Azeem
Ahmad
ab,
Vishesh
Dubey
ab,
Vijay Raj
Singh
cd,
Jean-Claude
Tinguely
a,
Cristina Ionica
Øie
a,
Deanna L.
Wolfson
a,
Dalip Singh
Mehta
b,
Peter T. C.
So
cd and
Balpreet Singh
Ahluwalia
*a
aDepartment of Physics and Technology, UiT The Arctic University of Norway, Tromsø N-9037, Norway. E-mail: ahmadazeem870@gmail.com; balpreet.singh.ahluwalia@uit.no
bDepartment of Physics, Indian Institute of Technology Delhi, New Delhi 110016, India
cDepartment of Mechanical & Biological Engineering, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
dBioSym IRG, Singapore-Alliance for Science & Technology Center, Singapore, Singapore
First published on 22nd August 2018
Red blood cells (RBCs) have the ability to undergo morphological deformations during microcirculation, such as changes in surface area, volume and sphericity. Optical waveguide trapping is suitable for trapping, propelling and deforming large cell populations along the length of the waveguide. Bright field microscopy employed with waveguide trapping does not provide quantitative information about structural changes. Here, we have combined quantitative phase microscopy and waveguide trapping techniques to study changes in RBC morphology during planar trapping and transportation. By using interference microscopy, time-lapsed interferometric images of trapped RBCs were recorded in real-time and subsequently utilized to reconstruct optical phase maps. Quantification of the phase differences before and after trapping enabled study of the mechanical effects during planar trapping. During planar trapping, a decrease in the maximum phase values, an increase in the surface area and a decrease in the volume and sphericity of RBCs were observed. QPM was used to analyze the phase values for two specific regions within RBCs: the annular rim and the central donut. The phase value of the annular rim decreases whereas it increases for the central donut during planar trapping. These changes correspond to a redistribution of cytosol inside the RBC during planar trapping and transportation.
Deformation of the red blood cells has been used for studying several diseases previously. Conventionally, the deformability of RBCs is studied using non-optical techniques such as micropipette aspiration and micro-fabricated channels.9–12 More recently, optical methods such as optical tweezers13–16 have been used to exert optical forces onto single RBCs and the response of optical forces/pressure on RBCs is studied using either bright field microscopy or fluorescence-based microscopy. Previous studies on RBC deformability have utilized techniques such as microfluidics17 or optical tweezers15,18 to simulate some of the forces encountered in vivo. With optical tweezers, a tightly focused laser beam uses force from the refractive bending of light to trap biological specimens in three-dimensions. Further, laser tweezers are more suited for studying single cells at a time.
Over the past decade, planar waveguide trapping (WT) has emerged as an alternative tool to optical tweezers for on-chip manipulation and propulsion of micro-particles, gold nano-particles, and various biological objects (e.g. cells, bacteria and viruses) on the top of waveguide surfaces.19–24 In contrast to the focused beam of traditional optical tweezers, WT works using an evanescent light field, which is generated from totally-internally reflected (TIR) light guided through a path of high refractive index contrast on a semiconductor chip. Trapping occurs due to the exponential decay of the evanescent field relative to the waveguide surface, which generates a vertical gradient force (Fx) that pulls a refractive objective (e.g. a cell) downwards towards the waveguide surface. A lateral gradient force (Fy) is generated across the waveguide, acting as a restoring force to keep the cells trapped on the waveguide. The radiation pressure of light propagating through the waveguide results in a forward scattering force along the length of the waveguide (Fz), and provides a forward push to propel the cells along the waveguide. Thus, while Fx and Fy stably trap the cells on top of the waveguide, Fz propels the cells slowly along the Z-axis shown in Fig. 1(b).
