Unparticles and Emergent Mottness

Similar documents
Unparticles in High T_c Superconductors

Absence of Luttinger s Theorem

Is Strongly Correlated Electron Matter Full of Unparticles? Kiaran dave Charlie Kane Brandon Langley

Is Strongly Correlated Electron Matter Full of Unparticles? Kiaran dave Charlie Kane Brandon Langley

Holography and Mottness: a Discrete Marriage

Thanks to: NSF, EFRC (DOE)

Thanks to: NSF, EFRC (DOE)

Optical Conductivity in the Cuprates: from Mottness to Scale Invariance

Optical Conductivity in the Cuprates from holography and unparticles

Holography and Mottness: a Discrete Marriage

Optical Conductivity in the Cuprates from Holography and Unparticles

Testing Mottness/unparticles and anomalous dimensions in the Cuprates

`Anomalous dimensions for conserved currents from holographic dilatonic models to superconductivity. Gabriele La Nave. Thanks to: NSF, EFRC (DOE)

Demystifying the Strange Metal in High-temperature. Superconductors: Composite Excitations

Anomalous dimensions, Mottness, Bose metals, and holography. D. Dalidovich G. La Nave G. Vanacore. Wednesday, January 18, 17

10 Interlude: Preview of the AdS/CFT correspondence

ds/cft Contents Lecturer: Prof. Juan Maldacena Transcriber: Alexander Chen August 7, Lecture Lecture 2 5

Emergent Quantum Criticality

Applications of AdS/CFT correspondence to cold atom physics

Detecting unparticles and anomalous dimensions in the Strange Metal

Introduction to AdS/CFT

Condensed Matter Physics and the Nature of Spacetime

Non-relativistic holography

Duality and Holography

Quantum Entanglement and the Geometry of Spacetime

Fun with 2-Group Symmetry. Po-Shen Hsin California Institute of Technology October 13, Benini, Córdova, PH

The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local Gauge Transformations Dynamics of Field Ten

The arrow of time, black holes, and quantum mixing of large N Yang-Mills theories

Topological Properties of Quantum States of Condensed Matter: some recent surprises.

8.821 F2008 Lecture 12: Boundary of AdS; Poincaré patch; wave equation in AdS

Quantum oscillations & black hole ringing

Holographic transport with random-field disorder. Andrew Lucas

Black Holes, Holography, and Quantum Information

!onformali" Los# J.-W. Lee D. T. Son M. Stephanov D.B.K. arxiv: Phys.Rev.D80:125005,2009

The Gauge/Gravity correspondence: linking General Relativity and Quantum Field theory

Holographic Geometries from Tensor Network States

Solvable model for a dynamical quantum phase transition from fast to slow scrambling

Introduction to AdS/CFT

Trapped ghost wormholes and regular black holes. The stability problem

Topological Kondo Insulator SmB 6. Tetsuya Takimoto

Potential Descending Principle, Dynamic Law of Physical Motion and Statistical Theory of Heat

Do Cuprates Harbor Extra Dimensions?

Holography of compressible quantum states

An Inverse Mass Expansion for Entanglement Entropy. Free Massive Scalar Field Theory

8.821 String Theory Fall 2008

Quantum fields close to black hole horizons

SM, EWSB & Higgs. MITP Summer School 2017 Joint Challenges for Cosmology and Colliders. Homework & Exercises

8.821 F2008 Lecture 13: Masses of fields and dimensions of operators

Glueballs at finite temperature from AdS/QCD

Lecture 6 The Super-Higgs Mechanism

Theory. V H Satheeshkumar. XXVII Texas Symposium, Dallas, TX December 8 13, 2013

Lecture 9: RR-sector and D-branes

Critical Spin-liquid Phases in Spin-1/2 Triangular Antiferromagnets. In collaboration with: Olexei Motrunich & Jason Alicea

Lecture 24 Seiberg Witten Theory III

Mean field theories of quantum spin glasses

7.4. Why we have two different types of materials: conductors and insulators?

Introduction to Instantons. T. Daniel Brennan. Quantum Mechanics. Quantum Field Theory. Effects of Instanton- Matter Interactions.

