Effect of Inhomogeneous Disorder on the Superheating Field of SRF - - PowerPoint PPT Presentation

effect of inhomogeneous disorder on the superheating
SMART_READER_LITE
LIVE PREVIEW

Effect of Inhomogeneous Disorder on the Superheating Field of SRF - - PowerPoint PPT Presentation

SRF2019, Dresden, July 4, 2019 Effect of Inhomogeneous Disorder on the Superheating Field of SRF Cavities James A. Sauls Department of Physics Center for Applied Physics & Superconducting Technologies Northwestern University & Fermilab


slide-1
SLIDE 1

SRF2019, Dresden, July 4, 2019

Effect of Inhomogeneous Disorder on the Superheating Field of SRF Cavities

James A. Sauls

Department of Physics Center for Applied Physics & Superconducting Technologies Northwestern University & Fermilab

  • Wave Ngampruetikorn
  • Mehdi Zarea
  • Fermilab Collaborators:

Anna Grassellino, Mattia Checchin, Martina Martinello, Sam Posen, Alex Romanenko

NSF-PHY 01734332

slide-2
SLIDE 2
  • V. Chandrasekhar
  • W. Halperin
  • J. Ketterson
  • J. Koch
  • D. Seidman
  • N. Stern

Anna Grassellino Mattia Checchin Martina Martinello Sam Posen Alex Romanenko

slide-3
SLIDE 3

Electrodynamics of Superconductor-Vacuum Interfaces ◮Program: First-Principles + Materials Inputs: Current Response & Local EM Fields for Superconducting-Vacuum Interfaces

Vacuum Nb

q

J(q,ω) = −1 c ↔ K

R

(q,ω; A ) · A(q,ω)

slide-4
SLIDE 4

Electrodynamics of Superconductor-Vacuum Interfaces ◮Program: First-Principles + Materials Inputs: Current Response & Local EM Fields for Superconducting-Vacuum Interfaces

Vacuum Nb

q

J(q,ω) = −1 c ↔ K

R

(q,ω; A ) · A(q,ω) ◮Material Inputs: ◮ Fermi Surfaces - DFT & dHvA ◮ Pairing/Decoherence via Electron-Phonon Coupling

slide-5
SLIDE 5

Electrodynamics of Superconductor-Vacuum Interfaces ◮Program: First-Principles + Materials Inputs: Current Response & Local EM Fields for Superconducting-Vacuum Interfaces

Vacuum Nb

q

J(q,ω) = −1 c ↔ K

R

(q,ω; A ) · A(q,ω) ◮Material Inputs: ◮ Fermi Surfaces - DFT & dHvA ◮ Pairing/Decoherence via Electron-Phonon Coupling ◮ Impurity & Structural Disorder ◮ Surface Scattering: Ssurf(p,p′)

◮ surface structure factor ◮ mesoscopic roughness backscattering Andreev scattering sub-gap dissipation

slide-6
SLIDE 6

Electrodynamics of Superconductor-Vacuum Interfaces ◮Program: First-Principles + Materials Inputs: Current Response & Local EM Fields for Superconducting-Vacuum Interfaces

Vacuum Nb

q

J(q,ω) = −1 c ↔ K

R

(q,ω; A ) · A(q,ω) ◮Material Inputs: ◮ Fermi Surfaces - DFT & dHvA ◮ Pairing/Decoherence via Electron-Phonon Coupling ◮ Impurity & Structural Disorder ◮ Surface Scattering: Ssurf(p,p′)

◮ surface structure factor ◮ mesoscopic roughness backscattering Andreev scattering sub-gap dissipation

◮Theoretical & Analytical Tools ◮ Migdal-Eliashberg: electron-phonon ◮ Asymptotic Expansions: kBTc/E f , ¯ h/τE f , ¯ h/p f ξ, ¯ hω/Ef ... ◮ Selection Rules & Scattering Theory ◮ Keldysh Transport Equations

slide-7
SLIDE 7

Electrodynamics of Superconductor-Vacuum Interfaces ◮Program: First-Principles + Materials Inputs: Current Response & Local EM Fields for Superconducting-Vacuum Interfaces

