Infrared spectroscopy is widely used for biomolecular studies, but struggles when investigating minute quantities of analytes due to the mismatch between vibrational cross sections and IR wavelengths. It is therefore beneficial to enhance absorption signals by confining the infrared light to deeply subwavelength volumes comparable in size to the biomolecules of interest. This can be achieved with surface-enhanced infrared absorption spectroscopy, for which plasmonic nanorod antennas represent the predominant implementation. However, unifying design guidelines for such systems are still lacking. Here, we introduce an experimentally verified framework for designing antenna-based molecular IR spectroscopy sensors. Specifically, we find that in order to maximize the sensing performance, it is essential to combine the signal enhancement originating from nanoscale gaps between the antenna elements with the enhancement obtained from coupling to the grating order modes of the unit cell. Using an optimized grating order-coupled nanogap design, our experiments and numerical simulations show a hotspot limit of detection of two proteins per nanogap. Furthermore, we introduce and analyze additional limit of detection parameters, specifically for deposited surface mass, in-solution concentration, and secondary structure determination. These limits of detection provide valuable reference points for performance metrics of surface-enhanced infrared absorption spectroscopy in practical applications, such as the characterization of biological samples in aqueous solution.
Infrared spectroscopy is widely used for biomolecular studies, but struggles when investigating minute quantities of analytes due to the mismatch between vibrational cross sections and IR wavelengths. It is therefore beneficial to enhance absorption signals by confining the infrared light to deeply subwavelength volumes comparable in size to the biomolecules of interest. This can be achieved with surface-enhanced infrared absorption spectroscopy, for which plasmonic nanorod antennas represent the predominant implementation. However, unifying design guidelines for such systems are still lacking. Here, we introduce an experimentally verified framework for designing antenna-based molecular IR spectroscopy sensors. Specifically, we find that in order to maximize the sensing performance, it is essential to combine the signal enhancement originating from nanoscale gaps between the antenna elements with the enhancement obtained from coupling to the grating order modes of the unit cell. Using an optimized grating order-coupled nanogap design, our experiments and numerical simulations show a hotspot limit of detection of two proteins per nanogap. Furthermore, we introduce and analyze additional limit of detection parameters, specifically for deposited surface mass, in-solution concentration, and secondary structure determination. These limits of detection provide valuable reference points for performance metrics of surface-enhanced infrared absorption spectroscopy in practical applications, such as the characterization of biological samples in aqueous solution.
Infrared (IR) spectroscopy is
a powerful analytical technique that provides remarkable insights
into the molecular world. IR light can excite molecular vibrations
whose resonance frequencies depend on the chemical nature of the bonds
as well as their configuration and surroundings.[1] This technique is particularly useful for investigating
the structure and behavior of biomolecules in their native environment,
since it operates without the need for extrinsic labels. For instance,
in proteins, amide bonds make up the backbone of their structure and
can support IR active molecular vibrations such as the amide I and
II bands at around 1650 and 1550 cm–1, respectively.[2] These intrinsic labels can be targeted with IR
sensors to provide chemically specific detection. Beyond the mere
identification of analytes, the amide I absorbance signature can be
analyzed to retrieve information about molecular secondary structure
and conformation.[3] This information, which
can be acquired in real-time, can be enhanced with precise three-dimensional
structures of biomacromolecules obtained with complementary techniques
such as X-ray crystallography and nuclear magnetic resonance (NMR)
spectroscopy.[4]In order to get relevant
insights about biomolecular interactions,
it is often crucial to probe them in physiological conditions, that
is, at low concentrations in aqueous solution or at the submonolayer
level.[5] The requirements of high sensitivity
and water-compatibility can usually not be fulfilled by traditional
IR spectroscopy techniques, in which large sample concentrations are
necessitated and strong vibrational bands of water mask much of the
proteins’ amide I absorption signature, which holds most of
the information related to secondary structure.[6] Surface-enhanced IR absorptin spectroscopy (SEIRAS) can
overcome these limitations by utilizing resonant nanoantennas, which
can strongly enhance the light absorption of near-surface analytes.[7−11] In recent years, the interest in SEIRAS and its application for
biological, chemical, and gas sensing has been increasing with the
use of plasmonic excitations in metallic and graphene resonators as
well as high-Q resonant modes of all-dielectric metasurfaces.[12−15] In metallic IR antennas, the incoming light can be coupled efficiently
due to the large oscillator strength of localized surface plasmon
resonances (LSPR). In contrast to traditional refractometric LSPR
sensors, SEIRAS provides chemical and conformational specificity.In this work, we introduce a plasmonic grating order-coupled nanogap
(GONG) design to probe the limits of detection for protein sensing
and find that we can detect as little as two proteins per nanogap.
