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HAL Id: jpa-00247527

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Submitted on 1 Jan 1991

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A longitudinal Stern-Gerlach interferometer : the

“beaded” atom

Ch. Miniatura, F. Perales, G. Vassilev, J. Reinhardt, J. Robert, J. Baudon

To cite this version:

Ch. Miniatura, F. Perales, G. Vassilev, J. Reinhardt, J. Robert, et al.. A longitudinal Stern-Gerlach interferometer : the “beaded” atom. Journal de Physique II, EDP Sciences, 1991, 1 (4), pp.425-436.

�10.1051/jp2:1991177�. �jpa-00247527�

(2)

Classification

Physics

Abstracts

32 60 32.90

A longitudinal Stern-Gerlach interferometer

:

the

«

beaded

»

atom

Ch.

Miniatura,

F. Perales

(*),

G.

Vassilev,

J.

Reinhardt,

J Robert and J. Baudon Laboratoire de

Physique

des Lasers

(**),

Universitk Pans-Nord, Avenue J. B. Cldment, 93430 Villetaneuse, France

(Received

I June 1990, revised 21 November 1990,

accepted14

January 1991)

Rksumk.- On donne le pnncipe d'un interfdromdtre atornlque dans lequel est utilisd l'effet Stem-Gerlach

longitudinal

Des rdahsations

possibles

d'un tel mterfdromdtre fonctionnant avec

des atomes mdtastables de gaz rares ou

d'hydrogdne

sont ddcntes Quelques exemples d'objets de

phase

sont discutds, et

quelques applications

sont

suggdrdes

A leur sortie de l'interfdromdtre, les atomes

possddent

des

propndtds

inhabituelles, telles qu'une locahsation

multiple

fi

l'dgard

des variables extemes

(atomes

« en

chapelet »)

Abstract. The

principle

of an atomic interferometer based on the

longitudinal

Stem-Gerlach effect is given Possible realizations using beams of metastable rare gas atoms or metastable

hydrogen

atoms are described Some

examples

of

phase-objects

are discussed and some

possible applications

are

suggested

The atoms

coming

out of the interferometer exhibit uncommon

properties,

particularly

a permanent

multiple

locahsation

regarding

the extemal atomic vanables (« beaded »

atoms)

1. Inwoduction.

In

spite

of the fundamental role

played by

the

phase

in

Quantum Mechanics, only

very few

experiments dealing

with atomic

physics

and atomic collisions have been camed

through

to

study

its properties. It is well known that a

specific

state

la>

of a quantum system is defined

by

a ket

ii

up to an overall

phase

factor :

[a>

=

exp(ia) jai

It means that all states defined

by

the same ket and different

phase

factors must'be

considered as a

single physical

state of the system This axiomatic

property

confers the

peculiar

mathematical structure of fibered space to the Hilbert space of state vectors

ill.

As the overall

phase

factor exp

(i

a

)

is not measurable

~postulate

of the

measure), nothing

can be

(*)

Present address

Department

of

Physics,

New York

University,

New York 10003, U-S-A-

(**)

Laboratoire associd au CNRS URA n° 282.

(3)

said about a. The

only

way to get some information about the

phase

is to prepare the system in a linear

superposition

of several states

(completely

coherent pure

state),

such as

[q2»

= aj

exp(iaj) I)

+

a~exp(ia2) (2)

In this case, if

nothing

can be said about a

j or a~, the

phase

difference

(

a

j a

2)

is, at least

in

pnnciple,

measurable In the atomic case, in order to acltleve the preparation of such a

superposition

and, eventually,

to

modify

and control the

phase difference,

it is

obviously

necessary to prepare, and

eventually modify

a pure atomic state further To describe these

operations properly,

one must consider the

complete

atomic state, i.e., at the same time, the internal state,

depending

on internal

variables,

and the extemal state

depending

on external

vanables,

e.g, those variables

descnbing

the motion of the atomic center of mass, in a fixed frame For sake of

simplicity,

let us consider the case in which the

(free)

external state has been

prepared

as a

plane

wave

(ideally

monokJnetic

beam).

In such

conditions,

the initial atomic state can be written as :

[a»

=

exp(ia) exp(IKZ) jai

where Z is a fixed axis, K the atomic

wavenumber, jai

a

specific

internal state and a an overall unknown

phase.

As K has the same value and as the internal state

a)

is the same for all the atoms, the

complete

states of the different atoms are all described

by

the previous

expression in which the

phase

a is

randomly

distributed.

Any evolution,

induced for instance

by imposed

extemal

fields,

will

generally

concern both internal and extemal states. An

enlightening example Qf

such an evolution is given

by

the famous Stern-Gerlach

expenment.