The capability of WT to trap large cell populations and its compatibility with microfluidics make it an ideal candidate to mimic the flow of RBCs in microcapillaries.25 Microfluidic devices have also been used for sorting and characterization of cells based on their size and stiffness contrast.26,27 Recently, it was shown that WT can be a useful tool for the assessment of the health or deformation of RBCs.25 In addition, this technique was also used to quantify the minute loss of RBC deformability during blood storage.16 More importantly, the optical forces imparted during waveguide trapping are in the order of 10 pN, in contrast to 50–400 pN (ref. 15, 25 and 28) optical forces being applied using laser tweezers. Besides being gentler, the optical forces imparted by the optical waveguide are spread over large surface areas in lateral dimensions (determine by the width of the waveguide) and are limited by the penetration depth of the evanescent field of the waveguide (typically 200 nm) in the axial direction. It was recently demonstrated that to detect the subtle loss of deformation of RBCs during blood storage lesion, it is necessary to impart minute optical forces.25 The optical force of around 10 pN imparted using the optical waveguide was found to be sufficient to detect a minute loss of deformability of RBCs within the first 10 days of blood storage.25
However, in the previously published paper, only bright field microscopy was used to investigate RBC deformation which did not provide any quantitative information during RBC deformation.25 The main motivation of this work is to integrate methodologies that can be used to a) trap and propel RBCs using minute optical forces from the planar waveguide; and b) can simultaneously obtain quantitative information about the RBCs during cell trapping and deformation.
Given the limitations of bright field microscopy, the combination of quantitative phase microscopy (QPM) and WT has high potential due to the ability to obtain label-free images and quantitative information about different parameters of biological cells. QPM is an emerging tool for studying weakly scattering and absorbing biological specimens.29 It provides information about the phase shift, i.e., the optical path length (OPL) distribution produced by the specimen with respect to the surrounding medium. The optical path length contains the local information about the cell's refractive index and thickness. The phase shift is further used to determine various optical parameters of the specimen, such as cell's membrane fluctuations and non-aqueous content, i.e., dry mass density of cells.30,31 Due to the ease of obtaining the interference pattern quickly, a number of non-common path and off-axis QPM methods based on coherent light sources have been developed for the quantitative phase measurement of living cells.32–36 In the off-axis set-up, the reference and the signal beams travel different light-paths. Furthermore, several other common-path QPM imaging techniques, such as diffraction phase microscopy (DPM),37 spatial light interference microscopy,38 and common-path diffraction optical tomography,39,40 have also been introduced for the quantitative measurement of different cell's parameters such as morphological, chemical, and mechanical parameters.
A phase microscopy set-up that is compatible for integration with the waveguide-trapping set-up was explored. In WT, the sample stage holding the waveguide is kept stationary during the image acquisition and the microscope is translated to capture the images of specimen during trapping and propulsion. However, in the conventional phase microscopy set-up, the microscope is kept stationary and only the sample is translated. Moreover, the phase microscopy set-up should be built in reflection mode as the waveguide chips are fabricated using opaque silicon substrates. In the present work, we developed a Linnik interferometer based reflection type QPM setup. As the Linnik interferometer is a compact reflection type QPM setup, its integration with WT is relatively straightforward. A Linnik interferometer has the capability to record off-axis holograms, which enables single shot Fourier transform based phase recovery of biological specimens and thus enables fast acquisition of the cell propulsion on top of the waveguide surface. By acquiring time-lapsed interferograms, the phase images and the morphological variation of the RBCs during the entire trapping process were obtained. The integrated WT and Linnik interferometric based QPM (WT-QPM) set-up was further employed for the quantitative measurement of various morphological parameters of the RBCs such as the surface area, volume, and sphericity during planar trapping and propulsion near the waveguide surface.
