Accelerator Physics Challenges of X-Ray FEL SASE Sources

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Presentation transcript:

Accelerator Physics Challenges of X-Ray FEL SASE Sources Paul Emma Stanford Linear Accelerator Center

Why a Linac-Based Free-Electron Laser (FEL*) ? Longitudinal emittance from linac is much smaller than ring Bunch length can approach 100 fsec with small energy spread Potential for 1010 brightness increase and 102 pulse length reduction Much experience gained from linear collider operation and study (SLC, JLC, NLC, TESLA, CLIC) At SLAC, the linac is available at DESY, XFEL fits well into TESLA collider plans Use SASE** (Self-Amplified Spontaneous Emission)  no mirrors at 1 Å * Motz 1950; Phillips 1960; Madey 1970 ** Kondratenko, Saldin 1980; Bonifacio, Pellegrini 1984

SASE Saturation Results LEUTL APS/ANL 385 nm September 2000 XFEL  0.1 nm (or 1 Å) Just 20 months ago: SASE saturation not yet demonstrated Since September 2000: 3 SASE FEL’s demonstrate saturation TTF-FEL DESY 98 nm VISA ATF/BNL 840 nm March 2001

Proposed/Planned SASE X-Ray FEL’s TESLA-XFEL at DESY (0.85-60 Å) LCLS at SLAC (1.5-15 Å) LCLS INFN/ENA FEL in Roma (15 Å) Fermi FEL at Trieste (12 Å) SCSS at Spring-8 (36 Å) 4GLS FEL at Daresbury (SXR) SASE-FEL at BESSY (12-600 Å)

Peak Brilliance of FEL’s 1 Å X-Ray ~109 photons per phase-space volume per band-width 103 by e- quality, long undulators 106 by FEL gain courtesy T. Shintake

TESLA XFEL at DESY 0.85-60 Å X-FEL Integrated into linear collider user facility 0.85-60 Å 3 compressors multiple undulators X-FEL Integrated into linear collider

X-FEL based on last 1-km of existing SLAC linac LCLS at SLAC 1.5-15 Å LCLS 2 compressors one undulator X-FEL based on last 1-km of existing SLAC linac

SASE FEL Electron Beam Requirements radiation wavelength (~1.5 mm realistic goal) transverse emittance: eN < 1 mm at 1 A, 15 GeV peak current undulator period energy spread: <0.08% at Ipk = 4 kA, K  4, lu  3 cm, … undulator ‘field’ beta function FEL gain length: 20Lg > 100 m for eN  1.5 mm Need to increase peak current, preserve emittance, and maintain small energy spread, all simultaneously AND provide stable operation

‘Slice’ versus ‘Projected’ Emittance For a collider… …collision integrates over bunch length — emittance ‘projected’ over the bunch length is important For an FEL… e- slips back in phase w.r.t. photons by lr per period lu Nlr  0.5 mm lr …FEL integrates over slippage length: ‘slice’ emittance (and E-spread) is important

Slice Emittance is Less Sensitive HEAD <1%sz however, centroid shifts of slices can be important transverse wakefield effect TAIL …as can b variations along bunch emittance of short ‘slice’ not affected by transverse wakes …also true for quad-misalignments, CSR, and RF kicks

RF Photo-Cathode Gun rapid RF-acceleration to avoid space-charge dilution Ipk  50-100 A Q  1 nC eN  1 mm laser beam electron beam emittance compensation solenoid courtesy J. Rossbach

Thermionic pulsed high-voltage gun …at Spring-8 SCSS (0.1-0.5 nC), CeB6 cathode and sub-harm. bunchers T. Shintake, TUPRI116

Emittance Results from Gun Test Facility at SLAC ‘projected’ emittance at reduced charge levels Parmela gaussian bunch at GTF limits gex Measurements 1 mm at 1 nC possible, but not demonstrated yet C. Limborg, TUPRI041, TUPRI042, TUPRI043 courtesy S. Gierman, J. Schmerge

Slice ey Measurements at BNL weak quad setting Slice ey Measurements at BNL dump 75 MeV 5 MeV undulators linac linac (off) DUVFEL medium quad setting projected gey  3.0 mm strong quad setting 200 pC, 50 A, 75 MeV care needed with image processing Data from SDL at BNL: W. Graves, et al.

Magnetic Bunch Compression DE/E z DE/E z ‘chirp’ DE/E z sz …or over-compression under-compression sz0 sE/E V = V0sin(wt) RF Accelerating Voltage Dz = R56DE/E Path Length-Energy Dependent Beamline

LCLS Linac Parameters for 1.5-Å FEL single bunch, 1-nC, 120-Hz SLAC linac tunnel FFTB hall Linac-0 L =6 m Linac-1 L =9 m rf = -38° Linac-2 L =330 m rf = -43° Linac-3 L =550 m rf = -10° BC-1 R56= -36 mm BC-2 L =22 m R56= -22 mm DL-2 L =66 m R56 = 0 DL-1 L =12 m R56 0 undulator L =120 m 7 MeV z  0.83 mm   0.2 % 150 MeV   0.10 % 250 MeV z  0.19 mm   1.8 % 4.54 GeV z  0.022 mm   0.76 % 14.35 GeV   0.02 % ...existing linac new rf gun 25-1a 30-8c 21-1b 21-1d X Linac-X L =0.6 m rf=180 21-3b 24-6d Two stages of bunch compression (RF phase: frf = 0 at accelerating crest)

Coherent Synchrotron Radiation Power coherent power N  6109 vacuum chamber cutoff ~l-1/3 incoherent power sz Wavelength

