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Electrostatics and magnetostatics on the hypersphere

While studying at Masaryk University in Brno, I wrote my bachelor thesis - Electrostatics and magnetostatics on the hypersphere. The title says it all. My task was to solve scalar and vector Poisson equations for electrostatic and magnetostatic potentials. I managed to find a solution for the electrostatic potential. Still, unfortunately, the magnetostatic (vector) potential was too much of a task and would require extra time, which I did not have at the time. I managed to defend my thesis with the grade A in June of 2024. If you are interested in the Thesis, you can download it here or here.

I wrote some code for my bachelor thesis which I share here for anyone interested.

Hypersphere

What do I mean by hypersphere? In my thesis by hypersphere I mean 3-sphere $\mathbb{S}^3$ - three dimensional sphere imbedded in $\mathbb{R}^4$. We can define hypersphere $\mathbb{S}^3$ like this

$$\mathbb{S}^3 = \{ (x_1,x_2,x_3,x_4) \in \mathbb{R}^4 \vert \sqrt{x_1^2 + x_2^2 + x_3^2 + x_4^2} = r \},$$

where $(x_1,x_2,x_3,x_4)$ is a point on $\mathbb{R}^4$ (expressed by Cartesian coordinates) and $r$ is the radius of the hypersphere. To make things little bit easier for me I set the hypersphere radius $r = 1.$

Hyperspherical coordinates

Cartesian coordinates are not the best coordinates for describing the hypersphere (trust me...) and more "natrual" choice of coordinates can make the work with the hypersphere a lot easier. One of the more "natural" coordinate system that I used in my thesis is hyperspherical coordinate system represented by the map $\alpha$

$$ \alpha: \qquad \begin{array}{l} x_1 = \cos\varphi, \\ x_2 = \sin\varphi\cos\vartheta, \\ x_3 = \sin\varphi\sin\vartheta\cos\zeta, \\ x_4 = \sin\varphi\sin\vartheta\sin\zeta. \end{array} $$

where $\varphi \in (0,\pi)$, $\vartheta \in (0,\pi)$ and $\zeta \in (0,2\pi)$ are the new coordinates - angles - of the hypersphere ($\zeta$ is analogous to azimuthal angle in spherical coordinates). We can derive the inverse map $\alpha^{-1}$

$$ \alpha^{-1}: \qquad \begin{array}{l} \varphi = \arctan\frac{\sqrt{x_2^2+x_3^2+x_4^2}}{x_1}+\frac{\pi}{2}, \\ \vartheta = \begin{cases} \arctan\frac{\sqrt{x_3^2+x_4^2}}{x_2}+\frac{\pi}{2}, & \mbox{if } x_2 \neq 0, x_3 \neq 0 \mbox{ and } x_4 \neq 0, \\ \text{undefined}, & \mbox{for } x_2 = x_3 = x_4 = 0, \end{cases} \\ \zeta = \begin{cases} \arctan\left(\frac{x_4}{x_3}\right), & \mbox{if } x_3>0, \\ \arctan\left(\frac{x_4}{x_3}\right) + \pi, & \mbox{if } x_3<0 \mbox{ and } x_4 \ge 0, \\ \arctan\left(\frac{x_4}{x_3}\right) - \pi, & \mbox{if } x_3<0 \mbox{ and } x_4<0, \\ +\frac{\pi}{2}, & \mbox{if } x_3=0 \mbox{ and } x_4>0, \\ -\frac{\pi}{2}, & \mbox{if } x_3=0 \mbox{ and } x_4<0, \\ \text{undefined}, & \mbox{if } x_3 = x_4=0. \end{cases} \end{array} $$

which will be useful later :).

