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Symmetry-protected topological phases of alkaline-earth ultra-cold fermionic atoms
in one dimension Keisuke Totsuka
Yukawa Institute for Theoretical Physics, Kyoto University
June 14, 2013 talk @ EQPCM (ISSP)
1. Introduction2. Symmetry-protected topological order in 1D3. Alkaline-earth cold atom & SU(N) Hubbard model4. SU(N) symmetry-protected topological phase5. Summary
Ref: Nonne et al. Phys.Rev.B 82, 155134 (2010) Euro.Phys.Lett. 102, 37008 (2013), and work in progress
Collaborators• Sylvain Capponi
(IRSAMC, Univ. Toulouse)
• Philippe Lecheminant (LPTM, Univ. Cergy-Pontoise)
• Marion Moliner (LPTM, Univ. Cergy-Pontoise)
• Héroïse Nonne (U-Cergy ⇒ Dept. Phys. Technion)
Symmetry and Phase Transitions• Landau picture of “phase transitions” (from L.L. vol. 5)
✓ phase transitions: spontaneous breaking of symmetry G (original) ⇒ H (subgroup) ex) G=SO(3), H=SO(2) for (collinear) magnetic order
✓ “Order Parameters”✓ classification in terms of SSB
patterns of G
1. “... the transition between phases of different symmetry .... cannot occur in a continuous manner”
2. “... in a phase transition of the second kind .... the symmetry of one phase is higher than that of the other..”
Challenges from quantum systems• fractional quantum-Hall systems
✓ Laughlin wave function ...“ψm” (ν=1/m)
✓ describes featureless uniform ground states,no symmetry breaking (locally)
✓ Nevertheless, different “phases” for different “m”
• quantum spin liquids (Z2/chiral-SL, quantum dimer,...)
✓ no magnetic LRO, no translation SSB, ...
✓ global (topological) properties (e.g. γtop)(≠boring paramagnet)
the new “holy bible”
1983--
1987--
a new paradigm?? ➡ topological order (Wen ’89)
“Topological Order” in 1D
• Q-information tells us:
✓ any gapped states can be approximated by MPS
✓ only short-range entanglement in 1D (i.e. γtop=0)
✓ can be smoothly deformed to trivial product state ➡ No (genuine) topological order in 1D !!
• but... still possible to define featureless “topological phases” protected by some symmetry
symmetry-protected topological (SPT) orderGu-Wen ’09, Chen et al. ’11
trivial phase trivial phase topological
Verstraete et al. ’05
Hastings ’07
protecting sym.
(1+1)D
“Topological Order” in 1D
• Phases-I ... long-range entanglement (LRE):
✓ genuine topological phases in (2+1)D, (3+1)D
✓ w/ symmetries, possible to have topological order + SSB (“symmetry-enriched” etc.)
• Phases-II ... short-range entanglement (SRE)✓ wo/ symmetries, only a single trivial product state ✓ w/ “protecting symmetries”, various topological phases
“Topological Order” in 1D
• Paradigmatic example: “Haldane phase”
✓ 1D integer-S spin chain
✓ featureless non-magnetic state w/ exponentially-decaying cor.
✓ existence of edge states (cf. ESR)
• Non-local (string) order parameters:✓ Z2×Z2 symmetry
✓ relation to SPT order
Miyashita-Yamamoto ’93
Oz
string ⌘ lim
|i�j|%1
DSz
i
exp
"i⇡
j�1X
k=i
Sz
k
#Sz
j
E
Ox
string ⌘ lim
|i�j|%1
DSx
i
exp
"i⇡
jX
k=i+1
Sx
k
#Sx
j
E.
Kennedy-Tasaki ’92
Pollmann-Turner ’12, Hasebe-KT ’13
Haldane ’83, Affleck et al. ’88
“Topological Order” in 1D
• Matrix-Product States (MPS):
✓ convenient rep. for generic gapped states in 1D (w/ SRE)
• existence of “edge states” (α,β)✓ featureless in the bulk ✓ special structure (“edge states”) localized at boundaries
bulk
cf. FQHE, topological insulators
✓|0ii
p2|�1ii
�p2|1ii �|0ii
◆
Kintaro Ame
: S=1 VBS
physical state
“Topological Order” in 1D
• edge states & “symmetry fractionalization”:
✓ symmetry operation on MPS :
• edge states = obey “projective representation”✓ classifying “topological phases” = classifying possible “edge states”
✓ “V” does not necessarily follow group-multiplication rule:
✓ catalogue of gapped symmetry-protected topological phases in 1D (in terms of proj. rep.)
