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Bo E' Sernelius, Dept' of Physics and Measurement Technology, Linkping University, SE581 83 Linkping

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The standard Fresnel coefficients may be used. Condition for modes between two half spaces ... The Fresnel coefficients can no longer be used ... – PowerPoint PPT presentation

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Title: Bo E' Sernelius, Dept' of Physics and Measurement Technology, Linkping University, SE581 83 Linkping


1
Bo E. Sernelius, Dept. of Physics and Measurement
Technology, Linköping University, SE-581 83
Linköping, Sweden
Full inclusion of spatial dispersion resolves the
controversy regarding the finite-temperature
Casimir-force between two metal plates.
  • QFEXT05

2
Outline of the talk
  • Neglect of spatial dispersion,
  • Derivation of the forces
  • Results
  • Nernst heat theorem
  • Inclusion of spatial dispersion
  • Derivation of the forces
  • Results
  • Nernst heat theorem
  • Conclusion

3
Spatial dispersion
  • To find the electromagnetic normal-modes of a
    system it is absolutely necessary to take the
    frequency dependence of the dielectric function
    into account.
  • In some situations it is also necessary to
    include the momentum-, or wave-vector-dependence,
    i.e., to take spatial dispersion into account.

4
Neglect of Spatial Dispersion
  • Then one may use the experimentally measured
    dielectric properties of the objects to find the
    normal modes of the system.
  • From these one finds the interaction energy and
    forces between the objects.
  • At zero temperature the energy is just the zero
    point energy of the normal modes.
  • At finite temperature also the occupation numbers
    affects the results.

5
How are the modes obtained?
  • One solves Maxwells equations in all regions and
    use the standard boundary conditions at all
    interfaces.
  • The parallel components of the E and H fields are
    continuous across the interfaces.
  • The normal components of the B and D fields are
    continuous across the interfaces.
  • The standard Fresnel coefficients may be used.

6
Condition for modes between two half spaces
7
Modes contributing to van der Waals and Casimir
forces
8
Modes between metal plates
9
Interaction energy
10
Interaction Potential between two Gold plates
11
Interesting region expanded
12
Energy correction factor in different
approximations
13
TM and TE integrands
14
Larger separation
15
Even larger separation
16
Temperature dependence of Entropy for modes
between two gold plates. The Nernst heat theorem
is obeyed!
17
Summands or integrands
18
The Nernst heat theorem, the third law of
thermodynamics.
  • The Nernst heat theorem is obeyed as long as
    there are any defects in the crystal.
  • This is of course the case in all real systems
  • For a perfect crystal without impurities and
    other lattice defects the Nernst heat theorem is
    not obeyed.
  • Why this is so is an academic question.
  • For Nernsts heat theorem to be fulfilled the
    Integrands have to be continuous functions of
    frequency at the small frequency end. The
    defect-less metal-crystal case has a TE integrand
    that is a step-function at zero frequency

19
Defect-less metal crystal
20
Spatial Dispersion
  • Taking spatial dispersion into account makes the
    calculations more involved.
  • The Fresnel coefficients can no longer be used
  • The experimentally obtained dielectric functions
    can no longer be used
  • One has to resort to theoretical dielectric
    functions
  • Both transverse and longitudinal versions are
    needed.
  • We use the RPA (random phase approximation) or
    Lindhard dielectric functions

21
Basics assumptions
  • The dielectric properties on each side of the
    interface is assumed to be valid all the way up
    to the interface.
  • We assume ideal interfaces, sharp with no
    defects.
  • This means that the in-plane momentum, k, is
    conserved. Thus k is a good quantum number for
    the modes.
  • For isotropic materials there is no preferred
    direction in the xy-plane
  • We arbitrarily choose the propagation of the
    mode to be in the x-direction.

22
  • The modes at an interface are characterized by
    the 2D (two-dimensional) wave vector, k, in the
    plane of the interface.
  • We let a general wave vector be denoted by q, and
    k is then the in-plane component.

