Real-space entanglement spectra of projected fractional quantum Hall states using Monte Carlo methods Abhishek Anand and G. J. Sreejith

2025-04-29 0 0 1.03MB 14 页 10玖币
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Real-space entanglement spectra of projected fractional quantum Hall states using
Monte Carlo methods
Abhishek Anand and G. J. Sreejith
Indian Institute of Science Education and Research, Pune 411008, India
Real-space entanglement spectrum (RSES) of a quantum Hall (QH) wavefunction gives a natural
route to infer the nature of its edge excitations. Computation of RSES becomes expensive with
an increase in the number of particles and included Landau levels (LL). RSES can be efficiently
computed using Monte Carlo (MC) methods for trial states that can be written as products of
determinants such as the composite fermion (CF) and parton states. This computational efficiency
also applies to the RSES of lowest Landau level (LLL) projected CF and parton states; however,
LLL projection to be used here requires approximations that generalize the Jain Kamilla (JK)
projection. This work is a careful study of how this approximation should be made. We identify the
approximation closest in spirit to JK projection and perform tests of the approximations involved
in the projection by comparing the MC results with the RSES obtained from computationally
expensive but exact methods. We present the techniques and use them to calculate the exact RSES
of the exact LLL projected bosonic Jain 2/3 state in bipartition of systems of sizes up to N= 24
on the sphere. For the lowest few angular momentum sectors of the RSES, we present evidence to
show that MC results closely match the exact spectra. We also discuss other plausible projection
schemes. We also calculate the exact RSES of the unprojected fermionic Jain 2/5 state obtained
from the exact diagonalization of the Trugman-Kivelson Hamiltonian in the two lowest LLs on the
sphere. By comparing with the RSES of the unprojected 2/5 state from Monte Carlo methods, we
show that the latter is practically exact.
I. INTRODUCTION
Fractional quantum Hall (FQH) effect1,2 provides a
rich set of experimentally realizable interacting topolog-
ically ordered quantum phases. Conceptual insights into
the microscopic structure of these phases have been aided
by careful numerical studies of variational wavefunctions
describing the phases. The many aspects of the FQH
states like fractional charge,3,4 non-trivial statistics4–8
and edge modes have been understood in the language of
such variational wavefunctions. Entanglement spectrum
(ES)9of a variational state is a key tool in the char-
acterization of the order in the state.10–14 The notion
of entanglement spectra was introduced as a means to
get more insights into the topological order beyond what
is provided by more succinct measures like the entan-
glement entropy.15–18 Entanglement spectra of a many-
body state is defined as the eigenvalue spectrum (typi-
cally represented in a negative log scale) of the reduced
density matrix after a bipartition of the system. Cor-
respondence between the entanglement Hamiltonian and
the edge spectrum has been explored both in the FQH
contexts and elsewhere.13,19–24 Being a quantity natu-
rally obtained during DMRG calculations, entanglement
spectrum has been used to characterize the phases of in-
teracting Hamiltonians in such studies.25–28
In quantum Hall systems, entanglement spectrum can
be defined by bipartitioning the system in the momen-
tum orbital space or in the real space producing the or-
bital space entanglement spectrum (OES) or real space
entanglement spectrum(RSES) respectively. Since under
Landau quantization, the single particle momentum or-
bitals are spatially localized, they contain closely related
information. Both OES and RSES have been studied
extensively for many QH states.29–34 Typically OES is
easier to compute for states obtained from exact diago-
nalization or DMRG calculations whereas RSES is easier
to compute for states described by variational wavefunc-
tions expressed in terms of particle coordinates. In this
paper, we focus on the RSES estimations using Monte
Carlo methods focusing on the Jain composite fermion
(CF) states.35
ES of CF wavefunctions have been studied but meth-
ods using exact evaluation of the LLL projected state
is computationally expensive, allowing studies only in
small systems (N10).30 On the other hand, entan-
glement spectrum of the unprojected CF state and par-
ton states35 can be efficiently obtained using Monte Carlo
methods.33,34 The bottleneck in extending the same tech-
nique to the projected CF states (which are energetically
more favorable) is the difficulty in implementing the LLL
projection. In a large number of studies involving en-
ergetics of the CF states, an approximate method in-
troduced by Jain and Kamilla (JK) to perform lowest
Landau level (LLL) projection has been found to pro-
vide computationally efficient and reliable results.36–38
Combining the JK projection with the MC methods
for RSES evaluation involves further approximations but
this can be used for calculations in systems upto hundred
particles.32–34 Testing the approximations require com-
parison with computationally expensive but exact RSES
calculated using alternate methods. This is the goal of
the paper.
