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Linear Collider Luminosity R. Brinkmann, DESY LC Workshop Chicago, - PowerPoint PPT Presentation

Linear Collider Luminosity R. Brinkmann, DESY LC Workshop Chicago, Jan. 7-9, 02 Acknowledgement Most of what will be presented here is work done by other colleagues in the different LC design groups worldwide. I am grateful for numerous


  1. Linear Collider Luminosity R. Brinkmann, DESY LC Workshop Chicago, Jan. 7-9, 02

  2. Acknowledgement • Most of what will be presented here is work done by other colleagues in the different LC design groups worldwide. I am grateful for numerous fruitful discussions and exchange of information and ideas over the past years. • This is a brief summary of some aspects regarding luminosity for both “warm” and “cold” LC’s. A much more comprehensive performance comparison is presently worked out by the International Linear Collider Technical Review Committee (“Greg Loew Committee”).

  3. � �� � � � Basic limitations and scaling • Beam power – determined by reasonable max. wall plug power P W and transfer efficiency η η η η AC � beam • Beamstrahlung – energy loss δ δ δ B and background at δ IP • Beam emittance – need to generate and preserve ! [ ] 2 N 1 N 1 = ⋅ = ⋅ ⋅ e e L f f n N E πσ σ π σ σ coll rep b e cm 4 4 E x y cm x y 1 / 2 σ ∝ ⋅ η ⋅ ⋅ ⋅ δ ε z / P H � → β W AC beam D B � *

  4. Luminosity challenge: it’s only 4 orders of magnitude from the SLC… SLC X-band / TESLA 500 ( → ~1000) Energy E cm 100 GeV Beam Power 0.04 6.6 / 11 MW Spot size at IP 500 (~50 FFTB) 2.7 / 5 nm Beamstrahlung 0.03 4.7 / 3.2 % 10 34 cm -2 s -1 3 ⋅ 10 -4 Luminosity 2 / 3.4

  5. Efficiency: “warm vs. cold” TESLA NLC η wall plug � RF 46.8 % 29.8 % η RF � beam 63.0 % 33.5 % η wall plug (RF) � beam 29.5 % 10 % (15 MW) 19.7 MW P wallplug for cooling 95 MW 132 MW (+15) two-linac P wallplug 22MW 13.2 MW two-linac P beam total η wall plug � beam 23.3 % 10% (9)

  6. Beamstrahlung and lumi spectrum γ γ 2 2 N N δ ∝ ⋅ → ph (Flat beam, low E cph ) e e ( ) U ( E / E ) σ σ B σ + σ σ 1 c beam 2 2 x z x y z Small # γ ’s per e ± : <n γ γ > ≈ ≈ ≈ ≈ 1…2 ( ∝ ∝ ∝ N e / σ ∝ σ σ σ x ) γ γ TESLA500 NLC500 δ B [%] 3.2 4.7 1.6 1.2 <n γ > < ϒ > 0.06 0.11 L 99% [10 34 ] 2.3 (68%) 1.4 ( 65%) (ISR and σ E,beam not included)

  7. Lower limit on β y* : synchr. rad. in quads (Oide 1988) and bunch length Oide effect, E_beam=500 GeV "hourglass effect" 4.50E-09 1.1 sig_y(0) 4.00E-09 1 luminosity [a.u.] 3.50E-09 sig_y(eff.) sigma_y at IP 3.00E-09 0.9 2.50E-09 2.00E-09 0.8 1.50E-09 NLC TESLA 1.00E-09 0.7 NLC TESLA 5.00E-10 0.6 0.00E+00 0 0.5 1 1.5 2 2.5 1.00E-05 1.00E-04 1.00E-03 beta_y / sigma_z beta_y at IP

  8. Side remark: all LC’s have flat beams – round beams might be nice, too! Suppose we could get small hor. emittance ε ε ε ε x = ε ε y , but with ε ε • unchanged phase space density N e / ε ε ε ε x , i.e. low bunch charge → collide round beams with β β x = β β β β β y β • Better relation L vs. δ B (ideally factor 2 higher L at same δ B ) • Larger enhancement factor H D (round) ≈ ≈ ≈ H D2 (flat) ≈ • • Single bunch wakefields strongly reduced Main challenge: injection system (conventional damping ring doesn’t work) (other issues: very small bunch spacing, triplet at IP, …)

  9. Example round beams: CLIC 3TeV flat round 4 ⋅ 10 9 2 ⋅ 10 8 N e ∆ t b 0.667ns 0.033ns ε x,y 0.68 ⋅ 10 -6 m , 2 ⋅ 10 -8 m 2 ⋅ 10 -8 m β x,y 8m m , 0.15m m 0.6m m σ x,y 43nm , 1nm 2nm σ z 0.03m m 0.1m m 0.1, 5.2 4.7 D x,y δ B 31% 28% < ϒ > 8.3 2.5 H D 2.1 4.1 9.6 ⋅ 10 3 4 10 ⋅ 10 34 L ∆ε / ε single 100% (?) 2% bunch (scaled)

  10. Emittance preservation: main linac displaced accelerating structure head tail Ratio deflecting wakefield to accelerating field (d y =1mm structure-to-beam offset) 0.001 W T * Q b / 2g 0.0001 0.00001 0.000001 TESLA C-band X-band CLIC