Topological phases of SU(N) spin chains and their realization in ultra-cold atom gases

Inverse square potential, scale anomaly, and complex extension

Axial symmetry in the chiral symmetric phase

Théorie des cordes: quelques applications. Cours IV: 11 février 2011

Green s function of the Vector fields on DeSitter Background

Symmetry Groups conservation law quantum numbers Gauge symmetries local bosons mediate the interaction Group Abelian Product of Groups simple

Solutions to gauge hierarchy problem. SS 10, Uli Haisch

Unaprticles: MEELS, ARPES and the Strange Metal

Dual quark condensate and dressed Polyakov loops

Holographic Space Time

arxiv:gr-qc/ v1 11 May 2000

8.821 String Theory Fall 2008

Strange metal from local quantum chaos

AdS/CFT duality. Agnese Bissi. March 26, Fundamental Problems in Quantum Physics Erice. Mathematical Institute University of Oxford

Symmetry, Topology and Phases of Matter

Topological insulator part II: Berry Phase and Topological index

String / gauge theory duality and ferromagnetic spin chains

Beyond the unitarity bound in AdS/CFT

QCD and a Holographic Model of Hadrons

Gauge/Gravity Duality: Applications to Condensed Matter Physics. Johanna Erdmenger. Julius-Maximilians-Universität Würzburg

Metals without quasiparticles

Non-Equilibrium Steady States Beyond Integrability

Topological Insulators in 3D and Bosonization

Landau-Fermi liquid theory

Quantum criticality of Fermi surfaces

Analog Duality. Sabine Hossenfelder. Nordita. Sabine Hossenfelder, Nordita Analog Duality 1/29

Entanglement, holography, and strange metals

NTNU Trondheim, Institutt for fysikk

Topological Physics in Band Insulators II

The Conformal Algebra

The holographic approach to critical points. Johannes Oberreuter (University of Amsterdam)

Emergent gravity. Diana Vaman. Physics Dept, U. Virginia. September 24, U Virginia, Charlottesville, VA

PION DECAY CONSTANT AT FINITE TEMPERATURE IN THE NONLINEAR SIGMA MODEL

Quantum Choreography: Exotica inside Crystals

Introduction to particle physics Lecture 6

Elementary/Composite Mixing in Randall-Sundrum Models

STABILIZING EXTRA DIMENSIONS

10 Thermal field theory

SPT: a window into highly entangled phases

Cold Holographic matter in top-down models

Black holes in the 1/D expansion

ASPECTS OF FREE FERMIONIC HETEROTIC-STRING MODELS. Alon E. Faraggi

Aspects of integrability in classical and quantum field theories

Transcription:

Unparticles and Emergent Mottness Thanks to: NSF, EFRC (DOE) Kiaran dave Charlie Kane Brandon Langley J. A. Hutasoit

Correlated Electron Matter

Correlated Electron Matter What is carrying the current?

fractional quantum Hall effect current-carrying excitations e = e q (q odd)

fractional quantum Hall effect current-carrying excitations e = e q (q odd)

fractional quantum Hall effect current-carrying excitations

fractional quantum Hall effect current-carrying excitations e =?

How Does Fermi Liquid Theory Breakdown? TRSB ρ at? LaSrCuO

How Does Fermi Liquid Theory Breakdown? TRSB ρ at? LaSrCuO

can the charge density be given a particle interpretation?

can the charge density be given a particle interpretation? does charge density= total number of electrons?

if not?

if not? charge stuff= particles + other stuff

if not? charge stuff= particles + other stuff unparticles!

counting particles

counting particles 1

counting particles 2 1

counting particles 2 3 1

counting particles 7 8 5 6 3 2 1 4

counting particles 7 8 5 6 3 2 1 4 is there a more efficient way?

n = µ N(ω)dω µ IR UV

n = µ N(ω)dω µ IR UV can n be deduced entirely from the IR(lowenergy) scale?

