Oct 072015
 

It’s time for me to write about physics again. I have a splendid reason: one of the recipients of this year’s physics Nobel is from Kingston, Ontario, which is practically in Ottawa’s backyard. He is recognized for his contribution to the discovery of neutrino oscillations. So I thought I’d write about neutrino oscillations a little.

Without getting into too much detail, the standard way of describing a theory of quantum fields is by writing down the so-called Lagrangian density of the theory. This Lagrangian density represents the kinetic and potential energies of the system, including so-called “mass terms” for fields that are massive. (Which, in quantum field theory, is the same as saying that the particles we associate with the unit oscillations of these fields have a specific mass.)

Now most massive particles in the Standard Model acquire their masses by interacting with the celebrated Higgs field in various ways. Not neutrinos though; indeed, until the mid 1990s or so, neutrinos were believed to be massless.

But then, neutrino oscillations were discovered and the physics community began to accept that neutrinos may be massive after all.

So what is this about oscillations? Neutrinos are somewhat complicated things, but I can demonstrate the concept using two hypothetical “scalar” particles (doesn’t matter what they are; the point is, their math is simpler than that of neutrinos.) So let’s have a scalar particle named \(\phi\). Let’s suppose it has a mass, \(\mu\). The mass term in the Lagrangian would actually be in the form, \(\frac{1}{2}\mu\phi^2\).

Now let’s have another scalar particle, \(\psi\), with mass \(\rho\). This means another mass term in the Lagrangian: \(\frac{1}{2}\rho\psi^2\).

But now I want to be clever and combine these two particles into a two-element abstract vector, a “doublet”. Then, using the laws of matrix multiplication, I could write the mass term as

$$\frac{1}{2}\begin{pmatrix}\phi&\psi\end{pmatrix}\cdot\begin{pmatrix}\mu&0\\0&\rho\end{pmatrix}\cdot\begin{pmatrix}\phi\\\psi\end{pmatrix}=\frac{1}{2}\mu\phi^2+\frac{1}{2}\rho\psi^2.$$

Clever, huh?

But now… let us suppose that there is also an interaction between the two fields. In the Lagrangian, this interaction would be represented by a term such as \(\epsilon\phi\psi\). Putting \(\epsilon\) into the “0” slots of the matrix, we get

$$\frac{1}{2}\begin{pmatrix}\phi&\psi\end{pmatrix}\cdot\begin{pmatrix}\mu&\epsilon\\\epsilon&\rho\end{pmatrix}\cdot\begin{pmatrix}\phi\\\psi\end{pmatrix}=\frac{1}{2}\mu\phi^2+\frac{1}{2}\rho\psi^2+\epsilon\phi\psi.$$

And here is where things get really interesting. That is because we can re-express this new matrix using a combination of a diagonal matrix and a rotation matrix (and its transpose):

$$\begin{pmatrix}\mu&\epsilon\\\epsilon&\rho\end{pmatrix}=\begin{pmatrix}\cos\theta/2&\sin\theta/2\\-\sin\theta/2&\cos\theta/2\end{pmatrix}\cdot\begin{pmatrix}\hat\mu&0\\0&\hat\rho\end{pmatrix}\cdot\begin{pmatrix}\cos\theta/2&-\sin\theta/2\\\sin\theta/2&\cos\theta/2\end{pmatrix},$$

which is equivalent to

$$\begin{pmatrix}\hat\mu&0\\0&\hat\rho\end{pmatrix}=\begin{pmatrix}\cos\theta/2&-\sin\theta/2\\\sin\theta/2&\cos\theta/2\end{pmatrix}\cdot\begin{pmatrix}\mu&\epsilon\\\epsilon&\rho\end{pmatrix}\cdot\begin{pmatrix}\cos\theta/2&\sin\theta/2\\-\sin\theta/2&\cos\theta/2\end{pmatrix},$$

or

$$\begin{pmatrix}\hat\mu&0\\0&\hat\rho\end{pmatrix}=\frac{1}{2}\begin{pmatrix}\mu+\rho+(\mu-\rho)\cos\theta-2\epsilon\sin\theta&(\rho-\mu)\sin\theta-2\epsilon\cos\theta\\(\rho-\mu)\sin\theta-2\epsilon\cos\theta&\mu+\rho+(\rho-\mu)\cos\theta+2\epsilon\sin\theta\end{pmatrix},$$

which tells us that \(\tan\theta=2\epsilon/(\rho-\mu)\), which works so long as \(\rho\ne\mu\).

Now why is this interesting? Because we can now write

\begin{align}\frac{1}{2}&\begin{pmatrix}\phi&\psi\end{pmatrix}\cdot\begin{pmatrix}\mu&\epsilon\\\epsilon&\rho\end{pmatrix}\cdot\begin{pmatrix}\phi\\\psi\end{pmatrix}\\
&{}=\frac{1}{2}\begin{pmatrix}\phi&\psi\end{pmatrix}\cdot\begin{pmatrix}\cos\theta/2&\sin\theta/2\\-\sin\theta/2&\cos\theta/2\end{pmatrix}\cdot\begin{pmatrix}\hat\mu&0\\0&\hat\rho\end{pmatrix}\cdot\begin{pmatrix}\cos\theta/2&-\sin\theta/2\\\sin\theta/2&\cos\theta/2\end{pmatrix}\cdot\begin{pmatrix}\phi\\\psi\end{pmatrix}\\
&{}=\frac{1}{2}\begin{pmatrix}\hat\phi&\hat\psi\end{pmatrix}\cdot\begin{pmatrix}\hat\mu&0\\0&\hat\rho\end{pmatrix}\cdot\begin{pmatrix}\hat\phi\\\hat\psi\end{pmatrix}.\end{align}

What just happened, you ask? Well, we just rotated the abstract vector \((\phi,\psi)\) by the angle \(\theta/2\), and as a result, diagonalized the expression. Which is to say that whereas previously, we had two interacting fields \(\phi\) and \(\psi\) with masses \(\mu\) and \(\rho\), we now re-expressed the same physics using the two non-interacting fields \(\hat\phi\) and \(\hat\psi\) with masses \(\hat\mu\) and \(\hat\rho\).

