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Spin Hamilton Operators, Symmetry Breaking, Energy Level Crossing, and Entanglement

Willi-Hans Steeba, Yorick Hardyb, and Jacqueline de Greefa

aInternational School for Scientific Computing, University of Johannesburg, Auckland Park 2006, South Africa

bDepartment of Mathematical Sciences, University of South Africa, Pretoria, South Africa Reprint requests to W.-H. S.; E-mail:steebwilli@gmail.com

Z. Naturforsch.67a,608 – 612 (2012) / DOI: 10.5560/ZNA.2012-0064 Received June 12, 2012 / published online August 20, 2012

We study finite-dimensional product Hilbert spaces, coupled spin systems, entanglement, and en- ergy level crossing. The Hamilton operators are based on the Pauli group. We show that swapping the interacting term can lead from unentangled eigenstates to entangled eigenstates and from an energy spectrum with energy level crossing to avoided energy level crossing.

Key words:Hilbert Space; Energy Level Crossing; Discrete Symmetries; Entanglement.

1. Introduction

LetH1,H2 be Hilbert spaces andH1⊗ H2be the tensor product Hilbert space [1,2]. Quite often a self- adjoint Hamilton operator acting on the tensor product Hilbert spaceH1⊗ H2can be written as

Hˆ =Hˆ1⊗I2+I1Hˆ2Vˆ, (1) where the self-adjoint Hamilton operator ˆH1acts in the Hilbert space H1, the self-adjoint Hamilton operator Hˆ2acts in the Hilbert spaceH2,I1is the identity oper- ator acting in the Hilbert spaceH1, andI2is the iden- tity operator acting in the Hilbert spaceH2. The self- adjoint operator ˆVacts in the product Hilbert space and ε is a real parameter. The main task would be to find the spectrum of ˆH.

In the following we consider the finite-dimensional Hilbert spaceH1=H2=Cnand then⊗denotes the Kronecker product [3–6]. LetInbe then×nidentity matrix. We consider the two hermitian Hamilton oper- ators

Hˆ =αA⊗In+In⊗βB+ε(A⊗B), (2) Kˆ=αA⊗In+In⊗βB+ε(B⊗A), (3) whereA,Bare nonzeron×nhermitian matrices and α, β,ε are real parameters with ε≥0. We assume that[A,B]6=0. The vector space of then×nmatrices

over Cform a Hilbert space with the scalar product hX,Yi:=tr(XY). We also assume thathA,Bi=0, i.e.

the nonzeron×n hermitian matricesAandBare or- thogonal to each other. Of particular interest would be the case whereAandBare elements of a semi-simple Lie algebra. We discuss the eigenvalue problem for the two Hamilton operators and its connection with entan- glement and energy level crossings for specific choices ofAandB. In the following the matricesAandBare realized by Pauli spin matrices. The Hamilton operator will be a linear combination of elements of the Pauli groupPn. The Pauli group [7] is defined by

Pn:={I2xyz}⊗n⊗ { ±1,±i}. (4) Such two-level and higher level quantum systems and their physical realization have been studied by many authors (see [8] and references therein). The thermo- dynamic behaviour is determined by the partition func- tions

ZHˆ(β) =tr(exp(−βH)),ˆ ZKˆ(β) =tr(exp(−βK)).ˆ Since

tr(H) =ˆ tr(Kˆ)

ntr(A) +βntr(B) +ε(tr(A))(tr(B)), the sum of the eigenvalues of the operators ˆHand ˆKare the same. However, in general, the partition functions will be different.

© 2012 Verlag der Zeitschrift f¨ur Naturforschung, T¨ubingen·http://znaturforsch.com

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2. Commutators, Eigenvalues, and Eigenvectors Let us first summarize the equations we utilize in the following. LetA,Bben×nmatrices overC. First note that we have the following commutators:

[A⊗In,InB] =0, [A⊗In,A⊗B] =0, [In⊗B,A⊗B] =0 and

[A⊗In,B⊗A] = ([A,B])⊗A, [In⊗B,B⊗A] =B⊗([B,A]).

The last two commutators would be 0 if [A,B] =0.

