Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 •...

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Review of high field Q slope, cavity measurements G. Ciovati Jefferson Lab 13 th SRF Workshop Oct. 15 th -19 th , 2007, Beijing, China

Transcript of Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 •...

Page 1: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Review of high field Q slope, cavity measurements

G. CiovatiJefferson Lab

13th SRF WorkshopOct. 15th-19th, 2007, Beijing, China

Page 2: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Tools

• Research on Q-drop and baking in Nb cavities is typically carried out on 1.3 GHz and 1.5 GHz single-cells

1.5 GHz CEBAF Shape

1.3 GHz Ichiro Shape

1.3 GHz TESLA Shape

Page 3: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Introduction• Typical Q0(Bp) curve for high-purity bulk niobium L-band cavities

Bp

Q0

90-100 mT

• High field Q-slope (or Q-drop): exponential increase of RF losses with no X-rays (field emission). First observed in 1997.

• In 1998 it was found that a low-temperature (100 – 140 °C, 48 h) bake strongly reduced the Q-drop

BCP, EP

Baking

Page 4: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Temperature maps

1

4

7

10

13

16

19

22

25

28

31

34S1

S3S5

S7S9 S1

1 S13 S1

5

0

0.02

0.04

0.06

ΔT (K)

AzimuthBottom I i

Top Iris

Equator

Q0 = 1.01 1010

Eacc = 8.7 MV/m

1E+09

1E+10

1E+11

0 15 30 45 60 75 90 105 120

Bp (mT)

Q0

T=1.7 K

• Temperature mapping show “hot-spots” in the equator region

JLab system: 576 carbon resistors, based on Cornell design1

1J. Knobloch, Ph.D. Thesis, Cornell University, 1997

G. Ciovati, JLab

Page 5: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Role of surface roughness

• Polycrystalline Nb surfaces obtained by buffered chemical polishing (BCP) are in general rougher than obtained by electropolishing (EP)

5-10 μm with BCPRMS step height: 1-5 μm with EP R.L. Geng et al.-SRF 99-TUP021

Quenches of grain boundaries when βmH > Hc

• Magnetic field enhancement model:

J. Knobloch et al.-SRF 99-TUA004

Page 6: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Nevertheless:

• Low temperature baking improves Q-drop without changing surface morphology

170 mT

BCP treated cavity (4÷8 μm step height)

B. Visentin et al.-EPAC 02-THPDO013

Exp. results against surface roughness (1)

Page 7: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

• The equator weld is typically the region of the cavity with morepronounced steps, yet the Q-drop occurs also in seamless cavities

R.L. Geng et al.-SRF 99-TUP021

SEM photo of typical EBW

1E+09

1E+10

1E+11

0 50 100 150

Bp (mT)

Q0

55V Anodization

120 C/3 h UHV bake

Cavity 1K2

Hydroformed, EP cavity

P. Kneisel, JLab

• The Q-drop occurs in cavities smoothened by barrel polishing and EP

Courtesy T. Saeki

Exp. results against surface roughness (2)

Page 8: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Role of the oxide layer• Niobium is naturally covered by a dielectric amorphous Nb2O5 layer (3-5 nm

thick) on top of a transition region (NbOx x ∼ 0.5 ÷ 2 suboxides) with metallic character

• Interface tunnel exchange model:

Band structure at Nb-NbOx-Nb2O5-y interfaces

Resonant energy absorption by quasiparticles in localized states in the oxide layer.

Driven by electric field* *

rRFE

e zεβ

Δ>

1E+09

1E+10

1E+11

0 50 100

Bp (mT)

Q0

T=1.37KITE Fit

109

1010

1011

J. Halbritter - SRF 03 - MoP44

Page 9: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Exp. results against oxide layer (1)

• UHV baking effect stable after re-oxidation (air exposure for 2 months and HPR, HF rinse)

B. Visentin - SRF 03 – TuO01

C1-03 ( EP @ KEK - Tests @ Saclay)E5 : after baking 120°C/60h

I1 = E5 + air exposure 46 months+ 20' HF + HPR

1E+08

1E+09

1E+10

1E+11

0 10 20 30 40Eacc ( MV/m )

Q0

Test E5 - March 2000

Test I1 - January 2004

quench

B. Visentin – Frontier Workshop – p. 94

Page 10: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

• Results show Q-drop driven by magnetic, rather than electric, field

1E+09

1E+10

1E+11

0 20 40 60 80 100 120 140 160

Bpeak (mT)

Q0

TE011TM010TE011 after 120C 30h bakeTM010 after 120C 30h bake

T = 2 K

G. Ciovati and P. Kneisel, PRSTAB 9 (2006) 042001

1E+09

1E+10

1E+11

0 20 40 60 80 100 120 140 160 180

Bpeak (mT)

