Information on the polarization properties of scattered light from plasmonic systems are of paramount importance due to fundamental interest and potential applications. However, such studies are severely compromised due to the experimental difficulties in recording full polarization response of plasmonic nanostructures. Here, we report on a novel Mueller matrix spectroscopic system capable of acquiring complete polarization information from single isolated plasmonic nanoparticle/nanostructure. The outstanding issues pertaining to reliable measurements of full 4 × 4 spectroscopic scattering Mueller matrices from single nanoparticle/nanostructures are overcome by integrating an efficient Mueller matrix measurement scheme and a robust eigenvalue calibration method with a dark-field microscopic spectroscopy arrangement. Feasibility of quantitative Mueller matrix polarimetry and its potential utility is illustrated on a simple plasmonic system, that of gold nanorods. The demonstrated ability to record full polarization information over a broad wavelength range and to quantify the intrinsic plasmon polarimetry characteristics via Mueller matrix inverse analysis should lead to a novel route towards quantitative understanding, analysis/interpretation of a number of intricate plasmonic effects and may also prove useful towards development of polarization-controlled novel sensing schemes.
Information on the polarization properties of scattered light from plasmonic systems are of paramount importance due to fundamental interest and potential applications. However, such studies are severely compromised due to the experimental difficulties in recording full polarization response of plasmonic nanostructures. Here, we report on a novel Mueller matrix spectroscopic system capable of acquiring complete polarization information from single isolated plasmonic nanoparticle/nanostructure. The outstanding issues pertaining to reliable measurements of full 4 × 4 spectroscopic scattering Mueller matrices from single nanoparticle/nanostructures are overcome by integrating an efficient Mueller matrix measurement scheme and a robust eigenvalue calibration method with a dark-field microscopic spectroscopy arrangement. Feasibility of quantitative Mueller matrix polarimetry and its potential utility is illustrated on a simple plasmonic system, that of gold nanorods. The demonstrated ability to record full polarization information over a broad wavelength range and to quantify the intrinsic plasmon polarimetry characteristics via Mueller matrix inverse analysis should lead to a novel route towards quantitative understanding, analysis/interpretation of a number of intricate plasmonic effects and may also prove useful towards development of polarization-controlled novel sensing schemes.
Optical properties of noble metal nanoparticles/nanostructures, governed by the so-called
surface plasmon resonance (SPR) effects have evoked intensive investigations in recent
times owing to their fundamental nature and potential applications12.
The SPR can be of two types- propagating at metal-dielectric interfaces, or localized in
the case of metal nanoparticles/nanostructures. The localized plasmon resonances, owing
to their distinctive spectral (wavelength dependent) characteristics and inherent
sensitivity towards local dielectric environment, are being pursued for numerous
practical applications. The applications include, biomedical and chemical sensing,
bio-molecular manipulation, contrast enhancement in optical imaging, surface enhanced
spectroscopy, development of novel nano-optical devices, optical information processing,
data storage, developing polarization measurement devices using plasmonic particles,
plasmonic metasurfaces and so forth123456789101112131415. Besides the potential
applications, a number of interesting and intricate fundamental effects associated with
the interaction of light with specially designed plasmonic nanostructures have also been
observed recently. Spin orbit interaction (SOI) and Spin Hall (SH) effect of light1617, Plasmonic Aharonov-Bohm effect18, optical analogue
of quantum weak measurements in plasmonic systems19, quantum spin hall
effect20, Goos–Hänchen (GH) and
Imbert–Fedorov (IF) shifts in plasmonic structures21, spin
controlled plasmonics22, coupled plasmons and plasmonic Fano
resonances232425, are some of the recently discovered plasmonic
effects having fundamental consequences in diverse areas ranging from quantum, atomic to
condensed matter systems. Knowledge on the polarization properties of the scattered
light is crucial for fundamental understanding of the aforementioned effects because
polarization plays an important role in the light-matter interactions leading to most
(if not all) of these effects. Moreover, the polarization information should also prove
useful for optimizing experimental parameters for many practical applications. For
instance, this can be exploited to develop polarization-controlled novel schemes for
contrast enhancement in biomedical imaging and for optimizing/enhancing sensitivity of
plasmonic sensors3. Although, some inroads in ‘plasmon
polarimetry’ has already been made, these are usually limited to
measurements involving excitation with selected state of polarization and subsequent
detection of the corresponding co- and/or the crossed polarized components of the
scattered light2627. Such approaches, limited by their framework of
obtaining partial information on the polarization transfer, have only proven moderately
successful in selected applications for empirically extracting semi-quantitative
information on the underlying complex nature of the polarized light-matter
interactions232627. But overall, the full potential of
quantitative polarimetry in the context of plasmonics is yet to be realized.
