axel pelster 1. introduction 2. dipolar bose-einstein condensates...
TRANSCRIPT
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On the Dipolar Dirty Boson ProblemAxel Pelster
1. Introduction
2. Dipolar Bose-Einstein Condensates
3. Bose-Einstein Condensates with Weak Disorder
4. Dipolar Bose-Einstein Condensates with Weak Disorder
5. Summary and Outlook
1
-
1.1 Identical Quantum Particles
Bosons:
• integer spin
• symmetric wave function
Fermions:
• half-integer spin
• anti-symmetric wave function
2
-
1.2 Time-of-Flight Absorption Pictures
JILA (1995): 8737Rb , N=20 000 , ω1 = ω2 = ω3/√8 = 2π× 120 Hz
3
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1.3 Periodic Table of Elements
4
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On the Dipolar Dirty Boson ProblemAxel Pelster
1. Introduction
2. Dipolar Bose-Einstein Condensates
3. Bose-Einstein Condensates with Weak Disorder
4. Dipolar Bose-Einstein Condensates with Weak Disorder
5. Summary and Outlook
5
-
2.1 Trapping and Interaction Potentials
• Harmonic trap and aspect ratios:
Utrap(x) =M
2
(ω2xx
2 + ω2yy2 + ω2zz
2), λx =
ωzωx, λy =
ωzωy
• Interaction potential: Vint(x) = gδ(x) + Vdd(x)
g =4π~2asM
, Vdd(x) =Cdd
4π|x|3[1− 3 cos2 θ
]
-�
Repulsion
6
?
Attraction�
��
��
��
��
θ
6
-
2.2 Magnetic versus Electric Dipolar Systems
• Magnetic systems:– Interaction strength: CBdd = µ0m
2, with m ∼ 1 to 10 µB– Realized samples
Boson: 52Cr Griesmaier et al., PRL 94, 160401 (2005)Boson: 87Rb Vengalattore et al., PRL 100, 170403 (2008)Fermion: 53Cr Chicireanu et al., PRA 73, 053406 (2006)Both: Dy Lu et al., PRL 104, 063001 (2010); PRL 107, 190401 (2011)
– Observed effects: magnetostriction (Cr), Bose-nova explosion (Cr)
• Electric systems:– Interaction strength: CEdd = 4πd
2, with d ∼ 1 Debye– Realized samples
Fermion: 40K87Rb Ospelkaus et al., Science 32, 231 (2008)Boson: 41K87Rb Aikawa et al., NJP 11, 055035 (2009)
– Observed effects: thermalization (40K87Rb)
• Ratio: CBdd/CEdd ≈ 10−47
-
2.3 Field Theoretical Description
• Hamilton operator: Ĥ = Ĥ0 + Ĥint
• Free Hamiltonian:
Ĥ0 =
∫
d3x Ψ̂†(x, t)
[
−~2∇22M
+ Utrap(x)
]
Ψ̂(x, t)
• Interaction Hamiltonian:
Ĥint =1
2
∫
d3x
∫
d3x′ Ψ̂†(x, t)Ψ̂†(x′, t)Vint (x− x′) Ψ̂(x′, t)Ψ̂(x, t)
• Bosonic commutation relations:[
Ψ̂(x, t), Ψ̂†(x′, t)]
= δ(x−x′),[
Ψ̂†(x, t), Ψ̂†(x′, t)]
=[
Ψ̂(x, t), Ψ̂(x′, t)]
= 0
• Bogoliubov prescription:
Ψ̂(x, t) → Ψ(x, t) + δψ̂(x, t), Ψ̂†(x, t) → Ψ∗(x, t) + δψ̂†(x, t)
8
-
2.4 Gross-Pitaevskii Theory
• Heisenberg equation:
i~∂
∂tΨ̂(x, t) =
[
Ψ̂(x, t), Ĥ]
• Zeroth order: Ψ̂(x, t) → Ψ(x, t), Ψ̂†(x, t) → Ψ∗(x, t)
• Gross-Pitaevskii equation:
i~∂Ψ(x, t)
∂t=
[
−~2∇22M
+Utrap(x)+
∫