In this

experiment,

internal states

corresponding

to different values of jy

(component

of the intemal

angular

momentum on axis Y

perpendicular

to

2~

are

spatially separated

from each other

by

a

magnetic

field

gradient

VB

parallel

to Y. In the

original

version of the

expenment,

the atomic beam is not

polarized,

the coherence is zero and there is no definite

phase relationship

between internal states In such

conditions,

the

experiment

is

usually

described

by

saying that some of the atoms are deflected in one

direction,

the other ones m the other direction. On the contrary, if the beam is

polarized,

i-e-

if all atoms are in the

sami

internal state, which

is a linear

superpos1tlon

of eigenstates of j y, then for one given atom there exJsts definite

phase

differences between the

components

of the intemal state

(total coherence).

As a consequence, the

spatial separation

induced

by

VB

now concerns each atoms

ind1vldually

: ifj

y is

double-valued,

the extemal state will consist of two waves,

travelling along

axJs Yin opposite directions. It should be

possible,

in

pnnciple, by

using a convement

magnetic

field

configuration,

with

opposite gradients,

to recover an atomic state s1mllar to the in1tlal one, except that different

phase-shifts

are now added to the different internal state components As far as we

know,

such an

expenmental

device has not been set up so far. It would constitute a realization of an atomic interferometer and

Schwinger

et al.

[2],

who

analyzed

it

theoretically

in great

detail, clearly

demonstrated its

feasibility.

From a

practical

point of view

however,

great difficu1tles are

expected

if a transverse magnetic field

gradient

is

used, especially

concerning the « recombination » of the

sphtted

atoms into a

single

beam. Another

configuration, suggested

and

bnefly

discussed in reference

[2],

consists of a

longitudinal gradient)

i,e, a

gradient parallel

to the direction Z of the atomic beam Phase

shift

effects,

and

correlatively

the

spatial

separation, now occur

solely along

the axis Z As a consequence, the initial

plane

wave remains a

plane

wave

along

the whole device. As it will be

seen

further,

the recombination becomes much

easier,

even in a realistic

expenment

in which neither VB nor the atomic

velocity

are

strictly parallel

to Z.

The mm of the

present

paper is to

suggest

an atomic

interferometry

method based upon the

longitudinal

Stern-Gerlach

effect,

to examine its

feasability

and to

investigate

some of its

(4)

fundamental consequences. In part

2,

the

pnnciple

of the

suggested expenment

is

detailed,

and

possible

realizations

using

beams of rare gas or

hydrogen

metastable atoms are discussed.

In

part 3,

two

particularly important examples

of

phase

effects are described :

(i) topological Berry's phases [3]

which can be used as a test,

(it)

the

phase-shift

induced

by

a

phase- object

», consisting of a

simple profile

of magnetic field the

gradient

of wltlch is

longitudJnal

Some

possible applications

of the method are

suggested.

Part IV is devoted to a

study

of the atoms coming out of the interferometer the

complete

coherence exJsting witltln their internal state also appears wltltln their external state as a kind of « delocahzation »

2. The

longitudinal

Stern-Gerlach interferometer.

2 PRINCIPLE. The

pnnciple

of a

longitudinal

Stem-Gerlach interferometer is based on

the Zeeman state

preparation

of the atoms, I-e- on the

polarization

of the atomic beam.

From this point of view, it is

quite

s1mllar to that of interferences obtained when a

crystal plate,

cut

parallel

to the

optical axis,

is traversed

by

a

parallel light beam,

the

polarization

of which is tilted with respect to the two

polarization eigenvectors

of the

plate.

Within the

plate,

the two

components

of the

polarization

accumulate different

phases,

but no interference

effects can be

directly

seen in a

detector,

since the two beams have

orthogonal polarizations.

However,

after a

polarizer

tilted

with,respect

to the

plate

eigenvectors, the

resulting amplitude

is a linear

superposition

of the two

amplitudes

coming out of the

plate,

and the

interference effects become observable.

The

pnnciple

of the

suggested

expenment is shown in

figure

I

together

with its

optical

counterpart. A

non-polarized

beam of atoms, of internal

angular

momentum

(«spin»)

j # 0 =

I in

Fig. I)

is first

passed through

a

polarizer

P which selects one Zeeman state

~,mo).

