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HAL Id: jpa-00247254

https://hal.archives-ouvertes.fr/jpa-00247254

Submitted on 1 Jan 1996

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Stability of Atomic Bose-Einstein Condensate with Negative Scattering Length

Weiping Zhang, B. Sanders, A. Mann

To cite this version:

Weiping Zhang, B. Sanders, A. Mann. Stability of Atomic Bose-Einstein Condensate with Neg- ative Scattering Length. Journal de Physique I, EDP Sciences, 1996, 6 (11), pp.1411-1415.

�10.1051/jp1:1996154�. �jpa-00247254�

(2)

Stability of Atomic Bose-Einstein Condensate with Negative Scattering Length

Weiping Zhang (~),

B-C- Sanders

(~)

and A. Mann (~~~,*)

(~) School of Mathematics,

Physics, Computing

and Electronics,

and Centre for Lasers and

Applications, Macquarie University,

North

Ryde,

New South Wales 2109, Australia

(~)

Department

of

Physics,

Technion-Israel Institute of

Technology,

Haifa 32 o00, Israel

(Received

26

February1996,

revised 24 June1996,

accepted

1

August 1996)

PACS.42.50.Vk Mechanical effects of

light

on atoms, molecules, electrons and ions PACS.32.80.-t Photon interactions with atoms

Abstract. We discuss the

stability

of

a small-scale Bose-Einstein condensate with nega- tive scattering

length.

The stable state is found

by obtaining

the appropriate basis using self-

consistent field theory for an attractive one-dimensional

potential.

Bose-Einstein Condensation in dilute atomic gases has been reaJized for

8~Rb Ill,

for

~Li

[2j and for

~~Na [3j.

In the latter case a condensate has formed

despite

the presence of an attractive

potentiaJ. Although suprising

at

first,

Bose-Einstein Condensation is

possible

in attractive

potentials.

Here we determine the

appropnate

basis states for an attractive one-dimensional

potential

and use this basis set to show that a stable Bose-Einstein Condensate with

negative scattering length

can indeed form.

A nonlinear Hamiltonian for an atomic beam in an attractive à-function

potential

is given

by

[4j

É

=

-j /

dz

)t(xj$il(xj

+

/

dz

dx' ôt(xjilt (xl jV(x x')il(x'jil(xj, (ij

where

/(x)

is the atomic field annihilation

operator,

and

V(x

-x' is the nonlinear

dipole-dipole

interaction

arising

in the

study

on nonlinear atom

optics [4, 5j.

The

potential

is assumed to extend over a range of the order of the

optical wavelength;

as this scale is much smaller than the interatomic

separation

for a dilute gas, we can

employ

the

pseudopotential approximation

[6]

vjx xl

t

-xôjx xl j. j2j

The

pseudopotential approximation

is

justified

for a dilute gas where the

density

of the gas n

and the s-wave

scattering length

a

satisfy

the condition

Ra~

< 1.

(3)

(*)

Author for

correspondence (e-mail: ady@physics.technion.ac.il)

@

Les

Éditions

de

Physique

1996

(3)

1412 JOURNAL DE

PHYSIQUE

I N°11

For N atoms in the

condensate,

the field

operators

can be

decomposed

as

Î~(X)

"

~7b(X)àb

+

à~Ç7~(X)â~

(4)

where the functions

qJb(x)

and

(qJ~(x))

are

eigenfunctions

of the self-consistent nonlinear

Schrôdinger equation

Î~ ~~~

~~~~~~~~~~~~~

~~

~~~

obtained

by applying

the

time-independent

Hartree-Fock

approximation

to

equation il)

with the

pseudopotential (2).

The function

I?i

qJb(x)

=

fisech ~

(N -1)xxi (6)

2 2

is an

eigenstate

of the nonlinear

equation

with

corresponding eigenvalue

Eb

=

ilN 1)xi~ /8, j7)

