Modeling
Question 5:
How does the polysilicate layer covered cell focus the light?
COMSOL modeling
Short intro about COMSOL Multiphysics:
The software COMSOL Multiphysics was used to model the electromagnetic field’s interaction with our structure. COMSOL Multiphysics is a CAE software package that can be used to model any physics based system and the interaction of different physics (COMSOL Multiphysics®, 2016). For this project the RF Module was used; this module is the best fit for the dimensions of our structure (micrometers) and the intended wavelength (in the visible spectrum). The figure below demonstrates the different options for different structure size and wavelengths (COMSOL, 2013).
![COMSOL modules](https://static.igem.org/mediawiki/2016/d/d4/T--TU_Delft--COMSOL_modules.png)
3D model – Sphere
For the Electromagnetic field–structure interaction there are two models built. The first and simplest assumes that the shape of our structure is a simple sphere. Using the simple sphere model we have symmetry allowing to model only a quarter of the sphere and we need smaller domain compared to a rod shaped structure resulting in a computational less expensive model and faster conversions. Also the case of spherical lenses is better design due to their independence from their orientation to the incoming radiation compared to the bacterial shaped lenses.
Furthermore parametric method of modelling was used, meaning that the most important parameters for the model were defined and then used for the model design. The parameters used for this model is the radius of the sphere, the wavelength, wavenumber and frequency of the intended light, the thickness of the silicate layer, air layer and Perfectly Matched Layer, the intensity of the intended electromagnetic field, and the material parameters epsilon defined later. The values of those parameters are shown in table 1 below.
Table 1: Values of parameters used in the model
Parameter | Value | Description |
---|---|---|
r0 | 5*10-7 [m] | Radius of the cell |
lda | 5*107 [m] | Wavelength |
k0 | 1.2566*107 [1/m] | Wavenumber in vacuum |
f0 | 5.9958*1014 [1/s] | Frequency |
t_medium | 2.5*10-7 [m] | Thickness of air layer |
t_pml | 2.5*10-7 [m] | Thickness of Perfectly Matched Layer |
t_sil | 8*10-8 [m] | Thickness of silicate layer |
E0 | 1 [V/m] | Intended electromagnetic field |
According to the aforementioned parameters a three dimensional model of a layered sphere, representing our structure, was created in COMSOL Multiphysics®. The 3D model can be seen in Figure 2. In that model the inner part is the r0, representing the cell, the first layer is the silicate layer covering the cell, then the other two layers are the medium with the outermost representing the world further away from the structure. It is important to note that the 3D model shown in Figure 2 is only a quarter of the actual structure but due to symmetry it is possible to use only that part to decrease the computational cost.
![3D sphere in small domain](https://static.igem.org/mediawiki/2016/5/57/T--TU_Delft--3D_model_sphere_small_domain.png)
Materials
Next the materials need to be determined. The RF module uses three important material parameters for its calculations: relative permeability ( \( \mu_r \) ), electrical conductivity ( \( \sigma \) ) and relative permittivity (\( \epsilon_r \)). The relative permeability is equal or almost equal to unity for most real materials for the optical frequency range that concern us (visible spectrum of the EM field) (Mcintyre and Aspnes, 1971). The values for the electrical conductivity were obtained from the material library of COMSOL Multiphysics® and from literature and the relative permittivity can be calculated from the refractive index (n) using the following formulas(Griffiths, 1999):
$$\epsilon = \epsilon ‘ – j \epsilon $$ $$ \epsilon ‘ = \frac{n^2 – k^2}{\mu} = n^2 – k^2$$ $$\epsilon ‘’ = 2 \times n \times \frac{k}{\mu} = 2 \times n \times k$$So it is:
$$\epsilon = n^2 – k^2 – j \times 2 \times n \times k $$Here n is the Real part of the refractive index and k is the Imaginary part. Because we assume that we have non absorbing materials and thus the complex part of the refractive index is zero ( \( k=0 \) ) the relative permittivity can be calculated from the refractive index as:
$$\epsilon = n^2$$Concluding the material parameters used for this model are summarized in Table 2 below. The refractive index of water is 1.33 (Daimon & Masumura, 2007) and of the cell 1.401 (Jericho, Kreuzer, Kanka, & Riesenberg, 2012) and the relative permittivity of both is calculated using the aforementioned formula. The same method was used to calculate the relative permittivity of Tin dioxide, with refractive index between 2.33 and 2.8 for 550 nm (Baco, Chik, & Md. Yassin, 2012) the relative permittivity is 6.58.
