Accelerator Vacuum Technology Challenges for Next-Generation Synchrotron-Light Sources

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Accelerator Vacuum Technology Challenges for Next-Generation P. He (IHEP) 14-19 May 2017, IPAC 2017, Copenhagen, Denmark 14-19 May 2017, IPAC 2017, Copenhagen, Denmark

Content 1. Introduction: Goals and Performance of Ring-Based LSs (Light Sources) 2. Future trends in DLSR (Diffraction Limited Storage Rings) 3. Associated Vacuum Issues and Special Hardware Development 4. Conclusions

Introduction Goals and the target performance of LS (Light Source) storage rings: Constant delivery of a high quality, intense and stable photon beam to a large number of beamlines High quality and intense photon beams: Often characterized in terms of Brilliance Photons I 0.1% x y 2 2 Second mrad mm BW I : Beam current, u : Transverse emittance Presently a big global wave for 3GLS DLSR (Diffraction Limited Storage Rings or 4GLS) Lowering of transverse beam emittance Optimal ring structure from DBA, TBA lattice MBA lattice

Ring-Based LS Future Trends A global wave today to construct (or reconstruct) ring-based LSs having the horizontal emittance H by tens of factors below the nm rad range HEPS

MBA (Multiple Bend Achromat) instead of DBA, TBA Comparison between ESRF and ESRF-EBS Especially for machine upgrades, the resultant ring configuration tends to be extremely dense APS APS_U, Spring_8 Spring_8 II, ESRF EBS Low emittance Strong focusing Smaller bore radii Narrower VC aperture Higher impedance (Resistive-Wall & Broadband) Lower vacuum conductivity Special vacuum technology (NEG, )

Challenges on vacuum systems for Low Emittance/DLSRs Main Purpose of DLSRs_Vacuum System Design: Have low dynamic pressure which gives good beam lifetime, and to handle the power deposited by SR. - High gradient quadruple Small magnet bore aperture Vacuum Chamber designs compatible with magnet poles, photon extraction and beam stay clear conditions(space limitation) - Handle the power deposited by SR Integration of pumping ports, photon absorbers, collimators and crotches(high SR power) - Small magnet bore aperture Low profile vacuum chamber(lumped pumping would not be as efficient in reducing the pressure) Detailed evaluation of vacuum profiles along the ring(conductance limitation) NEG coating must be a very helpful method for DLSRs to provide distributed pumping - Some specific hardware development in future DLSRs Zero-impedance flange, RF_shield Bellow, BPM etc - In-situ baking materials development thin Polyimide foil heater + Al coating polyimide foil

New LS s Parameters 14-19 May 2017, IPAC 2017, Copenhagen, Denmark

Vacuum Chamber Design(1) The clearance between the chambers and the magnets poles is 0.5~1.0 mm; the chambers are produced with tight mechanical tolerances to avoid any interference with the magnet poles and coils (for example, all tolerances of the chambers should be less than 0.3 mm). Ø22 mm Ø22 Aperture limiting sextupole MAX-IV Dipole Chamber Technologies applied: Wire erosion. TIG welding. E-beam welding Bending. Brazing. MAX-IV Sextupole Chamber with Key-Hole Technologies applied: Milling. Etching. Turning. NEG-coating Etc..

Vacuum Chamber Design(2) EBS chambers(low profile) are going to be installed in the central DQ (Dipole Quadrupole) magnets

Handle higher SR Power(1) Integration of pumping port and photon absorber Compact geometry with adequate cooling and minimized radiation scattering In-line absorber was used for shadow following BPM SIRIUS MAX-IV APS-U

Handle higher SR Power(2) Family Toothed (up to 110 W/mm 2 ) Family Frontal (up to 50 W/mm 2 ) EBS ABS CH5-1-1 Crotch 1 ABS CH9-1-29 ABS CH4-1-1 ABS CH13-1-13 12 lumped removable photon absorbers (on flanges) per cell These absorbers will be machined from a block CuCrZr, including the CF knife edge Single piece construction without brazing or welding.

