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Gapless spin liquids in frustrated Heisenberg models
Federico Becca
CNR IOM-DEMOCRITOS and International School for Advanced Studies (SISSA)
New Horizon of Strongly Correlated Physics, June 2014
Y. Iqbal (ICTP, Trieste), W.-J. Hu (now CSUN)
A. Parola (Como), D. Poilblanc (CNRS, Toulouse), and S. Sorella (SISSA)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 1 / 32
1 Introduction
2 The Heisenberg model on the frustrated square lattice
3 The Heisenberg model on the Kagome lattice
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 2 / 32
Ultimate frustration?
Looking for a magnetically disordered ground state?
• Many theoretical suggestions since P.W. Anderson (1973)Anderson, Mater. Res. Bull. 8, 153 (1973)
Fazekas and Anderson, Phil. Mag. 30, 423 (1974)
“Resonating valence-bond” (quantum spin liquid) states
Idea: the best state for two spin-1/2 spins is a valence bond (a spin singlet):
|VB〉R,R′ =1√2(| ↑〉R| ↓〉R′ − | ↓〉R| ↑〉R′)
Every spin of the lattice is coupled to a partnerThen, take a superposition of different valence bond configurations
Ψ = + + + ...
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 3 / 32
Valence-bond states: liquids and solids
Valence-bond solidbreaks translational/rotationalsymmetries
Short-range RVB + + ...
Long-range RVB + + ...
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 4 / 32
The Heisenberg model on the frustrated square lattice
H = J1∑
〈ij〉
Si · Sj + J2∑
〈〈ij〉〉
Si · Sj
Neel order Collinear order
Spin singlet
0 0.5 1
For J2/J1 ≪ 1: Antiferromagnetic order at Q = (π, π)
For J2/J1 ≫ 1: Antiferromagnetic order at Q = (π, 0) and Q = (0, π)
For J2/J1 ∼ 0.5: Disordered phase (RVB liquid, dimer order or more exotic?)
Experimental realization in Li2VOSiO4 (J2 & J1) and VOMoO4 (J2 < 0.5J1)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 5 / 32
Recent DMRG calculations
Jiang, Yao, and Balents, PRB 86, 024424 (2012)
• It has been criticized by Sandvik (possible dimer order)Sandvik, PRB 85, 134407 (2012)
• More recent calculations with both spin-liquid and dimer phases
Gong, Zhu, Sheng, Motrunich, Fisher, arXiv:1311.5962
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 6 / 32
Describing magnetically disordered phases
Sµi =
1
2c†i,ασ
µα,βci,β
H = −1
2
∑
i,j,α,β
Jij
(
c†i,αcj,αc
†j,βci,β +
1
2c†i,αci,αc
†j,βcj,β
)
c†i,αci,α = 1 ci,αci,βǫαβ = 0
• At the mean-field level:
HMF =∑
i,j,α
(χij + µδij)c†i,αcj,α +
∑
i,j
(ηij + ζδij)(c†i,↑c
†j,↓ + c
†j,↑c
†i,↓) + h.c.
〈c†i,αci,α〉 = 1 〈ci,αci,β〉ǫαβ = 0
• Then, we reintroduce the constraint of one-fermion per site:
|Φ(χij , ηij , µ, ζ)〉 = PG |ΦMF(χij , ηij , µ, ζ)〉
PG =∏
i (1− ni,↑ni,↓)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 7 / 32
Symmetry of the mean-field ansatz
In 2001, we guessed:χk = 2t(cos kx + cos ky )ηk = ∆x2−y2(cos kx − cos ky ) + ∆xy (sin 2kx sin 2ky )After Wen, called Z2Azz13
〈s〉 =∑
x
|〈x |Φ〉|2sign {〈x |Φ〉〈x |Ψex〉}
After the Wen’s classification, it is the best projected fermionic state
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 8 / 32
Towards the exact ground state
How can we improve the variational state?By the application of a few Lanczos steps!
|Ψp−LS〉 =(
1 +∑
m=1,...,p
αmHm
)
|ΨVMC 〉
For p → ∞, |Ψp−LS〉 converges to the exact ground state, provided 〈Ψ0|ΨVMC 〉 6= 0
On large systems, only FEW Lanczos steps are affordable: We can do up to p = 2
In addition, a fixed-node (FN) projection is possibleten Haaf et al., PRB 51, 13039 (1995)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 9 / 32
The variance extrapolation
A zero-variance extrapolation can be done
Whenever |ΨVMC 〉 is sufficiently close to the ground state:
E ≃ E0 + const× σ2 E = 〈H〉/Nσ2 = (〈H2〉 − E 2)/N
How does it work?Example: the t−J model
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 10 / 32
Going to the excitation spectrum
If a variational approach works also low-energy excitations must be described
HMF =∑
i,j,α
(χij + µδij)c†i,αcj,α +
∑
i,j
(ηij + ζδij)(c†i,↑c
†j,↓ + c
†j,↑c
†i,↓) + h.c.