We identify cases where alternate exact methods can
be employed to calculate RSES in relatively large sys-
tems. For the fermionic Jain 2/5th state, the Trugman-
Kivelson (TK) Hamiltonian39 can be diagonalized to pro-
duce an exact expansion of the unprojected CF state.
arXiv:2210.11514v1 [cond-mat.str-el] 20 Oct 2022
2
RSES of the state can be obtained using a generalization
of the method presented by Chandran et al. in Ref. 29 We
use this to show that the MC method indeed produces
practically exact results for the RSES.
Construction of exact Hamiltonians for the projected
state is an open problem,40 so a similar strategy cannot
be employed to test the RSES for the projected state.
Instead we consider the case of the bosonic Jain 2/3rd
state, where we employ exact projection in a manner
that allows us to exactly compute the low momentum
entanglement spectrum in systems as large as N= 24.
We find that as system size increases the results from
approximate projection employed in the MC method ap-
proach the exact RSES, at least in the low momentum
sectors.
We emphasize that the results presented in this work
is not a comparison of the RSES of the exact projected
CF states (ψEX) and the RSES of the JK projected CF
states (ψJK). Since the two states are nearly identically
to each other, we expect their RSES to be nearly the
same. Instead what we are testing is the effect of the
approximate projection used while implementing the MC
method for RSES calculation. The approximation in the
latter is similar in spirit to the JK projection but is not
the same. Secondly, the results presented compare the
approximate results from MC estimates of RSES with
the RSES of the ψEX. The comparison is done with ψEX
rather than with ψJK because, using methods described
in Sec. III B, RSES of ψEX can be computed exactly at
least for small systems. Doing the same for ψJK is harder.
This paper is structured as follows. We begin by pre-
senting the numerical techniques involved. We present,
in Sec II, a strategy for a numerically exact computation
of the RSES of the unprojected Jain 2/5th state obtained
from exact diagonalization of the TK Hamiltonian. We
will later use this to demonstrate that the RSES using
MC method is practically exact for the unprojected state.
In Sec. III, we give a summary of the method for com-
puting RSES of variational states by expanding them in
terms of entanglement wavefunctions (EWFs). The de-
tails of the method, originally introduced in Ref. 33, can
be found in Refs. 32 and 34. Section III B provides
the details for using this method with exactly projected
Jain 2/3rd state of bosons. We could use this to ob-
tain numerically exact RSES in systems up to size 24.
Section III D details the approximations that are made
to perform LLL projection of the EWFs, which makes
accessing large systems possible. All numerical results
benchmarking the methods are given in Sec. IV, and fi-
nally we conclude with Sec. V.
Notations: All calculations in the paper are performed
for systems in the spherical geometry where the sin-
gle particle Landau orbitals for a particle in the nth
LL and with angular momentum mare the monopole
harmonics,41–43 given by
YQnm =NQnm(1)Q+nmvQmuQ+m
×
n
X
s=0 n
s 2Q+n
Q+nms|v|2(ns)|u|2s(1)
where uand vare given by u= cos(θ/2)eιφ/2and v=
sin(θ/2)eιφ/2in terms of coordinates 0 θ < π and 0
φ < 2πon the sphere, and Qquantifies the strength of
monopole which produces a radial magnetic field of flux
2Qin units of flux quanta φ0=hc/e. The normalization
factor is given by
NQnm =
(2Q+ 2n+ 1)
4π
(Q+nm)!(Q+n+m)!
n!(2Q+n)! 1/2
(2)
II. RSES OF STATE EXPANDED IN SLATER
DETERMINANT BASIS
In this section, we describe the method to calculate
RSES for fermionic quantum Hall states which are ex-
pressed as linear combinations
ψ(r1,...,rN) = X
λ
cλMλ(r1,...,rN) (3)
where the basis states Mλare Slater determinants of
single particle momentum orbitals. The coefficients cλ’s
can, for instance, be from exact diagonalization. The
basis states Mλare parametrized by the ordered list of
occupied single particle orbitals λ(λ1, λ2. . . ) and can
be expanded as
Mλ(r1,...,rN) = 1
N!X
σ∈SN
(σ)
N
Y
i=1
φλσ(i)(ri) (4)
where φλi(ri)’s are the normalized single particle Landau
orbitals λi(ni, mi) specified by the LL-index niand
the angular momentum mi, and SNis the set of all per-
mutations of (1,2, . . . , N). In the spherical geometry, the
single particle orbitals are given by monopole harmonics
given in Eq.(1).
We present a method which enables us to compute
RSES for states with particles occupying different LLs.
For a real-space cut which respects the rotational symme-
try of the system, angular momentum states (projected
onto either subsystem) remain orthogonal to each other
as long as they are in same LL. However states with same
angular momentum but different LLs have non-zero over-
lap due to restricted limits of integration within each sub-
system. The method presented below extends the one
given in Ref. 29 which works for states restricted to the
LLL, by incorporating non-orthogonal momentum states.