d3x′Ψ∗(x′, t)Vint(x−x′)Ψ(x′, t)]
Ψ(x, t)
• Action principle:
δ
∫
d3x
t2∫
t1
dtΨ∗(x, t)
[
i~∂
∂t−H(x, t)
]
Ψ(x, t) = 0
• Action extremalization through suitable ansatz for Ψ(x, t)
9
-
2.5 Bogoliubov-de Gennes Theory (Stationary)
• Bogoliubov transformation:
δψ̂(x) =∑
ν
′ [Uν(x)α̂ν + V∗ν(x)α̂†ν
], δψ̂†(x) =
∑
ν
′ [U∗ν (x)α̂†ν + Vν(x)α̂ν
]
• Diagonalized Hamiltonian:
Ĥ ′ = E′G +∑
ν
′ενα̂
†να̂ν
• Bogoliubov-de Gennes equations:
[εν −HFl(x)]Uν(x) =∫
d3x′Vint
(
x−x′)[
Ψ(x′)Ψ(x)Vν(x
′)+Ψ
∗(x
′)Ψ(x)Uν(x
′)]
− [εν +HFl(x)]Vν(x) =∫
d3x′Vint
(
x−x′)[
Ψ∗(x
′)Ψ
∗(x)Uν(x
′)+Ψ(x
′)Ψ
∗(x)Vν(x
′)]
HFl(x) = −~2∇22M
+ Utrap(x)− µ+∫
d3x′Ψ∗(x′)Vint (x− x′)Ψ(x′)
10
-
2.6 Trapped Dipolar Bose Gases: MF Theory
• Action:
A[n0, χ] = −∫
dt
∫
d3xn0(x, t)
{
M
[
χ̇(x, t) +∇χ(x, t)2
2
]
+ ETF(x, t)}
ETF(x, t) = Utrap(x) +1
2gn0(x, t) +
1
2
∫
d3x′ Vdd(x− x′)n0(x′, t)
• Variational ansatz:
n0(x, t) = n0(t)
[
1−∑
i
x2iR2i (t)
]
, χ(x, t) =1
2
∑
i
αi(t)x2i
• Equations of motion:MR̈i = −
∂
∂RiEMF (Rx, Ry, Rz) , ǫdd =
Cdd3g
EMF (Rx, Ry, Rz) =M
2
∑
j
R2jω2j +
15Ng/(4π)
RxRyRz
[
1− ǫddf(RxRz,RyRz
)]
O’Dell et al., PRL 92, 250401 (2004) ; Eberlein et al., PRA 71, 033618 (2005)
11
-
2.7 Anisotropy Function
0
5
10
0
5
10
-2
-1
0
1
f(x, y)
x
y
0 2 4 6 8 10 12 14-2.0
-1.5
-1.0
-0.5
0.0
0.5
1.0
x
fs(x)
• Shift of critical temperature:Glaum, Pelster, Kleinert, and Pfau, PRL 98, 080407 (2007)
Glaum and Pelster, PRA 76, 023604 (2007)
• Dipolar Fermi Gas:Lima and Pelster, PRA 81, 021606(R) (2010); PRA 81, 063629 (2010)
12
-
2.8 Trapped Dipolar Bose Gases: MF Results• Stability diagram and aspect ratio:
0 1 2 3 4 5 60
2
4
6
8
10
ǫdd
Unstable
Metastable
Stable
λx = λy0 5 10 15 20 25 30
0
1
2
3
4
5
6R̃xλxR̃z
ǫbdd
λx = λy
O’Dell et al., PRL 92, 250401 (2004) ; Eberlein et al., PRA 71, 033618 (2005)
• Low-lying oscillations and time-of-flight:
0 1 2 3 40
2
4
6
8
rq
Ωrq
+
Ω+
−
Ω−
ǫbdd
λx = λy = 4
0 2 4 6 8 10 12 140
0.5
1
1.5
2
2.5
3
3.5
4
time of flight [ms]
aspect ra
tio
/RyRz
z
y
m Bm, along :B y
m, along :B zm B
Bismut et al., PRL 105, 040404 (2010) Stuhler et al., PRL 95, 150406 (2005)
13
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2.9 Trapped Dipolar Bose Gases: Beyond MF
• Semiclassical approximation:
εν → ε (x,k) , Uν → U (x,k) eik·x, Vν → V (x,k) eik·x
• BdG equations:[
ε (x, k) − ~2k2
2M
]
U (x, k) =√
n0(x)
∫
d3x′ Vint(
x−x′)
√
n0(x′)
[
V(x′, k)+U (x′, k)]
eik·
(
x′−x)
−[
ε (x, k) +~2k2
2M
]
V(x, k) =√
n0(x)
∫
d3x′Vint
(
x−x′)√
n0(x′)
[
V(x′, k)+U (x′, k)]
eik·
(
x′−x)
• Local density approximation for exchange term:√
n0(x)
∫
d3x′[
gδ(
x−x′)
+Vdd(
x−x′)]
√
n0(x′)q(
x′, k
)
eik·(x′−x)
≈ ξ (x, k) q (x, k)
with ξ (x,k) = gn0(x)[1 + ǫdd