Stereographic projection

For the human mind, the hypersphere $\mathbb{S}^3$ is not easily imaginable. Fortunately we can map the hypersphere $\mathbb{S}^3$ onto the $\mathbb{R}^3$ by stereographic map (more on stereographic projection here) $\beta$

$$ \beta: \qquad \begin{array}{l} \mu = \frac{x_1}{1-x_4}, \\ \nu = \frac{x_2}{1-x_4}, \\ \xi = \frac{x_3}{1-x_4}, \end{array} $$

where $\mathbf{p} = (x_1, x_2, x_3, x_4)$ represents a point on the hypersphere (and therefore it must be true that $\sqrt{x_1^2 + x_2^2 + x_3^2 + x_4^2} = 1$) and $\mu$, $\nu$ and $\xi$ are the new coordinates of $\mathbf{p}$ on $\mathbb{R}^3$. Inverse stereographic projection $\beta^{-1}$ will prove to be useful so let me write it down here

$$ \beta^{-1}: \qquad \begin{array}{l} x' = \frac{2\mu}{\mu^2+\nu^2+\xi^2+1}, \\ y' = \frac{2\nu}{\mu^2+\nu^2+\xi^2+1}, \\ z' = \frac{2\xi}{\mu^2+\nu^2+\xi^2+1}, \\ w' = \frac{\mu^2+\nu^2+\xi^2-1}{\mu^2+\nu^2+\xi^2+1}. \end{array} $$

Visualisation of functions on the hypersphere - finally some code!

Now we can visualize the functions on the hypersphere $f(\varphi, \vartheta, \zeta)$ using the stereographic projection. How? Let us start with the grid of $N^3$ (we will call $N$ the 'grid number') points in the closed subspace $M = \{p = (x_1, x_2, x_3) \vert x_1 \in [-2,2], x_2 \in [-2,2], x_3 \in [-2,2]\}$ of $\mathbb{R}^3$. In the code, this process looks like this

N_fig = 120                                              # Grid number defines the "resolution" of the Figures

x_values = np.linspace(-2,2,N_fig)                       # Defiing the grid for the plotting
y_values = np.linspace(-2,2,N_fig)
z_values = np.linspace(-2,2,N_fig)
x,y,z = np.meshgrid(x_values, y_values, z_values)

Then, using the inverse map $\beta^{-1}$ (inverse stereographic projection), we will express each point of the grid in $R^4$. Finally, we can use the inverse hyperspherical map $\alpha^{-1}$, we will end up with the hyperspherical coordinates of each point of the grid (from our subspace $M$) into which we want to project the function $f(\varphi, \vartheta, \zeta)$. These inverse maps are defined in the code by the functions R3_R4 and R4_S3 like this

def R3_R4(x_values, y_values, z_values):                 # Inverse stereographic projection
    X = (2*x_values)/(x_values**2+y_values**2+z_values**2+1) 
    Y = (2*y_values)/(x_values**2+y_values**2+z_values**2+1) 
    Z = (2*z_values)/(x_values**2+y_values**2+z_values**2+1) 
    W = (x_values**2+y_values**2+z_values**2-1)/(x_values**2+y_values**2+z_values**2+1) 
    return(X,Y,Z,W)

def R4_S3(X,Y,Z,W):                                      # Inverse hyperspherical map
    zeta = np.arctan2(W,Z)
    theta = np.arctan2(np.sqrt(Z**2+W**2),Y)
    phi = np.arctan2(np.sqrt(W**2+Z**2+Y**2),X)
    return(phi, theta, zeta)

To confuse the reader - the code denotes the coordinates in $\mathbb{R}^4$ as X, Y, Z, W and in $\mathbb{R}^3$ as x_values, y_values, z_values instead of $x_1$, $x_2$, $x_3$, $x_4$ or $\mu$, $\nu$, $\xi$ respectively.

Now, we can assign the hyperspherical coordinate to each point of the grid in the subspace $M$ of $\mathbb{R}^3$ and that means that we are also able to assign the function value of the function $f(\varphi, \vartheta, \zeta)$. The hard part is over... uff...

Now the only thing that remains to do is to plot the function. I decided to use the isosurfaces (surfaces with constant function value) to be plotted and used Plotly graphing library to plot the figure of the isosurfaces of the function.

func_values_g = np.real(func_g(zeta_g,theta_g,phi_g))    # Evaluation of the func_g for each point of the plot grid 

    fig = go.Figure(layout=layout, data = go.Volume(     # Making the plot
        x=x.flatten(),
        y=y.flatten(),
        z=z.flatten(),
        value = func_values_g.flatten(),
        isomin = np.min(func_values_g),
        isomax = np.max(func_values_g),
        # isomin = -1,
        # isomax = 1,
        surface_count = 10,
        opacity = 0.5,
        #surface_fill = 0.9,
        colorscale = "plasma",
        caps = dict(x_show = False, y_show = False, z_show = False)
    ))

    fig.update_layout(scene_camera=camera)

    fig.show()

