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High Temperature Superconductivity - After 25 years, where are we at? Michael Norman Materials Science Division Argonne National Laboratory Norman, Science 332, 196 (2011) Fermilab - June 22, 2011

High Temperature Superconductivity - After 25 years, where are we at?

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High Temperature Superconductivity - After 25 years, where are we at?. Michael Norman Materials Science Division Argonne National Laboratory. Norman, Science 332, 196 (2011). Fermilab - June 22, 2011. It All Started Back in 1986. T c Shot Up Like a Rock - PowerPoint PPT Presentation

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Page 1: High Temperature Superconductivity - After 25 years, where are we at?

High Temperature Superconductivity -After 25 years, where are we at?

Michael Norman

Materials Science DivisionArgonne National Laboratory

Norman, Science 332, 196 (2011)

Fermilab - June 22, 2011

Page 2: High Temperature Superconductivity - After 25 years, where are we at?

It All Started Back in 1986

Page 3: High Temperature Superconductivity - After 25 years, where are we at?

Tc Shot Up Like a Rock(many cuprates superconduct above 77K)

Page 4: High Temperature Superconductivity - After 25 years, where are we at?

Woodstock of Physics - March 1987

Page 5: High Temperature Superconductivity - After 25 years, where are we at?
Page 6: High Temperature Superconductivity - After 25 years, where are we at?

H. K. Onnes (1911)

Zero resistance

Meissner effect (1933)

Superconductors:(1) They are perfect conductors(2) They expel magnetic flux

Page 7: High Temperature Superconductivity - After 25 years, where are we at?

The Path to a Microscopic Theory was Littered with Many Famous Physicists

Einstein

Landau

Heisenberg

Feynman

Page 8: High Temperature Superconductivity - After 25 years, where are we at?

Eventually, Three Guys in Illinois Got It Right(Bardeen, Cooper, Schrieffer - 1956,1957)

Page 9: High Temperature Superconductivity - After 25 years, where are we at?

1. London theory - rigidity to macroscopic perturbations implies a “condensate” (1935,1950)

2. Ginzburg-Landau () theory - order parameter for condensate (1950)

3. Isotope effect (Maxwell, Serin & Reynolds, Frohlich, 1950)4. Cooper pairs (1956)5. Bardeen-Cooper-Schrieffer (BCS) microscopic theory (1957)6. Type-II superconductors (Abrikosov vortices, 1957)7. Connection of BCS to Ginzburg-Landau (Gorkov, 1958)8. Strong coupling superconductivity (Eliashberg, Nambu,

Anderson, Schrieffer, Wilkins, Scalapino …, 1960-1963)9. p-wave superfluidity in 3He (Osheroff, Richardson, Lee, 1972;

Leggett, 1972)10. Heavy Fermion Superconductivity (Steglich, 1979)11. High Temperature Superconductivity (Bednorz & Muller, 1986)12. Iron Arsenides (Hosono, 2008)

A (Very) Short History of Superconductivity

Page 10: High Temperature Superconductivity - After 25 years, where are we at?

From Steve Girvin’s lecture (Boulder Summer School 2000) courtesy of Matthew Fisher

Page 11: High Temperature Superconductivity - After 25 years, where are we at?

(the electron-phonon case)

1. 1st e- attracts + ions2. Ions shift position from red to blue3. 1st e- moves away4. 2nd e- sees + ion hole and moves to former position of 1st e-

Interaction is local in space(s-wave pairs, L=0, S=0)but retarded in time(Tc << Debye frequency)

Everything You Wanted to Know About Pair Formation(But Were Afraid to Ask)

Page 12: High Temperature Superconductivity - After 25 years, where are we at?

But cuprates haved-wave pairs!(L=2, S=0)

van Harlingen;Tsuei & Kirtley -Buckley Prize -1998

Artwork byGerald Zeldin (2000)

Page 13: High Temperature Superconductivity - After 25 years, where are we at?

Alex Abrikosov(small q phonons)

Bob Laughlin(competing phases)

Phil Anderson(RVB; interlayer tunneling; RVB)

Karl Mueller(bipolarons)

Bob Schrieffer(spin bags)

Tony Leggett(interlayer Coulomb)

Page 14: High Temperature Superconductivity - After 25 years, where are we at?
Page 15: High Temperature Superconductivity - After 25 years, where are we at?

