Accelerating Structure Feasibility W. Wuensch CLIC ACE 26-5-2009.

Slides:



Advertisements
Similar presentations
IWLC2010Walter Wuensch19 October 2010 Progress on CLIC rf structures.
Advertisements

Breakdown Rate Dependence on Gradient and Pulse Heating in Single Cell Cavities and TD18 Faya Wang, Chris Nantista and Chris Adolphsen May 1, 2010.
CLIC08 workshop Structure production: CERN activities and Master Schedule G. Riddone, W. Wuensch, R. Zennaro, Contributions from C. Achard, S. Atieh, V.
Choke-mode damped accelerating structures for CLIC main linac Hao Zha, Tsinghua University Jiaru Shi, CERN
CERN-KEK X-band collaboration 3 Dec T. Higo on behalf of X-band group of KEK.
INVESITGATION OF AN ALTERNATE MEANS OF WAKEFIELD SUPPRESSION IN CLIC MAIN LINACS CLIC_DDS.
Report from KEK High gradient study results from Nextef (+ other related activities) LCWS2011, Granada Sep. 27, 2011 T. Higo.
CARE07, 29 Oct Alexej Grudiev, New CLIC parameters. The new CLIC parameters Alexej Grudiev.
X-band Structures Test Results at NLCTA Faya Wang Chris Adolphsen, Christopher Nantista 9-Feb-11.
Experimental breakdown studies – breakdown diagnostics Linking simulation and experiment Jan W. Kovermann, CERN, RWTH Aachen SLAC workshop July 2009.
Recent 30 GHz CTF2 M. Gerbaux, S. Döbert, Jan Kovermann, R. Zennaro.
4th CLIC Advisory Committee (CLIC-ACE), 26 th - 28 th May Alternate Means of Wakefield Suppression in CLIC Main Linac Roger M. Jones, Vasim Khan,
INVESITGATION OF AN ALTERNATE MEANS OF WAKEFIELD SUPPRESSION IN CLIC MAIN LINACS CLIC_DDS.
1 X-band Single Cell and T18_SLAC_2 Test Results at NLCTA Faya Wang Chris Adolphsen Jul
ABSTRACT A damped detuned structure (DDS) for the main linacs of CLIC is being studied as an alternative design to the present baseline heavily damped.
Working Group 1: Microwave Acceleration Summary 10 July 2009.
ABSTRACT The main accelerating structures for the CLIC are designed to operate at 100 MV/m accelerating gradient. The accelerating frequency has been optimised.
CLIC MAIN LINAC DDS DESIGN AND FORTCOMING Vasim Khan & Roger Jones V. Khan LC-ABD 09, Cockcroft Institute /14.
Wakefield suppression in the CLIC main accelerating structures Vasim Khan & Roger Jones.
High Gradient and High Q R&D Topics 1- Explore Q > for TESLA parameter flexibility –higher luminosity through higher rep rate, longer rf pulse… 2-
Design of Standing-Wave Accelerator Structure
Vasim Khan X-Band RF Structures, Beam Dynamics and Sources Workshop, Cockcroft Institute /24 CLIC_DDS study
ABSTRACT The main accelerating structures for the CLIC are designed to operate at 100 MV/m accelerating gradient. The accelerating frequency has been optimised.
CMS HIP Multiscale simulation Model of Electrical Breakdown Helsinki Institute of Physics and Department of Physics University of Helsinki Finland Flyura.
Alessandro Cappelletti for CTF3 collaboration 5 th May 2010 RESULTS OF BEAM BASED RF POWER PRODUCTION IN CTF3.
DDS limits and perspectives Alessandro D’Elia on behalf of UMAN Collaboration 1.
Walter Wuensch CLIC project meeting, 31 March 2015 Accelerating structure program: design and testing.
5 th CLIC X-band collaboration meetingWalter Wuensch16 May 2011 CLIC rf structure program.
Accelerating structure test results and what’s next Walter Wuensch CTF3 collaboration meeting
Particle-in-Cell Modeling of Rf Breakdown in Accelerating Structures and Waveguides Valery Dolgashev, SLAC National Accelerator Laboratory Breakdown physics.
Course B: rf technology Normal conducting rf Part 5: Higher-order-mode damping Walter Wuensch, CERN Sixth International Accelerator School for Linear Colliders.