For efficient trapping, it is desirable to have a high intensity in the evanescent field. This is achieved by fabricating thin optical waveguides (150 nm thick) made of high refractive index contrast materials. Here, optical waveguides were made of tantalum pentoxide (Ta2O5),42 which has a refractive index of 2.1. The Ta2O5 platform possesses low auto-fluorescence and low propagation losses and has been previously employed for trapping of living cells.25
For on-chip manipulation, generally two different waveguide designs are used: strip and rib waveguides (Fig. 1(b and c)). Strip and rib waveguides were fabricated by sputtering a guiding layer Ta2O5 onto a silica (Si) layer followed by photolithography and argon ion-beam milling.42 For strip waveguides, the Ta2O5 layer (ncore = 2.1) had a thickness ‘H’ of 220 nm, and was completely etched down to the Si layer (n = 1.45). For the rib waveguides, the Ta2O5 layer is only partially etched down with different thicknesses ‘h’ of 4, 8, 20, 50, and 150 nm leaving a final slab thickness of ‘t’. A similar procedure was followed for the fabrication of 20 and 220 nm height waveguides having different widths ‘w’ of 2.5, 3, 4, 5, and 10 μm. More details on the optimization of waveguide fabrication can be found elsewhere.43
To measure the capability of the proposed technique for the quantification of small morphological changes, experiments were conducted on a standard flat mirror and a waveguide substrate. The spatial phase/height measurement sensitivity of the QPM setup was characterized by acquiring interferometric images using a flat mirror and a waveguide substrate as a test specimen. The peak to valley (P-V) spatial phase29 of the system for the standard flat mirror is found to be equal to 143 mrad, whereas it is measured to be equal to ∼313 mrad during optical trapping, which corresponds to the height measurement accuracy of 16–20 nm. This is further confirmed experimentally by employing the system for the height measurement of the 20 nm rib height waveguide. The 20 nm rib height of the optical waveguide is not visible, i.e., embedded with phase noise of the system, in the reconstructed RBC phase map (see ESI† Fig. S1–S3). A systematic study about the measurement capability, i.e., z resolution, of the system can be found in the ESI† note. Fourier transform-based image processing was used to retrieve the phase information of the specimen from the interferometric images. Additional information about retrieval of phase information is discussed in the ESI.†
To overcome this challenge, we have systematically investigated different waveguide geometries (rib and strip) and parameters (width and thickness). Fig. 1(b and c) show the schematic diagram of strip and rib waveguides. The core layer is completely etched for a strip waveguide while it is only partially etched for a rib waveguide as shown in Fig. 1c. A rib waveguide has a slab region (depicted as h in Fig. 1c) beneath the shallow rib region (depicted as t in Fig. 1c). The total thickness of a strip and a rib waveguide is denoted by H and t + h in Fig. 1(b and c), respectively. Both strip and rib waveguides have been used in the past for optical trapping applications.22,24 ESI† Fig. S4 and S5 show the phase map of RBCs placed on top of rib and strip waveguides with varying widths. Shallow rib waveguides are more suitable than the strip waveguides due to reduced phase noise of the waveguide core layer. To systematically study the influence of the waveguide core on phase noise, experiments on waveguides with varying waveguide rib height (h in Fig. 1c) were performed. ESI† Fig. S6 shows the phase map of RBCs placed on top of a rib waveguide as a function of the rib height for a given width of 2.5 μm. The waveguide with a rib height (h) of up to 50 nm could be used to reconstruct the RBC phase without appreciable phase noise from the waveguide. The intensity in the evanescent field decreases with decreasing rib height. Thus, a compromise must be made such that there is a high intensity in the evanescent field with little phase noise from the waveguide core. The shallow rib waveguide avoids unwanted phase information and consequently the phase artifacts during cell propulsion. In addition, the shallow rib height was shown to have lower propagation losses as compared to the strip waveguides.42 The rib waveguide with a rib height of 20 nm and a width of 3 μm was used for the remaining work.
In order to determine the defocus distance, first, the complex field retrieved from the Fourier transform method is numerically propagated across the range of −15 μm to +15 μm. Then amplitude variance is calculated corresponding to each propagated field and plotted as a function of the propagation distance. The minimum of the amplitude variance vs. propagation distance plot gives information about the defocus distance or true focal plane of the objective lens. Further, the complex field is propagated by the above calculated defocus distance using the angular spectrum approach to acquire accurate RBC phase information. Similar steps were followed for each interferometric frame of the recorded movie. The detailed information about the algorithm can be found elsewhere.45 Further, the influence of defocus on the quantitative phase measurement of RBCs is shown in ESI† Fig. S7.
Fig. 2 Time lapsed interferometric and quantitative phase images of RBCs propelling along the length of the waveguide. The horizontal red color lines are drawn to depict the position of the waveguide. The color bar is in radians. Associated ESI† Movie (Video S2). The phase of the trapped RBCs is only computed in the right column. |
To further quantify the phase variation and to minimize the experimental and processing errors, for example, due to hot spots in the phase images, the RBC was divided into four quadrants as shown in Fig. 3a. The maximum phase (φmax) value of each quadrant is calculated and then the average maximum phase value of the all four quadrants is determined, thus reducing the errors from any hot-spots. Fig. 3b depicts the 3D view of the reconstructed RBC phase map.