After a Bogoliubov transformation:
HMF =∑
k
(Ekψ†kψk − Ekφ
†kφk)
The ground state is:
|Φ0MF〉 =
∏
k
φ†k |0〉
Excited states are obtained by:
φq1. . . φqnψ
†p1. . . ψ†
pm |Φ0MF〉
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 11 / 32
Spin excitations
Considering excited states that can be described by a SINGLE determinant, we have:
• The S=0 ground state• The S=2 with momentum k = (0, 0)• The S=1 with momentum k = (π, 0) or k = (0, π)
Test case: J2/J1 = 0.5 and 6× 6 cluster
0.00 0.01 0.02
–0.495
–0.490
–0.485
–0.480
–0.475
0 0.01 0.02
–0.495
–0.485
–0.475
–0.465
Variance Variance0 3.10–3 6.10–3 9.10–3
–0.504
–0.502
–0.500
–0.498
–0.496
–0.494
Variance
E(S
) pe
r si
te
6x68x810x1014x1418x18
(a) (b) (c)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 12 / 32
Spin excitations
• The S=2 gap vanishes in the Neel phase• The S=1 gap at k = (π, 0) is instead finite in the Neel phase
The Lanczos extrapolation is performed on each state separately
Calculations on the 6× 6 cluster vs exact results
0.20 0.25 0.30 0.35 0.40 0.45 0.50 0.550.0
0.2
0.4
0.6
0.8
1.0
1.2
1.4
1.6
1.8
J 2/J 1
∆ 1
S=1 gap
0.20 0.25 0.30 0.35 0.40 0.45 0.50 0.550.0
0.2
0.4
0.6
0.8
1.0
1.2
1.4
1.6
1.8
J 2/J 1
∆ 2
exactp=0p=1p=2variance extrapolation
S=2 gap
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 13 / 32
The S=2 spin excitation for large sizes
0.00 0.02 0.04 0.06 0.08 0.10 0.12 0.14 0.16 0.180.0
0.2
0.4
0.6
0.8
1.0
1.2
1.4
1.6
1/L
∆ 2J2/J1=0.5, p=0
J2/J1=0.5, variance extrapolation
J2/J1=0.5, triplet gap from DMRG
J2/J1=0.55, p=0
J2/J1=0.55, variance extrapolation
J2/J1=0.55, triplet gap from DMRG
• J2/J1 = 0.5 −→ ∆2 = −0.04(5)• J2/J1 = 0.55 −→ ∆2 = −0.07(7)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 14 / 32
The S=1 spin excitation for large sizes
0.00 0.02 0.04 0.06 0.08 0.10 0.12 0.14 0.16 0.180.0
0.2
0.4
0.6
0.8
1.0
1/L
∆ 1
J 2/J1=0.45, p=0
J 2/J1=0.45, variance extrapolation
J 2/J1=0.5, p=0
J 2/J1=0.5, variance extrapolation
0.00 0.02 0.04 0.06 0.08 0.10 0.12 0.14 0.16 0.180.0
0.2
0.4
0.6
0.8
1.0
1.2
1.4
1/L
J 2/J1=0.3
J 2/J1=0.4
J 2/J1=0.45
J 2/J1=0.5
J 2/J1=0.55
∆1
0.30 0.35 0.40 0.45 0.50 0.550.0
0.1
0.2
0.3
0.4
0.5
0.6
J 2/J 1
∆ 1
0.48(2)
The spin gap is FINITE for J2/J1 < 0.48
Instead, it vanishes for J2/J1 > 0.48
NON-trivial aspect of the SL phase!
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 15 / 32
Conclusions (first part)
Very good energiesWith few (TWO-THREE) variational parameters: Educated guessTo be compared with about 16000 parameters in DMRG: Brute-force calculation
Direct calculation of the spin gap for S=2 and S=1 excitationsIn both cases, we find evidence for a GAPLESS spin liquid
Our calculations are done on L× L clusters with PBC in both directions
DMRG calculations are done on 2L× L cylinders with OBC along x and PBC along y
(but the gap is computed only in the central part of the cluster)
Our approach may capture both gapless and gapped states
DMRG algorithm favors low-entangled (gapped) states
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 16 / 32
The Heisenberg model on the Kagome lattice
H = J∑
〈ij〉
Si · Sj + . . .
