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U. Wienands, SLAC UA9 Workshop, 27-Oct-10 1 FACET: A Facility for Advanced Accelerator Research at SLAC U. Wienands, SLAC at CERN until 12-Nov. on a LARP-sponsored.

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Presentation on theme: "U. Wienands, SLAC UA9 Workshop, 27-Oct-10 1 FACET: A Facility for Advanced Accelerator Research at SLAC U. Wienands, SLAC at CERN until 12-Nov. on a LARP-sponsored."— Presentation transcript:

1 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 1 FACET: A Facility for Advanced Accelerator Research at SLAC U. Wienands, SLAC at CERN until 12-Nov. on a LARP-sponsored Long Term Visit Division Head for FACET Linac I am indebted to Mark Hogan for providing material on plasma acceleration

2 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 2 Overall Thrust of FACET The primary goal of FACET is proof in principle that plasma acceleration can accelerate a bunchThe primary goal of FACET is proof in principle that plasma acceleration can accelerate a bunch –characterize the mechanism under beam loading –estimate beam parameters (witness) –estimate the efficiency and gradient reachable in practice –demonstrate acceleration of a positron bunch Beyond that, FACET will provide a facility to explore other accelerator physics issuesBeyond that, FACET will provide a facility to explore other accelerator physics issues –Wakefield measurements (ILC, CLIC) –Matter in extreme fields –new radiation sources using crystals

3 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 3 The FACET Facility Driven by first 2/3 rd of the SLAC 2-mile linacDriven by first 2/3 rd of the SLAC 2-mile linac –new exp. area in Sec. 19-20. –new compressor chicane in Sec. 10 for e + –new compressor chicanes in Sec. 19. –e – and slightly later also e +

4 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 4 Energy 23 GeV Charge 3 nC Sigma z 14 µm Sigma r 10 µm Peak Current 22 kAmps Species e - & e + The FACET Facility Beam Parameters:Beam Parameters: –many of these can be tuned to match requirements –30 Hz repetition rate

5 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 5 Staged Bunch Compression

6 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 6 S10 Compressor Chicane

7 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 7 “Sailboat” Chicane (S20) 3rd-stage bunch compression3rd-stage bunch compression precision timing e + and e – bunches wrt. each otherprecision timing e + and e – bunches wrt. each other –allow e + bunch to sample wake from e – bunch

8 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 8

9 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 9

10 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 10 Linac Removed from FACET Expt. Area

11 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 11 Some of the Beam Diagnostics FACET IP SLAC linac: BPM’s, Toroids, Feedbacks, GADCs, triggers SLAC linac: BPM’s, Toroids, Feedbacks, GADCs, triggers

12 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 12 FACET Status Construction expected to finish early Summer 2011Construction expected to finish early Summer 2011 –accelerator and beam commissioning soon after. Experimental program to begin early Fall 2011Experimental program to begin early Fall 2011 First Users Workshop @ SLAC March 18-19, 2010First Users Workshop @ SLAC March 18-19, 2010 –http://www-conf.slac.stanford.edu/facetusers/spring2010/http://www-conf.slac.stanford.edu/facetusers/spring2010/ –40 people, 9 institutions Argonne, Brookhaven, Euclid Techlabs, Fermilab, SLAC, Stanford, UCLA, USC, UT Austin –4 Working groups considered ideas for first experiments: Plasma Wakefield Acceleration Dielectric Wakefield Acceleration Materials in Extreme Conditions Crystals & Novel Sources of Radiation Beamtime allocated in a proposal driven processBeamtime allocated in a proposal driven process

13 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 13 PWFA: Particle to Beam Acceleration Witness Bunch Drive Bunch x ∝ Δ E/E ∝ t Disperse the beam in energy Adjust final compression...selectively collimate x [mm] dp/p [%] z [mm] 80cm Plasma Collimation system to craft drive/witness bunch from single bunch (similar to BNL ATF wire system)Collimation system to craft drive/witness bunch from single bunch (similar to BNL ATF wire system)  Vary charge ratio, bunch lengths, spacing by changing collimators and linac phase, R56  Study wake loading in the non-linear regime for the first time