Luttinger s `theorem

Luttinger s theorem n =2 k Θ(G(k,ω = 0))

Luttinger s theorem n =2 k Θ(G(k,ω = 0))

Luttinger s theorem G(E) = 1 E ε p n =2 k Θ(G(k,ω = 0)) E>ε p ε p E E<ε p counting poles (qp)

Luttinger s theorem G(E) = 1 E ε p n =2 k Θ(G(k,ω = 0)) zero-crossing E>ε p ε p E ε p E E<ε p counting poles (qp)

Luttinger s theorem G(E) = 1 E ε p n =2 k Θ(G(k,ω = 0)) zero-crossing DetG(ω =0,p)=0 ε p E>ε p E ε p E E<ε p counting poles (qp)

singularities of ln G n = 2i (2π) d+1 d d p 0 dξ ln GR (ξ,p) G R (ξ,p) poles+zeros (all sign changes)

singularities of ln G n = 2i (2π) d+1 d d p 0 dξ ln GR (ξ,p) G R (ξ,p) n =2 k Θ(G(k,ω = 0)) poles+zeros (all sign changes)

what are zeros?

what are zeros? Im G=0 µ =0

what are zeros? Im G=0 µ =0 ReG(0,p)= ( ) dω ω Kramers -Kronig

what are zeros? Im G=0 µ =0 ReG(0,p)= ( ) dω ω Kramers -Kronig = below gap+above gap

what are zeros? Im G=0 µ =0 ReG(0,p)= ( ) dω ω Kramers -Kronig = below gap+above gap = 0

what are zeros? Im G=0 µ =0 ReG(0,p)= ( ) dω ω Kramers -Kronig = below gap+above gap = 0 DetG(k,ω = 0) =0 (single band)

what are zeros? Im G=0 µ =0 ReG(0,p)= ( ) dω ω Kramers -Kronig = below gap+above gap = 0 DetG(k,ω = 0) =0 (single band) strongly correlated gapped systems

NiO insulates d 8? Mott mechanism (not Slater) t

NiO insulates d 8? perhaps this costs energy Mott mechanism (not Slater) t

NiO insulates d 8? perhaps this costs energy Mott mechanism (not Slater) t U t

NiO insulates d 8? perhaps this costs energy Mott mechanism (not Slater) t U t µ =0

NiO insulates d 8? perhaps this costs energy Mott mechanism (not Slater) t U t µ =0 no change in size of Brillouin zone

NiO insulates d 8? perhaps this costs energy Mott mechanism (not Slater) t U t µ =0 no change in size of Brillouin zone DetReG(0,p)=0

NiO insulates d 8? perhaps this costs energy Mott mechanism (not Slater) t U t µ =0 no change in size of Brillouin zone DetReG(0,p)=0 =Mottness

simple problem: n=1 SU(2) U

simple problem: n=1 SU(2) µ U

simple problem: n=1 SU(2) µ U U 2

simple problem: n=1 SU(2) U 2 µ U U 2

simple problem: n=1 SU(2) U 2 µ U U 2 G = 1 ω + U/2 + 1 ω U/2

simple problem: n=1 SU(2) U 2 µ U U 2 G = 1 ω + U/2 + 1 ω U/2 =0 if ω =0

simple problem: n=1 SU(2) U 2 µ U U 2 G = 1 ω + U/2 + 1 ω U/2 n =2θ(0) = 1 =0 if ω =0

Fermi Liquids Mott Insulators Luttinger s theorem

Is this famous theorem from 1960 correct?