Fig. 3c shows the variation of the φmax value of the RBC as a function of time of the experiment shown in Fig. 2. During the first 14 s when the laser was switched off, only a small variation in the φmax value of the RBC (∼0.14 rad) was observed. This small phase variation could be due to Brownian motion or thermal fluctuation of the RBC. At t = 14 s, the laser is switched on and the φmax value of the RBC starts to decrease gradually. At the end of the movie, i.e. at t = 40 s, the maximum phase value of the RBC decreased to ∼1.92 rad (Fig. 3c). The difference (φdiffmax = φtrappedmax − φuntrappedmax) between the φmax value between the trapped (φtrappedmax) and untrapped φuntrappedmax RBCs is found to be ∼1.35 rad. It is quite evident that the decrease in the φmax value (∼1.35 rad) due to the trapping laser is much larger compared to the phase variation due to the Brownian motion or thermal fluctuation of the RBC (∼0.14 rad) when the laser was switched off.
Fig. 3d shows the whisker box plot of the maximum phase value (φmax) for laser off and on conditions of the same cell. The whisker box plot highlights that when the laser is switched on, the maximum phase value of the trapped RBC is decreased. The maximum phase of the RBC is found to be 3.59 rad and 2.24 rad when the laser is switched off and switched on, respectively, as illustrated in Fig. 3d. The recovered maximum phase values of the trapped and untrapped RBCs at different time intervals are also exhibited using a bar plot in ESI† Fig. S9a.
RBCs are bi-concave in shape; the maximum height of the RBC rim is around 2 μm and that of the central donut is around 0.5 μm. Therefore, the maximum phase value of the RBC is at the rim of the RBC. Assuming that the refractive index of the RBC does not change during waveguide trapping, the decrease of the maximum phase value indicates that the RBC is pushed downwards during the planar trapping and propulsion. This is also in accordance with previously published data, where three-dimensional finite element simulation showed that the intensity gradient generated by the exponentially decaying evanescent field of the waveguide attracts the biconcave shaped RBC towards the surface and presses it downwards. A previous study has explained the phenomenon of RBC deformation on top of the waveguide surface using the finite element numerical simulations of the optical forces and the optical pressure of trapped RBCs.25 It was reported that the net effect of the force density (i.e. pressure multiplied with surface normal) was to press the cell downwards and straighten (flatten) the part of the cell that is overlapping with the evanescent field and make it parallel to the waveguide. When this part of the cell becomes straight, the rest of the cell deforms and a change in the shape occurs. The elastic membrane of the RBC plays a crucial role in spreading the localized optical pressure over the entire cell. Further details can be found in the ESI.† However, in previous work23 only bright field microscopy was used and therefore no quantitative information was obtained. The present method maps the pseudo 3-D phase value of the RBC during planar trapping and could further elucidate the process of RBC deformation during planar trapping. Taken together with the previously published work,25 it can be suggested that the main effect of the waveguide trapping force is to pull the cell downwards and thus decrease the maximum phase.
RBCs are easily deformable; therefore the cytosol within the RBC could re-distribute between the donut and the annular rim during planar trapping. To shed more light on this process, the RBC phase images were divided into two different regions: region I: the central donut region (inside black circle) and region II: the annular rim of the RBC (region between outer red and inner black circle) as depicted in Fig. 4a. The edge detection image processing technique is employed for finding the boundaries of the RBC phase images by setting a threshold value (∼30% of the maximum value) using MATLAB. Edge detection is used for RBC phase image segmentation into three different regions: (1) region I, (2) region II, and (3) outermost region (Fig. 4a). In order to observe the change in the mean phase value of the RBC during the transportation, the shape as well as the area of segmented region ‘II’ was kept constant while analyzing the reconstructed phase maps of one experimental series. Finally, the mean phase values of regions ‘I’ and ‘II’ were measured for both laser off and on conditions.