Chen-Gu-Wen ’11, Schuch et al. ’11
symmetry fractionalizes
Perez-Garcia et al. ’08
Pollmann et al. ’10, ’12
V (g1)V (g2) = !(g1, g2)V (g1g2)
“Topological Order” in 1D
• Motivation....
• Given a “protecting symmetry”
✓ zoo of symmetry-protected topological (SPT) phases
• Realization of topological phases ✓ existence of (many) symmetry-breaking perturbations in real
systems (fine-tuning necessary to have high sym.)
✓ SPT phases protected by high symmetry unlikely ??
How to realize SPT phases in realistic systems ??
Alkaline-earth cold atoms... a realistic system bearing SPT phases
• alkaline-earth atoms: two electrons in the outer shell
• J=0 for both G.S. (1S0) and (metastable) excited state (3P0)
• decoupling of “nuclear spin I” from electronic states➡ I-independent scattering length
• SU(N) (N=2I+1) symmetry (to a very good approx.)
• 171Yb (I=1/2, SU(2)), 173Yb (I=5/2, SU(6)), 87Sr (I=9/2, SU(10)) ,....
Gorshkov et al ’10
Takahashi group ’10-’12 DeSalvo et al. ’10
1S0 3P0(G.S.) forbidden
Alkaline-earth cold atoms... a realistic system bearing SPT phases
• alkaline-earth atoms: two electrons in the outer shell
• p-band model ... another way of introducing 2-orbitals
Kobayashi et al. ’12
1S0 3P0
z // chain
✓1D optical lattice✓confinement in (xy) not
too strong✓fill s-band only
(G.S.)
Alkaline-earth cold atoms... Mott insulating phase (expt.)
• alkaline-earth atoms (173Yb, I=5/2): SU(6) Mott phase
✓ optical lattice, large-U: Mott phase (w/ n=1)
✓ charge gap, doublon, compressibility
✓ But.... still in high-T region (i.e. SU(N) paramagnet)
Taie et al. ’12
2-orbital SU(N) Hubbard model ... a minimal model
• “ingredients”
✓ charge
✓ nuclear-spin multiplet (Iz=−I,...,+I, N=2I+1, α=1,...,N)
✓ orbitals: ground state “g”, excited state “e” (m=1,2)cf. 2-orbitals px, py in p-band model
• Hubbard-like Hamiltonian: Gorshkov et al ’10Nonne-Moliner-Capponi-Lecheminant-KT ’13
c†m↵,i : creation op. for “orbital”=m, nuclear-spin=α
Machida et al. ’12
HG
=� tX
i,m↵
⇣c†m↵, icm↵, i+1
+ h.c.⌘� µ
G
X
i
ni +X
i
X
m=e,g
UG
2nm, i(nm, i � 1)
+ VG
X
i
ng, ine, i + V e-gex
X
i,↵�
c†g↵, ic†e�, icg�, ice↵, i
Hubbard-like int. within “e” & “g”
“e”-“g” exchangeCoulomb between “g”-”e”
U(1)c
⇥SU(N)s
⇥U(1)o
generic symmetry:
SU(N) Hubbard model ... simpler case
• quench “e”-orbital ➡ (single-band) SU(N) Hubbard
• insulating phases:
✓ 1/N-filling: MIT@U=Uc ➡ charge: gapped, “SU(N)-spin”: gapless
✓ deep inside Mott phase: SU(N)-Heisenberg
✓ for other commensurate fillings... f=p/q ??
