipole study