Bose 2.2 User Manual Page 103

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time (ms)
0
0 ms 0.1 ms 0.2 ms 0.4 ms0.3 ms
0
0
0 0.5 1 1.5
10
20
10
20
30
1
2 3
0.5 ms
(a) (c)
(b)
B
Fig. 6.1, Collapse dynamics of a dBEC in a single round trap:
(a) Experimental
sequence to induce the collapse. Both the programmed ramp (red line) of the
scattering length
a
(
t
) and the real ramp taking into account the eddy currents
(blue line) are shown. The stability threshold is
a
crit
= (15
±
3)
a
0
[35], the
uncertainty being illustrated by the grey zone. (b) Time evolution of the remnant
BEC for different values of
t
hold
: the upper row corresponds to experimental
images taken after TOF and the lower row shows the results of numerical
simulations. (c) Evolution of the atom number in the remnant BEC after TOF
as a function of
t
hold
, extracted from the measurements (dots) and from the
simulations (line). All figures are taken from Ref. [36].
Pitaevskii equation. A crucial point in the simulations is to include the three-body atom
losses that occur during the collapse dynamics. Else, the condensate only contracts to a
single point of the numerical grid and no collapse dynamics can be observed. With the
empirically chosen three-body loss rate
96
L
3
= 2 · 10
40
m
6
/s, the simulations reproduce
both the
d
-wave density pattern after TOF (see the lower row in Fig. 6.1(b)) and the
measured evolution of the atom number N
BEC
(t
hold
) shown in Fig. 6.1(c).
The simulations allow furthermore to reconstruct the in-trap time evolution of the dBEC
after the stability threshold has been passed: First, the dBEC contracts radially, forming
a very thin cigar along the direction of the external magnetic field. Then, strong atom
losses occur at the center of the cloud, such that the centripetal force of the dipoles
weakens and the BEC finally explodes in the radial directions (
x, y
) due to the surplus of
the quantum pressure. Since the atoms at both ends of the cigar are not involved in the
96
The three-body loss rate L
3
enters the Gross-Pitaevskii equation, as we show in section 6.2.3.
103
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