There is ann2×n2permutation matrixP(swap gate) such that P(AB)P−1=BA. This implies that P(A⊗In)P−1=InAandP(InB)P−1=BIn.

Now letAandBben×nhermitian matrices. If the eigenvalues and normalized eigenvectors of A and B areλj,ujj,vj,(j=1,2, . . . ,n), respectively, then the eigenvalues and normalized eigenvectors of the Hamil- ton operator (2) are given by [3–6]

α λj+β µk+ε λjµk, ujvk j,k=1,2, . . . ,n. Thus the eigenvectors are not entangled since they can be written as product states. These results can be ex- tended to the Hamilton operator

Hˆ =α(A⊗InIn) +β(InBIn) +γ(InIn⊗C) +ε(A⊗B⊗C)

and higher dimensions.

3. Pauli Spin Matrices and Entanglement

Since we realize the linear operators A andB by Pauli spin matrices we summarize some results for the Pauli spin matrices and their Kronecker products. Con- sider the Pauli spin matricesσzxy. The eigenval- ues are given by +1 and−1 with the corresponding normalized eigenvectors

1 0

, 0

1

, 1

√2 1

1

, 1

√2 1

−1

,

√1 2

−i 1

, 1

√ 2

i 1

forσzx, andσy, respectively. Consider now the three hermitian and unitary 4×4 matricesσx⊗σxy⊗σy, σz⊗σz. These matrices appear in Mermin’s magic square [9] for the proof of the Bell–Kochen–Specker theorem. Since the eigenvalues of the Pauli matrices are given by+1 and−1, the eigenvalues of the 4×4 matricesσx⊗σxy⊗σyz⊗σz are+1 (twice) and

−1 (twice). The eigenvectors can be given as product states (unentangled states), but also as entangled states (i.e. they cannot be written as product states). Obvi- ously,

1 0

⊗ 1

0

, 1

0

⊗ 0

1

, 0

1

⊗ 1

0

, 0

1

⊗ 0

1

are four normalized product eigenstates ofσz⊗σz. The normalized product eigenstates ofσx⊗σxare

1 2

1 1

⊗ 1

1

, 1

2 1

1

⊗ 1

−1

, 1

2 1

−1

⊗ 1

1

, 1

2 1

−1

⊗ 1

−1

.

The normalized product eigenstates ofσy⊗σyare 1

2 i

1

⊗ i

1

, 1

2 i

1

⊗ −i

1

, 1

2 −i

1

⊗ i

1

, 1

2 −i

1

⊗ −i

1

.

All three 4×4 matrices also admit the Bell basis

√1 2

 1 0 0 1

, 1

√2

 0 1 1 0

, 1

√2

 1 0 0

−1

, 1

√2

 0 1

−1 0

as normalized eigenvectors which are maximally en- tangled. As measure for entanglement the tangle [5,7, 10,11] will be utilized.

Consider now the hermitian and unitary 4×4 ma- trices σx⊗σz, σz⊗σx. Since the eigenvalues of the Pauli matrices are given by+1 and−1, the eigenval- ues of the 4×4 matricesσx⊗σzandσz⊗σx, are+1 (twice) and−1 (twice). The eigenvectors can be given as product states (unentangled states), but also as en- tangled states (i.e. they cannot be written as product states).

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The normalized product eigenstates ofσx⊗σzare

√1 2

1 1

⊗ 1

0

, 1

√2 1

1

⊗ 0

1

,

√1 2

1

−1

⊗ 1

0

, 1

√ 2

1

−1

⊗ 0

1

.

The normalized product eigenstates ofσz⊗σxare

√1 2

1 0

⊗ 1

1

, 1

√2 1

0

⊗ 1

−1

,

√1 2

0 1

⊗ 1

1

, 1

√ 2

0 1

⊗ 1

−1

.

The two 4×4 matrices also admit

1 2

−1

−1

−1 1

, 1

2

−1 1 1 1

, 1

2

 1

−1 1 1

, 1

2

 1 1

−1 1

as normalized eigenvectors which are maximally en- tangled. Note thatσy⊗σyalso admits these maximally entangled eigenvectors besides the Bell basis as eigen- vectors and the product eigenvectors.

