Anti e-Cloud Coatings “AEC'09” topical workshop on organized by EuCARD-AccNet-EuroLumi Summary for SPSU
Download ReportTranscript Anti e-Cloud Coatings “AEC'09” topical workshop on organized by EuCARD-AccNet-EuroLumi Summary for SPSU
topical workshop on Anti e-Cloud Coatings “AEC'09” http://indico.cern.ch/conferenceDisplay.py?confId=62873 organized by EuCARD-AccNet-EuroLumi http://eucard.web.cern.ch/EuCARD/index.html Summary for SPSU by Mauro Taborelli http://accnet.lal.in2p3.fr/ and SPS Upgrade Study Team http://paf-spsu.web.cern.ch/paf-spsu/ TiN as alternative? -TiN is good if conditioned in the lab (SEY=0.85), but also other materials have similar performance -The best value presented with moderate conditioning (air exp. time unknown) is SEY=1.2 for 10-5C/mm2 -TiN is good if conditioned in machines with photons (KEKB, SLAC…ions not quantified) -Degassing only slightly higher than Cu, improves with very moderate bake out (80C) KEK TiN 04Nov2008 4 10 -3 Near Beam Electron Cloud Density [m ] 11 D(D7)[4,200,3]Cu D(D7)[4,200,3]TiN D(D7)[1,1585,3.06]KEKTiN In KEK LER Copper 11 3 10 K. Kanazawa 11 2 10 TiN (KEK) 11 1 10 0 0 0.2 0.4 0.6 TiN 0.8 (BNL) LER Bunch Current [mA] Shibata 1 1.2 Conditioning in the lab: (S.Kato, KEK) As received state Dose of irradiation in the lab at 5KeV electrons S.Kato S.Kato After a strong conditioning by an e-beam almost everything is good Data consistent with other labs (CERN, SLAC) Carbon coatings: DLC as alternative to a-C? - it is worse than a-C (not the best DLC according to S.Kato, SEY=1.1 if sputter cleaned), sp2 is relevant -DLC is not simple: SiC or Cr adhesion layer+ stress releasing layer with DLC on top -ESD is better than Cu -no air exposure study As received surfaces KEKB 11 4 10 Electron Cloud Density [m -3] Cu (1400Ah) 11 Kato DLC 3 10 Graphitized Cu (1740Ah) K. Kato and M. Nishiwaki 11 2 10 NEG Coated Cu (1370Ah) 11 1 10 DLC (1980Ah) TiN Coated Cu (1094Ah) 0 0 0.2 0.4 0.6 0.8 LER Bunch Current [mA] 1 1.2 EM-study-FUJI[4-200-3]Cu-DLC.qpc S.Kato Conditioning of uncoated surfaces Why does StSt condition to 1.5-1.6 in SPS and to 1.1 in the lab? No difference for Cu in lab and KEKB KEKB Laboratory 0.6C/mm2 S.Kato S.Kato Conditioning in SPS SPS transfer sample (StSt) Measurements in situ on copper (N.Hilleret) ~1.4 Copper (N.Hilleret) Cu, LHC type beam in SPS, measured in situ Photons Cu lab conditioning Low SEY by rough surfaces (apart of grooves) Chemically prepared rough surfaces -SEY =1.2 at 800eV, SEY=1 at 400eV -Rough is OK in UHV only if we can bake to reduce outgassing -The surface is mechanically fragile (adhesion?) -Impedance? With insulating particles - SEY<1, higher above 800eV -Fundamental research necessary, principle still not understood -Would impedance hinder any application or can it be optimized? I.Montero 2,0 Al2O3 particle Al2O3 75%+Al 25%+Au 1,8 Al2O3 50%+ Al 50% +Au 1,6 SEY coefficient Al particle SEY Gold coated Al2O3 25%+ Al 25% +Au 1,4 1,2 1,0 0,8 0,6 0,4 0,2 0,0 0 200 400 600 Primary Electron Energy (eV) 800 1000 Surface top view Magnetically rough surfaces: -The best results are only for Au coated particles: is there more than the magnetic field effect or Au is “cutting off” the peak at low energy ? -Are there ideal values of magnetization, domain size and orientation? -Probably only for field free regions Au coated ferrite microparticles (topographic+magnetic roughness) Coated (blue) and uncoated (red) particles SEY 1.2 1.60 1.0 1.40 SEY coefficient SEY coefficient 1.20 1.00 0.80 MnZn/Cu 0.60 0.8 0.6 Ferrita+Au-312º 0.4 NiZn/Cu +Au Ferrita+Au-342º Ferrita +Au-300º 0.40 Ferrita +Au-352º 0.2 0.20 0.00 Ferrita +Au-352º 0.0 0 500 1000 1500 2000 2500 3000 Primary Electron Energy (eV) 3500 4000 0 200 400 600 Primary Electron Energy (eV) 800 1000 Simulation of one side of the chamber with low SEY (G.Rumolo) Keep in mind this if we put the grooves =1.50,Height=1.9mm, =20 0 0 2 1.8 1.6 Flat surface r=0.14mm,B=2 Tesla r=0.14mm,B=0.2Tesla r=0.09mm,B=2 Tesla r=0.09mm,B=0.2Tesla average,B=2 Tesla SEY 1.4 1.2 1 0.8 0.6 0.4 Lanfa Wang, SLAC 0.2 0 100 200 300 400 500 Energy (eV) 600 700