Avalanches of Bose-Einstein Condensates in Leaking Optical Lattices
G. S. Ng
1
, H. Hennig
2,3
, R. Fleischmann
2
, T. Kottos
1,2
, and T. Geisel
2,3
1
Department of Physics, Wesleyan University, Middletown, Connecticut 06459, USA
2
MPI for Dynamics and Self-Organization, Bunsenstraß e 10, D-37073 Göttingen, Germany
3
Institute for Nonlinear Dynamics, University of Goettingen, 37073 Goettingen, Germany
One of the most fascinating experimental
achievements of the last decade was the real-
ization of Bose-Einstein Condensation (BEC) of
ultra-cold atoms in optical lattices (OL's) [1, 2,
3, 4]. The extraordinary level of control over
these structures allows us to investigate complex
solid state phenomena [4, 5, 6, 7, 8, 9] and the
emerging field of �atomtronics� promises a new
generation of nanoscale devices. It is therefore
of fundamental and technological importance to
understand their dynamical properties. Here we
study the outgoing atomic flux of BECs loaded in
a one dimensional OL with leaking edges, using
a mean field description provided by the Discrete
Non-Linear Schrodinger Equation (DNLSE). We
demonstrate that the atom population inside the
OL decays in avalanches of size J . For intermedi-
ate values of the interatomic interaction strength
their distribution P (J) follows a power law i.e.
P(J) ∼ 1/Jα characterizing systems at phase tran-
sition. This scale free behaviour of P(J) reflects
the complexity and the hierarchical structure of
the underlying classical mixed phase space. Our
results are relevant in a variety of contexts (when-
ever DNLSE is adequate), most prominently the
light emmitance from coupled non-linear optics
waveguides [12].
An optical lattice with a controlled leakage of the
atomic BEC can be realized experimentally by the action
of two separate continous microwave or Raman lasers to
locally spin-flip BEC atoms (at the edges of the OL) to
a nontrapped state [10, 11]. The spin-flipped atoms do
not experience the magnetic trapping potential and are
released through gravity in two atomic beams at the ends
of the OL. The mathematical model (see Method section)
that describes the dynamics of the BEC in a leaking OL
of size M is
i
∂ψn
∂τ
= χ |ψn|2 ψn − 12 [ψn−1(1− δn,1) + ψn+1(1− δn,M )]
− iγψn[δn,1 + δn,M ]; n = 1, · · · ,M (1)
where γ describes the atomic losses and Nn = |ψn|2
is the atomic population at site n. Below we study
the decay (due to leakage) of the total atom population
N(τ) =
∑
nNn(τ) inside the OL as a function of the ini-
tial effective interaction strength i.e. Λ = χN(τ = 0)/M .
An exciting result appearing in the frame of nonlin-
ear lattices is the existence of stationary, spatially local-
ized solutions, termed Discrete Breathers (DB), which
emerge due to the nonlinearity and discreteness of the
system. DBs were observed in various experimental se-
tups [15, 16, 17, 18, 19, 20] while their existence and
stability were studied thoroughly during the last decade
[21, 22, 23, 24, 25]. Their importance was already recog-
nized in [26] where it was shown that they act as virtual
bottlenecks which slow down the relaxation processes in
generic nonlinear lattices [25, 26, 27]. Further works
[27] established the fact that absorbing boundaries take
generic initial conditions towards self-trapped DB's. Re-
cently the same scenario was proposed for a BEC in a
leaking OL where it was observed [10] that N(τ) decays
in sudden bursts J (see inset of Fig. 1). Here, for the
first time we present a full theoretical study of the decay
process of N(τ) and analyze the distribution P(J). We
find three types of dynamical behaviour [14]: For very
weak interactions Λ, the population decay is a smooth
process which does not involve any avalanches. As inter-
actions are increased, avalanches are created. For strong
interaction strength, their distribution P (J) is exponen-
tial. In contrast, for intermediate values of the interac-
tion strength, P (J) follows a power law indicating the
existence of a phase transition. Below, we will focus our
analysis in this critical regime.
Since we are interested in the effects of DBs on the re-
laxation process, we introduce a localization parameter
PR which provides a rough estimate of the relative num-
ber of sites that are occupied by the remaining atoms in
a leaking OL. It is defined as
PR(τ) = [N(τ)]
2
M
∑
n |ψn(τ)|4
(2)
which in case of γ = 0 is the standard participation
ratio. Accordingly, the more evenly the atoms spread
over the lattice, the closer PR is to a constant of or-
der 1. The PR approaches two limiting values [14]: (a)
PR = 1/2 corresponding to a random superposition of
uncoupled sine waves for U = Λ = 0 (linear regime) and
(b) PR = 5/9 corresponding to a configuration of atoms
trapped in M uncoupled (T → 0 ) wells for Λ → ∞,
which might be viewed as the formation of O(M) DB's
(multi-breather regime). In the closed system, the tran-
sition between these limiting cases is smooth (see lower
left inset of Fig. 1).
