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Angular correlation measurements in a thermal beam of H* (2s) atoms using a Stern-Gerlach atomic axicon

J. Robert, Ch. Miniatura, S. Nic Chormaic, J. Lawson-Daku, O. Gorceix, F.

Perales, J. Baudon

To cite this version:

J. Robert, Ch. Miniatura, S. Nic Chormaic, J. Lawson-Daku, O. Gorceix, et al.. Angular correlation

measurements in a thermal beam of H* (2s) atoms using a Stern-Gerlach atomic axicon. Journal de

Physique II, EDP Sciences, 1994, 4 (11), pp.2061-2071. �10.1051/jp2:1994247�. �jpa-00248109�

(2)

Cla,,iiication Pfiv.~« ; Al?~iiii.>,

12,61) 07.60L 03,65

Angular correlation measurements in

a

thermal beam of

H* (2s) atoms using

a

Stern-Gerlach atomic axicon

J. Robert

('),

ch. Miniatura

('),

S. Nic Chormaic

(2),

J. Lawson-Daku

(')~

O, Gorceix

').

F. Perales

('

and J. Baudon '

l'l Laboratoire de Phy,ique de, LJ,er,(~l. Univer,itd Pari~-Nord. Avenue J-B- Cldnient.

9343(1 Villetaneu,e. France

(2) Penuanent addre,, Dept of Experimental Phy,ic~. St Patrick', College. Maynooth. Ireland

(Ret <>11-«<' 6 Mai /994, Jai-J,e</ 7 Septemb<>1 /994, at apt<><' 9 .ieptem/><>1 /994)

Rdsumd. L'effet de gradient, magndtique, tran~ver,e, en interfdromdtrie atomique de type

Stern-Gerlach e,t de faire interfdrer de, onde~ plane, ayant initialeiuent de, vecteur, d'onde diffdrant par leurs directions. II en rdsulte que, dans le signal d'interfdrence~ induit par le

gradient

longitudinal, le contra,te e~t attdnud par une fonction d'autocorr61ation angulaire. Cet eflet e~t dtudid expdnmentalement,ur un jet thermique d'atome~ mdta~table, H (?, ), don, le ca~ d'un gradient tran,ver,e radial (« axicon,> atomique).

Abstract. The effect of tran,ver~e magnetic

gradient~

in Stern-Gerlach atom interferometry i, to make interfere plane ~ave, the momenta of which differ in their direction~ A, a re~ult the contra,t of the interference pattern

produced

by the

longitudinal gradient

i, attenuated by an angular auto-

correlation function in the momentum ,pace. Thi, effect i,,tudied experimeiitally on a thermal beam of meta~table H I (2,) atom,, with a radml tran,ver,e

gradient

(atomic « axicon »).

1. Introduction.

An atomic beam emitted

by

any kind of hource (an oven for alkali atom;, an electron

boinbardtnent

region

for ineta;table atomh, etc. j, can be characterized if one con~iders the

external motion

by

a

den;ity

matrix in momentum ,pace, or

equivalently by

a ;tati~tical

ensemble of

wavepackels~

or

by

a

« minimal

»

wavepacket

in the sense

given by

Gabor ]. In order to

investigate experimentally

the

angular

coherence~ in a beam, one need~ a

~ignal

in which

off-diagonal

terms of the

density

matrix, p (k, k'l, with i k i

iik'ii,

are involved.

Obviously,

an atomic interferometer in which incident

plane

waves

having originally

different momenta k, k' are allowed to

finally

interfere in the detected

signal,

i~ a device

adapted

to the measurement of such

quantities.

If two ~uch waves are made to interfere it

nece~~arily implies

that one of them (at least) experiences a transverse momentum tran~fer,

1') A~~ocid au CNRS. URA 282.

(3)

such that both final wavevectors be

equal.