Then a «mixer» or

spin-flipper M,

descnbed

below, produces

a coherent

superposition

of Zeeman states. This atomic

(intemal)

state enters an interaction zone in

which each Zeeman

component

accumulates its own

phase

In this region, it is assumed that the extemal fields do not cause any transfer of momenta to the extemal atomic motion

(except longitudinally)

Then a second

spin-flipper

M' builds a new coherent

superposition

in

which the

amplitudes

are linear combinations of the

amplitudes

conning out of the interaction

zone. An

analyzer

A selects one Zeeman state, and the final

intensity

is measured in a

detector D.

atoms

P M M' A D

unpolarized ,

~ ,

~~~~'

P A D

') n~,n~ ~

=. .

light i ,,

interaction

' zone

Fig. I -Scheme of the Stem-Gerlach interferometer

(upper part)

P is a

polarizer,

M and

M'are

spin-flippers

A is an

analyzer

and D a detector The lower part of the

figure

shows the

optical

counterpart, m which the interaction zone consists of a

birefnngent

medium (optical index n,_~

correspond

to polarization eigenvectors 1, 2).

(5)

For several

expenmental

reasons, metastable atoms of rare gases

(He*(~Sj), Ne*(~P~), )

and

hydrogen (H

*

(2sj

j~, F

= I

) )

are

good

candidates for this

expenment

:

(i)

their spin is non-zero and -their

hyperfine

structure is

generally much simpler

than that of alkali atoms,

(ii) they

are

easily produced,

and detected with a

high efficiency (10-30 9b), (iii) they

can be ekcited to upper radiative levels

by

standard low power

(10-20mW) CW-dye

lasers.

2.2 POLARIzERS In

pnnciple,

any transverse

gradient

of

magnetic

field

(Stern-Gerlach expenment, hexapole

magnet,

...)

is able to

polarize

the atomic beam.

However,

there exists other efficient methods which are more convenient to handle.

(i) By

means of a

circularly («* polarized laser,

tuned on a transition from the metastable level to a radiative level allowed to cascade down to the

groundstate,

it is

possible

to prepare

the metastable atoms in a pure Zeeman state mo = ±j. For

instance,

in the case of

Ne*(~P~),

a total

polarization (mo

= ±

2)

has been achieved

by using

the

~P~-~D~

transition

(A

=

614.3 nm wlth'a laser power of about 15-20

mW,

the

intensity

of the

polarized

atomic beam

being

about 50 9b of the initial

Ne*(~P~) intensity [4].

The same method can be used with

H*(2sjj~) htoms,

with a

CW-dye

laser locked in

frequency

on the Balrhefa line

(A

= 556.3 nm

)

(ii)

In the

specific

case of

hydrogen,

a

partial polarization

is achieved

by passing

the atomic beam

through

a

magnetic

fidld B of about 600 G

(Lamb

and Retherford's method

[5])

:

hyperfine

Zeeman levels

2sjj~,

F =

I, M~

= I and

2sjj~

F =

0, M~

= 0 are

degenerated

with the radiative levels

2pjj~,

F =

I, M~

= 0 and

2Pjj~,

F =

I, M~

=

I,

at B

= 530 G and

597 G

respectively.

The

coupling

induced

by

the

motionjl qlectric

field

E~

= v x B

(v

is the

atomic

velocity)

results into a

complete quenching

of both previous

2sjj~ Zeemai

states. As

a

consequence, an'incoherent mlxtilre of

hyperfine

states

2sjj~,

F =

I, M~'= 1,0

is obtained The

only disadvantage

of such a

partial polarization

is a loss of contrast in the interference

pattem observed on the

M~

= -I

component.

2 3 SPIN-FLIPPERS. The

problem

is now to prepare a linear

superposition

of Zeeman

states. If the first method

(i)

of 2.2 is used to

polarize

the beam into mo

= ±

j,

it is rather easy to

modify

it in order to

get

certain linear combination of

[j,m)

states: if the

«* laser excitation takes

place

within a

sufficiently

low

magnetic

field b non collinear to the laser beam so that the induced Zeeman

splitting

is

negligibly

small with respect to the laser line

width,

and the Larmor

penod

is

large compared

to the

time-of-flight through

the laser

beam,

then a definite

superposition

of

[j,m)

~states referred to axJs b is

prepared.

This combination can be modified in a controlled way

by changing

the

angle

between b and the laser beam.

A more

general

method has been used some years ago in neutron

[6]

and atom expenments

[7].

The basic idea is to

produce

a non-adiabatic evolution of the spin,

by sending

the atoms

through

a

special configuration

of magnetic field B : two

oppositely

wound solenoids

produce

a

B~ component

which reverses its sign

abruptly

in the middle of the device. As the beam direction is

parallel

but not identical to the solenoid

axis,

the atoms see a transverse

component B~

which has a

Gaussian-type profile.

Since the necessary fields are small

(B

few 10 mG

),

the

system

needs to be

carefully

shielded. For a

typical length

of few cm, the

dynamical phases

accumulated

by

each Zeeman state

along

its

path through

the spin-

flipper

are

negl1glbly

small

(~10~~ rd).

This means that the extemal atomic vanables are

almost unaffected. For an incoming atomic state exp

(iKZ)

j,

mo),

the

spin-flipper produces

the

outgoing

state :

exp

(iKZ) £ a~~~

j, m

)

m

(6)

The coefficients

a~~~

are controlled

by

the current i in the solenoids. As mentioned in

[7],

one of the difficulties is to ensure that the coefficients

a~~

~ are almost identical for all atoms in the beam It is a matter of

collimation,

the

key parameter being

the ratio

d/L,

where d is the beam

diameter,

L the

length

of the system. Such a device has been constructed and tested on

H*(2s) [8]

in an

expenment

similar to that of

Hight

et al

[7].

In our expenment, the Lamb-

Retherford method has been used to

polarize

the

incoming

beam and to

analyze

the

outgoing

one The

outcomlng H*(2s)

flux has been measured as a function of I, for

given

atomic velocities selected

by

the

time-of-flight technique (Fig. 2).

It is worthwhile

