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Atomic Fresnel images and possible applications in atom lithography

U. Janicke, M. Wilkens

To cite this version:

U. Janicke, M. Wilkens. Atomic Fresnel images and possible applications in atom lithography. Journal

de Physique II, EDP Sciences, 1994, 4 (11), pp.1975-1980. �10.1051/jp2:1994243�. �jpa-00248099�

(2)

J.

Phys.

II trance 4

(t994)

t975-1980 NOVEMBER1994, PAGE 1975

Classification

Physics

Abstracts

32.90 42.20 42.50

Atomic Fresnel images and possible applications in atom

lithography

U. Janicke and M. Wilkens

Fakultit fur

Physik,

Universitit Konstanz, 78434 Konstanz,

Germany

(Received

24

May1994,

re~ised 6

July 1994, accepted

lo

August 1994)

Abstract. In the near field

regime

of diffractive atom

optics,

amplitude

corrugations

of the de

Broglie

wave front are

important

and can lead to

interesting

effects. One class of

near field

phenomena

is the formation of Fresnel

images.

We

study

this effect and possible

applications

in atom

lithography using

wave

packet

simulations.

Diffraction of atoms most

clearly

demonstrates the ultimate wave character of the atomic center-of-mass

motion, opening

a broad class of

potential applications,

in

particular

in atom in-

terferometry.

Various

diffracting objects

like microfabricated transmittion

gratings

and double

slits, standing

wave

light fields,

and

magneto-optical

fields have been

investigated extensively

both

experimentally

and

theoretically

in the past

[1-6].

In a

typical diffraction experiment

one considers a beam of atoms,

traveling predominantly

in the

z-direction,

which traverses a

diffracting object, aligned

in the

x-direction, (see Fig. I).

Diffraction of the atoms occurs if the transverse coherence

length (in

the

x-direction)

is of the

same order or

larger

than the

spatial period

of the

diffracting object. Assuming

that the kinetic energy in the z-direction of the

incoming

atoms is much

larger

than the interaction energy and that the

diffracting object

is uniform in the

y-direction,

the diffraction is described

by

an

effectively

one-dimensional model of the quantum mechanical motion

along

the x-direction.

Utilizing

a

paraxial approximation,

the

spatial

evolution of the atomic wavefunction

16(x, z) along

the z-direction is described

by

the

Schr6dinger equation

ih~)~bix, z)

=

[ [

+

Uix, z) ~bix, z)

,

ii)

where ~ is the center-of-mass

velocity

of the

incoming

atoms in the

z-direction,

M the mass of the

atoms,

and

U(x, z)

is the interaction operator of the interaction between the atoms and

the

diffracting object.

It is convenient to

distinguish

between a

preparation region along

the

z-direction,

where

U(x, z)

is nonzero, and the

subsequent

free evolution for

z > zo, where

U(x,

z >

zo)

vanishes.

(3)

t976 JOUIINAL DE

PHYSIQUE

II N°11

t

~

~

z~~

~

fl

~

~

~

~

~

~

Fig.

I. The geometry of a

typical

diffraction

experiment.

A beam of atoms moves in the z-direction and traverses a

diffracting object (e.g,

a

standing

wave

light field)

which is

aligned

in the «-direction.

Behind the

diffracting object

one

distinguishes

between a near field

(nf)

and a far field

(ff).

For an

arbitrarily prepared

wavefunction

16(x,zo),

the state at distance z zo downstream is

given by

the Fresnel

integral

16(x, z)

c~

dx'

exp I ~~

(x x'

)~

lb(x',

zo

(2)

/

21t(z

zo

In

analogy

to classical

optics

one

distinguishes

between a far field

(z

zo »

a~ /ldB (Fraun-

hofer

limit, region

denoted

by

"ff' in

Fig. I)

and a near field

(z zo)

m

a~/ldB (Fresnel limit, region

denoted

by

"nf' in

Fig. I).

Here a is the illuminated size of the

diffracting object,

and

ldB

"

h/(M~)

is the atomic de

Broglie wavelength.

