Can a toroidal black hole exist?

Many years ago, a brilliant Berkeley mathematician Richard Borcherds started a blog on math. I have no doubt he has so many interesting things to share about math. Regrettably though, for whatever reason, it didn’t last long. In one of his earliest blog articles, he posed a question as to whether a toroidal (doughnut shaped) black hole can exist. We will answer this question here but first, what do we mean by the shape of a black hole? What is called the shape of a black hole is actually the shape of its event horizon. The simplest black hole is Schwarzschild black hole. It is a spherically symmetric solution of the vacuum Einstein’s field equations. The Schwarzschild solution is given by the metric
\begin{equation}
\label{eq:bh}
ds^2=-\left(1-\frac{2MG}{c^2r}\right)c^2dt^2+\left(1-\frac{2MG}{c^2r}\right)^{-1}dr^2+r^2(d\theta^2+\sin^\theta d\phi^2)
\end{equation}
The even horizon is the sphere of radius $r_g:=\frac{2MG}{c^2}$ which is called the Schwarzschild radius. The Schwarzschild solution \eqref{eq:bh} requires that $r>r_g$. The event horizon is what determines the inside and the outside of a black hole. \eqref{eq:bh} is a solution of the vacuum Einstein’d field equations, so it really doesn’t tell us anything happens once an object falls into a black hole past its event horizon. In order to see what happens inside of a black hole, we need information on the source of its gravity, i.e. the stress-energy tensor $T_{ij}$.

In 1923, an American mathematician George David Birkhoff proved the following theorem.

Theorem. Any spherically symmetric solution of the vacuum Einstein’s field equations must be static and asymptotically flat.

One may wonder if the converse of the Birkhoff’s theorem is also true, namely is any static asymptotically flat solution of the vacuum Einstein’s field equations spherically symmetric? The answer is affirmative and it is called Israel’s theorem named after Werner Israel (Phys. Rev. 164, 1776). So, Israel’s theorem settles it. There can’t be a doughnut shaped black hole which is static and asymptotically flat. This also can be shown directly. First the ansatz for a static toroidal black hole can be given by
\begin{equation}
\label{eq:toroidalbh}
ds^2=-A(r)dt^2+B(r)dr^2+r^2d\theta^2+(R+r\cos\theta)^2d\phi^2
\end{equation}
with asymptotically flat condition
$$\lim_{r\to\infty}A(r)=\lim_{r\to\infty}B(r)=1$$
The Ricci tensors are computed to be:
\begin{align*}
R_{tt}&=\frac{A”}{2B}-\frac{A’}{4B}\left(\frac{A’}{A}+\frac{B’}{B}\right)+\frac{A’}{2B}\left(\frac{1}{r}+\frac{\cos\theta}{R+r\cos\theta}\right)\\
R_{rr}&=-\frac{A”}{2A}+\frac{A’}{4A}\left(\frac{A’}{A}+\frac{B’}{B}\right)+\frac{B’}{2B}\left(\frac{1}{r}+\frac{\cos\theta}{R+r\cos\theta}\right)\\
R_{\theta\theta}&=-\frac{r}{2B}\frac{A’B-AB’}{AB}+\frac{r\cos\theta}{R+r\cos\theta}\left(1-\frac{1}{B}\right)\\
R_{\phi\phi}&=(R+r\cos\theta)\cos\theta\left[-\frac{1}{2}\frac{A’}{AB}+\frac{1}{2}\frac{B’}{B^2}+\frac{1}{r}\left(1-\frac{1}{B}\right)\right]
\end{align*}
$$BR_{tt}+AR_{rr}=\frac{1}{2B}\left(\frac{1}{r}+\frac{\cos\theta}{R_r\cos\theta}\right)(AB)’$$
Since $BR_{tt}+AR_{rr}=0$ regardless of what the value of $\theta$ is, $(AB)’=0$ i.e. $AB$ is a constant. The asymptotically flat condition indicates that $AB=1$. Consequently, $R_{\theta\theta}$ becomes
\begin{equation}
\label{eq:riccitheta}
R_{\theta\theta}=-rA’+\frac{r\cos\theta}{R+r\cos\theta}(1-A)
\end{equation}
$R_{\phi\phi}=0$ yields
\begin{equation}
\label{eq:ricciphi}
-\frac{1}{2}\frac{A’}{AB}+\frac{1}{2}\frac{B’}{B^2}+\frac{1}{r}-\frac{1}{rB}=0
\end{equation}
Finally, subtracting $r$ times \eqref{eq:ricciphi} from \eqref{eq:riccitheta} and then setting the result equal to 0 we obtain
$B=1$ and thereby $A=1$. Therefore, the ansatz \eqref{eq:toroidalbh} becomes the flat Minkowski space-time, so there is no toroidal black hole.