noticing that, actually,

such a

complex

device is not needed to

produce

a

superposition

of Zeeman states. It has been verified

that, by simply

passing the atoms

through

a short zero field

chamber,

such a

superposition

was

produced [8] However,

in this case, no control

parameter,

except the atomic

velocity,

is available.

N(AAB.

U

~

. o

D

. .

o .

. ~

~ , a

2 lo ~

° ~

i

A D

@o oo -

o o

~ 6

' °

~ j o

a a ,

o 1.5 ; ~

Fig 2

current i the spin-flipper The selected

atomic velocity is . (D)

v =10km/s, (.) v

z~

v 4 3

km/s,

(o) v =

5.8

km/s

3.

Experimental

tests.

3 TOPOLOGICAL PHASES.

Topological phases (also

known as

Berry's phases) developed

by

a

quantum

system

govemed by

an Hamlltonian

depending

on at least two

parameters

which

undergoes

a

cyclic

adiabatic

evolution,

have been

widely theoretically

studied

[3].

(7)

Experimental

measurements of such

phases

have

already

been

performed

on

photons [9],

neutrons

[10]

and nuclei

[I Ii.

This

type

of measurements is a

good

test for an atomic

interferometer insofar as :

(i) topological phases

are

predictable, (ii)

the measurements

imply

an ehmmatlon of the

dynaqJical part

of the

phase,

I e. that

part

coming from Zeeman

splittings

inside the interaction zone. Let us consider two

possible types

of interaction :

(i)

A conical magnetic field B

= B

(Z) Q(Z),

where

Q(Z)

is an unit vector

descnbmg

a

cone : ..

This is the

typical configuration

used in neutron expenments

[10].

In this case, the

topological phase

is

simply ma,

where D is the solid

angle

sustained

by

the cone

[12]

(ii)

A

loop skirting

round a conical intersection

point

:

Magnetic

B and electric E fields are two

parameters

in the Zeeman-Stark Hamiltonian. In the case of

H*(n=2),

the adiabatic energy

surfaces, corresponding

to

2sjj~,

F =

I, M~

=

I and

2pij

F

=

I, M~

= 0 levels at zero

fields,

exhibit a conical intersection

point

I at B

= 597 G and E

=

0

(Fig. 3)

The field

profiles

B

(Z)

and

E(Z)

can be chosen so that the atom

representative

point follows a closed

path

e in the B-E

plane.

If point I lies inside

e,

then the

predicted geometncal phase

is w, otherwise it is zero

[12]. Actually

these

predictions

can be made

only

for stable states. In the present case

however,

the

2pj/~

state has a short radiative

lifetime,

i-e- a width r

large compared

to the Stark

splitting

and of the same order of

magnitude

as the

2s-2p splitting.

It has been shown

recently [13]

that m such a case, for

special cycles,

the

Berry phase

can take an intermediate value

n/2 together

with an

exchange

of the

internal states.

2s~,F-i,m~--1

2p~

,

Fai,

m~_o

/2

,

/~ Cl

B

c~

E

Fig

3 -1 conical intersection point.

Cycle Cj (full line)

gives rise to a Berry's

phase equal

to w

whereas

cycle

C~

(broken line)

gives nse to a

Berry's phase equal

to 0

3 2 A SIMPLE PHASE-OBJECT Let us consider a magnetic field

profile

such as

(i)

the

gradient

VB is collinear to axis

Z,

I-e to the atomic

velocity (for

an ideal

atomic,beam coinciding

with axis

Z~, (it)

B=0 on both sides of the

profile,

i-e- for Z<0 and

Z>L. The tridimensional extemal motion of an atom of

spin j =1/2

m such a field is described

by

two equations which are

decoupled

m the adiabatic

approximation

:

T~

+ e~

(z) F~ (z)

=

EF~ (z)

TR is the kinetic energy of the extemal

motion, F=

are the

amplitudes corresponding

to the two intemal states w=

(for

which m

=

±1/2 respectively),

e=

(Z)

= ±

e(Z)

are the local

(8)

Zeeman energies in

B(Z).

It is seen that the local internal energies

play

the role of

potentials

for the extemal motion.

Owing

to the

separation

of variables

X,

Y,

Z,

the solutions take the form :

F~

= exp

ii (Kx

x +

Ky

Y~

f~ (z) f=

are solutions of the equation

1-)$+

E(Z)) f=

=

(E-)(K]+K()) f=

where M is the atomic mass. As

e(Z)

is a very

slowly

varying function at the atomic-

wavelength scale,

the JWKB approximation is

largely justified

The local wavenumbers are defined as :

K_ (Z)

=

[Kj± U(Z)]

~/~ where U

(Z)

=

~

) e(Z)

h

fi2 K~ is such that E

=

(Kj

+

K)

+

Kj)

2M

It is

readily

verified that the JIVKB solutions which behave as

exp(IK~Z)

for Z < 0 are given

by

;

f

z

f_ (Z)

=

0 exp I K_

(Z')

dZ'

K=

o

For Z >

L, they

become

z

f_ (Z)

= exp i

K= (Z') dZ')

o

As the Zeeman energy

splitting

is small

compared

to E

(typically e=10~~eV

for

B

=

200

G,

E

= 0. I

ev~,

the

approximation

K_=K~(1± 2K~ ~~)

is

justified

In such

conditions,

for Z

>

L,

one has

f=(Z)=exp[iK~(Z±@ )j

with

L L

AZ

=

Kj

~

U(Z)

dZ

=

Mg»~ Kj

~

B(Z)

dZ

o o

where g is the Landk factor and »~ is the Bohr magneton. As an

example,

for a

magnetic

field of 200G over L=

lsmm,

and a kJnetic energy

(along Z~

of

0.lev,

one

gets:

AZ = 800

A.

The solutions

F_ finally

consist of two

plane

waves, shifted

by

AZ with

respect

to each other :

F=(Z>L) =exp(iK. (R± @Q~) ).

(9)

As a consequence, to an

incoming (Z

<

0) complete

state :

[a~ [w~)

+a_

[w_)]exp(iK.R) corresponds

the

outgoing (Z >L)

state

a~ w~

)

exp iK R ~~

Q~ + a w exp iK

(R

+ ~~ Q~

2 2

This

analysis

can be

generalized

to any

type

of extemal motion For

example,

let us

consider an almost monochromatic

wavepacket,

the

spectral density

of

which,

p

(K),

is

sharply peaked

at a value

Ko

=

Ko

Q~ If the internal state is w_

),

the JIVKB solutions are :

F_

=

d~K

p

(K)

exp

Ii K~

X +

K~

Y +

j~ K_ (Z') dZ'j

~ t

R3 o h

By expanding

the

phase

term up to the first order m w

= K K

o, one gets.

1.

.z

E~

F=

= exp i

Ko~

X +

Ko

~

Y +

K(

dZ'

~

t x

0

x

d~w

p ~lLo + w

)

exp

iw V~ K~

X +

K~

Y +

j~

K_ dZ' ~ t

R~ o h

Ko

~ ~ ~~

h~

K(

