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ISSN 1054660X, Laser Physics, 2010, Vol. 20, No. 3, pp. 683–693. © Pleiades Publishing, Ltd., 2010.

Original Russian Text © Astro, Ltd., 2010.

683

1 1. INTRODUCTION

Recently, quantum degenerate atomic mixtures have been studied extensively both in theoretical and experimental directions. Fermionic degeneracy has been observed by means of sympathetic cooling with many alkali atom mixtures like 7Li–6Li [1, 2], 23Na– 6Li [3], 87Rb–40K [4–6], and recently with an isotopic mixture of ytterbium (Yb), 174Yb–173Yb [7]. Interac tion between the different species strongly affects the equilibrium properties of the mixture such that the mixture collapses [6] in the presence of attractive bosonfermion coupling, or in the opposite case, repulsion between the species causes spatial demixing [8, 9].

Boson–fermion (BF) mixtures can also be realized from an imbalanced twocomponent Fermi gas where bound fermions form a Bose–Einstein condensate (BEC). However, BF mixtures of two atomic species have the advantage that the interaction between the bosons and between the different species can be driven independently and attractive BF interaction is accessi ble [10, 11].

The properties of threedimensional (3D) trapped BF mixtures were studied in detail by using a modified Gross–Pitaevskii (GP) equation [12, 13], and by using the Thomas–Fermi (TF) approximation for the fer mionic component [14, 15]. In a quasi3D limit, where collisions can still be considered as 3D, effects of the geometry were also studied in the TF regime [16]. Such a simple model predicts, in a pancake 1The article is published in the original.

shaped trap, that the stability of the mixture depends only on the scattering length and the transverse width of the cloud. One should expect, in a true dimensional crossover, namely including dimensional effects in scattering events, that the mixture stability depends critically on the energy, and thus on the number of particles. There are also studies on BF mixtures in twodimensional (2D) [17] and onedimensional (1D) [18] optical lattices in which manybody phase diagrams has been obtained by the bosonization approach.

It is well known that a hardcore boson gas shows very different features from its 3D counterpart if the scatteringevents are twodimensional. In 3D, particle interactions can be described by the zeromomentum and zeroenergy limit of Tmatrix, leading to a con

stant coupling parameter. In 2D, the Tmatrix van

ishes at low momentum and energy [19, 20] and the firstorder contribution to the coupling is obtained by taking into account the manybody shift in the effec tive collision energy of twocondensate atoms [21, 22]. This causes an energy dependent coupling parameter which greatly affects the equilibrium and the dynami cal properties of the gas [23, 24].

The dimensional crossover from a 3D to a 2D trapped mixture may be studied in the experiments by flattening magnetic or dipolar confinements [25], or by trapping atoms in specially designed pancake potentials, as rotating traps [26], gravitooptical sur face traps [27], rfinduced twodimensional traps [28] or in onedimensional lattices [29] where a 3D gas can be split in several independent disks.

PHYSICS OF COLD TRAPPED ATOMS

Dimensional Crossover in TwoDimensional

Bose–Fermi Mixtures

1

A. L. Suba ia, S. Sevinçlib, P. Vignoloc, and B. Tanatara, * a Department of Physics, Bilkent University, Bilkent, Ankara 06800, Turkey

b MaxPlanckInstitut für Physik komplexer Systeme, Nöthnitzer Str. 38, 01187 Dresden, Germany c Institut Non Linéaire de Nice, Univeraité de NiceSophia Antipolis, CNRS,

1361 route de Lucioles, 06560 Valbonne, France *email: [email protected]

Received October 15, 2009; published online February 2, 2010

Abstract—We investigate the equilibrium properties of bosonfermion mixtures consisting of a Bose conden

sate and spinpolarized Fermi gas confined in a harmonic twodimensional (2D) trap using meanfield the ory. Bosonboson and bosonfermion coupling constants have a logarithmic dependence on the density because of the twodimensional scattering events when the swave scattering lengths are on the order of mix ture thickness. We show that this modifies the density profiles significantly. It is also shown that the dimen sional crossover stabilizes the mixture against collapse and spatial demixing is observed for the case of a neg ative bosonfermion scattering length.

