These are preliminary lecture notes, intended only for distribution to participants.
SMR: 1643/5
WINTER COLLEGE ON OPTICS ON OPTICS AND PHOTONICSIN NANOSCIENCE AND NANOTECHNOLOGY
( 7 - 18 February 2005)
"Optical Propertiesof Plasmonic Nanosystems"- II
presented by:
M. StockmanGeorgia State University
Atlanta
U.S.A.
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 1
Theory of Nanoplasmonics 2:Optical Properties of Plasmonic
NanosystemsMark I. Stockman
Department of Physics and Astronomy, Georgia State University, Atlanta, GA
30303, USA
Support:
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 2
LECTURE 2
Nanoplasmonics of Nanosystems1. Introduction; Local fields of a sphere
2. Quasistatic eigenmodes; Theorem on Anderson localization3. Giant SERS in fractals4. Nanospheres and their aggregates; Efficient nanolens made of nanospheres5. Enhancement, depolarization and dephasing of SHG
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 3
PROBLEMS IN NANOOPTICS
Microscale
Delivery of energy to nanoscale; Adiabatical conversion of propagating EM wave to local fields
Enhancement and control of the local nanoscale fields. Enhanced near-field responses
Generation of local fields on nanoscale: SPASER
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 4
Quasistatic Approximation and EigenmodesFor a nanosystem, size is much less than the radiation wavelength. In this case, one can neglect retardation, and describe the system by quasistatic equations for electrostatic potential.
Quasistatic approximation does not imply that the excitation processes are slow. Just to the opposite, the neglectable retardation allows one to use and study ultrafast processes in nanostructures.
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 5
Example: Quasistatic fields as expansion over eigenmodes for spherical particles
j 2@l_, m_, r_, q_, j _D:= ikjja@2, l, mD 1
rl+ 1+ b@2, l, mD rly{zz SphericalHarmonicY@l, m, q, jD
j 1@l_, m_, r_, q_, j _D:= ikjja@1, l, mD 1
rl+ 1+ b@1, l, mD rly{zz SphericalHarmonicY@l, m, q, jD�. a@1, l, mD® 0
l R1+2 lHe1 - e2Le2 + lHe1 + e2LMultipolar (l,m) polarizability:
Coefficients of eigenmodes expansion:9b@2, 1, 0D® - 2$%%%%%%p3
, a@2, 1, 0D®2 ######p
3R3He1 - e2L
e1 + 2 e2, b@1, 1, 0D® - 2�!!!!!!!3 p e2
e1 + 2 e2=
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 6
-3 -2 -1 0 1 2 3x
-3
-2
-1
0
1
2
3
z
-3 -2 -1 0 1 2 3x
-3
-2
-1
0
1
2
3
z
-3 -2 -1 0 1 2 3x
-3
-2
-1
0
1
2
3
z
Quasistatic local field intensity for silver sphere
SPωω < SPωω = SPωω >
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 7
We will follow the spectral theory that allows one to separate the material and geometric properties of the system.
1. M. I. Stockman, S. V. Faleev, and D. J. Bergman, Anderson Localization vs. Delocalization of Surface Plasmons in Nanosystems: Can One State Have Both Characteristics Simultaneously?, Phys. Rev. Lett. 87, 167401-1-4 (2001).
2. M. I. Stockman, D. J. Bergman, and T. Kobayashi, Coherent Control of Nanoscale Localization of Ultrafast Optical Excitation in Nanosystems, Phys. Rev. B. 69, 054202-1-10 (2004).
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 8
Quasistatic field equations and boundary conditions
. 0),,(),,(
, 1),,( , 0)0,,( , 0)(),(
,0,0=
∂∂
=∂∂
===∂∂
∂∂
==yx LyLx
z
zyxy
zyxx
Lyxyx
ϕϕ
ϕϕϕωε rr
rr
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 9
Eigenmode problem (depending only on geometry, material independent!)