Our theoretical investigations have indicated that recording of full spectral Mueller
matrices should prove to be extremely valuable in this regard28. Mueller
matrix is a 4 × 4 matrix representing the transfer
function of any optical system in its interaction with polarized light and all the
medium polarization properties are characteristically encoded in its various elements.
Recently, such Mueller matrix measurements have been performed in the reflection
geometry from plasmonic crystal sample (large scale periodic array of metallic
nanostructures), and analysis/interpretations of the matrix elements were done via the
Fresnel reflection coefficients and conventional ellipsometry parameters29. Recording of Mueller matrix from plasmonic nanostructures/nanoparticles exclusively
using the scattered light and its inverse analysis via the scattering polarimetry
parameters, on the other hand, should provide new insights and enable quantitative
analysis/interpretation of a number of intricate fundamental effects in plasmonic
systems. Once recorded, the scattering Mueller matrix can be analyzed to
extract/quantify the intrinsic polarization properties of the medium, namely,
diattenuation (differential attenuation of orthogonal polarization states
either by scattering or by absorption) and retardance (phase difference between
orthogonal polarizations)25. These Mueller matrix-derived parameters may
potentially be used to probe and quantify the relative strengths and phases of the
interfering plasmon modes in complex coupled plasmonic systems such as those exhibiting
plasmonic Fano resonance, analyze/interpret SOI and Spin Hall effect, GH and IF shifts
mediated by scattering from plasmonic systems and so forth212830.Despite the wealth of interesting effects that can be probed using spectral scattering
Mueller matrices of plasmonic nanostructures/nanoparticles, its experimental realization
remains to be an outstanding challenge. The challenges include: (1) the scattering
signal from plasmonic nanostructures is rather weak and is often swamped by the large
background unscattered light, (2) recording of full Mueller matrix over a broad
wavelength range simultaneously in combination with the corresponding spatial maps
(spectral Mueller matrix images) by itself is a formidable task, (3) this is confounded
further by the fact polarimetric measurements on plasmonic nanostructures often
necessitates use of high numerical aperture (NA) microscopic setting, (4) challenges in
analysis and quantification of the measured polarization signals or images and
complexities in understanding and interpreting the plasmon polarimetry results. In order
to address these outstanding challenges, in this paper, we present a novel experimental
system that integrates a Mueller matrix measurement scheme with dark-field microscope to
record full 4 × 4 spectroscopic scattering Mueller
matrices from a single isolated nanoparticle/nanostructure. The dark field microscopic
arrangement facilitates detection of weak scattering signal from the plasmonic
nanostructures and has been previously explored for scattering spectroscopic studies on
nanoparticles/nanostructures313233. Here, we integrate an
efficient Mueller matrix measurement scheme and a robust polarization calibration method
with the dark-field microscopic spectroscopy arrangement to facilitate recording of
complete polarization response of a single nanoparticle. Note that there are inherent
complexities of polarization measurements over broad spectral range due to the
wavelength dependent polarization response of the optical components. Moreover, for
polarization measurement in high NA geometry, one needs to account for the polarization
transformation due to the focusing and collection geometry. These problems are
systematically dealt with a robust eigenvalue calibration method. This approach enabled
determination and incorporation of the exact experimental polarization responses of the
polarization state generator/analyzer units (including the effect of the high NA imaging
geometry) over the wavelength range of interest. The developed approach thus facilitates
recording of the spectral polarization response (spectroscopic Mueller matrix)
exclusively of the plasmonic system with desirable accuracy. The experimental
polarimetry system is complemented with Mueller matrix inverse analysis models to
tackle the issues on analysis and quantification of the measured polarization signals
from plasmonic systems. Initial exploration of this ‘comprehensive
plasmon polarimetry platform’ on gold nanorods demonstrates the
promise of the Mueller matrix-derived plasmon polarimetry parameters as novel
experimental metrics for studying a number of interesting plasmonic effects. An
illustrative example is presented on how such information can be utilized to probe,
manipulate, and controllably tune the interference of the neighboring resonant modes
(orthogonal electric dipolar modes in plasmonic nanorods) and the resulting spectral
line shape of the plasmonic system via polarization control.
Results and Discussion
A comprehensive plasmon polarimetry platform, comprising of (a) dark-field
Mueller matrix spectroscopic microscopy experimental system and (b) Mueller matrix
inverse analysis models(shown in Fig. 1), was
explored to record and analyze the spectroscopic (wavelength
λ = 400–700 nm)
scattering Mueller matrices M(λ) from single isolated plasmonic
nanoparticle/nanostructure and other samples. The results of these studies are
presented here. Specifically, we (i) briefly describe the Mueller matrix
construction scheme and the inverse analysis approach, (ii) present
the results of system calibration and (iii) describe the results of spectral
Mueller matrix measurements and inverse analysis on single isolated plasmonic
gold (Au) nanorod samples. The potential utility of such quantitative Mueller matrix
polarimetry on plasmonic system is also illustrated and discussed in this
context.
