Chiral metallic nanostructures can generate evanescent fields which are more highly twisted than circularly polarized light. However, it remains unclear how best to exploit this phenomenon, hindering the optimal utilization of chiral electromagnetic fields. Here, inspired by optical antenna theory, we address this challenge by introducing chiral antenna parameters: the chirality flux efficiency and the chiral antenna aperture. These quantities, which are based on chirality conservation, quantify the generation and dissipation of chiral light. We then present a label-free experimental technique, chirality flux spectroscopy, which measures the chirality flux efficiency, providing valuable information on chiral near fields in the far field. This principle is verified theoretically and experimentally with two-dimensionally chiral coupled nanorod antennas, for which we show that chiral near and far fields are linearly dependent on the magnetoelectric polarizability. This elementary system confirms our concept to quantify chiral electromagnetic fields and paves the way toward broadly tunable chiral optical applications including ultrasensitive detection of molecular chirality or optical information storage and transfer.
Chiral metallic nanostructures can generate evanescent fields which are more highly twisted than circularly polarized light. However, it remains unclear how best to exploit this phenomenon, hindering the optimal utilization of chiral electromagnetic fields. Here, inspired by optical antenna theory, we address this challenge by introducing chiral antenna parameters: the chirality flux efficiency and the chiral antenna aperture. These quantities, which are based on chirality conservation, quantify the generation and dissipation of chiral light. We then present a label-free experimental technique, chirality flux spectroscopy, which measures the chirality flux efficiency, providing valuable information on chiral near fields in the far field. This principle is verified theoretically and experimentally with two-dimensionally chiral coupled nanorod antennas, for which we show that chiral near and far fields are linearly dependent on the magnetoelectric polarizability. This elementary system confirms our concept to quantify chiral electromagnetic fields and paves the way toward broadly tunable chiral optical applications including ultrasensitive detection of molecular chirality or optical information storage and transfer.
Chirality, the phenomenon of
handedness, is a distinctive property of living matter.[1] Molecular chirality arises due to the mirror-symmetric
arrangement of otherwise identical compounds. Because the structural
differences between these molecules, known as enantiomers, can impact
their biochemical function, techniques for selective detection and
separation of chiral molecules have been sought.[2] Chiral light, such as left- and right-handed circularly
polarized plane waves, offers a versatile and noninvasive means to
detect molecular chirality.[3] However, this
approach is intrinsically limited in sensitivity due to the dimensional
mismatch between molecules and the wavelength of light,[4] which leads to long integration times that hinder
applications.[5]Recent advances in
nanotechnology have enabled the fabrication
of chiral metallic nanostructures[6] (and
achiral nanostructures excited with chiral light[7−9]) that address
the above challenge in two ways. First, their evanescent fields can
exceed the chirality of circularly polarized light.[10] Second, their spatial extent can better match subwavelength
molecular dimensions.[11] These two factors
can increase detection sensitivity of chiral molecules by orders of
magnitude.[12−14] Thus, highly chiral evanescent fields offer a promising
avenue toward the realization of ultrasensitive on-chip selection
and separation of chiral molecules.[15−20]However, to move beyond initial demonstrations of highly chiral
light, criteria for effectively designing and tailoring nanostructures
for the chirality of their fields are needed. This requires methods
to characterize nanoscale chiral fields. Probing the near field directly
is experimentally challenging with existing techniques.[21] Ideally, we would extract information on chiral
evanescent fields from far-field measurements,[22] but this approach has not yet succeeded.Optical
antenna theory can help resolve this issue. Specifically,
just as classical electromagnetic antennas optimize energy transfer
between a localized receiver and the free radiation field,[23−25] an ideal chiral nanoantenna should enhance the transfer of chiral
optical information from a molecule placed in its near field to the
far field (Figure ). Thus, rather than directly probing chiral near fields, an appropriate
far-field technique should be sufficient.
Figure 1
Conceptual illustration
of (a) an optical antenna where energy
transfer to and from a receiver is enhanced and (b) a chiral optical
antenna where the receiver is a chiral molecule and the transfer of
chiral optical information to and from the far field is enhanced.
