Quantum Phase Transitions in Fermi Liquids

Similar documents
3. Quantum matter without quasiparticles

Fermi Liquid and BCS Phase Transition

Landau s Fermi Liquid Theory

Quantum criticality of Fermi surfaces

Wilsonian and large N theories of quantum critical metals. Srinivas Raghu (Stanford)

Notes on Renormalization Group: ϕ 4 theory and ferromagnetism

A non-fermi liquid: Quantum criticality of metals near the Pomeranchuk instability

Kolloquium Universität Innsbruck October 13, The renormalization group: from the foundations to modern applications

Part III: Impurities in Luttinger liquids

2D Bose and Non-Fermi Liquid Metals

Manifestly diffeomorphism invariant classical Exact Renormalization Group

Low dimensional interacting bosons

MODEL WITH SPIN; CHARGE AND SPIN EXCITATIONS 57

Metals without quasiparticles

Towards a manifestly diffeomorphism invariant Exact Renormalization Group

Many-Body Problems and Quantum Field Theory

REVIEW REVIEW. Quantum Field Theory II

Quantum Field Theory II

Phase Transitions and Renormalization:

Fermi liquids and fractional statistics in one dimension

Lecture 6. Fermion Pairing. WS2010/11: Introduction to Nuclear and Particle Physics

Magnets, 1D quantum system, and quantum Phase transitions

What is a particle? Keith Fratus. July 17, 2012 UCSB

Maxwell s equations. electric field charge density. current density

Holographic superconductors

Majorana Fermions in Superconducting Chains

Quantum phase transitions of insulators, superconductors and metals in two dimensions

Effective Field Theory Methods in Atomic and Nuclear Physics

Many-Body Fermion Density Matrix: Operator-Based Truncation Scheme

Renormalization Group Methods for the Nuclear Many-Body Problem

Fermi surfaces which produce large transverse magnetoresistance. Abstract

The phase diagram of the cuprates and the quantum phase transitions of metals in two dimensions

Universal theory of complex SYK models and extremal charged black holes

Review of scalar field theory. Srednicki 5, 9, 10

Holographic Branching and Entanglement Renormalization

Summary of free theory: one particle state: vacuum state is annihilated by all a s: then, one particle state has normalization:

Contents. 1.1 Prerequisites and textbooks Physical phenomena and theoretical tools The path integrals... 9

An imbalanced Fermi gas in 1 + ɛ dimensions. Andrew J. A. James A. Lamacraft

Exotic phases of the Kondo lattice, and holography

Quantum critical metals and their instabilities. Srinivas Raghu (Stanford)

Fermi liquid theory Can we apply the free fermion approximation to a real metal? Phys540.nb Strong interaction vs.

Quantum Algorithms for Quantum Field Theories

Tunneling Into a Luttinger Liquid Revisited

Emergent Quantum Criticality

Preface Introduction to the electron liquid

Chap.9 Fixed points and exponents

Some Mathematical Aspects of the Renormalization Group

LSZ reduction for spin-1/2 particles

REVIEW REVIEW. A guess for a suitable initial state: Similarly, let s consider a final state: Summary of free theory:

A FERMI SEA OF HEAVY ELECTRONS (A KONDO LATTICE) IS NEVER A FERMI LIQUID

Strongly correlated Cooper pair insulators and superfluids

The continuum limit of the integrable open XYZ spin-1/2 chain

Lecture 20: Effective field theory for the Bose- Hubbard model

Quantum Field Theory. Kerson Huang. Second, Revised, and Enlarged Edition WILEY- VCH. From Operators to Path Integrals

The underdoped cuprates as fractionalized Fermi liquids (FL*)

Landau-Fermi liquid theory

The path integral for photons

Density Waves and Supersolidity in Rapidly Rotating Atomic Fermi Gases

Intertwined Orders in High Temperature Superconductors

Spin-orbital separation in the quasi-one-dimensional Mott insulator Sr 2 CuO 3 Splitting the electron

Quantum disordering magnetic order in insulators, metals, and superconductors

PH575 Spring Lecture #26 & 27 Phonons: Kittel Ch. 4 & 5

FRG approach to interacting fermions with partial bosonization: from weak to strong coupling

Which Spin Liquid Is It?