To provide reference points for performance metrics of SEIRAS in practical
applications, we present additional sensitivity assessment criteria:
limits of detection for (i) deposited surface mass, (ii) in-solution
concentration, and (iii) secondary structure analysis. We demonstrate
the chemically specific detection of proteins in aqueous solution
with concentrations as low as 100 pg·mL–1 and
resolve their secondary structure content with concentrations down
to 500 ng·mL–1. Conventionally, the analysis
of protein secondary structure using IR absorbance spectroscopy in
aqueous solution is very challenging due to interfering water absorbance
and requires orders of magnitude higher concentrations with traditional
methods.[6] The presented quantitative study
of proteins using optimized resonant antennas shows that SEIRAS can
achieve limits of detection that are highly competitive with other
optical label-free biosensors,[16] with the
additional benefits of chemical and conformational specificity.In our study, gold antennas on an IR-transparent calcium difluoride
(CaF2) substrate are implemented, since this material system
can provide resonances with large excitation cross sections and strong
near-field enhancements required for efficient SEIRAS.[13,17,18] Another advantage of gold is
its biocompatibility with well-established surface functionalization
protocols. Furthermore, on-chip plasmonic nanoantennas allow for straightforward
integration with microfluidics.[18−23] Regarding resonator shape, nanorods are the most common plasmonic
structures for SEIRAS, as they can be tuned to access different spectral
ranges and fabricated easily and reproducibly. Their dipolar-like
shape makes them inherently efficient at generating high electric
near-field enhancements necessary for amplifying molecular vibrations.[24] Given the important role of these antenna systems
in SEIRAS, it is important to maximize their sensing performance.Nanogaps, that is, spacings between plasmonic structures below
a hundredth of the excitation wavelength, can generate strong field
enhancements[25] and are thus interesting
for SEIRAS applications.[26−31] Another effective method for increasing sensitivity is to make use
of the enhancement originating from grating order coupling.[32,33] Traditionally, plasmonic sensing geometries only focus on optimizing
one of these aspects, limiting the available design space. We present
a comprehensive framework for determining an optimal antenna unit
cell geometry that efficiently combines these two enhancement methods
simultaneously. Specifically, we demonstrate the importance of independently
tuning the unit cell x- and y-periodicities
to simultaneously achieve analyte-accessible nanogaps and strong grating
order coupling. Figure a displays a tilted view of a GONG sensor, which consists of unit
cells with nonequal periodicities P and P, each
containing a single rod antenna. As a consequence of this geometrical
arrangement, the nanogaps arise between the adjacent unit cells along
the x-direction of the array. Figure b is a schematic of a nanogap with two streptavidin
proteins in the electromagnetic hotspot region (nanogap surface).
The dimensions of the array parameters can be visualized in Figure c,d, which showcase
SEM micrographs. The gap has a width G = 32 nm and
the periodicities are P = 1516 nm and P =
3204 nm.
Figure 1
(a) 3D model of the grating order coupled nanogap (GONG) antenna
unit cell and array. (b) Schematic representing two streptavidin proteins
localized in a nanogap hotspot in which the electromagnetic fields
are represented in red and blue gradients (not to scale). (c) Scanning
electron microscope (SEM) image displaying the periodicities P and P of a GONG array. (d) SEM image of a nanogap
with a width of G.
(a) 3D model of the grating order coupled nanogap (GONG) antenna
unit cell and array. (b) Schematic representing two streptavidin proteins
localized in a nanogap hotspot in which the electromagnetic fields
are represented in red and blue gradients (not to scale). (c) Scanning
electron microscope (SEM) image displaying the periodicities P and P of a GONG array. (d) SEM image of a nanogap
with a width of G.We obtained the optimized GONG design by performing extensive
numerical
simulations in which we vary both the gap size G as
well as the strength of the grating order coupling, which is controlled
by the parameter P.