Conceptual illustration
of (a) an optical antenna where energy
transfer to and from a receiver is enhanced and (b) a chiral optical
antenna where the receiver is a chiral molecule and the transfer of
chiral optical information to and from the far field is enhanced.Here, we present a formalism for
the optical characterization of
chiral nanoantennas inspired by classical antenna theory. We introduce
physical quantities, the chirality flux efficiency and the chiral antenna aperture, that enable the
quantification of the chiral optical properties of a nanoantenna.
We then develop a label-free experimental technique, chirality
flux spectroscopy, to measure the chirality flux efficiency
and verify our results with both theory and experiment for coupled
nanorod dimers with two-dimensional (2D) chirality. We find that the
chiral fields of the system are driven by the magnetoelectric polarizability,
exhibiting a linear relationship between chirality flux efficiency
and the chiral near-field coupling of the two nanorods in the studied
regime. Thus, our method provides vital information on chiral near
fields that can be accessed in the far field, enabling rational nanoantenna
design based on chiral optical fields and the optimal utilization
of chiral light in specifically tailored applications.The handedness
of chiral electromagnetic plane waves is determined
by the rotation direction around the propagation axis. Locally, this
is quantified by the optical chirality density,[26] which in its time-averaged form (denoted with
an overbar) iswhere ω is the angular
frequency and and are the
complex amplitudes for the electric
displacement and magnetic fields, respectively, with the asterisk
indicating the complex conjugate. χ̅ is a chiral analogue
to the local density of optical states.[27] For a single plane wave, χ̅ reaches its extrema for
circularly polarized light (CPL).[28] This
limit (χ̅CPL) can be exceeded by evanescent
waves, due to their theoretically unlimited in-plane spatial frequencies.[29] Specifically, a z-decaying
evanescent wave with in-plane wavevector components k and k reaches its maximum optical chirality density atwhere ε0 is the vacuum permittivity
and is the
complex electric-field amplitude
with Cartesian components , , and (see
the Supporting Information). Chiral metallic nanostructures, which are effective
generators of chiral evanescent fields,[6] therefore offer an accessible route toward chiral sensing.Previously, these systems have been characterized using spectroscopic
techniques[21] designed to evaluate biomolecular
structure.[30] Most notably, circular dichroism
(CD) spectroscopy[3,4] measures the differential extinction
between illumination with left- and right-handed circularly polarized
light. In addition to the conventional extinction approach, variations
of CD have been developed on the basis of nonlinear optical response,[31] strong optical scattering,[32] and fluorescence.[33] These have
been successfully applied to chiral metallic nanostructures.[34−40] Compared to molecules, plasmonic resonances can exhibit CD signal
amplitudes that are orders of magnitude higher at ultraviolet, visible,
and near-infrared frequencies.[41−45] Indeed, geometries to maximize this effect have been proposed.[46] Moreover, these signals can be induced or altered
by ultraviolet-resonant molecules.[47] However,
while these spectra provide valuable structural information, their
relation to chiral evanescent fields is unclear.[22]Instead of alternating the handedness of circularly
polarized illumination
(as in CD spectroscopy), one can alternatively evaluate the degree
of circular polarization of the fields that are emitted or scattered
by a chiral sample. Circularly polarized luminescence[48] exploits this approach for chiral emitters. Moreover, it
has been applied to chiral metallic nanostructures by functionalizing
their surface with achiral fluorophores.[49,50] Although this strategy can probe chiral near fields, two disadvantages
remain: (i) the resulting spectra are convoluted with fluorophore
emission[51] and (ii) the metal surface must
be decorated with fluorescent labels, which can hinder subsequent
interactions between the near field and a chiral analyte of interest.We now introduce an approach that enables the label-free detection
of chiral optical fields. By extending optical antenna theory, we
can theoretically and experimentally quantify the generation and dissipation
of chiral light in terms of parameters that directly relate to the
chiral evanescent fields. As optical antenna parameters are derived
from energy conservation,[29] we base our
technique on the analogous conservation law of optical chirality in
lossy, dispersive media.[22] This requires
optical chirality dissipation to balance with the optical chirality
flux (see Table ).