Vacuum Nb

q

J(q,ω) = −1 c ↔ K

R

(q,ω; A ) · A(q,ω) ◮Material Inputs: ◮ Fermi Surfaces - DFT & dHvA ◮ Pairing/Decoherence via Electron-Phonon Coupling ◮ Impurity & Structural Disorder ◮ Surface Scattering: Ssurf(p,p′)

◮ surface structure factor ◮ mesoscopic roughness backscattering Andreev scattering sub-gap dissipation

◮Theoretical & Analytical Tools ◮ Migdal-Eliashberg: electron-phonon ◮ Asymptotic Expansions: kBTc/E f , ¯ h/τE f , ¯ h/p f ξ, ¯ hω/Ef ... ◮ Selection Rules & Scattering Theory ◮ Keldysh Transport Equations ◮ Developing Methods & Codes to Compute the Nonlinear A.C. Surface Impedance ◮ Nonequilibrium Quasiparticle, Cooper Pair & Vortex Dynamics

  • D. Rainer & J. A. Sauls, Strong-Coupling Theory of Superconductivity, World Scientific (1995); arXiv:1809.05264
slide-8
SLIDE 8

Electronic band structure of Niobium

DFT Calculation of the Electronic Band Strucuture 10 20 30 40 50 60 G H G P N E[eV] Ef= 18.1 eV Nb=[Kr]4d45s1 24 bands Fermi Energy = 18.1 eV 2 bands cross the Fermi energy

◮P . Giannozzi et al., J. Phys. Cond. Mat. 29 465901 (2017)

slide-9
SLIDE 9

Phonons in Niobium

50 100 150 200 250 G H N G P N

  • hω [1/cm]

Theory - Phonon dispersion Inelastic Neutron Scattering

– DFT Perturbation Theory

  • Inelastic Neutron Scattering;

Baroni, S., de Gironcoli, S., Dal Corso, A. & Giannozzi, P ., Rev. Mod. Phys. 73, 515562 (2001), Phonons and related crystal properties from density-functional perturbation theory

B.M. Powell, et al., Phonon properties of niobium ..., Can. J. Phys. 55, 1601 (1977)

slide-10
SLIDE 10

Electron-Phonon Spectral Function α2F(ω)

5 10 15 20 25 30 0.2 0.4 0.6 0.8 1 ¯ hω [meV] α2F Exp

◮ Maxium Phonon Frequency: ¯ hωmax = 27.0meV ◮ λ = 2

0 dω α2F(ω)

ω = 1.18 ◮ Electron-Electron Repulsion: µ∗ = 0.30 ◮ Eliashberg Theory: Tc = 9.47K ◮ Tunneling Inversion

  • G. Arnold et al., JLTP 40,

225 (1980). ◮ DFT Perturbation theory fails for Nb ? ◮ Inversion of dI/dV from PETS does not yield bulk α2F(ω) ? ◮ Nb surface has defects that suppress the high-ω spectrum ?

  • G. Schierning et al., Phys. Stat. Solidi RRL 9, 431 (2015)
slide-11
SLIDE 11

Eliashberg Equations

ˆ Σpa

nk(iωj) =

ˆ Gmk′(iωj′) ˆ Dk−k′ν(iωj − iωj′) gnm,ν(k′, k) gmn,ν(k, k′) +

Vk−k′(iωj − iωj′) ˆ Gmk′(iωj′)

Znk(iωj) = 1+ πT N(εF)ωj ∑

mk′ j′

ωj′

  • ω2

j′ +∆2 mk′(iωj′)

λ(nk,mk′,ωj −ωj′)δ(εmk′ −εf) Znk(iωj)∆nk(iωj) = πT N(εF) ∑

mk′ j′

∆mk′(iωj′)

  • ω2

j′ +∆2 mk′(iωj′)

[λ(nk,mk′,ωj −ω j′)− µ∗

c ]δ(εmk′ −εf)

slide-12
SLIDE 12

Strong coupling superconducting gap

2 4 6 8 0.5 1 1.5

∆0 = 1.56 meV Tc = 9.45 K

T [K] ∆ [meV] Eliashberg Theory Weak coupling BCS

slide-13
SLIDE 13

Anisotropy of the Gap and Fermi Velocity

∆ [meV] T = 0.5K speed [106m/s]