Numerical simulations are performed for multiple GONG designs in a
parameter space of gap size and y-periodicity, where
each data point is designated by the pair {G, P}. Specifically, we focus
on gap sizes between 20 and 100 nm, as this encompasses the relevant
range for protein studies (Figure a, bottom). Periodicities are selected so that the
associated lowest frequency grating orders are tuned over the resonance
frequency of the antennas. We benchmark the performance of these {G, P}-sensor
designs by comparing their maximum absorbance for a 5 nm thick model
protein layer placed on the surface of the nanogaps (Figure a, top). The protein layer
is modeled with custom optical constants in order to have its extinction
peak at 1600 cm–1, between the amide I and II bands,
and with the nondispersive component of the refractive index equal
to 1.
Figure 2
(a) Lower panel: Size of exemplary protein structures on a scale
from 20 to 100 nm. From smallest to largest: epidermal growth factor
(David Goodsell, doi: 10.2210/rcsb_pdb/mom_2010_6), IgG antibodies
sandwiching an antigen, fibrinogen (PDB ID: 1M1J,[34]), SMC protein (PDB ID: 5XEI,[35]), tripeptidyl
peptidase II (PDB ID: 3LXU,[36]), kinesin (David Goodsell,
doi: 10.2210/rcsb_pdb/mom_2005_4), and amyloid protofibril (reproduced
in part from Vestergaard et al.[37] under
the Creative Commons Attribution license, CC BY 4.0). Upper panel:
Meshed 3D model of a 30 nm gap with a 5 nm thick model protein film
(pink layer) on the nanogap surfaces as used in the numerical simulations.
(b) Reflectance spectra Rlayer and Rref obtained from numerical simulations of a
{G = 30 nm, P = 3.5
μm} sensor with and without model protein layer, respectively.
The vertical dashed line at the kink indicates the spectral position
of the corresponding grating order. (c) Absorbance spectrum calculated
from the reflectance spectra given in panel b. (d) Heatmap displaying
comparative absorbance strength as a function of gap size G and y-periodicity P. The asterisk indicates the array parameters
used for the calculations in panels a–c. (e) Spectral position
against P for the three
lowest frequency grating orders (dashed curves). The two vertical
dashed lines labeled A and B indicate the critical periodicities for
which each of the two lowest frequency grating orders transitions
from high to low frequency side of the near-field resonance peak at
1600 cm–1 (pink horizontal line) and thereby causes
a transition from evanescent (blue gradient area) to radiative regime
(gray shaded area).
(a) Lower panel: Size of exemplary protein structures on a scale
from 20 to 100 nm. From smallest to largest: epidermal growth factor
(David Goodsell, doi: 10.2210/rcsb_pdb/mom_2010_6), IgG antibodies
sandwiching an antigen, fibrinogen (PDB ID: 1M1J,[34]), SMC protein (PDB ID: 5XEI,[35]), tripeptidyl
peptidase II (PDB ID: 3LXU,[36]), kinesin (David Goodsell,
doi: 10.2210/rcsb_pdb/mom_2005_4), and amyloid protofibril (reproduced
in part from Vestergaard et al.[37] under
the Creative Commons Attribution license, CC BY 4.0). Upper panel:
Meshed 3D model of a 30 nm gap with a 5 nm thick model protein film
(pink layer) on the nanogap surfaces as used in the numerical simulations.
(b) Reflectance spectra Rlayer and Rref obtained from numerical simulations of a
{G = 30 nm, P = 3.5
μm} sensor with and without model protein layer, respectively.