For the triple spin interaction termσx⊗σy⊗σz, we obtain the eigenvalues+1 (fourfold) and−1 (fourfold) and all the eight product states as eigenstates given by the eigenstates ofσxyz. Owing to the degeneracies of the eigenvalues, we also find fully entangled states such as

1

2 1 1 0 0 0 0 i −iT

with the three-tangle as measure [11].

4. Examples

Consider now a specific example for αA and βB withn=2 andε>0. Utilizing the Pauli spin matri- ces

αA=¯ 1σz, βB=¯ 2σx,

whereα=¯ 1,β =¯ 2andω12are the frequen- cies. Note that[σzx] =2iσyand tr(H) =ˆ 0, tr(K) =ˆ 0.

The elements of the set

{I2⊗I2zI2,I2⊗σxz⊗σx}

form a commutative subgroup of the Pauli groupP2. The elementsσzI2,I2⊗σxx⊗σzare generators of

the Pauli groupP2. Now the eigenvalues and eigenvec- tors ofαAare given by

λ1=¯ 1, u1= 1

0

, λ2=−¯1, u2= 0

1

, and the eigenvalues and eigenvectors ofβBare given by

µ1=¯ 2, u1= 1

√ 2

1 1

,

µ2=−¯2, u2= 1

√2 1

−1

.

The Hamilton operator ˆHis given by the 4×4 matrix which can be written as direct sum of two 2×2 matri- ces:

He=

¯

1 ¯ 2+ε 0 0

¯

2¯ 1 0 0

0 0 −¯1 ¯ 2−ε

0 0 ¯ 2−ε −¯1

 .

The eigenvalues ofHeare

E112,ε) =¯ 1+¯ 2+ε, E212,ε) =¯ 1¯ 2−ε, E312,ε) =−¯1+¯ 2−ε, E412,ε) =−¯1¯ 2

with the corresponding eigenvectors (which can be written as product states)

1 0

⊗ 1

√ 2

1 1

, 1

0

⊗ 1

√ 2

1

−1

, 0

1

⊗ 1

√2 1

1

, 0

1

⊗ 1

√2 1

−1

. The Hamilton operator ˆKis given by the 4×4 matrix

Ke=

¯ 1 ¯ 2 ε 0

¯

2 ¯ 1 0 −ε ε 0 −¯1 ¯ 2 0 −ε ¯ 2 −¯1

with the four eigenvalues k112,ε) =−

q

¯

h212)22,

k212,ε) = q

¯

h212)22,

k312,ε) =− q

¯

h21−ω2)22, k412,ε) =

q

¯

h21−ω2)22

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and the corresponding unnormalized eigenvectors

ε ε k1h(ω¯ 12) k2+h(ω¯ 12)

 ,

ε ε k2h(ω¯ 12) k1+h(ω¯ 12)

 ,

ε

−ε k3h(ω¯ 1−ω2) k3h(ω¯ 1−ω2)

 ,

ε

−ε k4h(ω¯ 1−ω2) k4h(ω¯ 1−ω2)

 .

Thus for the Hamilton operator ˆH, we have energy level crossing [10,12] which is due to the discrete symmetry of the Hamilton operator ˆH. The permuta- tion matricesPwithPHPˆ T=Hˆ are given byP0=I4

and

P1=

1 0 0 0

0 1 0 0

0 0 0 1

0 0 1 0

 , P2=

0 1 0 0

1 0 0 0

0 0 1 0

0 0 0 1

 ,

P3=

0 1 0 0

1 0 0 0

0 0 0 1

0 0 1 0

 ,

whereP0=I4is the 4×4 identity matrix. The matri- cesP0,P1,P2,P3form a commutative group under ma- trix multiplication. These permutation matrices satisfy Pj2=I4for j=1,2,3,4. Thus 12(I4+Pk)and12(I4−Pk) (k=1,2,3) are projection matrices and the Hilbert spaceC4can be decomposed into invariant sub Hilbert spaces. In the present caseC2andC2.

For the Hamilton operator ˆK, we have no energy level crossing forε>0. The symmetry is broken, i.e.

the Hamilton operator ˆK only admitsP0=I4as dis- crete symmetry. Forε→∞and fixed frequencies, the eigenvalues for the two Hamilton operators approachε (twice) and−ε(twice). The four eigenvectors are en- tangled forε>0.