◮Gap Anisotropy: ∆max = 2.54 meV ∆min = 1.38 meV ∆av = 1.56 meV ◮Velocity Anisotropy: vmax

f

= 1.3×106 m/s vmin

f

= 0.2×106 m/s ◮Strong Anisotropy of the Fermi Velocity - Impact on Critical Currents?

slide-14
SLIDE 14

Theoretical Program

◮ Develop Computational Code & Tools for Electronic Structure of Nb

  • Phonon Spectra & Density of States - DFT Perturbation Theory
  • Electron-Phonon Coupling - Eliashberg Theory
  • Strong-Coupling Superconducting Gap on the Fermi Surface

◮ Incorporate Disorder and Surface Scattering

  • Constraints from Surface and Materials characterization

⇓ ◮ Develop computational transport theory - charge and heat response under strong EM field conditions at the superconductor-vacuum interface

slide-15
SLIDE 15

SRF Performance Goals - What Can Theory Provide?

◮ Push to high Q-factor & Reduce a.c. dissipation up to high Eacc ◮ Understand physics of current response at f GHz at high Bs ◮ Push Emax

acc - processes determining Meissner stability/breakdown

⇓ Materials based theory of Non-Equilibrium Superconductivity under Strong Nonlinear A.C. Conditions

slide-16
SLIDE 16

Type-I

Meissner

Bc B T Tc

Type-II

Meissner

B T Tc Bc2 Bc1

Bsh

metastable Meissner metastable Meissner

Meissner state is metastable up to the superheating field

Superheating field

(Max Field Gradient)

slide-17
SLIDE 17

Superheating field is determined from local critical current

  • We solve simultaneously
  • 1. Eilenberger equation
  • for quasiparticle spectrum
  • 2. Gap equation
  • for excitation gap
  • 3. Impurity T-matrix equation
  • for the effect of disorder
  • 4. Maxwell’s equation
  • for B-field and current profiles
  • To obtain superheating field,

increase surface field until current reaches critical value

superconductor surface field

Bsh B Magnetic field x ps Superfluid momentum (Vector potential) 1 js/jc Supercurrent density

6

slide-18
SLIDE 18

Nonlinear D.C. Current Response

  • js(x) = −eNf
  • dε tanh ε

2T

  • vf A (ˆ

p,ε,x)

  • ˆ

p

◮ Spectral Function: A (ˆ p,ε;x) ≡ −1

π ImG(ˆ

p,ε;x) ◮ local impurity self-energies, Σimp(x) = γ(x) G ◮ local superconducting order parameter: ∆(x) ◮ local condensate momentum, ps = ¯

h 2∇rϑ − e cA

◮ perturbation expansion in ε ∈ {ξ/λL, ξ/ζ} Propagator for Quasiparticles and Cooper Pairs: −1 π

  • G(ˆ

p,ε,x)=[˜ ε(ε,x)−vf ·ps(x)] τ3−˜ ∆(ε,x)(iσy τ1)

∆(ε,x)|2 −[˜ ε(ε,x)−v f ·ps(x)]2 ≡ [G τ3 −F(iσy τ1)] ˜ ε(ε,x) = ε +γ(x)G(ˆ p,ε,x)ˆ

p

˜ ∆(ε,x) = ∆(x)+γ(x)F(ˆ p,ε,x)ˆ

p

∆(x) = g 2

  • dε tanh ε

2T Im f(ˆ p,ε,x)ˆ

p ,

∂ 2

x ps(x)− 4πe

c2 js[ps(x),γ(x)] = 0

slide-19
SLIDE 19

Bsh is affected via 2 mechanisms

✓Longer penetration depth

➤ more screening current ✗Lower critical supercurrent ➤ less screening current

Effective penetration depth Impurity scattering rate, γ

λ ≡

− ∞

γ Critical current density Impurity scattering rate, γ 0.84 0.80 Bsh/ B0 Impurity scattering rate, γ

For uniform disorder

Penetration depth dominates Current suppression dominates

Disorder Suppresses Supercurrents

  • G. Catelani and J. P

. Sethna, The superheating field for superconductors in the high-κ London limit, PRB 78, 224509 (2008). ◮ F. P .-J. Lin and A. Gurevich, Effect of impurities on the superheating field of type-II superconductors, PRB 85, 054513 (2012).

slide-20
SLIDE 20

Enhanced Superheating Fields in Multi-Layer Systems

  • T. Kubo, Y. Iwashita, and T. Saeki, R.F

. electromagnetic field and vortex penetration in multi-layered superconductors, Appl.