In the open system (γ > 0) PR is a time dependent
quantity. We numerically study the value PRS=PR(τ∗)
for large times τ∗ when the system has evolved from its
initial thermalized state into a quasi-steady state [31].
For nonzero γ, instead of a smooth transition between
the two extremes we observe a sharp drop of the PRS at
a critical interaction strength of Λb ≈ 0.15 resembling a
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phase transition (our numerics indicate that this transi-
tion becomes a step function in the limitM →∞). PRS
drops down to its lowest possible value (∝ 1/M) corre-
sponding to a single occupied site, i.e. the final state
consists of a one self-trapped DB. If Λ increases further
(Figs. 2b-c) the final state consists of a successively larger
number of breathers, while for some critical Λ it evolves
into a more complicated state with a power-law distribu-
tion of norms Nn (see Fig. 1 left upper inset) [32].
In the following it is important to realize that if a
breather solution exists for some value of Λ, it exists for
all Λ′s > 0 (and for large enough M). This conclusion
can be easily drawn by noting that a self-trapped DB is
not directly coupled to the leaking edges, thus we can
assume γ = 0 and then appropriately scale Eq. 5. There-
fore breather solutions in particular do exist for Λ < Λb
as well. So, what is the nature of the sharp transition
at Λb? To answer this question, we have to examine the
thermalized random initial states more closely. For small
Λ ≈ 0 these states have exponentially distributed norms
PNn(x) = Mexp(−Mx) [14]. In addition, our numerical
calculations (see the phase space analysis below) indi-
cate that the minimal total nonlinearity associated with
the central site of a self-trapped DB solution satisfy the
relation MΛ |ψ|2 ≈ 1 . Thus, a necessary condition in
order to excite such a DB is that at least one site of the
thermalized initial state has a norm x > x0 = 1/(MΛ).
Assuming independent random norms for the individ-
ual sites we get that the probability for such an event
is WM (x) = 1 − (1 − exp(−Mx))M . By increasing M ,
we find that WM (x) posseses a steep transition from 1 to
0 at approximately x1/2 with WM (x1/2) = 1/2. We can
thus give a rough estimation of the lower bound for Λb
by demanding x1/2 ≥ x0, which leads to
Λb ≥ − 1
ln
(
1− [0.5]1/M
) ≈ 1
lnM − ln ln 2 (3)
in fair agreement with the value Λb ≈ 0.15 for the system
sizes we studied [33].
The most interesting situation emerges for large
enough system sizes and (for the system sizes we could
numerically study) interatomic interactions in the range
of Λ ≈ 0.5 − 1 [34]. In this case we have found that
the atoms leak out of the lattice in avalanches follow-
ing a scale-free distribution, i.e. P(J) ∼ J−α, while the
norms Nn at individual lattice sites are distributed as
PNn(x) ∼ x−βwith α ≈ β (see Fig. 1 left upper inset).
This power law behavior for a whole range of parameter
values Λ could be interpreted as a signature of a self-
organized critical state [28].
Let us study in more detail the dynamics that lead to
the creation of an avalanche in this parameter regime.
One such event is depicted in Fig. 2d. A moving DB,
coming from the bulk of the lattice, collides with the
outer most self-trapped DB. As a result the self-trapped
breather is shifted inwards by one site while at the same
time a particle density proportional to the density of the
moving breather tunnels through the self-trapped DB.
Eventually this particle density will reach the leaking
edge of the OL and decay in a form of an avalache.
We have also found numerically [14] that during the
migration process of the self-trapped DB, the number
of particles and the energy of the three lattice sites in-
volved is conserved, thus allowing us to turn the problem
to the analysis of a reduced M = 3 system with inter-
action strengths Λ in the critical range. As shown in
Fig. 3a (inset), the non-linear trimer exhibits a hierar-
chical mixed phase space structure with islands of regular
motion (tori) embedded in a sea of chaotic trajectories.