Extensions to higher order spin systems such as spin-1 are straightforward. An extension is to study the

Hamilton operators with triple spin interactions:

Hˆ=¯ 1x⊗I2I2) +¯ 2(I2⊗σy⊗I2) +¯ 3(I2⊗I2⊗σz) +γ12x⊗σyI2) +γ13xI2⊗σz) +γ23(I2⊗σy⊗σz) +ε(σx⊗σy⊗σz)

and

Kˆ=¯ 1x⊗I2I2) +¯ 2(I2⊗σy⊗I2) +¯ 3(I2⊗I2⊗σz) +γ12x⊗σyI2) +γ13xI2⊗σz) +γ23(I2⊗σy⊗σz) +ε(σz⊗σy⊗σx).

Triple spin interacting systems have been studied by several authors [13–15]. For ˆH, we find the eight prod- uct states given by the eigenstates ofσxyz. We also have energy level crossing owing to the symmetry of the Hamilton operator ˆH. For the Hamilton opera- tor ˆK, the symmetry is broken and no level crossing occurs. We also find entangled states for this Hamilton operator. As an entanglement measure, the three-tangle can be used [11]. Also the permutationsσz⊗σx⊗σy, σy⊗σz⊗σx of the interacting term could be investi- gated.

The question discussed in the introduction could also be studied for Bose systems with a Hamilton op- erator such as

Hˆ=α(bb⊗I)

+β(I⊗(b+b)) +γ(bb⊗(b+b)), whereIis the identity operator and⊗denotes the ten- sor product.

In conclusion, we have shown that swapping the terms in the interacting part of Hamilton operators act- ing in a product Hilbert space breaks the symmetry and thus the behaviour about entanglement and energy level crossing will change.

[1] E. Prugove´cki, Quantum Mechanics in Hilbert Space, 2nd edition, Academic Press, New York 1981.

[2] W.-H. Steeb, Hilbert Spaces, Wavelets, Generalised Functions and Modern Quantum Mechanics, Kluwer, Dordrecht 1998.

[3] W.-H. Steeb and Y. Hardy, Matrix Calculus and Kro- necker Product, 2nd edition, World Scientific, Singa- pore 2011.

[4] W.-H. Steeb, Problems and Solutions in Introductory and Advanced Matrix Calculus, World Scientific, Sin- gapore 2006.

[5] W.-H. Steeb and Y. Hardy, Problems and Solutions in Quantum Computing and Quantum Information, 3rd edition, World Scientific, Singapore 2011.

[6] W.-H. Steeb, Problems and Solutions in Theoret- ical and Mathematical Physics, 3rd edition, Vol-

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ume II: Advanced Level, World Scientific, Singapore 2009.

[7] M. A. Nielsen and I. L. Chuang, Quantum Comput- ing and Quantum Information, University Press, Cam- bridge 2000.

[8] D. Kielpinski, J. Opt. B: Quantum Semiclass. Opt. 5, R121 (2003).

[9] N. D. Mermin, Rev. Mod. Phys.65, 803 (1993).

[10] W.-H. Steeb and Y. Hardy, Quantum Mechanics using Computer Algebra, 2nd edition, World Scientific, Sin- gapore 2010.

[11] A. Wong and N. Christensen, Phys. Rev. A63, 044301 (2001).

[12] W.-H. Steeb, A. J. van Tonder, C. M. Villet, and S. J. M. Brits, Found. Phys. Lett.1, 147 (1988).

[13] C. Vanderzande and F. Igl´oi, J. Phys. A: Math. Gen.20, 4539 – 4549.

[14] R. Somma, G. Ortiz, E. Knill and J. Gubernatis, Int. J.

Quant. Inf.1, 189 (2003).

[15] B. P. Lanyon, C. Hempel, D. Nigg, M. M¨uller, R. Ger- ritsma, F. Z¨ahringer, P. Schindler, J. T. Barreiro, M. Rambach, G. Kirchmair, M. Heinrich, P. Zoller, R. Blatt, and C. F. Roos, arXiv:1109.1512v1 [quant- ph].

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