Figure 1
A schematic of the comprehensive plasmon polarimetry platform.
(a) Dark-field Mueller matrix spectroscopic microscopy system: White
light from the mercury lamp after passing through the PSG unit, is focused
to an annular shape at the sample site using a dark-field (DF) condenser.
PSG: Polarization state generator, PSA: Polarization state analyzer. (P1,
P2): fixed linear polarizers, (QWP1, QWP2): achromatic quarter waveplates.
The sample-scattered light is collected by an objective and passed through
the PSA unit for spectrally resolved signal detection, performed by a
spectrometer (S). The 4 × 4 spectral
scattering Mueller matrices are constructed using sixteen measurements
performed with sixteen optimized combinations of PSG and PSA units.
(b) The Mueller matrix inverse analysis models enable
decomposition of the experimental Mueller matrix into basis matrices of
depolarizing (depolarization matrix) and non-depolarizing (diattenuation and
retardance matrices) effects for subsequent extraction/quantification of the
constituent polarimetry parameters.
Scheme for Mueller matrix construction
The 4 × 4 spectral Mueller matrices were
constructed by combining sixteen spectrally resolved intensity measurements
(spectra) for four different combinations of the optimized elliptical
polarization state generator (using the PSG unit) and analyzer (using the PSA
unit) basis states (see Fig. 1a and Experimental Materials
and Methods). The four elliptical polarization states are generated by
sequentially changing the fast axis of QWP1 to four angles
(ϑ = 35°,
70°, 105° and 140°) with respect to the axis
of P1. These four sets of Stokes vectors
(4 × 1 vector) are grouped as column vectors
to form the 4 × 4 generator matrixW.
Similarly, the four elliptical analyzer basis states are obtained by changing
the fast axis of QWP2 to the corresponding four angles (35°,
70°, 105° and 140°). The analyzer states are
analogously written as a 4 × 4 analyzer
matrix A. The sixteen sequential intensity measurements (at any
wavelength) are grouped in a 4 × 4 matrix
M, which is related to A, W matrices
and the sample Mueller matrix M as,The Mueller matrix M can be determined using known forms of the A
and W matrices asThe optimal generator and the analyzer basis states were obtained via
optimization of the ratio of the smallest to the largest singular values of the
individual square matrices Wand A. The orientation angles of the
quarter waveplates
(ϑ = 35°,
70°, 105° and 140°) were decided based on
this34. In principle, M can be determined from
experimental M, by using theoretical forms of
Wand A matrices (obtained by using the standard Mueller matrices
of the polarizer and the quarter waveplates). However, this is confounded by
– (1) the complex nature of the polarization transformation due to
the high NA imaging geometry leading to significant changes in the
W(λ) and A(λ) matrices; (2) the
W(λ) and A(λ) matrices may vary
significantly with wavelength due to the non-ideal behavior of the polarizing
optics over the wavelength range. We tackled these issues using a robust
eigenvalue calibration method, which takes care of the spectral polarization
responses of the polarization state generator, analyzer units, the focusing and
the detection systems (imaging geometry) by determining the exact experimental
forms of the W(λ) and A(λ) matrices35. Using this approach, the W(λ) and
A(λ) matrices are determined by performing measurements on a
set of ideal calibrating samples (pure diattenuators (polarizers) and retarders
(waveplates)). The specifics of the various steps of this method can be found
elsewhere (see Supplementary information)3435. Note that on
conceptual ground, Mueller matrix is ideally defined for plane waves. However,
for practical purposes, such measurements can be extended towards low/high NA
imaging geometry, where excitation is done using finite beams (even paraxial
beams represent spread in excitation angle) or focused light and the resulting
sample-scattered light is collected over a finite detection angle. In such
situations, if the polarization transformation due to the imaging geometry
(focusing and collection) is appropriately accounted for, the resulting
scattering Mueller matrix should still encode exclusive information on the
sample scattering polarimetry effects integrated over the excitation and the
scattering angles. Since, in our approach, the polarization transformation due
to the high NA imaging geometry is taken care by using the eigenvalue
calibration method, this approach facilitated recording of the spectral
polarization response (Mueller matrix) exclusively of the plasmonic and other
scattering samples. The effect of the excitation/collection geometry on the
Mueller matrix-derived polarimetry parameters of our plasmonic (Au nanorod)
samples are discussed subsequently.
