Emittance preservation in the main linacs of ILC and CLIC Andrea Latina (CERN) Kiyoshi Kubo (KEK) LCWS 2012 - University of Texas at Arlington - Oct 22-26.

Slides:



Advertisements
Similar presentations
Update of RTML, Status of FNAL L-band and CLIC X-band BPM, Split SC Quadrupole Nikolay Solyak Fermilab (On behalf of RTML team) LCWS2010 / ILC 10, March.
Advertisements

Q20: The X-band collider has much tighter requirements for the alignment of the beam orbit with the structure axis, yet the basic instrumental precision.
Emittance dilution due to misalignment of quads and cavities of ILC main linac revised K.Kubo For beam energy 250 GeV,
Emittance dilution due to misalignment of quads and cavities of ILC main linac K.Kubo For beam energy 250 GeV, TESLA-type optics for 24MV/m.
On Cavity Tilt + Gradient Change (Beam Dynamics) K. Kubo K. Kubo.
Issues in ILC Main Linac and Bunch Compressor from Beam dynamics N. Solyak, A. Latina, K.Kubo.
Main Linac Simulation - Main Linac Alignment Tolerances - From single bunch effect ILC-MDIR Workshop Kiyoshi KUBO References: TESLA TDR ILC-TRC-2.
ATF2 FB/FF layout Javier Resta Lopez (JAI, Oxford University) for the FONT project group FONT meeting January 11, 2007.
ILC BDS Collimation Optimisation and PLACET simulations Adina Toader School of Physics and Astronomy, University of Manchester & Cockcroft Institute, Daresbury.
Luminosity Stability and Stabilisation Hardware D. Schulte for the CLIC team Special thanks to J. Pfingstner and J. Snuverink 1CLIC-ACE, February 2nd,
Feed forward orbit corrections for the CLIC RTML R. Apsimon, A. Latina.
LCLS-II Transverse Tolerances Tor Raubenheimer May 29, 2013.
CLIC programme at FACET Update on CERN-BBA A. Latina, J. Pfingstner, G. De Michele, D. Schulte (CERN) E. Adli (Univ. of Oslo), J. Resta Lopez (IFIC) In.
Alignment and Beam Stability
Ground Motion + Vibration Transfer Function for Final QD0/SD0 Cryomodule System at ILC Glen White, SLAC ALCPG11, Eugene March 21, 2011.
ATF2 Javier Resta Lopez (JAI, Oxford University) for the FONT project group 5th ATF2 project meeting, KEK December 19-21, 2007.
Summary of AWG4: Beam Dynamics A. Latina (CERN), N. Solyak (FNAL) LCWS13 – Nov 11-15, 2013 – The University of Tokyo, Japan.
Verification of Beam-Based Alignment Algorithms at FACET A. Latina, J. Pfingstner, D. Schulte (CERN) E. Adli (Univ. of Oslo) With the collaboration of:
Drive Beam Linac Stability Issues Avni AKSOY Ankara University.
Main Linac Integration Work Packages Chris Adolphsen Dec 11, 2007 High Priority Items in Red.
For Draft List of Standard Errors Beam Dynamics, Simulations Group (Summarized by Kiyoshi Kubo)
Feed forward orbit corrections for the CLIC RTML R. Apsimon, A. Latina.
@ Fermilab May 15-17, 2006, FNAL KIRTI RANJAN – DOE Review1 ILC Simulation for RDR Kirti Ranjan Fermilab.
ILC Feedback System Studies Nikolay Solyak Fermilab 1IWLC2010, Geneva, Oct.18-22, 2010 N.Solyak.
Summary of WG1 K. Kubo, D. Schulte, P. Tenenbaum.
Beam dynamics on damping rings and beam-beam interaction Dec 포항 가속기 연구소 김 은 산.
ILC BDS Static Beam-Based Alignment and Tuning Glen White SLAC 1.Aims. 2.Error parameters and other assumptions. 3.Overview of alignment and tuning procedure.
Simulations Group Summary K. Kubo, D. Schulte, N. Solyak for the beam dynamics working group.
Dynamic Tuning Selected Highlights Freddy Poirier (DESY) ILC accelerator physics group meeting 28 th January 2008.
Report of 2 nd ILC Workshop (Snowmass) Working Group Kiyoshi KUBO references: Slides of the plenary talks in the workshop by P.Tenembaum and.