How about then for a rotating black hole? Can there be a rotating toroidal black hole? The answer is negative for this case also. Hawking and Ellis proved that the shape of a rotating black hole has to be a sphere and it can be found in Proposition 9.3.2 of S. W. Hawking and G. F. R. Ellis, The Large Scale Structure of Space-Time, Cambridge University Press, 1973. (Hat tip to David Garfinkle.)

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diff (A Linux Command)

diff is one of my favorite Linux commands, which is very useful. What does it do? It does compare two text documents and shows their differences if there are any. The syntax is as simple as

diff textfile1 textfile2

and so it is easy to use even if you are not so familiar with command lines. Here is an example.

I am currently working on my old MacBook, so you see an Apple terminal in the above image. But diff is a common Linux command for any Linux distribution, of course, including Ubuntu. I have two files named caesar.py and caesar2.py in my ~/Desktop/python folder. I ran diff command to compare these two. What the output says is that caesar.py has the following two lines:

# every possible symbol that can be encrypted
LETTERS = 'ABCDEFGHIJKLMNOPQRSTUVWXYZ'

that caesar2.py does not have. Pay attention to the direction of the arrow <. This is particularly useful when you are programming. Suppose that you have a backup of the original code say caesar.py and you are editing its copy caesar2.py. Somehow you deleted or incorrectly altered certain lines by mistake and you couldn’t identify your mistakes. In that case, you can solve the issue by simply running the command diff as shown in the example.

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Constellation (TV series) and Many-Worlds Interpretation

There is a new TV series titled Constellation on Apple TV+. The plot so far (I don’t intend to be a spoiler and I don’t actually know much about the plot either because there have been only three episodes) is that a Swedish astronaut Jo Ericsson (portraited by Noomi Rapace) has returned to Earth after a catastrophic disaster led by a weird circumstance hit the ISS. But somethings in Jo’s life are amiss after her return home …

The show is entertaining, but more interestingly it appears to embrace Hugh Everett’s many-worlds interpretation of quantum mechanics. This perspective of quantum mechanics assumes the existence of the universal wavefunction which is the wave function of the entire universe and it never collapses unlike wave functions in Copenhagen interpretation. In this perspective, all the possible quantum states as different realities exist simultaneously, hence the name many-worlds interpretation. Another peculiar aspect of this perspective is that the observers are part of the wavefunction, i.e. the observers and the observed are all mixed together. What this implies is that there is no measurement in many-worlds interpretation. The proponents of many-worlds interpretation seem to support the idea of philosophical realism regarding the universal wavefunction, that it exists even in the absence of any mind perceiving it. It is an interesting concept but I am not buying it. Perhaps no one cares whether I believe it and this is merely my own opinion. First, my impression is that often physicists don’t seem to distinguish hypotheses and facts, and mathematical entities and physical entities (that we can actually measure and/or observe). Wave functions are not physical entities but merely convenient mathematical entities to represent the wave nature of particles and their quantum states. Extending the wave nature of matter (consequently, the probabilistic nature of quantum mechanics) to the macroscopic world or to the entire universe is too far-fetched to be even remotely true. More importantly, you cannot have a viable physical theory without considering measurement.  If there is no measurement, the theory is not even falsifiable, quoting Wolfgang Pauli, it is not even wrong.