Q0

pi-mode 120C/48h bake0-mode, 120C/48h bake

T = 2 K

Ep=77MV/m

Ep=19MV/m

G. Ciovati, Ph.D. Thesis, Old Dominion Univ., 2005

Exp. results against oxide layer (2)

Page 11: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

• Anodization experiments show that the baking effect occurs within a ∼ 20 nm depth from the surface

Exp. results against oxide layer (3)

1E+09

1E+10

1E+11

0 15 30 45 60 75 90 105 120 135 150Bp (mT)

Q0

120C/12h bake

40V anodization

G. Eremeev and H. Padamsee, Physica C 441 No. 1-2 (2006) 62

G. Ciovati, P. Kneisel and A. Gurevich, PRSTAB 10 (2007) 062002

Page 12: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Role of grain size and chemical treat. (1)

• On BCP treated surfaces, the baking improves Q-drop on:– Post-purified fine-grain Nb (final grain size ∼ 1-2 mm)– Large grain Nb (cm-size)

1.00E+09

1.00E+10

1.00E+11

0 5 10 15 20 25 30 35

Eacc [MV/m]

Q0

T=1.37K T=1.37K, 120C 48hr bake

G. Ciovati-J. Appl. Phys. 96, p. 1591 (2004)

1E+09

1E+10

1E+11

0 20 40 60 80 100 120 140 160 180Bp (mT)

Q0

before bake

120C/9h bakeT = 1.7 K

Quench

G. Ciovati, P. Kneisel and A. Gurevich, PRSTAB 10 (2007) 062002

B. Visentin et al.- EPAC’06 – p.381.

Page 13: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Role of grain size and chemical treat. (2)

• Duration of 120°C baking on large-grain BCP cavities can be reduced to 12 h, while 48 h seems necessary for EP cavities

120°C/12h baked

1E+09

1E+10

1E+11

0 5 10 15 20 25 30 35 40Eacc (MV/m)

Q0

NingxiaHeraeusCBMM

T = 2 K

P. Kneisel, EPAC’06, WEXPA01

Bp=148mT

Z. G. Zong, PAC’07, p. 2143

Bp=155mT

Page 14: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Role of grain size and chemical treat. (3)

• Recipes necessary to overcome the Q-drop, depending on the starting material, based on current data:

Large grain/Single crystal niobium

Fine grain niobium

BCP EP

Titanization

120 °C/12 h UHV bake

120 °C/48 h UHV bake

Page 15: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Role of grain boundaries

• Regions of degraded superconducting properties due to preferential segregation of impurities such as O, H, C.

Exp. results:Large grain Fine grain

G. Eremeev and H. Padamsee, EPAC’06, p. 475

• Lower density of hot-spots has been observed in a large-grain cavity than fine grain• In a recent study, the statistic of 33 RF tests on the same large grain cavity showed that ∼ 30% of

hot-spots occurred within 1 cm from a grain boundary*

*G. Ciovati, P. Kneisel and A. Gurevich, PRSTAB 10 (2007) 062002

Page 16: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Role of interstitial oxygen

• High concentrations of interstitial oxygen (∼ 10 at. %) were found at the Nb/oxide interface

• Oxygen diffusion model:– Q-drop caused by local reduction of Hc1 due to high O

concentration

0

0.2

0.4

0.6

0.8

1

1.2

100 120 140 160 180 200

c(0, 48 h)u(0, 48 h)v(0, 48 h)

Oxy

gen

conc

entra

tion

(at.

%)

癈T ( )

Nb2O5

Suboxides (NbO2, NbO)

Interstitial oxygen

λ

Before baking

Oxide cluster

λ

After baking

G. Ciovati, Appl. Phys. Lett. 89 (2006) 022507

Page 17: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Data supporting oxygen diffusion (1)• Reduction of low-field RBCS for increasing baking temperature

and time (reduction of mean free path, increase of energy gap)

Saturation of RBCS reduction at ∼ 140°C, ∼ 48h measured on fine-grain Nb cavities

G. Ciovati, J. Appl. Phys. 96 (2004) p. 1591 P. Kneisel, SRF’99, TuP044

Page 18: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Data supporting oxygen diffusion (2)

• Q-drop onset increases for longer baking time

C1-16 ( EP )

1E+09

1E+10

1E+11

1E+12

0 10 20 30 40Eacc ( MV/m )

Q0

F1 - EPF2 - Baking 100°C / 3hF4 - Baking 100°C / 60h

quench

fieldemission

RFpower

B. Visentin, Pushing the Limits of SRF Workshop, 2004, p. 94

• Oxygen diffusion length at ∼ 120 °C/48 h compatible with RF penetration depth and anodization results

Page 19: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Data supporting oxygen diffusion (3)

• Baking in 1 atm Argon at 145°C/3h gives similar Q-drop improvement as 120°C/48h in UHV (similar oxygen diffusion depth)