A model with zeros but Luttinger fails

A model with zeros but Luttinger fails e t t t t t t t t

A model with zeros but Luttinger fails e t t t t t t t t

A model with zeros but Luttinger fails e t t t t t t t t no hopping=> no propagation (zeros)

A model with zeros but Luttinger fails N flavors e t t t t t of e- t t t no hopping=> no propagation (zeros)

SU(N) H = U 2 (n 1 + n N ) 2 2E 25 N =5 16 4 9 1

SU(N) for N=3: no particle-hole symmetry

SU(N) for N=3: no particle-hole symmetry lim µ(t ) T 0

compute Green function exactly (Lehman formula) G αβ (ω) = 1 Z ab exp βk a Q ab αβ Q ab αβ = a c α bb c β a ω K b + K a + a c β bb c α a ω K a + K b do sum explicitly

G αβ (ω = 0) = δ αβ K(n + 1) K(n) 2n N N

G αβ (ω = 0) = δ αβ K(n + }> 1) K(n) 0 2n N N

G αβ (ω = 0) = δ αβ K(n + }> 1) K(n) 0 2n N N

< 0 G αβ (ω = 0) = δ αβ K(n + }> 1) K(n) 0 2n N N

< 0 > 0 G αβ (ω = 0) = δ αβ K(n + }> 1) K(n) 0 2n N N

a zero must exist < 0 > 0 G αβ (ω = 0) = δ αβ K(n + }> 1) K(n) 0 2n N N

Luttinger s theorem n = NΘ(2n N)

Luttinger s theorem n = NΘ(2n N) { 0, 1, 1/2

Luttinger s theorem n = NΘ(2n N) n =2 N =3 { 0, 1, 1/2

Luttinger s theorem n = NΘ(2n N) n =2 N =3 { 0, 1, 1/2 2=3

Luttinger s theorem n = NΘ(2n N) n =2 N =3 { 0, 1, 1/2 2=3

Luttinger s theorem n = NΘ(2n N) n =2 N =3 { 0, 1, 1/2 even 2=3

Luttinger s theorem n = NΘ(2n N) n =2 N =3 { 0, 1, 1/2 even 2=3 odd

Luttinger s theorem n = NΘ(2n N) n =2 N =3 { 0, 1, 1/2 even 2=3 odd no solution

does the degeneracy matter? e t t t t t t t t t =0 +

G ab (ω) =Tr c a 1 ω H c 1 b + c b ω H c a ρ(0 + )

G ab (ω) =Tr c a 1 ω H c 1 b + c b ω ω H c a ρ(0 + )

G ab (ω) =Tr c a 1 ω H c 1 b + c b ω ω HU c a ρ(0 + )

G ab (ω) =Tr c a 1 ω H c 1 b + c b ω ω HU c a ρ(0 + ) G ab (ω) = ωδ ab Uρ ab ω(ω U)

G ab (ω) =Tr c a 1 ω H c 1 b + c b ω ω HU c a ρ(0 + ) ρ ab =Tr c ac b ρ(0 + ) = u 0 c ac b u 0 G ab (ω) = ωδ ab Uρ ab ω(ω U)

G ab (ω) =Tr c a 1 ω H c 1 b + c b ω ω HU c a ρ(0 + ) ρ ab =Tr c ac b ρ(0 + ) = u 0 c ac b u 0 G ab (ω) = ωδ ab Uρ ab ω(ω U) 1/N diag(1, 1, 1, ) mixed state

G ab (ω) =Tr c a 1 ω H c 1 b + c b ω ω HU c a ρ(0 + ) ρ ab =Tr c ac b ρ(0 + ) = u 0 c ac b u 0 G ab (ω) = ωδ ab Uρ ab ω(ω U) 1/N diag(1, 1, 1, ) mixed state as long as SU(N) symmetry is intact zeros in the wrong place

G ab (ω) =Tr c a 1 ω H c 1 b + c b ω ω HU c a ρ(0 + ) ρ ab =Tr c ac b ρ(0 + ) = u 0 c ac b u 0 G ab (ω) = ωδ ab Uρ ab ω(ω U) 1/N diag(1, 1, 1, ) mixed state as long as SU(N) symmetry is intact zeros in the wrong place limiting procedure: lim lim t 0 ω 0