The vertical dashed line at the kink indicates the spectral position
of the corresponding grating order. (c) Absorbance spectrum calculated
from the reflectance spectra given in panel b. (d) Heatmap displaying
comparative absorbance strength as a function of gap size G and y-periodicity P. The asterisk indicates the array parameters
used for the calculations in panels a–c. (e) Spectral position
against P for the three
lowest frequency grating orders (dashed curves). The two vertical
dashed lines labeled A and B indicate the critical periodicities for
which each of the two lowest frequency grating orders transitions
from high to low frequency side of the near-field resonance peak at
1600 cm–1 (pink horizontal line) and thereby causes
a transition from evanescent (blue gradient area) to radiative regime
(gray shaded area).Each {G, P} sensor is adjusted
to provide a near-field resonance maximum
at 1600 cm–1, and the structures are then simulated
both with and without model protein layer in order to obtain the reflectance
spectra (Figure b),
from which we calculate the absorbance spectra (Figure c). Using the maximum absorbance of each
point of the {G, P} parameter space, we generate a heatmap allowing us to compare
the performance of the sensors (Figure d).This map shows that both the gap size and
the y-periodicity strongly influence the performance
of the sensors. Notably,
for a given gap size, we observe that performance is highest for designs
directly to the left of the dashed lines A and B. This behavior can
be understood by considering the position of the lowest frequency
grating modes with respect to the localized resonance frequency of
the antennas. These grating orders λ are commonly accessed at the conditions of i = 0 and j = ±1 and can be described by the
following equations derived from previous works:[38,39]Here, ns is the
refractive index of the antennas’ surroundings, θ is
the incident light’s inclination angle, TE corresponds to transverse
electric, and TM corresponds to transverse magnetic light polarization
(see section 1 in the Supporting Information for more details). These equations confirm that only the y-periodicity of the GONG unit cell needs to be tuned in
order to achieve strong coupling to the grating order at the lowest
frequency. Consequently, P could be freely adjusted to achieve a desired nanogap size G and resonance position, which can be tuned by choosing
the right antenna length L. This results in the following
condition for the x-periodicity of the GONG unit
cell:Using eqs and 2, we can plot
the grating order positions as a function
of P (Figure e). We observe that the lines
A and B correspond to the periodicities for which the grating orders
λ0,–1TE and λ0,±1TM, respectively, transition from the high frequency
to the low frequency side of the antenna’s localized resonance
at 1600 cm–1. Therefore, to maximize both far-field
and near-field responses, we need to place the grating orders with
the lowest frequencies directly at the high frequency side of the
antenna far-field resonance in order to ensure that the antennas are
in an evanescent regime, that is, their interacting electric field
components add in phase to reduce the amount of energy that can escape
the array as electromagnetic radiation.[32]For increasing y-periodicity from 2 to 3.5
μm,
the position of the lowest frequency grating order, that is, λ0,–1TE, approaches
the resonance from the high frequency side (Figure e), until it reaches 1711 cm–1, as can be seen as a kink in the reflectance curve in Figure b (indicated by the vertical
dashed line). The array is thus in a purely evanescent regime, as
opposed to the case when P = 4 μm, for which the position of λ0,–1TE moves
to the low frequency side of the far-field resonance (Figure e), thereby dampening the resonance
in the TE channel and consequently decreasing the sensor’s
overall response (Figure d). For P =
4.5 μm, the position of λ0,–1TE is further in the radiative regime
area, but now we also observe λ0,±1TM at 1644 cm–1, that
is, positioned at the high frequency side of the antenna resonance
(Figure e). This yields
an overall high performance of the sensor, however, not as high as
for P = 3.5 μm.
For P = 5 μm,
the array is in a highly radiative regime which explains the drastically
weakened sensor performance observed for the sensors featuring this y-periodicity value.Within the explored parameter
space, the sensor {G = 20 nm, P = 3.5 μm}
yields the best performance for protein measurements. Consequently,
we choose antenna parameters in the direct vicinity of this combination
to obtain a high-performance sensor compatible with practical considerations
regarding nanofabrication reproducibility and the size of the biomacromolecules.
In particular, a gap size of 32 nm is chosen to accommodate a wider
range of biomolecules with dimensions above 20 nm, such as antibodies
sandwiching an antigen (Figure a), thus making our design broadly applicable to the study
of proteins. Another parameter that influences the performance of
antenna-based sensors is the decay characteristics of the electromagnetic
near-fields around the hotspots. Through full-wave simulations of
the electromagnetic fields, we have estimated the decay length as
125 nm for a {G = 32 nm, P = 3204 nm}-GONG sensor (Figure S4b). This decay range makes the sensors effective for probing
a large range of analyte molecules and changes in the environment.In the following biomolecular studies in dry conditions, {G = 32 nm, P = 3204 nm}-GONG arrays with a size of 200 × 200 μm2 are used for absorbance measurements using Fourier-transform
infrared (FTIR) spectroscopy. To assess the performance of this optimized
design for the detection of protein submonolayers, we perform experiments
in which minute quantities of proteins are bound onto the antennas.
