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Extracting the number of type-B Goldstone modes and the dynamical critical exponent for a type of scale-invariant states

Huan-Qiang Zhou Centre for Modern Physics, Chongqing University, Chongqing 400044, The People’s Republic of China    Yan-Wei Dai Centre for Modern Physics, Chongqing University, Chongqing 400044, The People’s Republic of China    Qian-Qian Shi Centre for Modern Physics, Chongqing University, Chongqing 400044, The People’s Republic of China    Ian P. McCulloch Department of Physics, National Tsing Hua University, Hsinchu 30013, Taiwan School of Mathematics and Physics, The University of Queensland, St. Lucia, QLD 4072, Australia Centre for Modern Physics, Chongqing University, Chongqing 400044, The People’s Republic of China    Murray T. Batchelor Mathematical Sciences Institute, The Australian National University, Canberra ACT 2601, Australia Centre for Modern Physics, Chongqing University, Chongqing 400044, The People’s Republic of China
Abstract

A generic scheme is proposed to perform a finite-entanglement scaling analysis for scale-invariant states which appear as highly degenerate ground states arising from spontaneous symmetry breaking with type-B Goldstone modes. This allows us to extract the number of type-B Goldstone modes and the dynamical critical exponent, in combination with a finite block-size scaling analysis, from numerical simulations of quantum many-body systems in the context of tensor network representations. The number of type-B Goldstone modes is identical to the fractal dimension, thus reflecting an abstract fractal underlying the ground state subspace. As illustrative examples, we investigate the spin-ss Heisenberg ferromagnetic model, the SU(3)\rm{SU}(3) ferromagnetic model and the SO(4)\rm{SO}(4) spin-orbital model.

I Introduction

In the last decades, much attention has been paid to investigations into quantum critical phenomena QPT . In particular, significant effort has been made in achieving a long-term goal towards a complete classification of quantum phase transitions and quantum states of matter in one-dimensional quantum many-body systems wen ; pollmann1 . Historically, this may be dated back to the early work by Polyakov Popkov , who speculated that scale invariance implies conformal invariance. This speculation eventually led to the creation of conformal field theory Belavin , thus making it possible to classify all possible critical points in terms of central charge and conformal dimensions. Given a few counter-examples are known Hortacsu ; Strominger ; LeClair ; Zamolodchikov , it appears to be necessary to launch a systematic search for scale-invariant, but not conformally invariant, quantum states of matter.

Indeed, the presence of scale-invariant, but not conformally invariant, quantum states of matter strongly suggests that the current classification of quantum phase transitions and quantum states of matter is far from complete, even for those relevant to spontaneous symmetry breaking (SSB) anderson . As it turns out, highly degenerate ground states arising from SSB with type-B Goldstone modes (GMs) are scale-invariant FMGM ; golden ; LLspin1 , with the SU(2){\rm SU}(2) Heisenberg ferromagnetic model being a paradigmatic example. In fact the highly degenerate ground states admit an exact singular value decomposition, thus exhibiting self-similarities underlying the ground state subspace. In other words, an abstract fractal is revealed, living in a Hilbert space, which may be characterized in terms of the fractal dimension, first introduced by Castro-Alvaredo and Doyon doyon for the SU(2){\rm SU}(2) Heisenberg ferromagnetic states. A remarkable fact is that the fractal dimension may be identified with the number of type-B GMs FMGM ; golden , thus unveiling a deep connection between scale-invariant states and the counting rule of the GMs Watanabe . The establishment of the counting rule is largely based on an insightful observation made by Nambu nambu , culminating in the classification of type-A and type-B GMs.

In addition, our current understanding of quantum critical phenomena has been reshaped from the novel perspective of quantum information science nielsen ; amico . In particular, the entanglement entropy is demonstrated to be a powerful means for characterizing quantum phase transitions vidal ; Korepin ; cardy ; zhou . This in turn motivated the development of powerful tensor network representations to simulate quantum many-body systems itebd ; idmrg ; Orus ; ipeps ; frank ; corboz ; czarnik . As a by-product, a finite-entanglement scaling analysis is developed to replace a finite-size scaling analysis, as advocated tagliacozzo ; wanghl ; pollmann for conformally invariant quantum states, which allows to extract central charge from numerical simulations in the infinite Matrix Product State (iMPS) representation for one-dimensional quantum many-body systems. A natural question arises as to whether or not there is a parallel between scale-invariant quantum states and conformally invariant quantum states. That is, a generic scheme to perform a finite-entanglement scaling analysis is needed for scale-invariant quantum states.