B. Visentin, TTC Meeting, FermiLab, April 2007.B. Visentin, Y. Gasser, J.P. Charrier, Physica C 441 (2006) p. 66

Page 20: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Data contradicting oxygen diffusion (1)

• By baking in UHV at 400°C/2h, oxygen diffuses to depths > λand a thinner oxide layer (NbO) is left at the surface

• Hot-spots with high Rres and quadratic losses after baking• Hot-spots with Q-drop behavior still present

G. Eremeev and H. Padamsee, PAC’07, p. 2334

~ 1-3 mm grain size, vertical EP + flash BCP

Page 21: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Data contradicting oxygen diffusion (2)• Oxygen concentration near the surface and oxide layer thickness

were increased by baking at 120°C/12h in 1 atm O2 and in air up to 180°C a previously baked large grain cavity

T-map after 180°C/12h air bake

• Q-drop not restored after baking in pure O2 or air• High Rres and quadratic losses after 180°C air bake

G. Ciovati, P. Kneisel and A. Gurevich, PRSTAB 10 (2007) 062002

Page 22: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Role of the interface (1)

• In a systematic study* on the oxidation of a large grain cavity, it was found that baking and anodization affect the avg. value of the energy gap Δ over ∼ λ [Obtained from BCS fit of Rs(T, 12mT)]

• Typical value of Δ/kTc after chemical etching ∼ 1.75

Δ/kTc of pure Nb ∼ 2.01

• Baking for longer time increases Δ/kTc up to ∼ 1.95• Anodization at higher voltages reduces Δ/kTc down to ∼ 1.75

*G. Ciovati, P. Kneisel and A. Gurevich, PRSTAB 10 (2007) 062002

Page 23: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Role of the interface (2)

• A correlation between Δ and Q-drop-onset/Quench-after-baking was found to be consistent with thermal feedback model*

02

0kT

b bH H eΔ−Δ

=

Dependence of breakdown field# Hb on Δ:

*A. Gurevich, Physica C 441 (2006) p. 38

#“Defect free” case

Hb0 ≅ critical field

Δ0 ≅ gap of pure niobiumG. Ciovati, P. Kneisel and A. Gurevich, PRSTAB 10 (2007) 062002

Hb: breakdown of the Meissner state

Page 24: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Hot-spots and thermal feedback• Thermal feedback for uniform Rs

does not reproduce the Q-drop• Introducing “hot-spots” (regions of

higher dissipation) makes it workH(t)

TTm

T0Ts

coolant

xd

Hot-spot

( )

( )( )

22

20

00 2

0

21 1 4

0

1 1

p

b

p b

Bg u g u u

B

Q eQ

g B B

θ−

= + + − + + −

=⎡ ⎤+ −⎢ ⎥⎣ ⎦

2h hg N Lη π=

3 fit parameters:

Q0(0) Bb0A. Gurevich, Physica C 441 (2006) p. 38

Page 25: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Conclusions (1)

Experimental results on Nb cavities show that:μm-scale surface roughness

– Nb2O5 oxide layer– Grain boundaries

The optimal baking procedure seems to depend on the metallurgical state (large-grain vs. fine-grain) and surface treatment (EP vs. BCP)

Do NOT play a dominant role in causing the Q-drop

Page 26: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Conclusions (2)

Q-drop and baking effect are related to changes up to a depth ∼ 20 nm from the outer surface (interface?)– A good amount of data indicates interstitial oxygen

diffusion as the mechanism involved during baking but recent results are in contradiction

– Oxygen is the impurity that has been looked at more systematically. The role of hydrogen (high concentration near the surface) is not quite clear

Q-drop is driven by high magnetic fieldSurface treatments which affect the energy gap also affect the Q-drop onset and the quench field after baking

Page 27: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Conclusions (3)

The introduction of regions with higher dissipation (“hot-spots”, observed experimentally) in a thermal feedback model gives a good description of Q0(Bp) curve. The same type of model explains the correlation between energy gap and “breakdown field” which leads to either Q-drop or quench depending on the thermal stability of the cavity

↓ Δ

↑ Δ

↓ Hb0 ↑ Hb0

Q0

Bp

Page 28: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Conclusions (4)

We have a good-working model which describes phenomenological aspects of Q-drop and baking effect

It is not yet clear what physical entity is involved. In principle this should be easier to discover by surface analytical methods…

Let’s hear about it in the next talk!

Page 29: Review of high field Q slope, cavity measurementsG. Eremeev and H. Padamsee, EPAC’06, p. 475 • Lower density of hot-spots has been observed in a large-grain cavity than fine grain

Acknowledgements

G. Eremeev, A. Gurevich, P. Kneisel, G. Myneni, H. Padamsee, T. Saeki, B. Visentin

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