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Energy Level Crossing and Entanglement

Willi-Hans Steeb

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

Reprint requests to W.-H. S.; E-mail: steebwilli@gmail.com

Z. Naturforsch.64a,445 – 447 (2009); received November 24, 2008 / revised January 15, 2009 We consider a Hamilton operator in a finite dimensional Hilbert space with energy level crossing.

We discuss the question how energy level crossing and entanglement of states in this Hilbert space are intertwined. Since energy level crossing is related to symmetries of the Hamilton operator we also derive these symmetries and give the reduction to the invariant Hilbert subspaces.

Key words:Energy Level Crossing; Symmetries; Group Theory; Entanglement.

1. Introduction

A basic problem in quantum mechanics is the cal- culation of the energy spectrum of a given (hermi- tian) Hamilton operator ˆH. It is assumed that the her- mitian Hamilton operator acts in a Hilbert spaceH. Here we assume we have a finite dimensional Hilbert space. Thus the spectrum is discrete. In many cases the Hamilton operator depends on a real parame- ter. The question whether or not energy levels can cross by changing the parameter was first discussed by Hund [1]. He studied examples only and conjec- tured that, in general no crossing of energy levels can occur. In 1929 von Neumann and Wigner [2] inves- tigated this question more rigorously and found the following theorem: Real symmetric matrices (respec- tively the hermitian matrices) with a multiple eigen- value form a real algebraic variety of codimension 2 (respectively 3) in the space of all real symmetric ma- trices (respectively all hermitian matrices). This im- plies the famous “non-crossing rule” which asserts that a “generic” one parameter family of real symmetric matrices (or two-parameter family of hermitian ma- trices) contains no matrix with multiple eigenvalue.

“Generic” means that if the Hamilton operator ˆH ad- mits symmetries the underlying Hilbert space has to be decomposed into invariant Hilbert subspaces using group theory [3]. Meanwhile a large number of re- searcher have studied energy level crossing (see [4] and references therein).

Entanglement of states in finite-dimensional Hilbert spaces(dimH ≥4)has been investigated by many au- thors (see [5], [6] and references therein). The measure

0932–0784 / 09 / 0700–0445 $ 06.00 c2009 Verlag der Zeitschrift f¨ur Naturforschung, T ¨ubingen·http://znaturforsch.com

of entanglement for bipartite states are the von Neu- mann entropy, concurrence and the 2-tangle.

2. Theory

We consider the Hilbert spaceC4and the Hamilton operator

Hˆ=h¯ω(σzσz) +∆(σxσx),

whereω>0 and∆>0. The Hamilton operator shows energy level crossing and the unitary operatorU(t) = exp(−i ˆHt/h)¯ can generate entangled states from unen- tangled states.

The eigenvalues of ˆHare given by E1=h¯ω+∆, E2=−(h¯ω+∆), E3=−h¯ω+∆, E4=h¯ω

with the corresponding normalized eigenvectors

|Φ+= 1

2



 1 0 0 1



, |Ψ= 1

2



 0 1

1 0



,

|Ψ+= 1

2



 0 1 1 0



, |Φ= 1

2



 1 0 0

−1



.

Note that the states do not depend on the parameters ω and∆. These states are the Bell states [4]. The Bell states are fully entangled. As a measure of entangle- ment we can apply the tangle which is the squared

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446 W.-H. Steeb·Energy Level Crossing and Entanglement concurrence. The concurrenceC for a pure state|ψ

inH=C4is given by C=2

det

c00c01

c10c11

with the state|ψwritten in the form

|ψ=

1

j,k=0

cjk|j ⊗ |k,

and|j(j=0,1)denotes the standard basis inC2. Energy level crossing occurs if∆=h¯ω. Then we have the eigenvaluesE1=2 ¯hω,E3=0,E4=0,E2=

2 ¯hω. For the degenerate eigenvalue 0 we have the eigenvectors

|Ψ+= 1

2



 0 1 1 0



, |Φ= 1

2



 1 0 0

−1



.

Since we have energy level crossing the Hamilton op- erator ˆHadmits a symmetry. We have

xσx,σzσz] =0. Thus

[H,ˆ σxσx] =0, [H,ˆ σzσz] =0.