Specifically, a piezoelectric microdispenser is used to spot droplets
of controlled volume containing precise quantities of streptavidin
in phosphate buffered saline (PBS) onto the antenna arrays (Figure a). The dispenser
is equipped with a side camera to accurately measure the droplet size
to be spotted on a specific region and by using this volume and the
number of droplets being spotted, the total mass deposited on each
sensor is controlled. Prior to spotting, the antenna surfaces are
functionalized using biotinylated thiols. This allows us to probe
the limit of amide I absorbance detection for specifically bound proteins
on GONG arrays tuned to have their near-field resonance peaks at the
amide I absorbance peak (Figure S4a).
Figure 3
(a) Schematics
depicting the experimental procedure for the preparation
of chips with bound streptavidin proteins (not to scale) with the
use of a microspotting dispenser. (b) Plot in which the black data
points correspond to the experimentally measured absorbance at the
amide I peak for different amounts of spotted protein mass. The colored
triangular data points correspond to absorbance at the amide I peak
obtained via simulations with different numbers of proteins per nanogap.
(c) Exemplary absorbance curves which showcase the amide I peak. (d)
3D model of the simulation strategy followed to obtain the triangular
data points shown in the plot of panel b. The streptavidin proteins
were homogeneously distributed in the nanogaps and modeled as 4 ×
5 × 5 nm3 blocks with optical constants extracted
from infrared reflection absorption spectroscopy (IRRAS) measurements
(Figure S2b).
(a) Schematics
depicting the experimental procedure for the preparation
of chips with bound streptavidin proteins (not to scale) with the
use of a microspotting dispenser. (b) Plot in which the black data
points correspond to the experimentally measured absorbance at the
amide I peak for different amounts of spotted protein mass. The colored
triangular data points correspond to absorbance at the amide I peak
obtained via simulations with different numbers of proteins per nanogap.
(c) Exemplary absorbance curves which showcase the amide I peak. (d)
3D model of the simulation strategy followed to obtain the triangular
data points shown in the plot of panel b. The streptavidin proteins
were homogeneously distributed in the nanogaps and modeled as 4 ×
5 × 5 nm3 blocks with optical constants extracted
from infrared reflection absorption spectroscopy (IRRAS) measurements
(Figure S2b).Figure b
displays
absorbance at the amide I peak against the spotted protein quantity.
For spotted masses of 99 and 199 pg, the observed amide I absorbance
is very strong compared to the noise level, but for spotted masses
of 6 and 26 pg, we only observe the amide I absorbance peak at 1641
cm–1, just above three times the negative control
signal level (Figure c). By using a surface-functionalization protocol, we ensure that
our measured signals originate from specifically bound proteins. It
is important to note that the measured surface masses are lower than
the spotted mass quantities due to the thorough rinsing steps after
incubation of the protein solutions. Thus, these values are conservative
estimates and the measured signals should be generated from even lower
quantities of analytes. Next, we correlate our measured signals with
the corresponding number of proteins per nanogap using numerical simulations.
We model the streptavidin proteins as blocks of 4 × 5 ×
5 nm3, in agreement with reported streptavidin volumes[40,41] and use optical constants extracted from IRRAS measurements (Figure S2b). In order to not overestimate the
sensitivity of our sensors, we introduce a 1 nm thick layer with refractive
index of 1.4 in between the antenna surface and the protein blocks
to model the biotinylated thiol layer. Furthermore, we do not locate
the blocks at the positions of the highest field enhancement, that
is, the rounded corners and antenna/substrate intersections, but rather
homogeneously space them on the gap surface (Figure d). Given that our antennas have a gap cross
section of 100 × 100 nm2, a maximum of approximately
800 proteins can be bound per nanogap surface area. We find that the
numerical simulations for this case match the experimentally measured
maximal signals very well, and similar results are obtained in the
case of complete antenna coverage with a streptavidin layer (Figure S4c). This confirms that the simulations
are in line with our measurements and that the signal predominantly
originates from proteins within the gaps. From simulations with less
than 800 proteins per nanogap, we can infer that measurements with
spotted quantities of 199, 99, 26, and 6 pg correspond to approximately
128, 50, 8, and 2 proteins per nanogap.Protein studies are
usually conducted in solutions in order to
maintain their native conformational state and biological function,
therefore it is also crucial to establish the concentrations required
for protein detection and secondary structure analysis in aqueous
media. To perform in-solution absorbance measurements, we use {G = 32 nm, P = 3264 nm}-GONG arrays with a size of 200 × 200 μm2Since our CaF2 substrate is highly transparent
in the
mid-IR range, we can illuminate our chips from the backside and integrate
them within custom-made microfluidic devices, as shown in Figure a. By injecting streptavidin
at increasing concentrations, we can establish the curve shown in Figure b. We chose this
additive injection method due to the strong streptavidin–biotin
interaction, which prohibits surface regeneration. The obtained S-shaped
curve covers a large concentration range from 100 pg·mL–1 to 100 μg·mL–1. We fit the data using
a Hill equation-derived fit, which empirically describes the correlation
between the absorbance response A of the biosensor
and the concentration C of the analytes in aqueous
solution:Here, Amin and Amax correspond to
the minimum and maximum absorbance
signals, C0.5 represents the concentration,
which yields , n is an exponent that
is related to binding cooperativity, similarly to the Hill coefficient.[42,43] In our case, we have n < 1 in accordance with
the expected negative cooperative binding behavior. The inset of Figure b shows a zoomed
linear plot for the lowest concentrations ranging from 100 pg·mL–1 to 1 ng·mL–1. The absorbance
signal from an injection of 100 pg·mL–1 streptavidin
corresponds to approximately three times the absorbance signal from
the injection of analyte-devoid buffer (negative control) and, thus,
we can infer that our limit of detection is around 100 pg·mL–1.