Thus, by detecting the degree of circular polarization of the scattered
light in the far field, the optical chirality flux can be determined.
This then provides information about the chiral near field (see the Supporting Information).
Table 1
Comparison
of Optical Antenna Parameters
(left) and Chiral Optical Antenna Parameters (right) Based on Their
Governing Conservation Laws, Where ω is the Angular Frequency
and n Is the Normal Vectora
In the left column, we and wm are the complex harmonic
electric and magnetic energy densities,[22], is the
Poynting vector, Pdiss is the dissipated
power, Pscat is the scattered power, Pext = Pdiss + Pscat is
the extinction power, and Iinc is the
incident light intensity. In the right column, χe and χm are the complex harmonic electric and magnetic
optical chirality densities,[22], is the
optical chirality flux, c is the speed of light, Ptot is the total power of the outgoing light,
and pinc is the incident power density.
In the left column, we and wm are the complex harmonic
electric and magnetic energy densities,[22], is the
Poynting vector, Pdiss is the dissipated
power, Pscat is the scattered power, Pext = Pdiss + Pscat is
the extinction power, and Iinc is the
incident light intensity. In the right column, χe and χm are the complex harmonic electric and magnetic
optical chirality densities,[22], is the
optical chirality flux, c is the speed of light, Ptot is the total power of the outgoing light,
and pinc is the incident power density.We define two antenna parameters
to characterize chiral nanoantennas,
the chirality flux efficiency [-] and the chiral antenna aperture [m2] (see
the Supporting Information for further
details)where c is
the speed of light in vacuum andis the
integral of the optical chirality flux, , through
the surface S,[22] with is the complex amplitude of the H field, and Ptot is the total power of
the outgoing light. Further,is the volume-integrated optical chirality
dissipation[22,69] withwith ϵ = ϵ′
+ iϵ″ as the complex permittivity, μ = μ′
+ iμ″ as the complex permeability, and χe, χm as
the complex harmonic electric and magnetic optical chirality densities.[22] Finally, pinc is
the incident power density.While the conventional antenna efficiency
quantifies radiative
power generation,[29]eq describes the ability of the antenna to scatter
chiral optical fields. Similarly, as the conventional antenna aperture
describes power dissipation, related to the absorption cross section,[29]eq describes the dissipation of chiral optical fields which, for small
metallic nanostructures with negligible damping and retardation, can
be brought into connection with the near-field optical chirality density.[22] The comparison to optical antenna parameters
is summarized in Table .We now apply the chiral antenna parameters in eqs and 4 to
an analytical
model of the 2D chiral metallic nanoantenna studied here. In the quasi-static
electric-dipole limit, this system is described by the dipole moment .[52,53] The electric polarizability
is written as αe and the chiral optical properties
are attributed to αc, the coupled magnetoelectric
polarizability.[54] Inserting this model
into eqs 1, 3, and 4, we obtain (see the Supporting Information)where r and ζ
are the
radial and longitudinal cylindrical coordinates, μ0 is the vacuum permeability, and k is the wavevector
magnitude. Equations –11 have several important physical
implications. First, the resonant properties of , , and χ̅d are linearly
dependent on Re(αc). Due to this proportionality,
the magnetoelectric polarizability αc directly determines
the strength of the chiral optical fields generated. Second, in the
dipole limit, the resonance of , which is measurable in the far field,
matches the resonance of χ̅d, which describes
the local near fields. Third, quantifies the ability of the dipolar nanoantenna
to dissipate optical chirality. As predicted by the conservation law
of optical chirality (see the Supporting Information), the resonance with maximum matches that of , which is measurable
in the far field.We verify our theoretical findings experimentally
with 2D chiral
nanorod dimers (NRDs) whose dominant properties are dipolar in the
studied regime. Figure a,b shows scanning-electron micrographs of right- (R) and left-handed
(L) NRDs, arranged periodically with an edge-to-edge distance of p = 600 nm (>6 × 104 unit cells). The
rod
dimensions are 70 nm × 230 nm × 50 nm in x, y, and z (with axes as in Figure ) to generate sufficient
antenna-scattered light. 2D chirality arises due to a ±140 nm
vertical and 60 nm horizontal shift (h) between the
nanorods in each pair (see the Supporting Information). Nonlinear, multipolar effects arising at small h are negligible.[55] The chiral coupling
between two metallic nanorods induces a magnetoelectric polarizability,[56] and the physical behavior of this system can
thus be modeled analytically as a single 2D chiral dipole.