Now both {I2⊗I2,σxσx} and {I2⊗I2,σzσz} form a group under matrix multiplication, where I2

is the 2×2 identity matrix. Both can be used to find the reduction to Hilbert subspaces. Consider first the group{I2⊗I2,σxσx}. The character table provides the projection operators

Π1=1

2(I2⊗I2xσx), Π2=1

2(I2⊗I2σxσx).

The projection operator Π1 projects into a two- dimensional Hilbert space spanned by the Bell states

1 2



 1 0 0 1



, 1

2



 0 1 1 0



with the corresponding matrix for the Hamilton opera-

tor

h¯ω∆ 0 0 −h¯ω−∆ .

The projection operator Π2 projects into a two- dimensional Hilbert space spannded by the Bell states

1 2



 1 0 0

1



, 1

2



 0 1

−1 0



with the corresponding matrix for the Hamilton opera-

tor

h¯ω+∆ 0 0 −h¯ω+∆ .

Consider now the group{I2⊗I2,σzσz}. The char- acter table provides the projection operators

Π1=1

2(I2⊗I2zσz), Π2=1

2(I2⊗I2σzσz).

The projection operator Π1 projects into a two- dimensional Hilbert space spanned by elements of the standard basis



 1 0 0 0



,



 0 0 0 1



with the corresponding matrix for the Hamilton opera-

tor

h¯ω ∆

h¯ω .

The projection operator Π2 projects into a two- dimensional Hilbert space spanned by the elements of the standard basis



 0 1 0 0



,



 0 0 1 0



with the corresponding matrix for the Hamilton opera-

tor

−h¯ω ∆

−h¯ω .

Note that the elements of these two groups are ele- ments of the Pauli groupP2which is defined by

Pn:={I2,σx,σy,σz}⊗n⊗ {±1,±i} whereI2is the 2×2 identity matrix.

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W.-H. Steeb·Energy Level Crossing and Entanglement 447 Next we look at the time evolution U(t) =

exp(−i ˆHt/h)¯ . We obtain

exp(−i ˆHt/h) =¯ e−iωt(σz⊗σz)e−it∆(σx⊗σx)/¯h. Since

e−iωt(σz⊗σz)=I4cos(ωt) +i(σzσz)sin(ωt) and

e−i∆t(σx⊗σx)/¯h)=I4cos(t∆/h)+¯ i(σxσx)sin(t∆/h)¯ we obtain

e−i ˆHt/¯h=I4cos(ωt)cos(t∆/h)¯

+i(σzσz)sin(ωt)cos(t∆/h)¯ +i(σxσx)cos(ωt)sin(t∆/h)¯

zσx)zσx)sin(ωt)sin(t∆/h).¯

[1] F. Hund, Z. Phys.40, 742 (1927).

[2] J. von Neumann and E. Wigner, Phys. Z.30, 467 (1929).

[3] W.-H. Steeb, Problems and Solutions in Theoretical and Mathematical Physics, Volume II: Advanced Level, World Scientific, Singapore 2003.

[4] W.-H. Steeb, A. J. van Tonder, C. M. Villet, and S. J. M.

Brits, Found. of Phys. Lett.1, 147 (1988).

[5] W.-H. Steeb and Y. Hardy, Problems and Solutions in Quantum Computing and Quantum Information, sec- ond edition, World Scientific, Singapore 2006.

[6] M. A. Nielsen and I. L. Chuang, Quantum Comput- ing and Quantum Information, Cambridge University Press, Cambridge 2000.

ApplyingU(t)to the unentangled state(1 0 0 0)Tyields

U(t)



 1 0 0 0



=



cos(ωt)cos(t∆/h) +¯ i sin(ωt)cos(t∆/h)¯ 0

0

sin(ωt)sin(∆t/h) +¯ i cos(ωt)sin(t∆/h)¯



.

Depending on t, ω and ∆ we can obtain entangled states using the concurrence as measure. For the case h¯ω=∆(level crossing) the state reduces to



cos2(ωt) +i sin(ωt)cos(ωt) 0

0

sin2(ωt) +i cos(ωt)sin(ωt)



.

The results given above can be extend to the Hamilton operator

Hˆ=h¯ω(

N-factors σzσz⊗ ··· ⊗σz)+∆(

N-factors σxσx⊗ ··· ⊗σx) withN>2 andNeven. For this case we also have

xσx⊗ ··· ⊗σx,σzσz⊗ ··· ⊗σz] =0.

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