• No magnetic order down to 50mK (despite TCW ≃ 200K)
• Spin susceptibility rises with T → 0 but then saturates below 0.5K
• Specific heat Cv ∝ T below 0.5K
• No sign of spin gap in dynamical Neutron scattering measurements
Mendels et al., PRL 98, 077204 (2007)
Helton et al., PRL 98, 107204 (2007)
Bert et al., PRB 76, 132411 (2007)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 17 / 32
Some of the previous results
Nearest-neighbor Heisenberg model on the Kagome lattice
Author GS proposed Energy/site Method used
P.A. Lee U(1) gapless SL −0.42866(1)J Fermionic VMC
Singh 36-site HVBC −0.433(1)J Series expansion
Vidal 36-site HVBC −0.43221 J MERA
Poilblanc 12- or 36-site VBC QDM
Lhuillier Chiral gapped SL SBMF
White Z2 gapped SL −0.4379(3)J DMRG
Schollwoeck Z2 gapped SL −0.4386(5)J DMRG
Xie et al. gapped SL −0.4364(1)J PESS
Ran, Hermele, Lee, and Wen, PRL 98, 117205 (2007)
Yan, Huse, and White, Science 332, 1173 (2011)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 18 / 32
Results with projected wave functions
A variational ansatz with ONLY hopping but non-trivial fluxes has been proposed with
• π fluxes through hexagons and 0 fluxes through triangles• Dirac points in the mean-field spinon spectrumRan, Hermele, Lee, and Wen, PRL 98, 117205 (2007)
a
b c
d
1 5
6
a
b c
d
dd
1
3
5
6
(a)
(b)
(d) (e)
0 a1
2a
0
1 2
3
4 5
6
(c)
0
0 0
• 0 fluxes everywhere• Fermi surface in the mean-field spinon spectrum
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 19 / 32
Can we have a Z2 gapped spin liquid (as in DMRG)?
Projective symmetry-group analysis
Lu, Ran, and Lee, PRB 83, 224413 (2011)
uij =
(
χ∗ij ∆ij
∆∗ij −χij
)
a
b c
d
1 5
6
a
b c
d
dd
1
3
5
6
(a)
(b)
(d) (e)
0 a1
2a
0
1 2
3
4 5
6
(c)
0
0 0
Only ONE gapped SL connected with the U(1) Dirac SL:
FOUR gapped SL connected with the Uniform U(1) SL:
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 20 / 32
The Dirac U(1) SL is stable against opening a gap
• By optimizing the variational state, the breaking terms go to zero
• The best variational energy is obtained by the U(1) Dirac state
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 21 / 32
Calculations on the 48-site cluster
Our zero-variance extrapolation gives: E/N ≃ −0.4378
0 0.005 0.01 0.015 0.02 0.025
Variance of energy (σ2)
-0.435
-0.43
-0.425
-0.42
-0.415
-0.41E
nerg
y pe
r si
te
Uniform RVB ([0,0]) SL {VMC}Z
2[0,π]β SL {VMC}
U(1) Dirac ([0,π]) SL {VMC}U(1) Dirac ([0,π]) SL {FN}DMRG (Torus) [Jiang et al.]
0 0.001 0.002-0.438
-0.437
-0.436
E/N ≃ −0.4387 by ED, A. Lauchli (seen at APS in Boston)E/N ≃ −0.4381 by DMRG, S. White (private communication)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 22 / 32
Calculations on larger clusters
0 0.005 0.01 0.015
Variance of energy (σ2)
-0.438
-0.436
-0.434
-0.432
-0.43
-0.428
Ene
rgy
per
site
48 sites {VMC}108 sites {VMC}144 sites {VMC}192 sites {VMC}DMRG (Torus 108) [Depenbrock et al.]
0 0.001 0.002
-0.438
-0.437
0 0.005 0.01 0.015
Variance of energy (σ2)
-0.438
-0.436
-0.434
-0.432
-0.43
-0.428
Ene
rgy
per
site
48 sites {FN}108 sites {FN}144 sites {FN}192 sites {FN}DMRG (Torus 108) [Depenbrock et al.]
0 0.001 0.002
-0.438
-0.437
• NO substraction techniques to get the energy• The state has ALL symmetries of the lattice• The extrapolated values are essentially size consistent
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 23 / 32
Extrapolations for Dirac and Z2 states
Starting from a Z2 state the extrapolation is worse than for the Dirac state
0 0.005 0.01 0.015 0.02 0.025
Variance of energy (σ2)
-0.436
-0.432
-0.428
-0.424
Ene
rgy
per
site
192 sites - U(1) Dirac SL {VMC}192 sites - Z
2[0,π]β SL {VMC}
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 24 / 32
The thermodynamic limit
0 0.01 0.02 0.031/N
-0.4385
-0.438
-0.4375
-0.437
-0.4365G
roun
d st
ate
ener
gy p
er s
ite 2d estimate from Lanczos+VMC (current work)2d estimate from DMRG (Depenbrock et al.)2d estimate from DMRG (Yan et al.)2d estimate from CCM (Götze et al.)