23
Charge and current densities
  • The modes are associated with induced volume
    charge and current densities inside the objects
  • Induced two dimensional charge and current
    densities at the interfaces
  • The charge and current densities are not
    independent
  • They are coupled through the equation of
    continuity

24
Potentials in coulomb gauge
Fields from potentials
25
Assume a surface charge density at an interface
  • A time varying charge density is associated with
    a current density via the equation of continuity
  • Thus the charge density couples to a current
    density in the x- direction only

26
  • The electric fields associated with this mode are
    in the plane of incidence (xz-plane) and the
    magnetic fields are perpendicular to this plane.
  • The fields are p-polarized or TM-fields
    (Transverse Magnetic)
  • One could be led to believe that there are also
    modes associated with a Jy-component and with no
    accompanying induced charge density.
  • However, there are no such solutions to the
    Maxwell equations whose resulting fields obey the
    boundary conditions.

27
  • in the geometry with two parallel interfaces
    there are modes generated by coupled
    Jy-components at the two interfaces.
  • These modes are TE-modes with s-polarized fields.

28
Let us now return to our mode
  • The charge density gives rise to a scalar
    potential and
  • the current density to a vector potential.
  • Since we are working in Coulomb gauge, only the
    transverse part of the current contributes to the
    vector potential.
  • To get the transverse part we subtract the
    longitudinal part from the current density

29

30
Study a single interface
31
The B-field
32
In real space we have
33
g-functions
34
g-functions in vacuum
35
Gamma-functions
36
Conditions for modes at a flat interface
  • The modes at a single flat interface are
    TM-modes.
  • The magnetic field has only y-components while
    the electric field has both x- and z-components.
  • The condition for modes is expressed in terms of
    these g-functions.

37
Two parallel interfaces
  • At a single interface there is also a component
    of the current pointing in the y-direction, but
    this does not couple to the charge density and do
    not help in the formation of self-sustained
    fields.
  • Now if we have two interfaces these current
    components at the two interfaces may couple and
    give rise to a mode this is the TE-mode.
  • The scalar potential does not contribute to the
    fields in this case.

38
  • The TE fields are genuinely transverse in
    character and only the transverse dielectric
    function enters the relations.
  • The TM-modes on the other hand have both
    longitudinal and transverse character and both
    types of dielectric function enter the formalism.

39
Condition for modes between two interfaces
40
Interaction energy
41
Tilde-g-functions
  • The tilde over a g-function means the g-function
    calculated inside the medium minus the
    corresponding function calculated in vacuum.
  • The tilde versions of the g-functions were
    introduced since they represent faster converging
    integrals. To benefit from this the two integrals
    in each tilde version of a g-function should be
    combined into one.

42
TM and TE Integrands
43
Same figure but with linear scales
44
Expanded energy scale
45
  • We find that the drop in the TE-integrand is so
    close to the axis that the zero-temperature
    result is not affected.
  • For room-temperature the drop affects only the
    TE, n 0 term.
  • The integrands are continuous so the Nernst heat
    theorem is fulfilled even in absence of
    dissipation.

46
Results for different approximations
47
Why is the TE modes behaving as they do?
  • Let us look at GTE

48
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49
Integrand for the gb(k,w) function for w 0.
50
Integrand for the gb(k,w) function for k 0.01
51
Summary
  • I have presented the results for the force
    between two metal plates taking spatial
    dispersion into account.
  • One then needs theoretical dielectric functions.
  • I used the RPA or Lindhard dielectric functions,
    both transverse and longitudinal versions.
  • No fiddling around with asymptotic expansions.
  • In the results presented here no dissipation was
    assumed.
  • The same striking results as we obtained earlier
    when spatial dispersion was neglected but
    dissipation was included
  • The academic question involving the Nernst heat
    theorem for a system without defects was
    resolved.

52
References
  • The present work on spatial dispersion, Bo E.
    Sernelius, Phys. Rev. B 71, 235114 (2005).
  • Our previous work on dissipation M. Boström and
    Bo E. Sernelius, Thermal effects on the Casimir
    force in the 0.1-5 mm range, Phys. Rev. Lett. 84,
    4757 (2000) Bo E. Sernelius and M. Boström, 
    Dispersion forces between real metal plates at
    finite temperature and the Nernst heat theorem ,
    in Quantum Field Theory Under the Influence of
    External Conditions, Ed. K. A. Milton (Rinton
    Press, USA, 2004) M. Boström and Bo E.
    Sernelius,  Entropy of the Casimir effect between
    real metal plates, Physica A 339, 53 (2004).
  • Experimental paper by Lamoreaux S.K. Lamoreaux,
    Phys. Rev. Lett.78, 5 (1997).
  • If you want to read more about the modes Bo E.
    Sernelius, Surface Modes in Physics, Wiley-VCH
    2001.
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