(3 cos2 θ − 1
)]
Timmermans, Tommasini, and Huang, PRA 55, 3645 (1997)
14
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2.10 Trapped Dipolar Bose Gases: Beyond MF
• Bogoliubov spectrum:
ε2 (x,k) =
[~2k2
2M+ ξ (x,k)
]2
− ξ2 (x,k)
• Bogoliubov amplitudes:
U (x,k)2 − 1 = V (x,k)2 = 12
[~2k2
2M + ξ (x,k)
ε (x,k)− 1
]
• Depletion: ∆NN
=5√π
8Q3(ǫdd)
√
n(0)a3s
• Energy: ∆E = 5√π
8gn(0)Q5(ǫdd)
√
n(0)a3s0.0 0.2 0.4 0.6 0.8 1.0
1.0
1.5
2.0
2.5
Ql(x)
x
• Beyond mean-field equations of motion:
MR̈i = −∂
∂Ri
[
EMF (Rx, Ry, Rz) +7
N∆E (Rx, Ry, Rz)
]
15
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2.11 Trapped Dipolar Bose Gases: Beyond MF Results
• Aspect ratio in equilibrium:
κ ≡ RxRz = κ0 (1 + δκ)
δ̃κ = 105√π
32
√
a3sn(0) ≈ 0.06 0.0 0.5 1.0 1.5 2.0 2.5 3.005
10
15
20δκ
δ̃κ
ǫb
dd= 0.97
ǫb
dd= 0.95
ǫb
dd= 0.8
λx = λy
• Low-lying oscillations: typical for Cr
Ω = Ω0 (1 + δΩ)
δ̃Ω = 63√π
128
√
a3s n(0) ≈ 0.01 0 1 2 3 4 5-0.20.0
0.2
0.4
0.6
0.8
1.0
1.2δΩδ̃Ω ǫbdd = 0
ǫbdd = 0.16, as = 100a0
MonopoleQuadrupole
λx = λy
• Time-of-flight: expected for Dy
κ(t) =Rx(t)Rz(t)
0 5 10 15 200.0
0.2
0.4
0.6
0.8
1.0κ(t)
λx = λy = 0.5
ǫbdd
= 0.9, as = 150a0
Quantum CorrectedMean Field
ωxt
Lima and Pelster, PRA 84, 041604(R) (2011); arXiv:1111.0900
16
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On the Dipolar Dirty Boson ProblemAxel Pelster
1. Introduction
2. Dipolar Bose-Einstein Condensates
3. Bose-Einstein Condensates with Weak Disorder
4. Dipolar Bose-Einstein Condensates with Weak Disorder
5. Summary and Outlook
17
-
3.1 Overview of Set-Ups
• Superfluid Helium in Porous Media: persistence of superfluidityReppy et al., PRL 51, 666 (1983)
• Laser Speckles: controlled randomnessBilly et al., Nature 453, 891 (2008)
• Wire Traps: undesired randomnessKrüger et al., PRA 76, 063621 (2007)
Fortàgh and Zimmermann, RMP 79, 235 (2007)
• Localized Atomic Species: theoretical suggestionGavish and Castin, PRL 95, 020401 (2005)
• Incommensurate Lattices: quasi-randomnessRoati et al., Nature 453, 895 (2008)
18
-
3.2 Laser Speckles
global condensate vanishesLye et al., PRL 95, 070401 (2005)
19
-
3.3 Wire Trap
0 100 200
−5
0
+5
Longitudinal Position (µm)
∆B/B
(10
−5 )
−20 0 20∆B/B (10−6)
arbi
trar
y un
its
Distance: d = 10 µm Wire Width: 100 µm
Magnetic Field: 10 G, 20 G, 30 G Deviation: ∆B/B ≈ 10−4
Krüger et al., PRA 76, 063621 (2007)
Fortàgh and Zimmermann, RMP 79, 235 (2007)
20
-
3.4 Model System
Action of a Bose Gas:
A =∫ ~β
0
dτ
∫
d3x
{
ψ∗[
~∂
∂τ− ~
2
2M∆+U (x) + V (x)− µ
]
ψ +g
2ψ∗2ψ2
}
Properties:
• harmonic trap potential: U(x) = M2ω2x2
• disorder potential: V (x)
V (x1) = 0 , V (x1)V (x2) = R(x1 − x2) , . . .