. 0),,(),,(
and , 0),,()0,,(
; 0)host( and 1)inclusion( where
,)( )()(
,0,0
2
2
=∂∂
=∂∂
===∈=∈
∂∂
=∂∂
∂∂
== yx Lyn
Lxn
znn
nnn
zyxy
zyxx
Lyxyx
s
ϕϕ
ϕϕθθ
ϕϕθ
rr
rr
rr
rr
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 10
Green’s function as an eigenmode expansion:( ) )()(
)(;, * rrrr ′
−=′ ∑ nn
n n
n
sssG ϕϕ
ωω
1
host
metal
)()(1)( parameter spectral thewhere
,)(equation an from found becan frequency complex whoseexcitation elementary are plasmons surface Physical
−
⎟⎟⎠
⎞⎜⎜⎝
⎛−=
=+
ωεωεω
γω
s
sis nnn
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 11
Local fields on nanoscale for harmonic excitation with external field at frequency ω:
( ) , ;,)()()( 3200 rdG ′′∇′−= ∫ ′ ωϕϕϕ rrrrr r
( ) , ;,),(
),(),(32
0
0
tdrdttGt
tt′′′−′∇′′
−=
∫ ′ rrr
rr
rϕ
ϕϕ
Local fields on nanoscale for short-pulse excitation with pulse field
)(0 rϕ
),(0 trϕ
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 12
Theorem on Localization of Surface Plasmons:
Any Anderson-localized (or, strongly localized) mode is dark.
Corollary: It is impossible that all surface-plasmon modes of any system are Anderson-localized (or, strongly localized).
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 13
Geometry of Random Planar Composite
0 5 10 15 20Li10 - 14
10 - 11
10 - 8
10 - 5
10 - 2
fi
Distribution of Eigenmodes over their Oscillator Strength fiand Localization Radius Li
Phys. Rev. Lett. 87, 167401 (2001).
0 10 20 30y0
10
20
30
z
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 14
Local Field Intensities for Four Eigenmodes Representative of Each Class of Eigenmodes
si=0.1995 , Li=2.1
30
y 30 z
0.1
0.3
Ei2
30
y
si=0.2, Li=11.2
30y 30 z
0.01
0.03
Ei2
30y
si=0.201 , Li=9.6
30
y 30 z
0.
0.01
Ei2
30
y
si=0.2015 , Li=1.
30
y 30 z
0
0.1
0.2
0.3
Ei2
30
y
Localized Luminous Delocalized Luminous
Delocalized Dark Localized Dark
07.0=f 02.0=f
910~ −f 910~ −f
si=0.1995 , Li=2.1
30y 30 z
0.
0.0005
0.001
Ei2
30y
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 15
0. 0.5 1.
4
8
12
16
20
s
L 3D Space 8‰32‰32
0. 0.5 1.
4
8
12
16
20
s
L 3D Space 4‰32‰32
0. 0.5 1.
4
8
12
16
20
s
L 2D Space 32‰32
0. 0.5 1.
2
4
6
8
10
s
L 3D Space 16‰16‰16
0. 0.5 1.
2
4
6
8
10
s
L 3D Space 4‰16‰16
0. 0.5 1.
2
4
6
8
10
s
L 2D Space 16‰16
L
Distribution of Eigenmodes over their Localization Length and Spectral Parameter
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 16
Giant Surface Enhanced Raman Scattering
M. I. Stockman, V. M. Shalaev, M. Moskovits, R. Botet, and T. F. George, Enhanced Raman Scattering by Fractal Clusters: Scale Invariant Theory,Phys. Rev. B 46(5), 2821-2830 (1992).
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 17
Single-molecule Surface-Enhanced Raman Scattering:
•K. Kneipp, Y. Wang, H. Kneipp, L. T. Perelman, I. Itzkan, R. Dasari, and M. S. Feld, Single Molecule Detection Using Surface-Enhanced Raman Scattering (SERS), Phys. Rev. Lett. 78, 1667-1670 (1997).
•S. M. Nie and S. R. Emery, Probing Single Molecules and Single Nanoparticles by Surface-Enhanced Raman Scattering, Science 275, 1102-1106 (1997).