  • Phys. Lett. 104, 032603 (2014).

  • S. Posen, M. K. Transtrum, G. Catelani, M. U. Liepe, and J. P

. Sethna, Shielding Superconductors with Thin Films as Applied to RF Cavities for Particle Accelerators, Phys. Rev. Applied 4, 044019 (2015). ◮

  • A. Gurevich, Maximum screening fields of superconducting multilayer structures, AIP Adv. 5, 017112 (2015).

  • D. B. Liarte, M. K. Transtrum, and J. P

. Sethna, Ginzburg-Landau theory of the superheating field anisotropy of layered superconductors, Phys. Rev. B 94, 144504 (2016). ◮

  • D. B. Liarte, S. Posen, M. K. Transtrum, G. Catelani, M. Liepe, and J. P

. Sethna, Theoretical estimates of maximum fields in superconducting resonant radio frequency cavities: stability theory, disorder, and laminates, Supercond. Sci. Tech. 30, 033002 (2017). ◮

  • T. Kubo, Multilayer coating for higher accelerating fields in superconducting radio-frequency cavities: a review of theoretical

aspects, Supercond. Sci. Tech. 30, 023001 (2017).

slide-21
SLIDE 21

Maximum Gradient increased with N infusion into Nb

  • A. Grassellino, et al. arXiv:1701.06077
slide-22
SLIDE 22

Disorder heterogeneity can enhance Bsh

γ js Screening current density Bsh B Magnetic fi eld x superconductor surface f eld γ Impurity scattering rate fi clean dirty

slide-23
SLIDE 23

Disorder heterogeneity can enhance Bsh

γ js Screening current density Bsh B Magnetic fi eld x superconductor surface f eld γ Impurity scattering rate fi clean dirty

✓Longer effective penetration

depth due to dirty layer

  • Slowly varying B-f eld

requires less screening current density

slide-24
SLIDE 24

Disorder heterogeneity can enhance Bsh

γ js Screening current density Bsh B Magnetic fi eld x superconductor surface f eld γ Impurity scattering rate fi clean dirty

✓Longer effective penetration

depth due to dirty layer

  • Slowly varying B-f eld

requires less screening current density

✓Most screening current is in

the clean region and is not suppressed by disorder

slide-25
SLIDE 25

Superheating Field with an Impurity Diffusion Region

Superheating Field at T = 0

0.5

240

1

120

2

60

3

40

4

30

0.8

(160)

1.0

(200)

1.2

(240)

Bsh/B0

(mT)

γ0/∆00

ℓ0 [nm]

ζ/λL0 0.3 0.5 1.0 3.0 ∞

  • Clean Limit Critical Field: B0 =
  • 4πNf ∆2

00

Impurity Diffusion Profile γ(x) = nimp(x) 2π ¯ h |T|2FS

50 100 150 200

x

(nm)

γ(x) = γ0e−x/ζ

0.5 1.0 3.0

2 4 1.0 1.5 2.0

Clean Limit London Penetration Length: λL0 = 1/(8πe2v2

f Nf /3c2) 1 2

◮ The Effect of Inhomogeneous Surface Disorder on the Superheating Field of Superconducting RF Cavities,

  • V. Ngampruetikorn & JAS, arXiv:1809.04057
slide-26
SLIDE 26

Summary plus Comments

◮ Ongoing development of computational transport theory for Superconductors under strong EM field conditions directed at understanding of physics of SRF cavities ◮ Nonlinear Current Response for Impurity Diffusion into Nb

  • Increase the Superheating Field with Impurity Disorder
  • Balance between increased λeff & decreased Jc

◮ Instabilities before the Superheating Field:

  • Dangerous local regions of high current density
  • For Js → Jc, ∆(Js) → 0 Nonequilibrium QP generation @ 1 GHz