Mueller matrix inverse analysis
In general, plasmonic samples may exhibit all the polarimetry effects, namely,
diattenuation, retardance and depolarization. These may contribute in a complex
interrelated way to the Mueller matrix elements, masking potentially interesting
information and hindering their interpretation. This issue was addressed by
performing inverse analysis on the experimental Mueller matrices using
Polar decomposition method, which is a reliable and widely used approach for
solving the inverse problem in polarimetry36. Using this
approach, the experimental Mueller matrix is decomposed into three basis
matrices corresponding to the three elementary polarimetry effectsHere, M, M and
M describe the depolarizing effects, the
retardance effect (both linear and circular), and the diattenuation effect
(linear and circular) of the medium, respectively (shown in Fig.
1b). The latter two are combined as the
‘non-depolarizing’ diattenuating retarder Mueller matrix
M here. Note that the scattering matrix (defined
in a given scattering plane) for regular shaped scatterer is generally
non-depolarizing and represents a preferentially oriented diattenuating retarder
Mueller matrix for a chosen scattering plane (specified by an azimuthal angle of
scattering)30. However, when excitation and collection of
scattered light is performed over a range of angles (as in high NA imaging
geometry), incoherent addition of the individual (corresponding to each
azimuthal and polar angle of scattering) non-depolarizing Mueller matrices leads
to the depolarization effect (arises due to orientation averaging of
diattenuating retarder Mueller matrices, as discussed subsequently). In our
approach, we have therefore filtered out this depolarized component (where the
intrinsic sample polarization information is scrambled) via
MΔ in Eq. 3, and
extracted the polarized component of the scattered light (via
M). The intrinsic sample polarization
information is therefore contained in the resulting (non-depolarizing)
diattenuating retarder matrix M, which is subjected
to further analysis (results presented subsequently).Once decomposed, the constituent polarimetry parameters depolarization
(Δ), linear diattenuation (d) and linear retardance
(δ) are quantified as36Note that we have not considered circular diattenuation and circular
birefringence effects (which can also be extracted from the decomposed matrices)
due to the achiral nature of our samples. The accuracy of spectral
Mueller matrix measurements in high NA microscopic setting and the ability to
quantify the constituent polarimetry effects from experimental Mueller matrices
were first tested on calibrating sample exhibiting diattenuation and retardance
effects. Following successful calibration, this was explored on single isolated
plasmonic gold (Au) nanorod samples, as described subsequently.
System calibrations results
The results of the eigenvalue calibration on reference samples (linear polarizer
as pure diattenuator and achromatic quarter waveplate as pure retarder) are
summarized in Fig. 2. Note that there are practical
limitations in performing the eigenvalue calibration on the transparent
(non-scattering) reference samples because one can only detect the
sample-scattered light in the exact dark-field configuration. To allow the
detection of signal from the reference samples which are non-scattering elements
(a polarizer and a quarter wave plate) in our case, the collection objective was
kept marginally away from the exact focus thus allowing a very weak leakage
signal in the form of an annular ring from the dark field aperture to be
detected by the spectrally resolved detection unit. This approach adequately
incorporated the wavelength dependent response of the polarizing optical
components and the polarization transformation of the high NA imaging geometry,
by determining the actual experimental W(λ) and
A(λ) matrices, as demonstrated in Fig.
2. The blank (with no sample) Mueller matrices constructed using the
experimental W(λ) and A(λ) matrices in
Eq. 2, nearly resemble identity matrices (Fig. 2a, off-diagonal elements are nearly zero,
≤0.05) over the wavelength range
(λ = 500–700 nm,
shown here). The Mueller matrices of the achromatic quarter waveplate (Fig. 2b) exhibit the expected behavior of a pure linear
retarder over the entire λ-range (characterized by significant
magnitudes of the elements of the lower
3 × 3 block along with the associated
symmetries in the elements). Further, the expected null elements of the retarder
(the elements of the first row and the first column) are also nearly zero (Fig. 2c, elemental error ≤0.05). The values for
linear retardance (δ) and linear diattenuation (d) of
the quarter waveplate and the linear polarizer (respectively) were determined
from their experimental Mueller matrices (using Equation.
4) and are shown in Fig. 2d. The derived magnitudes
of and
d ~ 0.98 (over
λ = 500–700 nm) are
in good agreement with the expected ideal values (
for quarter waveplate and d = 1 for linear
polarizer). Based on these and calibration studies on various other reference
samples, the measurement strategy appears valid for performing accurate sample
Mueller matrix measurements despite numerous complexities associated with the
high NA microscopic imaging geometry that too over a broad wavelength range. The
ability to record full 4 × 4 spectroscopic
Mueller matrices in the dark-field configuration and to quantify the
intrinsic sample polarimetry characteristics bodes well for
quantitative polarimetric investigations on plasmonic
nanoparticles/nanostructures, which is our primary goal.
Figure 2
Results of eigenvalue calibration of the dark-field Mueller matrix
spectroscopic microscopy system.