Figure 2
(a, b) Scanning-electron
micrographs of (a) R-NRD and (b) L-NRD
arrays with a horizontal shift of h = 60 nm and edge-to-edge
distance of p = 600 nm (between outer NRD edges).
The scale bars are 500 nm. (c) Extinction spectrum of the R-NRD array, h = 60 nm. Inset: schematic of an R-NRD unit cell where
∗ denotes the center point (0, 0, 0). (d) The
experimental setup for measuring chirality flux efficiency (, eq ). Inset: Schematic
of sample excitation with achiral, linearly
polarized light. While generated chiral evanescent fields decay, is detected in the far field by analysis
of the scattered degree of circular polarization. For this, the light
is sent through a photoelastic modulator (PEM) and subsequent linear
polarizer (LP). The optical signal is detected by a photomultiplier
tube (PMT) and filtered with a lock-in amplifier at the PEM modulation
frequency.
(a, b) Scanning-electron
micrographs of (a) R-NRD and (b) L-NRD
arrays with a horizontal shift of h = 60 nm and edge-to-edge
distance of p = 600 nm (between outer NRD edges).
The scale bars are 500 nm. (c) Extinction spectrum of the R-NRD array, h = 60 nm. Inset: schematic of an R-NRD unit cell where
∗ denotes the center point (0, 0, 0). (d) The
experimental setup for measuring chirality flux efficiency (, eq ). Inset: Schematic
of sample excitation with achiral, linearly
polarized light. While generated chiral evanescent fields decay, is detected in the far field by analysis
of the scattered degree of circular polarization. For this, the light
is sent through a photoelastic modulator (PEM) and subsequent linear
polarizer (LP). The optical signal is detected by a photomultiplier
tube (PMT) and filtered with a lock-in amplifier at the PEM modulation
frequency.The antennas were fabricated by
template stripping[57] thermally evaporated
silver from a structured silicon template
onto a glass coverslip, after selective removal of the flat silver
deposited around the nanorods[58] (see the Supporting Information). An example of the optical
extinction spectrum for a specific R-NRD array (h = 60 nm) can be seen on a linear scale in Figure c (see the Supporting Information) for x-polarized incident light
(axes as in Figure ). The inset of Figure c indicates one R-NRD unit cell with an asterisk marking the center
point at (0, 0, 0). The spectrum is broad because in
this demonstration we are exploiting a higher-order resonance of the
system to increase the scattering signal from the NRDs at visible
frequencies.The principle of chirality flux spectroscopy, our
experimental
technique to measure , is shown schematically in Figure d. Light from a broadband illumination
source (100 W halogen lamp) is passed through a monochromator and
a linear polarizer (LP) before it is weakly focused [20×, 0.45
numerical aperture (NA) objective] onto the sample. The outgoing signal
is collected with a 10×, 0.3 NA objective. As this study focuses
on single NRD coupling, low NA collection avoids lattice effects arising
at higher angles.[50]Next, a photoelastic
modulator (PEM, Hinds Instruments I/FS50)
applies quarter-wave retardation to the collected light at 50 kHz,
which is subsequently analyzed by another LP. The excitation and collection
LPs are aligned precisely ±45° to the PEM optical axis as
even minor misalignments can lead to linear birefringence artifacts.
