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CERN Studies on Niobium-Coated 1.5 GHz Copper Cavities

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Presentation on theme: "CERN Studies on Niobium-Coated 1.5 GHz Copper Cavities"— Presentation transcript:

1 CERN Studies on Niobium-Coated 1.5 GHz Copper Cavities
Sergio Calatroni C. Benvenuti M. Hakovirta H. Neupert M. Prada A.-M. Valente

2 Motivation for the study: the high-field residual resistance
Outline of the talk Motivation for the study: the high-field residual resistance Thermal effects Surface defects and roughness Role of the grain size and purity Hydrogen studies: RF measurement Thermodynamics Conclusions Sergio Calatroni - CERN

3 Motivation: the high-field residual resistance
Coatings performed using krypton on electropolished spun copper cavities (Santa Fe 1999) Limited by RF power Sergio Calatroni - CERN

4 Testing: higher field operation
The performance can be extended straightforwardly at higher fields Limited by RF power (250 W) (Thermal instability of the standard small cryostat is not a limiting issue) Sergio Calatroni - CERN

5 Testing: thermal effects
In Nb/Cu cavities we must cope with several thermal impedances: Cu/He (~6000 W/m2K), across Cu (negligible), Nb/Cu interface (?), across Nb film (negligible) If the Rs increase would only be due to some heating of the film -> RBCS It is then possible to estimate the temperature increase that corresponds to the measured Rs increase. The dissipated power is also easily calculated A Kapitza-like mechanism would give a straight line in the plot Sergio Calatroni - CERN

6 Surface defects & roughness
2.0 µm 2.0 µm Chemically polished copper average roughness: 0.2 mm pinholes of 0.3 mm Electropolished copper average roughness: 0.02 mm nearly no defects Sergio Calatroni - CERN

7 Surface defects: measurement of pinholes
Irregularities on the substrate surface shadowing effect film inhomogeneities He leak rate experiment ‹inc› fraction of leaky film surface - equator 9° ppm - (~iris ° 25 ppm) - equator 9° ppm CP EP Substrate disk Machining and cleaning Film deposition Substrate removal p1 p2 film Sergio Calatroni - CERN

8 Copper roughness I: electropolishing
The window of optimum polishing parameters is rather narrow. Reproducing these parameters over the entire surface of the cavity cell needs further R&D Production of O2 bubbles! Production of Cu(OH)2 on the surface! Sergio Calatroni - CERN

9 Copper roughness II: electropolishing
Electropolishing parameters: 55% vol. H3PO4 45% vol. butanol Current density: 200A/m2 HP water rinsing Electropolishing with a quasi-homotetic cathode has replaced chemical polishing (LEP standard) for surface preparation. Sergio Calatroni - CERN

10 Copper roughness III: electropolishing
current density is 5 times larger at iris current density is identical The electropolishing cathode is being optimised by means of a sophisticated computer simulation code. The current density can be made uniform Sergio Calatroni - CERN

11 Intrinsic film roughness & incidence angle of the niobium atoms
10 20 30 40 50 60 70 80 degrees mm 50 mm 0 mm Sergio Calatroni - CERN

12 Intrinsic film roughness: incidence angle and residual resistance
An issue which is of great interest also for low-ß cavities, is the correlation between the incidence angle of the film and the residual resistance Sergio Calatroni - CERN

13 Digression: new ideas for low-beta cavities coating
Nb ring Cu half-cell Problem: coating incidence angle in low-beta cavities Solution: coat at favourable angle before welding Sergio Calatroni - CERN

14 Recall: standard and oxide-free coatings
Sergio Calatroni - CERN

15 Properties of the coatings I : grain size with FIB micrographs
Standard films Oxide-free films 0.5 µm 0.5 µm Courtesy: P. Jacob - EMPA Sergio Calatroni - CERN

16 Properties of the coatings II: purity, Hc1, texture, etc...
Standard Oxide-free RRR ± ± 0.9 TC ± 0.01 K ± 0.04 K Ar cont ± 70 ppm ± 43 ppm Texture (110) (110), (211), (200) Hc ± 3 mT ± 5 mT Hc ± 0.1 T ± 0.05 T a (10)Å (6) Å Da/a ± % ± % Stress ± 56 MPa ± 78 MPa Grain size 110 ± 20 nm > 1 µm Sergio Calatroni - CERN

17 Properties of the coatings III: effect on residual resistance
OX: oxidised copper substrate OF: oxide-free copper substrate CP: chemical polishing EP: electropolishing Oxide-free films (larger grains, better purity, less stress, etc...) have on average a larger residual resistance (measured at low field) In contrast with models linking the residual resistance with Josephson dissipation at grain boundaries Sergio Calatroni - CERN

18 Hydrogen studies I: film loading
Spun cavities coated using argon as sputter gas loaded with 1.4 at.% of hydrogen Hydrogen loading induces a much larger degradation for oxide-free films Sergio Calatroni - CERN

19 Hydrogen studies II: outgassings
Question: why were coatings on oxide-free hydroformed cavities consistently worse than for spun cavities? (Legnaro 1997) Possible answer: a larger quantity of hydrogen was migrating into the film from the hydroformed cavity Sergio Calatroni - CERN

20 Hydrogen studies III: outgassings
Bare Cu The hydrogen content and has been measured also by thermal outgassing to 350 ºC, for passivated and non-passivated Nb films (i.e. NbxOy at the surface) Oxidised copper: 2200±200 ppm 800±200 ppm Oxide free: 2000±200 ppm 980±200 ppm Sergio Calatroni - CERN

21 Hydrogen studies IV: isosteres
Oxidised copper pH2(cH)2exp(-EH/kT) The hydrogen content and its binding energy with the lattice can be measured with isosteric cycles and successive injections of known quantities of hydrogen. Oxidised copper: 400±200 ppm 340±10 meV/at Oxide free: 1000±200 ppm 320±10 meV/at Sergio Calatroni - CERN

22 HPWR effectively reduces Rres0 (1999 result)
Digression: HPWR I Nb/Cu film on CP copper HPWR effectively reduces Rres0 (1999 result) Sergio Calatroni - CERN

23 Digression: HPWR II Before HPWR After HPWR 10 µm 10 µm
Bulk Nb - EP with KEK bath HPWR smoothens the grain boundaries (2001 results) Sergio Calatroni - CERN

24 Conclusions The maximum field of Nb/Cu cavities is not limited by any intrinsic phenomena. However, the residual resistance suffers from a steep increase at high field (threshold ~15 MV/m). Several possible causes have been investigated. The most probable sources are: surface defects, hydrogen content. Possible cures are: better electropolishing (under way), reducing hydrogen content (difficult). Coating for low-beta cavities are being addressed with a suitable modification of the sputtering technique. Sergio Calatroni - CERN


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