On the polarizability and capacitance of the cubePolarizability Superellipse and Square The cube...
Transcript of On the polarizability and capacitance of the cubePolarizability Superellipse and Square The cube...
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
On the polarizability and capacitance of the cube
Johan Helsing
Lund University
Talk at FACM ’12, NJIT, May 19, 2012
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Acknowledgement
The work presented has in part been carried out in cooperationwith or supported by:
Alexandru Aleman
Anders Karlsson
Ross McPhedran
Graeme Milton
Rikard Ojala
Karl-Mikael Perfekt
Daniel Sjoberg
the Swedish Research Council
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
A dielectric inclusion in a dielectric medium
νrS
e
VE
ǫ2 ǫ1
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
The electrostatic boundary value problem
U(r) continuous
limr→∞
∇U(r) = e
∆U(r) = 0
∆U(r) = 0
ǫ2∂
∂νr
U int(r) = ǫ1
∂
∂νr
Uext(r)
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
The polarizability α is given by
α = (ǫ2 − ǫ1)
∫
V
(e · ∇U(r))dr .
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
The polarizability α is given by
α = (ǫ2 − ǫ1)
∫
V
(e · ∇U(r))dr .
When does α exist? For what ǫ1, ǫ2 does the cube have an α?
Is it difficult to compute α?
Does a small rounding of a corner correspond to a small relativeperturbation of input data?
Is it important to compute α?
How high accuracy should one demand of a fast α-solver?
Are there many failed attempts to compute α for non-smooth S inthe literature?
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Equivalent integral equation formulation
Ansatz which solves the PDE and takes care of r → ∞:
U(r) = e · r +
∫
S
G (r , r ′)ρ(r ′)dσr ′ ,
where ρ(r) is an unknown layer density.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Equivalent integral equation formulation
Ansatz which solves the PDE and takes care of r → ∞:
U(r) = e · r +
∫
S
G (r , r ′)ρ(r ′)dσr ′ ,
where ρ(r) is an unknown layer density. Insertion of U(r) in theboundary condition at S :
(ǫ2 + ǫ1)
(ǫ2 − ǫ1)ρ(r) + 2
∫
S
∂
∂νrG (r , r ′)ρ(r ′)dσr ′ = −2 (e · νr ) , r ∈ S .
Abbreviated notation:
(−z + K ) ρ(r) = g(r) . (1)
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Equivalent integral equation formulation
Ansatz which solves the PDE and takes care of r → ∞:
U(r) = e · r +
∫
S
G (r , r ′)ρ(r ′)dσr ′ ,
where ρ(r) is an unknown layer density. Insertion of U(r) in theboundary condition at S :
(ǫ2 + ǫ1)
(ǫ2 − ǫ1)ρ(r) + 2
∫
S
∂
∂νrG (r , r ′)ρ(r ′)dσr ′ = −2 (e · νr ) , r ∈ S .
Abbreviated notation:
(−z + K ) ρ(r) = g(r) . (1)
The polarizability from ρ(r):
α = −ǫ1
∫
S
ρ(r) (e · r) dσr . (2)
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
When does(−z + K ) ρ(r) = g(r)
have a (unique) solution?
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
When does(−z + K ) ρ(r) = g(r)
have a (unique) solution? Well, when z is not an eigenvalue of K .
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
When does(−z + K ) ρ(r) = g(r)
have a (unique) solution? Well, when z is not an eigenvalue of K .
What does the spectrum of K look like?
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
When does(−z + K ) ρ(r) = g(r)
have a (unique) solution? Well, when z is not an eigenvalue of K .
What does the spectrum of K look like? If S is smooth, then K iscompact and has a discrete spectrum accumulating at zero. Alleigenvalues zi are real and less than one in modulus.
The electrostatic equation is uniquely solvable for z /∈ [−1, 1], andoften otherwise as well.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
When does(−z + K ) ρ(r) = g(r)
have a (unique) solution? Well, when z is not an eigenvalue of K .
What does the spectrum of K look like? If S is smooth, then K iscompact and has a discrete spectrum accumulating at zero. Alleigenvalues zi are real and less than one in modulus.
The electrostatic equation is uniquely solvable for z /∈ [−1, 1], andoften otherwise as well.
Eigenvalues zi correspond to PLASMONS in α(z).
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
When does(−z + K ) ρ(r) = g(r)
have a (unique) solution? Well, when z is not an eigenvalue of K .