The transition from near field to far field behavior is shown in

figure

2 which

depicts

the free evolution of a coherent array of atomic wave

packets. Up

to

date,

most of the

experiments

have been discussed in the Fraunhofer limit z - oo. In this limit the

spatial

atom distribution which is observed far behind the interaction

region

is

essentially given by

the momentum distribution of the atoms after the interaction. The dimension of the diffraction

pattern

scales

linearly

with the distance from the

preparation plane.

In contrast in the near

field,

no

simple scaling

can be observed.

Here, corrugations

of the wave front are

important

and interferences

between different

spatial parts

of the wavefunction lead to a

complicated

evolution of the atomic wavefunction in the z-direction.

To discuss the near field effects which occur in atom diffraction in more

detail,

we turn to the concrete

example

of diffraction of atoms from an off-resonant

standing

wave laser field

(scalar Kapitza-Dirac effect). Figure

3 shows a wave

packet

simulation of this process. An atomic beam of

ground

state two level atoms, modelled

by

a broad Gaussian wave

packet spanning

several

optical

wave

lengths,

moves

through

a

standing

wave laser field with

wavelength I,

located at

z = 0. The width of the wave

packet corresponds

here to the transverse coherence

length

of the atomic beam. The

light

field has a Gaussian

envelope exp(-z~ /w~

and is

sufficiently

detuned from the atomic transition

frequency,

so that the

population

of the excited state

during

the

interaction is

negligible. Figure

3 shows the

intensity

distribution of the

ground

state atoms as a function of x and z. The atoms are focussed

by

the antinodes of the

standing

wave

light

field

[7,

8] which act as an array of thin lenses

(phase grating).

In the focal

plane

of these lenses at z =

f

an array of narrow

peaks

with

period

d

=1/2

is formed

(first

bold line behind the

light

field in

Fig.

3 and thin solid line in

Fig. 4).

(4)

N°11 ATOMIC FRESNEL IMAGES ATOM LITHOGRAPHY 1977

z=0

j

l

@

~

x

Fig.

2. Natural

spreading

of an array of Gaussian wave

packets.

In the near field the formation of Fresnel

images

is visible. The far field reveals the Fourier transform of the initial array, which scales

linearly

with the distance.

The focal

length f

is

approximately given by

~ lt~T ~B

~

~

~~

~

~~~

~~~

Here fl is the Rabi

frequency

of the

light field,

b is the

detuning

of the

light

field from the atomic transition

frequency,

and T

=

@ w/~

is the interaction time

(note

that fl and b are

angular frequencies).

In the

following

it is convenient to use recoil units

fl/wrec

-

fl, b/wr~c

-

b,

Twr~c - T,

ldBk

-

ldB,

where wr~c

=

ltk~/(2m)

is the recoil

frequency.

The

parameters

used in the simulation were fl

=

280,

b

=

-200,

and T

= 0.044. As

T <

(fl)~~/2,

the interaction time is within the Raman-Nath

regime [6].

The focal

spot

size Ax

(left-to-right

minimum

distance)

can be estimated

by Iii

Ax =

21dB~ (4)

This

gives Ax/d

= 0.354 in

good agreement

with the value which can be read off from

figure

4.

The

focussing

of an atomic beam

by

the antinodes of a

standing

wave

light

field is not restricted to the situation in which the

incoming

beam has a

large

transverse coherence

length.

Even a

completely

incoherent

beam,

which in this context may be

regarded

to as an ensemble of

(5)

1978 JOURNAL DE

PHYSIQUE

II N°11

j

.,

atomic

beam ',

Standing

WaVB

_' ,-.~

jjght

field

t>'<l't

f+U3

~ f+U2

L

f+L

~

X

Fig.

3. A coherent atomic

beam,

modelled

by

a broad Gaussian, traverses a red detuned

standing

wave

light

field. The atoms are focussed at the antinodes of the

light

field which acts

as an array of thin lenses with focal length f. At z

= f an array of

narrow peaks with period d

=

~/2

is formed

(first

bold

line).

Natural

spreading

of the atom distribution leads to the formation of Fresnel

images

with

periods d/3

and

d/2

at z

=

f

+

L/3

and z

=

L/2, respectively (second

and third bold

line).

At

z = f + L the initial distribution from z

=

f

is reconstructed

(fourth

bold

line).

j~

l$

c

©

x-direction

Fig.