Fig. 4 Quantitative phase imaging highlights the change in the RBC phase value during waveguide trapping and propulsion. (a) Shows the RBC phase image divided into region I (inside black dotted circle), i.e., donut and region II (annular region between red and black dotted circle), i.e., non-donut region. Whisker box plot (b and c) of the mean phase values of the time lapsed frames (shown in Fig. 2) of region I and region II for a single movie (experiment). The central red lines indicate the median, and the bottom and top sides of the blue box indicate the 25th and 75th percentiles, respectively. The black lines extended vertically from the blue boxes specify extreme data points without outliers, and ‘+’ symbols in red color are plotted for outliers. (d) Variation of the mean phase values of region I and region II as a function of time. |
Fig. 4b and c show the mean phase value box plots of the trapped and untrapped RBCs (shown in Fig. 2) for region I and II, respectively. To understand the influence of trapping forces on RBCs, the recovered time-lapsed mean phase values of the trapped and untrapped RBCs for both regions are also presented by bar plots as illustrated in ESI† Fig. S9b and c. For the measurement of the above values, 40 frames each (from Movie S1†) were selected from the single interferometric movie when the laser was switched on and off. The chosen time points for laser off was 0–14 s and for laser on 26–40 s with an interval of 0.33 s each. The image acquisition was set to 30 frames per second. Interestingly, the mean phase value of region ‘I’ is increased by ∼32%, whereas the mean phase value of region ‘II’ is decreased by ∼40% during RBC trapping. For region ‘I’, the average mean phase obtained from the 40 frames used was 0.65 ± 0.07 rad and 0.86 ± 0.18 rad for trapping laser off and on conditions, respectively. Meanwhile, for region ‘II’ the average mean phase obtained from the 40 frames used was 2.00 ± 0.10 rad and 1.21 ± 0.14 rad for trapping laser off and on conditions, respectively.
The difference (φdiffmean = φtrappedmean − φuntrappedmean) between the mean phase values of the time lapsed frames of the trapped (φtrappedmean) and untrapped (φuntrappedmean) RBCs for both regions was found to be 0.21 rad for region I and −0.79 rad for region II, respectively. The positive and negative values of φdiffmean for region ‘I’ and region ‘II’ suggest the re-distribution of the cytosol inside the RBC (which mostly consists of hemoglobin) from region ‘II’ (annular ring) to region ‘I’ (donut) during planar trapping. The variation of mean phase values of region I and II as a function of time is illustrated in Fig. 4d.
The results shown in Fig. 3 and 4 correspond to a single experiment and the results from additional experiments (9 in total) are presented in Fig. 5. The phase difference is calculated by taking the difference between phase values corresponding to the trapped and untrapped RBCs, i.e., using the following expression: φdiffmax or mean = φtrappedmax or mean − φuntrappedmax or mean. The overall trends of the maximum and mean RBC phase values (region I and II) during waveguide trapping (see Fig. 5) were similar to the results obtained for a single movie presented in Fig. 3 and 4. Similar to the results obtained in Fig. 3c, the maximum phase value of the RBCs also decreases during waveguide trapping which was observed for other experiments (see Fig. 5).
The difference φdiffmean plot of the RBC phase values corresponding to region I and II before and after trapping from the additional 9 experiments is presented by the scattering plot in Fig. 5. The φdiffmean is calculated from 40 different frames under laser on and off conditions at an interval of 0.3 s. The red circles in the scattering plot correspond to φdiffmean for different experimental movies. The horizontal blue line corresponds to the average value of nine different movies for both laser off and on conditions.
The decrease of V and ψ combined with the increase of S indicates that the shape of the RBC approaches a plano-concave shape during planar trapping. Under the assumption that the refractive index of the RBCs remains constant during the waveguide trapping, the decrease in the RBC internal volume when the trapping laser is switched on could possibly be occurring due to the elongation of the RBC under the stress condition, i.e., out flux of cell water and solute.46 It was previously reported that stressing the RBC membrane can lead to the opening of pores that allow exit of intracellular materials.47 At the same time, the S/V of the cell increases (Fig. 7c), indicating that the shape of the RBC is elongated during planar trapping (see Fig. 6). The mean values with standard deviation (SD) of the surface area, volume, surface area-to-volume ratio, and sphericity of RBCs under trapped and untrapped conditions can be found in Table 1. During waveguide trapping, the surface area increased by 5%, the volume decreased by 28%, the S/V ratio increased by 44% and the sphericity decreased by 23%. These values are calculated only for a single experimental movie.