An Overview of the CLIC Testing Program W. Wuensch CLIC ACE
Overview of the CLIC RF Structure Development Program W. Wuensch Second Collaboration Meeting on X-band Structures KEK,
Overview of CLIC main linac accelerating structure design 21/10/2010 A.Grudiev (CERN)
X-Band: test stand and structure program
High gradient acceleration Kyrre N. Sjøbæk * FYS 4550 / FYS 9550 – Experimental high energy physics University of Oslo, 26/9/2013 *k.n.sjobak(at)fys.uio.no.
Recent High-gradient test result at KEK Linear Collider Workshop 2012 Arlington, Texas (WebEx) 25 October, 2012 Toshi Higo and X-band group of KEK.
PBG Structure Experiments, AAC 2008 Photonic Bandgap Accelerator Experiments Roark A. Marsh, Michael A. Shapiro, Richard J. Temkin Massachusetts Institute.
Recent high-gradient results, rf testing, places and plans Steffen Döbert, CLIC Workshop, Test facilities High gradient results Future testing.
Progress in Breakdown Modelling – MD and PIC Breakdown Simulations Helga Timkó, Flyura Djurabekova, Kai Nordlund, Aarne Pohjonen, Stefan Parviainen Helsinki.
Summary of progress towards CLIC goals and next steps for structure testing 6 th X-band collaboration workshop, April 18 th- 20 th 2012 Steffen Döbert,
KEK workshopWalter Wuensch18 April 2012 Status and objectives of the CLIC X-band and high- gradient activity.
The CLIC accelerating structure development program Walter Wuensch CARE05 23 November 2005.
The NLC RF Pulse Compression and High Power RF Transport Systems Sami G. Tantawi, G.Bowden, K.Fant, Z.D.Farkas, W.R.Fowkes J.Irwin, N.M.Kroll, Z.H.Li,
CLIC Accelerating Structure R&D Introduction W. Wuensch X-band workshop
Progress of X-Band Accelerating Structures LINAC10, Tsukuba 17 Sep T. Higo (KEK)
WP 9.2 DDS Status, R.M. Jones, 25 th Oct 2010, WebEx Phone-in, Geneva 1 WP 9.2: DDS Status Roger M. Jones Cockcroft Institute and The University of Manchester.
Hybrid designs - directions and potential 1 Alessandro D’Elia, R. M. Jones and V. Khan.
TD18 High Power Test Results Faya Wang Chris Adolphsen May 3, 2010.
CLIC accelerating structures: study of the tolerances and short range wakefield considerations R. Zennaro CERN.
W. Wuensch CLIC project meeting High-power rf structure testing.
HIP News from Helsinki… Flyura Djurabekova Helsinki Institute of Physics and Department of Physics University of Helsinki Finland.
Status of high gradient experiments at Nextef Kazue Yokoyama, Toshiyasu Higo, Yasuo Higashi, Shuji Matsumoto, Shigeki Fukuda Accelerator Laboratory, KEK.
Peak temperature rise specification for accelerating structures: a review and discussion CLIC meeting
Optimization of CLIC-G structure & Design of CLIC open structure Hao Zha, Alexej Grudiev (CERN) Valery Dolgashev (SLAC) 27/01/2015.
High-gradient rf constraints W. Wuensch X-band workshop
1 Design and objectives of test accelerating structures Riccardo Zennaro.
Accelerating structure prototypes for 2011 (proposal) A.Grudiev 6/07/11.
Update on PETS experiments (Igor for the CLIC collaboration)
Structure Wakefields and Tolerances R. Zennaro. Parameters of the CLIC structure “CLIC G” (from A. Grudiev) StructureCLIC_G Frequency: f [GHz]12 Average.
CERN, 27-Mar EuCARD NCLinac Task /3/2009.
Test Accelerating Structures Designs, Objectives and Critical Issues
Breakdown experiments
NC Accelerator Structures
CLIC_DDS study
Review of rf structure test results
Developments on Proposed
Summary of the test structure design
Update of CLIC accelerating structure design
Progress in the design of a damped an
Presentation transcript:

Accelerating Structure Feasibility W. Wuensch CLIC ACE

Outline Requirement summary Demonstration status Near-term prospects Contingency planning Longer-term development

Performance requirements oversimplified into a few numbers: Loaded gradient: 100 MV/m Pulse length total/flat top: 240/160 ns Breakdown rate in the range of a few /m Minimum average a/λ: 0.11 (short range wake) Maximum long range wake: 6 V/pC/m/mm

Status

Two T18_VG2.4_DISC Structures Structure for KEK Test Structure for SLAC Test

For Constant Breakdown Rate Unloaded Gradient at Different Conditioning Times C. Adolphsen

BKD Distribution Along Structure at Different Stages of Processing Did not find visual evidence related to the hot cell in a post-run boroscope exam – typical of NLC/GLC structures, many of which had hot cells C. Adolphsen

BDR at 252nsec ACC breakdowns are defined as sudden breakdowns from normal running. This excludes events following such breakdowns, typically only the very first pulse. Even if include such associated breakdowns, the BDR stays within a factor two. Comparable or larger number of FC- UP events are still to be investigated in their origin. T18 - KEK test

Status summary Two undamped T18 structures have run at an unloaded accelerating gradient at around 100 MV/m with the CLIC specified 4x10 -7 /m breakdown rate with 230/250 ns rectangular pulses. The CLIC flat-top is 160 ns, full width at 90% maximum gives effective pulse length, so we are above specification here. Beam loading typically reduces the gradient by 15 to 20% (18% in CLIC_G), but this may be partially compensated by a corresponding decrease in breakdown rate, especially in strongly tapered structures. The magnitude of the beam loading effect is to be studied in two beam test stand. The increased gradient was achieved through the use of high-power scaling laws in the design process.

Near-term prospects

Then next crucial step for the accelerating structure feasibility demonstration is to determine the influence of the damping features on gradient. We believe that this effect will be small because, - The (smaller) damping features of the NLC/JLC structures did not affect high-gradient performance. The H75 with manifold damping ran at 102 MV/m, 150 ns rectangular pulse, 6x10 -6 BDR/structure for example. - An artful analysis of the slotted-iris quadrant (HDS60 in particular) data indicates their (smaller) damping features did not affect performance. Requires geometric scaling of gradient, so not definitive demonstration. HOWEVER the pulsed surface heating we have now, over 50 C, is significantly higher than other structures, around 20 C, and breakdown and pulsed surface heating could be linked in a number of ways. We also move towards the nominal CLIC_G geometry which has what we now, through better understanding of iris scaling, believe is a more optimum iris range. This helps also with pulsed surface heating.

undampeddamped Transition from undamped to damped in the CLIC_vg1 type

Structures under test

Structures are directly relevant for determining the effect of damping StructureBuilt byStatusScheduled test date Test location TD18 #1CERNReadyMarch, but on hold SLAC TD18 #2KEK/SLACUnder assembly SeptemberKEK TD18 #3KEK/SLACUnder assembly AugustSLAC TD24 #1 and 2CERNUnder assembly AugustSLAC TD18 QUAD #2KEKFinal assemblyJuneKEK If any one of these structures show a satisfactory gradient we will have demonstrated feasibility.

Fabrication issues Currently the majority of the test structures are made by KEK and SLAC due to their extensive experience in building low-breakdown rate structures. These structures are made by 1020 °C hydrogen brazing. In recent months we have made our first brazed disk X-band structure since the early nineties. Our technique, 820 °C bond/braze, is basically the same as Fermilab’s. Unfortunately this T18 ran very badly. We have cut it apart, compared it to measurements and analyzed it,

T18_CERN Breakdown distribution of T18Disk_SLAC (red, last 500hrs), 210~230 ns,110~120 MV/m T18Disk_CERN (Blue,40hrs). 180 ns,45~49 MV/m ‘Hot’ phases All iris - presence of small craters. S particles along grain boundaries – from bulk Iris 12 – contamination (Ca, C)

Reacting to the CERN T18 result The poor performance was probably determined by a contamination on iris 12. However the discovery of presence of S particles from the bulk Cu is indicative of a more systematic problem – which calls into question our 30 GHz results… Our response is to now assemble under a laminar flow hood to reduce the chances of contamination like that seen on iris 12. In addition we have also adopted the main difference with the Fermilab procedure, a 1000 °C disk pre-fire. One benefit is this seems to ensure that S stays disolved in the bulk and doesn’t collect on grain boundaries. Our T18 was preceded at SLAC by a number of ‘exotic’ structures which also ran badly. These structures incorporated many new ideas – materials and quadrants - from the 30 GHz, 150 MV/m program. I believe these structures were not limited by fundamental issues and that we will return to the ideas one day and get them to work. But the consequence is that CERN has a credibility problem for delivering good structures. An excellent new team with a rigorous approach is learning to build structures and I believe we will resolve our problems soon (maybe already). We hope our collaborators are patient with us. Making duplicate structures according to KEK/SLAC techniques (mainly high-temp bonding in H 2 atmosphere) should help clear things up. And we must have a testing program here at CERN to get the timely feedback that we need.