What does the spectrum of K look like? If S is smooth, then K iscompact and has a discrete spectrum accumulating at zero. Alleigenvalues zi are real and less than one in modulus.
The electrostatic equation is uniquely solvable for z /∈ [−1, 1], andoften otherwise as well.
Eigenvalues zi correspond to PLASMONS in α(z).
Repetition: z = (ǫ1 + ǫ2)/(ǫ1 − ǫ2).
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
The Superellipse
The superellipse|r1|
k + |r2|k = 1
is a circle for k = 2 and “numerically” a square for k = 1016.
−1.5 −1 −0.5 0 0.5 1 1.5
−1
−0.5
0
0.5
1
Superellipse at k=2, 8, 32, 128
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
What does the spectrum of K look like for a superellipse?
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
What does the spectrum of K look like for a superellipse?
100
105
1010
1015
−0.5
−0.4
−0.3
−0.2
−0.1
0
0.1
0.2
0.3
0.4
0.5
superellipse |r1|k+|r
2|k=1
k
eige
nval
ues
z i
dark plasmonsbright plasmons
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
A zoom at low k reveals a fascinating pattern
2 3 4 5 6 7 8 9 1010
−8
10−6
10−4
10−2
100
superellipse |r1|k+|r
2|k=1
k
posi
tive
eige
nval
ues
z i
dark plasmonsbright plasmons
Are there any phase transitions or critical points here?
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
The polarizability α(z), z ∈ [−1, 1], of a superellipse at k = 1012
(almost a square):
−1 −0.5 0 0.5 1
−10
−8
−6
−4
−2
0
2
4
6
8
10
superellipse |r1|k+|r
2|k=1 with k=1012
x
α(x)
A myriad of PLASMONS.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Can we guess the spectrum of K for a square by studying thesuperellipse in the limit k → ∞?
100
105
1010
1015
−0.5
−0.4
−0.3
−0.2
−0.1
0
0.1
0.2
0.3
0.4
0.5
superellipse |r1|k+|r
2|k=1
k
eige
nval
ues
z i
dark plasmonsbright plasmons
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Can we guess the spectrum of K for a square by studying thesuperellipse in the limit k → ∞?
100
105
1010
1015
−0.5
−0.4
−0.3
−0.2
−0.1
0
0.1
0.2
0.3
0.4
0.5
superellipse |r1|k+|r
2|k=1
k
eige
nval
ues
z i
dark plasmonsbright plasmons
The answer depends on what function space we consider.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
What does the limit polarizability α+(x) = limy→0+ α(x + iy) looklike for a square? Does it exist at all? and if so, in what functionspaces lie the corresponding limit solutions ρ+(r) and U+(r)?
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
What does the limit polarizability α+(x) = limy→0+ α(x + iy) looklike for a square? Does it exist at all? and if so, in what functionspaces lie the corresponding limit solutions ρ+(r) and U+(r)?
−1 −0.5 0 0.5 1
−10
−8
−6
−4
−2
0
2
4
6
8
10
The square: polarizability
x
α+(x
)
real{α+(x)}
imag{α+(x)}
Yes, α+(x) exists, but do we see any PLASMONS?
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Comparison:
−1 −0.5 0 0.5 1
−10
−8
−6
−4
−2
0
2
4
6
8
10
superellipse |r1|k+|r
2|k=1 with k=1012
x
α(x)
−1 −0.5 0 0.5 1
−10
−8
−6
−4
−2
0
2
4
6
8
10
The square: polarizability
x
α+(x
)
real{α+(x)}
imag{α+(x)}
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Theory for Lipschitz sets
The polarizability α+(x) exists.
The polarizability α(z) admits an integral representation
α(z) =
∫
R
dµ(x)
x − z=
∫
σµ
µ′(x)dx
x − z,
where σµ = {x : µ′(x) > 0} and the measure dµ(x) relate toα+(x) as
µ′(x) = ℑ{α+(x)}/π , x ∈ R .
The spectral measure is of great interest in theoretical materialscience.
One can show that for z ∈ L, L : σµ ⊂ L ⊂ [−1, 1], theelectrostatic equation has no finite-energy solution U(r). For allother z there are solutions U(r). This has consequences.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
What about the cube?
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
What about the cube?