G ab (ω) =Tr c a 1 ω H c 1 b + c b ω ω HU c a ρ(0 + ) ρ ab =Tr c ac b ρ(0 + ) = u 0 c ac b u 0 G ab (ω) = ωδ ab Uρ ab ω(ω U) 1/N diag(1, 1, 1, ) mixed state as long as SU(N) symmetry is intact zeros in the wrong place limiting procedure: lim lim t 0 ω 0 limits do not commute

Problem DetG =0 G = 1 E ε p =0??

Problem DetG =0 G = 1 E ε p =0?? G = 1 E ε p Σ

Problem DetG =0 G = 1 E ε p =0?? G = 1 E ε p Σ G=0

if Σ is infinite

if Σ is infinite lifetime of a particle vanishes

if Σ is infinite lifetime of a particle Σ < p vanishes

if Σ is infinite lifetime of a particle Σ < p vanishes no particle

what went wrong?

what went wrong? δi[g] = dωσδg

what went wrong? δi[g] = dωσδg if Σ

what went wrong? δi[g] = dωσδg if Σ integral does not exist

what went wrong? δi[g] = dωσδg if Σ integral does not exist No Luttinger theorem!

zeros and particles are incompatible

Luttinger s theorem

are zeros important?

Fermi Arcs

Fermi Arcs

Fermi Arcs Re G Changes Sign across An arc

Fermi Arcs Re G Changes Sign across An arc Must cross A zero line (DetG=0)!!! Fermi arcs necessarily imply zeros exist.

what is seen experimentally? Fermi arcs: no double crossings (PDJ,JCC,ZXS)

what is seen experimentally? Fermi arcs: no double crossings (PDJ,JCC,ZXS) seen infinities not seen zeros E F k

experimental data (LSCO) `Luttinger count k F 1 x FS Bi2212 zeros do not affect the particle density

experimental data (LSCO) `Luttinger count k F 1 x FS Bi2212 zeros do not affect the particle density each hole = a single k-state

where do these zeros come from?

counting electron states need to know: N (number of sites)

counting electron states x = n h /N need to know: N (number of sites)

counting electron states x = n h /N removal states 1 x need to know: N (number of sites)

counting electron states x = n h /N removal states 1 x addition states 1+x need to know: N (number of sites)

counting electron states 2x x = n h /N removal states 1 x addition states 1+x need to know: N (number of sites)

counting electron states 2x x = n h /N removal states 1 x addition states 1+x low-energy electron states 1 x +2x =1+x need to know: N (number of sites)

counting electron states 2x x = n h /N removal states 1 x addition states 1+x low-energy electron states 1 x +2x =1+x high energy 1 x need to know: N (number of sites)

spectral function (dynamics)

spectral function (dynamics)

spectral function (dynamics) density of states 1+x + α>1+x U t Harris and Lange (1967)

spectral function (dynamics) density of states 1+x + α>1+x α t/u U t 1 x α Harris and Lange (1967)

spectral function (dynamics) density of states 1+x + α>1+x α t/u U t 1 x α Harris and Lange (1967) not exhausted by counting electrons alone

how to count particles? 7 8 5 6 3 2 1 4 some charged stuff has no particle interpretation

what is the extra stuff?

scale invariance

new fixed point (scale invariance)?

new fixed point (scale invariance)

new fixed point (scale invariance) unparticles (IR) (H. Georgi)

what is scale invariance? invariance on all length scales

spectral function from scale invariance A(Λω, Λ α k k)=λ α A A(ω, k)

spectral function from scale invariance A(Λω, Λ α k k)=λ α A A(ω, k) k A(ω, k)=ω α A f ω α k

what s the underlying theory?