Stern-Gerlach or

polarization

interferomet- ry

[2]

is one of the

Simplest

methods that can be used for this purpo~e. Let us

briefly explain

the

principle

of this type of interferometer

(see Fig,

lj : first the atomic beam is

spin-polarized (polarizer

P), then a linear

superposition

of Zeeman states

M)

i~ built

by

a

Majorana spin- flipper (F)

the atoms then pass

through

a

magnetic

field

region (B)

where each state

M)

accumulates its own

phaseshift

a second

spin-flipper

IF'j builds another

superposition

of Zeeman states, one of these

being finally

filtered

by

an

analyzer (A)

; the

emerging

atomic flux is measured

by

a detector

ID

). In this

device,

Zeeman

energie~

F~

=

Mgp

B

B,

where g is the Landd factor and p

~ the Bohr magneton,

play

the role of

potentials

for the external motion.

If B is

time-independent

the incident atomic wave is

elastically

scattered

by

these

potentials

in

a way

specific

to each M value. When there are transverse

gradient~

of B, momentum transfers k

- k'

= k + 6k with k

=

k', will occur. This is

just

the desired effect and it is the

general

principle

nf the method used here. It is also worthwhile

making

~ome

practical

considerations,

particularly concerning

the orders of

magnitude

of

energies,

momentum transfers and various

sizes

iii

with the low fields used here IS G I the Zeeman

energies

l~ nev are very small

compared

to the kinetic energy 11 0.5eV in the present

experiment using

metastable

hydrogen

atoms) ; deflection

angles

induced

by

transverse

gradients

are also

quite

small

(6k/k

5

10~~

rd)

iii)

the de

Broglie wavelength

is very small at the

macroscopic

scale of the

magnetic

field

profile

(here A

=

0.41

whereas B is

varying

at

a mm

scale) (iit)

it is assumed that the

diaphragms provide

a

good

collimation of the beam (the

angular

aperture is less than 2°

FWHM)

this allows us to use a

paraxial approximation,

H2

~

p

A

o

Fig. I. Experimental ~etup : electron gun G, polarizer P and analyzer A, spin-flipper~ F. F', magnetic

~hielding M, detector D B I, the region where the variou, magnetic gradient, acting on the external

motion of H ~ atom~ are pre,ent.

2. General form of the

signal.

Suppose

that a

wavepacket (produced by

the source and all

diaphragms preceeding

the interferometer itself) is incident on the interferometer

*,1)

= dK

i,

C iK<,

K<,)

(1)

where

K,,)

is a

plane

wave of momentum

K,,.

Becau~e of the presence of

diaphragms

within

the

interferometer,

this

wavepacket

is not allowed to reach the detector, even if this is very

wide. If no

magnetic

field is

applied

then the incident wave (I)

produces

an

outgoing

wavepacket

V/,,~) =

dK,,

dk C

(Kj,

D

(K,,,

k

k)

12)

(4)

where the D-s are characteristic of the inner

diaphragms.

In the present ca~e the size of these

diaphragms

is

macroscopic

(~mm) and the Fresnel diffraction at their

edges

can be

completely ignored.

Nevertheless

they

will

play

a

key

role here.

simply

because

they

truncate the wavefronts incident on them. AS the deflection caused

by

the

magnetic

field is

extremely

small, the effect of these

diaphragms

remains the wme in the presence of B.

Consequently

V/,,~)

(multiplied by

the linear combination of M-states

produced by spin-flipper

F) can be

regarded

as the

incoming

state in the collision with the

magnetic potentials,

Conditions

(ii

and

(it) being

fulfilled, the Glauber

approximation

[31 i~

widely justified

in the treatment of the collision itself. In the case of a

plane

wave

k)

incident on the limited range

B-profile,

and for

a

specific

M level

(referred

to

quantization

axi~

fi),

the

phase

at

a

point

r

beyond

the

profile

is

readily

calculated as an

integral along

the rectilinear ray

parallel

to k

passing through

this

point

~P k r + M~ (k, r j (3)

where

gp~

,,rJ

~ (k, r)

=

B d-I.

