ondas de densidade de carga em 1d: hubbard vs. luttinger? thereza paiva (uc-davis) e raimundo r dos...
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Ondas de densidade de carga em 1D:
Hubbard vs. Luttinger?
Thereza Paiva (UC-Davis)
e
Raimundo R dos Santos (UFRJ)
Work supported by Brazilian agencies and
Outline
• Motivation
• Luttinger liquid description
• Hubbard model
• Hubbard superlattices
• Conclusions
• (References)
Motivation
Strongly correlated electrons: interplay between charge and spin degrees of freedom
determines magnetic and transport (including superconducting) properties
Quasi-2D example: high Tc superconductors
Striped phase?
Stripes in CuO2 planes
[from Kivelson et al., (‘99)]
Direction of charge modulation
1D examples: organic conductors,…
[from Gruner (‘94)]
Chain direction
SeC
F
P
Spin density waves disappear for P ~ 6.0 kbar and triplet superconductivitysets in [Lee et al. (00)]
... quantum wires, carbon nanotubes, etc.
Here: focus on charge distribution
Charge-density waves
Well known example of CDW: the Peierls instability
Electron-phonon couplingleads to a modulation of thecharge distribution:
Dynamics of collective modes (x,t)
t
ejCDW
e.g., TTF-TCNQ, NbSe3,...
Here: interested only in effects of e--e- interactions on CDW’s
[from Gruner (88)]
Luttinger Liquid (LL) description
• Excitations: Fermi Liquid theoryFermi gas Fermi liquid (interactions on)
quasi-particlesare fermions
n
FF
nT=0
• OK in 3D• ? in 2D• Breaks down in 1D (Peierls instability) need new framework
• The Luttinger model [Voit (‘94)]
q
kF
kF
g2
kF
kF
qg4
Linear dispersion
Gapless excitations
Forward scattering (i.e. momentum transfer q << 2kF):
Effect of dimensionality and spin-charge seperation:• Let us inject an e- in 2nd plane-wave state, |2, above Fermi surface• g4 only connects |2 to |1, the 1st plane wave state above Fermi surface
Effective Hamiltonian in this subspace:
L
v
L
gL
g
L
v
HF
d
dF
eff
42
24
4
4
,4
Thus, g4 irrelevant (RG: L ) for d=3, but marginal for d=1
Diagonalizing H4,eff yields
u= vF + g4/2 velocity of charge excitations
u= vF g4/2 velocity of spin excitations
u u spin-charge separation
Solution of the Luttinger modelNote low-T specific heat for fermions: C ~ Tc.f., low-T specific heat for d-dimensional bosons with k s : C ~ T d/s linear for d=s=1
Quasi-particles are bosons soluble via bosonization
• Charge-density correlation function
KF
KF
x
x)kA
xx
xkA
x
Kxnn 422/31 12
4cos(
ln
)2cos(
)()()0(
K is a non-universal (interaction-dependent) exponent
2kF n, where n is electron density
2kF dominates if 1K 4K K 1/3
• Other measurable quantities– Specific heat: C = T
where 2 = 0 vF [u-1
+ u -1], with 0 = 2 kB
2 /3vF
– Spin susceptibility: = 2 K / u
– Compressibility: = 2 K / u
– Drude weight (DC conductivity): D = 2 u K
• Parametrization of theory
(u, K) and (u, K)
depend on the coupling constants g2 & g4
• The Luttinger Liquid conjecture
The LL is believed to provide the (gapless) low-energy phenomenology for all 1D metals
• LL theory of single-wall metallic nanotubes:
2/12
)2/ln(8
1
R
v
eg
F
dielectric constanttube length tube radius
g ~ 0.2; c.f. g = 1 for Fermi gas
LL behaviour observed through tunnelling experiments[see Egger et al. (‘00)]
The Hubbard model• Simplest lattice model to include correlations:
Tight binding with one orbital per site Coulomb repulsion: on-site only Nearest neighbour hoppings only
i
iiiii
ii nnUcccctH ][ ,,1,
,1,
• Bethe ansatz solution [Lieb & Wu (‘68)] Ground state but not correlation functions
• Connection with LL [Schulz(90)]:
K
u
n
nE
L 2
)(12
02
system size
Calculated from Bethe ansatz solution
K (n,U)
K 1/2 2kF charge mode dominates over 4kF
c.f. early Renormalization Group predictions [Sólyom(‘79)]
• Quantum Monte Carlo (world-line) simulations [Hirsch & Scalapino (83,84)]:
first suggestions of 4kF charge mode dominating over 2kF as U increases
attributed to finite-temperature effects; should not prevail at lower temperatures
Is it really so?
