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HARVARD
International Center for Theoretical SciencesBangalore
June 20, 2015
Subir Sachdev
Talk online: sachdev.physics.harvard.edu
Exploring quantum matter in the high temperature
superconductors
YBa2Cu3O6+x
High temperature superconductors
CuO2 plane
Cu
O
“Undoped”Anti-
ferromagnet
FilledBand
“Undoped”Anti-
ferromagnet
Anti-ferromagnetwith p holesper square
Anti-ferromagnetwith p holesper square
But relative to the band
insulator, there are 1+ p holesper square
SM
FL
Figure: K. Fujita and J. C. Seamus Davis
SM
Antiferromagnet
FL
Figure: K. Fujita and J. C. Seamus Davis
SM
High temperature Superconductor
FL
Figure: K. Fujita and J. C. Seamus Davis
Conventional metal
Area enclosed by Fermi surface =1+p
M. Plate, J. D. F. Mottershead, I. S. Elfimov, D. C. Peets, Ruixing Liang, D. A. Bonn, W. N. Hardy,S. Chiuzbaian, M. Falub, M. Shi, L. Patthey, and A. Damascelli, Phys. Rev. Lett. 95, 077001 (2005)
SM
FL
SM
FL
Figure: K. Fujita and J. C. Seamus Davis
Pseudogap
“Fermi arcs” at
low p
Kyle M. Shen, F. Ronning, D. H. Lu, F. Baumberger, N. J. C. Ingle, W. S. Lee, W. Meevasana,Y. Kohsaka, M. Azuma, M. Takano, H. Takagi, Z.-X. Shen, Science 307, 901 (2005)
SM
FL
Strange metal
Metal(gapless,
compressible state)
without quasi-
particles
SM
FL
1. The pseudogap metal
Fermi liquid co-existening with topological order
2. The strange metal
Metal without quasiparticles
Infinite-range model: dual to extremal charged
black holes and yields
Bekenstein-Hawking entropy
Outline
Pseudogap
“Fermi arcs” at
low p
Kyle M. Shen, F. Ronning, D. H. Lu, F. Baumberger, N. J. C. Ingle, W. S. Lee, W. Meevasana,Y. Kohsaka, M. Azuma, M. Takano, H. Takagi, Z.-X. Shen, Science 307, 901 (2005)
SM
FL
A new metal — a fractionalized
Fermi liquid (FL*) — with electron-like quasiparticles on a Fermi surface of size p coexisting
with topological order
Y. Qi and S. Sachdev, Phys. Rev. B 81, 115129 (2010)M. Punk, A. Allais, and S. Sachdev, arXiv:1501.00978
SM
FL
Pseudogap
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
A fermionic “dimer” describing a “bonding” orbital between two sites
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Fractionalized Fermi liquid (FL*)
T. Senthil, S. S., M. Vojta Phys. Rev. Lett. 90, 216403 (2003) R. K. Kaul, A. Kolezhuk, M. Levin, S. S., and T. Senthil, Phys. Rev. B 75, 235122 (2007)
E. G. Moon and S. S. Phys. Rev. B 83, 224508 (2011); M. Punk, A. Allais, and S. S., arXiv:1501.00978.
= | ⇥⇤⌅ � | ⇤⇥⌅
Realizes a metal with a
Fermi surface of
area p co-existing
with “topological
order”
Place pseudogap metal on a
torus;
Topological order
Place pseudogap metal on a
torus;obtain
“topological” states nearly degenerate
with the ground state: change sign of every dimer
across red line
Topological order
= | ⇥⇤⌅ � | ⇤⇥⌅
Topological order Place
pseudogap metal on a
torus;obtain
“topological” states nearly degenerate
with the ground state: change sign of every dimer
across red line
= | ⇥⇤⌅ � | ⇤⇥⌅
-1 -1-1-1
Topological order Place
pseudogap metal on a
torus;obtain
“topological” states nearly degenerate
with the ground state: change sign of every dimer
across red line
= | ⇥⇤⌅ � | ⇤⇥⌅
-1-1
Topological order Place
pseudogap metal on a
torus;obtain
“topological” states nearly degenerate
with the ground state: change sign of every dimer
across red line
= | ⇥⇤⌅ � | ⇤⇥⌅
-1 -1-1-1
Topological order Place
pseudogap metal on a
torus;obtain
“topological” states nearly degenerate
with the ground state: change sign of every dimer
across red line
A new metal — a fractionalized
Fermi liquid (FL*) — with electron-like quasiparticles on a Fermi surface of size p coexisting
with topological order
Y. Qi and S. Sachdev, Phys. Rev. B 81, 115129 (2010)M. Punk, A. Allais, and S. Sachdev, arXiv:1501.00978
SM
FL
Pseudogap
1. The pseudogap metal
Fermi liquid co-existening with topological order
2. The strange metal
Metal without quasiparticles
Infinite-range model: dual to extremal charged
black holes and yields
Bekenstein-Hawking entropy
Outline
Strange metal
Metal(gapless,
compressible state)
without quasi-
particles
SM
FL
Q =1
N
X
i
Dc†i ci
E.
