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Secondary Electron 
Yield for SRF Materials 
Sarah Aull
Looking back to the SRF13 
• 500 nm MgB2 on a Nb substrate 
(deposited by Chris Yung at STI) 
• Strong multipacting on 1st RF test 
• After new rinsing: even stronger 
multipacting + „burn marks“ in high E 
field regions 
• XPS measurements show only 70% 
MgB2 
Cause for multipacting? 
Emax 
sarah.aull@cern.ch 2
Secondary Electron Yield (SEY) 
• SEY = 
# 푠푒푐표푛푑푎푟푦 푒푙푒푐푡푟표푛푠 
푝푟푖푚푎푟푦 푒푙푒푐푡푟표푛 
• Primary electron travels through the 
material, creating secondaries 
• Most secondaries are produced at the 
end of the primary path 
• Penetration depth 푅푚푎푥~퐸0 primary 
energy 
• Probability of emission decreases 
exponentially with depth XS 
• 푅푚푎푥 ≪ 푋푆: Few secondaries, but 
easy emission 
• 푅푚푎푥 ≫ 푋푆: Many secondaries, but 
low emission 
sarah.aull@cern.ch 3
SEY of (non) conductors 
• SEY is closely connected to the electrical conductivity 
• Metals: 
• internal secondaries scatter mainly with free electrons 
• Vacuum barrier is in the order of 10 eV 
• low SEY: 0.5 (Li) – 1.8 (Pt); SEY(Nb) = 1.3 
• Insulators: 
• Internal secondaries scatter with phonons and defects 
• Vacuum barrier is in the order of 1 eV 
• High SEY: 4 – 15 (MgO) 
• The SEY of alloys ranges usually between 1.5 and 3 
Literature values usually refer to pure material, 
not the technical surfaces! 
sarah.aull@cern.ch 4
Influence of the Surface 
• If the primary electron arrives in a grazing angle, 
secondaries are more likely emitted ( higher SEY) 
• If the surface is rough, emitted secondaries can be 
reabsorbed ( lower SEY) 
• Oxides and contamination on the surface might influence 
the SEY significantly 
• Contamination: hydrocarbons, condensed water and gases 
(especially on a cryogenic surface), foreign material 
sarah.aull@cern.ch 5
SEY setup at CERN 
• SEY measurement 
• under UHV 
• at room temperature 
• with normal angle 
• SEY = 
퐼collector 
퐼sample+퐼collector 
• Sample can be transferred to the XPS 
setup under vacuum so that the 
surface condition is not altered. 
sarah.aull@cern.ch 6
• The XPS setup includes a sputter ion gun (Argon) 
• XPS measurements were performed with every SEY measurement 
(before and after sputtering) to estimate the cleanliness of the 
surface 
• Sputtering removes contaminants but also changes the chemical 
composition of the surface! 
• Few nm were sputtered off for removal of the carbon peak 
sarah.aull@cern.ch 7 
XPS & Sputtering 
Nb
From SEY data to multipacting in a cavity 
• Gases will condense on the cold surface 
• RF conditioning will not remove nm of material, but 
helium processing might 
• Angular dependence might play an important role 
• It is unknown if the SEY changes below Tc 
The SEY data before and after sputtering serves as a 
bad case and good case scenario! 
sarah.aull@cern.ch 8
SEY of technical bulk Nb 
• Both samples cut from same Nb sheet. 