I selected a few simple functions as examples to show the output image. You may see them below.
f=phi $f(\varphi, \vartheta, \zeta) = \varphi$ f=theta $f(\varphi, \vartheta, \zeta) = \vartheta$
f=zeta $f(\varphi, \vartheta, \zeta) = \zeta$ f=cos(phi)cos(theta)cos(zeta) $f = \cos\varphi \cos\vartheta \cos\zeta$

Poisson equation

As I said in the beginning, I managed to only solve electrostatic part of the problem but I generalized both electrostatic and magnetostatic Poisson equations to the hypersphere $\mathbb{S}^3$. For this generalization I used the language of the differential forms. For more details on how did I make this generalization have a look at my thesis.

In the hyperspherical coordinates the Laplace operator applied on the function $f(\varphi, \vartheta, \zeta)$ is

$$ \Delta f = \frac{1}{\sin^2\varphi} \frac{\partial \sin^2\varphi \frac{\partial f }{\partial \varphi} }{\partial \varphi} + \frac{1}{\sin^2\varphi \sin\vartheta} \frac{\partial \sin\vartheta \frac{f}{\partial \vartheta}}{\partial \vartheta} + \frac{1}{\sin^2\varphi\sin^2\vartheta} \frac{\partial^2 f}{\partial \zeta} $$

The classic Poisson equation for the eletrostatic potential $\phi$ in our flat space $\mathbb{R}^3$ is

$$ \Delta \phi = -\frac{\rho}{\varepsilon_0}, $$

where $\rho$ is the charge density and $\varepsilon_0$ is the vacuum permittivity constant. Because I was able to generalize the Laplace operator $\Delta$ to the hypersphere $\mathbb{S}^3$ I can write the Poisson equation on the hypersphere as

$$ \Delta_{\mathbb{S}^3} \phi(\varphi, \vartheta, \zeta) = \frac{\rho(\varphi, \vartheta, \zeta)}{\varepsilon_0}. $$

From now on I will omit the index in $Delta_{\mathbb{S}^3}$ and the function variables $\varphi, \vartheta, \zeta$.

With the assumption of separation of variables

$$ \Delta \phi(\varphi, \vartheta, \zeta) = \Delta \Phi(\varphi)\Theta(\vartheta)Z(\zeta) $$

I was able to find eigenfunctions of the Laplace operator $\Delta$ which I denoted as $H_{nlm}$ - Hyperspherical haromincs - where $n \in \mathbb{N}_0$, $l \leq n; l \in \mathbb{N}_0$ and $-l \leq m \leq l; m \in \mathbb{Z}$. Each eigenfunction has an eigenvalue $\lambda = -(n+2)n$ so we can write

$$ \Delta H_{nlm} = -(n+2)n H_{nlm}. $$

You may be interested in how does the hyperspherical harmonic function $H_{nlm}$ look like. In my thesis I derived the formula for $H_{nlm}$

$$ H_{nlm} = \sqrt{\frac{(2l+1)(n+1)(l-m)!(n-l)!}{2\pi^2(l+m)!(n+l+1)!}} C_{n}^{1,l}(\cos\varphi) C_{l}^{1/2,m}(\cos\vartheta) e^{im\zeta}, $$

where $C_n^{\alpha,n} are associated Gegenbauer polynomials which are disccused in the appendix B of my thesis. The constant in the front is normalization consstant which ensures that the hyperspherical harmonic function is normalized with respect to the inner product (integral over the hypersphere)

$$ \left< f, g \right> = \int_0^\pi \sin^2\varphi \text{d}\varphi \int_0^\pi \sin\vartheta \text{d}\vartheta \int_0^{2\pi} \bar{f}g \text{d}\zeta, $$

where $\bar{f}$ is complex conjugate of the function $f$.

Solutions!