(41

h~

i,J,

Here v fit/ui where iii i~ the atomic ma;~. .~ i; the absci;ha

along

the ray. Therefore for a

plane

wave

[k) passing through

the entire interferometer (I,e. P. F. B, F'. A), the

outgoing

external motion ha~ the form

jj Au

exp ii (k r + M~ lk. r

,1

where A,w are coefficient~

characterizing

F and F'. Then for the

incoming

~tate

(2),

one gets the

outgoing

state

P,~~,, =

~

AJ~

dK,,

dk C

(K,,

D

(K,,,

k exp ii (k r +

M~

(k, r

))]

(5

u ~

In such conditions, a wide detector (I.e. not

participating

in the beam collimation) measures a

time

independent

flux

proportional

to

~'oUl

=

jj Au

AIi

dK,, dK,(

dk dk' C

(K,,

D

(K,j,

k C ~

(K,[

D *

(K,[,

k' x

,i,,i

x dr exp ii ((k k'j r +

M~

(k, r M' ~ (k', r)

j] (6j

In this very

general

form of the

signal,

it may be

already

noticed that ~ince the

integral~

over r

lead to a set oi functions

f'u,,j.(k, k'),

different wave vector; will be allowed to

participate

in the interference

;ignal.

A SIMPLE EXAMPLE. In order to di~cuh; more

specifically

the role of transver;e

gradients,

let

u; con~ider the case of a unidimensional

gradient

(I,e, the ;tandard Stem-Gerlach

configur-

ation) :

B=(B,,+Gi)I,

for =e

(0,L(

= o elsewhere

(7)

J<JUR~AL DE PHYS'QUE II T 4 N' '' NO'EMBER lL<u4 77

(5)

where k i~

orthogonal

to the axis I of the beam. Thi~

simple

form of B is

actually

an

approximate

one,

only

valid in the

vicinity

of the I axis. If one assumes a k vector

slightly

inclined with respect to

I,

then the

phase

can be

explicitely

calculated irom

equations

13 and (4)

4l=

(k+M6k).r+M~P,, (81

where

This means that the

emerging

wave is a

plane

wave, the momentum of which i~

k + M 6k

(in optics

thi~ would be the effect of a

prism), phaseshifted by M~Po, by

the

longitudinal

Stern-Gerlach effect due to

B,,.

In this

special

case the

signal given by equation (6)

can be

simplified

to

yield

( v'~~~(~ =

jj

AJ~

A(,

du

e'~'~

~'~'~ ~~"~~ r (u M 6k (u

))

r * (u M' 6k (u )) (9)

M,w

where

r ju

=

dK,,

c

(K,,)

D

jK,,,

u

lo)

Here r represents a momentum distribution

combining

that of the wave incident on the interferometer with the collimation effect due to the inner

diaphragms.

It is

clearly

seen in

(9)

that the

longitudinal

Stem-Gerlach interference pattern,

governed by

the

phaseshift

(M M')

4lj,,

will be

damped by

an

an,qulai

auto-c.r~iielatir~n

jiifictir)fi.

In

principle

it is

possible

to

change

either C

(Kj,), by acting

on the source, or (more

easily) D(K,j,

u),

by changing

the inner

diaphragms.

Notice that if a ~tatistical ensemble of

wavepackets

is considered, one has to

replace

rr* in

(9) by

the average

@ (off-diagonal

element of the

density

matrix).

An

expression

of the

outgoing

state

(Eq.

(5)) in the

~pecial

case of a unidimensional

gradient

was

given

a

long

time ago

by

Bloom and Erdman

[4].

The

expression they

obtained for the

signal

is identical to that

given

in

equation

(9), except that interferential crossed terms are

missing simply

because these authors

only

considered the effect of the

magnetic

field and not of an interferometer.

REMARK ABOUT THE CALCULATION usiNG cLAssicAL TRAJECTORIES. Let us consider a

monokinetic beam

consisting

of

independent

atoms, each of them

following

a classical

trajectory (approximately

a

straight line)

at a given

velocity

vi,.