Contingency planning (also stuff which might be better in the long run)

Contingency planning – What can we do if the effect of the heavy damping features on gradient is significant? A lot of course depends on why the gradient is reduced. But to cover this possibility we are actively considering different damping mechanisms. In addition, the “classic” problem of surface damage through pulsed surface heating fatigue has not gone away. We have a ΔT of 56 °C in the nominal CLIC structure, which is very high for our baseline design of brazed copper disks. We could end up with a 4000 hour test that goes fine, but the structures all fall apart after a couple of years. We believe we have two types of solutions – damping configuration and material.

Manifold damping – Roger Jones (now at Cockcroft Inst/ and Manchester U.) and Vasim Kahn are applying the DDS concept to 100 MV/m using our scaling laws. The high gradient performance of the damping has already demonstrated. However the much weaker damping means the bunch spacing must go up and efficiency down. That is unless we have the tolerances for dipole mode zero crossings… A CLIC DDS design and prototype is an FP7 activity.

4th CLIC Advisory Committee (CLIC-ACE), 26 th - 28 th May Wake-field Suppression in CLIC_DDS Main Linac -Initial design  Circuit model provides rapid determination of optimal wakefield suppression results in a bandwidth of 3.6  (3.36 GHz) and  f/ f c =20%.  Leftmost indicates the modal distribution and rightmost the coupled and uncoupled wakefield  Four-fold interleaving of successive structures results in excellent wake- field suppression at the location of each bunch  Meets CLIC beam dynamics requirements!  However, breakdown considerations require a redesign with additional constraints imposed Envelope of Wakefield for Single 25-Cell Structure (Q ~ ∞ ) Wakefield for 8-Fold Interleaved Structure (Q ~ ∞) Kick Factor Weighted Density Function Envelope of Wakefield for 4-Fold Interleaved Structure (Finite Q ) dn/df Kdn/df Coupled Uncoupled

Choke mode damping Valery’s first try at a choke mode cavity didn’t work very well at high power. However Alexej has proposed a new configuration which will be high-power tested with a CD10- choke structure. Igor’s choke flange is working beautifully. We will study a choke mode CLIC structure in a collaboration with Tsinghua University and they will build a prototype. Fellow hopefully approved by end of week. Pulse surface heating is way down compared to waveguide damping but so is the damping strength. Plus this assembly can be done without brazing, so high-strength copper alloys for example can be used. Probably implies a larger bunch spacing. Damping loads are going to be tough…

Slotted-iris structures made from quadrants Excellent damping characteristics, especially with iris slots. Full range of materials and preparation techniques possible. We had hints of success but mostly problems. The HDS60 had a performance consistent with brazed disks if you use scaling laws. The HDX-11 worked well for about 20 hours and an HDS4 worked well for about 7 hours. Is the subsequent deterioration fundamental or due to specific rf design features? Other quadrants didn’t work well but were these problems fundamental or technical? 160 mm 30 GHz HDS60X-band HDX11

Longer-term prospects

Quantitative approach to high-gradients and efficient linacs Comprehensive rf design High-power scaling laws Simulation and theory Diagnostics Rf experiments Dc spark experiments Integrated rf and beam dynamics optimization

The importance of iris aperture It is quite clear that iris aperture is the single most important structure parameter for both beam dynamics and gradient and consequently for overall efficiency. The computation of short range wakes is well established. Original theory is by Karl Bane and others. We have even had a EuroTeV fellow (Riccardo Zennaro) to cross check theory with computation by GDFDL in our parameter range. Analysis of existing high gradient data combined with some physical reasoning by Alexej and myself has resulted in gradient scaling parameters, P/C and S c, which reflect and give, respectively, a very strong dependence of gradient on iris diameter. To determine this crucial dependency more precisely, and to give input for further gradient scaling studies, a series of 10 cell structure tests, called C10’s, with different iris sizes has been launched. Fabrication is at KEK and SLAC.