Now that I have the eigenfunctions of the Laplace operator we can finally solve some problems! How? Lets assume that we know the chrage density function $\rho(\varphi, \vartheta, \zeta)$. That is enough to solve our Poisson equaiton

$$ \Delta \phi = -\frac{\rho}{\varepsilon_0}. $$

So why did we bother with finding the eigenfunctions of the Laplace operator? If the results of the Sturm--Liouville theory are applied on our set of eigenfunctions $H_{nlm}$ it can be shown that the hyperspherical harmonics $H_{nlm}$ form an orthonormal basis on the space of square-itegrable functions (on the hypersphere $\mathbb{S}^3$ of course) with respect to the innerproduct of two functions mentioned above. This means that we can express any (square-integrable) function $f$ on $\mathbb{S}^3$ as the generalized Fourier series

$$ f(\varphi, \vartheta, \zeta) = \sum_{nlm} c_{nlm}H_{nlm}, $$

where $c_{nlm}$ are the Fourier coefficients gyven by the relation

$$ c_{nlm} = \left< H_{nlm}, f \right>. $$

Now we will use the important property of the Laplace operator - is is self-adjoint operator.

$$ \left< \delta f, g \right> = \left< f, \delta g \right>. $$

Now we have all the instruments we need to express our electrostatic potential $\phi$ as the Fourier series with $H_{nlm}$ as a basis. How? Lets have a look at this series of functions

$$ \begin{gathered} \left< H_{nlm}, \Delta \phi \right> = \left< \Delta H_{nlm} , \phi \right> = \left< H_{nlm} , -\frac{\rho}{\varepsilon_0} \right>, \\ \left< \Delta H_{nlm} , \phi \right> = -(n+2)n \left< H_{nlm}, \phi \right> = \left< H_{nlm} , -\frac{\rho}{\varepsilon_0} \right>. \\ \left< H_{nlm} , \phi \right> = \frac{1}{(n+2)n} \left< H_{nlm} , \phi \right> \end{gathered} $$

These equations follow from the things that have been said earlier. How would the Fourier series of the electrostatic function $\phi$ look like? Like this

$$ \phi(\varphi, \vartheta, \zeta) = \sum_{nlm} \left< H_{nlm} , \phi \right> H_{nlm}, $$

and if we look closely we can see, that we expressed the coefficients $\left&lt; H_{nlm}, \phi \right&gt;$ in the previous equaitons! And just like that we have a solution to our problem - Poisson equation with known charge density function

$$ \phi(\varphi, \vartheta, \zeta) = \sum_{nlm} \frac{1}{\varepsilon_0 (n+2)n} \left< H_{nlm} , \rho \right> H_{nlm}. $$

Pictures of the solutions

Becuase I cannot sum all of the terms in the infinite series in my solutions I ommited the terms with $n &gt; 7$ (this number was selected as good enough. I know, not very rigourous...) si the series becomes finite. Now we can visualise the solution (or rather its approximation) using our script! But first we need to compute the Fouerier components of the generalized Fouerier series $\left< H_{nlm}, \rho \right> which is the hardest part to compute. I have done that using the following part of the script.

def components_simps(n,l,m):                                        # Calculation of the Fourier coefficient for the input function
    function_values = np.conjugate(eigen_func(zeta,theta,phi,n,l,m))*func_g(zeta,theta,phi)
    jacobian = (np.sin(phi))**2*np.sin(theta)
    result = simpson(simpson(simpson(function_values*jacobian,zeta_values, axis = 2), theta_values, axis = 1),phi_values, axis = 0)
    return(result)

The script then multiplies this component by $\frac{1}{\epsilon_0 (n+2)n} H_{nlm}$ and we have one term of the (now) finite series! After we sum up all of the terms we have the solution which we can now visualize using the stereographic projeciton. In the table belov we can see the charge density functions and the solution.

Analytic function of charge density $\rho$ Charge density Electrostatic potential
$\rho_1 = 30 A \sin{\vartheta}\cos{\zeta}-A \left(\varphi-\frac{\pi}{2}\right)^3$ rho1 phi1
$\rho_2 = A \left(\varphi - \frac{\pi}{2} + \sin2\vartheta\right), \qquad [A] = \text{ Cm}^{-3}$ rho1 phi1
$\rho_3 = A \left( \cos{\varphi}+2\cos{\vartheta} \right) \sin{2\varphi} \sin{\zeta}, \qquad [A] = \text{ Cm}^{-3}$ rho1 phi1