~~~~~

~* ~~°

~ ~

~~~~~

~~~

2 M ForZ<0:

F=

=exP

i(Ko.R-~tj Eo dWP~Ko+W)exPliw. (R-vat)j

R~

The first

exponential

factor is the carder-wave whereas the

integral

over w is the

slowly

varying

envelop

of the

packet,

which is a function

L(R

v

o

t)

where vo =

AK

o/M

is the group

velocity.

It is

readily

verified that for Z

> L the

wavepacket

becomes :

AZO Eo AZO

F_ =exp(i(Ko. (R±jQ~) --tj) xL(R±-Q~-vat)

h 2

where

AZO

is the value of

AZ,

defined

before,

for

K~

=

Ko.

As a consequence, to the

incoming complete

state :

ia+lw+) +a-lw-)iexp

I

Ko.R- ~°t) .L(R-vat)

corresponds

the

outgoing

one :

[P~ a~[w~)

+P a

[w )],exp

i

Ko.R-~°t

h

~

where :

AZO AZO

~*

~~~ ~

~~°

2 ~

~~

~ 2 ~~ ~°

(10)

Therefore,

as far as its extemal motion is

concemed,

the atom appears

sphtted

into two coherent

parts, corresponding respectively

to the

orthogonal

mtemal states w~

).

This is a standard result of a

longitudinal

Stern-Gerlach

experiment operating

with

polarized

atoms More

generally,

if the total atomic momentum is

j,

then

(2

j + I

wavepackets

are obtained

for the extemal

motion,

each of them

corresponding

to one of the

(2j +1) mutually

orthogonal

internal states

[j,

m

).

The major interest of such a

longitudinal

Stern-Gerlach

expenment

is that the

spatial separation

induced

by

the

magnetic gradient

remains

finite,

whereas in a transversal Stern-Gerlach

expenment

this

separation

becomes

asymptotically

a

linearly

increasing function of Z.

Obviously,

the

previous

calculation has been canned out in

an idealized situation, since a

strictly longitudinal gradient

has been assumed. Cumbersome effects induced in the extemal motion

by

transfers of transversal momenta will be examined m the next

paragraph.

3.3 APPLICATIONS. Since the interaction between

polarized

atoms A

(spin j)

and

sphencally symmetric

atoms B is

anisotropic,

the « elastic » scattenng is

actually

descnbed

by

a set of Zeeman transition

amplitudes f~~~(#),

where

[j, mo)

is the initial Zeeman state,

[j,

m

)

the final one and

fi

the

scattering

direction.

Anisotropy (or

«

polarization »)

effects have been

already

observed m collisions between oriented excited alkali atoms and

heavy

rare

gas atoms

[14],

or m collisions between oriented metastable Neon atoms

Ne*(~P~,

m

= ± 2

and rare gas atoms or molecules

[15].

In these expenments, the difference A of the differential

cross sections

corresponding

to

opposite

initial onentations

(mo=±3/2

for

alkalis,

mo= ±2 for

Ne*)

is measured. In absence of fine structure transitions

(eg.

m the

Ne*-Ne

collision)

one has :

A

=

£ ((f+2,m(Jl)(~ (f-2,m(#)(~)

Using

a laser-induced fluorescence

detector,

operating within a

magnetic

field of few

10~G,

it is

possible

to

improve

our information

by individually measuring

the

squared amplitudes [f=~,~[~.

Further

information,

about the relative

phases

between these

amplitudes

can be obtained

by

using the interference method

by inserting

a

spin-flipper

between the collision volume and the

detector,

one is able to transform the

onginal outcoming

state

£ fmom (k) lj,

m ~

i

m

into the new

superposition

of Zeeman states :

£

A

,

f~ ~(fi)[j, m')

~

o

j/

m,m'

Then, by

measunng Zeeman states

populations

1_

2

£A~,f~~~(R)

m

one gets interference terms such as

(f~~~, ft~~~+c,c.) containing

the relative

phase

between the two

amplitudes.

Another type of

possible application

deals with the

phase-imaging,

m a bulk or at a surface The basic

pnnciple

is s1mllar to that of the

phase-imaging

of an

accidentally birefnngent

medium

(e,g,

a

mechanically

constrained

isotropic medium)

using a wide

light

beam. In the

(11)

present

case,

by

use of a wide atomic

beam, together

with a

position-sensitive detector,

it would be

possible

to

get

a two-dimensional picture of the

phase

accumulated

along

each

trajectory,

either in a bulk