Schematic View for C10 Structures - II Subassembly for Test Cells

C10 structures

Other important effects The next step will be to quantify the effect of tapering, which luckily seems to have a beneficial effect. Comparison of the T18, very strongly tapered, and the T24 will address this issue. We believe this is due to transient power flow into a breakdown. And have made a 30 GHz test to address this issue, the “speed-bump” Gradient might also be dependant on group velocity. To investigate this we have made the 30 GHz TM 020 structure.

31 Speed bump (TM 03 ) R= mm R_iris= mm Iris_thickness= 1mm Goal : « protect » the structure by lowering V g in the first cell (usually the most damaged). Tested in both direction : RF fed from the input (4.1×10 6 pulses, 2186 breakdown) → the speed bump plays its role RF from the output (1.7×10 6 pulses, 501 breakdown) → the speed bump has no effect Test structure in disks: 30 cell and identical mode launcher of the “conventional” 2π/3 Ø 3.5 mm

-- Conventionnal 3.5mm structure Speed bump (TM 03 ) - results No effect observed on the breakdown rate : similar results in both directions and for the 3.5 mm structure (same design without speed bump), but… Standard disc 1Standard disc 28

33 Same phase advance Same P/c Same aperture and iris shape Same field configuration in the iris region Is it possible to change some global parameter without changing local field distribution? TM 01 regular cell “reference” TM 02 regular cell Only by changing the propagating mode. Different group velocity: 4.7% and 2% Different R/Q: 29 kΩ/m and 12 kΩ/m but PRELIMINARY TM 02 structure – separate effect of group velocity and local fields

Dark current: Direct comparison between simulation and measurement in the T18 structure. Simulation by SLAC ACG using Track3P. Fermilab is starting tracking simulation activities too. Measured at KEK

Multiscale Modelling of Vacuum Arcs in Breakdowns Flyura Djurabekova, Helga Timkó, Kai Nordlund Helsinki Institute of Physics and CERN

36 May 2009 H. Timkó, CERN & HIP Multiscale model Our model corresponds to the above 3 phases. Stage 1: Charge distribution at the surface Method: DFT with external electric field Stage 2: Atomic motion & evaporation Method: Hybrid ED&MD model Classical MD Solution of Laplace equation Stage 3: Evolution of surface morphology due to the given charge distribution Method: Kinetic Monte Carlo Stage 4: Plasma evolution, burning of arc Method: Particle-in-Cell (PIC) Feedback: Electron & ion & cluster emission ions Feedback: Energy & flux of bombarding ions Stage 5: Surface damage due to the intense ion bombardment from plasma Metod: Arc MD Onset of plasma

37 May 2009 H. Timkó, CERN & HIP Achievements 1. Onset: direct field evaporation from surfaces and tips could be simulated 2. Plasma build-up: currently under development is a 1D PIC code (from MPG) that used a simplified model; now we are modelling the experimental DC setup including All possible collisions, experimental and simulated sputtering yields, secondary electron yield Dynamic field emission and erosion of the tip 3. Cratering: using PIC input (flux & energy distribution of incident ions), erosion and sputtering was simulated Comparing arc plasma bombardment and thermal heating, we found that: -  threshold, corresp. to the melting point -Only in the case of plasma bombardment we see a heat spike & cluster emission above the threshold and experimentally seen complex crater shapes can form threshold

Comparison between effect of thermal heating and ion bombardment on surface – same amount of energy but different mechanism

Breakdown diagnostics Jan W. Kovermann The connection between simulation and experiment Emitted currents -Dark current spectrum -OTR -X-rays -Trigger mechanism -Missing energy -Breakdown rate -Ion currents -Fowler-Nordheim distribution Plasma characteristics -Time structure -Physical dimension (imaging) -Ion species (opt. spectroscopy) -Ion currents -Vacuum behaviour Surfaces -Crater morphology -Material diagnostics -Fatigue process

Breakdown diagnostics Jan W. Kovermann Breakdown diagnostics: some results RFDC OTR (Copper) Opt. spectroscopy Found Cu I, Cu II, Cu III ions Will be measured soon at

Breakdown diagnostics Jan W. Kovermann Breakdown diagnostics: further measurements RFDC RF (I,Q), Xray, Current, voltage and delay SEM of single breakdowns