Bose 2.2 User Manual Page 28

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operators
11
ˆa
k
and ˆa
k
, such that
ˆ
Ψ (r) =
X
k
φ
k
(r) ˆa
k
and
ˆ
Ψ(r) =
X
k
φ
k
(r) ˆa
k
, (2.11)
with
φ
k
(
r
) a set of single-particle states. Assuming a macroscopic population
N
of the
lowest lying single-particle state
φ
0
(such that
N
+ 1
' N
1) we can replace the
according operators by numbers [91], with
ˆa
0
=
ˆa
0
=
N
. We may then rewrite the field
operator in the form
ˆ
Ψ(r) =
N φ
0
(r) +
X
k>0
φ
k
(r) ˆa
k
def
=
N ψ(r ) + δ
ˆ
Ψ(r), (2.12)
where we have introduced the complex function
ψ
(
r
), defined by the expectation value
of the field operator
12
D
ˆ
Ψ(r)
E
=
Nψ
(
r
). The function
ψ
(
r
) has the meaning of an
order parameter and exhibits a well defined phase, which is spontaneously chosen at
the phase transition from the normal gas to a Bose-Einstein condensate [91]. Hence, the
phase transition to a BEC manifests itself by a broken gauge symmetry in the many-body
system. In the following, we will call ψ(r) the wave function of the condensate.
In general, the field operator is time-dependent with a time evolution described by the
Heisenberg equation,
i~
t
ˆ
Ψ(r, t) =
h
ˆ
Ψ,
ˆ
H
i
=
"
~
2
2m
2
+ V
ext
(r) +
Z
d
3
r
0
ˆ
Ψ (r
0
, t) V
(2)
int
(r r
0
)
ˆ
Ψ(r
0
, t)
#
ˆ
Ψ(r, t).
(2.13)
With the field operator given by Eq.
(2.12)
, and neglecting the fluctuations
δ
ˆ
Ψ
(
r
), we
obtain the time-dependent Gross-Pitaevskii equation (GPE) of a dipolar condensate
i~
t
ψ(r, t) =
~
2
2m
2
+ V
ext
(r)
+ gN |ψ(r, t)|
2
+ N
Z
d
3
r
0
V
0
dd
(r r
0
) |ψ(r
0
, t)|
2
ψ(r, t),
(2.14)
where we have inserted the two-body interaction potential
V
(2)
int
(
r r
0
), given by Eq.
(2.8)
.
Note that the DDI potential
V
0
dd
(
r r
0
) adds a non-local character to the Gross-Pitaevskii
equation. In contrast, the “standard” GPE of a purely contact interacting BEC depends
only on the local density n(r, t) = N |ψ(r, t)|
2
of the condensate.
11
The operators ˆa
k
and ˆa
k
obey the usual bosonic commutation relations
h
ˆa
α
, ˆa
β
i
= δ
α,β
, a
α
, ˆa
β
] = 0, and
h
ˆa
α
, ˆa
β
i
= 0.
12
We choose the function ψ(r) to be normalized to unity.
28
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