(magnetic agreggates),

or after a reflection on a

surface,

even if the

interaction

responsible

for the

phase

shifts is so small that no

significant

effect is observable

on the atomic trajectories

Experiments

of this kind have

already

been realized with electrons

(e.g.

impinging on a

ferro-magnetic surface) [16]. Owing

to the shortness of the atomic

wavelength,

a

high

sensitivity is

expected

In

addition,

the use of beaded atoms

(described

m

part 4)

is

expected

to

provide original

information about

crystal

surfaces.

4. Beaded atoms.

4.I PREPARATION. As mentioned m

3.2,

within the

interferometer, just

after a

phase-

object

consisting of a

longitudinal

magnetic field

gradient,

the

complete

atomic state

~

=

l/2

for sake of

simplicity)

has the

general

form

(apart

a common

phase factor)

a+

iw+ P+

+ a~

iw-

P~

Therefore the atomic state consists of two

wavepackets depending

on the extemal vanables R, shifted

by AZ,

each of them

being

associated to one of the two

orthogonal

internal states

w_ Now if

such

a state is sent

through

the second

spin-flipper

charactenzed

by (almost)

real coefficients «~

~

(i,

j

= ±

)

it becomes :

~(+ ) lW+

+

~(~ lW- )

where :

£(+ )

# a,

~ ~~ P

~ + a~ ~_ P_

Hence,

for each internal state

[w~),

the extemal motion is described

by

a double

wavepacket,

with the

spatial separation

AZ. As a consequence, at the

output

of the

interferometer,

i-e- after the

analyzer,

one

gets

beaded atoms, for which each mtemal

state is combined with a double

(or

more

generally

a

(2

j + I

)-fold) wavepacket,

charac-

terized

by

the interval AZ

along

the atomic

velocity Obviously,

m a real

experiment,

because of the field

configuration

itself and because of the

angular

aperture of the atomic

beam,

VB

cannot be considered as

stnctly longitudinal.

Then the different components of the atomic

state will

undergo

different transversal momentum transfers. This results into a

angular

separation of the

wavepackets,

I-e-

finally

into an «

explosion

of the beaded atom.

Actually

one has to answer the

following question

how

long

m time or m distance is a beaded atom

observable? In other

words,

how

long

does the transversal

separation by

remain small

enough compared

to the

longitudinal

one AZ? Let p be the

order'of magnitude

of

d~

Bid

y B and 3t a reasonable value of

AZ/A

Y. It is

easily

shown that the observation

length L,

within which

AZ/A

Y m

3t,

is

given by

L

=

fp /3t,

where

f

is the width of the

magnetic

field

profile

m the

phase-object. Finally,

this shows that the condition to be

imposed

to the

gradient

m order to

get

a value of L

comparable

to that of

f (few cm)

is not drastic.

4 2 DETECTION OF BEADED ATOMS In order to detect the beaded atoms

produced by

the

longitudinal

Stern-Gerlach

interferometer,

it is necessary to induce a transition from the intemal metastable level to an internal radiative level. This can be

easily

achieved

by

means of

a laser

optical

excitation

(e,g,

for rare gas metastable

atoms)

or

by

a static extemal field

(like

m the Lamb and Retherford's method used for metastable

hydrogen

atoms

[5]).

In the

following,

we will focus our attention on this latter case as an

example.

The external static

magnetic

field gives nse to a motional electric field m the reference frame of the atom which induces a transition from the

2si/2, 1/2 )

state to the

2pim

+

1/2 )

state

(m

a fine structure

(12)

description).

This transition is followed

by

the radiative

decay

of the

[2pj/~

+

l/2)

state

resulting

m the emission of a

Lyman

«

photon. Therefore, by detecting

the emitted

photon,

one measures the

population

of the

)2sjj-1/2)

state. In other

words,

the detected

fluorescence

signal

3 is

proportional

to

[[£_

[[~ =

d~R £~_ ~(R),

i e..

3 cc

d~K30(K)jl

+ C

(K )cos 1l~~K)j

with :

=

«'-+

a+

, » = « a-,

Jo(K)

=

jp(K)j2 jjA

j2 +

j2j