Lieb-Wu ’68, Assaraf et al. ’99Manmana et al. ’11
Sutherland ’75Affleck ’88
Uc=0 Uc>0(BKT)
TLL charge: gap, “spin”: criticalcharge: gap, “spin”: critical
N=2 N >2
Sutherland ’75, Affleck ’88Manmana et al. ’11
Assaraf et al. ’99
(typically, U /t >11)
SU(N) Hubbard model ... simpler case
• single-band SU(N) Hubbard
• For other commensurate fillings ... f=p/q
✓ q > N: gapless charge/”spin”, C1S(N-1) (c=n) ➡ critical phase
✓ q < N: full gap (C0S0), spatially non-uniform insulating phase
Szirmai et al. ’05, ’08
possible to have “fully-gapped uniform states” ??
SU(5) [email protected] realistic interacting models....
Szirmai et al. ’05, ’08
➡ No featureless fully-gapped phase
Phases of 2-orbital SU(N) Hubbard
• plan of attack:
✓ 2-orbital (“g” & “e”), SU(N)-fermion, @half-filling
✓ Maximal filling: 2N fermions/site (2N boxes)ex) half-filling = N fermions/site (N boxes out of 2N)
✓ Mathods:
1. weak-coupling (RG + duality)➡ low-energy field theory: 4N Majorana fermions (+ int.)
2. strong-coupling (approach from Mott sides)➡ effective spin/orbital models
3. numerical ➡ DMRG
Phases of 2-orbital SU(N) Hubbard... N=2, half-filling
• 4 Mott phases wo/ G.S. degeneracy:
spin-HaldaneSspin=1
rung-singletorbital large-D
charge-Haldane
orbital-HaldaneSorb=1
“charge” “orbital” “spin”
(a) spin-Haldane gapped local singlet spin-1 Haldane
(b) rung-singlet gapped Tz=0 (large-D) local singlet
(c) charge-Haldane gapped singlet/triplet local singlet
(d) orbital-Haldane gapped spin-1 Haldane local singlet
orbital-”e”
orbital-”g”
Della Torre et al. ’06Nonne et al. ’10
Kobayashi et al. ’12
Phases of 2-orbital SU(N) Hubbard... N=2, half-filling (weak-coupling)
• 4 Mott phases + 3 phases w/ degenerate G.S.:
Vex
= �0.03t Vex
= 0.01t
spin-HaldaneSspin=1 (“RT”)
rung-singletorbital large-D (“RS”)
charge-Haldane (“HC”)
orbital-HaldaneSorb=1 (“HO”)
CDW(2kF)
ODW(2kF)
weak-couplingphase diag.
Nonne et al. ’10
degenerate non-degenerate, Mott-like
Phases of 2-orbital SU(N) Hubbard... N=2, half-filling (numerical)
• 4 Mott phases + 3 insulating phases w/ degenerate G.S.:
Vex
= �0.03t Vex
= 0.01t
DMRG
Nonne et al. ’10
weak-couplingphase diag.
Vex
= �t Vex
= t
2-orbital SU(N) (N>2) Hubbard ... half-filling
• weak-coupling: (very) complicated, but still doable...
Nonne et al. ’13
g1 =N
4⇡g21 +
N
8⇡g22 +
N
16⇡g23 +
N + 2
4⇡g27 +
N � 2
2⇡g28 +
N � 2
4⇡g29
g2 =N
2⇡g1g2 +
N2 � 4
4N⇡g2g3 +
1
2⇡g3g4 +
1
2⇡g2g5 +
N
⇡g7g8 +
N � 2
⇡g8g9
g3 =N
2⇡g1g3 +
N2 � 4
4⇡Ng22 +
1
⇡g2g4 +
N
⇡g7g9 +
N � 2
⇡g28
g4 =1
2⇡g4g5 +
N2 � 1
2⇡N2g2g3 +
2(N � 1)
N⇡g8g9
g5 =N2 � 1
2⇡N2g22 +
1
2⇡g24 +
2(N � 1)
N⇡g28
g6 =N + 1
4⇡Ng27 +
N � 1
2⇡Ng28 +
N � 1
4N⇡g29
g7 =N2 +N � 2
2N⇡g1g7 +
2
⇡g6g7 +
N � 1
4⇡g3g9 +
N � 1
2⇡g2g8
g8 =N + 1
4⇡g2g7 +
N2 �N � 2
4N⇡g2g9 +
2
⇡g6g8 +
N2 �N � 2
2N⇡g1g8 +
1
2⇡g5g8 +
1
2⇡g4g9 +
N2 �N � 2
4N⇡g3g8
g9 =N + 1
4⇡g3g7 +
2
⇡g6g9 +
N2 �N � 2
2N⇡g1g9 +
1
⇡g4g8 +
N2 �N � 2
2N⇡g2g8
RG-flow patterndifferent from N=2
✓ SP✓ 2kF-CDW✓ orbital-Heisenberg (S=N/2) ⬅ regardless of “N”
2-orbital SU(N) (N>2) Hubbard ... half-filling
• (very) schematic phase diagram for N=even:
•
pseudo-spin=N/2Heisenberg
SU(N) Heisenberg (N=even) J/t
U/t“magic line”✓ spin-Peierls (SP)
✓CDW✓ orbital T=N/2 SU(2) HAF✓ SU(N) HAF
Nonne et al. ’13
HH =� tX
i
2X
m=1
NX
↵=1
⇣c†m↵, i
cm↵, i+1 + h.c.
