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Erratum : Cyclic geometrical quantum phases : group theory dérivation and manifestations in atomic physics

C. Bouchiat

To cite this version:

C. Bouchiat. Erratum : Cyclic geometrical quantum phases : group theory dérivation and manifestations in atomic physics. Journal de Physique, 1987, 48 (10), pp.1627-1631.

�10.1051/jphys:0198700480100162700�. �jpa-00210601�

(2)

Erratum : Cet article remplace l’article

"Cyclic

geometrical quantum phases : group

theory

dérivation and manifestations in atomic

physics"

J.

Physique

48

(1987)

1401-1406, qui a été

publié

sans que les corrections nécessaires aient été faites, ce dont la rédaction prie l’auteur et les lecteurs de bien vouloir l’excuser.

Cyclic geometrical quantum phases : group theory dérivation and manifestations in atomic

physics

C. Bouchiat

Laboratoire de Physique Théorique E.N.S. Paris*, 24, rue

Lhomond,

75231 Paris Cedex 05, France

(Reçu

le 5 juin 1987, accepti le ler juillet

1987)

Résumé.-Nous présentons une démonstration de la phase quantique adiabatique de Berry basée sur la théorie des groupes. Notre formalisme est ensuite utilisé pour analyser des manifestations possibles en Physique Atomique et

pour étudier la nouvelle phase quantique cyclique introduite récemment par Aharonov et Anandan.

Abstract.-We present a derivation of the Berry quantum adiabatic phase using group theory. Our formalism is used to discuss possible manifestations in Atomic Physics and to investigate the new cyclic quantum phase recently

introduced by Aharonov and Anandan.

Classification

Physics

Abstracts

03.65 - 42.50

In this note we shall first’ derive the adiabatic quantum phase discovered by Berry

[1,2]

by a group theoretical method. Our derivation applies to Hamil-

tonians having covariance properties with respect to

group transformations acting upon the external pa- rameters space. Our method which allows a system- atic evaluation of the non adiabatic corrections will be used to discuss a possible way to measure the Berry phase in optical pumping experiments. Finally we in- vestigate within our formalism the new cyclic quan- tum phase introduced by Aharonov and Anandan

[9].

Let us consider a class of Hamiltonians

H(B)

which describe quantum systems interacting with an

external uniform magnetic field B. The Hamiltonian

H(B)

is assumed to be invariant upon a simultaneous rotation of the quantum system and the external field B. More precisely let

R(n, cue)

be a rotation of axis n

and angle a and J the total angular momentum of the system, the following operator identity is assumed to

hold :

where

A time dependent Hamiltonian

H(t)

is generated by

applying

to a given initial field configuration Bo, a

time dependent rotation

R(t)

=

R(n(t), a(t)) :

Using

(1)

we can rewrite

H(t)

as :

In order to solve the time dependent Schrodinger equation :

it is convenient

to introduce the rotated frame state

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198700480100162700

(3)

1628

With the help of

(4)

one finds that

I(t))

obeys

the following Schr6dinger

equation :

with

The unitarity relation

U(R)t

=

U(R)-1

implies

that

H1 (t)

is indeed a Hermitian operator. In order

to evaluate explicitly

Hl (t)

we introduce a system of spherical coordinates to describe the motion of

B(t)

as given in figure 1

(X, y,

z are unit vectors along the

x, y, z axis

respectively).

It is convenient to take Bo in the z x plane :

We write the field

B(t)

corresponding to a given position on the closed curve

(C)

as :

For t = T

B(t)

is assumed to coincide

again

with Bo ; it implies

O(T)

= Oo and

cp(T )

= 2r.

We are now in position to compute

H1 (t)

in term

of the angular momentum operator J of the system :

Using (10)

and simple properties of the rotation group

one gets :

where we have set

By making a first order expansion of the unitary operator associated with the above product of rota-

tions one gets the following expression

forfil (t) :

It is convenient to introduce the projections of

the angular momentum Ju, J, Jw upon the orthonor- mal set of unit vectors

(u, v, w)

associated with Bo :

u =

Bo/-B,

w = y, v = wAu. In particular we have :

Fig.l.-Spherical coordinates for the closed curve (C) drawn by B(t) during the adiabatic cycle.