14 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 14 Beam Loading & Wake Evolution QuickPIC simulation, D:  z =30µm, N=3x10 10 e -, W:  z =10µm, N=1x10 10 e -,  r0 =3µm, ∆z=115µm, n e =10 17 cm -3 Energy [GeV] Propagation Distance [cm] Beam loading at 37GeV/m (z = 0)Beam loading at 37GeV/m (z = 0) After 80 cm plasma, gain 25 GeV with 3%  E/EAfter 80 cm plasma, gain 25 GeV with 3%  E/E Wake evolution due to bunch head erosion, but no dephasingWake evolution due to bunch head erosion, but no dephasing Wake evolution “bends” energy gain but preserves low ∆E/EWake evolution “bends” energy gain but preserves low ∆E/E Drive to witness Energy transfer efficiency ~ 30%Drive to witness Energy transfer efficiency ~ 30%

15 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 15 PWFA Collider Concept for a beam-driven PWFA collider (1TeV)Concept for a beam-driven PWFA collider (1TeV) –R&D: e +, emittance, efficiency

16 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 16 FACET Beam is Well Suited for Studying DWA A ‘‘drive’’ beam excites wake-fields in the tube, while a subsequent witness beam (not shown) would be accelerated by the Ez component of the reflected wakefields (bands of color). For large wakes want high charge, short bunches and narrow tubes, e.g. 2E10 e-, σ z =20µm, Si with 200µm ID get 85GV/m surface fields! For large wakes want high charge, short bunches and narrow tubes, e.g. 2E10 e-, σ z =20µm, Si with 200µm ID get 85GV/m surface fields!

17 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 17

18 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 18 Other Proposed Research Ultrafast processes in magnetic solids.Ultrafast processes in magnetic solids. Wakefield measurements of CLIC structuresWakefield measurements of CLIC structures Optical diffraction radiation testsOptical diffraction radiation tests Time profile of 50 fs bunchesTime profile of 50 fs bunches Test of advanced Feedback Algorithms (CLIC).Test of advanced Feedback Algorithms (CLIC). These are submitted proposals or LOIs

19 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 19

20 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 20 Other Research Considered Crystal Accelerator:Crystal Accelerator: –idea has been around for a while, inverse FEL process –at FACET could be done with high-energy photons Crystal collimation and X-ray generationCrystal collimation and X-ray generation –use the strong bending in channeling to make Xrays –some work at other facilities (mostly e – ) –at FACET can use e +, higher energies & non-negligible intensities Beam collimation studiesBeam collimation studies Bragg diagnostics.Bragg diagnostics. High-gradient structure tests.High-gradient structure tests.

21 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 21 Crystal Channeling @ FACET Study of volume reflection of e + and e –Study of volume reflection of e + and e – –test continuum model of VR for light particles –study effect of multiple scattering on vr –possible application for halo cleaning in lin. colliders Physics of volume-reflection radiation by e + & e –Physics of volume-reflection radiation by e + & e – –test radiation models for channeled light particles in region of undulator parameter K = E/m*  ≈ 1. –possible application as new photon source Noble, Ng, Stupakov, Seryi et al.

22 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 22 VR Simulation for FACET Noble et al., CERN, 2009 But FACET can make divergence < 1 µr at ≈ 100 µm

23 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 23 Carrigan, Channeling 2008

24 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 24 X-ray Generation Bolognini, Thesis 180 GeV e – and e +

25 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 25 Undulator Radiation possible?

26 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 26 Crystal Accelerator Idea: intense Xrays (40 keV, 10 9 W) shone on crystal at Bragg angle setup accelerating fieldIdea: intense Xrays (40 keV, 10 9 W) shone on crystal at Bragg angle setup accelerating field –channeled µ + see accelerating field of GV/m –(Tajima & Cavenago 1987)

27 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 27 Summary FACET will be a unique facility to advance the high-gradient acceleration research with plasmas and dielectricaFACET will be a unique facility to advance the high-gradient acceleration research with plasmas and dielectrica Beyond this, FACET will allow a number of advanced experiments in solid-state physics and the study of particle interaction with matter.Beyond this, FACET will allow a number of advanced experiments in solid-state physics and the study of particle interaction with matter. An open, proposal-driven process of experiment approval will allow equitable access to the facility to fore-front experimentsAn open, proposal-driven process of experiment approval will allow equitable access to the facility to fore-front experiments

28 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 28 Apply Now!