The CLIC decelerator Instrumentation issues – a first look E. Adli, CERN AB/ABP / UiO October 17, 2007.
BDS Andrei Seryi, Deepa Angal-Kalinin, Emmannual Tsesmelis, Rogelio Tomas, Andrea Latina, Daniel Schulte Detectors Civil engineering.
July 19-22, 2006, Vancouver KIRTI RANJAN1 ILC Curved Linac Simulation Kirti Ranjan, Francois Ostiguy, Nikolay Solyak Fermilab + Peter Tenenbaum (PT) SLAC.
Simulations (LET beam dynamics ) Group report Kiyoshi Kubo.
Introduction: Tasks of “Information for simulations”, hardware specs K.Kubo
Beam Dynamics WG Summary N.Solyak, K.Kubo, A.Latina LCWS 2014 – Oct 6-10, 2014 – Belgrade, Serbia.
Beam Dynamics WG K. Kubo, N. Solyak, D. Schulte. Presentations –N. Solyak Coupler kick simulations update –N. Solyak CLIC BPM –A. Latina: Update on the.
13 September 2006 Global Design Effort 1 ML (x.7) Goals and Scope of Work to end FY09 Nikolay Solyak Fermilab Peter Tenenbaum SLAC.
Placet based DFS simulations in the ILC Main Linac. Some preliminary results of error scans open for discussion Javier Resta Lopez JAI, Oxford University.
J. Pfingstner Imperfections tolerances for on-line DFS Improved imperfection tolerances for an on-line dispersion free steering algorithm Jürgen Pfingstner.
Kiyoshi Kubo Electron beam in undulators of e+ source - Emittance and orbit angle with quad misalignment and corrections - Effect of beam pipe.
Low Emittance Generation and Preservation K. Yokoya, D. Schulte.
1 DFS Studies on the Main Linac with Rnd-walk-like motion (preliminary) Accelerator Physics Meeting 02 october 2007 Freddy Poirier.
1 DFS Studies on the Main Linac with Rnd-walk-like motion LET Beam Dynamics Workshop 12 th December 2007 Freddy Poirier.
DMS steering with BPM scale error - Trial of a New Optics - Kiyoshi Kubo
Main Linac Tolerances What do they mean? ILC-GDE meeting Beijing Kiyoshi Kubo 1.Introduction, review of old studies 2.Assumed “static” errors.
Simulations - Beam dynamics in low emittance transport (LET: From the exit of Damping Ring) K. Kubo
Introduction D. Schulte for K. Kubo and P. Tenenbaum.
Emittance preservation in the RTML of ILC and CLIC Andrea Latina (CERN) Nikolay Solyak (FNAL) LCWS University of Texas at Arlington - Oct
Progress in 2006 of ELAN- BDYN and INSTR D. Schulte G. Blair.
DRAFT: What have been done and what to do in ILC-LET beam dynamics Beam dynamics/Simulations Group Beijing.
Wakefield effect in ATF2 Kiyoshi Kubo
8 th February 2006 Freddy Poirier ILC-LET workshop 1 Freddy Poirier DESY ILC-LET Workshop Dispersion Free Steering in the ILC using MERLIN.
Progress in CLIC DFS studies Juergen Pfingstner University of Oslo CLIC Workshop January.
Review of Alignment Tolerances for LCLS-II SC Linac Arun Saini, N. Solyak Fermilab 27 th April 2016, LCLS-II Accelerator Physics Meeting.
ILC Main Linac Beam Dynamics Review K. Kubo.
Effects of Accelerating Cavities on On-Line Dispersion Free Steering in the Main Linac of CLIC Effects of Accelerating Cavities on On-Line Dispersion Free.
From Beam Dynamics K. Kubo
Arun Saini, N. Solyak Fermi National Accelerator Laboratory
RF-kick in the CLIC accelerating structures
For Discussion Possible Beam Dynamics Issues in ILC downstream of Damping Ring LCWS2015 K. Kubo.
Emittance Dilution and Preservation in the ILC RTML
Beam Dynamics in Curved ILC Main Linac (following earth curvature)
ILC Z-pole Calibration Runs Main Linac performance
SC Quadrupole Magnets in ILC Cryomodules
DFS Simulations on ILC bunch compressor
Adaptive Alignment & Ground Motion
Accelerator Physics Technical System Group Review
Beam-Based Alignment Results
Start-to-End Simulations for the TESLA LC
Presentation transcript:

Emittance preservation in the main linacs of ILC and CLIC Andrea Latina (CERN) Kiyoshi Kubo (KEK) LCWS University of Texas at Arlington - Oct

Table of contents Main sources of emittance growth in a linac and their cure Low emittance transport in the ILC and CLIC main linacs (LET) Simulations, Code benchmarking Experimental program 2

Main sources of emittance growth and their cure Transverse wakefields in the accelerating structures -Single-bunch break-up : careful lattice design / BNS damping -Bunch-to-bunch instabilities: damping by RF design / detuning Static imperfections – Quadrupole / BPM misalignments : pre- and beam-based alignment Others – Resistive wall wakes : strong focusing – Fast beam-ion instability : high vacuum – RF kicks: RF design – Ground motion : feedback loops – BPM scaling errors: tuning and BBA 3

Wakefields The beam pipe is not a perfectly conducting pipe of constant aperture. A beam passing through a cavity radiates electromagnetic fields and excites the normal modes of the cavity. 4 The consequences are: 1)the beam loses energy; 2)energy can be transferred from head to tail of a bunch; 3)the head of the bunch can deflect the tail; 4)energy and deflections can be transferred between bunches if there are normal mode with high Q (quality factor). 2) - 4) can give rise to instabilities.

Long-range wakefields Bunch-to-bunch long-range wakefields can induce transverse instabilities leading to beam break-up. Long-range wakefields are sine-like functions: They can be reduced by – damping – Detuning 5

Beam-based alignment, tuning strategy 6

Emittance budgets 7

CLIC main linac lattice design The main linac injection emittances are 600 and 10 nm respectively. The lattice is designed with the following criteria: Strong focusing lattice, to balance the impact of the transverse wakefields in the accelerating structures Lattice strength is varied along the linac to have an almost constant fill factor BNS damping is used to compensate for short- range wakefield effects. The RF phases offset chosen is 8 o at the beginning and 30 o at the end of the linac The linac is composed by five types of modules that accommodate two beams: drive beam and main beam 8 The total emittance growth in a linac without imperfections is about zero. Schematic of the CLIC Type-0 module Linac optics, the beta function scales with sqrt(E)

Main Linac Tolerances D. Schulte9 1)Pre-align BPMs+quads accuracy O(10μm) 2) Beam-based alignment 3) Use wakefield monitors accuracy O(3.5μm) Stabilise quadrupole 1Hz

Tolerance for static imperfections in CLIC 10 ErrorCLICwith respect to Quad Offset17 μmgirder/survey line Quad roll≤100 μradsurvey line Girder Offset9.4 μmsurvey line Girder tilt9.4 μradsurvey line Acc Structures Offset5 μmgirder Acc Structures tilt200 μradgirder BPM Offset14 μmgirder/survey line BPM resolution0.1 μmBPM center Wakefield monitor3.5 μmwake center In ILC the specifications have much larger values than in CLIC More difficult alignment in super-conductive environment Dedicated effort for CLIC is needed Wakefield monitors are currently foreseen only in CLIC