A photomultiplier tube (PMT, Hamamatsu R928) then detects the optical
signal. The output is fed into a lock-in amplifier (Zurich Instruments,
HF2) connected to the electronic signal from the PEM.The PEM
transforms R- or L-CPL, scattered from the sample, into
linear polarization at ±45° to the PEM axis, leading to
50 kHz modulation after the analyzing LP. In contrast, linear polarization,
predominantly from the excitation beam, is transformed into circular
polarization, which is then modulated at 100 kHz. This polarization-selective
modulation enables the isolated detection of circularly polarized
scattered fields, directly proportional to , in a bright-field measurement.The inset of Figure d illustrates how the measurement
of quantifies the ability of a nanoantenna
to generate chiral optical fields. The excitation with achiral, linearly
polarized light is key to this method, as becomes meaningful for a system where the
sample is the only source of chiral optical fields. In this case,
a relationship between chiral near and far fields can be established,
because the chiral light scattered into the far field is a direct
consequence of the rapidly decaying chiral evanescent fields. Specifically, selectively detects the excess of one handedness
of chiral light scattered by the sample, modulated at 50 kHz, while
equal amounts of L- and R-CPL recombine additively to linear polarization, modulated at 100 kHz.We emphasize
that this near-field information is not revealed with
CD spectroscopy, in which circularly polarized excitation is used.
In that case, the chiral sample’s preferential extinction of
one handedness of CPL results in differential amplitudes
of L- and R-CPL generating an outgoing elliptical beam (see the Supporting Information).[4] Thus, a CD spectrum describes how the sample alters incident chiral
light, providing information on chiral geometry,[32] but does not reveal its ability to generate chiral fields.Furthermore, in optical rotatory dispersion (ORD), a spectroscopic
technique which is Kramers–Kronig-related to CD,[56] a sample is excited with linearly polarized
light and the rotation plane of the outgoing elliptical beam is recorded.
This effect is related to the net phase retardation experienced by
L- and R-CPL when traversing a circularly birefringent medium.[30] Thus, ORD is clearly distinct from chirality
flux spectroscopy, where polarimetric analysis directly detects an
excess of L- or R-CPL in the scattered fields.We note that
plasmonic quarter-wave plates have been developed
to generate CPL upon linearly polarized excitation.[59,60] These systems rely on linear birefringence, where two orthogonal
components of the incident linearly polarized beam obtain a net phase
retardation.[30] Linear birefringence does
not occur for our measurement of , as our x-polarized excitation
(axes as in Figure ) experiences a single refractive index. Thus, the chiral fields
detected here result from the nanoantenna’s near-field chiral
coupling or, in other words, intrinsic rather than extrinsic chirality.[61,62]Figure a shows
experimental spectra for R-NRDs (red) and L-NRDs (blue),
respectively (h = 60 nm, achiral NRDs in black, see
the Supporting Information). The NRD handedness
determines the sign of the generated chiral optical fields, leading
to mirror-symmetric spectra. These results are well reproduced numerically
in Figure b, where
finite-element simulations (COMSOL Multiphysics 5.2) were conducted
with x-polarized plane-wave excitation with periodic
boundary conditions (see the Supporting Information). Amplitude differences between experimental (Figure a) and simulated data (Figure b) can be attributed to the higher collection
angle in experiment (NA = 0.3, see the Supporting Information). The feature at 600 nm (marked with ∗)
in Figure b arises
from the surface lattice resonance of the periodic array (see the Supporting Information). It is not seen in experiment,
presumably due to damping effects and fabrication imperfections.[50] By setting the edge-to-edge NRD distance to
600 nm, we sufficiently separate lattice and single-nanoantenna resonances
to distinguish their effects.
Figure 3
Experimental and simulated analysis of chiral
optical fields for
R-NRDs (red), L-NRDs (blue), and achiral NRDs (black) with h = 60 nm. (a) Experimental chirality flux efficiency () spectra. NRDs of opposite handedness show
mirror-symmetric spectra, while achiral NRDs show negligible . (b) Simulated spectra, in good agreement with the experimental
data in part a. Surface lattice effects (marked with ∗) are
not seen in experiment due to damping and fabrication imperfections.