This work aims to address this question for scale-invariant states, which appear to be highly degenerate ground states arising from SSB with type-B GMs. This allows us to extract the number of type-B GMs and the dynamical critical exponent, in combination with a finite block-size scaling analysis, from numerical simulations of quantum many-body systems in the context of tensor network representations. As recently argued FMGM ; golden , the number of type-B GMs is identical to the fractal dimension, thus reflecting an abstract fractal underlying the ground state subspace. As illustrative examples, we investigate the spin-ss Heisenberg ferromagnetic model, the SU(3)\rm{SU}(3) ferromagnetic model and the SO(4)\rm{SO}(4) spin-orbital model.

II Finite-entanglement scaling for scale-invariant states

Let us consider a quantum many-body system described by Hamiltonian \mathscr{H} on a lattice. If the Hamiltonian \mathscr{H} possesses the symmetry group GG, which is spontaneously broken into HH, then the counting rule is established as NA+2NB=NBGN_{A}+2N_{B}=N_{BG} Watanabe , where NAN_{A} and NBN_{B} are the numbers of type-A and type-B GMs, and NBGN_{BG} is equal to the dimension of the coset space G/HG/H. Here and hereafter, we focus on a one-dimensional quantum many-body system, with LL being the system size. According to the Mermin-Wagner-Coleman theorem mwc , no type-A GM survives in one spatial dimension. Hence the number NAN_{A} of type-A GMs must be zero.

Suppose the system is partitioned into a block BB and its environment EE, with the block consisting of nn (contiguous) lattice sites, and the other LnL-n lattice sites constituting the environment EE. As demonstrated in Refs. FMGM ; golden , for any non-zero fillings fαf_{\alpha}  (α=1,,R\alpha=1,\cdots,R, with RR beng the rank of GG, if it is semisimple), the block entanglement entropy Sf(n)S_{f}(n) scales logarithmically with the block size nn in the thermodynamic limit LL\rightarrow\infty:

Sf(n)=NB2lnn+Sf0,S_{f}(n)=\frac{N_{B}}{2}\ln n+S_{f0}, (1)

where Sf0S_{f0} is an additive non-universal constant. Combining with a field-theoretic prediction made by Castro-Alvaredo and Doyon doyon , one is able to identify the number of type-B GMs with the fractal dimension df=NBd_{f}=N_{B} FMGM ; golden . Such a logarithmic scaling behavior of the block entanglement entropy Sf(n)S_{f}(n) provides an efficient way to extract the number of type-B GMs, or equivalently, the fractal dimension from numerical simulations of quantum many-body systems in the context of the iMPS representation idmrg . However, this requires us to ensure that the simulation results be accurate, with the bond dimension χ\chi being extremely large. We have described a subroutine to efficiently evaluate the block entanglement entropy Sf(n)S_{f}(n) in Section A of the Supplementary Material (SM). In this way we are able to perform a finite block-size scaling analysis of the entanglement entropy Sf(n)S_{f}(n) for scale-invariant states, which appear to be highly degenerate ground states for quantum many-body systems undergoing SSB with type-B GMs (for more details, cf. Section B of the SM).

A more convenient way is to develop a finite-entanglement scaling analysis for scale-invariant states in the context of the iMPS representation, in parallel to conformally invariant states tagliacozzo ; wanghl ; pollmann . For this purpose, we turn to the entanglement entropy Sf(χ)S_{f}(\chi) for the semi-infinite chain instead of a finite-size block, which is defined as Sf(χ)=αΛα2lnΛα2S_{f}(\chi)=-\sum_{\alpha}\Lambda^{2}_{\alpha}\ln\Lambda^{2}_{\alpha}, in terms of the singular values Λα\Lambda_{\alpha} (α=1,,χ\alpha=1,\ldots,\chi, with χ\chi being the bond dimension). To achieve this goal, we remark that, for a finite-size block, the time τ\tau taken for a local disturbance to propagate through the entire block in a coherent way scales linearly with nn: τn\tau\sim n. Taking into account the dispersion relation ωkz\omega\sim k^{z}, with zz being the dynamical critical exponent, we have ξτz\xi\sim\tau^{z}, where ξ\xi is the correlation length. Hence it is plausible to replace nn by ξ1/z\xi^{1/z}. Accordingly, for any nonzero fillings fα(α=1,,R)f_{\alpha}(\alpha=1,\cdots,R), the entanglement entropy Sf(χ)S_{f}(\chi) for the semi-infinite chain takes the form

Sf(χ)=NB2zlnξ(χ)+Sf0(χ).{S_{f}(\chi)=\frac{N_{B}}{2z}\ln\xi(\chi)+S_{f0}}(\chi). (2)

Here Sf0(χ)S_{f0}(\chi) is an additive non-universal constant. We remark that the correlation length ξ(χ)\xi(\chi) scales as ξχκ\xi\sim\chi^{\kappa}, with κ\kappa being the finite-entanglement scaling exponent, introduced in Ref. tagliacozzo for conformally invariant states.