Test of prototype shows vertical RMS error of 11μm i.e. accuracy is approx. 13.5μm Improvement path identified Pre-alignment System D. Schulte11 Required accuracy of reference point is 10μm

Emittance growth in CLIC 12 Simple orbit correction

Dispersion-Free Steering in CLIC 13 Dispersion-free correction (DFS) The emittance growth is largely reduced by DFS, but it is still too large Main cause of emittance growth are: Trajectory is smooth but not centered in the structures Effective coherent structure offsets Structures initial scatter remains uncorrected

RF-structure alignment in CLIC 14 RF structures are equipped with wakefield position monitors: girders are moved to zero the average center of the beam w.r.t. the structures Beam trajectory is hardly changed by structure alignment but emittance growth is strongly reduced

Final emittance growth in CLIC 15 Selected a good DFS implementation Trade-offs are possible Multi-bunch wakefield misalignments of 10 μm lead to 0.13 nm emittance growth Performance of local pre-alignment is acceptable ImperfectionWith respect toValueEmittance growth Wakefield monitorwake center3.5 μm0.54 nm Acc Structures tiltgirder200 μrad0.38 nm BPM Offsetgirder/survey line14 μm0.37 nm Quad rolllongitudinal axis100 μrad0.12 nm Articulation point offsetwire reference12 μm0.10 nm BPM resolutionBPM center0.1 μm0.04 nm Acc Structures Offsetgirder10 μm0.03 nm Girder end pointarticulation point5 μm0.02 nm TOTAL1.60 nm

Ground Motion and Its Mitigation 16D. Schulte Natural ground motion can impact the luminosity typical quadrupole jitter tolerance O(1nm) in main linac and O(0.1nm) in final doublet -> develop stabilisation for beam guiding magnets

Active Stabilisation Results 17D. Schulte B10 No stab.53%/68% Current stab.108%/13% Future stab.118%/3% Luminosity achieved/lost [%] Machine model Beam-based feedback Code Close to/better than target

ILC static errors and cures Agreed “standard” errors: Next slide – Random Gaussian distributions are used for most studies DMS (Dispersion Matching Steering) correction as standard correction method – For dispersion measurement, change beam energy 10% ~ 20% – Simulation studies using many different codes and by different persons. – BPM scale error is important  non-zero design dispersion (see 3 rd next slide) Other methods (Kick minimum, Balistic, wake bumps, etc.) as additional or alternative corrections. Studies for upgrade to 1TeV ECM No serious problem expected. – An example shown: next-next slide 18

ILC static imperfections 19 ErrorML Coldwith respect to Quad Offset300 μmcryo-module Quad roll300 μraddesign RF Cavity Offset300 μmcryo-module RF Cavity tilt300 μradcryo-module BPM Offset (initial)300 μmcryo-module Cryomoduloe Offset200 μmdesign Cryomodule Pitch20 μraddesign “standard” errors

Dependence on Initial and Final energy “Standard” static errors + BPM resolution 1um + DMS K.Kubo LCWS 2011 Oregon  E init : Change of initial energy for dispersion measurement 20

BPM Scale error affects DMS K.Kubo, ILC-CLIC-LET-Workshop, 2009 CERN Vertical Orbit and Dispersion Base line optics (same as RDR) and new possible optics In DMS, dispersion is measured at each BPM and adjusted as design. For non-zero design dispersion, BPM scale error affects the accuracy. We will need good BPM scale calibration (< 5%) for baseline optics. Alternative optics may mitigate the effect. (Zero dispersion at every other BPM) 21

Lattice of upgraded linac (1 TeV ECM) Part of E_beam 25~250 GeV of old linac will be used for 275~500 GeV of new linac. For using the same quad magnet (week for higher energy), FOFODODO lattice will be used instead of FODO. 22