(c) Experimental circular dichroism (CD) spectra, which differ from in magnitude, sign, and resonant wavelengths.
(d) Simulated optical chirality enhancement (χ̅/|χ̅CPL|) spectra, evaluated at (0, 0, 0), the center
point between nanorods (see Figure c). The spectral properties match those of , where the spectral shift and broadening
in parts a and b are explained by damping, retardation, ensemble effects,
and low NA collection. (e, f) Simulated near-field maps (z = 0 plane, NRD center) of χ̅/|χ̅CPL| for (e) R-NRDs and (f) L-NRDs at various wavelengths (λ),
which further illustrate the trends in part d.
Experimental and simulated analysis of chiral
optical fields for
R-NRDs (red), L-NRDs (blue), and achiral NRDs (black) with h = 60 nm. (a) Experimental chirality flux efficiency () spectra. NRDs of opposite handedness show
mirror-symmetric spectra, while achiral NRDs show negligible . (b) Simulated spectra, in good agreement with the experimental
data in part a. Surface lattice effects (marked with ∗) are
not seen in experiment due to damping and fabrication imperfections.
(c) Experimental circular dichroism (CD) spectra, which differ from in magnitude, sign, and resonant wavelengths.
(d) Simulated optical chirality enhancement (χ̅/|χ̅CPL|) spectra, evaluated at (0, 0, 0), the center
point between nanorods (see Figure c). The spectral properties match those of , where the spectral shift and broadening
in parts a and b are explained by damping, retardation, ensemble effects,
and low NA collection. (e, f) Simulated near-field maps (z = 0 plane, NRD center) of χ̅/|χ̅CPL| for (e) R-NRDs and (f) L-NRDs at various wavelengths (λ),
which further illustrate the trends in part d.For comparison, the experimental setup in Figure d was modified to perform CD
measurements
(see the Supporting Information). The resulting
spectra in Figure c show that, while both techniques yield characteristic mirror-symmetric
trajectories for R- and L-NRDs, they clearly differ in magnitude,
sign, and resonant wavelengths. The discrepancy between Figure a and c verifies that and CD provide different physical information.In Figure d, the
numerical optical chirality enhancement (χ̅/|χ̅CPL|) of the NRD evanescent fields is plotted versus wavelength.
This parameter was evaluated at the NRD center (0, 0, 0)
(marked with ∗ in Figure c). For both R- and L-NRDs, χ̅/|χ̅CPL| retains the same sign at all wavelengths, with its maximum
magnitude at 470 nm. This trend is further confirmed in numerical
colormaps of χ̅/|χ̅CPL| (z = 0 plane at NRD center) shown in Figure e,f for various wavelengths (λ). Here,
the handedness of χ̅/|χ̅CPL| arises
due to NRD near-field coupling and changes sign depending on the vertical
shift (positive or negative) between the nanorods. This does not occur
for the achiral NRDs, where no such excess is present (see the Supporting Information).Comparing these
results to Figure a,b, we find good agreement in the relative magnitude
and sign of χ̅/|χ̅CPL| and . This confirms the relationship between and chiral evanescent fields. However,
differences between χ̅/|χ̅CPL|
and are also observed. These include (i) a
∼50 nm spectral shift and (ii) a broadening between near- and
far-field spectra. Indeed, as with the analogous energy parameters,
(i) and (ii) are plausible effects arising due to damping and retardation
beyond the dipole limit,[63] as well as ensemble
effects and low NA collection.[64] In contrast,
no such connection can be drawn between χ̅/|χ̅CPL| and the CD spectrum (Figure c).As derived from our theoretical
model, Figure demonstrates
how the magnetoelectric polarizability
αc drives the NRD’s chiral fields, which arise
from plasmonic near-field coupling between two nanorods. Experimental spectra are shown in Figure a where the horizontal shift h varies from
60 to 200 nm. We note that different lattice densities
were accounted for by our normalization procedure (see the Supporting Information). R- (red) and L-NRDs
(blue) maintain mirror-symmetric spectra for all h. As h increases
and the nanorod near-field coupling decreases,
the magnitude of also decreases. Specifically, Figure b reveals a linear
trend for the extrema of vs h. This was predicted
by our analytical model (eq ), which states that is dependent on the magnetoelectric polarizability
Re(αc) in the 2D chiral dipole limit. In our system,
Re(αc) is linearly related to h,
because the magnetoelectric polarizability is induced by chiral near-field
coupling between nanorods. The relationship between Re(αc) and h can be understood by comparison to
magnetostatics:[65] due to plasmon hybridization,[66] the plasmon-induced surface charges cause oscillating
currents across the chiral NRD which induce the magnetoelectric dipolar
component. Just as the current density along a circular loop is inversely
proportional to the loop radius, by increasing h in
our chiral NRD system, the effective NRD radius increases and we expect
a decrease in the chiral optical fields, which is well-approximated
as linear in the studied h-regime.