One readily obtains the following final

expression

for H1 (t) :

We shall assume now that

H(Bo)

is the Hamil- tonian of a complex atom interacting with Bo, writ-

ten in the gauge Ao =

1/2r A

Bo. The eigenstates

of

H(Bo) lot m)

are, in general, non degenerate and eigenstates of J.Bo = JuB :

Let us take as initial state an eigenstate of

H(Bo) :

Following the usual adiabatic approximation, we shall

first keep only the diagonal part of

H1 (t) :

Using

(7), (13)

and

(6)

we obtain the state vector at time t = T :

The Berry quantum adiabatic phase is readily

obtained from the two above formulae :

(4)

with

where

fl(C)

is the solid angle enclosed by the

curve

(C).

A very remarkable feature of the Berry phase is the

fact that it can be written as the circulation of a

classical gauge field

along

a closed loop. As Berry first

noted the gauge field relevant for the case considered here is that of magnetic monopole of charge m. This

result is

easily

recovered by noting that :

where Am is the monopole vector potential

(3).

Since it seems

difficult,

at least for atoms, to per- form a true interference experiment involving angular

momentum eigenstates we suggest to study the evo-

lution of a coherent mixture of state vectors having

different magnetic quantum numbers. This can be done by looking at the time dependence of the aver-

age value of J. Rare gas atoms with a non zero nuclear

spin appear to be convenient for our purpose. The in- teraction of a rare gas atom in its ground state with a

static magnetic field can be described

by

the effective Hamiltonian :

where I is the nuclear spin and -IN is given in term of

the nuclear magnetic moment by --IN Ih = UN - We associate with the spin

density

matrix

p(t)

a

rotated frame density matrix

p(t) :

We have the set of relations :

It

is

convenient to

study

the time variation of it is

given by

the

equations :

Keeping for the moment only the diagonal part of

Hl (t),

we obtain after

simple algebra

involving angu- lar momentum commutation relations :

with

One gets immediately using the same

manipula-

tions as in equations

(14) :

The operator I± having non zero matrix element

only between states with Am = ±1 the time evo-

lution of

(I:t:.)

involves, as expected, the difference

1m (C) - 1m:t:.l (C) = ±fl (C).

For practical purposes

we give the values of

( I" y

and

(Iw)

at time t = T, assuming

(Iw (0))

= 0 :

As a way to arrive at an

empirical

determina-

tion of the difference of the Berry phases associated

with states differing by one unit of angular momen-

tum ym

(C)-

ym,

(C) = - (m - m’)fZ(C),

we propose

to measure the phase shift of the nuclear spin pre- cession of atoms interacting with a magnetic field

B which varies slowly following a closed path on a sphere of radius B, with respect to that of atoms for which the field stays fixed during the same time in-

terval T. Such an experiment would be the quantum spin counterpart of the geometrical light polarization phase shift measurement performed recently with op- tical fibres

[4].

It is, in principle, possible to get the difference of Berry phases for states differing by more than one

unit of h when I >

1/2.

One may study the time evo-

lution of the spin alignment normal to the precession

axis :

We would like now to evaluate the non adiabatic corrections to formula

(18),

associated with the non

diagonal part of

Hl (t) :

The equation giving the time evolution oaf gets an extra term involving

To lowest order in

(ill (t))

n.d.

we

can neglect the

time variation of

(Iu).

The correcting term A

(I± (T))

to formula

(17)

is then obtained by a simple quadra-

ture :

(5)

1630

with

To formulate the adiabatic approximation we

write

0(t)

=

Ðo/(t/T)

and

p(t)

= 27r

g(t/T)

with

f (0) -

1,

g(o) =

0 and

f (1) = g(l) =

1. We as-

sume that the first and second order derivatives of the functions

f(s)

and

g(s)

are finite in the closed interval 0 s 1. The adiabatic approximation cor- responds to the limit

wNT --+

oo.

Using

an

integra-

tion

by

part one proves that the absolute value of the

correcting

term given by

(20)

behaves like

1 /WN T

when

IWNTI

--+ oo. If the system is prepared in such as

way that

(Iu (0))

= 0, it can be shown then that the

correcting

term is of the order of

(WNT) 2

In the above considerations we have ignored the

relaxation processes

during

the time interval T.

They

do not really constitute a problem

since,

for instance in the case of

’He,

the relaxation time T2 which de- scribes the

decay

of the transverse polarization can

be as

long

as several hours. The Larmor precession

of 3He nuclear polarization

has

been observed

by

C.