With the above discussions in mind, we are able to extract the number of type-B GMs, or equivalently, the fractal dimension, from the iMPS representation for scale-invariant states, if the dynamical critical exponent is known, and vice versa. Here we remark that an alternative way to extract the dynamical critical exponent zz from simulation results of the infinite Density Matrix Renormalization Group (iDMRG) algorithm idmrg is described in Section C of the SM.

III Illustrative examples

To illustrate the generic scheme we focus on three fundamental models, which are chosen as typical examples to exhibit SSB with type-B GMs.

The first model is the spin-ss Heisenberg ferromagnetic model described by the Hamiltonian

=j𝐒j𝐒j+1,\mathscr{H}=-\sum_{j}\mathbf{S}_{j}\cdot\mathbf{S}_{j+1}, (3)

where 𝐒j=(Sjx,Sjy,Sjz)\mathbf{S}_{j}=(S_{j}^{x},S_{j}^{y},S_{j}^{z}) denotes the spin-ss operator at site jj. The model possesses the symmetry group SU(2)\rm{SU}(2), with the generators being Sx=jSjx,Sy=jSjyS^{x}=\sum_{j}S_{j}^{x},S^{y}=\sum_{j}S_{j}^{y} and Sz=jSjzS^{z}=\sum_{j}S_{j}^{z}. In this case, SSB occurs from SU(2)\rm{SU}(2) to U(1)\rm{U}(1), with the number of type-B GMs NB=1N_{B}=1 Watanabe .

The second model is the SU(3)\rm{SU}(3) spin-1 ferromagnetic model described by the Hamiltonian

=j[(𝐒j𝐒j+1)+(𝐒j𝐒j+1)2],\mathscr{H}=-\sum_{j}\left[(\mathbf{S}_{j}\cdot\mathbf{S}_{j+1})+(\mathbf{S}_{j}\cdot\mathbf{S}_{j+1})^{2}\right], (4)

where 𝐒j=(Sjx,Sjy,Sjz)\mathbf{S}_{j}=(S_{j}^{x},S_{j}^{y},S_{j}^{z}) are spin-11 operators at site jj. Note that this model appears as a special case of the well-studied spin-1 bilinear-biquadratic model, with its peculiarity being that the Hamiltonian (4) is exactly solvable by means of the Bethe ansatz Sutherland . The model possesses the symmetry group SU(3)\rm{SU(3)}, with the generators being realized in terms of the spin-1 operators Kα=jKαjK_{\alpha}=\sum_{j}K_{\alpha}^{j} (α=1,2,,8)(\alpha=1,2,\ldots,8), where K1=1/2jSjxK_{1}=1/2\sum_{j}S_{j}^{x}, K2=1/2jSjyK_{2}=1/2\sum_{j}S_{j}^{y}, K3=1/2jSjzK_{3}=1/2\sum_{j}S_{j}^{z}, K4=13/2j(Sjz)2K_{4}=1-3/2\sum_{j}(S_{j}^{z})^{2}, K5=1/2j((Sjx)2(Sjy)2)K_{5}=1/2\sum_{j}({(S_{j}^{x})}^{2}-{(S_{j}^{y})}^{2}), K6=1/2j(SjySjz+SjzSjy)K_{6}=1/2\sum_{j}(S_{j}^{y}S_{j}^{z}+S_{j}^{z}S_{j}^{y}), K7=1/2j(SjzSjx+SjxSjz)K_{7}=1/2\sum_{j}(S_{j}^{z}S_{j}^{x}+S_{j}^{x}S_{j}^{z}) and K8=1/2j(SjxSjy+SjySjx)K_{8}=1/2\sum_{j}(S_{j}^{x}S_{j}^{y}+S_{j}^{y}S_{j}^{x}). In this case, the number of type-B GMs NB=2N_{B}=2, given SSB occurs from SU(3)\rm{SU}(3) to U(1)×U(1)\rm{U}(1)\times\rm{U}(1) FMGM .