Trajectories inside the islands correspond to self-trapped
DBs, provided that their frequency is outside the linear
spectrum. In contrast, chaotic trajectories have contin-
uous Fourier spectra, parts of which overlap with the
linear spectrum of the infinite lattice [21]. As long as the
self-trapped DB is stable, it acts as a barrier which pre-
vents atoms from reaching the leaking boundary. Thus, a
necessary condition for an avalanche event is the destabi-
lization of the DB. This is caused by a lattice excitation
with particle density Npert1 greater than a critical value
which can push the regular orbit out of the island. At
the same time a portion Nmax3 ∝ Npert1 transmits through
(see Fig. 3a). As can be seen from Fig. 2, the migra-
tion process usually moves the DB inwards by one site
which correspond to another island in the phase space of
the extended lattice. Details of the migration process are
still under investigation [14, 30].
We conjecture that the size of avalanches J is propor-
tional to the size S of islands in the mixed phase space
found in the Poincaré section of the non-linear trimer. A
heuristic model [14] that mimics the hierarchical (`island-
over island') structure of a typical mixed phase space
leads us to a power law distribution P (S) ∼ S−α where
1 < α < 3. The lower bound comes from the requirement
of having an infinite number of islands (self-similar prop-
erty) while the upper-bound results from the requirement
that the total volume of the phase space be finite. To ver-
ify the above prediction for P (S) is a computationally
demanding task. Therefore we used a numerically more
convenient model: the kicked rotor which is a paradig-
matic model of mixed phase space dynamics [29]. Leav-
ing aside the technical details [14], we present in Fig. 3b
the outcome of our numerical calculations. The results
confirm the power law scaling of the island sizes over
more than three orders of magnitude thus confirming the
validity of our conjecture.
In conclusion, we have shown that there is a critical
regime of interatomic interactions, where particles are
ejected out of a leaky OL in scale free avalanches. The
observed power law distribution, is dictated by the hier-
archical structure of the mixed phase space. Our results
are quite universal and should be observable in many
other experimental realizations of the DNLSE including
molecular crystals, globular proteins and non-linear op-
tics.
3
METHODS
The simplest model that captures the dynamics of a
dilute gas of bosonic atoms in a deep OL with chemical
potential small compared to the vibrational level spac-
ing, is the Bose-Hubbard Hamiltonian. In the case of
weak interatomic interactions (superfluid limit) and/or a
large number of atoms per well (so that the total num-
ber of atoms N ∼ O(104 − 105) is much bigger than the
number of wells M), a further simplification is available
since the BECs dynamics admits a semiclassical mean
field description [13]. The resulting Hamiltonian is
H =
M∑
n=1
[U |ψn|4 +µn|ψn|2]− T2
M−1∑
n=1
(ψ∗nψn+1 + c.c.) (4)
where n is the well index, |ψn(t)|2 ≡ Nn(t) is the mean
number of bosons at well n, U = 4pi~2asVeff/m de-
scribes the interaction between two atoms on a single
site (Veff is the effective mode volume of each site, m is
the atomic mass, and as is the s-wave atomic scattering
length), µn is the well chemical potential, and T is the
tunneling amplitude. The "wavefunction amplitudes"
ψn(t) ≡
√
Nn(t) exp(−iφn(t)) can be used as conjugate
variables with respect to the Hamiltonian iH leading to
a set of canonical equations i∂tψn = ∂H/∂ψ∗n; i∂tψ∗n =
−∂H/∂ψn. Substituting (4) we get the DNLSE. To sim-
ulate the leaking process at the two edges, we supplement
the standard DNLSE with a local dissipation at the two
edges of the lattice. The resulting leaking DNLSE is [10]
i
∂ψn
∂τ
= (χ |ψn|2 + µ˜n)ψn − 12 [ψn−1(1− δn,1) + ψn+1(1− δn,M )]
− iγψn[δn,1 + δn,M ]; n = 1, · · · ,M (5)
where the normalized time is defined as τ = Tt, χ =
2U/T is the rescaled nonlinearity, µ˜n = µn/T is the
rescaled chemical potential and γ is the atom emission
probability describing atomic losses. It is useful to de-
fine the initial effective interaction per well i.e. Λ = χρ
where ρ = N(τ = 0)/M is the initial average density of
atoms in the OL. In our numerical experiments we have
used initial conditions with randomly distributed phases,
and an almost constant amplitude with only small ran-
dom fluctuations across the OL. We normalized the wave
functions such that N(τ = 0) = 1. The initial states
are first thermalized during a conservative (i.e. γ = 0)
transient period of, typically, τ = 500. The dissipation
at the lattice boundaries is switched on only after this
transient is completed, leading to a progressive loss of
atoms. We study the decay and the statistical properties
of N(τ) as a function of the parameter Λ. The results
reported in this Letter correspond to µ˜n = 0 and dissi-
pation rate γ = 0.2 which is within the experimentally
accessible range [10]. Nevertheless we have checked that
we get the same qualitative behavior for other values of
γ [14].
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