4. The initial atom distribution at z = f, the successive Fresnel

images,

and the reconstruction image denoted

by

the four bold lines in

figure

3. Thin solid line: initial distribution at z

= f with

period

d, bold solid line: Fresnel

image

with

period d/3,

bold dotted line: Fresnel

image

with

period

d/2,

thin dotted line: reconstruction

image

with

period

d,

phase

shifted

by

~.

(6)

N°11 ATOMIC FRESNEL IMAGES ATOM LITHOGRAPHY 1979

classical

point-like particles,

is focussed as the antinodes of the

light

field form

quasi-harmonic potentials. However,

the

subsequent

free evolution in the z-direction is very different in the

two cases. For z >

f

the

peaks

in the distribution

spread

out and

overlap.

For a coherent

beam the

peaks

have a well-defined

phase

relation and

spatial

interferences between the

peaks

lead to

fringes

in the

intensity

distribution. The

period

of these

fringes

which form the Fresnel

images

discussed below can be much smaller than d. For an incoherent beam no smaller

periods

appear as the

outspreading peaks

have no fixed

phase

relation. Their intensities

simply

add and the initial

periodic

modulation is smoothed out.

The free evolution in the z-direction of a coherent distribution with a

phase

or

amplitude

modulation of

period

d leads after the so called Talbot

length

L

=

d2/ldB

to a reconstruction of the initial

distribution,

an effect first observed with

light by

Talbot

[9].

At intermediate

distances

L/m,

m

=

2, 3,...,

distributions with smaller

periods d/m

appear. The

images

with smaller

periods

are referred to as Fresnel

images,

the reconstruction

images

are often called Fourier

images [10, iii.

The locations of Fresnel

images

were first found in

[12]

and

[13].

The

general

ID Talbot

problem, including

both finite width and infinite width

complex-valued

diffraction

gratings,

has been

analysed

in detail

by

Clauser and Reinsch

[15].

For matter waves,

experimental

observations of Fourier

images

were

reported

in

[16, Iii,

observations of Fresnel

images

were

reported

in

[18].

In

figure 3,

the

amplitude

modulation at z =

f

with

period

d leads to the formation of Fresnel

images

with

periods d/3

at z

=

f

+

L/3 (second

bold

line)

and

d/2

at z =

f

+

L/2 (third

bold

line).

At z

=

f

+L the distribution from z

=

f, phase

shifted

by

ir, is reconstructed

(fourth

bold

line).

At z

= 0 the

incoming

wave

acquires

a

periodic phase

modulation from the

light

field which acts as a

phase grating leaving

the

amplitude

of the wave

basically unchanged.

This leads to the formation of a

nearly fringe-free

reconstruction

image

at z

= L. The

plane

at z =

f

+ L can be viewed as well as the focal

plane

of this reconstruction

image.

The four distributions

depicted by

the bold lines are also shown in

figure

4 for better

comparison.

The ratio of Talbot

length

to focal

length

in this simulation was

L/ f

= S-G-

Fresnel

images

have

potent1al applications

in atom

lithography making

it

possible

to write very small

periodic

structures on a substrate

placed

in the

plane

of a Fresnel

image.

The

visibility

of the Fresnel

images depends strongly

on the ratio between the width of the

peaks

and their

separation

in the

original

array: the smaller the width

compared

to the

separation,

the

higher

is the maximal order of

periods.

Note that

standing

wave diffraction allows a more flexible

preparation

of the initial atomic array than the use of transmittion

gratings (as

used e-g- in

[16-18]),

because both the

periodicity

and the width of the diffraction

peaks

can be

changed

at will

by varying

the

period

and the

intensity

of the

diffracting light

field.

A favorable candidate for atom

lithography

is chromium with the transition

~S3 -~P(

at

1 = 425.6 nm and M

= 52 u [8]. With these values the recoil

frequency

is wr

=

132,

kHz and

the

parameters

used in the simulation become fl

= 37

MHz,

b

= -26

MHz,

and T

= 330 ns.

For a

typical longitudinal velocity

of ~

= 1000

m/s

the Talbot

length

is L

= 6 mm, so that

the Fresnel

images

with

periods d/2

and

d/3

in

figure

3 would appear at distances behind the focal

plane

of 3 mm and 2 mm,

respectively.

