1 / 37

Technological aspects of crab cavities

This article discusses the technological aspects of crab cavities and their impact on beam dynamics. Topics covered include RF phasing, cavity size and frequency, cavity fabrication, multipacting studies, and cavity coupling schemes.

glennae
Télécharger la présentation

Technological aspects of crab cavities

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Technological aspects of crab cavities CARE-HHH-Lumi-06, 16-20 Oct 06, Valencia, Spain J. Tückmantel, CERN Thanks to R. Calaga, F. Caspers, R. Tomas Garcia, F. Zimmermann, …

  2. Frequency and Cavity Size Panofsky- Wenzel: Need gradient of Vz! TE modes: E- and B-deflection cancel (integrated) Dpx = -ie/w  dVz/dx   exp(-iwz/v) (Vz and Dp in quadrature; z = lag) Longitudinal interaction not desired: beam passage should be at zero of Vz

  3. Crab cavity: RF phasing such that bunch centre gets zero kick ( -> beam and Vz in phase) BunchcentrelinesatIP: If not B.L. << lRF: lumi loss (transverse dimensions …) design and real kick for long bunches

  4. 4s-bunch length in coast: 30 cm 1 ns (present LHC) l800MHz = 37.5 cm (-> ±0.4): 800 MHz excluded for larger crossing angles Present LHC bunch spacing 25 ns -> 40 MHz Future bunch spacing under discussion • 12.5 ns -> 80 MHz (200 MHz incompatible) • 10/15 ns -> 100/66.6 MHz (200 MHz compatible) Next lower common denominator: 400 MHz (as main RF) If 400 MHz still too high: choice will exclude options

  5. Minimum cavity dimensions: estimate by box-cavity Lowest w field map: round cavities: need more space for same f

  6. For LHC IP4: beam-beam (centre) distance exceptionally spread to 42 cm (present design -> Rogelio) (required magnets already difficult for 7 TeV; 14 TeV ??) r400MHz,main = 345 mm fits next to opposite beam Oppos. beam in tube inside cryostat Accelerated beam 1/2 Lx ≤ 35 cm

  7. Up-down and right-left symmetric cavity of classical sc. design with horizontal kick at 400 MHz excluded (with IP4 config.) (only vertical kick while horizontal (macroscopic) beam separation) • Re-entrant shape (lowers f): was ‘forbidden’ for sc. cavities: bad rinsing conditions (liquid cannot flow out easily); exists proposal for ILC cavity version (‘slighty’ re-entrant): experts not unanimous: test series pending (danger: field emission limiting performance!) • Other ‘adventurous shapes’: Danger of multipacting (MP)

  8. ‘Adiabatic deformation’ to get room for opposing beam: • (upward) displaced beam tube - lower kick efficiency - kick depends already in 1st order on vertical position (2nd for up-down sym. structures) • Beam still passes at Vz = 0 3D RF structure simulations if acceptable: beam dynamics Multipacting studies, …

  9. Cavity fabrication • Standard: Niobium sheet metal -> spinning/deep drawing, welding, chemical treatment(s), rinsing, …, ‘witchcraft’ • Stiff cavities (vibration, vacuum forces on non-round cav.): Thicker material: Nb layer on (thick) copper is an option if specs can be met (e.g. by sputtering as for LEP2), + (OFHC) copper is a better thermal conductor than best Nb + no (earth-)magnetic shielding required (up to about 2 G) – steeper Q drop (… less adapted for very high fields)

  10. Sergio Calatroni (…, R&D for LEP2 sputtering, …): • Bpeak is at iris: maximum damage during cavity forming -> sc. layer on it ? • angle of incidence (while sputtering) is steeper: Nb film forms under less favorable conditions (‘columnar film’) R&D to validate technology and performance

  11. n-cell cavities • Higher real estate gradient (voltage/total length) • n times less couplers, tuners, controlers, …. • Each single-cell mode has n instances, each with different frequency, (R/Q), cell-to-cell-polarity, … - Crab cavity ‘HOM’ coupling scheme relies (partly) on frequency offset wrsp. to crab-mode: now (n-1) ‘close’ modes (with lower (R/Q) …); use power-coupler as damper ? - if vector feedback necessary for impedance reduction, ‘filter box’ is required (possibly with amplifiers -> maybe more noise)

  12. Reference pick-up not on same cell as power coupler: direct cross-talk For well adjusted π-mode, 0-mode would auto-oscillate !! ‘filter’ has to turn 0-mode signal by 180º without perturbing π-mode signal (4-cell LEP2 cavities in SPS as injector: cable nl at fπ, (n–1/2)l at f 3π/4) …. phase noise (amplifiers) ? RF (power) system should cover whole pass-band !!