Figure 4
(a) Experimental chirality
flux efficiency ( spectra
for R-NRDs (red) and L-NRDs (blue)
for varying horizontal shifts h. for achiral NRDs is shown at h = 60 nm (black).
Insets: scanning-electron micrographs of a single
NRD in the studied array. (b) Extrema of from part a. A linear trend with respect
to h (dashed lines provide linear fits) is observed.
(c) Extrema of simulated χ̅/|χ̅CPL| evaluated at (0, 0, 0) also show a linear trend with
respect to h (dashed lines provide linear fits).
The data in parts b and c verify analytical calculations (eqs –11) and reveal that h determines
the magnetoelectric polarizability αc in this system.
(d) Numerical colormaps of χ̅/|χ̅CPL| (z = 0 plane) for R-NRDs further confirm the trends
shown in part c.
(a) Experimental chirality
flux efficiency ( spectra
for R-NRDs (red) and L-NRDs (blue)
for varying horizontal shifts h. for achiral NRDs is shown at h = 60 nm (black).
Insets: scanning-electron micrographs of a single
NRD in the studied array. (b) Extrema of from part a. A linear trend with respect
to h (dashed lines provide linear fits) is observed.
(c) Extrema of simulated χ̅/|χ̅CPL| evaluated at (0, 0, 0) also show a linear trend with
respect to h (dashed lines provide linear fits).
The data in parts b and c verify analytical calculations (eqs –11) and reveal that h determines
the magnetoelectric polarizability αc in this system.
(d) Numerical colormaps of χ̅/|χ̅CPL| (z = 0 plane) for R-NRDs further confirm the trends
shown in part c.Further, our analytical
model predicts that the chiral near fields
also depend linearly on Re(αc) (eq ). Indeed, Figure c confirms this numerically for χ̅/|χ̅CPL| evaluated at the NRD center (0, 0, 0) (marked
with ∗ in Figure c). The decrease in near-field optical chirality with increasing h is further illustrated with numerical colormaps of χ̅/|χ̅CPL| for varying h in Figure d. These results allow two important conclusions:
the predominant optical properties of the studied NRD system are dipolar,
and the antenna parameter can predict the enhancement of near-field
optical chirality.Finally, we show that the antenna parameters and enable broad spectral
tunability of chiral
optical fields. Figure a plots experimental spectra for R-NRDs with varying h. In addition to the decrease of shown in Figure , we observe a spectral redshift with increasing h. The experimental wavelengths at which the extrema of occur, shown with respect to h in Figure d, reveal
a linear trend that qualitatively agrees with the simulated in Figure b. Similar
linear shifts have been reported for energy
and have been attributed to changes in the aspect ratio of the structure.[55,67] As expected, comparable behavior is found in the chiral near fields
(Figure c), evaluated
at the R-NRD center (0, 0, 0) (marked with ∗
in Figure c).