• chemical potential: µ
• repulsive interaction: g = 4π~2a
M
• periodic Bose fields: ψ(x, τ + ~β) = ψ(x, τ)
21
-
3.5 Grand-Canonical Potential
Aim:
Ω = − 1βlnZ
Z =∮
DψDψ∗ e−A[ψ∗,ψ]/~
Problem:
lnZ 6= lnZ
Solution: Replica Trick
Ω = −1β
limN→0
ZN − 1N
22
-
3.6 Replica Trick
Disorder Averaged Partition Function:
ZN =∮
{N∏
α′=1
D2ψα′
}
e−∑Nα=1 A([ψ∗α,ψα])/~ =
∮{
N∏
α=1
D2ψα
}
e−A(N)/~
Replicated Action:
A(N) =∫
~β
0
dτ
∫
dDx
N∑
α=1
{
ψ∗α(x, τ)
[
~∂
∂τ− ~
2
2M∆ + U(x) − µ
]
ψα(x, τ)
+g
2|ψα(x, τ)|4
}
+∞∑
n=2
1
n!
(−1~
)n−1 ∫ ~β
0
dτ1 · · ·∫ ~β
0
dτn
∫
dDx1 · · ·∫
dDxn
×N∑
α1=1
· · ·N∑
αn=1
R(n)
(x1, . . . , xn)∣
∣ψα1(x1, τ1)∣
∣
2 · · · |ψαn(xn, τn)|2
=⇒ Disorder amounts to attractive interaction for n = 2=⇒ Higher-order disorder cumulants negligible in replica limit N → 0
23
-
3.7 Condensate Density
Assumptions:
homogeneous Bose gas: U(x) = 0
δ-correlated disorder: R(x) = Rδ(x)
Bogoliubov Theory:
background method: ψα(x, τ) = Ψα + δψα(x, τ)
replica symmetry: Ψα =√n0
Result: n0 = n−8
3√π
√an0
3 − M2R
8π3/2~4
√n0a
Huang and Meng, PRL 69, 644 (1992)
Falco, Pelster, and Graham, PRA 75, 063619 (2007)
24
-
3.8 Superfluid Density
Galilei Boost:
∆A =∫ ~β
0
dτ
∫
d3xψ∗(x, τ)u~
i∇ψ(x, τ)
dΩ = −S dT − p dV −N dµ− p du
p = − ∂Ω(T, V, µ,u)∂u
∣∣∣∣T,V,µ
=MV nn u+ . . .
Result: ns = n− nn = n−4
3
M2R
8π3/2~4
√n0a
Huang and Meng, PRL 69, 644 (1992)
Falco, Pelster, and Graham, PRA 75, 063619 (2007)
25
-
3.9 Collective Excitations
Typical Values:
Inguscio et al., PRL 95, 070401 (2005)
ξ = 10 µmRTF = 100 µmlHO = 10 µm
}
ξ̃ =ξRTF
l2HO√2≈ 7
~�
Æ! 0(�)=Æ!0(0)
54321010:80:60:40:20
n = 0, l = 1
n = 0, l = 2
=⇒ Disorder effect vanishes in laser speckle experiment
Improvement:
laser speckle setup with correlation length ξ = 1 µm
Aspect et al., NJP 8, 165 (2006)
=⇒ Disorder effect should be measurableFalco, Pelster, and Graham, PRA 76, 013624 (2007)
26
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On the Dipolar Dirty Boson ProblemAxel Pelster
1. Introduction
2. Dipolar Bose-Einstein Condensates
3. Bose-Einstein Condensates with Weak Disorder
4. Dipolar Bose-Einstein Condensates with Weak Disorder
5. Summary and Outlook
27
-
4.1 Disorder Induced Depletions
• Condensate:
n− n0n
=
∫d3k
(2π)3R(k)
[~2k2/2M + 2nVint(k)]2 + . . .
