Research for SRF Cavities T. Tajima, G. Eremeev*, M. Hawley, R. - - PowerPoint PPT Presentation

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Research for SRF Cavities T. Tajima, G. Eremeev*, M. Hawley, R. - - PowerPoint PPT Presentation

Update on MgB 2 Thin Film Research for SRF Cavities T. Tajima, G. Eremeev*, M. Hawley, R. Schulze, LANL J. Guo, S. Tantawi, V. Dolgashev, D. Martin, C. Yoneda, SLAC B. Moeckly, Superconductor Technologies, Inc. (STI) I. Campisi, ORNL TTC


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U N C L A S S I F I E D

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Update on MgB2 Thin Film Research for SRF Cavities

  • T. Tajima, G. Eremeev*, M. Hawley, R. Schulze, LANL
  • J. Guo, S. Tantawi, V. Dolgashev, D. Martin, C. Yoneda, SLAC
  • B. Moeckly, Superconductor Technologies, Inc. (STI)
  • I. Campisi, ORNL

TTC Meeting, FNAL, Batavia, IL, USA, 19-22 April 2010

LA-UR-10-02476

*Presently at JLab

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U N C L A S S I F I E D

We are trying to demonstrate Gurevich’s multi-layer superconductor proposal

Simple single layer example

Assumptions Hc1(Nb) = 170 mT λL(MgB2) = 140 nm ξ(MgB2) = 5 nm

Hc1(MgB2) = 355 mT

d = 105 nm

The film thickness needs to be determined so that the decayed field at the Nb surface is below the RF critical field of Nb (~200 mT). H0 = 355mT Hi = 170mT d = 105 nm

Nb MgB2 Eacc ~ 100 MV/m

Dielectric material

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U N C L A S S I F I E D

2-inch disk experiments have been carried out at SLAC using a 11.4 GHz 50 MW Klystron to generate short pulses (≤ 2 µs) and a TE013-mode copper hemispheircal host cavity

2 inches (~50 mm)

Currently: Pulse width 1.6 µs Rep rate 1 Hz

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U N C L A S S I F I E D

The RF breakdown (quench) normally starts on the ring at half radius where the surface magnetic field peaks

Typical distribution of superconducting and normal- conducting regions after quench

surface sample

/R G Q Sample 

  • The cavity Q starts to

decrease when part of sample quenches

  • One can calculate approx.

surface resistance from sample Q0 H G: Geometrical factor

Magnetic field profile

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U N C L A S S I F I E D

Sample setup detail and current MgB2 coating method

B.H. Moeckly and W.S. Ruby, Supercond. Sci.

  • Technol. 19 (2006) L21–L24

Reactive co-evaporation of MgB2 at Superconductor Technologies, Inc. (STI), Santa Barbra, CA.

Sample setup at SLAC

Sample: <1.5 mm thick Cold head Temperature sensor Copper sample holder: 6.35 mm thick

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U N C L A S S I F I E D

So far, 4 types of coatings have been tried in addition to bare Nb reference samples

Bulk Nb Bulk Nb MgB2 Bulk Nb B

MgB2

B (10 nm) MgB2 (100 nm) 1000 nm 200 nm 200 nm

#1 #2 #3

MgB2 300 nm Sapphire ~450 µm

#4

C-plane

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U N C L A S S I F I E D

Bulk Nb B (10 nm) MgB2 (100 nm)

Coating #1 Element depth profile

Planned Actual B Mg O Nb Mg Note the increase of O and Mg

A number of cracks on MgB2 were observed after tests.

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U N C L A S S I F I E D

Coating #2 Elements depth profile

Planned Actual Bulk Nb MgB2 1000 nm B Mg O Nb Note the increase of O

A number of cracks on MgB2 were observed after tests.

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U N C L A S S I F I E D

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Coating #3 Elements depth profile

Planned Actual Bulk Nb B

MgB2

200 nm 200 nm B Mg O Nb Mg Note the increase of O and Mg!