1. Resonating valence bonds2. Spin fluctuations3. Stripes4. Anisotropic phonons5. Bipolarons6. Excitons7. Kinetic Energy lowering8. d-density wave9. Charge fluctuations10.Flux phases11.Gossamer superconductivity12.Spin bags13.SO(5)14.BCS/BEC crossover15.Plasmons16.Spin liquids

Not to Mention

Interlayer tunneling

Marginal Fermi liquid

van Hove singularities

Quantum critical points

Anyon superconductivity

Slave bosons

Dynamical mean field theory

Theories Connected with High Tc Superconductivity

Page 16: High Temperature Superconductivity - After 25 years, where are we at?

Famous Books

Abrikosov - Nobel Lecture - Dec. 2003

Famous Quotes

“On this basis I was able to explain most of the experimental data about layered cuprates . . .

As a result I can state thatthe so called “mystery” of high-Tc

superconductivity does not exist.”

Page 17: High Temperature Superconductivity - After 25 years, where are we at?

Ten Weeks of High Tc (to the tune of Twelve Days of Christmas)

On the first week of the program Friend Philip said to me All simply RVB (All sim-pl-ee R-r V B)

On the second week of the program Friend Douglas said to me Pair in a d-wave All simply RVB

On the third week of the program Friend David said to me It's magnons Pair in a d-wave All simply RVB

On the fourth week of the program Friend Chandra said to me Four current rings (fo-or current rings) It's magnons Pair in a d-wave All simply RVB

At the end of the program Friend Philip said to me Big Tent is stretching Visons escaping Visons are gapping Slave spinons pairing T sym-try breaking Stripes fluctuating S - O - 5 Four current rings It's magnons Pair in a d-wave All simply RVB    

--Ilya Gruzberg Smitha Vishveshwara Ilya Vekhter Aditi Mitra Senthil Matthew Fisher - -

KITP Web SiteHigh Tc Program - Fall 2000

Page 18: High Temperature Superconductivity - After 25 years, where are we at?

Why is the High Tc Problem So Hard to Solve?(Laughlin’s Lecture for Teachers - ITP, 2000)

Page 19: High Temperature Superconductivity - After 25 years, where are we at?

Electronic Structure of Cuprates

Page 20: High Temperature Superconductivity - After 25 years, where are we at?

Len MattheissPRL (1987)

Energy vs Momentum

Fermi surface

Electronic structure from density functional theory

Page 21: High Temperature Superconductivity - After 25 years, where are we at?

Cu2+Large U

charge-transfer gap pd ~ 2 eV

Mott insulatormetal?

doping

t = 0.3 eV, U = 2 eV, J = 4t2/U = 0.12 eV

J~1400 K

best evidence for large Uantiferromagnet

Hubbard

Short (and biased!) tutorial on cuprates

(slide from Phil Anderson)

Page 22: High Temperature Superconductivity - After 25 years, where are we at?

Phase Diagram of Cuprates

Page 23: High Temperature Superconductivity - After 25 years, where are we at?

1. There are 2e- pairs2. The pairs are d-wave (L=2, S=0)3. There are “normal” (i.e., 2e-) vortices4. Quasiparticles exist (but only below Tc)

What We DO Know

d-wave pairing observed by phase sensitive tunneling -

van Harlingen, Kirtley & TsueiKirtley et al, Nat. Phys. (2006)

Page 24: High Temperature Superconductivity - After 25 years, where are we at?

Extraction of the Superconducting Energy Gap from Photoemission

Campuzano, Shen, Johnson – Buckley Prize (2011)

k --> cos(kxa) - cos(kya) --> Implies near-neighbor pairs

Bi2212, Tc=87K

Dirac cone Ding et al., PRB (1996)

Page 25: High Temperature Superconductivity - After 25 years, where are we at?

Photoemission spectrum above and below Tc at momentum k=(,0) for Bi2212

Norman et al, PRL (1997)

peak

dip

Incoherent normal state

Coherent superconductor

Page 26: High Temperature Superconductivity - After 25 years, where are we at?

Neutron Spin Resonance (S=1 excitation)Rossat-Mignod/Bourges, Mook/Dai, Keimer/Fong

Dai et al, Nature (1999)

Page 27: High Temperature Superconductivity - After 25 years, where are we at?

Dispersion of magnetic excitations has the form of an hourglassArai et al, PRL (1999)

Page 28: High Temperature Superconductivity - After 25 years, where are we at?

The “strange metal” phase exhibits linear T resistivity

Martin et alPRB (1990)

Page 29: High Temperature Superconductivity - After 25 years, where are we at?

1. Spin singlets

2. Pre-formed pairs

3. Spin density wave

4. Charge density wave

5. d density wave

What is the Pseudogap Due to?