Actually

the external motion is seuii-classical since, for each M, value a

phase

is accumulated

along

the

trajectory.

The

phase

difference

(M

M') ~ can be calculated as before

by

use of the Glauber

approximation.

For

the sake of

~implicity

let us assume that a

single

inner

diaphragm

ID is present. The

signal

takes the form

S

=

jj

AJ~J~. dS exp [I (M M') ~ (l

,i,,i

D

where p

=

4l~

+ 6k.x. One may notice that for Ml M' the

integral

is similar to the

Fraunhofer diffraction

auiplitude

in the direction k'= k+ 6k.

Using

the definition of

(6)

D(Kj,,

k)

(Eq.

(2) and

Eq. (8)),

it is

easily

verified that

e'"~

~'~ '~"

ldu

D

(Kj,,

u M 6k D *

(K,,,

u M' &k j =

=

ids e'~'~

~'~ "~" ~ ~~ ''

=

dS

e'~~

~'~ ~ l

2)

D

D

This means that the

signal given by equation

is identical to that

given by equation (9)

for

an incident

plane

wave of momentum

K,j uivj,/h.

The

physical meaning

of this result is the

following (cf.

the treatment of

impact

parameters in semi-classical

collisions)

the size of the

diaphragm

is so

large

that it can be divided into domains

A,, ~~,

...,

A,,, the sizes of which

are

large compared

to A, but also small

enough

to

give

an almost constant value

~,, of ~ for all the rays

starting

from any

point

in

~,,.

The intensities

corresponding

to all these domains have to be added to get the

signal.

It is then

easily

under~tood that the distribution of initial

phases

among the different domains A,,

plays

no role in the final

intensity, giving

the

same result for an

incoming plane

wave

[K,,)

and for a random distribution of the initial

phases.

This property can be

generalized

to any

configuration

of B and any

configuration

of

inner

diaphragms, provided they

are wide at a A-scale. The fact that in this case a treatment

using quasi-geometrical optics

is valid does not at all invalidate the more

general

result~

derived

previously (e.g. Eqs.

(6) and (9)), which involve

angular

correlation functions in

momentum space.

A CYLINDRICALLY SYMMETRIC GRADIENT. The use of a Cartesian-unidimensional

gradient

is

experimentally

difficult because it cannot be

produced independently

of a uniform field

Bj, which in addition needs to be

sufficiently large (B,,»

G i-vi ). As a consequence the

interference order for the

longitudinal

Stem-Gerlach effect is

necessarily high

(m 6) which

cau~es a severe loss of contrast, even if a

velocity

selection is made, because of unavoidable

instrumental

imperfections

Humpty-Dumpty

» effect

[5().

Most of the

experiments

de-

scribed later use a

magnetic quadrupole.

This consists of two identical and

orthogonal pairs

of

oppositely

wound

rectangular

Helmholtz coils. In the

vicinity

of the I axis the field can be

approximated by

B

= G (- ii +

_vj),

for = e [0. L

= o elsewhere II ~)

Within the interval [0, L], the field lines are

hyperbolae

(i_>. C~t. and the

magnitude

of the field is B

=

Gi~,

where i~ is the distance to the I axis. This lead~ to a radial

gradient

of B. For each M value this

configuration

behaves as a

parallel plate,

the index of which is

proportional

to i~, I-e- an

optical

« axicon

». For an incident

plane

wave

k),

the momentum of which lies

in direction

I(0,

p,

y ) with p « y w I,

equation

(4)

give~

qJ (k, r)1 ~~ ~ G

~'~

dir

.v~

+ »

~

= +

pit j

~'~

'4) fir

,, y

For a

specific

M value, the total

phase

at a

point

r

beyond

the B

region

(= m

L)

is then

~P

=

I.(P-v

+ Y=) +

M~. jis)

A wavevector can be defined at this

point by

K(rj

=

V,4l

k+M 6k(r) (16)

(7)

6k(rj

has the

following

components

&l~

j~~

G

~

(Ar;h )

Ar~h

)

ii P ' '

61,

=

j~~

G

) (,fi ,fi)

'7)

iv

61- ~

fit,

Y

where l'j = v

~

= ><, = i'-

~

IL

=). It may be noticed that k &k

=

0 (elastic collision)

Y Y

and that

61=[

«

61,.

