1Claire AntoineCEA/Saclay - Fermilab (Innovative) Processing of materials SRF materials Workshop Fermilab May 23-24, 2007 Today’s process is long, complex,

Slides:



Advertisements
Similar presentations
The Continuing Role of SRF for AARD: Issues, Challenges and Benefits SRF performance has been rising every decade SRF installations for HEP (and other.
Advertisements

Superconducting Materials R&D: RRCAT-JLAB Collaboration S B Roy Materials & Advanced Accelerator Science Division RRCAT, Indore Collaborators: M. K. Chattopadhyay,
- Motivation - Cleaning mechanism, technique & apparatus - Nb cavity results - Copper rf gun cleaning - Summary, open topics + next steps Detlef Reschke,
R&D For Accelerating Structures H. Padamsee. TESLA Niobium, one meter length, rf = 1.3 GHz Copper, 53 cm, rf = 11.4 GHz.
ECR Deposition of Niobium 10/09/2006 Thin Films and new ideas for pushing the limits of RF superconductivity 1 ECR Deposition of Niobium ECR plasma principle.
PEALD/CVD for Superconducting RF cavities
Thin Films for Superconducting Cavities HZB. Outline Introduction to Superconducting Cavities The Quadrupole Resonator Commissioning Outlook 2.
Cavity package T.Saeki BCD meeting 20 Dec Cavity shape BCD: TESLA shape Pros: small wakefield, HOM thoroughly investigated single-cell: 43 MV/m.
ILC PM Meeting S0 Webex Global Design Effort 1 S0/S1 Next Steps Lutz Lilje GDE.
Superconducting RF Materials University Collaboration STATUS Lance Cooley June 07, 2010.
Cavity status; recent KEK activities : Hayano (1) STF CM-1 cavities are; MHI-014: 3-rd VT:36MV/m (finished) MHI-015: 3-rd VT: > 18.4MV/m.
R EVIEW ON Q - D ROP M ECHANISM B ernard V ISENTIN International Workshop on Thin Films 9 th - 12 th October 2006.
Americas S0 Plan in USA Shekhar Mishra Fermilab/GDE US Main Linac Cavity and Cryomodule WBS.
Surface Preparation of superconducting cavities and industrial Production Experience Dietrich Bloess International Workshop on Thin Films applied to superconducting.
Mechanical Issues SPL cavities/cryomodules Workshop CERN 30 Sep. 2009
EuCARD Task 10.4 Sergio Calatroni. Sub-task New and improved techniques for the production of Nb sputtered Quarter Wave (QW) cavities (CERN, INFN-LNL)
Deposition of Pure Lead Photo-Cathodes by Means of UHV Cathodic Arc
High Q R&D at JLab G. Ciovati, P. Dhakal, R. Geng, P. Kneisel, G. Myneni TTC Topical Meeting on CW SRF Cornell Univ., June 12 th -14 th, 2013.
CAVITY TREATMENT (BCP, HEAT TREATMENT & HPR) Sergio Calatroni with many contributions from: Rama Calaga, Leonel Ferreira, Antonio Mongelluzzo LHC CCEM,
Achievement of 41 MV/m Gradient by AES8 Rong-Li Geng Jefferson Lab ALCPG09, October 1, 2009.
CERN status - Nb cavity – Manufacturing 1 15/Nevember/2010, Ofelia Capatina EN/MME 1 SPL Cavity Working Group Meeting TaskExternal Company CERN Provide.
R.L. Geng, 5/27-31,2013 ECFA LC2013, DESY 1 Update on Raising Q0 at Ultra-High Gradient via Large-Grain Niobium Material Rongli Geng Jefferson Lab ECFA.
Center for Materials for Information Technology an NSF Materials Science and Engineering Center Substrate Preparation Techniques Lecture 7 G.J. Mankey.
Q-Slope at High Gradients ( Niobium Cavities ) Review about Experiments and Explanations Bernard VISENTIN CEA - Saclay.
SRF Processing at ANL: Progress and Plans ANL: Mike Kelly, Scott Gerbick FNAL: Dan Olis, Allan Rowe Speaker: Mike Kelly November 17, 2008.
Advances in Large Grain Resonators Activities of DESY, W.C. Heraeus and RI material and fabrication aspects preparation and RF test results W. Singer,