If you don’t care about all this, I think you can enjoy the show.

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Coffee and Mathematics

I don’t remember who said it but someone (could be one of French mathematicians) said “Mathematicians are those who turn coffee into theorems“. It rings so true to me. I love coffee. I love its smell and taste. The smell of freshly brewed coffee in the morning is the second best thing to the fresh scent of cool morning breeze and dew. But more importantly, it is a great brain stimulant. I can’t do math without having a (or two) nice cup(s) of coffee.

Ever since my wife was influenced by those damn Korean YouTube doctors who are bull-shitting that coffee is bad for cancer, I have been pretty much stressed out by her constant barrage of complaints about me drinking coffee. By the way, I thought good doctors would be too busy to make YouTube videos for taking care of patients, studying and doing research, no? Whatever truth there may be in their claims about coffee, the stress I am getting will be definitely worse for me than whatever bad coffee does to me.

If I can’t have coffee without freedom and peace, I might as well quit drinking coffee after all. Alas, here is another reason I may have to quit doing math.

Update: I just remembered this story. Both Ron Graham and Paul Erdös were working at the Bell Lab. Erdös was suffering from a depression after his wife passed away and he was prescribed methamphetamine. Worried about his addiction, Graham offered \$500 to Erdös if he could stop taking it for a month. (\$500 was a lot of money back then.) Erdös managed to stop taking methamphetamine for a month and after he took \$500 from Graham, he started taking it again. Erdös said during the time he stopped taking methamphetamine, he couldn’t do math. Every time he looked at a piece of paper, he only saw white blank space but nothing else. I think I can see what he must have felt, probably more or less the same feeling I had every time I stopped drinking coffee.