Emittance growth along ML Cavity tilt random change 15 urad, equivalent to Fixed 300 urad + 5% gradient change Emittance growth proportional to square of the change Emittance growth by Cavity tilt 23

Final emittance growth in ILC Initial vertical normalized emittance at the exit of the DR is 20 nm. Vertical emittance at the exit of the ML must be 31 nm or below. 24

ILC ML major dynamic errors SourceAssumption (Tolerance) Induced orbit jitter Induced emittance growth Quad vibration (offset change)100 nm1.5 sigma0.2 nm Quad+steering strength jitter1E-41 sigma0.1 nm Cavity tilt change3 urad0.8 sigma0.5 nm Cavity to cavity strength change, assuming 300 urad fixed tilt 1%0.8 sigma 0.5 nm Pulse to pulse and in each pulse (flatness) ML 15 GeV to 250 GeV 25

ILC Other considered issues, examples Coupler wake and RF transverse kicks – No problem because of short bunch length (compare with in RTML) Emittance dilution in undulator for e+ production – Dispersive effect will be small. – Wakefield in the narrow beam pipe can be significant. May need movers. Specification of magnet change speed – For BBA, or startup after shutdown, etc. – Required speed will be achievable without serious R&D. 26

Code benchmarking 27 We rely on simulations: code validation is essential. Emittance dilution after performing DFS in LIAR and reading misalignments and corrector settings into the other codes. SLAC-TN

Experimental Activities Simulations are not sufficient. Measure of transverse wakefields in the CLIC accelerating structures (CLASSE, ex-ASSET) – So far we rely on simulations, experimental verification needed – Short- and long- wakefields at FACET/SLAC Beam-based Alignment algorithms and System Identification Procedures at SLC (T-501 at SLAC) – Dispersion-Free steering in a linac has never been proven Collimator wakefields measurement at ESTB (SLAC) – Critical for beam delivery system performance (next talks) 28

T501: FACET test-beam proposal to study advanced global correction schemes for future linear colliders. CERN-SLAC collaboration where algorithms developed at CERN are tested on the SLAC linac. The study includes linac system identification, global orbit correction and global dispersion correction. Successful system identification and global orbit correction has been demonstrated on a test-section of 500 m of the linac. (Above) Identified Rx response matrix for the test-section of the linac (17 correctors, 48 BPMs) (Above) Global orbit correction of test-section, with feed-forward to prevent the correction to affect FACET S20 experimental area. Horizontal and Vertical Obrits Convegence T501: CERN BBA at SLAC A. Latina, J.Pfingstner, D. Schulte (CERN), E. Adli (SLAC) 29

Conclusions Extensive studies exist both for CLIC and ILC CLIC requirements are tighter but beam-based alignment procedures seem to fully recover the performance CLIC showed an excellent synergy with the pre-alignment / stabilization groups Simulation code are growing and becoming more trustworthy Experimental programs are on-going with promising results 30

Possible Further studies (some studies already exist but not completed) Studies with realistic alignment model – Alignment engineers and beam dynamics physicists should agree. More realistic DMS procedure – E.g. Simulations combined with upstream (RTML) Optics choice, for making less sensitive to BPM scale error (ILC) Simulations with failed components (BPM, Cavities, Magnets) … None of these are expected to be critical. 31

Acknowledgements These results have been obtained by the efforts of many people Alignment and stabilization team: H. Meinaud Durand, K. Artoos, J. Snuverink, J. Pfingstner et al. CLIC Beam Physics Group: D. Schulte, P. Eliasson, G. Rumolo, R. Tomas, Y. Papaphilippou, B. Dalena, B. Jeanneret et al. ILC International Collaborators: N. Solyak, K. Ranjan, K. Kubo, J. Smith, P. Tenenbaum, N. Walker, F. Poirier et al. 32