Table 2: Material parameters used in the model
Parameters/Materials | Medium (water) | Glass Layer | Tin dioxide (SnO2) | Cell |
---|---|---|---|---|
Relative permeability (μr) | 1 | 1 | 1 | 1 |
Electrical conductivity (σ) | 0.05 [S/m] | 10-14 [S/m] | 0.025 (Banyamin, et al., 2014) | 0.48 [S/m] (Castellarnau, et al., 2006) |
Relative permittivity (εr) | 1.77 | 2.09 | 6.58 | 1.96 |
Whispering Gallery Modes
![](https://static.igem.org/mediawiki/2016/2/21/T--TU_Delft--modeling2.png)
In both methods of capturing light (PHB granules and covering the cell with silica), the light will become trapped by whispering gallery mode (WGM) resonance (Humar et al., 2015). WGM resonance is the phenomenon where waves travel around a concave surface in a closed path (figure 2). Every time the wave hits the surface, total internal reflection occurs. When light hits a interface between two materials the light gets refracted as in figure 3A. If the angle \(\theta_i\) is large enough, the lights does not go trough the interface and gets reflected as in figure 3B. Whispering gallery mode resonance was first explained by Lord Rayleight in the St Paul’s Cathedral for sound waves. When you whisper to the wall of the cathedral the sound waves were able to travel along the wall and a person at the other side of the cathedral could hear it. However someone standing in the middle of the cathedral was not able to hear the whispering. Therefore this phenomenon was called whispering gallery mode resonance. (Rayleigh et al., 1877)
![](https://static.igem.org/mediawiki/2016/a/a4/T--TU_Delft--modeling4.png)
It is important that the waves follow a closed path forming a polygon so that constructive interference takes place. Constructive interference occurs when two waves travel in phase so that their amplitudes add up (figure 4). We need constructive interference so that every cycle in the resonater adds to the constructive interference. To make sure the waves travel in phase so that constructive interference can take place, the optical path length (OPL) is required to be an integer number of wavelengths (equation 1). In equation 1 n is the number of sides of length l, and m an integer number of wavelengths \(\lambda\).
$$OPL=n\cdot l = m\lambda$$![](https://static.igem.org/mediawiki/2016/0/0d/T--TU_Delft--modeling5.png)
PHB Granules
In order to get WGM resonance the light beam has to be reflected by total internal reflection every time it hits the surface. Therefore the light beam has to approach the surface at a minimal angle larger than the critical angle. From Snell’s law (equation 2) we can compute the critical angle (Hecht, 2001) where the incoming light is refracted to have an outgoing angle of exactly 90 degrees (figure 3C). In equation 2 and 3, \(n_1\) and \(n_2\) are the refractive indices of the materials at the interface.
$$n_1 sin(\theta_{i}) = n_2 sin(\theta_{f})$$ $$\theta_{c} = \arcsin\Big(\frac{n_2}{n_1}\sin\big(\frac{\pi}{2}\big)\Big)=\arcsin\Big(\frac{n_2}{n_1}\Big)$$The outgoing light in total internal reflection should have an angle \(\theta_f>\theta_c\) to be reflected. When we look into geometrical optics the path of the light is as shown in figure 5. Since we want a closed optical path (polygon), we have an integer number of sides on the polygon. Using equation 4 from we can determine the number of sides \(n_{sides}\) of the polygon as in equation 5.
![](https://static.igem.org/mediawiki/2016/6/60/T--TU_Delft--modeling6.png)
We can calculate the number of sides by using the reflected angle \(\theta_f\) in equation 4 and round the \(n_{sides}\) up to an integer. This will give us the smallest polygon possible for WGM. We can then calculate the smallest possible value of \(\theta_f\) to get total internal reflection with a closed optical path as in equation 6.
$$\theta_f = \frac{\pi}{2}-\frac{\pi}{round(n_{sides})} $$Now that we know how many sides the polygon has, we can compute the minimal size for the granule sphere so that an integer number of wavelengths fit into the optical path length:
$$m\lambda = n_{sides}l$$ $$l = 2Rcos(\theta_{f})$$We suggest that at least one wavelength should fit into \(l\) ( \(l=\lambda\) ) so that the waves can get trapped. Therefore the minimum size of the granule should be as in equation 9:
$$R = \frac{\lambda}{2\cos(\theta_{f})}$$Results
For PHB granules the refractive index at a wavelength of 580 nm is \(n_{PHB} = 1.468\) (Huglin et al., 1991). The refractive index of cytosol is \(n_{cytoplasm} = 1.37\) (Liang et al., 2007). Putting these values into our model, we find that the minimal size of the PHB granules is \(1.7\mu m\) (figure 6). This is quite a bit larger than we expect the granules to be since the size of E. coli is only \(1-2 \mu m\) long and the granules will not fill the entire bacterium.
![](https://static.igem.org/mediawiki/2016/f/f1/T--TU_Delft--modeling7.png)
Silica covered cells
Since the size of the PHB granules that can be grown inside an E. coli bacterium was expected to be smaller than the required size for lasing, we investigated the option of making a biolaser out of the entire cell. Therefore we encapsulated the cell with a layer of biosilica and tin dioxide. The gain medium in this method is provided by fluorophores which we expressed in the cytosol of the cell. To determine the minimal size in this case the calculation was a bit more tricky than for the PGB granules, since we had to take the layer into account and the optical path has a star-like shape (figure 3A) .