DOI: 10.1134/S1054660X1005018X

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684

LASER PHYSICS Vol. 20 No. 3 2010

SUBASI et al., In this paper, the equilibrium properties of a mix

ture of condensed bosons and spinpolarized fermions are studied, through the dimensional crossover from three to two dimensions. There is no fermionfermion interaction and we include the BF swave interaction selfconsistently in a suitably modified GP equation for bosons [30]. The chemical potentials and the radii of the clouds are also obtained by using the TF approx imation.

2. MEANFIELD MODEL

We consider a 2D BF mixture in harmonic trap with potentials VB(F) = and particle numbers NB and NF. Here, mB(F) is the boson (fermion) mass and ωB(F) is the radial trap frequency as seen by boson (fermion) species. Within the meanfield approach the total energy functional at T = 0 is written as

(1)

where ψB is the groundstate wave function of bosons and |ψF|2 = nF gives the fermion density. In the above expression, boson species are in the condensed state and fermion component is assumed to be spinpolar ized, there is no fermionfermion interaction, and gBB and gBF are the interaction couplings between the bosons and between bosons and fermions, respectively. There is a significant difference between the form of the energy functional given above and that in 3D, which is that the BB and BF interaction strengths are in general density dependent in contrast to the situa tion in 3D. The term TF in Eq. (1) is the kinetic energy of the fermions written within the Thomas–Fermi– Weizacker approximation as [31–33]

(2) where the Weizsacker constant is λW = 1/4. The Euler–Lagrange equations for the mixture are [32, 33]

(3)

where Ᏺ = Ᏹ – μBB|2 – μFF|2 with μB and μF, the boson and fermion chemical potential entering as Lagrange multipliers to satisfy the normalization con

1 2 mB F( )ωB F( ) 2 r2 EBF] = d2r ប 2 2mB  ∇ψB 2 VB( ) ψr B 2 1 2 gBBψB 4 + + ⎩ ⎭ ⎨ ⎬ ⎧ ⎫

+ d

2r T{ F+VF( ) ψr F2}+

d2rgBFψBF2, TF ប 2 mF  πnF 2 λW 8 ∇nF 2 nF  + ⎝ ⎠ ⎛ ⎞ , = ∂Ᏺ ∂ψB  ∇ ∂Ᏺ ∂ ∇ψ( B)  – = 0 and ∂Ᏺ ∂ψF  ∇ ∂Ᏺ ∂ ∇ψ( F)  – = 0,

ditions NB = and NF = . Then, the explicit form of the equations of motion are

(4)

and

(5)

The above equations of motion are obtained by neglecting the higherorder terms involving δg/δψB, F which is valid in the dilute gas limit Ⰶ 1 and Ⰶ 1. The beyond meanfield corrections can become notable when aBB, aBF and/or NB, NF are large for fixed trap frequencies. For the systems under con sideration we have chosen the parameters appropri ately so the diluteness conditions hold for our numer ical calculations. Therefore, the beyond meanfield terms in the energy functional are not important in our examples.

One should also note that the existence of BEC in 2D needs to be examined carefully. Initial studies have concluded that no BEC could occur in 2D trapped gases but recent considerations within the Hartree Fock–Bogoliubov approximation [34], the density dependent interaction strength [35] and numerical simulations [36] have established firmly the occur rence of BEC for such systems. Thus, our assumption of a 2D condensate at T = 0 is justified.

When the number of atoms is large one can use the Thomas–Fermi (TF) approximation, i.e., the kinetic energy terms can be neglected in the GP equations, which simplifies them to coupled algebraic equations

(6) (7) In the above, |ψB|2, |ψF|2≥ 0 and we have defined the effective fermionfermion interaction coupling gFF = 2πប2/m

F. We have also introduced the TF radii RB, RF where boson and fermion wave functions go to zero respectively through |ψB(RB)|2 = 0 and |ψF(RF)|2 = 0. Assuming RF RB (since gFF Ⰷ gBB, fermions are pushed out further due to Pauli exclusion principle)

d2rψB2

d2rψF2 – ប 2 2mB ∇2+VB+gBBψB2+gBFψF2–μB ⎩ ⎭ ⎨ ⎬ ⎧ ⎫ ψB = 0, – ប 2 2mF λW∇ 2 VF + ⎩ ⎨ ⎧ + ប 2 mF 2π ψF 2 gBFψB 2 μF – + ⎭ ⎬ ⎫ψ F = 0. nBaBB 2 nFaBF 2 gBB ψB 2 gBFψF 2 VB + + = μB, gFFψF2+gBFψB2+VF = μF.

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