29 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 29 Backup Slides

30 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 30 1 GeV 1.5 TeV

31 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 31

32 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 32 Outline The FACET ProjectThe FACET Project The Experimental ProgramThe Experimental Program ConclusionConclusion

33 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 33 Accelerator Evolution Primary tools to advance HEPPrimary tools to advance HEP Reaching limits of supportReaching limits of support –size, costs, time scales –Internationalization can buy time, but only a little Advance can come from fundamental research into new accelerating mechanismsAdvance can come from fundamental research into new accelerating mechanisms –Different materials –Higher frequencies –…

34 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 34 High Gradient Acceleration The fundamental parameter is the accelerating gradientThe fundamental parameter is the accelerating gradient –reduce size, thus costs, of new facilities –may help in increasing beam brightness as well Candidate technologies for high gradients:Candidate technologies for high gradients: –High-frequency metallic structures (=> CLIC) –Dielectric structures (beam or laser driven) –Plasma wakefields FACET aims at plasma and dielectric accelerationFACET aims at plasma and dielectric acceleration O(100) MV/m O(1) GV/m O(10) GV/m

35 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 35 World-wide interest in Plasma- Wakefield Acceleration T. Katsouleas

36 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 36 Checking out the Linac…

37 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 37

38 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 38 9 mm Si Crystal, 400 GeV p Rotation angle (µrad ) Angular profile (µrad) de- channel volume capture Channeling Volume Reflection

39 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 39 Crystal Collimation p Beam propagation Primary halo (p) Absorber  Coherent deviation of the primary halo  Very small probability of inelastic interaction in the crystal  Larger collimation efficiency  Less impedance  Reduced tertiary halo Crystal Beam Core E. Tsyganov & A. Taratin (1991)  = O(100µrad) l = O(10 -2 m)

40 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 40 Motivation Accelerators for HEP are reaching a limit in size and cost.Accelerators for HEP are reaching a limit in size and cost. –Time to approval is becoming too long –Power consumption is becoming a limit –The destructive power in the beams is enormous How are we dealing with this situation?How are we dealing with this situation? –internationalizing: good, but not enough –“Value Engineering”: necessary, but not enough –Push technology (higher frequency, gradient): better –…but really need a breakthrough…

41 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 41 Primary Challenges for Accelerator R&D Primary Challenges for Accelerator R&D Beam PowerBeam Power –directly relates to (average) luminosity & energy –MW scale, technical and physical limitations Beam brightness (intensity/phase-space volume)Beam brightness (intensity/phase-space volume) –directly relates to peak luminosity (for given power) –important parameter for light & X-ray sources Beam energyBeam energy –Energy reach in HEP, wavelength reach in X-ray sources

42 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 42 Primary Challenges for Accelerator R&D Presently most radical new mechanisms:Presently most radical new mechanisms: –Plasma wave acceleration –Dielectric wake acceleration –other schemes based on the inverse FEL process These clearly need demonstration of capabilityThese clearly need demonstration of capability –not just accelerate tail-particles, need to create and accelerate a beam (bunch) –ability to accelerate both polarities

43 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 43 Dielectric Wake Accelerator Proof-of-principle experimentsProof-of-principle experiments (W. Gai, et al.) (W. Gai, et al.) –ANL AATF Mode superpositionMode superposition (J. Power, et al. and S. Shchelkunov, et al.) (J. Power, et al. and S. Shchelkunov, et al.) –ANL AWA, BNL Transformer ratio improvementTransformer ratio improvement (J. Power, et al.) (J. Power, et al.) –Beam shaping Tunable permittivity structuresTunable permittivity structures – For external feeding (A. Kanareykin, et al.) (A. Kanareykin, et al.) Tunable permittivity ΔE vs. witness delay Gradients ~100 MV/m, limited by available beam DWA Experimental History: Argonne / BNL experiments  Material limited breakdown (metal < dielectric < plasma)  Nearly symmetric response for positrons

44 U. Wienands, SLAC UA9 Workshop, 27-Oct-10 44 Summary of non-WFA expts. At FACET, we canAt FACET, we can –Study collimation schemes for a linear collider e+ and in particular e– as well crystals may offer important advantages extension of proton expts. at FNAL and CERN (UA9) –behaviour of crystals at high intensities –Study the generation of X-rays by the extreme fields equivalent to kTesla of magnetic fields use e+: stronger effects than with e– Possible to get coherent light? –with sizeable intensities??


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