The third model is the SO(4){\rm SO}(4) spin-orbital model described by the Hamiltonian So4

=j(ζ+𝐒j𝐒j+1)(ζ+𝐓j𝐓j+1),\mathscr{H}=-\sum_{j}(\zeta+\mathbf{S}_{j}\cdot\mathbf{S}_{j+1})(\zeta+\mathbf{T}_{j}\cdot\mathbf{T}_{j+1}), (5)

where 𝐒j=(Sjx,Sjy,Sjz)\mathbf{S}_{j}=(S_{j}^{x},S_{j}^{y},S_{j}^{z}) are spin-1/21/2 operators and Tj=(Tjx,Tjy,Tjz)\textbf{T}_{j}=(T_{j}^{x},T_{j}^{y},T_{j}^{z}) are orbital pseudo-spin 1/2 operators at site jj. Here we restrict ourselves to the two particular points ζ=3/4\zeta=3/4 and ζ=\zeta=\infty, both of which share the same ground state subspace. Actually, the model (5), with ζ=3/4\zeta=3/4 and ζ=\zeta=\infty, may be recognized as the model studied by Kolezhuk and Mikeska kolezhuk , with the opposite sign, and a model consisting of two decoupled SU(2){\rm SU(2)} spin-1/21/2 Heisenberg ferromagnetic chains. The model possesses the symmetry group SO(4){\rm SO(4)}, isomorphic to SU(2)×SU(2){\rm SU(2)}\times{\rm SU(2)}, with the generators of the two copies of SU(2){\rm SU(2)} being Sx=jSjxS^{x}=\sum_{j}S_{j}^{x}, Sy=jSjyS^{y}=\sum_{j}S_{j}^{y}, and Sz=jSjzS^{z}=\sum_{j}S_{j}^{z}, and Tx=jTjxT^{x}=\sum_{j}T_{j}^{x}, Ty=jTjyT^{y}=\sum_{j}T_{j}^{y} and Tz=jTjzT^{z}=\sum_{j}T_{j}^{z}. In this case, SSB occurs from SO(4){\rm SO(4)} to U(1)×U(1){\rm U(1)}\times{\rm U(1)}, with the number of type-B GMs NB=2N_{B}=2.

IV Simulation results

In order to simulate the three selected models (3), (4) and (5), one needs to develop the iDMRG algorithm idmrg , with U(1){\rm U}(1), U(1)×U(1)\rm{U}(1)\times\rm{U}(1) and U(1)×U(1)\rm{U}(1)\times\rm{U}(1) being implemented as a symmetry group, respectively. This is necessary, since we have to target a specific ground state with a given filling. In this sense, the iDMRG algorithm is the method of choice, which is able to efficiently produce the iMPS representation for one of the highly degenerate ground states arising from SSB with type-B GMs.

Refer to caption
Figure 1: The entanglement entropy Sf(χ)S_{f}(\chi) versus lnξ(χ)\ln\xi(\chi) for the spin-ss Heisenberg ferromagnetic model (3) with ss being 1/2,1,3/21/2,1,3/2 and 2. The different fillings (a) f=sf=s and (b) f=s1/2f=s-1/2 have been chosen. The bond dimension χ\chi ranges from 2020 to 160160.
Refer to caption
Figure 2: The entanglement entropy Sf(χ)S_{f}(\chi) versus lnξ(χ)\ln\xi(\chi) for the SU(3)\rm{SU}(3) ferromagnetic model (4). Here we have chosen the fillings f=(1/3,1/3)f=(1/3,1/3) and f=(1/4,1/2)f=(1/4,1/2), with the bond dimension χ\chi ranging from 8080 to 10001000.
Refer to caption
Figure 3: The entanglement entropy Sf(χ)S_{f}(\chi) versus lnξ(χ)\ln\xi(\chi) for the SO(4){\rm SO}(4) spin-orbital model (5) with ζ=3/4\zeta=3/4 and ζ=\zeta=\infty. Here we have chosen the fillings f=(1/2,1/2)f=(1/2,1/2) and f=(5/12,5/12)f=(5/12,5/12), with the bond dimension χ\chi ranging from 100100 to 10001000.