Quantum Quenches in Extended Systems

Condensed matter theory Lecture notes and problem sets 2012/2013

Phase Transitions in Condensed Matter Spontaneous Symmetry Breaking and Universality. Hans-Henning Klauss. Institut für Festkörperphysik TU Dresden

I. Collective Behavior, From Particles to Fields

Landau-Fermi liquid theory

Section B. Electromagnetism

Attempts at relativistic QM

REFLECTIONS ON THE PAST, PRESENT AND FUTURE OF CONDENSED MATTER PHYSICS. A. J. Leggett

General relativity and the cuprates

Enhancing Superconductivity by Disorder

Quantum Spin Liquids and Majorana Metals

Quantum Field Theory II

Physics 212: Statistical mechanics II Lecture XI

(r) 2.0 E N 1.0

Broken Symmetries in the One-Dimensional Extended Hubbard Model

Two Dimensional Many Fermion Systems as Vector Models

Outline for Fundamentals of Statistical Physics Leo P. Kadanoff

Chapter 4: Summary. Solve lattice vibration equation of one atom/unitcellcase Consider a set of ions M separated by a distance a,

Physics 562: Statistical Mechanics Spring 2003, James P. Sethna Homework 5, due Wednesday, April 2 Latest revision: April 4, 2003, 8:53 am

Who is afraid of quadratic divergences? (Hierarchy problem) & Why is the Higgs mass 125 GeV? (Stability of Higgs potential)

Continuum limit of fishnet graphs and AdS sigma model

Let There Be Topological Superconductors

Quasi-1d Antiferromagnets

The general solution of Schrödinger equation in three dimensions (if V does not depend on time) are solutions of time-independent Schrödinger equation

Ising Model and Renormalization Group

ɛ(k) = h2 k 2 2m, k F = (3π 2 n) 1/3

Renormalization Group for the Two-Dimensional Ising Model

Applications of Renormalization Group Methods in Nuclear Physics 2

3 Symmetry Protected Topological Phase

Lattice modulation experiments with fermions in optical lattices and more

Quantum gases in the unitary limit and...

Particle Physics Today, Tomorrow and Beyond. John Ellis

Finite Temperature Field Theory

Mathematical Analysis of the BCS-Bogoliubov Theory

A Renormalization Group Primer

Metal-Insulator Transitions in a model for magnetic Weyl semimetal and graphite under high magnetic field

Transcription:

Quantum Phase Transitions in Fermi Liquids in d=1 and higher dimensions Mihir Khadilkar Kyungmin Lee Shivam Ghosh PHYS 7653 December 2, 2010

Outline 1 Introduction 2 d = 1: Mean field vs RG Model 3 Higher Dimensions d = 2 Circular Fermi Surface Other Fermi Surfaces 4 Conclusions

Revision Last time Mihir talked about what is a Fermi liquid Replace interacting electron system by weakly interacting quasiparticles Renormalize interactions between quasiparticles Kyungmin did the calculations for complex scalar field We will now talk about a real system

What are spinless fermions? Fermions, but no spin-spin interaction in the Hamiltonian Exclusion principle still applies Can think of it as electrons in a very high external field The instabilities of the Fermi liquid are due to the features of the Fermi surface Actual instabilities are different but crucial feature will turn out to be the surface itself

What are spinless fermions? Fermions, but no spin-spin interaction in the Hamiltonian Exclusion principle still applies Can think of it as electrons in a very high external field The instabilities of the Fermi liquid are due to the features of the Fermi surface Actual instabilities are different but crucial feature will turn out to be the surface itself

Model d = 1: Mean field vs RG

Model The Model H = H 0 + H I = 1 2 X j X + U 0 (n j with n j = y (j) (j) j y (j + 1) (j) + y (j) (j + 1) 1 2 )(n j+1 and f y (j); (m)g = mj 1 2 ) We will work at half filling For spinless fermions, this means 1 2 particle per site

Model The Model H = H 0 + H I = 1 2 X j X + U 0 (n j with n j = y (j) (j) j y (j + 1) (j) + y (j) (j + 1) 1 2 )(n j+1 and f y (j); (m)g = mj 1 2 ) We will work at half filling For spinless fermions, this means 1 2 particle per site

Model In the limit U0 = 0 H = H 0 Taking Fourier transform and solving, Z dk y H 0 = (K) (K)E(K) 2 E(K) = cos K Fermi surface consists of two points Π Π 2 Π 2 Π K F = =2

Model In the limit U0! 1 X H = H I = U 0 (n j j 1 2 )(n j+1 1 2 ) Only nearest neighbour repulsion Ground state when there are no nearest neighbours Alternate sites occupied Charge density wave ordering (CDW): hn j i = 1 2 + ( 1)j 1 2

Model 1

Model Mean Field Result, n j = hn j i How does depend upon U 0? = U 0 e 2U 0 This is non-zero for all non-zero U 0 This suggests that we will get CDW at arbitrarily small U 0 Similar result for arbitrarily small negative U 0 Cooper pair formation leads to superconductivity