Americas Cavity Specification C.M. Ginsburg (Fermilab) On behalf of the Fermilab cavity crew October 20, 2010.
ANL/FNAL/UC Collaboration meeting 27 June 2008 SRF Materials: First Acceleration Test of Coated Cavities Pellin 1, Zasadzinski 2, Proslier 1,2, Norem 3,
CRAB for HL-LHC KEK activity 2010DEC Yoshiyuki MORITA.
Superconducting rf test facility LCWS 2010 in Beijing, 28 Mar 2010, Ken Watanabe Replica-method and local grinding repair K. Watanabe (KEK) LCWS 2010 in.
LHC vacuum chamber dust High Pressure pure water rinse –Developed at CERN for LEP sputtered SCRF NEG Coating –Most likely must be re-applied Nozzles and.
Update on S0 Work in the Americas Region Mark Champion 17 June 2008.
Lutz Lilje DESY -MPY- Summary of the Superconducting RF WG DESY -MPY Overview on talks given List European Assets.
CLIC09 WG4 RF Structure1 Engineering Perspectives on Quadrants (2) CLIC09 Workshop KEK Y.Higashi.
ALCPG2011, 3/19- 23, SRF Group Institute of Heavy Ion Physics, Peking University ALCPG /3/19-23, Eugene, Oregon, USA RF superconducting Cavity.
Peking University Improvement of Multilayer Film Growth for Accelerator Cavity by ECR deposition Jiao, Fei.
How important is the surface finish/roughness in determining the performance of Nb cavities? Introduction Peter Kneisel Jlab.
High Temperature Heat Treatment to Raise the Quality Factor of Large Grain Niobium Cavities Pashupati Dhakal Gianluigi Ciovati Ganapati Rao Myneni July.
Centrifugal Barrel Polishing at Fermilab (Tuesday, December 6th at 10:20) Tesla Technology Collaboration IHEP, Beijing December 5 th -8 th, 2011.
Annual Meeting CERN - November 2005 Bernard V ISENTIN.
W. Singer. SRF2011, July 25 ‐ 29, 2011, Chicago, Illinois, U.S.A. XFEL Cavity Recipe for Mechanical Fabrication and Treatment Waldemar Singer/DESY.
State of ECR Plasma Test & Measurement of Ferrite Materials Permittivity Summer student meeting August 27, 2007 Ivan Pechenezhskiy, MIPT. Supervisor: Genfa.
1 Guided Cavity Repair with Laser, E ‐ Beam and Grinding Genfa Wu Recent cavity processing statistics indicate that the development of RF superconductivity.
Field emission in SRF Cavities
RF Superconducting Materials Workshop at Fermilab, May 23 & 24, 2007 Advanced Nb oxide surface modification by cluster ion beams Zeke Insepov, Jim Norem.
Surface Resistance of a bulk-like Nb Film Sarah Aull, Anne-Marie Valente-Feliciano, Tobias Junginger and Jens Knobloch.
Rongli Geng ILC Cavity Group Meeting October 25, 2011
Pulsed Energetic Condensation of Nb Thin Film Cavities at JLab
Electropolishing of Dressed ILC 9-cell Cavity
Condition of electron beam welding toward a high gradient application
ILC-SCRF Test Facilities considerations
Energy (ILC) and Intensity (Project X) SRF Cavity Needs
New Cavity Techniques and Future Prospects
JLab infusion and LG flux expulsion update
State of the Art and Future Potential of Nb/Cu Coatings
Peng Sha Institute of High Energy Physics, CAS
Fabrication of Nb and Cu SPL cavities and required tools CERN status
High Q via N infusion R&D at Jefferson Lab
THE HIE-ISOLDE SUPERCONDUCTING CAVITIES:
Superconducting Cavities: Development/Production
Some History of Electropolishing of Niobium 1970 – 1990
A COMMON R&D ON THE HIGH GRADIENT Nb CAVITIES
R&D Activity for Field Emission and Vertical EP
P. Maesen for CERN BE/RF-SRF team
Working Group 3 Summary TTC Meeting INFN Milan,March 3, 2011
Future Thin Film Deposition Efforts at FNAL
Performance of Large Grain TESLA cavities
ON THE HIGH GRADIENT Nb CAVITIES
SRF Surface Studies and the High Field Q-slope Mystery
SRF Science and Technology
Presentation transcript:

1Claire AntoineCEA/Saclay - Fermilab (Innovative) Processing of materials SRF materials Workshop Fermilab May 23-24, 2007 Today’s process is long, complex, expensive … and not very efficient

2Claire AntoineCEA/Saclay - Fermilab Why do we need to process the cavities ? 1) Getting a “good” superconductor OOPS !? What is a good SC ? Empirically inferred with time: Good thermal conductivity (need to use high RRR material) EB-welding, in very good vacuum (Nb = good getter!) Low interstitials (don’t anneal in poor vacuum, avoid hydrogen…) No damage layer ? (need to chemically remove  m of the surface before achieving “good performances”) No inclusion (metallic inclusion = hot spot for sure !) Smooth surface ? (EP better than BCP) …. ? Other suspects : surface oxides, chemical residues, grain boundaries, adsorbed layers,…

3Claire AntoineCEA/Saclay - Fermilab Damage layer:  m Origin: previous mechanical history (rolling, deep drawing/spinning…) Not controlled yet, batch to batch variations Various recipes tried: Chemical etching (BCP) Quick, efficient, reproducible… but rough surfaces But : ~ 30 MV/m Problem = roughness near the weld area ? Alternative solutions: monoXstals, hydroforming (no welding seam, no roughness!) Electropolishing (EP) Slow, expensive, higher risk of H contamination Gives the best results:  40mV/m Lack of reproducibility (aging of solution, chemical residues… ?) Alternative EPs under study … BCP+ EP: need to remove ~ 100  m (EP) to achieve smooth surface Barrel polishing (mechanical) + BCP/EP: need to remove ~ 100  m (EP) to get rid of the damage layer… Ideal surface processing: removes 200  m of internal surface no damage layer, no roughness no chemical contamination (e.g. hydrogen)…

4Claire AntoineCEA/Saclay - Fermilab Why do we need to process the cavities ? 2) Get a dust free surface to prevent filed emission (high electric field regions = cavities’ irises) Emitting sites = dusts, scratches Dust particles gather and weld together and to surface Local enhancement of E =>   E Field emission is the main practical limitation in accelerator operation  ~ 3  ~ Ni particles

5Claire AntoineCEA/Saclay - Fermilab Detail of the usual process(1/2) Forming WHY COMMENT EB welding Clean welding Nb = getter. Degraded weld => Q 0 /10 Ti purification Deep etching Increase RRRRRR now commercially available BCP EP Remove damage layer ( µm) BCP limited to ~ 30MV/m; EP => >40 mV/m but lack of reproducibility 800°C annealing Remove Hydrogen contamination hydrogen source : wet processes Hydrogen segregates at the surface and form hydrides (poor SC) Diffusion layer < ~1µm Light etching Remove diffusion layer (O, C, N)

6Claire AntoineCEA/Saclay - Fermilab Detail of the usual process(2/2) WHY COMMENT HPR HF, H 2 O 2, ethanol, degreasing,… Fight field emission gt rid of S (after EP) …Special rinse …Light etching Get rid of dust particlesMost convenient, but not sufficient Ancillaries: couplers antennas… In clean room. But re-contamination still possible Baking, 120°C, 48h Get rid of the high field losses (Q-drop) Mechanism not understood, concerns the first 10 nm of the material assembly Post processing Get rid of dust particles Due to assembly Under development Ex: dry ice cleaning, plasma RF test He processing, HPP Field emissionField emission: SRF accelerator plague !