In Fig. 1, we plot the entanglement entropy Sf(χ)S_{f}(\chi) versus lnξ(χ)\ln\xi(\chi) for the spin-ss Heisenberg ferromagnetic model (3) with s=1/2,1,3/2s=1/2,1,3/2 and 22. Here we have chosen different fillings: (a) f=sf=s and (b) f=s1/2f=s-1/2, with the bond dimension χ\chi ranging from 2020 to 160160. To this end, the unit cell in the iMPS representation consists of two lattice sites. For f=sf=s, the number of type-B GMs is extracted to be NB=0.9924,0.9904,0.992N_{B}=0.9924,0.9904,0.992 and 0.99120.9912 for s=1/2,1,3/2s=1/2,1,3/2 and 22, respectively. The relative error is less than 1%1\%, if we adopt the value of the dynamical critical exponent to be z=2z=2, as predicted from the conventional spin wave theory. Conversely, the other way around is to extract the dynamical critical exponent if we adopt NB=1N_{B}=1. The dynamical critical exponent is extracted to be z=2.0153,2.0194,2.0161z=2.0153,2.0194,2.0161 and 2.01782.0178 for s=1/2,1,3/2s=1/2,1,3/2 and 22, respectively. The relative error is less than 1%1\%. Similarly, for f=s1/2f=s-1/2, the number of type-B GMs is extracted to be NB=0.9928,0.992,0.9904N_{B}=0.9928,0.992,0.9904 and 0.99160.9916 for s=1/2,1,3/2s=1/2,1,3/2 and 22, respectively. Then a relative error is less than 1%1\%, if we adopt the dynamical critical exponent value z=2z=2. Conversely, the dynamical critical exponent is extracted to be z=2.0145,2.0161,2.0194z=2.0145,2.0161,2.0194 and 2.01692.0169 for s=1/2,1,3/2s=1/2,1,3/2 and 22, respectively, with the relative error again less than 1%1\%.

In Fig. 2, we plot the entanglement entropy Sf(χ)S_{f}(\chi) versus lnξ(χ)\ln\xi(\chi) for the SU(3)\rm{SU}(3) ferromagnetic model (4). The filling factors are chosen to be f=(1/3,1/3)f=(1/3,1/3) and f=(1/4,1/2)f=(1/4,1/2), with the bond dimension χ\chi ranging from 8080 to 10001000. Here the unit cell in the iMPS representation consists of three and four lattice sites, respectively. The number of type-B GMs is extracted to be NB=1.9804N_{B}=1.9804 for f=(1/3,1/3)f=(1/3,1/3) and 1.98161.9816 for (1/4,1/2)(1/4,1/2), with the relative error being less than 1%1\%, if we adopt the dynamical critical exponent z=2z=2, as predicted from the conventional spin wave theory. Conversely, adopting the value NB=2N_{B}=2, the dynamical critical exponent is extracted to be z=2.0198z=2.0198 for f=(1/3,1/3)f=(1/3,1/3) and 2.01862.0186 for (1/4,1/2)(1/4,1/2), with again the relative error less than 1%1\%.

Fig. 3 shows plots of the entanglement entropy Sf(χ)S_{f}(\chi) versus lnξ(χ)\ln\xi(\chi) for the SO(4){\rm SO}(4) spin-orbital model (5), with (a) ζ=3/4\zeta=3/4 and (b) ζ=\zeta=\infty. Here we have chosen the fillings f=(1/2,1/2)f=(1/2,1/2) and f=(5/12,5/12)f=(5/12,5/12), with the bond dimension χ\chi ranging from 100100 to 10001000. The unit cell in the iMPS representation consists of four and six lattice sites, respectively. If we adopt the dynamical critical exponent z=2z=2, as predicted from the conventional spin wave theory, the best linear fit is exploited to estimate the number of type-B GMs as NB=1.9296N_{B}=1.9296 and 1.94681.9468 in Fig. 3(a), with relative error less than 4%4\%, and NB=1.9512N_{B}=1.9512 and 1.95241.9524 in Fig. 3(b), with relative error less than 3%3\%. Here if we adopt NB=2N_{B}=2, the dynamical critical exponent is extracted to be z=2.073z=2.073 and 2.0592.059 in Fig. 3(a) and z=2.05z=2.05 and 2.04882.0488 in Fig. 3(b), with in each case a relative error less than 4%4\%.

V Summary

A generic scheme to perform a finite-entanglement scaling analysis has been put forward for highly degenerate ground states arising from SSB with type-B GMs, which are scale-invariant, but not conformally invariant. Extensive numerical simulations have been performed for the three selected models – the spin-ss Heisenberg ferromagnetic model, the SU(3)\rm{SU}(3) ferromagnetic model and the SO(4)\rm{SO}(4) spin-orbital model. Actually, the number of type-B GMs NBN_{B} may be reliably extracted from finite block-size scaling, as long as the bond dimension χ\chi is large enough, within a reasonable accuracy. A detailed exposition for a finite block-size scaling analysis to extract the number of type-B GMs has been described in Section D of the SM. This in turn allows us to extract the dynamical critical exponent from finite-entanglement scaling.

Acknowledgements.
We appreciate insightful discussions with John Fjaerestad about the counting rule for the GMs.

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