and trie set of states

~~~~~

fi~~~~ ~~~

l

)XX /2j

i~

i + i~

e~~~'/-iix~/2

~

are

eigenstates

of trie modified version of

(5),

with

corresponding eigenvalues E~

=

(N

1)~x~~~/8,

where trie effective

density

)qJbÎ~

replaces

trie exact

density

)qJ)~

iii.

Trie

eigenfunc-

tion

qJb(x)

is trie

unique

bound state for trie

system

with a

negative

energy value.

Conversely,

trie

eigenfunctions (qJ~(x)), corresponding

to trie continuum index ~, possess

nonnegative

en-

ergy values. Trie energy gap betweenlhe bound state and trie continuum mdicates that a stable state is

possible,

in contradistinction to trie momentum

eigenstate

expansion of

/(x)

where trie zero-momentum

eigenstate

is unstable due to trie presence of trie attractive

poten-

tial.

(This instability

is manifested

by

trie appearance of

an

imaginary

excitation spectrum in the

Bogoliubov approximation

for this

case.)

The

decomposition (4)

aJlows the Hamiltonian

É

to be rewritten in terms of the annihilation operators

âb

and

â~

and their

conjugates à)

and

âÎ.

The

Bogoliubov approximation

[8] involves

replacing âÎ

and

âb by @, replacing

N-1

by N,

and

discarding

lower-order terms with

respect

to N for

sufficiently large

N.

Thus,

the Hamiltonian

(1)

reduces to

Éred

=

NEb

+

/ d~E~âlâ~

+

xN~ )qJb(x))~dx

2

~~

d~

dl

(E$~, â~â~,

2

+(E$~, )"âÎâÎ,

+

2E[~,âlâ~, ), (9j

"~~~~~

Bj~,

=

/

dz

jç7llx)l~

v7~lx)v7~,lx) ~~°~

and

E[~,

"

/ dz1i7b(xji~ ç7i(xjç7~,ixj. Ill)

(4)

are the collision

coefficients,

which can be

written, using equations (6, 8),

as

~~~' ÎÎ /

~~~~~~Î~Î~

~~~

~~~Î~ÎÎ~'

~~~~

~ÎI~~ÎÎÎI'

~~~~

Integrating (12) produces

trie

expression

I?1

~~~' ~Î ÎÎ/~Î~ÎÎ/Î~ÎÎ' sinh[(Î Î Î)r

/2]

~~~~

which is

sharply peaked

at ~ + ~'. Trie

major

contribution to trie Hamiltonian

(9)

is from terms for which ~

= +~'.

Trie reduced Hamiltonian is still not amenable to an exact

analytic

solution.

However,

trie Hamiltonian can be

separated

into two

components: (a)

trie

approximate

reduced Hamiitoman which retains

only

trie dominant

diagonal

terms ~ = ~' and trie dominant

ofl-diagonal

terms ~ =

-~' and

(b)

trie residual terms which are treated later. Trie

approximate

reduced Hamiltonian is thus written as

ÉS~~~

"

Êb

+

/

d~

lE~ 91~)1àlà~ /

d~

91~)

(à~à-~

+

àlà~

~j li~)

Î Î

~°~

E~

=

NE~

+

1~N2 / jç~~j~)j4dx. (15)

2

~~~~

~~~~

Î~Î~ ÎÎÎ

~~~~

With

respect

to the

approximate

reduced Hamiltonian

(14),

the

integrals

can be restricted to

nonnegative

~

by rewriting

the

expression

as

É]fl~~°~

=

Êb

+ ~ d~

[E~ g(~)] âlâ~

+

âÎ ~â-~

~ d~

g(~) â~â-~

+

âÎâÎ

~

(17)

Using

the

Bogoliubov

transformation [8],

Î~

=

u~â~ ~~âÎ

~

(18)

and its

conjugate

expression, we obtain the final energy

spectrum

E]$~~°~

=

~/[E~ Eb g(x)]~ [g(~)]~

ç~

~~X~ ~/(~~ ~)

~

~j~ ~)~2

+ 3~~4_

(ig)

4/à

The reduced energy

(19)

is a

positive

real number in the limit that ~ - 0. The excitation

spectrum

contains a finite gap which anses from the bound state nature of the

condensate;

therefore,

at

sulliciently

low

temperatures,

the atoms will

stay

in the condensate until the

temperature

increases to the order of the gap. This is similar to the situation in the BCS

theory

of

superconductivity

where the finite gap

prevents

energy

dissipation.

Of course trie

approximate

reduced Hamiltonian

(14) neglects

the residual terms in the re-

duced Hamiltonian

(9).

The reason for

neglecting

these terms is that a resonance is evident

(5)

1414 JOURNAL DE

PHYSIQUE

I N°11

in the collision coefficients

(10)

and

(11).

The dominant contribution to the collision coeffi- cient

(13)

arises for ~

= +~'. The residual terms will

modify

trie size of trie gap.