No. | Morphological parameters | Laser off | Laser on |
---|---|---|---|
1. | Surface area ‘S’ (μm2) | 138.96 ± 3.64 | 146.00 ± 5.70 |
2. | Volume ‘V’ (fl) | 89.04 ± 6.51 | 63.93 ± 7.93 |
3. | S/V (μm−1) | 1.56 ± 0.12 | 2.30 ± 0.19 |
4. | Sphericity ‘ψ’ | 0.69 ± 0.04 | 0.52 ± 0.03 |
To investigate the morphological alterations statistically in the RBCs while propelling them on the top of the waveguide, we quantitatively analyzed the phase maps and subsequently retrieved important cell's morphological parameters such as the surface area, volume, S–V ratio, and sphericity, for nine different experiments. Fig. 8 shows the scattering plots of the difference between morphological parameters such as the surface area, volume, S–V ratio, and sphericity, for the trapped and untrapped RBCs for 9 different experiment series. These values were chosen from 40 different frames at an interval of 0.3 s when the laser is off and on for the individual experiments. Each red circle shown in Fig. 8 corresponds to an individual experiment. The morphological parameter (MP) difference is calculated by taking the difference between their values corresponding to trapped and to untrapped conditions, i.e., using the following expression: . The positive and negative values indicate either an increase or a decrease in the parameter's value respectively during trapping. The values of the different morphological parameters corresponding to different experiment series followed a similar trend to that presented in Fig. 7, i.e. during waveguide trapping, the surface area and the volume of the RBC is slightly increased and decreased, respectively. This leads to an increase in the surface-to-volume ratio and a decrease of RBC sphericity with waveguide trapping.
Although our motivation to integrate waveguide trapping with quantitative phase microscopy was driven by RBC application, the proposed methodology can also be employed for studying cellular changes in other cells (such as bacteria and platelets) when exposed to optical forces. The stiffness of the biological cells can further lead to analysis of several diseases like sickle cell anemia, malaria, etc. The proposed approach can be utilized for the quantitative assessment of the health of the RBC, for example in blood storage lesion.23
The spatio-temporal phase sensitivity of the present microscope is around 40 and 20 mrad, which can be increased further by employing a common path interferometer and a low spatial coherent monochromatic light source. The spatio-temporal phase sensitivity of the phase microscope has been improved by using a compact Mirau interferometric objective lens and a synthesized pseudo thermal light source previously.34,48 This can further lead to an increase in the phase measurement accuracy of biological objects during planar trapping and propulsion.
The integrated waveguide chip platform is compatible with other integrated on-chip optical functions such as micro-fluidics and on-chip nanoscopy,49 sensing50 and spectroscopy.51 Recently, chip-based nanoscopy34 has been demonstrated by employing a similar waveguide chip to that used in this work. Therefore, our existing WT-QPM set-up can be easily combined with on-chip fluorescence nanoscopy techniques for simultaneously acquiring super-resolved fluorescence images and the phase image of the biological specimen.
Further, the surface area of the RBC was measured using Monge parametrization defined as , where dA is the area element of the RBC surface, Gx and Gy are the gradients along the x and y directions, and dx and dy are the calibrated pixel width along the x and y directions, respectively.29 The surface area ‘S’ of the RBC is then the sum of all the area elements and projected area (see the ESI† note and Fig. S11). Next, the sphericity ‘ψ’ of trapped and non-trapped RBCs was determined, whose values lie between 0 (for a laminar disk) and 1 for a perfect sphere. It is defined as the ratio between the surface area (S) of a sphere with the same volume as the cell, to the actual surface area of the cell29,53 and is calculated as ψ = 4.84 v2/3 s−1.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c8lc00356d |
This journal is © The Royal Society of Chemistry 2018 |