Model Mean Field Result, n j = hn j i How does depend upon U 0? = U 0 e 2U 0 This is non-zero for all non-zero U 0 This suggests that we will get CDW at arbitrarily small U 0 Similar result for arbitrarily small negative U 0 Cooper pair formation leads to superconductivity

Model THIS IS WRONG

Model The Answer The system forms a Luttinger liquid Some of the differences from Fermi liquid: Excitations are not quasiparticles, but collective excitations of charge and spin (spinons and holons) Non-universal critical exponents depending on Luttinger liquid exponent Depends upon interaction strength This can be thought of as a system having a line of fixed points No flow along this line

Formulation of problem We will consider excitations near the Fermi surface Different from complex scalar field because there are two points Π Π 2 Π 2 Π Inter-branch excitations can occur Umklapp processes also possible

Formulation of problem We will consider excitations near the Fermi surface Different from complex scalar field because there are two points Π Π 2 Π 2 Π Inter-branch excitations can occur Umklapp processes also possible

Formulation of problem X Z H 0 = i=l;r dk 2 y i (k) i(k)k with k = jkj K F Note that E(K) has been linearized about K F. We are looking at excitations within a cutoff

Formulation of problem X Z H 0 = i=l;r dk 2 y i (k) i(k)k with k = jkj K F Note that E(K) has been linearized about K F. We are looking at excitations within a cutoff

Road map for the analysis Write down partition function Z 0 and free field action S 0 Find RG transformation which lowers cutoff keeping S 0 constant Introduce perturbations to this fixed point Try to find flow equations

Road map for the analysis Write down partition function Z 0 and free field action S 0 Find RG transformation which lowers cutoff keeping S 0 constant Introduce perturbations to this fixed point Try to find flow equations

Road map for the analysis Write down partition function Z 0 and free field action S 0 Find RG transformation which lowers cutoff keeping S 0 constant Introduce perturbations to this fixed point Try to find flow equations

Road map for the analysis Write down partition function Z 0 and free field action S 0 Find RG transformation which lowers cutoff keeping S 0 constant Introduce perturbations to this fixed point Try to find flow equations

Partition function and free field action Z 0 = Z Y Y d i(!; k)d i (!; k)e S0 i=l;r jkj< X Z Z dk 1 d! S 0 = i (!; k)(i! k) i (!; k) 2 i=l;r 1 2 Compare with the complex scalar action: Z S 2 = d d x (R 0 j(x)j 2 + R 2 jrj 2 ) which when Fourier transformed, gives: S 2 = Z jkj< d d k (2) d (r 0 + r 2 k 2 ) (k)(k)

Partition function and free field action Z 0 = Z Y Y d i(!; k)d i (!; k)e S0 i=l;r jkj< X Z Z dk 1 d! S 0 = i (!; k)(i! k) i (!; k) 2 i=l;r 1 2 Compare with the complex scalar action: Z S 2 = d d x (R 0 j(x)j 2 + R 2 jrj 2 ) which when Fourier transformed, gives: S 2 = Z jkj< d d k (2) d (r 0 + r 2 k 2 ) (k)(k)

Rescaling and renormalization We want to integrate out all the "fast" modes ( =s jkj ) Since S 0 is quadratic, slow and fast modes separate Coarse-graining reduces! =s To get back original action, k 0 = sk! 0 = s! 0 i (k0 ;! 0 ) = s 3=2 i(k;!) We can now consider perturbations to this fixed point action

Rescaling and renormalization We want to integrate out all the "fast" modes ( =s jkj ) Since S 0 is quadratic, slow and fast modes separate Coarse-graining reduces! =s To get back original action, k 0 = sk! 0 = s! 0 i (k0 ;! 0 ) = s 3=2 i(k;!) We can now consider perturbations to this fixed point action

Quadratic perturbations S 2 = X i=l;r Z Z dk 1 2 1 d! 2 (!; k) i(!; k) i (!; k) Again, slow and fast modes separate out Coupling rescales as 0 (! 0 ; k 0 ) = s(!; k) Taylor expanding, we see that only the constant term 0 is relevant Readjustment of the chemical potential

Quadratic perturbations S 2 = X i=l;r Z Z dk 1 2 1 d! 2 (!; k) i(!; k) i (!; k) Again, slow and fast modes separate out Coupling rescales as 0 (! 0 ; k 0 ) = s(!; k) Taylor expanding, we see that only the constant term 0 is relevant Readjustment of the chemical potential