If p

=

0, one get~

&k1 ~~ ~

GLi~

(18)

In other word; the outgoing waveiront (for each M ;tate) i, a cone, the normal oi which make;

an

angle ~~~

GL with I, where E is the kinetic energy. It can be shown that thi~ re~ult E

remains

approximately

true for

p

# 0 but ~mall and in the

vicinity

of the output

plane

= = L, where 6k has an

expre;sion

similar to (18),

i~ being replaced by

another radial unit

vector I

[

centered at the point (.I

=

0. >'= ~

L).

2

In order to calculate the

;ignal

obtained in this case more

explicitely

we can u~e a « coaoe

graining

» method I-e- divide the detector

plane (assumed

to be not too far

beyond

the output

plane

=

=

L) into domain~

(di)

centered at

points

i-I, the ~ize; oi which are at the same time

large compared

to and ~mall

enough

to con;ider that

6k=61i~

is uniiorm over

di.

Then starting irom equation (6) and after ~ome calculations one

finally

gets

i P~,~,,11~ = Cst,

jj

AJ~J~ du r(u ) r ~[u + (M M') 61(ii FL (19)

~iu

an

expre~sion

very ~imilar to (9) (with 4l,>

= 0), except that the direction oi the momentum transier is no

longer

fixed but I; radial. In thi~ case the

longitudinal

Stem-Gerlach interference will be

damped by

a « radial

»

angular

autocorrelation function.

3.

Experiment

and discussion.

The

general principle

of the

experiment

ha; been

already explained

in section I, and a detailed

description

of the technical a,pect; ha~ been given

previously

elsewhere [6].

Only

the main features will be

briefly reported

here. A beam of H~ (?s) atom~ is

produced by

electronic

bombardment or a thermal beam oi

Hi

molecules. The main contribution to the

resulting

normalized time of

flight

distribution is well fitted

by

f'(ii

=

12.5 ii~ ~ exp (- ?.5 ii~ ~

(20)

where ii

=

tit,,,

t,,

being

the mo~t

probable

time of

flight,

which

corresponds

to a

velocity

of 10km/~ (i.e.

A10.41).

The bedim is

partially polarized

in the

hyperfine

~tate;

?sj~~,

F

=

I.

M~

=

0,

by

passage

through

a transverse field

Bp

of 600 G (Lamb and Retherford's

method

[7]j.

The

Majorana spin flipper

F operate~

by

a non-adiabatic passage from the

attenuated

Bp

field to the iield

existing

in the B

region.

In the low fields used here,

(8)

H'~ atoms behave ah

spin particles,

hence the

operation

can be de~cribed

by

a

Wigner

rotation matrix D

(p

=

D~

'(0, p, 0).

In the

following

treatment both

velocity

and field

dependences

oi the Euler

angle p

will be

ignored.

The spin

flipper

F' and the

analyzer

A work in the same

manner a; F and P

respectively. Finally

the radiative

decay

of

emerging

atom~ i~ induced

by

~tatic Stark

quenching

and the

re~ulting Lyman

cv

photons

are detected

through

a

Mgfj

window

by

a channel electron

multiplier.

In

region

B (~ee

Fig.

2) the

magnetic

field is

produced by

a

magnetic quadrupole (ci.

Sect.

?)

in addition to two

parallel

horizontal wires which

produce

a uniform field

B,, j

in the

vicinity

of

the I axis. The total iield can be

approximated by

Bi[-Gii+(B,,+G>.)I(,

ior =e

(0,L(

~ ° el~ewhere

(?