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Square Root of Klein-Gordon

Replacing $E$ and $p$ by $i\hbar\frac{\partial}{\partial t}$ and $-i\hbar\nabla$, respectively, in the energy-momentum relation
$$E^2=p^2c^2+m_0^2c^4$$
we obtain the Klein-Gordon operator
$$\square=\frac{m_0^2c^2}{\hbar^2},$$
where
$$\square=-\frac{1}{c^2}\frac{\partial^2}{\partial t^2}+\nabla^2$$
$\square$ is called the d’Alembertian or the wave operator. This time, replacing $E$ and $p$ by $i\hbar\frac{\partial}{\partial t}$ and $-i\hbar\nabla$ in the square root of the energy-momentum relation
\begin{equation}
\label{eq:sqrte-m}
E=\sqrt{p^2c^2+m_0^2c^4}
\end{equation}
we obtain
\begin{equation}
\label{eq:sqrtkg}
i\hbar\frac{\partial}{\partial t}=\sqrt{-\hbar^2c^2\nabla^2+m_0^2c^4}
\end{equation}
\eqref{eq:sqrtkg} is called the square root of Klein-Gordon operator. I said mathematics is full of weird stuff here but so is physics. The RHS of \eqref{eq:sqrtkg} is pretty weird. It is supposed to be an operator, meaning supposed to act on a wave function. But how does it do that? Does it even exist? I read or heard somewhere (sorry I don’t remember details) that Schrödinger studied the equation
\begin{equation}\label{eq:sqrtkg2}i\hbar\frac{\partial\psi(\mathbf{r},t)}{\partial t}=\sqrt{-\hbar^2c^2\nabla^2+m_0^2c^4}\psi(\mathbf{r},t)+V(\mathbf{r})\psi(\mathbf{r},t)\end{equation}
before he discovered his celebrated equation, the one we now call the Schrödinger equation. What I vaguely remember is that the equation was too difficult or inconvenient to deal with so he eventually gave up on it. I am not really privy to the history of quantum mechanics let alone the history of physics in general, so I couldn’t find a reference to this. But that is not important anyway. What’s important is to make sense of the operator $\sqrt{-\hbar^2c^2\nabla^2+m_0^2c^4}$. Let us go back to the square root of the energy-momentum relation \eqref{eq:sqrte-m}. With $p^2=m^2v^2$ and $m=\frac{m_0}{\sqrt{1-\frac{v^2}{c^2}}}$, we have
\begin{align*}
E&=\sqrt{p^2c^2+m_0^2c^4}\\
&=m_0c^2\sqrt{1+\frac{p^2}{m_0^2c^2}}\\
&=m_0^2c^2\sqrt{1+\left(\frac{m}{m_0}\right)^2\left(\frac{v}{c}\right)^2}
\end{align*}
Since $v<c$,
\begin{align*}
\left(\frac{m}{m_0}\right)^2\left(\frac{v}{c}\right)^2&=\frac{1}{1-\frac{v^2}{c^2}}\frac{v^2}{c^2}\\
&=\left(1+\frac{v^2}{c^2}+\frac{v^4}{c^2}+\frac{v^6}{c^6}+\cdots\right)\frac{v^2}{c^2}
\end{align*}
For a particle with speed $v$ slower than $c$, certain high-order terms of $\frac{v^2}{c^2}$ can be negligible. This means that, mathematically speaking, $\left(\frac{m}{m_0}\right)^2\left(\frac{v}{c}\right)^2=\frac{p^2}{m_0^2c^2}$ is nilpotent. Also, if any physical effect of certain high-order terms of $\frac{v^2}{c^2}$ is not observed from experiments, we can safely assume that $\left(\frac{m}{m_0}\right)^2\left(\frac{v}{c}\right)^2=\frac{p^2}{m_0^2c^2}$ is nilpotent. In here, we proved that if $N$ is a nilpotent operator, $I+N$ has a square root and it is given by
$$\sqrt{I+N}=I+\frac{1}{2}N-\frac{1}{8}N^2+\frac{1}{16}N^3-\cdots$$
So, $\sqrt{p^2c^2+m_0^2c^4}$ can be understood as an operator as
\begin{align*}
\sqrt{p^2c^2+m_0^2c^4}&=m_0c^2\sqrt{1+\frac{p^2}{m_0^2c^2}}\\
&=m_0c^2\left(1+\frac{p^2}{2m_0^2c^2}-\frac{1}{8}\frac{p^4}{m_0^4c^4}+\frac{1}{16}\frac{p^6}{m_0^6c^6}+\cdots\right)\\
&=m_0c^2+\frac{p^2}{2m_0}-\frac{1}{8}\frac{p^4}{m_0^3c^2}+\frac{1}{16}\frac{p^6}{m_0^5c^4}+\cdots
\end{align*}
For example, in one-dimensional case, since $\hat p=-i\hbar\frac{\partial }{\partial x}$, we have
$$\sqrt{-\hbar^2c^2\frac{\partial^2}{\partial x^2}+m_0^2c^4}=m_0c^2-\frac{\hbar^2}{2m_0}\frac{\partial^2}{\partial x^2}-\frac{1}{8}\frac{\hbar^4}{m_0^3c^2}\frac{\partial^4}{\partial x^4}-\frac{1}{16}\frac{\hbar^6}{m_0^5c^4}\frac{\partial^6}{\partial x^6}+\cdots$$
where $\frac{\partial^2}{\partial x^2}$ is assumed to be nilpotent.

Update: While \eqref{eq:sqrtkg} is Lorentz invariant, one cannot add a potential energy like \eqref{eq:sqrtkg2} in Lorentz invariant way. This is another reason square root of Klein-Gordon equation was not favored by physicists. The relativistically corrected $s$-wave equation in the paper Relativistically corrected Schrödinger equation with Coulomb interaction by J. L. Friar and E. L. Tomusiak, Physical Review C, Volume 29, Number 4, 1537, is not really relativistic as it is not Lorentz invariant.

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