Interaction-induced Symmetry Protected Topological Phase in Harper-Hofstadter models
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1 Interaction-induced Symmetry Protected Topological Phase in Harper-Hofstadter models arxiv: Lode Pollet Dario Hügel Hugo Strand, Philipp Werner (Uni Fribourg)
2 Algorithmic developments diagrammatic Monte Carlo, (bosonic) cluster methods, the quest for novel numerical methods going beyond the state of the art: EF numerics 0.1 EF model experiment 0.01 EF EF material
3 Harper-Hofstadter model hardcore bosons
4 Hall effect R H = E y j x B z = 1 ne Integer Quantum Hall effect Landau levels topological invariant: first Chern number (TKNN) n = 1 2 i BZ xy = ne 2 /h d 2 k ku(k) ku(k)
5 spin-quantum Hall Effect Z2 topological invariant protected by time reversal symmetry (TKNN integer is 0) eg : spin-orbit coupling in graphene (but too weak), CdTe/HgTe/CdTe structures (band inversion as function of thickness) (CL Kane)
6 cold atom experiments very strong effective magnetic fields all optical setup with bosonic atoms Chern number has been measured (also for hexagonal lattice with fermions (ETHZ)) add interactions? M. Aidelsburger et al, Phys. Rev. Lett. 111, (2013) M. Aidelsburger et al, Nature Physics 11, (2015), AOP 3171 (2014)
7 how to study? The usual path integral Monte Carlo simulations do not work because of the infamous sign problem intermezzo: develop an approximate method and benchmark it
8 mean-field theory classical Ising (ferromagnet J > 0): H = J X hi,ji S i S j + h X i S i we are interested in the magnetization on every site: m i = hs i i Weiss field: H e = X i h e i S i h e i = tanh 1 m i approximation: h e i h + X j Jm j = h + zjm selfconsistency equation : m = tanh( h + z Jm)
9 We want to develop the dynamical mean-field solution for the 3d Bose-Hubbard model ~2010 H = t X hi,ji b i b j + U 2 X n i (n i 1) µ X i n i i write down single-site action : S imp = Z 0 d b ( )[@ µ] b( )+ U 2 0 we lose the momentum dependence for the self-energy works fine for normal phase and Mott phase. we want: include the physics of the weakly interacting Bose gas non-perturbatively, which is the limit t >>U we want: correction on top of mean-field Z d n( )[n( ) 1]
10 let s add a symmetry breaking field : zt Z 0 d [b( )+b ( )] this is the same as in static mean-field which can produce a condensate Bogoliubov prescription : for infinite coordination number, this term is zero b( ) =hbi + b( ) imag time dynamics can be added in the two-particle channel. The second source field can only couple to the normal bosons, otherwise double counting will occur (Nambu notation): 1 2 Z 0 d d 0 b ( ) ( 0 ) b( 0 ) which contains normal and anomalous propagators. see J. W. Negele and H. Orland, Quantum Many-Particle Systems (Addison-Wesley Publishing Company 1988) ISBN for how to treat broken symmetry Final step : re-express δb in terms of full b
11 weakly-interacting Bose gas Why BDMFT should be good: look at self-energies of weakly interacting Bose gas (Beliaev) momentum independent to leading order B. Capogrosso-Sansone, S. Giorgini, S. Pilati, L. Pollet, N. V. Prokof ev, B. V. Svistunov, and M. Troyer, New J. Phys. 12, (2010) similar in magnitude at low temperature, but opposite in sign µ = µ 2nU Hohenberg P C and Martin P C 1965 Ann. Phys Hugenholtz N M and Pines D S 1959 Phys. Rev Nepomnyashchii A A and Nepomnyashchii Yu A 1978 Zh. Eksp. Teor. Fiz [1978 Sov. Phys. JETP ] Nepomnyashchii Yu A 1983 Zh. Eksp. Teor. Fiz [1983 Sov. Phys. JETP ]
12 comparison in 3 dimensions 1 0 B DMFT Monte Carlo Mean Field 1 E kin /t 2 3 E kin /t T/t
13 phase diagram in 3 dimensions finite temperature, unit density ground state T/t SF B DMFT Monte Carlo Bethe z=6 Mean Field normal µ/u Mott Mott B DMFT Monte Carlo Bethe z=6 Mean Field SF U/t Mott t/u
14 results in two dimensions finite temperature, ground state unit density normal B DMFT Monte Carlo Mean Field Mott B DMFT Monte Carlo Bethe z=4 Mean Field T/t 3 µ/u 1 SF 2 1 SF U/t Mott Mott t/u
15 Bosonic self-energy functional theory only 3 parameters needed, determined variationally accuracy better than 1% for Bose-Hubbard model in every parameter regime D. Hügel and L. Pollet, PRB 2015 D. Hügel, P. Werner, L. Pollet, and H. Strand, arxiv/
16 Harper-Hofstadter model hardcore bosons
17 Chern numbers for noninteracting problem +1 diagonalize singleparticle H: c=+1-2
18 - real-space cluster mean-field - studied several fluxes - did not look at hopping anisotropy - found metastable (f)qh phases, almost degenerate with the superfluid - many density-wave instabilities Phys. Rev. A 93, (2016)
19 our method cluster mean-field but in momentum space hence: simpler than BDMFT or SFT (only Φ, no pair terms) impurity problem (4x4) solved with Lanczos no connected Green function of non-condensed particles of original model
20 reciprocal cluster mean-field method do NOT break translational invariance by working with clusters in momentum space instead of real space (but simpler than selfenergy functional theory): divide the Brillouin zone into patches: this breaks up Hamiltonian: H = Hc intra + Hc inter care is needed in case of symmetry breaking: cluster-hamiltonian can be written as (K, Q), ( k, q) (X, Y ), ( x, ỹ) coarse grain the dispersion:
21 benchmarking 2d Bose Hubbard model, no anisotropy, no flux (MF: meanfield; CG cluster Gutzwiller) 2d Bose Hubbard model, no flux; black = half filling chiral ladder system
22 ground state phase diagram non-degenerate gapped SPT phase has Z2 index; reminiscent of quantum spin Hall symmetry operation: T U T U = e FQHE: found, but all unstable against superfluidity
23 compare with free fermions: SPT at filling 1 strongly reduced SPT at filling 2 absent for free fermions
24 Chern numbers for interacting problem twisted boundary conditions: T x/y ( x, y) =e i x/y ( x, y) t y t y e i y/l y in the thermodynamic limit reciprocal space is continuous, and the phase twist infinitesimal this is just a momentum shift for every momentum we hence look at the winding of h projected on the space of hard-core bosons
25 density condensate density current striped superfluid supersolid
26 coincidence? project interacting problem onto non-interacting bands: n =1/4 ( = 1) n =1/2 ( = 2) occupation numbers: observe: 0 =1, 1 =0, 2 =0 c 0 0 = 1 occupation numbers: observe: 0 =1.45, 1 =0.25, 2 =0.05 (the result of this procedure is 0 for the trivial band insulators) (not the same as the approach by T. Neupert et al)
27 Summary Bosonic dynamical mean-field theory, bosonic self-energy functional theory cluster extensions SPT phases in interacting Harper-Hofstadter models; one purely due to interactions and of quantum spin-hall like nature perhaps the easiest around to check experimentally checks: extend to selfenergy functional methods, other fluxes, seeing topological phase transition? many interesting extensions possible (disorder, dynamics)
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