−1 −0.5 0 0.5 1−10
−5
0
5
10
15
20
The cube: polarizability
x
α+(x
)
real{α+(x)}
imag{α+(x)}
No one has succeeded in computing this (in its entirety) before.The reason being, perhaps, the behavior of U+(r) and ρ+(r).
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Some cube records
Table: Reference values, estimated relative errors, and best previousestimates of the polarizability α+(x) and the capacitance C of the cube.
present reference values relerr previous results relerr
α+(−1) 3.644305190268 10−11 3.6442 3 · 10−5
α+(−0.6) 5.85574775 + 16.64205643i 10−8
α+(0.25) −2.76289925 + 3.08034035i 10−7
α+(1) −1.638415712936517 10−14
−1.6383 6 · 10−5
C 0.66067815409957 10−13 0.66067813 10−7
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
103
104
105
10−15
10−10
10−5
100
The cube: convergence
Number of discretization points n
Est
imat
ed r
elat
ive
erro
r in
α+(x
) an
d C
α+(−1)
α+(−0.6)
α+(0.25)
α+(1)
C
Figure: Convergence of α+(x) and the capacitance C of a unit cube.The values of x correspond to: cube with infinite permittivity (x = −1),resonance in corners (x = −0.6), resonance along edges (x = 0.25), andcube with zero permittivity (x = 1).
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Table: Numerical progress for the capacitance of the unit cube.
value year Author0.6555 1957 Reitan–Higgins0.661 1961 Greenspan–Silverman0.6596 1967 Cochran0.661 1990 Brown0.66067475 1992 Goto–Shi–Yoshida0.6632 1994 Douglas–Zho–Hubbard0.6606751 1997 Given–Hubbard–Douglas0.6606785 1997 Read0.660692 2001 Mansfield–Douglas–Garboczi0.6601 2002 Bai–Lonngren0.6606835 2003 Hwang–Mascagni0.6606782 2004 Hwang–Mascagni0.6606 2004 Wintle0.6606780 2004 Mascagni–Simonov0.66067674 2004 Read0.6606749 2005 Ong–Lim0.66067786 2008 Lazic–Stefancic–Abraham0.6606746 2009 Mukhopadhyay–Majumdar0.66067813 2010 Hwang–Mascagni–Won0.678 2011 Bontzios–Dimopoulos–Hatzopoulos0.66067815409957 2012 Helsing–Perfekt
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Numerical method
The computation of α+(x) relies on the solution ρ+(r) to
(I + λK ) ρ+(r) = λg(r) ,
but how is it possible to obtain accurate numerical approximationsto ρ+(r), which barely lies in W−1,∞?
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Numerical method
The computation of α+(x) relies on the solution ρ+(r) to
(I + λK ) ρ+(r) = λg(r) ,
but how is it possible to obtain accurate numerical approximationsto ρ+(r), which barely lies in W−1,∞?
Well, thanks toK = K ⋆ + K ◦ ,
ρ(r) = (I + λK ⋆)ρ(r) ,(
I + λK ◦(I + λK ⋆)−1)
ρ(r) = λg(r) ,
which gives a solution ρ+(r) in L∞.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Discretization
Discretization of(I + λK ) ρ(r) = λg(r)
gives(Icoa + λK◦
coaR) ρcoa = λgcoa , (3)
where the small block diagonal matrix
R = PTW (Ifin + λK⋆
fin)−1P
is obtained via a fast recursion.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
12
3
4
56
7
8
γ1
Figure: A coarse mesh with eight quadrature panels on a closed surface.A fine mesh with 14 panels is created by refinement in a direction towardthe corner γ1.
0 50 100 150 200
0
50
100
150
200
nz = 501760 50 100 150 200
0
50
100
150
200
nz = 163840 50 100 150 200
0
50
100
150
200
nz = 33792
Figure: Kfin = K⋆
fin+ K◦
fin.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Details
(I + λK ) ρ(r) = λg(r) .
Assumption: K is compact some distance away from the corners γj
and g(r) is piecewise smooth.
Let K (r , r ′) be the kernel of K . Split K (r , r ′) into two functions
K (r , r ′) = K ⋆(r , r ′) + K ◦(r , r ′) ,
where K ⋆(r , r ′) is zero except for when r and r ′ simultaneously lieclose to the same γj . In this latter case K ◦(r , r ′) is zero.
