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8/12/2019 Slides - Piasecki, Jarosaw
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CASIMIR FORCES INDUCED BYBOSE-EINSTEIN CONDENSATION
Jarosaw Piasecki
Institute of Theoretical Physics
Faculty of Physics
University of Warsaw
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MOTTO
Tis much better to do a little with certainty
& leave the rest for others that come after,
than to explain all things by conjecture
without making sure of any thing.
Isaak Newton
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HENDRIK BRUGT GERHARD
CASIMIR (1909 - 2000)
H. B. G. Casimir
"On the attraction between two perfectly conductingplates"Proc. K. Ned. Akad. Wet. 51, 793-795 (1948).
cr4
2
240
H. B. G. Casimir, D. Polder
"The influence of retardation on the London-van derWaals forces"Phys. Rev. 73, 360-372 (1948).
U(r) = 12
r723c
4KMMF, 08.11. 2012 p. 3/21
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TYPES OF THE CASIMIR EFFECT
electromagnetic
in quantum field theory
in particle physics
in cosmologyin critical phenomena
dynamical Casimir effect
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STATING THE PROBLEM:
Derive the Casimir effect in an imperfect (interacting) Bose
gas filling the volume contained between two infiniteparallel plane walls.Hamiltonian of the imperfect Bose gas:
H=H0+ aV
N2
2
H0=kinetic energy (perfect gas Hamiltonian)a/V >0=repulsive mean-field interaction per pair ofbosonsV =volume occupied by the system.H is superstable!
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METHOD OF ANALYSIS
Bose gas occupies volumeV =L2Dof a rectangular box
with linear dimensionsL LD.Ddenotes the distance between twoL Lsquare walls.The excess grand canonical free energy per unit wall areais defined by
s(T , D , ) = limL
(T , L , D , )
L2
D b(T, )
whereb(T, )denotes the grand canonical potential perunit volume evaluated in the thermodynamic limit.The Casimir force equals
F(T , D , ) = s(T , D , )D
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BOUNDARY CONDITIONS
One-particle kinetic energy(k) = (k2x+k2y+k
2z)
2/2m
z-axis perpendicular toL Lwallsperiodic
kz =2
D
nz, nz = 0,
1,
2,...
Dirichlet
kz =
Dnz, nz = 1, 2,...
Neumann
kz =
Dnz, nz = 0, 1, 2,...
kx, ky -periodic b.c.
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IMPORTANT RELATION
Grand canonical potential
(T , L , D , ) = kBTln (T , L , D , )(T , L , D , )is related to the analytic continuation of theperfect gas partition function0 by
(T , L , D , ) = exp
L2D
2a 2
L2D
2a
(i) +ii
dt exp
L2D
a
t2
2 t
0(T , L , D , t)
(
-
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BULK PROPERTIES OF THE
IMPERFECT BOSE GAS
The bulk grand canonical free-energy density
b(T, ) = limL
1L3
kBT ln(T,L,L,) = p(T, )
can be calculated with the use of the steepest descent
method.If < c=an0,c
p(T, ) =
1
2 an2
(T, ) +p0(T, an(T, ))wheren(T, )is the unique solution of the equation
n=n0(T, an)KMMF, 08.11. 2012 p. 9/21
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BULK PROPERTIES OF THE
IMPERFECT BOSE GAS
If > c=an0,c
p(T, ) =2
2a+p0(T, 0)
In the two-phase region
n=
a
and the density of condensate is equal to
a n0,c
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CASIMIR FORCE: PERIODIC
BOUNDARY CONDITIONS
The steepest descent method yields the asymptotic form ofthe excess free energy density. The Casimir force in theone-phase region near the condensation point equals
F(T , D , )
kBT
=
1
D3
[2(x)
x (x) ]
with
(x) =
n=1
1 + 2nx
n3 exp(
2nx)
x= D
per, per = =
anc(anc
)
21/2
(3/2)
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CASIMIR FORCE IN THE PRESENCE
OF CONDENSATE
In the two-phase region (in the presence of condensate)one observes a power-law decay
F(T , D , )kBT =2(3) 1D3 , > anc
exactly the same, and with the same amplitude as in the
perfect Bose gas.
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IMPERFECT AND PERFECT GAS:
COMPARING CRITICAL BEHAVIOR
Divergence of the range of exponential forces at theapproach to condensation:
imperfect (mean-field) Bose gas
(anc )1
perfect Bose gas
0 ()1/2
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ONE PARTICLE DENSITY MATRIX
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ONE-PARTICLE DENSITY MATRIX
FOR=
/KBT >0
THE CASE OF A PERFECT GAS:
< x2|1|x1 >=F(|x2 x1|)
3F(x) =
j=1
1
j3/2
exp j x2
j2
=
xexp2
x
+
s=1
xexp A
+(s)x
2cos A(s)
x
with
A(s) =
2(2 + 42s2)1/4 1
(2 + 42s2)1/2 .
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BULK CORRELATION LENGTH AND
RANGE OF CASIMIR FORCES
Correlation function of a perfect Bose gas
6[n2(r; , T) n2] = j=1
1
j3/2exp
j r
2
j2
2
= /kBT, =h/
2mkBT
Large distance (r ) asymptotics
6[n2(r; , T) n2] =
r
2
exp
r
0()
.
0() = h4
2m1 = range of Casimir force !
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ELEMENTS OF CALCULATION
Knowledge of the asymptotic behavior of Bose functions
gr() =q=1
exp(q)qr
when 0
g1/2() =
, g1/2() = 1
permits to evaluate derivatives of the density with respectto the chemical potential at the condensation point=imp,c=nca.
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BULK CORRELATIONS AND
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BULK CORRELATIONS AND
CASIMIR FORCES
=range of Casimir forces.=range of bulk correlations
perfect gas
0,periodic= 20,Dirichlet = 20,Neumann=0
critical exponent= 1/2
imperfect (mean field) gasperiodic = 2Dirichlet = 2Neumann= 2
critical exponent= 1
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SOME REFERENCES
M. Krech, Casimir Effect in Critical Systems, World Scientific,
Singapour (1994).G. Brankov, N.S. Tonchev, and D. M. Danchev, Theory ofCritical Phenomena in Finite-Size Systems, World Scientific,Singapore (2000).
L. Palova, P. Chandra, P. Coleman, The Casimir effect fromcondensed matter perspective, Am. J. Phys. 77(2009) 1055.
E. Elizalde, A, Romeo, Essentials of the Casimir effect and itscomputation, Am. J. Phys. 59(1991) 711.
Ph.A. Martin, P.R. Buenzli, The Casimir effect,Acta.Phys.Polon.B 37(2006) 2503-2559.
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SOME REFERENCES
Ph. A. Martin and V. A. Zagrebnov, The Casimir effect
for the Bose-gas in slabs, EPL 73, 15 (2006).
M. Napirkowski and J. Piasecki , Phys. Rev. E 84,061105 (2011).
M. Napirkowski and J. Piasecki , J. Stat. Phys. 147,1145 (2012).
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