(a) The experimental spectral
(λ = 500–700 nm)
Mueller matrices for blank (with no sample) nearly resemble the identity
matrices. (b) The spectral Mueller matrices of a calibrating
achromatic quarter waveplate exhibit characteristic behaviour of linear
retarder associated with symmetries in the off-diagonal elements of the
lower 3 × 3 block (highlighted in
redcolour). The Mueller matrices in (a,b) are shown in normalized
unit (normalized by the element M11(λ)).
(c) The expected null elements of the quarter waveplate (the
elements of the first row shown here). (d) The Mueller matrix-derived
(using Eq. 4) linear retardance
δ(λ) (right axis, reddotted line) and linear
diattenuation d(λ) (left axis, bluesolid line) of the
achromatic quarter waveplate and a linear polarizer, respectively.
Mueller matrix studies on plasmonic Au nanorods
Figure 3 displays the results of spectroscopic Mueller
matrix measurements on single isolated Au nanorod. The Au nanorods were
chemically synthesized following the procedure described in Experimental
Materials and Methods37. The average dimensions of the Au
nanorods were as follows:
diameter = 14 ± 3 nm,
length = 40 ± 3 nm,
aspect ratio (ratio of diameter to length)
ε ~ 0.35 (determined from the
SEM image, Fig. 3a). The solution containing the Au
nanorods was diluted adequately so that there was a single isolated nanorod in
the field of view of the dark-field microscopic arrangement (shown in Fig. 3b). Typical scattering spectra recorded from the Au
nanorod (Fig. 3c) exhibits two distinct peaks
corresponding to the two electric dipolar plasmon resonances, one at shorter
λ (transverse resonance along the short axis at
λ ~ 525 nm) and the
other at longer λ (longitudinal resonance along the long axis at
λ ~ 650 nm)38. The corresponding scattering Mueller matrices
M(λ) exhibit several interesting spectral trends (Fig. 3d). The complicated nature of M(λ)
with essentially all sixteen non-zero matrix elements underscore the fact that
even a single isolated plasmonic Au nanorod exhibit all the elementary
polarimetry characteristics (diattenuation, retardance and depolarization), thus
highlighting the need for Mueller matrix inverse analysis. The
considerably low magnitudes of the diagonal elements
(M, M and
M) imply overall strong depolarizing nature
of the scattered light. Non-zero intensities of the elements in the first row
and the first column
(M/M,
M/M), on the other
hand, is a manifestation of the linear diattenuation effect. Strong signature of
the linear retardance effect is also evident from significant intensities of the
off-diagonal elements in the lower 3 × 3
block of M(λ)
(M/M and
M/M representing
retardancefor horizontal/vertical and
+45°/−45° linear polarizations
respectively). The spectral trends of the effects are gleaned further and become
more evident in the decomposed (using Equation. 3) basis
matrices, the depolarization effect in the matrix
−MΔ(λ) (Fig. 3e) and the diattenuation and retardance effects in the
non-depolarizing matrix-M(λ) (Fig. 3f). The observed linear diattenuation in the plasmonic
nanorods originates from the differential excitation of the two orthogonal
dipolar plasmon resonances (transverse and the longitudinal) by orthogonal
linear polarizations. Linear retardance, on the other hand, is a manifestation
of the inherent phase retardation between the two competing dipolar plasmon
modes28. As previously discussed, that under plane wave
excitation, the scattering Mueller matrix from preferentially oriented plasmonic
nanorod should be non-depolarizing (diattenuating retarder) in nature. However,
unlike ideal plane wave excitation, here the nanorod is excited by focused light
beam and the scattered light is also detected in high NA imaging geometry (using
an objective lens). This leads to orientation averaging (orientation of the axis
of the rod with respect to the illuminating polarization) and averaging over
several forward scattering angles (decided by the NA of the objective) and
scattering planes (azimuthal angles of scattering). The resulting incoherent
addition of diattenuating retarder Mueller matrices (representing intensities
corresponding to the individual constituent polarization preserving scattered
fields) eventually manifest as depolarization effect. It is evident from the
magnitudes of the diagonal elements of the decomposed depolarization matrix
MΔ(λ) (Fig.
3e) that despite the high NA imaging geometry,
~30–40% of the detected light is still polarized (on an
average the polarized fraction is
~[1 − Δ], with
maximum magnitude of
Δ(λ) ~ 0.65, see
subsequent Fig. 4a). The resulting (non-depolarizing)
diattenuating retarder matrix M (which contains
intrinsic sample polarization information) can therefore be used to reliably
extract the scattering-induced diattenuation and the retardance effects, and may
also be relevant for further analysis on the polarized component of the
scattered light.
Figure 3
Results of spectroscopic Mueller matrix measurements on single isolated Au
nanorod.