Figure 4
(a) Schematic of the in-solution experimental setup with
the fluidic
inlet and outlet as well as the optical path (not to scale). The flow
channel height H of the polydimethylsiloxane (PDMS)
device is 30 μm. The zoomed schematic displays functionalized
gold antennas displaying biotin groups and the captured proteins from
the flowing solution. (b) Plot of absorbance at the amide II peak
for different concentrations of streptavidin. A linear fit is displayed
in the inset and a fit using eq is displayed in the logarithmic plot.
(a) Schematic of the in-solution experimental setup with
the fluidic
inlet and outlet as well as the optical path (not to scale). The flow
channel height H of the polydimethylsiloxane (PDMS)
device is 30 μm. The zoomed schematic displays functionalized
gold antennas displaying biotin groups and the captured proteins from
the flowing solution. (b) Plot of absorbance at the amide II peak
for different concentrations of streptavidin. A linear fit is displayed
in the inset and a fit using eq is displayed in the logarithmic plot.Using the same experimental data set, we can also estimate
the
concentration limit for secondary structure analysis. Information
regarding the secondary structure of proteins is of great interest
for unravelling complex biological processes[44] such as protein misfolding, which play a major role in diseases
including Alzheimer’s and Parkinson’s disease.[45] Conventional IR spectroscopy of proteins in
aqueous solution typically requires concentrations >10 mg·mL–1, which can be very challenging for the study of aggregation-prone
proteins and peptides as well as rare samples.[6] It is thus of great interest to find new methods that can reduce
the necessary concentrations for IR spectroscopy of proteins in aqueous
solution.[46] In fact, it has recently been
shown in a pioneering work that the secondary structure of the protein
α-synuclein, which is involved in Parkinson’s disease,
can be analyzed in aqueous solution and in real-time using nanorod
antennas.[20] The amide I band of proteins
mainly arises from the C=O stretching of its backbone. This
backbone configuration will influence the observed amide I absorbance
spectrum as a consequence of transition dipole coupling between the
different amide group oscillators and the particular hydrogen bonding
patterns. Consequently, amide I absorbance spectra result from the
superposition of sub-bands associated with different secondary structures
present in a particular protein.The secondary structure content
of tetrameric streptavidin extracted
from the current Uniprot database is 47.5% β-strands, 22.4%
disorder, 11.5% helices, and 18.5% loops and turns. The deconvolution
of the absorbance spectrum obtained for a submonolayer of streptavidin
in aqueous solution (Figure a), which was obtained upon injection of 2.65 μg·mL–1, yields a secondary structure content which agrees
well with the database values, that is, we obtain 53.5% β-strands,
16.9% disorder, 11.3% helices, and 18.3% loops and turns. Noticeably,
we observe two bands for the helices centered at 1650 and 1666 cm–1, which are known to correspond to regular α-helices
and 310-helices, respectively (Table ). Furthermore, since in the literature the
spectral position of turns tends to be reported at slightly higher
wavenumbers than the spectral position of loops, we refine our analysis
by associating the band at 1674 cm–1 with loops
and the band at 1679 cm–1 with turns. This yields
contents of 6.6%, 4.7%, 11.1%, and 7.2% for 310-helices,
α-helices, loops, and turns, respectively. These values are
in good agreement with the average values calculated from Meskers
et al.:[47] 55.5% β-strands, 19.4%
disorder, 5.8% 310-helices, 2.5% α-helices, 12.3%
loops, and 4.5% turns.