H =1
(2N)3/2
NX
i,j,k,`=1
Jij;k` c†i c
†jckc`
1 23 4
5 6
78
9
10
11 12
12 1314
J3,5,7,13J4,5,6,11
J8,9,12,14
cicj + cjci = 0
cic†j + c†jci = �ij
Jij;k` independent
random numbers
An infinite-range model of a strange metal
S. Sachdev and J. Ye, Phys. Rev. Lett. 70, 3339 (1993)A. Kitaev, unpublished
S. Sachdev, arXiv:1506.05111
Q =1
N
X
i
Dc†i ci
E.
H =1
(2N)3/2
NX
i,j,k,`=1
Jij;k` c†i c
†jckc`
1 23 4
5 6
78
9
10
11 12
12 1314
J3,5,7,13J4,5,6,11
J8,9,12,14
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
cicj + cjci = 0
cic†j + c†jci = �ij
Jij;k` independent
random numbers
S. Sachdev and J. Ye, Phys. Rev. Lett. 70, 3339 (1993)
Q =1
N
X
i
Dc†i ci
E.
H =1
(2N)3/2
NX
i,j,k,`=1
Jij;k` c†i c
†jckc`
1 23 4
5 6
78
9
10
11 12
12 1314
J3,5,7,13J4,5,6,11
J8,9,12,14
Known ‘equation of state’
determines E as a function of Q
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
cicj + cjci = 0
cic†j + c†jci = �ij
Jij;k` independent
random numbers
A. Georges, O. Parcollet, and S. Sachdev Phys. Rev. B 63, 134406 (2001)
Q =1
4(3� tanh(2⇡E))� 1
⇡tan�1
�e2⇡E
�
Q =1
N
X
i
Dc†i ci
E.
H =1
(2N)3/2
NX
i,j,k,`=1
Jij;k` c†i c
†jckc`
1 23 4
5 6
78
9
10
11 12
12 1314
J3,5,7,13J4,5,6,11
J8,9,12,14
Known ‘equation of state’
determines E as a function of Q
Microscopic zero temperature
entropy density, S, obeys@S@Q = 2⇡E
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
cicj + cjci = 0
cic†j + c†jci = �ij
Jij;k` independent
random numbers
O. Parcollet, A. Georges, G. Kotliar, and A. Sengupta Phys. Rev. B 58, 3794 (1998)
A. Georges, O. Parcollet, and S. Sachdev Phys. Rev. B 63, 134406 (2001)
Q =1
N
X
i
Dc†i ci
E.
H =1
(2N)3/2
NX
i,j,k,`=1
Jij;k` c†i c
†jckc`
1 23 4
5 6
78
9
10
11 12
12 1314
J3,5,7,13J4,5,6,11
J8,9,12,14
Known ‘equation of state’
determines E as a function of Q
Microscopic zero temperature
entropy density, S, obeys@S@Q = 2⇡E
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
Einstein-Maxwell theory
+ cosmological constant
Q =1
N
X
i
Dc†i ci
E.
H =1
(2N)3/2
NX
i,j,k,`=1
Jij;k` c†i c
†jckc`
1 23 4
5 6
78
9
10
11 12
12 1314
J3,5,7,13J4,5,6,11
J8,9,12,14
Known ‘equation of state’
determines E as a function of Q
Microscopic zero temperature
entropy density, S, obeys@S@Q = 2⇡E
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
Einstein-Maxwell theory
+ cosmological constant
Boundary
area Ab;
charge
density Q
⇣~x
Horizon area Ah;AdS2 ⇥R
d
ds
2 = (d⇣2 � dt
2)/⇣2 + d~x
2
Gauge field: A = (E/⇣)dt
⇣ = 1
A. Chamblin, R. Emparan, C. V. Johnson, and R.C. Myers Phys. Rev. D 60, 064018 (1999)
Q =1
N
X
i
Dc†i ci
E.