(a) SEM image of Au nanorods. (b) Dark-field image of a single
Au nanorod. (c) Typical scattering spectra (with un-polarized
excitation, corresponding to M11(λ) element)
recorded from the Au nanorod exhibits two distinct peaks corresponding to
the two (transverse and longitudinal) electric dipolar plasmon resonances.
(d) The spectral scattering Mueller matrices
M(λ) of the Au nanorod exhibit characteristic features of
the constituent elementary polarimetry properties - depolarization reflected
in the diagonal elements (black); diattenuation in the first row and column
(blue); linear retardance in the off-diagonal elements of the lower
3 × 3 block (red). (e,f) The
wavelength dependence of the decomposed(using Eq. 3)
basis matrices encoding the depolarizing (in depolarization matrix
−MΔ(λ)) and the
non-depolarizing (in diattenuating retarder
matrix-M(λ)) effects. All the
matrices are shown in normalized unit (normalized by
M11(λ)).
Figure 4
The results of the inverse analysis on the spectral scattering Mueller
matrices M(λ) of the Au nanorod (corresponding to Fig. 3).
(a) The Mueller matrix-derived wavelength variation of the linear
retardance δ(λ) (right axis, red dotted line)
and linear diattenuation d(λ) (left axis, blue solid
line) parameters. The inset shows wavelength variation of the
decomposition-derived depolarization coefficient
Δ(λ). (b) The corresponding theoretically
computed d(λ) and δ(λ)
parameters for a preferentially oriented similar Au nanorod, under plane
wave excitation. (c) The spectral line shapes of the scattered
intensity I(λ) for excitation with
−45° linear polarization (M) and subsequent
detection using +45° (P) analyzer basis (blue solid line) and
without any analyzer (polarization-blind detection, black dotted line). The
strength of the interference signal
(I(λ)) is displayed in the inset,
wherein a cartoon of the polarization state generator and the analyzer is
also displayed.
Interestingly, despite such high NA imaging geometry, the intrinsic spectral
characteristics of the linear diattenuation and the retardance effects of single
plasmonic nanorod are preserved. This is illustrated in Fig.
4a, wherein the decomposition-derived (using Equation.
4) linear diattenuation d(λ) and linear retardance
δ(λ) parameters are displayed. Whereas the
magnitude of d(λ) peaks at the wavelengths corresponding to
the two orthogonal dipolar plasmon resonances
(λ ~ 525 nm for the
transverse and ~650 nm for the longitudinal), the
magnitude of δ(λ) attains its maximum value at
the spectral overlap region of the two resonances
(λ ~ 575 nm). For
comparison, the theoretically computed (using T-matrix approach39) scattering Mueller matrix-derived d(λ) and
δ(λ) parameters for a preferentially oriented
Au nanorod (having similar dimension as the experimental one) under plane wave
excitation, are displayed in Fig. 4b. The spectral
behavior of the experimental d(λ) and
δ(λ) parameters are in good agreement to the
corresponding theoretical predictions. The corresponding wavelength dependence
of the derived depolarization coefficient Δ(λ) is shown
in the inset of Fig. 4a. The observed intriguing spectral
diattenuation and retardance effects can be interpreted via the relative
amplitudes and the phases of the two orthogonal dipolar plasmon polarizabilities
of the Au nanorod. In the dipole approximation (valid for scatterer dimension
a ≪ λ), the two
orthogonally polarized amplitude scattering matrix elements (representing the
scattered fields) of the nanorod can be modeled as s
∝
α cos θ
and s ∝
α, where
α and
α are the longitudinal and the
transverse dipolar plasmonpolarizabilities, respectively, and
θ is the scattering angle38. The
diattenuation d and the linear retardance δ parameters
are linked to the two competing resonant polarizabilities as28As apparent from Eq. 5, the magnitude of
δ is directly related to the phase difference between the
two orthogonal dipolar plasmon polarizabilities (longitudinal
α and transverse
α). The diattenuation, on the
other hand, is primarily determined by the relative strengths of the two
orthogonal dipolar plasmon polarizabilities
(|α| and
|α|).