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U N C L A S S I F I E D

Coating #4 Elements depth profile

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Planned MgB2 Sapphire C-plane 300 nm ~450 µm

  • The actual depth profile

showed very small amount of oxygen and very close to the planned coating.

  • This indicates that the

increased amount of

  • xygen shown in the

previous MgB2/(B)/Nb systems was from bulk Nb

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U N C L A S S I F I E D

50,000 100,000 150,000 200,000 250,000 300,000 350,000 400,000 20 40 60 80 100 120

Q0 Sample temperature (K)

#1: MgB2(100nm)/B(10nm)/Nb #2: MgB2(1000nm)/Nb #3: MgB2(200nm)/B(200nm)/Nb #4: MgB2(300nm)/Sapphire Nb (single crystal RRR~300) Copper

Comparison of low-power Q0 –T data: MgB2(300nm)/Sapphire showed significantly higher Q0

MgB2(300nm)/Sapphire limited by the Q0 of copper dome

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U N C L A S S I F I E D

Coating #4, MgB2(300nm)/Sapphire: Q0 vs. Bpeak at 3 K MgB2 quenches at 25 mT (Only one sample has been tested so far.)

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50,000 100,000 150,000 200,000 250,000 300,000 350,000 400,000 5 10 15 20 25 30

Q0 Bpeak (mT)

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U N C L A S S I F I E D

Coating #4, MgB2(300nm)/Sapphire: BC,RF vs. T

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5 10 15 20 25 30 5 10 15 20 25 30 35 40

BC,RF (mT) T (K)

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U N C L A S S I F I E D

Measured quench fields at 3 K have been low. For #1- #3, thermal effect due to high surface resistance and effect of cracks are involved and confusing.

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Coating Series No. Planned coating Quench field (mT) #1 MgB2 (100nm)/B(10nm)/Nb ~30 #2 MgB2 (1000nm)/Nb ~30 #3 MgB2(200nm)/B(200nm)/Nb 10 (~50 on Nb) #4 MgB2 (300nm)/Sapphire 25

Actual T was probably higher!

Nb alone has shown a quench field of 60-70 mT and it is likely to be a thermal quench not magnetic, which is caused by high residual resistance.

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U N C L A S S I F I E D

Issues and plans to address them

Unexpectedly high residual resistance of Nb (~2 mΩ) compared to the expected BCS resistance of ~15 µΩ at 11.4 GHz at 3 K

  • Measure the external magnetic field and try to shield it and see the effect

The effect of reducing the film thickness has not been seen

  • A series of MgB2/Al2O3/Nb is under test to reduce the reaction between

MgB2 and Nb

  • Try MgB2 (<100nm)/Al2O3/MgB2 (<100nm)/Al2O3/MgB2

(<100nm)/Sapphire

Non-uniform coating due to relatively rough surface (Ra >10 nm)

  • We started to use mechanical-chemical polishing by Cabot

Microelectronics Polishing Company that produces Ra <1 nm

Cracks

  • Changing substrate thickness from ~0.6 to ~1.2 mm has helped.

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U N C L A S S I F I E D

Summary

 We are trying to demonstrate the principle of multi-

layer superconductor coating to increase the achievable magnetic field

 We have not been successful yet, but there has been

increased understanding on what is happening

 Our goal in 2010 is to demonstrate the first milestone

  • f >200 mT (0 K) or equivalent fields at respective

temperatures with flat 2-inch diameter samples after addressing some issues that have emerged.

Slide 16

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U N C L A S S I F I E D

Acknowledgements

 Many thanks to:

  • Sponsor (DTRA)
  • P. Kneisel (JLab)
  • A. Canabal (U. Maine)
  • S. Lesiak (CMPC)
  • Other LANL workers:

— R. Depaula, I. Apodaca (MPA-STC) — B. Day (MST-7) — R. Montoya (PF-FS) — J. Harrison, (AOT-MDE)