Cohen-Tannoudji

et al.

[5]

using an

optically

pumped 17 Rb cell as magnetometer. This very sensitive tech-

nique, which has been used recently to search for a

permanent electric dipole of l2gXe

[6],

seems to be

well

adapted

to a measurement of the

Berry

phase in quantum spin systems.

To measure the phase shift in formula

(18)

one

has to know accurately the

dynamical

phase wNT. We have assumed that in the cyclic evolution of the mag-

netic field its modulus remains constant. In practice

such a condition may be rather difficult to

satisfy.

To

account for possible deviations one writes :

B(t) = A(t)U(R(t))Bo

where

A(t)

is a

slowly varying

positive

scale factor with

Ã(O)

=

A(T).

The

Berry

phase re-

mains

unchanged

but the dynamical phase is replaced

by

wN

fo A(t)dt.

There is, in

principle

a way to can- cel out the dynamical phase and, at the same

time,

to double the

Berry

phase. At t = T one performs

a rapid reversal of the magnetic field :

B(T

+

6t) = -B(T) =

-Bo, where 6t > 0 is such that 6twN « 1, in order to insure the

validity

of the sudden approx- imation. Then a new adiabatic cycle is started for T t 2T with a magnetic field

B(t) = -B (t - T) = A(t - T) R(t - T) (-Bo).

The

Berry

phase

depends

upon

f3 (t)

only

through

the rotation

R(t)

=

R (t - T)

which is identical to

R(t)

up to a time translation. It follows then that :

On the contrary the dynamical phase mWN

fT, A (t -

T)dt

changes its sign. The average value of is then given at time t = 2T by :

In practice, the validity of the above result de-

pends upon the accuracy with which the magnetic

field can be monitored during the time intervals 0 t T, T t 2T, and reversed at time t = T + 0.

After the

writing

of a

preliminary

version of this

note we become aware of a preprint of D. Suter et al.

[7]

where the Berry phase for a quantum spin system is measured by a high field nuclear magnetic reson-

nance method following a suggestion of F. Moody et

al.

[8].

Although the N.M.R. experiment gives a clear

evidence for the Berry phase associated with simple

conical circuits, it does not provide an

experimen-

tal proof of the topological invariance properties of

the Berry phase :

"1m (C)

is invariant upon the set

of continuous deformations of the circuit

(C)

which

preserve the solid

angle

inclosed by

(C).

The optical

pumping method which involves low magnetic fields

could be a suitable way to test this fundamental prop- erty of the Berry phase for quantum spin systems.

Another

application

of the formalism developed

in this note concerns the cyclic geometrical phase in-

troduced recently by Aharonov and Anandan called thereafter the A.A.

phase [9].

A quantum physi-

cal system described by a Hilbert space state vec-

tor 11j1(t))

performs a cyclic evolution generated by a

Hamiltonian

H(t)

during the time interval 0 t T

i.e.

11j1(T))

coincides with

10(0))

up to a phase fac-

tor :

11j1(T))

=

exp(io) ltk(O)). (The

states

10(t))

are

assumed to be of unit

norm).

Let us consider the set

of vectors obtained from

11j1(t))

by multiplication by

an

arbitrary

time dependent phase factor :

10 (t)) !4 Ip (t))’

=

exp(if(t)) 10 (t)) .

The A.A.

phase is defined in such a way as to stay invariant under the above Abelian gauge transformation :

The density matrix

p(t) = 10(t)) (,P(t)

gives a

gauge invariant description of the system at time t.

The A.A.

phase

can be then associated with a closed

curve in the space

E(p)

of the pure state density ma-

trices i.e. such that

p2

= p. In the case of a spin

1/2

system the general form of p is :

where

p(t) = (6(t))

is a unit vector. The quantum cycle is associated with a closed curve drawn on the unit sphere S. It is easily seen that different Hamil- tonians could lead to the same curve

(C).

One takes

(6)

advantage of this freedom to search for a Hamiltonian

H(t) _ 1i/2ü.b(t)

such that the

dynamical phase

van-

ishes identically :

One verifies easily that

b(t)

=

p(t)

n

d/dt p(t)

is

the correct choice by showing that

p(t)

obeys the

evolution equation for

(a(t)).