• OUR thermodynamic energy is: E/J = −0.4365(2)• DMRG thermodynamic energy is: E/J = −0.4386(5)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 25 / 32
The variational S = 2 gap
0 0.05 0.1 0.15 0.2 0.25Inverse geometrical diameter (1/L)
0
0.2
0.4
0.6
0.8
1
1.2
S=2
Spi
n G
ap (∆
2)
Projected U(1) Dirac SLMean field U(1) Dirac SL
• The Gutzwiller projected state is still gapless• Remarkable stability of the U(1) Dirac spin liquid
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 26 / 32
The Lanczos step extrapolations
0 0.005 0.01 0.015
Variance of energy (σ2)
-0.438
-0.436
-0.434
-0.432
-0.43
-0.428
Ene
rgy
per
site
(E/J
)
48-sites108-sites192-sites432-sites
0 0.005 0.01 0.015 0.02
Variance of energy (σ2)
-0.436
-0.432
-0.428
-0.424
-0.42
-0.416
Ene
rgy
per
site
(E/J
)
48-sites108-sites192-sites432-sites
• We separately extrapolate both S = 0 and S = 2 energies• Then the gap (zero-variance) gap is computed
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 27 / 32
The S = 2 gap of the kagome Heisenberg model
0 0.05 0.1 0.15 0.2 0.25Inverse geometrical diameter (1/L)
0
0.1
0.2
0.3
0.4
0.5
S=2
Spi
n G
ap (∆
2)
p = 0 Lanczos stepsp = 2 Lanczos steps extrapolated
• The final result is ∆2 = −0.04± 0.06• The “upper” bound is given by ∆2 ≃ 0.02• The S = 1 gap should be ∆1 . 0.01
Much smaller than previous DMRG estimationsMore similar to recent calculations by Nishimoto et al. ∆1 = 0.05± 0.02Nishimoto, Shibata, and Hotta, Nat. Commun. 4, 2287 (2013)
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 28 / 32
Adding the next-nearest-neighbor super-exchange
0 0.1 0.2 0.3 0.4 0.5J
2
-0.5
-0.48
-0.46
-0.44
-0.42
-0.4
-0.38
Ene
rgy
per
site
U(1) Dirac SLZ
2[0,π]β SL
q=0 magnetically ordered state2 Lanczos steps + ZVE {Z
2[0,π]β SL}
48-sites
0 0.1 0.2 0.3 0.4 0.5J
2
-0.5
-0.48
-0.46
-0.44
-0.42
-0.4
-0.38
Ene
rgy
per
site
U(1) Dirac SLZ
2[0,π]β SL
q=0 magnetically ordered state
192-sites
• The gapped Z2 state overcomes the U(1) Dirac one for J2/J1 > 0.1
• The magnetic state with q = 0 (Jastrow) is stabilized for J2/J1 > 0.3
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 29 / 32
Adding the next-nearest-neighbor super-exchange
Applying Lanczos steps on 48 sites
0 0.005 0.01 0.015 0.02 0.025 0.03
Variance of energy-0.46
-0.456
-0.452
-0.448
-0.444
-0.44
-0.436
Ene
rgy
per
site
Z2[0,π]β SL
U(1) Dirac SL
48-site torus, J2=0.20
• For finite J2/J1 the gapped Z2 state has a “better” extrapolation with Lanczos steps
• Calculations on larger clusters are in progress...
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 30 / 32
Conclusions
Results up to now:
Very good energiesWith TWO variational parameters: Educated guessTo be compared with about 16000 parameters in DMRG: Brute-force calculation
Direct calculation of the S = 2 gapNo evidence for a finite gap in thermodynamic limit
Pros• Very flexible approach that may describe several different phases
(gapped and gapless, not only low-entanglement states)
• Natural way of constructing and understanding low-energy excitations
• Applying few Lanczos steps allows for a sizable improvement
Cons• Still, it is a biased approach and more work must be done
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 31 / 32
Different kinds of spin liquids
The folklore is that
• DMRG always produces excellent spin liquids
• Other numerical methods produce no good liquids
We are trying to improve the quality of our liquids
Federico Becca (CNR and SISSA) Gapless Spin Liquids NHSCP at ISSP 32 / 32