x
= M
Ns
M
The space–imaginary-time lattice for QMC simulations
)(det)(det OOTrZ
/
/
s
sAA
The “minus-sign problem”:
Sign of det ·det
T 0: Quantum Monte Carlo (determinantal) simulations
Charge susceptibility:
As U increases, 4kF susceptibility still grows as T 0, while 2kF
seems to stabilize. (Ns 36 sites)
Neither finite-size nor finite-temperature effects: simulations with Ns 96
N(4kF) ln
n 1/6
[Paiva & dS (00a)]
0,0 0,2 0,4 0,6 0,8 1,0
-0,10
-0,05
0,00
0,05
0,10
0,15
0,20
U=0 U=2 U=4 U=6 U=9 U=12 U=20
n =1/6 NS=24
C(q
)
q/
T 0: Lanczos diagonalizations on finite-sized lattices
…and is notis not a finite-sizeeffect: cusps get sharperas Ns increases
As U increases the cuspmoves towards 4kF ...
n 1/6
0,0 0,2 0,4 0,6 0,8 1,0
0,00
0,05
0,10
0,15
0,20
U=3 NS=12
U=12 NS=12
U=3 NS=24
U=12 NS=24
n =1/6 NS=12 and NS=24
C(q
)
q/
The same happens for other occupations
n 1/3
n 1/2
0,0 0,2 0,4 0,6 0,8 1,0-0,2
-0,1
0,0
0,1
0,2
0,3
U=0 U=4 U=6 U=8 U=9 U=12 U=20
Ns=18 n=1/3
C(q
)
q/
0,0 0,2 0,4 0,6 0,8 1,0
-0,1
0,0
0,1
0,2
0,3
0,4
0,5
U=0 U=3 U=6 U=9 U=12
Ns=16 n=1/2
C(q
)
q/
Thus, 4kF charge mode indeed dominates over 2kF, at least for sufficiently large values of U.
Agreement with LL description: 2kF amplitude A1(n,U) 0 for U U (n)
Schematically:
n1
0
U
2kF
4kF
U (n)
Hubbard superlattices
• Model for layered systems [Paiva & dS (96)]: e.g., (thin) magnetic metallic multilayers
U 0 U 0
L0 LU
• Interesting magnetic behaviour and metal-insulator transitions [Paiva & dS (‘98,’00)]; see also LL superlattices [Silva-Valencia et al. (‘00)]. With attractive interactions leads to coexistence between superconductivity and magnetism [Paiva (‘99)]• Which is the dominant CDW mode?
0,2 0,4 0,6 0,8 1,00,0
0,1
0,2
0,3
0,4 (c) L0=3
q/
0,0
0,1
0,2
0,3
0,4
0,5
(a) L0=1
n=1/6 Ns=24LU=1 U=12
C(q
)
(b) L0=2
0,2 0,4 0,6 0,8 1,0
(d) L0=5
q/
Important parameter is # of electrons per cell:
neff n (L0 LU)
Define 2kF
* neff
cusp is located at
4kF*
Conclusions
• For sufficiently large values of U, 4kF charge mode dominates over 2kF
• The LL description can only be made consistent if the amplitude of the 2kF mode vanishes
• For Hubbard superlattices the same results apply, with redefined neff and kF
* talk downloadable from
http://www.if.ufrj.br/~rrds/rrds.html
References• R Egger at al., cond-mat/0008008• G Grüner, Rev.Mod.Phys. 60, 1129 (1988)• G Grüner, Rev.Mod.Phys. 66, 1 (1994)• J E Hirsch and D J Scalapino, Phys.Rev.B 27, 7169 (1983)• J E Hirsch and D J Scalapino, Phys.Rev.B 29, 5554 (1984)• S Kivelson et al., cond-mat/9907228• I J Lee et al., cond-mat/0001332• E H Lieb and F Y Wu, Phys.Rev.Lett. 20, 1445 (1968)• T Paiva, PhD thesis, UFF (1999)• T Paiva and R R dos Santos, Phys.Rev.Lett. 76, 1126 (1996)• T Paiva and R R dos Santos, Phys.Rev.B 58, 9607 (1998)• T Paiva and R R dos Santos, Phys.Rev.B 61, 13480 (2000)• T Paiva and R R dos Santos, Phys.Rev.B 62, 7004 (2000)• H J Schulz, Phys.Rev.Lett. 64, 2831 (1990)• J Silva-Valencia, E Miranda, and R R dos Santos, preprint (2000)• J Sólyom, Adv.Phys. 28, 209 (1979)• J Voit, Rep.Prog.Phys. 57, 977 (1994)