Handle higher SR Power(3) Material Selection Glidcop AL-15 Vs Copper Chromium Zirconium (C18150)

Distribution Pumping_NEG coating(1) NEG coating, which turned out to be very effective in pumping the residual gases without pumping ports, is more and more used in ring-based LSs. MAX-IV MAX-IV and SIRRUS NEG coating for whole ring EBS and APS-U NEG coating for partial ring NEG coating issues Coating very small aperture even <10mm chambers Surface roughness Coating photon extraction key hole(~6mm gap) is challenging Fabrication methods compatibility with coating processes Coating development in industry. Very limited vendor capability-a possible risk NEG impedance might become a problem for very short bunches

NEG Coating Facility around the world ESRF (France) LNLS (Brazil) KEK (Japan) CERN (Swiss) GSI (Germany)

NEG Coating Procedure LNLS/SIRIUS

Coating Parameters Optimizations Daresbury/UK

NEG Coating/Double Layer Coating Daresbury/UK

NEG Coating Benefit for Other Components ESRF NEG coating R&D is continuing with the objective to explore if it is advantageous to coat the photon absorbers of the new machine.

NEG Coating Cons(impedance issue)

NEG Coating Cons(impedance issue) KEK_LS

Some Specific Hardware Development Impedance: More gentle transition, no gap between flanges, RF shielded bellows round chambers improve geometric impedance, smaller cross section SOLEIL in-vacuum ID tapers In-vacuum taper structure: Initial (above). Improved (below) - Initial tapers creating a cavity structure when the ID gap was opened had a serious problem of beaminduced heating. - New tapers greatly improved the heating issues.

Some Specific Hardware Development SIRIUS

Some Specific Hardware Development GlidCop or CrZrCu flanges KEK_B

Some Specific Hardware Development Simulations of narrow finger bellows: Inside fingers : K loss 1.9 x10-2 V/pC Outside fingers : K loss 2.1 x10-2 V/pC ± 2 mm offset 21.4 x10-2 V/pC ± 2 mm offset 8.7 x10-2 V/pC

Some Specific Hardware Development SuperKEK_B The comb-type RF shield has a structure of nested comb teeth, and has higher thermal strength and lower impedance than the conventional finger-type one. Advantages of the comb-type RF-shield are as follows: (1)The RF shield, i.e. the copper teeth, has a high thermal strength compared to thin fingers. (2)There is no transverse step at inside surface in principle, and the shield has low impedance. (3)The TE-mode like HOM, which can easily couple with the finger-type RF shield, hardly goes through due to the large radial thickness of teeth. (4)There is no sliding point on the inner surface of beam duct, which otherwise could be a source of arcing. (5) The RF shield can fit for beam ducts with various cross sections. The potential disadvantages compared to the finger-type RF shield, on the other hand, are the limited stroke of expansion/contraction, typically ±4 mm, and the small bending angle, ±30 mrad at most.

Some Specific Hardware Development EBS Omega Stripe RF shield CuBe to be gold plated SIRIUS

In-situ bake out/neg coating activation Minimum gap needed between chamber and magnet poles(0.5~1.0mm) Chamber heating methods, how to apply thin radiation resistant heat films Different configurations of heating element arrangement have been developed Thermal simulation is being carried out by means of FE module of Solid Works EBS 316L Sheathed heaters Test shaping insulation coats (aluminum coated PI)

In-situ bake out/neg coating activation SIRIUS

In-situ bake out/neg coating activation Temperature Rise Curve IHEP

Summary The vacuum system for the next-generation ring-based LSs has to cope with high synchrotron radiation, high photon flux, intense HOM excitation, strong collective effect, and so on. The low emittance lattice is making the vacuum chambers and components more and more miniature, both transversely and longitudinally, making their designs and vacuum pumping difficult with classical pumps. Vacuum pumping with NEG coating on the other hand is becoming increasingly attractive for the future machines. The use of NEG coated chambers must be considered right on the beginning of the design phase since it has a huge impact on infrastructure, fabrication strategy, cleaning procedures, baking strategy, etc. We have experienced various problems during the operation 3 rd generation LSs, and learned lots of things. These experiences should be some of help for the future design of next-generation LSs.

Thank you for your attention 14-19 May 2017, IPAC 2017, Copenhagen, Denmark