The kernel split corresponds to an operator split K = K ⋆ + K ◦,where K ◦ is compact. Discretization on a fine mesh gives
(Ifin + λK⋆
fin + λK◦
fin) ρfin = λgfin .
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Details
The transformρfin = (Ifin + λK⋆
fin)−1ρfin
leads to(
Ifin + λK◦
fin (Ifin + λK⋆
fin)−1)
ρfin = λgfin .
Note:
K◦
fin(Ifin + λK⋆
fin)−1 is, in practice, a compact operator
ρfin is piecewise smooth
neither gfin, ρfin, nor K◦
finneeds a fine mesh for resolution.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Details
Let P be a prolongation operator from the coarse mesh to the finemesh and let Q be a restriction operator in the opposite direction
QP = I .
Then
gfin = Pgcoa
ρfin = Pρcoa
K◦
fin = PK◦
coaPTW .
Compare reduced SVD. Here PW = WfinPW−1coa and W has
quadrature weights on the diagonal. Taken together
(
Icoa + λK◦
coaPTW (Ifin + λK⋆
fin)−1P
)
ρcoa = λgcoa . (4)
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Details
WithR = PT
W (Ifin + λK⋆
fin)−1
P
(4) becomes(Icoa + λK◦
coaR) ρcoa = λgcoa .
We only need the fine mesh for the construction of the small blockdiagonal matrix R. One block per corner.
The blocks of R can be obtained via a fast recursion, where step i
inverts and compresses contributions to R involving the outermostpanels on level i of a locally n-ply refined mesh.
Newton’s method can accelerate the recursion in situations thatdemand extreme refinement (very many recursion steps). Thiscorresponds to inverting a giant full matrix in sublinear time.Boundary singularities do no longer pose any practical problems.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
The fast recursion
Ri = PTWbc
(
F{R−1(i−1)} + I◦b + λK◦
b
)
−1Pbc , i = 1, . . . , n .
part ofcoarse mesh
refined n = 4
i = 1
i = 2
i = 3
Figure: Recursion on a refined mesh surrounding a corner.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
Matlab
Kmat=Kinit(zloc,wloc,nzloc,96);
MAT=eye(96)+lambda*Kmat;
starL=[17:80];
R=inv(MAT(starL,starL));
myerr=1;
while myerr>eps
Rold=R;
MAT(starL,starL)=inv(R);
R=Pwbc’*inv(MAT)*Pbc;
myerr=norm(R-Rold,’fro’)/norm(R,’fro’);
end
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
An extreme example – 20 years too late?
Figure: A unit cell of a random checkerboard with a million squares. Thepermittivity ratio is ǫ2/ǫ1 = 106 and the effective permittivity is obtainedwith a relative error of 10−9.
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Polarizability Superellipse and Square The cube Numerical method Details To the movies
References
J. Helsing and K.-M. Perfekt (2012) “On the polarizability andcapacitance of the cube”, arXiv:1203.5997v2.
J. Helsing, R.C. McPhedran, and G.W. Milton (2011) “Spectralsuper-resolution in metamaterial composites”, New J. Phys., 13(11),115005.
J. Helsing (2011) “The effective conductivity of arrays of squares: largerandom unit cells and extreme contrast ratios”, J. Comput. Phys.,230(20), 7533–7547.
J. Helsing (2011) “A fast and stable solver for singular integral equationson piecewise smooth curves”, SIAM J. Sci. Comput., 33(1), 153–174.
J. Helsing (2009) “Integral equation methods for elliptic problems withboundary conditions of mixed type”, J. Comput. Phys., 228(23), pp.8892–8907.
J. Helsing and R. Ojala (2008) “Corner singularities for elliptic problems:integral equations, graded meshes, quadrature, and compressed inversepreconditioning”, J. Comput. Phys., 227(20), 8820–8840.
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−6 −5 −4 −3 −2 −1 0 1−5
−4
−3
−2
−1
0
1
2
3
4
5
Staggered array of square cylinders at p1=0.49999999995
permittivity ratio σ
effe
ctiv
e pe
rmitt
ivity
εef
f(σ)
real{εeff}
imag{εeff}
−6 −5 −4 −3 −2 −1 0 1
10−15
10−10
10−5
100
Staggered array of square cylinders at p1=0.49999999995
|εef
f(σ)ε
eff
∗(1
/σ∗ )−
1|
permittivity ratio σ
Figure: Effective permittivity (polarizability) and error estimates.