Figure 5
(a) Deconvoluted absorbance spectrum of a submonolayer of streptavidin
in aqueous solution at a concentration of 2.65 μg·mL–1 for quantitative identification of different secondary
structure motifs, which are listed in the legend on the side. The
pink dotted curve corresponds to the sum of Gaussian peaks which were
used for fitting the experimental data (solid black curve). (b) The
procedure shown in panel (a) is used to obtain the NRMSE for the experimental
absorbance spectra at lower concentrations (colored dots) with respect
to the (scaled) fit of the absorbance spectra shown with colored curves
in the inset. The black dot with the lowest NRMSE corresponds to the
data shown in panel (a).
Table 1
Secondary Structure
Absorption Band
Positions[2,3]
secondary structures
band positions (cm–1)
antiparallel β-strands
1629, 1639, 1693, 1696
disorder
1643
helices
1650, 1666
loops and
turns
1674, 1679
(a) Deconvoluted absorbance spectrum of a submonolayer of streptavidin
in aqueous solution at a concentration of 2.65 μg·mL–1 for quantitative identification of different secondary
structure motifs, which are listed in the legend on the side. The
pink dotted curve corresponds to the sum of Gaussian peaks which were
used for fitting the experimental data (solid black curve). (b) The
procedure shown in panel (a) is used to obtain the NRMSE for the experimental
absorbance spectra at lower concentrations (colored dots) with respect
to the (scaled) fit of the absorbance spectra shown with colored curves
in the inset. The black dot with the lowest NRMSE corresponds to the
data shown in panel (a).By calculating the normalized root-mean-square error (NRMSE)
for
the spectra obtained for lower concentrations (Figure b) with respect to our scaled fit (Figure a), we see that we
can retrieve the secondary structure content with high accuracy down
to 530 ng·mL–1, where the NMRSE remains below
1%. For 160 ng·mL–1, the NMRSE falls in the
range 1–7.5%, which still allows for secondary structure analysis
but with reduced accuracy. For 80 ng·mL–1 the
NMRSE is in the range 7.5–15%, in which it is no longer possible
to reliably quantify the complete secondary structure content. Nonetheless,
it is still possible to retrieve the amide I peak position, which
can be used to draw qualitative conclusions on the dominant secondary
structure motif (antiparallel β-sheet in our case). Such information
can provide important insights into biological processes, for example,
as a means to diagnose prodromal Alzheimer’s disease.[48]Even though our GONG design provides high
sensitivities down to
ng·mL–1 and pg·mL–1 levels,
its performance could still be boosted if an increase in structural
complexity is acceptable. For instance, it has been shown that the
access of the enhanced near-fields to the target analyte can be increased
by placing the plasmonic antennas on pedestals.[49,50] Furthermore, in situations where a more spatially homogeneous near-field
enhancement distribution is desired, other plasmonic designs such
as ones based on annular gaps could be implemented.[28]In conclusion, we have introduced a framework for
designing optimized
nanogap arrays as well as assessing their performance for SEIRAS of
minute quantities of biomolecules. We have used the optimized arrays
for protein experiments and have shown that concentrations as low
as 100 pg·mL–1 can be detected in aqueous solution
using protein-specific absorbance signals and that the secondary structure
can be accurately retrieved at concentrations on the order of 500
ng·mL–1. Our results emphasize the potentials
of SEIRAS and nanoplasmonics for protein studies, as traditional IR
spectroscopy would require orders of magnitude higher concentrations.
In addition to protein analysis, GONG arrays can be adapted to the
study of other classes of biomolecular systems such as lipid vesicles
and exosomes, which currently attract significant interest due to
their relevance to health and disease (Supporting Information, section 8). In this context, it has recently been
shown that nanophotonic platforms based on metallic rods can resolve
complex interaction processes in vesicular systems, such as the toxin-induced
release of neurotransmitter molecules from synaptic vesicle mimics.[18] The versatility of nanorod antennas for the
study of a broad range of biological samples combined with the optimization
principles presented in this work opens up exciting new applications
in fields such as diagnostics and pharmacology.