These distances and the

parameters

for the

light

field seem to be well in

experimental

reach.

A restriction for the

quality

of the Fresnel

images

in a continuous beam

experiment

is the

longitudinal velocity

distribution

A~/~

of the atoms which leads to different interaction times and to a

smearing

out of the Fresnel

images. By taking

into account a

longitudinal velocity

distribution with a

rectangular profile

in our

simulations,

we found that up to

A~/~

= 0.25 the Fresnel

images

of

figure

3 are still observable. This

velocity

distribution is narrower than the one for a thermal

beam,

but with

velocity selecting

devices it should be

experimentally

accessible.

(7)

1980 JOURNAL DE

PHYSIQUE

II N°11

Summarizing,

it has been demonstrated that wave

packet

simulations allow for a

qualitative

and

quantitative study

of the formation of atomic Fresnel

images.

We showed that Fresnel

images

can be created

by focussing

an coherent atomic beam at the antinodes of a

standing light

field. Possible

applications

in atom

lithography

were

investigated

for the

potential

candidate

chromium. The necessary

parameters

found are well in

experimental

reach.

Acknowledgments.

Fruitful discussions with C-R-

Ekstrom,

U.

Drodofsky,

and M. Drewsen are

gratefully

ac-

knowledged.

The authors

acknowledge support by

the Deutsche

Forschungsgemeinschaft

and

hospitality

in the group of Professor J.

Mlynek.

References

ill

Sleator T., Carnal

O.,

Pfau T., Faulstich A., Takuma H, and

Mlynek

J., Laser Spectroscopy X:

Proc. 10th Int. Conf, on Laser

Spectroscopy,

M.

Ducloy,

E. Giacobino and G.

Camy

Eds.

(World Scientific, Singapore, 1991).

[2] Keith

D-W-,

Ekstrom C-R-, Turchette

Q-A.

and Pritchard D-E-,

Phys.

Rev. Lett. 66

(1991)

2693.

(3] Gould PI., Ruff G.A. and Pritchard D-E-, Phys. Rev. Lett. 56

(1986)

827.

[4] Adams C-S-, Pfau T., Kurtsiefer Ch, and

Mlynek

J.,

Phys.

Rev. A 48

(1993)

2108.

(5] Pfau T., Kurtsiefer

C.,

Adams

C-S-, Sigel

M. and

Mlynek

J.,

Phys.

Rev. Lett. 71

(1993)

3427.

(6] Janicke U. and Wilkens

M.,

to appear in

Phys.

Rev. A

(1994).

(7] Sleator T., Pfau

T., Balykin

V, and

Mlynek J., Appl. Phys.

B 54

(1992)

375.

(8] Mcclelland J-J-, Scholten R-E-, Palm E-C- and Celotta R.J., Science 262

(1993)

877.

(9] Talbot

H-F-,

Philos.

Mag.

9

(1836)

401.

[10] Cowley J. and Moodie A., Proc.

Phys.

Soc. B 70

(1957)

486, 497, 505.

[t ii Winthrop

J-T- and

Worthington C-R-,

J.

Opt.

Soc. Am 55

(1965)

373.

(12] Gori

F., Opt.

Commun. 31

(1979)

4.

[13] Sudol R. and

Thompson B-J-, Opt.

Commun. 31

(1979)

105.

[14] Patorski K., Progress in

Optics

XXVII, E. Wolf Ed.

(Elsevier,

Amsterdam,

1989).

(15] Clauser J-F- and Reinsch M.,

Appl.

Phys. B 54

(1992)

380.

[t6]

Carnal

O.,

Turchette

Q.A.

and Kimble

H-J.,

Near Field

Imaging

with Two Transmission

Gratings

for Sub-Micron Localization of Atoms, to be submitted.

(17]

Chapman

M-S-, Ekstrom

C-R-,

Hammond

T-D-, Schmiedmayer

J., Tannian

B-E-, Wehinger

S.

and Pritchard

D-E-,

Near Field

Imaging

of Atom Diffraction

Gratings:

the Atomic Talbot

Effect,

to be submitted.

(18] Clauser J-F- and Li

S., Phys.

Rev. A 49

(1994)

2213.

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