This iield has

properties quite

,imilar to those of a

quadrupole

iield

(Eq.

l~)) except that now

i~ I; centered in the (.i, _i')

plane

on the

point

(0,

Bjj/G).

z

2L

x 2d

x

io io

~i

y z

' 2h

Fig. ?.- The magnetic

contigurition

u;ed

in region B con,i,t~ of two pa>r, of orthogonal anti- Helmholtz coil~

~upplied

with current ii and of a ,traight frame ;upplied with current in (L

=

4? mm,

</=6 mm, h =8 mm). Such a configuration tran,form, a plane ~ave

(K,j)

with internal ,tote

M)

into a conical wave.

In the first ~et of

experiments B,,

i~ scanned ior a fixed value of G

(Fig.

3). Here the inner

diaphragmq

consist of two holes of radiu~ 2 mm

separated by

15 cm. It i~ worthwhile

noticing

that

only

the~e hole; deiine the beam collimation. When G

=

0 one finds the standard

longitudinal

Stern-Gerlach pattern with

only

a few

fringes

visible since the atom~ are not

velocity

~elected. The contrast around the central

bright fringe

is about 30 %. A, G is increased

the overall contrast

continuously

decreases and no more

fringes

are ob~erved once

G ~ ??5 mG/cm.

In the ~econd set of

experiment,

we have studied, with the same set of collimation holes, the attenuation oi the central

fringe (B,j

= 0), oi the first minimum

(B,,

=

3~ mG and of the iir;t lateral maximum

(B,,

=

78 mG ), as a function of G

Fig.

4).

Finally

in the third ~et oi

experiments

the effect of the inner collimation on the central

fringe

attenuation ha~ been

investigated (Fig.

5). When the radius of both hole~ is reduced

by

a factor of ?, it is ~een that, apart from an obvious reduction of the atomic flux, the new pattern is twice

a~ wide as the fir~t one. When the two hole~ are

replaced by

two annular apertures (internal

(9)

a

b

c

d

e

-0.15 0

B~(Gj

0.15

F>g. 3.- Interference pattern; obtained a, a function of Bu, for variou~ fixed value~ of G:

G 0 (a) ; 55 mG/cm (bj ; 110 mG/cm (c) 167 mG/cm (dj 2?0 mG/cm (e). The light line~ are

calculation~.

6

a

i i

iGimGicm))

Fig. 4.- Interference pattern~ obtained as functions of G for variou, fixed value~ of Bu;

B~j 0 mG (a 32 mG (b) 78 mG (c). The light lines are calculation~.

radius 1.5 mm, external radius 2 mm) a

clearly oscillatory

~tructure with a better contrast i~

observed.

Ajj these

experimental

features are in

qualitative

agreement with the theoretical

predictions

oj~ section 2. A

quantitative interpretation

needs a

slightly

more elaborate treatment than that

u,ed in the case of a radial

gradient, firstly,

because the initial

spin polarization

is not

perfect

(10)

a

~

Z

b

c

O.5 0 o.5

G(mG/cm)

Fig. 5. Interference pattern~ obtained a~ function~ of G with two collimation hole~ of diameter

4 mm (a) 2 mm (hi and with two annuli (internal diameter 3 mm, external diameter 4 mm) (c). The

light lines are calculations.

and

secondly,

because a uniform field is added to the

quadrupole

field. Nevertheless the same basic

principles

and

approximations

will be u~ed here in the framework of the vectorial model for a

spin

F

=

I. Let

f

be a column vector the components of which are

v'~,

the extemal

motion a~~ociated with the Zeeman ~tate M

)

referred to the

j

axis. For an incident

plane

wave

of momentum k,

slightly

inclined with re~pect to the I axis, let us ~et

flf

=

exp(il=),

4l j22)

As the elements of ~P are

slowly varying

functions one can

neglect

their second derivative~ (cf.