H =1
(2N)3/2
NX
i,j,k,`=1
Jij;k` c†i c
†jckc`
1 23 4
5 6
78
9
10
11 12
12 1314
J3,5,7,13J4,5,6,11
J8,9,12,14
Known ‘equation of state’
determines E as a function of Q
Microscopic zero temperature
entropy density, S, obeys@S@Q = 2⇡E
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
Einstein-Maxwell theory
+ cosmological constant
Boundary
area Ab;
charge
density Q
⇣~x
Horizon area Ah;AdS2 ⇥R
d
ds
2 = (d⇣2 � dt
2)/⇣2 + d~x
2
Gauge field: A = (E/⇣)dt
⇣ = 1
L = �↵D↵ +m
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
T. Faulkner, Hong Liu, J. McGreevy, and D. Vegh Phys. Rev. D 83, 125002 (2011)
Q =1
N
X
i
Dc†i ci
E.
H =1
(2N)3/2
NX
i,j,k,`=1
Jij;k` c†i c
†jckc`
1 23 4
5 6
78
9
10
11 12
12 1314
J3,5,7,13J4,5,6,11
J8,9,12,14
Known ‘equation of state’
determines E as a function of Q
Microscopic zero temperature
entropy density, S, obeys@S@Q = 2⇡E
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
Einstein-Maxwell theory
+ cosmological constant
Boundary
area Ab;
charge
density Q
⇣~x
Horizon area Ah;AdS2 ⇥R
d
ds
2 = (d⇣2 � dt
2)/⇣2 + d~x
2
Gauge field: A = (E/⇣)dt
⇣ = 1
L = �↵D↵ +m
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
‘Equation of state’ relating Eand Q depends upon the geometry
of spacetime far from the AdS2
S. Sachdev, arXiv:1506.05111
Eliminate r0 between
Q =rd�10
p2d [(d� 1)R2 + (d+ 1)r20]
2gF
E =gF r0
p2d [(d� 1)R2 + (d+ 1)r20]
2 [(d� 1)2R2 + d(d+ 1)r20]
Q =1
N
X
i
Dc†i ci
E.
H =1
(2N)3/2
NX
i,j,k,`=1
Jij;k` c†i c
†jckc`
1 23 4
5 6
78
9
10
11 12
12 1314
J3,5,7,13J4,5,6,11
J8,9,12,14
Known ‘equation of state’
determines E as a function of Q
Microscopic zero temperature
entropy density, S, obeys@S@Q = 2⇡E
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
Einstein-Maxwell theory
+ cosmological constant
Boundary
area Ab;
charge
density Q
⇣~x
Horizon area Ah;AdS2 ⇥R
d
ds
2 = (d⇣2 � dt
2)/⇣2 + d~x
2
Gauge field: A = (E/⇣)dt
⇣ = 1
L = �↵D↵ +m
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
‘Equation of state’ relating Eand Q depends upon the geometry
of spacetime far from the AdS2
S. Sachdev, arXiv:1506.05111
Black hole thermodynamics
(classical GR) yields
1
Ab
@Ah
@Q = 8⇡GNE
Q =1
N
X
i
Dc†i ci
E.
H =1
(2N)3/2
NX
i,j,k,`=1
Jij;k` c†i c
†jckc`
1 23 4
5 6
78
9
10
11 12
12 1314
J3,5,7,13J4,5,6,11
J8,9,12,14
Known ‘equation of state’
determines E as a function of Q
Microscopic zero temperature
entropy density, S, obeys@S@Q = 2⇡E
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
Einstein-Maxwell theory
+ cosmological constant
Boundary
area Ab;
charge
density Q
⇣~x
Horizon area Ah;AdS2 ⇥R
d
ds
2 = (d⇣2 � dt
2)/⇣2 + d~x
2
Gauge field: A = (E/⇣)dt
⇣ = 1
L = �↵D↵ +m
Local fermion density of states
⇢(!) ⇠⇢
!�1/2 , ! > 0
e�2⇡E |!|�1/2, ! < 0.
‘Equation of state’ relating Eand Q depends upon the geometry
of spacetime far from the AdS2
S. Sachdev, arXiv:1506.05111
Black hole thermodynamics
(classical GR) yields
1
Ab
@Ah
@Q = 8⇡GNE
Combination:
S =
Ah
4GNAb
SM
FL
Figure: K. Fujita and J. C. Seamus Davis
Pseudogap Strange metal
1. The pseudogap metal
Fermi liquid co-existening with topological order
2. The strange metal
Metal without quasiparticles
Infinite-range model: dual to extremal charged
black holes and yields
Bekenstein-Hawking entropy