~~~~

"

IA12+ 1»12

In this

expression,

the atomic

phase 1l'(K)

stands for :

'l'(K)

"

i'~K)

+

~fiat(K)

Mg»~ IL B(Z')

dZ'

where, w(K)

=

Arg (» IA )

and

~fi~~(K)

=

Kz AZ(K)

=

° Note that w

Kz

depends

bn K since the

mixing

coefficients of the

spin-flipper depend

on K.

The expression

given

for 3 shows

clearly

that the fluorescence

signal

is the sum of the

various atomic interference pattems

(intensity 30~lL)

and contrast

C(K

associated with the

various atomic wavenumbers

describing

the ingoing

state)

If one

excepts

the slow K-

dependence

of the contrast, one has here the

equivalent

of the interference pattern obtained

m an

optical

interferometer using a non-monochromatic

light

source. As it is well known m

such a case,

only

few

fringes

around the

bnght

central

fnnge

are observable. It will be the

same for the atomic interference

pattern provided AZ(K )

is of the order of

magnitude

of the

atomic

wavelength

Ao

= 2

w/Ko (where Ko

is the wavenumber for which 30~lL

)

is

maximum).

As the

typical

values for

o are of the order of few

Angstrom,

it means that the

magnetic

field

responsible

for the

longitudinal

Stem-Gerlach effect has to be small

(typically

a few

mG).

But it is not a necessary cond1tlon to observe structures in the fluorescence

signal

for indeed it may

exist several wavenumbers K~ for which

[VK1l'(K)]~,

~ 0.

This means that the wavenumbers K~ are stationary

phase points.

In this case, the

fluorescence

signal

exhibits slow variations around these points, even if

AZ(K)

is

large compared

to

Ao. Unfortunately,

the

problem

of the existence of such

stationary phase

points

is rather difficult to solve because it

depends

on the kind of

spin-flipper

one uses and because it relies on the exact

knowledge

of the

expression

of the

phase

of the

mixing

coefficients 5. Conclusion.