In this work, we will use this method to compute
the RSES of unprojected Jain 2/5-state, which we get
3
as the ground state (using ED) of Trugman-Kivelson
Hamiltonian39 projected into the lowest 2 LLs treated
as degenerate.
For any wavefunction ψ(r1,...,rN) for Nparticles,
the density matrix is given by
ρ(r0
1, . . , r0
N;r1, . . , rN) = ¯
ψ(r1, . . , rN)ψ(r0
1, . . , r0
N)
RQid2ri|ψ(r1, . . , rN)|2
(5)
We partition the system into two subsystems Aand B
using an azimuthally symmetric cut (Fig.1) and con-
sider the sector where region Acontains NAparticles
(and Bhas NB=NNAparticles). We use the
following shorthands for collections of particle coordi-
nates R(r1,...,rN), RA(r1,...,rNA) and RB
(rNA+1,...,rN). The reduced density matrix for subsys-
FIG. 1. Azimuthally symmetric cut for the spherical geom-
etry.
tem Ais then given by
ρNA(R
0
A;RA) = RBdRBρ(RA,RB;R0
A,RB)
RAdRARBdRBρ(RA,RB;RA,RB)
=1
pNAN
NAZB
dRBρ(RA,RB;R
0
A,RB)
(6)
where pNAis the probability that subsystem Acontains
exactly NAparticles. Using Eqs.(3) and (4), we can
rewrite the Eq.(6) as
ρNA=1
pNAN
NAX
λ,λ0
¯cλcλ0ZB
dRBMλMλ0(7)
To simplify further, we will use the following property
Mλ(R) = rNA!NB!
N!X
µ,ν
hµ;νi=λ
µν Mµ(RA)Mν(RB).
(8)
Here the Slater determinant of Nparticles is expanded
as anti-symmetrization of products of Slater determi-
nants corresponding to ordered set of orbitals µ(of size
NA) and ν(of size NB) such that the ordered com-
bination of two is equal to λ( this constraint is rep-
resented by hµ;νi=λ). The sign corresponding to
the permutation σ, which makes (λσ(1), . . . , λσ(N)) =
(µ1, . . . , µNA, νNA+1, . . . , νN) is given by µν =(σ).
This allows us to rewrite ρNAas
ρNA(R
0
A,RA) = X
µ,µ0
Qµ,µ0Mµ(RA)Mµ0(R
0
A) (9)
where
Qµ,µ0=1
pNAX
ν,ν0ZB
dRB¯
Fµ
ν(RB)Fµ0
ν0(RB)
Fµ
ν(RB) = µν chµ;νiMν(RB) (10)
This integral contains the overlaps between the angular
momentum states which are restricted in Bsubsystem.
As mentioned before, overlap between single particle mo-
mentum orbitals in subsystem Bis non-zero only when
they have same angular momentum. Hence, only those
ordered sets ν,ν0contribute in the sum in Eq.(II) which
have identical set of angular momentum quantum num-
bers. Note that the LL-indices need not be the same.
The matrix Qin Eq.(10) can be numerically computed
by summing over such ordered sets νand ν0.
The reduced density matrix ρNAis block-diagonal
in angular momentum. Its LA
z-sectors, represented as
ρNA,LA
zis
ρNA,LA
z(R
0
A,RA) =
0
X
µ,µ0Mµ(RA)Qµ,µ0Mµ0(R
0
A).(11)
where we the restricted sum is over ordered sets µ,µ0of
size NAwhich have the correct total angular momentum
i.e. Lz(µ) = Lz(µ0) = LA
z. As the Slater determinant
states Mµs span the entire Hilbert space of A-subsystem,
any eigenvector χof ρNAwith eigenvalue kcan be written
as following linear combination
χ(RA) = X
µ
aµMµ(RA) (12)
where the basis Mµs are generally not orthogonal if they
contain states from higher LLs (n > 1). Using the eigen-
value equation, given by
ZA
dRAρNA(RA,R
0
A)χ(RA) =kχ(R
0
A) (13)
and Eq.(12), it can be shown that a matrix Mcan be
constructed such that it has same set of non-zero eigen-
values as that of ρNA, where M=QP where Qis defined
in Eq.(10) and Pis given by
Pµ,µ0=ZA
dRAMµ(RA)Mµ0(RA) (14)
which is the overlap matrix (inside A) for EWFs, which
can be computed using accurate numerical integration.
摘要:

Real-spaceentanglementspectraofprojectedfractionalquantumHallstatesusingMonteCarlomethodsAbhishekAnandandG.J.SreejithIndianInstituteofScienceEducationandResearch,Pune411008,IndiaReal-spaceentanglementspectrum(RSES)ofaquantumHall(QH)wavefunctiongivesanaturalroutetoinferthenatureofitsedgeexcitations.C...

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