However,

trie

Bogoliubov approach provides

a

good approximation

for trie

ground

and low-excited

states, and,

as trie exact Hamiltonian bas a gap, trie terms

neglected

in going from

equations il, 2)

to

equation (9)

do not

substantially

alter trie value of trie gap. Trie modification to trie size of trie gap caused

by

trie

neglected

residual terms is

certainly

of interest but not amenable to ana-

lytical

calculation.

Therefore,

trie final energy

spectrum (19)

represents trie closest calculation achievable

by analytic

means.

At low

temperatures,

the condensate formed

by putting

the atoms in the bourra state

(6)

is indeed

stable,

and an attractive

potential

does allow the existence of a stable Bose conden-

sate.

However,

this bound state condensate can be very diflerent from the condensate for the

field in the absence of an attractive

potential

or in the presence of a

repulsive potential.

In the attractive interaction à-function

potential

the zero-momentum state is not a stable Bose

condensate;

instead the stable state is

given by equation (6). Creating

a stable Bose-Einstein condensate with the attractive interaction would require

'cooling'

the atoms into such a state.

Once the

temperature drops

below the gap energy, a swift condensation into this bound state condensate may be

expected.

It is

interesting

to contrast this

stability

for any number N of atoms in the condensate with trie result of

Baym

and Pethick [9]. Their solution is stable for N restricted between 0 and a

specific

upper bound. Trie diflerent result is a consequence of trie diflerent

approaches adopted

here and in reference [9]. In reference [9] the

three-dimensional trap potential

is assumed to be the dominant

potential

and is used to determine the nature of the

macroscopic

wavefunction of the condensate. In contrast our

approach,

which

employs

a one-dimensional self-consistent field theoretic

technique, yields

exact solutions of the

Schrôdinger equation:

the resultant

wavefunction narrows in space and the energy gap increases with

N~.

This

ensures that the

wavefunction chosen here is stable for all N.

Extending

this

analysis

to the three-dimensional version of the self-consistent nonlinear

Schrôdinger equation (5)

would be

interesting,

but the

three-dimensional case is much more

complicated

where even issues such as the existence of a stable sohton solution itself must be considered

[loi.

Whereas the above results are

obviously

tied to the

specific

interaction

being considered,

the

qualitative

results should holà for

general

attractive one-dimensional

potentials.

The restriction here to one dimension is motivated

by

the treatment of a confined Bose gas as treated in

reference [4]. For an attractive interaction the self-consistent Hartree-Fock

equations

will

yield

a lowest

single-partiale state,

and the Hartree state obtained

by putting

all the atoms into this

single partiale

state will form a stable condensate with a real excitation spectrum

containing

a finite energy gap. This will support the condensate

against breakup

at

sufficiently

low

temperatures

and may cause a swift condensation when the

temperature

is lowered below the gap energy.

Acknowledgments

This research has been

supported by

a

Macquarie University

Research

Grant, by

the Fund for

Promotion of Research at the

Technion, by

the Technion VPR

Fund,

and

by

GIF German-

Israeh Foundation for Research and

Development.

WZ is

supported by

an Austrahan Research Council Research

Fellowship.

(6)

ILeferences

[1] Anderson

M.H.,

Ensher

J-R-,

Matthews

M.R.,

Wieman C.E. and Cornell

E-A-,

Science 269

(1995)

198.

[2]

Bradley C.C.,

Sackett

C.A.,

Tollett J-J- and Hulet

R-G-, Phys.

Reu. Lett. 75

(1995)

1687.

[3] Davis

K-B-,

Mewes

M.-O.,

Andrews

M.R.,

van Druten

N-J-,

Durfee

D.S.,

Kurn D.M. and Ketterle

W., Phys.

Reu. Lett. 75

(1995)

3969.

[4]

Zhang W., Phys.

Lett. A 176

(1993) 225; Zhang W.,

Walls D.F, and Sanders

B.C., Phys.

Reu. Lett. 72

(1994)

60.

[5] Lenz

G., Meystre

P, and

Wright E-M-, Phys.

Reu. Lett. 71

(1994)

3271.

[6]

Huang K.,

Statistical Mechanics

(Wiley,

New

York, 1963).

I?i Yoon B, and

Negele J-W-, Phys.

Reu. A 16

(1977)

1451.

[8] N-N-

Bogoliubov,

J.

Phys. (Moscow)

11

(1947)

23.

[9]

Baym

G, and Pethick

C.J., Phys.

Reu. Lett. 76

(1996)

6.

[loi

See Kuznetsov

E-A-,

Rubenchik A.M., and Zakharov

V.E., Phys. Rep.

142

(1986)

103:

particularly equation (149)

and discussion.

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