massive free theory mass L = 1 2 µ φ µ φ + m 2 φ 2

massive free theory mass L = 1 2 µ φ µ φ + m 2 φ 2 x x/λ φ(x) φ(x)

massive free theory mass L = 1 2 µ φ µ φ + m 2 φ 2 x x/λ φ(x) φ(x) m 2 φ 2

massive free theory mass L = 1 2 µ φ µ φ + m 2 φ 2 Λ 2 1 2 µ φ µ φ x x/λ φ(x) φ(x) m 2 φ 2

massive free theory mass L = 1 2 µ φ µ φ + m 2 φ 2 Λ 2 1 2 µ φ µ φ x x/λ φ(x) φ(x) m 2 φ 2

massive free theory mass L = 1 2 µ φ µ φ + m 2 φ 2 Λ 2 1 2 µ φ µ φ x x/λ φ(x) φ(x) m 2 φ 2 no scale invariance

mass sets a scale

unparticles from a massive theory?

L = µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m)

L = µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 dm 2

L = µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 dm 2 theory with all possible mass!

L = µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 dm 2 theory with all possible mass! φ φ(x, m 2 /Λ 2 ) x x/λ m 2 /Λ 2 m 2

L = µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 dm 2 theory with all possible mass! φ φ(x, m 2 /Λ 2 ) x x/λ m 2 /Λ 2 m 2 L Λ 4 L scale invariance is restored!!

L = µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 dm 2 theory with all possible mass! φ φ(x, m 2 /Λ 2 ) x x/λ m 2 /Λ 2 m 2 L Λ 4 L scale invariance is restored!! not particles

unparticles L = µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 dm 2 theory with all possible mass! φ φ(x, m 2 /Λ 2 ) x x/λ m 2 /Λ 2 m 2 L Λ 4 L scale invariance is restored!! not particles

propagator 0 dm 2 m 2γ i p 2 m 2 + i 1 p 2 γ

propagator 0 dm 2 m 2γ i p 2 m 2 + i 1 p 2 γ d U 2

n massless particles G (E ε p ) n 2

n massless particles G (E ε p ) n 2 G (E ε p ) d U 2

n massless particles G (E ε p ) n 2 G (E ε p ) d U 2 unparticles=fractional number of massless particles

n massless particles G (E ε p ) n 2 G (E ε p ) d U 2 unparticles=fractional number of massless particles d U < 2 almost Luttinger liquid no pole at p_f

n massless particles G (E ε p ) n 2 G (E ε p ) d U 2 unparticles=fractional number of massless particles d U > 2 d U < 2 zeros almost Luttinger liquid no pole at p_f

n massless particles G (E ε p ) n 2 G (E ε p ) d U 2 unparticles=fractional number of massless particles d U > 2 d U < 2 zeros no simple sign change almost Luttinger liquid no pole at p_f

no particle interpretation mass-distribution φ U = B(m 2 )φ(m 2 )dm 2 unparticle field (non-canonical) particle field

d U?

what really is the summation over mass?

what really is the summation over mass? mass=energy

L = summation over mass? µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 m 2δ dm 2

L = summation over mass? µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 m 2δ dm 2 m = z 1

L = summation over mass? µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 m 2δ dm 2 m = z 1 L = 0 dz 2R2 z 5+2δ 1 2 z 2 R 2 ηµν ( µ φ)( ν φ)+ φ2 2R 2

L = summation over mass? µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 m 2δ dm 2 m = z 1 L = 0 dz 2R2 z 5+2δ 1 2 z 2 R 2 ηµν ( µ φ)( ν φ)+ φ2 2R 2 can be absorbed with

L = summation over mass? µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 m 2δ dm 2 m = z 1 L = 0 dz 2R2 z 5+2δ 1 2 z 2 R 2 ηµν ( µ φ)( ν φ)+ φ2 2R 2 can be absorbed with ds 2 = R2 z 2 ηµν dx µ dx ν + dz 2