•Z. J. Wang, S. L. Pan, T. D. Krauss, H. Du, and L. J. Rothberg, The Structural Basis for Giant Enhancement Enabling Single-Molecule Raman Scattering, Proc. Natl. Acad. Sci. USA 100, 8638-8643 (2003).
SERS Enhanced by factor of 1310~
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 18
Enhancement of Optical Responses in Fractals
Self-similar fractal geometry
Eiz
yx
0
100
200
t= 39.01 fs
Local optical fields in fractal cluster [MIS, Phys. Rev. Lett. 84, 1011 (2000) ].
9
4SERS
10~~ EG
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 19
SERS enhanced by a factor 1012 - 1014
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 20
Theory
Experiment
Comparison of theoretical predictions and experimental data for the SERS enhancement coefficient from silver colloid clusters.
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 21
K. Li, M. I. Stockman, and D. J. Bergman, Self-Similar Chain of Metal Nanospheres as an Efficient Nanolens, Phys. Rev. Lett. 91, 227402 (2003).
Efficient Self-Similar Nanolens of Nanospheres
Silver Nanospheres
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 22
++
+++++
--
--
--
-
Optical Electric Field
-
Underlying physics of local field enhancement in efficient nanolens: Cascade enhancement
Giant local fields in the minimum gap:
Nanoscale localization of optical energy
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 23
Local Fields for Silver 3-Sphere Nanolens
d=0.3R
w=3.37 eV
100
300
500
ÈEÈw=3.25 eV
0
500
1000
1500
ÈEÈ0
w=0.77 eV
0
5
10
15
ÈEÈ0
K. Li, M. I. Stockman, and D. J. Bergman, Self-Similar Chain of Metal Nanospheres as an Efficient Nanolens, Phys. Rev. Lett. 91, 227402 (2003).
Giant Local Field Enhancement in Nanolens
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 24
FDTD computations. C. Oubre and P. Nordlander (Private Communication).
d= 0.3 R
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 25
R. Hillenbrand and F. Keilmann, Optical oscillation modes of plasmon particles observed in direct space by phase-contrast near-field microscopy, Appl. Phys. B 73, 239–243 (2001)
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 26
CONCLUSIONS
• A self-similar chain of metal nanospheres makes an efficient nanolens focusing energy of optical field, concentrating it a nanoscale gap between the smallest nanosphere
• The optical field in the nanofocus is enhanced by more then three orders of magnitude
• A molecule adsorbed in this nanofocus will exhibit Raman scattering enhanced by a factor on order or greater than 1013.
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 27
DEPOLARIZATION AND DEPHASING IN SECOND HARMONIC GENERATION IN RANDOM METAL
NANOSTRUCTURED SYSTEMS
Mark I. Stockman, David J. Bergman, Cristelle Anceau, Sophie Brasselet, and Joseph Zyss, Enhanced Second Harmonic Generation By Metal Surfaces with Nanoscale Roughness: Nanoscale Dephasing, Depolarization, and Correlations, Phys. Rev. Lett. 92, 057402-1-4 (2004).
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 28
Experimental evidence of strong depolarization, dephasing, and giant fluctuations of SHG:C. Anceau, S. Brasselet, J. Zyss, and P. Gadenne, Local second harmonic generation enhancement on gold nanostructures probed by 2-photon microscopy, Opt. Lett. 28, 713 (2003).