Coherent Synchrotron Radiation (CSR) Powerful radiation generates energy spread in bends Energy spread breaks achromatic system Causes bend-plane emittance growth (short bunch worse) bend-plane emittance growth e– R coherent radiation for l > sz DE/E = 0 sz l  L0 s DE/E < 0 Dx Dx = R16(s)DE/E overtaking length: L0  (24szR2)1/3 CSR wake is strong at very small scales (~1 mm) ~

CSR Microbunching* Animation f(s) DE/E0 gex * First observed by M. Borland (ANL) in LCLS Elegant tracking

…Energy Profile also modulated DE/E vs. z energy profile Next set of bends will magnify this again…  ‘slice’ effects current profile

CSR Microbunching Gain vs. l gex=1 mm ‘cold’ beam see also E. Saldin, Jan. 02, and Z. Huang, April 02 Initial modulation wavelength prior to compressor gex=1 mm, sd=310-5 “theory”: S. Heifets et al., SLAC-PUB-9165, March 2002

Evolution of LCLS Longitudinal Phase Space after L2 energy profile phase space time profile after DL1 sz = 830 mm sz = 190 mm after L1 after BC2 sz = 830 mm sz = 23 mm Current spikes further drive CSR after X-RF after L3 sz = 830 mm sz = 23 mm after BC1 at und. sz = 190 mm sz = 23 mm

CSR Micro-bunching in LCLS energy profile long. space temporal profile CSR can amplify small current modulations: micro-bunching sd  310-6 230 fsec Super-conducting wiggler prior to BC increases uncorrelated E-spread (310-6  310-5) R. Carr SC-wiggler damps bunching sd  310-5 tracking with Elegant code, written by M. Borland, ANL

CSR in Chicane (animation through LCLS BC2) f(s) DE/E0 gex

CSR Projected Emittance Growth (simulated) projected emittance growth is simply ‘steering’ of bunch head and tail x-pos 0.5 mm ‘slice’ emittance is not altered LCLS Tracking using Elegant z-pos

Energy Spectrum at TTF-FEL (DESY) no SASE T. Limberg, P. Piot, et al. TraFiC4 simulation

SPARC Project at INFN-LNF 1st stage bunch compression without bend magnets 122 MeV (simulation) SPARC Project @ INFN-LNF Collab. Among ENEA-INFN-CNR- Univ. Roma2-ST- INFM 9.4 M€ funding velocity compression with no bends ge  0.6 mm peak current >500 A ~100 mm L Serafini, WEYLA001 M. Ferrario, TUPRI056 C. Ronsivalle

Harmonic RF used to Linearize Compression RF curvature and 2nd-order compression cause current spikes Harmonic RF at decelerating phase corrects 2nd-order and allows unchanged z-distribution 1  -40° x = p Slope linearized lx = ls/4 830 mm avoid! 200 mm 3rd harmonic used at TTF/TESLA 4th harmonic used at LCLS 0.5-m X-band section for LCLS (22 MV, 11.4 GHz)

Diagnostics: Transverse RF Deflector sz  20 mm, E  5 GeV, V0  15 MV sx RF ‘streak’ off-axis screen 2.4 m V(t) S-band transverse RF deflector e- sz single-shot, absolute bunch length measurement V0 = 0 LCLS simulation V0 = 20 MV resolves ~20-fsec structure 230 fsec RF streak R. Akre, THPRI097

Measurements with Deflector at SLAC 46 GeV y = V0sin(f) voltage was calibrated with BPM 12 mm built in 1960’s (G. Loew…) 20 MV Planned also for TTF at DESY bunch length measurements in the SLAC linac sz<500 mm

Machine Stability Simulations (M. Borland, ANL) Track 105 particles with Parmela Elegant Genesis Repeat 230 times with ‘jitter’ in gun, RF, magnets, etc. Include wakefields and CSR Lg Ipk gex Pout <10% <10% Provides realistic estimate of operational stability and verifies machine ‘jitter budget’ <4% ~25%

Undulator Beam-Based Alignment (LCLS) uncorrected undulator trajectory sx > 500 mm S/m Undulator trajectory must be straight to ~5 mm level  simulate beam-based alignment procedure with realistic errors: BPMs, quads, poles… Quadrupole positions Trajectory BPM read-back trajectory after 3rd pass of BBA S/m sx  1.5 mm Df  82º beam size: 30 mm BBA also used for TESLA-FEL: DESY (B. Faatz)

Resistive-Wall Wakefields in the Undulator Strong magnetic field in undulator requires small gap… Need small radius pipe (r  2.5 mm, Lu  120 m: LCLS) Wake changes ‘slice’ energy during exponential gain regime — more damaging than incoming ‘chirp’ X-ray pulse r limit gap due to wake Courtesy S. Reiche Need smooth copper pipe

FEL Output Power with Undulator Wakefields ~40% power loss due to wakefield LCLS Genesis 1.3, S. Reiche, NIM A 429 (1999) 242.

Emittance Exchange: Transverse to Longitudinal transverse RF in a chicane… h k ex0 ez0 Electric and magnetic fields hk = 1 ex  ez0 ez  ex0 x0 , x0 z0 , d0 gex0 =5 mm gez0 =1 mm system also compresses bunch length x, x z, d gex0 =1 mm gez0 =5 mm M. Cornacchia, P. Emma, SLAC-PUB-9225, May 2002

Final Comments Merci Beaucoup For LCLS, slice emittance >1.8 mm will not saturate (TESLA ?) courtesy S. Reiche P = P0 eN = 1.2 mm P = P0/100 eN = 2.0 mm Merci Beaucoup SASE FEL is not forgiving — instead of mild luminosity loss, power nearly switches OFF electron beam must meet brightness requirements