• Carbon and oxides have strong impact on the SEY. 
sarah.aull@cern.ch 9 
47 
5 
38 
10 
23 
7 
57 
13 
32 
18 
45 
47 
43 
5 5 
4 
60 
50 
40 
30 
20 
10 
0 
C Nb O Rest 
Atomic Composition [%] 
BCP BCP degreased EP degreased EP sputtered
NbTiN 
• Kindly prepared by A-M Valente-Feliciano, JLab 
• NbTiN on Nb via HIPIMS 
sarah.aull@cern.ch 10 
33 
9 
2 
11 
41 
35 
5 3 
0 
29 
23 
9 
50 
40 
30 
20 
10 
0 
C 1s N 1s Na 1s Nb 3d5 O 1s Ti 2p3 
Atomic Composition [%] 
before sputtering 
after sputtering
Nb3Sn 
• Kindly prepared by Sam Posen, Cornell 
• Nb3Sn on Nb via reactive evaporation 
• Nb3Sn cavity did not reach multipacting band yet 
sarah.aull@cern.ch 11 
26 
48 
8 
2 
15 
5 
55 
26 
1 
13 
60 
50 
40 
30 
20 
10 
0 
C 1s O 1s Nb 3d5 Cu 2p Sn 3d5 
Atomic Composition [%] 
before sputtering 
after sputtering
MgB2 
• Kindly provided by X.X. Xi, Temple University 
• No sputtering to avoid further oxidation 
• Formation of MgO will increase the SEY. 
sarah.aull@cern.ch 12 
18 
21 
1 1 
16 
43 
17 
25 
2 
0 
15 
41 
50 
40 
30 
20 
10 
0 
B 1s C 1s Cl 2p3 F 1s Mg 2s O 1s 
Atomic Composition [%] 
1018c 
1018d
Conclusion 
• The SEY of technical surfaces 
need to be considered for SRF 
applications. 
• SEY of NbTiN & Nb3Sn 
comparable to Nb (after 
sputtering). 
• Validation through RF tests is 
however needed. 
• MgB2 needs a non-dissipating 
passivation with low SEY. 
sarah.aull@cern.ch 13
Acknowledgements 
• Thank you for providing and preparing samples: 
• MgB2 for the QPR: Chris Yung, STI 
• MgB2 for SEY: Xiaoxing Xi, Temple University 
• NbTiN; Anne-Marie Valente-Feliciano, Jefferson Lab 
• Nb3Sn: Sam Posen, Cornell 
• Nb: Nuria Valverde Alonso, CERN 
• BCP/EP: Serge Forel & Leonel Ferreira, CERN 
• Mauro Taborelli for access to the SEY setup 
• Mounir Mensi and Holger Neupert for performing the 
measurements with me (and answering all my questions). 
sarah.aull@cern.ch 14

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Sarah aull secondary electron yield of srf materials

  • 1. Secondary Electron Yield for SRF Materials Sarah Aull
  • 2. Looking back to the SRF13 • 500 nm MgB2 on a Nb substrate (deposited by Chris Yung at STI) • Strong multipacting on 1st RF test • After new rinsing: even stronger multipacting + „burn marks“ in high E field regions • XPS measurements show only 70% MgB2 Cause for multipacting? Emax sarah.aull@cern.ch 2
  • 3. Secondary Electron Yield (SEY) • SEY = # 푠푒푐표푛푑푎푟푦 푒푙푒푐푡푟표푛푠 푝푟푖푚푎푟푦 푒푙푒푐푡푟표푛 • Primary electron travels through the material, creating secondaries • Most secondaries are produced at the end of the primary path • Penetration depth 푅푚푎푥~퐸0 primary energy • Probability of emission decreases exponentially with depth XS • 푅푚푎푥 ≪ 푋푆: Few secondaries, but easy emission • 푅푚푎푥 ≫ 푋푆: Many secondaries, but low emission sarah.aull@cern.ch 3
  • 4. SEY of (non) conductors • SEY is closely connected to the electrical conductivity • Metals: • internal secondaries scatter mainly with free electrons • Vacuum barrier is in the order of 10 eV • low SEY: 0.5 (Li) – 1.8 (Pt); SEY(Nb) = 1.3 • Insulators: • Internal secondaries scatter with phonons and defects • Vacuum barrier is in the order of 1 eV • High SEY: 4 – 15 (MgO) • The SEY of alloys ranges usually between 1.5 and 3 Literature values usually refer to pure material, not the technical surfaces! sarah.aull@cern.ch 4