• Superfluid:
nδij − nS,ijn
=
∫d3k
(2π)34R(k)kikj
k2 [~2k2/2M + 2nVint(k)]2 + . . .
• Isotropy: Vint(k) = Vint(|k|) and R(k) = R(|k|) yield
n− nS =4
3(n− n0)
28
-
4.2 Specialization
• Dipoles polarized along z-direction:
Vint(k) = g[1 + ǫdd
(3 cos2 θ − 1
)]
• Relative interaction strength:
ǫdd =Cdd3g
, Cdd =
{µ0m
2 magnetic dipoles4πd2 electric dipoles
• Gaussian correlated disorder:
R(k) = Re−σ2k2
29
-
4.3 Condensate Depletion
n− n0 = nHM f(
ǫdd,σ
ξ
)
Coherence length: ξ =
√
~2
4Mng
Huang-Meng depletion: nHM =(M
2π~2
)32√
π
2gnR
00.5
11.5
22.5
3 00.2
0.40.6
0.810
0.5
1
1.5
2
σξ
ǫdd
f(
ǫdd,σξ
)
0
0.4
0.8
1.2
1.6
2
Krumnow and Pelster, PRA 84, 021608(R) (2011)
30
-
4.4 Superfluid Depletion
n− nS = nHM
f⊥(
ǫdd,σξ
)
0 0
0 f⊥(
ǫdd,σξ
)
0
0 0 f||(
ǫdd,σξ
)
00.5
11.5
22.5
3 00.2
0.40.6
0.810
0.2
0.4
0.6
0.8
1
1.2
1.4
σξ
ǫdda)
f||
(
ǫdd,σξ
)
00.20.40.60.811.21.4
00.5
11.5
22.5
3 00.2
0.40.6
0.810
0.5
1
1.5
2
2.5
3
σξ
ǫddb)
f⊥
(
ǫdd,σξ
)
00.511.522.53
Krumnow and Pelster, PRA 84, 021608(R) (2011)
=⇒ Finite localization timeGraham and Pelster, IJBC 19, 2745 (2009)
31
-
4.5 Hydrodynamic Theory
• Two-fluid model: n = nS + nN , j = nSvS + nN vN︸︷︷︸=0
• Continuity equation: ∂∂tn+∇j = 0
• Euler equation: M ∂∂t
vS +∇(
µ+1
2Mv2S
)
= 0
• Linearization around equilibrium:nS = nS,eq + δnS(x, t) , vS = δvS(x, t)
n = neq + δn(x, t) , µ = µ (neq) +∂µ
∂n
∣∣∣∣eq
δn(x, t)
• Wave equation:
∂2
∂t2δn(x, t)− 1
M
∂µ
∂n
∣∣∣∣eq
∇[
nS,eq(x)∇δn(x, t)]
= 0
32
-
4.6 Speed of Sound
• Delta correlated disorder and dipole-dipole interaction:
c2(ǫdd, ϑ) =ng
M
[3ǫdd cos
2 (ϑ) + 1− ǫdd]+nHMg
Ms(ǫdd, ϑ)
• Special case of contact interaction: s(0, ϑ) = 53Giorgini, Pitaevskii, and Stringari, PRB 49, 12938 (1994)
00.2
0.40.6
0.81
−π −π/20
π/2 π
00.20.40.60.8
11.21.41.61.8
ǫdd
a) ϑ
c0(ǫdd,ϑ)√ng/m
0
0.4
0.8
1.2
1.6
00.2
0.40.6
0.81
−π −π/20 π/2
π
-1
0
1
2
3
ǫdd
b) ϑ
s (ǫdd, ϑ)
-10123
Krumnow and Pelster, PRA 84, 021608(R) (2011)
=⇒ Measurable via Bragg spectroscopy
33
-
On the Dipolar Dirty Boson ProblemAxel Pelster
1. Introduction
2. Dipolar Bose-Einstein Condensates
3. Bose-Einstein Condensates with Weak Disorder
4. Dipolar Bose-Einstein Condensates with Weak Disorder
5. Summary and Outlook
34
-
5.1 Summary
• Frozen Disorder Potential :arises both artificially (laser speckles) or naturally (wire trap)
• Bosons:local condensates in minima + global condensate + thermally excited
• Localization Versus Transport: disorder reduces superfluidity
• Phase Diagram: yet unknown for strong disorderNavez, Pelster, and Graham, APB 86, 395 (2007)
Graham and Pelster, IJBC 19, 2745 (2009)
• Anisotropic superfluidity at zero temperature:delicate interplay between isotropic disorder and dipolar interaction−→ characteristic direction dependent sound velocity−→ possible experimental detection: Bragg spectroscopy