the Glauber

approximation),

which allows us to determine the evolution operator

connecting

# (,t, I', Z < 0 tO ~fi I, V, Z ~ L)

gp~ La U

= exp i [- G-t-F +

(B,j

+

IF,

123)

hvi>

where

u/v,,

= Iv, v hl./ui. Now

taking

into account the presence of a

single

inner

diaphragm

D of area S

together

with the

partial

initial

polarization

of the beam and the time of

flight

distribution

given

in

equation

(20), one can calculate the normalized

signal

N

=

j

da

f(ui

~~

i-

i o+

(p

uD

(p )j 1)

j2

(24)

D S

Using polar

coordinates p, in the

plane

t., >., with the

origin

at

point (0, Bj,/G

I, one gets

N

=

j~

da

j

(u ~

~~

~~ [a cos (2 cup + b cos (cup + c. (25)

i> D .~

(11)

where :

gv ~ LGU

~

'

cos4

(o

p

. h '

1' ~'~~

~

~~

cv

~~~, 16 ~

t =

-a-b.

The numerical value p =60° is derived from the

experimental

contrast observed when

G

=

0

(Fig. 3a).

The

regular

full lines in

figures

3, 4, 5 repreqent the calculated patterns obtained in the various situations considered here. The agreement with the

experimental

results is

quite satisiactory

even

though

there is a small

discrepancy

for the annulus

(Fig.

5c) in the

matching

of the horizontal scale, which is

probably

due to the

approximate expre~sion

for B

(Eq. (21)) being

less valid in this case.

In order to get a better

physical understanding

of the result (25) and make a connection with the

general

formulation of section 2, let us assume that (I)

Bj,

0 it) the incident beam on

the interferometer is characterized

by

a

diagonal den~ity

matrix

C(K,,)C*(K,(j=

F(K,j) 6(K,[ Kj,),

where F is

strongly peaked

in the I direction. In such conditions in

equation

(19) one has :

rju

r~(u

+

(M

M~ 51(ii

i~

= dK,~ F

(K,,)

o

jK,,,

u o

*(K,,,

u +

jM

M~ j

&ii~

j

Thi~ means that

only

the inner

diaphragm;

are involved here. With a

~ingle diaphragm,

D(K,,,

u m 5)(u) is

simply

the ?D-Fourier transform oi a square function R( t, >')

=

in;ide the

diaphragm,

= 0 outside, I-e- the Fraunhofer difiraction

amplitude

of the

diaphragm.

For a

given

value of K,> the

integral

over u in

equation

(19) can be written

Ida, da,

51(u 51* (u +

(M

M')

61i~

) =

at-

d>'R~(

t,

>. exp

ii

(M M') 6k i~ =

=

dS exp [I (M M') fit i~

v

Finally

the

signal given by equation (19)

takes the

following

form

jj

A,w,,i.

j~ dKjj fi(K,j)

dS exp ii (M M') 61 i~ (26)

jj~t iJ D

where

fi(K,j)

is the

K,,

distribution. Let us now turn to

equation

(25). In the present case p = i~

,

cv =

61. The

integral~

over

only

contain the three coefficients a, b, c. and

give fjnally

three constants

characterizing

the

spin flipper efficiency.

In conclusion~ apart from

some

normalizing

constant, the re;ult

given by equation (25)

is identical to that

given by equation

(191.

4. Conclusion.

We have shown that a Stem-Gerlach atomic interferometer

using time-independent

transverse

gradients

of

magnetic

fields

provides

on a wide detector a

signal

which contains (as attenuation

factors in the contrast oi the

fringes) angular

correlation functions oi the beam in the

momentum space. The~e functions are

generally

determined

by

the atomic source,

by

the

collimating diaphragm~ preceeding

the interferometer a; ~i,ell as

by

the

diaphragm~

present

within the interferometer. The basic proces; here is the elastic transverse momentum transfer

(12)

(M

6k ) induced

by

the transverse

gradient,

which make interfere

plane

waves which have initial momenta

differing