  • 5. Influence of the Surface • If the primary electron arrives in a grazing angle, secondaries are more likely emitted ( higher SEY) • If the surface is rough, emitted secondaries can be reabsorbed ( lower SEY) • Oxides and contamination on the surface might influence the SEY significantly • Contamination: hydrocarbons, condensed water and gases (especially on a cryogenic surface), foreign material sarah.aull@cern.ch 5
  • 6. SEY setup at CERN • SEY measurement • under UHV • at room temperature • with normal angle • SEY = 퐼collector 퐼sample+퐼collector • Sample can be transferred to the XPS setup under vacuum so that the surface condition is not altered. sarah.aull@cern.ch 6
  • 7. • The XPS setup includes a sputter ion gun (Argon) • XPS measurements were performed with every SEY measurement (before and after sputtering) to estimate the cleanliness of the surface • Sputtering removes contaminants but also changes the chemical composition of the surface! • Few nm were sputtered off for removal of the carbon peak sarah.aull@cern.ch 7 XPS & Sputtering Nb
  • 8. From SEY data to multipacting in a cavity • Gases will condense on the cold surface • RF conditioning will not remove nm of material, but helium processing might • Angular dependence might play an important role • It is unknown if the SEY changes below Tc The SEY data before and after sputtering serves as a bad case and good case scenario! sarah.aull@cern.ch 8
  • 9. SEY of technical bulk Nb • Both samples cut from same Nb sheet. • Carbon and oxides have strong impact on the SEY. sarah.aull@cern.ch 9 47 5 38 10 23 7 57 13 32 18 45 47 43 5 5 4 60 50 40 30 20 10 0 C Nb O Rest Atomic Composition [%] BCP BCP degreased EP degreased EP sputtered
  • 10. NbTiN • Kindly prepared by A-M Valente-Feliciano, JLab • NbTiN on Nb via HIPIMS sarah.aull@cern.ch 10 33 9 2 11 41 35 5 3 0 29 23 9 50 40 30 20 10 0 C 1s N 1s Na 1s Nb 3d5 O 1s Ti 2p3 Atomic Composition [%] before sputtering after sputtering
  • 11. Nb3Sn • Kindly prepared by Sam Posen, Cornell • Nb3Sn on Nb via reactive evaporation • Nb3Sn cavity did not reach multipacting band yet sarah.aull@cern.ch 11 26 48 8 2 15 5 55 26 1 13 60 50 40 30 20 10 0 C 1s O 1s Nb 3d5 Cu 2p Sn 3d5 Atomic Composition [%] before sputtering after sputtering
  • 12. MgB2 • Kindly provided by X.X. Xi, Temple University • No sputtering to avoid further oxidation • Formation of MgO will increase the SEY. sarah.aull@cern.ch 12 18 21 1 1 16 43 17 25 2 0 15 41 50 40 30 20 10 0 B 1s C 1s Cl 2p3 F 1s Mg 2s O 1s Atomic Composition [%] 1018c 1018d
  • 13. Conclusion • The SEY of technical surfaces need to be considered for SRF applications. • SEY of NbTiN & Nb3Sn comparable to Nb (after sputtering). • Validation through RF tests is however needed. • MgB2 needs a non-dissipating passivation with low SEY. sarah.aull@cern.ch 13
  • 14. Acknowledgements • Thank you for providing and preparing samples: • MgB2 for the QPR: Chris Yung, STI • MgB2 for SEY: Xiaoxing Xi, Temple University • NbTiN; Anne-Marie Valente-Feliciano, Jefferson Lab • Nb3Sn: Sam Posen, Cornell • Nb: Nuria Valverde Alonso, CERN • BCP/EP: Serge Forel & Leonel Ferreira, CERN • Mauro Taborelli for access to the SEY setup • Mounir Mensi and Holger Neupert for performing the measurements with me (and answering all my questions). sarah.aull@cern.ch 14