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Delay times in chiral ensembles—signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December 2015

Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

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Order = broken symmetry → order parameter 2 nd order 1 st order phase transition

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Page 1: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Delay times in chiral ensembles—signatures of chaotic scattering from

Majorana zero modes

Henning SchomerusLancaster University

Bielefeld, 12 December 2015

Page 2: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Order = broken symmetry → order parameter

2nd order

1st order

phase transition

Page 3: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

quasicrystals

JP Sethna

Page 4: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

liquid crystals

nematic

smectic

chiral

Wikipedia

Page 5: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Ψ

→ Superfluidity

VUERQEX

Helium

(macroscopic) wave function Ψ is a possible order parameter

Page 6: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Ψ

→ Superconductivity

(Cooper pairs: electrons+holes)

metallurgyfordummies,.com

(macroscopic) wave function Ψ is a possible order parameter

Page 7: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Ψ

→ Bose-Einstein condensates

ultracold monatomic gas

NIST

(macroscopic) wave function Ψ is a possible order parameter

Page 8: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Edge dislocation in a crystal

www.ndt-ed.org

Defect in a nematic liquid

Robust excitations from winding of the order parameter

JP Sethna

But none for a magnet!

Page 9: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Midgap state

Transfer to electronic band structures:e.g. conjugated polymers (Su, Schrieffer, Heeger 1979)

Winding of pseudospin

Page 10: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

H = H †: unitary (complex) H =T H T = H *, T 2 = +1: orthogonal (real)H = T H T = H d, T 2 = ‒1: symplectic (quaternion)

• particle-hole symmetry C in superconductors: H = ‒C H C 4 additional classes, including D

• chiral (anti)symmetry X H X = ‒H : 3 additional classes, including BDI

RMT classification: Hamiltonian

Verbaschoot et al 1993,Altland & Zirnbauer 1996

Topological QuantumNumbers

Page 11: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Common features• Symmetric spectrum• Winding numbers/Berry phase• Effect on quantization

— from superconductivity— depend on class

— zero modes

Majoranas

Page 12: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Mourik et al 2012

N ST

midgap differential conductance peak [Law, Lee, and Ng (2009), ...] Þ conductance peak as a signature

Or weak antilocalization? Usually lost in magnetic field, but restored by particle-hole symmetry [Brouwer and Beenakker (1995), Altland and Zirnbauer (1996)]

indium antimonide nanowires contacted with one normal (gold) and one superconducting (niobium titanium nitride) electrode

Page 13: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Majorana peak vs weak antilocalization…

Pikulin, Dahlhaus, Wimmer, HS & Beenakker, New J Physics. 14, 125011 (2012)

Page 14: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

N ST

Conductance of nanowire

Scattering formalism: Andreev reflection

Wave matching conductance

Diffusive scattering with fixed T = T:

RMT for

Q: topological invariant

Page 15: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

RMT of in symmetry class D:

Dyson’s Brownian motion approach

Page 16: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Dyson’s Brownian motion approach

Page 17: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

RMT of in symmetry class BDI:

Dyson’s Brownian motion approach

Page 18: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Dyson’s Brownian motion approach

Page 19: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Average conductance

Zero-bias anomaly no proof of Majorana fermionsQ-independent!

Re-insert into

large-N limit:

Pikulin, Dahlhaus, Wimmer, HS & Beenakker, New J Physics. 14, 125011 (2012)

Page 20: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Deeper understanding: density of states

independent of absence or presence of Majorana bound state

Scattering matrix

Density of states

Scattering rate has distribution

Page 21: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

RMT classification: HamiltonianH = H †: unitary (complex) H =T H T = H *, T 2 = +1: orthogonal (real)H = T H T = H d, T 2 = ‒1: symplectic (quaternion)

• particle-hole symmetry C in superconductors: H = ‒C H C 4 additional classes, including D

• chiral (anti)symmetry X H X = ‒H : 3 additional classes, including BDI

Z2 quantum number

Z quantum number

Page 22: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

chiral Boguliubov-De Gennes Hamiltonian:multiple Majorana modes

Z quantum number

Page 23: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Scattering matrix

Chiral Boguliubov-De Gennes Hamiltonian

Top. quantum number

Chiral symmetry

Page 24: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Meaning of the quantum number

Page 25: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Density of states

Chiral symmetry

which depends on ν!HS, M. Marciani, C. W. J. Beenakker, PRL 114, 166803 (2015)

Page 26: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Details

Need nullspace of this,treat rest as perturbation

Page 27: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Test: RMT scattering rates versus direct sampling

Page 28: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Fermi-level density of states

Page 29: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

partially transparent contactsTwo sets of rates from

Marginal distributions

disentangle

constraint

Page 30: Delay times in chiral ensembles signatures of chaotic scattering from Majorana zero modes Henning Schomerus Lancaster University Bielefeld, 12 December

Summary

• In superconducting universality classes, signatures of Majorana zero modes compete with weak antilocalization effects

• chiral superconductors may show clearer signatures

HS, M. Marciani, C. W. J. Beenakker, PRL 114, 166803 (2015)

Pikulin, Dahlhaus, Wimmer, HS & Beenakker, New J Physics. 14, 125011 (2012)