L = summation over mass? µ φ(x, m) µ φ(x, m)+m 2 φ 2 (x, m) 0 m 2δ dm 2 m = z 1 L = 0 dz 2R2 z 5+2δ 1 2 z 2 R 2 ηµν ( µ φ)( ν φ)+ φ2 2R 2 anti de Sitter can be absorbed with space! ds 2 = R2 z 2 ηµν dx µ dx ν + dz 2

generating functional for unparticles action on AdS 5+2δ a Φ a Φ+ Φ2 S = 1 2 d 4+2δ xdz g R 2

generating functional for unparticles action on AdS 5+2δ a Φ a Φ+ Φ2 S = 1 2 d 4+2δ xdz g R 2 ds 2 = L2 z 2 ηµν dx µ dx ν + dz 2 g =(R/z) 5+2δ

generating functional for unparticles action on AdS 5+2δ a Φ a Φ+ Φ2 S = 1 2 d 4+2δ xdz g R 2 ds 2 = L2 z 2 ηµν dx µ dx ν + dz 2 g =(R/z) 5+2δ unparticle lives in d =4+2δ δ 0

gauge-gravity duality (Maldacena, 1997) UV IR gravity QF T

gauge-gravity duality (Maldacena, 1997) UV IR gravity IR?? QF T

gauge-gravity duality (Maldacena, 1997) UV IR gravity IR?? QF T dg(e) dlne = β(g(e)) locality in energy

gauge-gravity duality (Maldacena, 1997) implement E-scaling with an extra dimension UV IR gravity IR?? QF T dg(e) dlne = β(g(e)) locality in energy

Claim: Z QFT = e Son shell ADS (φ(φ ADS=JO ))

Claim: Z QFT = e Son shell ADS (φ(φ ADS=JO )) S = 1 2 d d xg zz g Φ(z,x) z Φ(z,x) z=

Claim: Z QFT = e Son shell ADS (φ(φ ADS=JO )) S = 1 2 d d xg zz g Φ(z,x) z Φ(z,x) z= Φ U (x)φ U (x ) = 1 x x 2d U

Claim: Z QFT = e Son shell ADS (φ(φ ADS=JO )) S = 1 2 d d xg zz g Φ(z,x) z Φ(z,x) z= Φ U (x)φ U (x ) = 1 x x 2d U d U = d 2 + d2 +4 2 > d 2

Claim: Z QFT = e Son shell ADS (φ(φ ADS=JO )) S = 1 2 d d xg zz g Φ(z,x) z Φ(z,x) z= Φ U (x)φ U (x ) = 1 x x 2d U d U = d 2 + d2 +4 2 > d 2 scaling dimension is fixed

G U (p) p 2(d U d/2) d U = d 2 + d2 +4 2 > d 2 G U (0) = 0

unparticle (AdS) propagator has zeros! G U (p) p 2(d U d/2) d U = d 2 + d2 +4 2 > d 2 G U (0) = 0

interchanging unparticles fractional (d_u) number of massless particles

interchanging unparticles fractional (d_u) number of massless particles

interchanging unparticles fractional (d_u) number of massless particles

interchanging unparticles fractional (d_u) number of massless particles

interchanging unparticles fractional (d_u) number of massless particles e iπd U = 1, 0

interchanging unparticles fractional (d_u) number of massless particles e iπd U = 1, 0 fractional statistics in d=2+1

d U = d 2 + d2 +4 2 > d 2 e iπd U = e iπd U time-reversal symmetry breaking from unparticle (zeros=fermi arcs) matter

d ln g d ln β = 4d U d>0 fermions T c unparticles with unparticle propagator BCS g tendency towards pairing (any instability which establishes a gap)

TRSB

TRSB

TRSB unparticles

TRSB unparticles particles

breaking of scale invariance TRSB unparticles particles

emergent gravity High T_c unparticles variable mass

emergent gravity High T_c unparticles variable mass fractional statistics in d=2+1