in their directions (but not in

magnitude).

As a consequence there is a strong

similarity

between these attenuation factors and the Fraunhofer diffraction

amplitude

at an

angle

the order of

magnitude

of which is &I/k. In the present conditions this

angle

is

extremely

small

(5 10~~

rd)

: this is the reason

why

the attenuation patterns are so

clearly

visible when

diaphragms

the size of which is very

large compared

to are u~ed. It may be

noticed that in such a situation the

signal

can be calculated as well

by quasi-geometrical optics,

I-e-

by averaging

the

inhomogeneous longitudinal-gradient

induced interference patterns over

all rectilinear

trajectorie~ passing through

the

diaphragms.

In the

experiments reported

here the whole

generality

of the method is

obviously

not

exploited

since the source itself is

highly

incoherent and the beam collimation is

entirely

made

by

the inner

diaphragms.

Nevertheless these

experiments quantitatively

demon;trate the

validity

of the theoretical

predictions

and show the

capability

of the method in

measuring angular

correlations in an atomic beam.

Variou~ further

developments

of this

technique

can be

imagined.

Let us summarize very

briefly

some of them :

(I)

mea~urement of the

signal

received on a detector

having

a small size (at the

macroscopic scale),

the

question

addressed here

being

how is the

signal

distributed in the detection

plane

'? (in

spite

of its

difficulty

the use of a uni-dimen~ional

gradient

would allow the easiest

interpretation

of the results)

(it)

construction of a

(slightly) separated

beam

interferometer,

by

use of four successive

gradients

(+ G, G, G, + G) (iiij effect of a

put.led

transverse

gradient:

in this case the momentum tran~fer is no

longer dispersive (thereiore

an easier

operation

of a

separated

beam interferometer

using

four

gradient pulses

can

be

expected).

Acknowledgments.

The authors wish to thank K. Rubin

(City College,

New

York)

for his enthousiasm in the work.

S-N-C- wishes to thank the Commis~ion of the

European

Communitie~ for the

provision

of a

SCIENCE

bursary (BS/SCI*/915186).

J. L. D. thanks the ALBAR fundation for grant.

References

Ii Gabor D., Re,,. Mod Ph_v.I 28 (1956) 260 ;

The fact that time-independent >nterferometric experiment~ cannot dist>ngui~h between the coherent wavepacket ~tructure and the incoherent m>xture of ~uch packets has been pointed out by Mopurgo G., Awl Ph>'.I (N Y 97 (19761 519 :

~ee also Bernste>n H. J. and Low F. E., Ph_i'i Rei'. Lent. 59 (19871951.

[2] Miniatura Ch., Perale~ F., Vassilev G., Reinhardt J., Robert J. and Baudon J., / Phv.< II Fiaiite 1 (1991) 425 ;

For other atomic

>nterferometry

techniques. ~ee App/ Ph_;I B 54(51 (1992), special i~~ue « Optic~

and Interferometry with Atom~ » and reference; therein.

[3] Glauber R. J., in Lecture~ in Theoretical

Phy~ic~,

vol. I, W. E. Brittin and L. Dunham Ed~.

(Inter~cience Pub(., New York, 1959) p. 135.

[4] Bloom M. and Erdman K., Can ./ Ph_i'.I 40 (1962) 179

See al~o Bloom M., Enga E. and Low H., Can../ Phi'.I. 45 (1967) 1481.

[5]

Englert

B. G., Schwinger J. and Scully M. O., Ffiwi</ Flit-( 18 (1988) 1045 Schwinger J., Scully M. O and Englert B. G., z Ph_;~ D lo (1988) 135.

j6( Robert J., Miniatura Ch., Le Boiieux S.. Reinhardt J.. Bocvar,Li V. and Baudon J., Ew.I>phi I. Lent.

16 (199 II 29.

[7( Lamb W. E. and Retherford R C. Phv~ Rei' 79 (1950) 549.

JOURNAL DE PHhSIOUE H T 4 N II NUVLMBER 1~~4 78

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