Figure 5
(a) R-NRD experimental
chirality flux efficiency () spectra for various horizontal shifts h. A redshift is observed with increasing h. (b) Corresponding simulated spectra are in agreement with experiments
(* indicates the surface lattice resonance). (c) Simulated χ̅/|χ̅CPL| spectra evaluated at (0, 0, 0) for R-NRDs
replicate far-field trends seen in parts a and b. (d) Extrema of the
dominant feature of experimental spectra and simulated chiral antenna aperture
() spectra for various h (dashed lines provide linear fits). As is driven by the surface
lattice resonance,
the redshift is attributed to the increasing surface lattice distance.
The results in part d reveal tunability of chiral fields across the
visible spectrum.
(a) R-NRD experimental
chirality flux efficiency () spectra for various horizontal shifts h. A redshift is observed with increasing h. (b) Corresponding simulated spectra are in agreement with experiments
(* indicates the surface lattice resonance). (c) Simulated χ̅/|χ̅CPL| spectra evaluated at (0, 0, 0) for R-NRDs
replicate far-field trends seen in parts a and b. (d) Extrema of the
dominant feature of experimental spectra and simulated chiral antenna aperture
() spectra for various h (dashed lines provide linear fits). As is driven by the surface
lattice resonance,
the redshift is attributed to the increasing surface lattice distance.
The results in part d reveal tunability of chiral fields across the
visible spectrum.The second antenna parameter (eq ) provides further useful chiral optical information.
Due
to chirality conservation (Table ), the integrated optical chirality dissipation (proportional
to ) is equal to the optical
chirality flux
through the entire surface enclosing the studied structure. Thus,
while we minimize the effect of surface lattice resonances (SLRs)
by evaluating at small angles (SLRs are increasingly
observed at higher angles, as shown in the Supporting Information), the dominant resonances are caused by SLRs in a 2D chiral
system. As we designed our system with an edge-to-edge NRD distance p of 600 nm (see Figure c), the effective surface-lattice-resonance wavelength
increases with increasing h, as shown in Figure d. The spectral SLR
redshift is also seen in the simulated spectra (marked with ∗ in Figure b), while damping
and fabrication imperfections suppress this effect in experiment (Figure a). Indeed, this
SLR redshift confirms our statement with regard to Figure b, where we attributed the
resonance at 600 nm (marked with ∗) to a lattice effect (see
the Supporting Information for further
confirmation). The low-wavelength feature in Figure b, which arises with increasing h, can therefore be attributed to a higher-order lattice mode, explaining
its absence in experiment.[68] Thus, the
tunability shown in Figure d makes it apparent that our combined understanding of and enables the design of
chiral optical fields
across the visible spectrum.In summary, we introduce the optical
antenna approach to chiral
plasmonics to fully characterize and tune antenna-mediated chiral
light with the chiral antenna parameters and . With chirality flux
spectroscopy, a specifically
designed experimental technique to determine , we show that this approach provides valuable
information on chiral near fields that is accessible in the far field.
We verify this principle with simple 2D chiral coupled nanorod dimers
and find that chiral near and far fields are linearly driven by the
magnetoelectric polarizability. In analogy to energetic enhancement
induced by classical optical antennas, this new approach can lead
to optimized chiral optical applications, where highly chiral evanescent
fields enhance the transmission of chiral information from a chiral
receiver to the free radiation field.
Authors: Marco Esposito; Vittorianna Tasco; Francesco Todisco; Massimo Cuscunà; Alessio Benedetti; Mario Scuderi; Giuseppe Nicotra; Adriana Passaseo Journal: Nano Lett Date: 2016-08-31 Impact factor: 11.189
Authors: V K Valev; J J Baumberg; B De Clercq; N Braz; X Zheng; E J Osley; S Vandendriessche; M Hojeij; C Blejean; J Mertens; C G Biris; V Volskiy; M Ameloot; Y Ekinci; G A E Vandenbosch; P A Warburton; V V Moshchalkov; N C Panoiu; T Verbiest Journal: Adv Mater Date: 2014-04-17 Impact factor: 30.849