Quartic perturbations S 4 = 1 4 Z K! where (i) = (K i ;! i ) Z = K! 2 Y 4 4 j=1 Z dk j 2 (4) (3) (2) (1)u(4; 3; 2; 1) Z 1 1 d! j 2 3 5 [2 (K 1 + K 2 K 3 K 4 )2(! 1 +! 2! 3! 4 )]

Order-u level Analysis At the order-u level, only tree-level and tadpole diagrams survive Tree-level Simple change in cutoff, leading to renormalized coupling u 0 (k 0 ;! 0 ) = u(k;!) Thus, we get that only the constant term u 0 is marginal; rest irrelevant Tadpole As before the tadpole graph graph renormalizes the quadratic coupling d = u0 d` 2 TADPOLE TREE LEVEL

Order-u level Analysis At the order-u level, only tree-level and tadpole diagrams survive Tree-level Simple change in cutoff, leading to renormalized coupling u 0 (k 0 ;! 0 ) = u(k;!) Thus, we get that only the constant term u 0 is marginal; rest irrelevant Tadpole As before the tadpole graph graph renormalizes the quadratic coupling d = u0 d` 2 TADPOLE TREE LEVEL

Order-u 2 Analysis Feynman Diagrams with one Loop

3 4 3 4 1 2 ZS 3 4 1 2 ZS 1 2 BCS

Order-u 2 Analysis We must consider the three graphs, ZS, ZS and BCS On doing the integrals, we see that du = 0 d` ZS du ZS0 = u2 d` du d` = BCS Thus, we get the flow equation du d` = 0 2 u 2 2

Order-u 2 Analysis We must consider the three graphs, ZS, ZS and BCS On doing the integrals, we see that du = 0 d` ZS du ZS0 = u2 d` du d` = BCS Thus, we get the flow equation du d` = 0 2 u 2 2

So... du d` = 0 ; d d` = u 0 2 Interaction strength does not flow Quadratic coupling gives change in chemical potential Kept constant to keep number density of particles constant Luttinger liquid

Higher Dimensions

d = 2 Circular Fermi Surface d = 2 Now you have a Fermi surface instead of a discrete number of points We must integrate over all of these directions In 1-d, we had u LRLR Now we have u[ 4 ; 3 ; 2 ; 1 ] in 2-d But only two angles are independent Two distinct cases: u[ 2 ; 1 ; 2 ; 1 ] = F ( 1 ; 2 ) and u[ 3 ; 3 ; 1 ; 1 ] = V ( 1 ; 3 )

d = 2 Circular Fermi Surface d = 2 Now you have a Fermi surface instead of a discrete number of points We must integrate over all of these directions In 1-d, we had u LRLR Now we have u[ 4 ; 3 ; 2 ; 1 ] in 2-d But only two angles are independent Two distinct cases: u[ 2 ; 1 ; 2 ; 1 ] = F ( 1 ; 2 ) and u[ 3 ; 3 ; 1 ; 1 ] = V ( 1 ; 3 )

d = 2 Circular Fermi Surface d = 2 Now you have a Fermi surface instead of a discrete number of points We must integrate over all of these directions In 1-d, we had u LRLR Now we have u[ 4 ; 3 ; 2 ; 1 ] in 2-d But only two angles are independent Two distinct cases: u[ 2 ; 1 ; 2 ; 1 ] = F ( 1 ; 2 ) and u[ 3 ; 3 ; 1 ; 1 ] = V ( 1 ; 3 )

d = 2 Circular Fermi Surface Flows Convenient to examine flows of V l = R 2 0 dv l dt = cvl 2, c>0 If even one coupling is negative, we get flow d 2 eil v() Cooper pair formation leading to BCS fixed point

Other Fermi Surfaces Other Fermi Surfaces For 3D spherical Fermi surface, same result For non-circular Fermi surfaces, result depends on whether there is time-reversal invariance Nested Fermi surfaces are special New coupling constant W flows to CDW state

Other Fermi Surfaces Other Fermi Surfaces For 3D spherical Fermi surface, same result For non-circular Fermi surfaces, result depends on whether there is time-reversal invariance Nested Fermi surfaces are special New coupling constant W flows to CDW state

Other Fermi Surfaces Π Π 0 K N Π, Π 0 Π Π

Conclusions For system of 1D spinless Fermions Mean field analysis gives wrong result for small U 0 Luttinger liquid scale invariant system formed For higher dimensions, we see flows to BCS instabilities Nested Fermi surfaces produce charge density wave Now Shivam will talk about spin-spin interactions