• Quantum and thermal fluctuations necessitate 3-fluid model
35
-
5.2 Optical LatticesQuantum Phase Transition:
Greiner, Mandel, Esslinger, Hänsch, and Bloch, Nature 415, 39 (2002)
Theoretical Description:
• Bose-Hubbard Hamiltonian:ĤBH = −t
∑
〈i,j〉â†i âj +
∑
i
[U
2n̂i(n̂i − 1)− µn̂i
]
, n̂i = â†i âi
• Landau Theory: dos Santos and Pelster, PRA 79, 013614 (2009)• Ginzburg-Landau Theory:
Bradlyn, dos Santos, and Pelster, PRA 79, 013615 (2009)
36
-
5.3 Quantum Phase Diagram ( T = 0,D = 3)
• Blue line: Strong-coupling, Freericks and Monien, PRB 53, 2691 (1996)• Error bar: Extrapolated strong-coupling series• Black line: Mean-field theory, Fisher et al., PRB 40, 546 (1989)• Red line: Landau theory, dos Santos and Pelster, PRA 79, 013614 (2009)• Blue dots: QMC data, Capogrosso-Sansone et al., PRB 75, 134302 (2007)
Numerical extension of Landau theory to higher hopping orde rs:Teichmann et al., PRB 79, 224515 (2009)
=⇒ Convergence of hopping expansion for Landau theory37
-
5.4 Excitation Spectra near Phase Bouncary
Grass, dos Santos, and Pelster, PRA 84, 013613 (2011)
Bragg spectroscopy: Bissbort et al., PRL 106, 205303 (2011)
38
-
5.5 Disordered Bosons in LatticeBose-Hubbard Hamilton Operator:
ĤBH = −t∑
â†i âj +∑
i
[U
2n̂i(n̂i − 1) + (ǫi − µ) n̂i
]
• = ∏i∫ +∞−∞ • p(ǫi) dǫi , p(ǫi) =
{1/∆ ; ǫi ∈ [−∆/2,+∆/2]0 ; otherwise
Mean-Field Phase Diagram:
0 1 2
0.05
0.1
0.15
0 1 2
0.05
0.1
0.15
µ/Uµ/U
2dt/U2dt/U
MIMI
T = 0∆/U = 0.5
SF
0 1 2
0.05
0.1
0.15
0 1 2
0.05
0.1
0.15
SF
MIMIµ/Uµ/U
2dt/U2dt/U
BGBG
kT/U = 0.01∆/U = 0.5
Krutitsky, Pelster, and Graham, NJP 8, 187 (2006)
Stochastic Mean-Field Theory: Bissbort and Hofstetter, EPL 86, 50007 (2009)
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5.6 Acknowledgement
Postdocs:
• Aristeu Lima (DFG)• Ednilson Santos (FAPESP)
PhD students:
• Javed Akram (DAAD)• Hamid Al-Jibbouri (DAAD)• Mahmoud Ghabour• Tama Khellil (DAAD)• Mohamed Mobarek (Egyp. Gov.)• Tao Wang (CSC)
Diploma students:
• Max Lewandowski (Potsdam)• Tobias Rexin (Potsdam)• Falk Wächtler (Potsdam)
Bachelor students:
• Tomasz Checinski (Bielefeld)• Christian Krumnow (FU Berlin)• Moritz von Hase (FU Berlin)• Carolin Wille (FU Berlin)• Nikolas Zöller (FU Berlin)
Volkswagen: Bakhodir Abdullaev , Abdulla Rakhimov (Tashkent)DAAD: Antun Balaz, Vladimir Lukovic, Branko Nikolic (Belgrade)Mentors: Robert Graham (Duisburg-Essen), Hagen Kleinert (FU Berlin)
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5.7 Announcement
Wilhelm and Else Heraeus Seminar
Quo Vadis BEC? IV
organized by Carlos S á de Melo and Axel Pelster
Physikzentrum, Bad Honnef
August 21 – 25, 2012
applications possible at the beginning of 2012:http://users.physik.fu-berlin.de/˜pelster
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