In order to solve the

Schrodinger equation for

H(t)

one writes

p(t) = R(t)

.u. As before one introduces the rotated state

l"b(t))

=

U-1(R(t)) l,p(t)) ;

its evolution is governed by the

Hamiltonian

H(t)

=

Ho (t)± H1 (t)

where

H1 (t)

is

given by equation

(11)

and

Ho (t)

by :

Writing the action of the infinitesimal rotation

R-I(t)

d

R(t)

on any vector x as

w(t)dt 1B

x, the

Hamiltonians

Ho (t)

and

fl, (t)

read as follows :

The total Hamiltonian

Íl(t)

=

Ho(t)

+

H1 (t)

reduces

to :

We recognize the operator called previously

(H1

(t))d.

For t = 0 we have

p(t)

= u so that

1"’(0))

is

an eigenstate of s.u with eigenvalue

h/2.

For now on,

the calculation is identical to that of the Berry phase

for m

= 1/2

so that the A.A. phase reads :

Unlike the case of the Berry phase where one had

to rely upon the adiabatic

approximation (neglect

of

the

(H1(t))n.d.),

the result given in

equation (26)

is

exact. It has to be noted it can also be obtained within the adiabatic approximation by taking, this time, as Hamiltonian :

H(t)

=

w.s.p(t).

For spin higher than

1/2

the Berry and A.A. phases, except for those quantum cyclic evolutions which can

be

generated

by Hamiltonians linear in the

angular

momentum, are expected to be different, the reason being that the manifold associated with the pure state

density matrices is no longer the sphere S2 but in-

stead the

complex projective

space

Pn (C)

with n =

2S.

Ground state atomic hydrogen could be a

good

testing

ground

for the A.A. phase. Let

IF, M)

with

F = 1, 0 stand for the hydrogen

hyperfine

states. Let

us assume that the system is prepared in a coherent.

superposition of

)0,0) and 11, 1)

states by a 21 cm ra-

diofrequency

pulse.

(One

can keep track of the

(0,0) p 1,1)

coherence by measuring its beat with a refer-

ence hydrogen

maser).

Then one

applies

a variable

magnetic field

B (t)

with an intensity low

enough

so

that its action upon the state

0, 0)

can be

neglected.

The field is monitored in such a way that the state

1, 1)

undergoes a cyclic evolution. The A.A. phase

is then detected by its effects upon the phase of the

(0, 0 p 11, 1)

coherence.

A discussion of the Berry phase involving group

theory considerations has appeared in print recently

[10].

The point of view of the authors is rather differ- ent from the one adopted here : they stay within the adiabatic

approximation

while the method developed

here allows, in

principle,

a systematic evaluation of the non adiabatic corrections.

We would like to acknowledge very

stimulating

discussions with Prof. M. Berry and Prof. A. Pines.

After

completion

of this work appeared a paper which reports on the observation of the Berry phase involving a sample rotation in nuclear quadrupole res-

onance

[11].

However, to the best of our

knowkedge,

an experimental investigation of the topological in-

variance properties of the Berry phase is still

lacking.

References

[1]

BERRY, M.V., Proc. Roy. Soc. London, Ser

A392

(1984)

45.

[2]

SIMON, B., Phys. Rev. Lett. 51

(1983)

2176.

[3]

COLEMAN, S., Les Houches 1981 Session 37

Gauge Theories in H.E. Physics, GAILLARD,

M.K. and STORA, R. eds

(North Holland)

1983,

464.

[4]

CHIAO, R.Y. and Wu, Y.S., Phys. Rev. Lett.

57

(1986)

933.

TOMITA, A. and CHIAO, R.Y., Phys. Rev. Lett.

57

(1986)

937.

[5]

COHEN-TANNOUDJI, C. et al., Phys. Rev. Lett.

22

(1969)

758.

[6]

VOLD, T.G. et al., Phys. Rev. Lett. 52

(1984)

2229.

[7]

SUTER, D. et al., University of California pre-

print, Berkeley

1987.

[8] MOODY,

J. et al., Phys. Rev. Lett. 56

(1986)

893.

[9]

AHARONOV, Y. and ANANDAN, J., Phys. Rev.

Lett. 58

(1987)

1593.

[10]

ANANDAN, J. and STObOLSKY, L., Phys. Reu.

D35

(1987)

2597.

[11]

TYCKO, R., Phys. Rev. Lett. 58

(1987)

2281.

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