  13. N cavities with one transmitter One mother with N children: while looking for one, the other N-1 do what they want …. N degrees of freedom with 1 knob -> add knobs (at a price) Possibility: • Ferrite phase and amplitude modulators (as tested at CERN for SPL at 352 MHz) • Serrodyne (ferrite) phase shifter ( <- F. Caspers), www: 8-140 GHz commercially available ??? 400 MHz ???

  14. Ferrite amplitude and Phase Modulators with hybrids Cav. reflection not completely absorbed, more complex in application Cav. reflection absorbed

  15. One problem: precision of vector sum calibration (esp. ampliude) ‘fast delta’: transmitter; ‘slow delta’: device ‘X’

  16. CW mode (problem much ‘older’ than ‘pulsed sc. Cavity problem’, both related)

  17. N cavities of n cells with one transmitter LEP2: 8 cavities of 4 cells on one transmitter Basically each cavity had a ‘scalar’ amplitude measurement; assuming cavities in phase: (digital) sum was used for control. ‘Once there was a time’ when a vector sum feedback was tried: relatively low gain, ‘a pain to set up’, and caused frequent trips: operational people were happy when switched off again. Combination of ‘problems’ • each cavity needs a ‘filter box’ -> unique ‘reference signal’ • vector sum calibrated for crab-mode, not very good for others: rely on low (R/Q) of other pass-band modes.

  18. ‘H’OM damping The Problem: • Keep ‘workhorse mode’ field inside cavity • Get the other fields out of the cavity (strong damping) Mode distinction: • By frequency • By field configuration Two methods: • Lumped circuit Coupler with filter, …. -> line outside cryostat -> dump power outside (LHC sc. main RF) • Transport away from cold area -> dump inside cryostat (cooling)

  19. KEK/Cornell cavity uses symmetrized (no crab-mode pick-up) coaxial coupler -> some MP problems • option: resonant (enhances coupling) lumped circuit coupler in coupling port (as LHC main RF ‘dipole mode coupler’) • first distinction on E-minimum (antenna) or B-minimum (loop) of crab-mode, but always couples to TM0 modes (as coaxial) (coupler with filter (!) has to be superconducting !) R&D necessary (CERN’s main expert Ernst Haebel retired)

  20. Transient beam loading: beam in phase with crab-field: ‘no’ phase error induced, only amplitude error Both systems give kick in same direction (same polarity) !!! Off axis beam: one system increases, one decreases field: amplitude difference error induced

  21. RF power / Qext considerations Longitudinal Vz and beam are in phase: strong interaction Ideally beam passes at Vz zero-crossing -> no RF power In reality: LHC orbit can be / is displaced -> -> ‘static’ adaptation by physically moving the cavity/cryostat (remote controlled set-up with low intensity beam, dumped) -> keep a ‘dynamic’ range for ‘online’ orbit changes • the crab RF system has to deliver / absorb power; • the main RF has to absorb / deliver complement (DE=0 in coast)

  22. 2-cell cavity with 5 MV nominal kick (-> Rama’s design) model current (tuned cav.) measurable RF power Optimum Qext (i.e. Ir=0) Minimum installed power: Maximum beam excursion: (for optimum Qext !)

  23. A 500 W solid-state amplifier per cavity (Ib,ult=1A) would • allow up to ±12 µm ‘excursion’ • at a Qext,opt=5·108 -> BW < 1 Hz (untunable) For a ‘reasonable’ Qext=1·106 (BW =400 Hz) • to keep the field up for a perfectly centered beam Pg 100…150 kW/cav. tetrode Pr klystron (noisy) displacement [m]

  24. Kick errors (‘additive’) Perfect case: bunch centre and bunch line on axis (after crab 2) Always respected: Keep beam 1 and beam 2 RF wise separate: no common high power equipment