Department of Physics and Astronomy Georgia State University Atlanta, GA 30303-3083
2/14/05 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy 02/10/2005 29
S. I. Bozhevolnyi, J. Beermann, and V. Coello, Phys. Rev. Lett. 19, 197403 (2003)
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 30
rrrr
∂∂
=)( )()( 2(2))2( θχ EPNL
The total SH Polarization is found as:
rdG rNL
host′′⋅⎥⎦
⎤⎢⎣⎡ ′
′∂∂
= ∫ 3)2()2( )2 ;,( )(4)( ωεπϕ rrrP
rr
⎥⎦
⎤⎢⎣
⎡−=
∇−=
)2()(1)2 ,( where
),(4
1-)2 ,()()(
host
)2()2(NL
)2(total
ωθεωε
ϕπωε
s
PP
rr
rrrr
The SH potential is calculated as:
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 31
Geometry of the system SH Polarization
20
)2(
)2( )(
E
rP
χ
0 10 20 30x0
10
20
30
z
0
)(
E
rE
Local linear field
102030x
102030 z
0
100
200
102030x
10 20 30
10
20
30
10 20 30x
10
20
30
z102030
x102030 z
0
20
40
102030x
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 32
Im Pz(2)Re Pz
(2)
Re Px(2) Im Px
(2)
Depolarization of SH
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 33
Dephasing of SH
Polarized component Depolarized component
500ReP z
H2L
ImPzH2L
- 500 500ReP x
H2L
- 500
ImPxH2L
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 34
Correlation Functions for Different Fill Fractions p (Color Coded):
P = 0.35, 0.50, 0.60, 0.75, 0.95
0 2 4 6 8r0.
0.5
1.
CHrL
0 2 4 6 8r0.
0.5
1.
Cphase HrL
0 2 4 6 8r0.
0.5
1.
Cpolariz HrLH.J.Simon
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 35
Giant fluctuations of SHG local fields (new result)
Giant fluctuations of local optical fields introduced:M.I.Stockman, L.N.Pandey, L.S.Muratov, and T.F.George, Giant Fluctuations of Local Optical Fields in Fractal Clusters, Phys. Rev. Lett. 72(15), 2486-2489 (1994). The universal index –1.5 for fundamental and –2.5 for SH
10 - 210 - 1 10 102 103ISH
10 - 6
10 - 4
10 - 2
PHISHL- 0.773087 - 2.39585 x
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 36
CONCLUSIONS•Second harmonic polarization P(2)(r) in a nonlinear random planar composite is a highly singular function concentrated in hot spots. P(2)(r) is significantly different from local fields E(r).
•SHP P(2)(r) is both dephased and depolarized at the nanoscale. SHG from a random composite on any microscopic scale is incoherent, i.e., hyper-Raleigh scattering
•The local intensity of SHG undergoes giant (non-Gaussian) fluctuations with scaling distribution function whose index is not universal
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 37
Ivan A. Larkin and Mark I. Stockman, Imperfect Perfect Lens, Phys. Nano Lett. 5, 339 – 343 (2005)
Extreme Nanoplasmonics: Fundamental limit on the minimum scale of the energy concentration/spatial resolution
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 38
At small distances a, interactions transfer large momentum a
p h~
or wave vector a
k 1~
For large enough k, interacting electron system exhibits strong spatial dispersion and Landau damping . These effects are described by Klimontovich-Silin-Lindhart (RPA) formula
scm 10~~ 8
Fvak
≤ωω
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 39
Pendry’s Perfect Lens in near field
Metal slab
a
bObject2a-b
Ideal image
λ<<ba,It is required that the relative dielectric permittivity 1−=ε
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 40
Estimate of the ultimate spatial resolution of the “perfect lens”
where Q~10-100 is the surface plasmon resonance quality factor
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 41
Imaging
Image of a washer as produced by a silver slab of 5 nm thickness in GaAs host: (a) without spatial dispersion, (b) with spatial dispersion. Photon energy: 2.2 eV.
10 20
0.5
1.
Image of a point charge produced by a 5 nm silver slab in GaAs environment, photon energy: 2.2 eV
r
Department of Physics and AstronomyGeorgia State UniversityAtlanta, GA 30303-3083
2/14/2005 Web: http://www.phy-astr.gsu.edu/stockmanE-mail: [email protected]
ITCP, Trieste, Italy02/10/2005 42
CONCLUSIONS
1. At small distances (on order of a few nanometers), the conventional local electrodynamics is no more applicable.
2. Nonlocality of permittivity and Landau damping become important.
3. These effects limit the spatial resolution of the “perfect lens” to no better than 5 nm
4. Other resonant, plasmonic effects are also limited by these effects and die out at the scale of a few nanometers.