6. Orbital currents

7. Flux phase

8. Stripes/nematic

9. Valence bond solid/glass

10. Combination?

Page 30: High Temperature Superconductivity - After 25 years, where are we at?

Norman et al., Nature (1998)

T < Tc

(node)

Tc < T < T*(Fermi arc)

T > T*(full FS)

Temperature evolution of the Fermi surface

Page 31: High Temperature Superconductivity - After 25 years, where are we at?

Is the T=0 limit of the pseudogap phase a nodal metal?

Kanigel et al, Nat Phys (2006)Chatterjee et al, Nat Phys (2010)

Page 32: High Temperature Superconductivity - After 25 years, where are we at?

A Nernst signal (due to fluctuating vortices?) appears above Tc

Wang et alPRB (2001)

Page 33: High Temperature Superconductivity - After 25 years, where are we at?

Evolution of the Fermi surface with doping

Doiron-Leyraud et alNature (2007)

Page 34: High Temperature Superconductivity - After 25 years, where are we at?

The Hall number is negative!

Doiron-Leyraud et al.Nature (2007)

LeBoeuf et al.,Nature (2007) and PRB (2011)

RH < 0 forms a dome around 1/8

electron pockets due to magnetic stripes?

Page 35: High Temperature Superconductivity - After 25 years, where are we at?

Antiphase Stripes - Tranquada et al. - Nature (1995)Charge peaks at (±2x,0), Spin peaks at (1/2±x,1/2), x~1/8

spinpeaks

chargepeaks

dopedholes

localspins

Page 36: High Temperature Superconductivity - After 25 years, where are we at?
Page 37: High Temperature Superconductivity - After 25 years, where are we at?

Circular dichroism above Tc in the pseudogap phase?

Kaminski et alNature (2002)

Page 38: High Temperature Superconductivity - After 25 years, where are we at?

Orbital moments above Tc in the pseudogap phase?

Fauque et alPRL (2006)

Page 39: High Temperature Superconductivity - After 25 years, where are we at?

Science, February 1987

Page 40: High Temperature Superconductivity - After 25 years, where are we at?

RVB has many critics

Bob LaughlinAnnals of Improbable Research, May-June 2004

Page 41: High Temperature Superconductivity - After 25 years, where are we at?

Neel Lattice RVB

RVB (“resonating valence bond”) is a ‘strong coupling’ theory for cuprates developed by Phil

Anderson and his colleagues

It postulates a liquid of spin singlets

Page 42: High Temperature Superconductivity - After 25 years, where are we at?

The pseudogap phase corresponds to a d-wave pairing of spins (left). At zero doping, this is quantum mechanically equivalent to an orbital current phase (middle). The spin gap, , is not equivalent to the superconducting order parameter, sc, as it would be in BCS theory (right).

RVB Model (Phil Anderson - 1987, Gabe Kotliar - 1988, Patrick Lee, Mohit Randeria, Maurice Rice, etc.)

Page 43: High Temperature Superconductivity - After 25 years, where are we at?

Two Theories of the Phase Diagram

Relation of T* to Tc

RVB Quantum Critical

Page 44: High Temperature Superconductivity - After 25 years, where are we at?

Chatterjee et al., PNAS (2011)

Page 45: High Temperature Superconductivity - After 25 years, where are we at?

“Emery-Kivelson” picture Nature (1995)

Pairing occurs below mean field transition temperatureCoherence occurs below phase ordering temperatureSuperconductivity occurs only below both temperatures

Page 46: High Temperature Superconductivity - After 25 years, where are we at?

SO(5) vs SU(2)

Demler, Hanke, and Zhang Lee, Nagaosa, and Wen Rev Mod Phys (2004) Rev Mod Phys (2006)

Page 47: High Temperature Superconductivity - After 25 years, where are we at?

Antiferromagnetic spin fluctuations can lead to d-wave pairs(an e- with up spin wants its neighbors to have down spins)

Heavy Fermions - Varma (1986), Scalapino (1986)High Tc - Scalapino (1987), Pines (1991)

< Repulsive

< Attractive

Page 48: High Temperature Superconductivity - After 25 years, where are we at?

d-wave pairing due to a half-breathing phonon mode?Shen, Lanzara, Ishihara, Nagaosa - Phil Mag B (2002)

Page 49: High Temperature Superconductivity - After 25 years, where are we at?

Hartnoll, Science (2008)

Holographic approach to high temperature superconductors?

Page 50: High Temperature Superconductivity - After 25 years, where are we at?