7Claire AntoineCEA/Saclay - Fermilab High pressure rinsing (HPR) 1/2 ultra pure H 2 O, ultra filtered, bars (Droplets) (Flow) FeFe v f ~ 160 m/s FeFe 100 bars Particles are displaced when F e > F ad

8Claire AntoineCEA/Saclay - Fermilab High pressure rinsing (HPR) 2/2 HPR is due to mechanical effect of the droplets F e is high enough to deform Nb (  l Nb ~ MPa ) post contamination after HPR is still possible HPR is not very efficient on S particles after EP (S embedded in organic material ?) Before HPR After HPR [M. Luong, PhD, 1998]

9Claire AntoineCEA/Saclay - Fermilab RF post processing : He processing & HPPP Helium processing Developed CERN Helium gaz + RF => plasma Low efficiency, mainly low field High Peak Power processing (HPP) Concept Cornell: burning out particles at high field Pulsed RF to prevent quench High power klystron or adjustable coupling (expensive) High risks: limitations of the couplers, creation of stable emitters Advantage: in situ, after assembly [H.Padamsee et al., RF superconductivity for accelerators, 1998]

10Claire AntoineCEA/Saclay - Fermilab High Peak Power processing (HPP) [1] A. Boechner et al., Proc. of EPAC06, p413, 2006 [2] W-D. Moeller et al., Proc. of EPAC96, p2013, 1996 HPP in a Cryomodule at ELBE, Rossendorf [1] HPP for C19 at DESY [2] For ILC: 10MW (1.565mS) klystron and 1MW power coupler. Q ext = 3.5x10 -6 Power could be available but needs re- configuration of RF distribution (expensive!!!) HPP power and field in Tesla 9-cell cavity SC=>long pulses to compensate filling time Need for high power or adjustable couplers Need for high power Klystron Was never tested for field higher than 25 MV/m (no power source available until recently) Reliability and thermal load issues

11Claire AntoineCEA/Saclay - Fermilab Other post processing Advantage: applicable in situ, after assembly Dry ice cleaning DESY Carbonic snow => residuals = CO 2 Mechanical effect, similar to HPR Applicable on horizontal cavities In situ ECR plasma cleaning FNAL Applicable on equipped cavities: usual antennas, RF source Need for a valve + external magnet, no internal parts Cleaning of particles/surface layers by plasma Possible post/ (dry) oxidation to protect surfaces ECR = electron cyclone resonance [courtesy of D.Reschke, DESY] [courtesy of G. Wu, FNAL]

12Claire AntoineCEA/Saclay - Fermilab Coating as a bulk niobium cavity treatment 1.M. J. Sadowski et al., The Andrzej Soltan Institute 2.A-M. Valente et al., JLAB 3.S. Calatroni, CERN Standard Nb coating methods: Electron cyclotron resonance plasma deposition 2 Vacuum Arc deposition 1 Concept: overlay bulk Nb defects by a “good”, very pure Nb layer, no wet process. Drawback : thin layers are usually less good than bulk Nb Advantage: substrate = Nb => annealing (recrystallization) = possible Other drawback : post contamination still possible (complex assembly/re-assembly process) Biased magnetron sputtering 3

13Claire AntoineCEA/Saclay - Fermilab Other possible processing methods: Laser, electron or ion beam irradiation: Recrystallization of the surface, vaporization of defects, particles Non-HF wet chemical etching, polishing, other recipes… To replace EP Alternative rinsing (for S, organic contamination, EP specific) US degreasing Ethanol rinsing H 2 O 2 UV ozone Plasma processing/etching Electrohydrodynamic cleaning (corona plasma) Ion beam Ion cluster beam etching… Ultrasonic, megasonic Better cleaning of sub micron particles Field emission +

14Claire AntoineCEA/Saclay - Fermilab Conclusion Deep etching cannot be prevented, but better definition/specifications of the material could help to reduce it. Final treatment should produce smooth surface and be able to get rid of chemical residues as well as dust particles. In situ post processing should be developed since recontamination during assembly is still possible. Processing of ancillaries parts should also be addressed. New ideas are awaited