Information on the relative strengths and phase differences between the two
resonant plasmon polarizabilities are therefore characteristically encoded in
the d(λ) and δ(λ) parameters,
respectively. Note that in the dipolar approximation, the magnitude of
δ does not depend on the polar scattering angle
θ or angle of excitation (exclusively related to the
phase difference between the two intrinsic plasmon modes). The magnitude of the
parameter d would however, weakly depend on the scattering angle
θ also (thus on the choice of the excitation/scattering
direction) because of the cos2 θ
factor associated with dipolar scattering. In conformity with this, while the
computed δ parameters for the Au nano-rod shows no angular
dependence, the magnitude of d varies weakly with increasing forward
scattering angle θ (see the computed angular dependence of
the d and δ parameters for Au nano-rod, Supplementary
Figure S1). The magnitude of the derived δ(λ)
parameter is accordingly reasonably close to the theoretical prediction for
preferentially oriented Au nano-rod under plane wave excitation (Fig. 4a,b). The magnitude of the d(λ) parameter,
on the other hand, is lower than the corresponding theoretical predictions
(Fig. 4a,b), as averaging over forward scattering
angles affects this parameter. Importantly, the characteristic plasmonic
spectral behaviour of the d(λ) and
δ(λ) parameters are retained because these are
directly linked to the relative strengths of the orthogonal dipolar plasmon
polarizabilities and phase difference between them, respectively.The ability to capture and quantify unique information on the relative strengths
and the phases of the contributing plasmon resonance modes via the wavelength
dependence of the d(λ) and
δ(λ) parameters may open-up interesting new
avenues for the analysis/interpretation of the interference of the neighboring
modes in coupled plasmonic structures. An illustrative example of this for the
Au nanorod is demonstrated in Fig. 4c (corresponding to
the Mueller matrices of Fig. 3f). The results are
displayed for excitation with −45° linear polarization
(denoted by M) and subsequent detection of the scattered light intensity
(I(λ)) with +45°
analyzer basis state (denoted by P) and that without any analyzer
(polarization-blind detection). For the sake of comparison, the spectral line
shapes of I(λ) (normalized by the total
intensity ) rather than the absolute values of the
detected intensities are shown (as expected for the polarization preserving
component of the scattered light, the detected cross-polarized M-P component was
much weaker in intensity than the polarization-blind detected M-Unpol
component). Polarization blind detection leads to no interference effect of the
two plasmon resonance modes, leading to mere addition of scattered intensities
of the two modes (the detected signal is typically
I(λ) ~ |s(λ)|2 + |s(λ)|2).
Projection of the scattered light into +45° linear polarization
basis detection, on the other hand, leads to contribution of the interference
signal [ as encoded in the Mueller matrix elements
M33(λ)/M44(λ)]
in addition to the scattered intensity contributions of the two individual
plasmon modes
[|s(λ)|2 + |s(λ)|2].
The appearance of the interference signal leads to distinct changes in the
spectral line shape, manifesting as an asymmetry in the resulting line shape
(Fig. 4c). The corresponding strength of the
interference signal and its wavelength dependence
I(λ) is separately shown (in relative
units) in the inset of Fig. 4c. These results initially
demonstrate the potential utility of the spectral scattering Mueller matrices
M(λ) and the derived d(λ) and
δ(λ) polarization parameters for probing,
manipulating and controllably tuning the spectral interference effect in a
simplest possible plasmonic system. Its potential applications on more complex
coupled plasmonic structures (such as those exhibiting plasmonicFano
resonances202122) can now be envisaged.
Conclusions
To summarize, a novel experimental system is developed for the recording of full
4 × 4 spectroscopic scattering Mueller matrices
from single isolated plasmonic nanoparticle/nanostructure. The system overcomes the
outstanding issues pertaining to reliable measurements of weak scattering
polarization signals from nanoparticle/nanostructures over broad spectral range that
too in high NA imaging geometry, by integrating an efficient Mueller matrix
measurement scheme and a robust eigenvalue calibration method with a dark-field
microscopic spectroscopy arrangement. Feasibility of quantitative Mueller matrix
polarimetry using the developed system is illustrated on a simple plasmonic
system, that of gold nanorods. To the best of our knowledge, this is the first ever
report on quantitative Mueller matrix polarimetry on plasmonic systems. The results
revealed intriguing spectral diattenuation d(λ) and retardance
δ(λ) effects from single isolated plasmonic Au
nanorod, as quantified via Mueller matrix inverse analysis. It is demonstrated
further that these Mueller matrix-derived plasmon polarimetry parameters,
d(λ) and δ(λ) encode potentially
valuable information on the relative strengths (amplitudes) and phases of competing
neighboring resonant modes in plasmonic structures. These polarimetry parameters
therefore hold considerable promise as novel experimental metrics for the
analysis/interpretation of a number of interesting plasmonic effects; for instance,
these can be used to probe, manipulate and tune the interference of the neighboring
modes in complex coupled plasmonic structures, to study SOI30, Spin
Hall effect and other polarization-dependent shifts in plasmonic structures21, to optimize/develop polarization-controlled novel plasmonic sensing
schemes, and so forth. We are currently expanding our investigations in these
directions. In general, the unprecedented ability to record full polarization
information over a broad wavelength range and to quantify the intrinsic polarimetry
characteristics from even a single isolated nanoparticle/nanostructure may prove
useful for spectro-polarimetric characterization of a wide class of complex nano
materials.