![](https://static.igem.org/mediawiki/2016/b/bd/T--TU_Delft--modeling8.png)
The critical angle can again be computed by equation 3, where \(n_1\) is the refractive index of the layer \(n_f\), and \(n_2\) is the refractive index of the buffer outside the cell \(n_b\). When the angle is slightly larger than the critical angle we have total internal reflection where the outgoing angle is equal to the incoming angle, therefore we may set \(\alpha = \theta_c\). In this model we will neglect the curvature of the surface which means that we can also set \(\theta_i=\alpha\). Using Snell’s Law (equation 2) again we can compute the outgoing angle \(\theta_0\) (equation 10) where \(n_f\) is the refractive index of the layer and \(n_c\) the refractive index of the cytosol.
$$\theta_0 = asin\Big(\frac{n_f}{n_c} sin(\alpha)\Big) $$From \(\theta_0\) we can easily determine the angle \( \phi \) since all the angles in a triangle add up to \(\pi\) (equation 11).
$$\phi = \pi-2 \theta_0 = \pi-2\arcsin\Big(\frac{n_f}{n_c} sin(\alpha)\Big)$$Here the path of the light is star-shaped and the \( OPL=k_{sides}\lambda\). Furthermore we will assume that the total path length per side is minimally \(\lambda\) and that one side is taken as the path from point A to D. The optical path length per side is given as \(OPL_{side}=2\cdot x+l\geq\lambda\). \(X\) and \(l\) can be determined as in equation 12. From equation 12 the minimal radius can be determined for the criteria where \(OPL_{sides} = \lambda\) (equation 13).
$$\left.\begin{matrix} OPL_{sides} =2x+l\geq \lambda \\ x=\frac{t}{\cos\alpha}\\ l =2R\cos\theta_o \end{matrix}\right\} OPL_{sides} = \lambda = \frac{2t}{\cos\alpha}+2R \cos\theta_o =\frac{2t}{\cos\alpha}+2R \sqrt{1-(\frac{n_f}{n_c}\sin\alpha)^2}\geq\lambda $$ $$ R_{min} = \frac{\lambda-\frac{2t}{\cos\alpha}}{2\cos\theta_o}$$Using the minimal radius of R we can determine the angle \(\psi\) as in equation 14.
$$ \psi=2\arcsin(\frac{t \tan\alpha}{R_{min}})$$Using \(\psi\) and \(\phi\) we can determine the minimal number of sides of the optical path (equation 15).
$$k_{sides} = \frac{2\pi}{\psi+\phi}$$In equation 15, \(k_{sides}\) has to be an integer to have a closed optical path. Taken together the constraints as in equation 16 we get an equation for \(\phi\) and \(\psi\) as a function of \(\alpha\).
$$\left.\begin{matrix} \frac{2\pi}{k_{sides}}=\phi+\psi\\ \phi = \pi-2\arcsin(\frac{n_f}{n_c}\sin\alpha)\\ \psi = 2\arcsin(\frac{t\tan\alpha}{R_{min}})\\ OPL_{sides}=2x+l \rightarrow R_{min} = \frac{\lambda-\frac{2t}{\cos\alpha}}{2\sqrt{1-(\frac{n_f}{n_c}\sin\alpha)^2}} \end{matrix}\right\} \frac{2\pi}{k_{sides}}=\pi-2\arcsin(\frac{n_f}{n_c}\sin\alpha)+2\arcsin(\frac{2t\sin\alpha\sqrt{1-(\frac{n_f}{n_c}\sin\alpha)^2}}{\lambda\cos\alpha-2t})$$Solving equation 16 for \(\alpha\) and using this in the equation for the radius results in the minimal radius required for WGM in a cell covered with a layer of biosilica or tin dioxide.
Results
Using the model described above we determined the minimal radius of a cell covered with polysilica and tin dioxide to create a cavity that allows for whispering gallery modes. The refractive index of polysilica is 1.47 (Liang et al., 2007). The refractive index of tin dioxide is 2 (Pradyot, 2003). For both cases we calculated the minimal radius assuming the thickness of the layer to be 50 nm and a wavelength of 509 nm, the emission wavelength of GFP. From our model we found a minimal diameter of \(1.2 \mu m\) and \(1.6 \mu m\) (figure 8) for polysilica and tin dioxide respectively. These sizes are comparable to the size of a bacterium, so whispering gallery modes should in principle be possible inside a covered cell. However, we made a number of simplifications in our model that will in practice probably prevent the system from lasing at this minimum scale. First, we did not take the polarization of the light into account. Second, the length scales we work with here are only about twice the wavelength, and the thickness of the boundary layer is much smaller than the wavelength. A more accurate description of what is happening within the cell would require us to work in the thin layer limit (known as Mie theory) as we do in Q4. There we calculate the quality factor for the cavity, which indicates how well the light can be trapped within the structure. Third, in this model we only determined whether light waves will fit into the cavity, in Q3 we will also determine whether lasing can take place with the size of the cell and the reflectivity of polysilica and tin dioxide.
![](https://static.igem.org/mediawiki/2016/2/2f/T--TU_Delft--modeling9.png)
References
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