  25. Optic transfer function not π between 2 crab system: Bunch centre on axis, bunch line oscillates Mutual amplitude deviation between 2 crab system: Bunch centre on axis, bunch line oscillates (absolute amplitude error: non-zero crossing angle)

  26. Common phase shift of two crab systems (shifted tilt point): Bunch centre off-axis at IP, perfect again after crab 2 Independent phase shifts of two crab systems: Bunch centre off-axis at IP and later

  27. Noise table (F. Zimmermann, Arcidosso  Ohmi-san) RF is ‘blind’ concerning mechanical displacements by Dz as vibrations, drifts F. Caspers (… , stochastic cooling, … ): “ …. to measure 0.03 ps might be possible at the limit of today’s technology, but 0.002 ps (@400 MHz) is out of range” Josef Frisch, SLAC: 0.003º@357MHz (0.025 ps) was done … To control means to measure at least with the same quality (provided ‘actuator’ does not inject new noise)

  28. Questions by F. Caspers • What are phase noise properties of power amplifier (caution AMPM  conversion!!) systems typically used to drive such cavities. CW amplitude foreseen; beam-loading transients to be ‘recovered’ by transmitter ? • To what precision can it be measured ? (0.025 ps possible, which technical reliability ?, need 10x • To which precision can it be controlled ? ???? • Which technology to be used (klystrons , solid state?)

  29. Questions by F. Caspers (cntd.) • Where is the limit between jitter and drift? is betatron frequency decisive ? Coherence-length ? how stable is b-freq in practice ? Spectrum ? • How about the (blow-up) impact of amplitude noise (AM/PM conversion). • What are the phase noise properties of the beam itself ? (e.g. from power supply ripple, parametrically excited modulation etc etc..) phase different from bunch to bunch “is planned” (and unavoidable in any case): each bunch pairing is different !!

  30. Proposal F. Caspers, similar J. Frisch, SLAC (ILC) ???? Does this really help or not ????

  31. Problems with this proposal: • How to build a RF vector-feedback (impedance !) around? (slow changes ( kHz) can be handled by individual amp&phase modulators for each cavity, but not coupled bunch) • For each ‘pair’ a bulky HIGH POWER LINE has to run along the tunnel between Crab 1 and Crab 2 • Ideally klystrons at IP (where ?), else asymmetric design

  32. Bunch to bunch positions are fixed but not ‘regular’ in coast • Beam and RF are in quadrature: each bunch ‘turns’ RF vector • For ‘regular beam’: detune cavity such that it drifts back automatically till next bunch (react. beam loading compensation) • Beam with gaps: ‘half detuning’ to make the best out of it: RF has to fight keeping bunches in regular position (and only partly succeeds due to limited loop gain) In coast at full voltage: RF system comes to limits -> let bunches drift (<< B.L.) on ‘easier’ positions (status depends on individual bunch charges, ….)

  33. RF power Already after injection (1 MV/cavity) bunches have ‘individualized’ z-position (due to technical limitation of RF vector feedback)

  34. End injection, V = 1MV/cav Adapted on flat bottom Half ramp, V rising flat top reached, V=2 MV/cav The ‘bunch sliding’ during 7 TeV-ramp up to coast. Possibly redone during coast (if beam changes conditions) Adapted for coast

  35. RF power Bunches ‘slide’ to ‘individual’ z-position not to overload RF system in coast (2 MV/cavity)

  36. Summary • At 400 MHz horizontal kick with present horizontal beam-beam distance not possible         -> need different cavity shapes or more beam-line separation (-> Rogelio) • Nb/Cu technology might be an option: need R&D to verify film quality for this shape • n-cell (low n !!) cavities and N cavities per transmitter possible (space, $$$), but more complex installation with probably higher noise • Limited beam excursions in LHC cannot be exploited for low power consumption:         system BW too low -> Qext 106 -> 100-150 kW / 2-cell cavity (wasted) • Role of different type of noise (amplitude, phase; does coherence between both crab systems help) has to be analyzed in more detail to find best technical options • Is the fact that each bunch has its ‘private phase’ a real problem or only a nuisance ? • The announced required noise level is about 10 below present technology. This is no reason for despair, but caution should be kept when extrapolating technology:

  37. One should not overrate technical advancement potentials: Reliability is cornerstone for integrated luminosity in LHC

More Related