Experimental Materials and Methods
Mueller matrix experimental system
The experimental system (shown in Fig. 1a) is capable of
acquiring full 4 × 4 spectroscopic
scattering Mueller matrices from single isolated plasmonic
nanoparticle/nanostructure over a broad wavelength range
(λ = 400–700 nm).
The system essentially comprises of three units- conventional inverted
microscope (IX71, Olympus) operating in the dark-field imaging mode,
polarization state generator (PSG) and polarization state analyzer (PSA) units,
and spectrally resolved signal detection (spectroscopy) unit. Collimated white
light from a mercury lamp (U-LH100L-3, Olympus) is used as an excitation source
and is passed through the PSG unit for generating the input polarization states.
The PSG unit consists of a horizontally oriented fixed linear polarizer P1 and a
rotatable achromatic quarter waveplate (QWP1, AQWP05M-600, Thorlabs, USA)
mounted on a computer controlled rotational mount (PRM1/M-27E, Thorlabs, USA).
The PSG-emerging light is then focused to an annular shape at the sample site
using a dark-field condenser (Olympus U-DCD, NA = 0.92).
The sample-scattered light is collected by the microscope objective (MPlanFL N,
NA = 0.8), passed through the PSA unit (for the analysis
of the polarization state of the scattered light) and is then relayed for
spectrally resolved signal detection. The dark-field arrangement facilitates
detection of exclusively the sample-scattered light (scattering spectra). The
PSA unit essentially comprises of the same polarization components with a fixed
linear polarizer (P2, oriented at vertical position) and a computer controlled
rotating achromatic quarter waveplate (QWP2), but positioned in a reverse order.
Spectrally resolved signal detection is performed by a spectrometer (HR 2000,
Ocean optics, USA). This enables recording of scattering spectra
(λ = 400–700 nm)
with a resolution ~1.5 nm. The spectra were recorded
with an acquisition time of ~0.05s and for each polarization
resolved measurements averaging were done over 100 spectra.The salient advantages of the experimental system are worth a brief mention.
First of all, the issues pertaining to polarization measurements over broad
spectral range and the polarization transformation due to the high NA imaging
geometry are tackled by determining the actual experimental
W(λ) and A(λ) matrices (over
λ = 400–700 nm).
Secondly, this measurement scheme is independent of the polarization response of
the spectrometer (detector) and the source, since it uses fixed linear
polarizers at both the excitation (P1-horizontal) and the detection
(P2-vertical) end. Finally, the entire experimental system is automated using
Labview for easier and faster data acquisition. The system is capable of
recording the spectroscopic Mueller matrices by using the spectrometer.
Plasmonic sample preparation
Gold (Au) nanorods were synthesized as described in the literature by Babak et
al.37. All the chemicals like tetrachloroauric acid
(HAuCl4.3H2O), L-ascorbic acid, silver nitrate
(AgNO3) sodium borohydride (NaBH4) and CTAB
(cetyltrimethylammonium bromide) were procured from Sigma-Aldrich. The entire
reaction was carried out in two parts at room temperature. In the first part, we
synthesized the seed solution by mixing both 5 mL of 0.2 MolCTAB and
5 ml of 0.5 mMol HAuCl4 solutions. Then
0.6 ml of ice-cold 0.01 Mol NaBH4 was added to the above
mixture under continuous stirring for 5 min which produces seed
solution with nanoparticles of size less than 10 nm. The second part
is about the preparation of growth solution where we would like to grow Au
nanorods from the existing nanoparticles in seed solution. Growth solution is
prepared by mixing 5 ml of 0.2 Mol CTAB, 5 ml of
1 mMol HAuCl4, 150 μl of 0.0064
Mol AgNO3, and 85 μl of 0.0788 Mol L-ascorbic
acid. To obtain the required size of Au nanorods, 36 μl
of seed solution was mixed with the growth solution under continuous stirring
for 1 hour. Au nanorod images were recorded by a Zeiss SUPRA
55VP-Field Emission Scanning Electron Microscope (FE-SEM) by spin coating the Au
nanorod solution on a clean silicon (100) substrate. For the Mueller matrix
spectroscopic and imaging studies, the samples were diluted as required and then
fixed on a glass cover slip by spin coating (Apex Instrumentation, spinNXG -
P1), which was then kept at the sample stage of the dark-field microscopic
arrangement.
Additional Information
How to cite this article: Chandel, S. et al. Complete polarization
characterization of single plasmonic nanoparticle enabled by a novel Dark-field
Mueller matrix spectroscopy system. Sci. Rep. 6, 26466; doi:
10.1038/srep26466 (2016).
Authors: Stefan A Maier; Pieter G Kik; Harry A Atwater; Sheffer Meltzer; Elad Harel; Bruce E Koel; Ari A G Requicha Journal: Nat Mater Date: 2003-04 Impact factor: 43.841