  11. Scaling of W trans helps to understand differences in tolerances – insufficient to understand beam dynamics in detail! • Accurate alignment inside a cryostat is more difficult than outside • diagnostics equipment can have better resolution in high-freq. than in low-freq. Linac (BPM’s in small vs. large beam pipe) • Effects causing emittance growth which are not (or not strongly) related to linac frequency (RF kicks, initial beam energy spread) • High linac rep. rate helps to cope with mechanical vibrations (higher frequency – lower amplitude) • Limitations on making and preserving small emittance from subsystems other than main linac (e.g. beam delivery) • More subtle differences: � “banana” effect at IP

  12. Beam Break-up • Head-to-tail defocusing effect of W trans can lead to exponential growth of betatron oscillation amplitude (BBU instability) � apply BNS damping with correlated energy spread dE/E vs. z (autophasing condition cancels wakefield defocusing with chromatic focusing of quadrupole lattice) • Remaining emittance growth from free oscillation is due to uncorrelated dE/E, filamentation and non- perfect autophasing

  13. • TESLA is not in BBU regime – autophasing still helps to TESLA reduce sensitivity to orbit jitter: with expected ~0.5 σ pulse-to- pulse jitter → correlated emittance growth ∆ε / ε ~ 0.1% • NLC requires 0.6% correlated energy spread to avoid BBU

  14. Beam based alignment • BPM’s can’t be pre-aligned along a straight (or: smooth) line with sufficient accuracy � need beam based methods to reduce dispersive emittance growth from random orbit kicks (BPM-to-quad with “shunt” method, DF steering by varying quad strengths or beam energy, …) � effectively replace BPM offset error by BPM resolution • In strong wakefield regime, active alignment of accelerator structures is also required ( RF-BPM’s and micro-movers )

  15. Linac tolerances & emittance growth ∆ ∆ε ε / ε ε ∆ε ∆ ε / ε ε ∆ ∆ ε ε ε ε ∆ ∆ ε ε ε ε TESLA NLC 300 µ m 20 µ m RF structures 4% 4% 200 µ m 5 µ m Girders 20% 3% # of RF BPM’s p. - 10,000 linac # of micro- - 1,700 movers p. linac 10 µ m 0.3 µ m quad-BPM 4% 25% resolution # of 360 800 quads/BPM’s p. linac total ∆ε / ε (budget 28% (50%) 32% (75%) DR � IP)

  16. “Plan B”: wakefield and dispersion correction with steering bumps TESLA NLC Filamentation ~10% full # of ε -diagnostic stations 1 (+ lumi) 7 (+lumi) reduce static emittance < 2% < 10% growth to Simulation of wakefield bumps in TESLA

  17. Multi-bunch effects Avoid HOM-driven BBU by detuning and damping � beam stability OK with tolerances specified by single bunch effects transverse long range wake 1.00E+02 W_T / V/(pC*m^2) 1.00E+01 1.00E+00 1.00E-01 1.00E-02 1.00E-03 1.00E+01 1.00E+02 1.00E+03 1.00E+04 1.00E+05 time / ns TESLA NLC y-scale factor 10 3

  18. Static part of HOM driven orbit pattern can be removed with fast correctors 14 TESLA: just program 12 10 Offset [um] feed-forward table of 8 6 3MHz bandwidth intra- 4 No initial bunch offset train feedback system… 2 Initial bunch offset = 18 um 0 0 100 200 300 400 500 Bunch number NLC: several stations Orbit motion in TESLA very small compared to cavity alignment (filamentation!) with fast errors � HOM pattern is static kickers (few 100Mhz) required

  19. Ground motion • Model for TESLA derived from HERA ground and orbit motion data • rms amplitude ~70nm for f>1Hz, essentially uncorrelated • Large amplitude for f<0.3Hz not critical because of large wavelength & strong correlation

  20. 6.3 km HERA ring in Hamburg Waste processing & power plant

  21. SLAC linac tunnel and SLD hall data absolute • Correlation vs. frequency Diff., spacing similar as at HERA, but 100m amplitudes smaller by factor 10…50 • Amplitudes increase in SLD hall by factor ~5 due to infrastructure (cooling, ventilation)

  22. Slow diffusive motion ∆ ≈ ⋅ ⋅ 2 ( y ) A T L • HERA model, from orbit • SLAC model from linac drift data (minutes to tunnel and FFTB weeks): measurements: − − − − = ⋅ µ ⋅ = ⋅ µ ⋅ 6 2 1 7 2 1 A 4 10 m ( m s ) A 5 10 m ( m s )

  23. Linac quadrupole position errors from ground motion (SLAC and HERA models) TESLA NLC HERA SLAC tolerance HERA SLAC tolerance quad jitter 10Hz (not relevant) 8nm 0.5nm 10nm quad jitter 1Hz 70nm 2nm 200nm 70nm 2nm ~few 10nm quad alignment 1h -1 1.2 µ m 0.4 µ m 10 µ m 0.6 µ m 0.2 µ m 2 µ m orbit feedback intra-train at end of linac + pulse-to-pulse, 5 – 10 sections pulse-to-pulse Note: temperature drifts, time varying stray fields, etc. may not be negligible!

  24. Beam Delivery and Final Focus TESLA BDS TESLA NLC σ x,y at IP 553nm, 5nm 245nm, 2.7nm β x,y at IP 15mm, 0.4mm 8mm, 0.1mm type of FFS FFTB-like Raimondi bunch spacing 337ns 1.4ns correlated σ E /E 0.05% 0.3% uncorrelated σ E /E 0.15% (e-), 0.05% (e+) 0.05%

  25. Luminosity Stability “Jitter”: steering at IP “Drift”: spot size at IP Ground motion 10Hz: SLAC model NLC FFS SLD “On” tolerances HERA model HERA 1Hz

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