The

interferometry

method described m this paper is

actually

a new

development

of ancient basic

ideas, onginated

at the very

beginning

of quantum

physics by Stern, Gerlach, Rabi, Schwmger

and others and

mainly developed

m neutron expenments. The central

problem

here is the atomic

phase,

and the

only

purpose of all devices descnbed m this paper is to

measure and to

study

the charactenstics of this

phase

m vanous situations

fjoq_

the

viewpoint

of the

phase,

these

problems

are

very

close to those encountered m

optics.

This

analogy explains

the

necessity

of using

well-collimated,

and

polanzed

atomic beams In such

conditions,

it is

obviously

an

advantage

to preserve

(as

far as

possible)

the

longitudinal

(13)

geometry

of the

beam,

all

along

the interferometer. The easiest way to fulfill this condition is to use a

longitudinal

Stem-Gerlach

configuration.

Since the atomic

wavelength

is very short

(sac),

at least at thermal energy

(few 10~~eV),

the

phases developed through

usual

magnetic

fields

(0,I-few l0~tJauss)

are

generally

very

large. Nevertheless,

small

phases,

of the order of w, are sufficient to

change

the interference

pattem significantly

Such small

phases

are

accompanied by negligibly

small

(on

a

macroscopic scale)

effects on the extemal motion.

Therefore,

the atomic

mterferometry

can be

applied

to the

analysis

of small

perturbations,

which would be

completely

invisible on

atomic

trajectories.

One of the most

promising

consequences of the use of a

longitudinal

Stern-Gerlach interferometer is the

production

of « beaded atoms. Further

investigations

of the

properties

of these very

special

species are

certainly needed, particularly

m the

following

directions

(i) Complete

treatment of the interaction with radiation

(spontaneous emission,

laser

fields, squeezed fields, microcavities,

beaded

planetary Rydberg atoms,...).

(ii)

Collisional properties : the standard collisional treatments have to

be'modified

since

the incident wave is now a

(2 j

+ I

)-uple plane

wave this is

expected

to

deeply modify

the effect of resonances, atomic

exchange, itc...

The present

method,

which

simply

needs

polarized

neutral

beams,

can be extended to other species and would be of

great

interest m the case of cold atoms where the atomic

wavelength

can be

Very large.

Acknowledgments.

The authors wish to thank Pr. J.

Bellissard,

Dr. V. Lorent and Dr M.

Ducloy

for

stimulating

discussions. The authors also thank the Referee for his criticisms which have led to a clarified version of

part

4.

References

[Ii

THIRRING W., Course in Mathematlcal

Physics,

Vol. I

(Spnnger-Verlag)

1978 [2] SCHWINGER J, SCULLY M. O, ENGLERT B. G., Z

Phys.

D

2/3 (1988)

135

[3] Geometnc Phases in Physics, Advanced Senes in Mathematical Physics, Vol 5, Eds F Wilczek and A

Schapere

~world

Scientific)

1989

[4] PERALES F., Thdse de l'Un1versitd Pans-Sud

(1990)

[5] LAMB W E Jr and RETHERFORb R. C.,

Phys

Rev 86

(1952)

1014 [6] WEINFURTER H and BADUREK G,

Phys.

Rev. Lett 64

(1990)

1318,

,SCHRODER

ly

and BAUM G, Rev. Sci Insirum 16

(1983)

52

[7J HIGHT R D, ROBISCOE R. T and THORSON W.

R,'Phys

Rev A lS

(1977)

1079,

HIGHT R D. and ROBISCOE R. T,

Phys.

Rev A17

(1978)

561

[8] MINIATURA Ch, Thdse de l'Universitd Pans-Nord (1990) [9] CHIAO R Y and Wu Y S,

Phys.

Rev Lett 57

(1986)

933

TOMITA A and CHIAO R. Y,

Phys.

Rev. Len. 57 (1986) 937'

[10] BITTERS T and DUBBERS D,

Phys

Rev Lett 59

(1987)

251

[1Ii

TYCKO R, Phys. Rev. Lett 58

(1987)

2281.

[12]

BERRY M V, Proc. R Sac Land. A392

(1984)

45

[13]

MINIATURA Ch, SIRE C, BAUDON J and BELUSSARD J,

Europhys

~Lett 13

(1990)

199.

[14] DUREN R and HASSELBRINK E., J Chem

Phys

85

(1986)

1880.

[15] BAUDON J., PERALES F, MINIATURA Ch, ROBERT J, VASSILEV G, REINHARDT J. and

HABERLAND H, Chem.

Phys. Special

Issue Penning

Workshop

14S

(1990)

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TONOMURA A, Rev Mod Phys 59 (1987) 639

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