⌘� µ
X
i
ni
+U
2
X
i
n2i
+ JX
i
�(T x
i
)2 + (T y
i
)2 + J
z
X
i
(T z
i
)2,
J = V e-gex
, Jz = UG
� VG
,
U =UG
+ VG
2, µ =
UG
+ V e-gex
2+ µ
G
2-orbital SU(N) (N>2) Hubbard... SU(4) SPT phase (new!)
• “Magic line”: N=even
• strong-coupling effective Hamiltonian:
• generalize AKLT-idea: ex) SU(4) VBS
He↵ =N2�1X
A=1
SAi S
Ai+1
Jz = J , J =2NU
N + 2
HVBS = JsX
i
⇢SAi S
Ai+1 +
13
108(SA
i SAi+1)
2 +1
216(SA
i SAi+1)
3
�
N/2 rows, 2 columns
parent Hamiltonian:
hSA(j)SA(j + n)i =(
125
�� 1
5
�nn 6= 0
45 n = 0N=4
N=6 Nonne et al. ’13
N=2N=4
N=6
NB) consistent w/ DMRG sim.
Nonne et al. ’13
2-orbital SU(N) (N>2) Hubbard... SU(4) SPT phase (new!)
• SU(4) VBS
✓ 6-fold degenerate edge states
✓ one of N(=4) SPT phases (protected by SU(N))
✓ When U↘, QPT out to (“spin”-orbital entangled) “SP” phase (univ. class SU(N)2)
HVBS = JsX
i
⇢SAi S
Ai+1 +
13
108(SA
i SAi+1)
2 +1
216(SA
i SAi+1)
3
�
N=4
N=6
Nonne et al. ’13
N=4 (DMRG, L=36)
Duivenvoorden-Quella ’12, ’13
QPT: top ⇒ SP
edge states(nα)
Comparison: N=3 and N=4 cases... numerics (DMRG)
• drastic difference between N=odd / even
• (preliminary) DMRG results:
✓ L=36 sites
✓ order parameter & edge states
-6 -4 -2 0 2 4 6U
-20
-10
0
10
20
J
CDWSPcriticalJ=6U/5
N=3 phase diag. based on L=36 DMRG (Nf=3*L)
-6 -4 -2 0 2 4 6U/t
-10
-5
0
5
10
15
J/t
CDWSPHOtopo
J=4U/3
N=3 N=4
S=3/2 Heisenberg(gapless)
SU(4) topological
orbital-Haldane
3 phases (2 gapped, 1 gapless)
cf. Nonne et al. ’13
2kF-CDW
SU(4)-top⇔SP QPT
J
U
Summary• Symmetry-protected topological order in 1D
• SU(N) Hubbard model with 2-orbitals (N=2I+1)
✓ alkalline-earth Fermi gas in optical lattice (@half-filling)
✓ phase diagram depends on N=even / odd
✓ symmetry-protected topological phases for N=even (I=1/2,3/2,..)
✓ stable topological phases for N/2=odd, i.e. I=1/2 (171Yb), 5/2 (173Yb), 9/2 (87Sr), ...
• Outlook:
✓ Effects of trap (SPT phase & Mott core) ?
✓ quantum-optical detection of topological order ??
✓ higher-D ???
Kobayashi et al. ’12
“Mott core”