So what is actually taking place here? Suppose that the doublet \((\phi,\psi)\) interacts with some other field, allowing us to measure the flavor of an excitation (particle) as being either a \(\phi\) or a \(\psi\). So far, so good.

However, when we attempt to measure the mass of the doublet, we will not measure \(\mu\) or \(\rho\), because the two states interact. Instead, we will measure \(\hat\mu\) or \(\hat\rho\), corresponding to the states \(\hat\phi\) or \(\hat\psi\), respectively: that is, one of the mass eigenstates.

Which means that if we first perform a flavor measurement, forcing the particle to be in either the \(\phi\) or the \(\psi\) state, followed by a mass measurement, there will be a nonzero probability of finding it in either the \(\hat\phi\) or the \(\hat\psi\) state, with corresponding masses \(\hat\mu\) or \(\hat\rho\). Conversely, if we first perform a mass measurement, the particle will be either in the \(\hat\phi\) or the \(\hat\psi\) state; a subsequent flavor measurement, therefore, may give either \(\phi\) or \(\psi\) with some probability.

In short, the flavor and mass eigenstates do not coincide.

This is more or less how neutrino oscillations work (again, omitting a lot of important details), except things get a bit more complicated, as neutrinos are fermions, not scalars, and the number of flavors is three, not two. But the basic principle remains the same.

This is a unique feature of neutrinos, by the way. Other particles, e.g., charged leptons, do not have mass eigenstates that are distinct from their flavor eigenstates. The mechanism that gives them masses is also different: instead of a self-interaction in the form of a mass matrix, charged leptons (as well as quarks) obtain their masses by interacting with the Higgs field. But that is a story for another day.

 Posted by at 9:47 pm
Sep 292015
 

In Douglas Adams’s immortal Hitchiker’s Guide to the Galaxy, someone builds a device called the Total Perspective Vortex. This device invariably drives people insane by simply showing them exactly how insignificant they are with respect to this humongous universe.

The Total Perspective Vortex may not exist in reality, but here is the next best thing: A model of the solar system, drawn to scale.

moonpixel

The scale of this page is set so that the Moon occupies one screen pixel. As a result, we have an image that is almost a thousand times wider than my HD computer monitor. It takes a while to scroll through it.

Thankfully, there is an animation option that not only scrolls through the image automatically, but does so at the fastest speed possible, the speed of light.

Oh, did I mention that it still takes well over five hours to scroll all the way to Pluto?

By the way, the nearest star, our closest stellar neighbor is roughly 2,000 times as far from us as Pluto.

Or, once again in the words of Douglas Adams, “Space is big. Really big. You just won’t believe how vastly, hugely, mind-bogglingly big it is. I mean, you may think it’s a long way down the road to the chemist, but that’s just peanuts to space.”

 Posted by at 12:41 pm
Aug 182015
 

I woke up this morning to the news that Mexican-Israeli physicist Jacob Bekenstein died two days ago, at the age of 68, in Helsinki, Finland. I saw nothing about the cause of death.

Bekenstein’s work is well known to folks dealing with gravity theory. Two of his contributions stand out in particular.

First, Bekenstein was first to suggest that black holes should have entropy. His work, along with that of Stephen Hawking, led to the Bekenstein-Hawking entropy formula \(S=kc^3A/4G\hbar\), relating the black hole’s surface area \(A\) to its entropy \(S\) using the speed of light \(c\), the gravitational constant \(G\), the reduced Planck constant \(\hbar\) and Boltzmann’s constant \(k\). With this work, the science of black hole thermodynamics was born, leading to all kinds of questions about the nature of black holes and the connection between thermodynamics and gravity, many of which remain unanswered to this day.

Bekenstein’s second contribution was to turn Morehai Milgrom’s MOdified Newtonian Dynamics (MOND) into a respectable relativitistic theory. The MOND paradigm is about replacing Newton’s law relating force \(({\mathbf F})\), mass \((m)\) and acceleration \(({\mathbf a})\), \({\mathbf F}=m{\mathbf a}\), with the modified law \({\mathbf F}=\mu(a/a_0)m{\mathbf a}\), where all we know about the function \(\mu(x)\) is that \(\lim_{x\to 0}\mu(x)=x\) and \(\lim_{x\to\infty}\mu(x)=1\). Surprisingly, the right choice of \(a_0\) results in an acceleration law that explains the anomalous rotation of galaxies without the need for dark matter. However, in this form, MOND is theoretically ugly: it is a formula that violates basic conservation laws, including the consevation of energy, for instance. Bekenstein’s TeVeS (Tensor-Vector-Scalar) gravity theory provides a general relativistic framework for MOND, one that does respect basic conservation laws, yet reproduces the MOND acceleration formula in the low energy limit.

I never met Jacob Bekenstein, and now I never will. A pity. May he rest in peace.

 Posted by at 11:17 am
Aug 082015
 

I was startled by this photo that appeared in today’s Globe and Mail:

zavikon

I’ve heard about this bridge! Many decades ago, in Hungary. It was described to me as an international bridge between two islands, both owned by a Hungarian family who then declared the “no man’s land” in the middle of the bridge Hungarian territory.

Well… almost. The flag in the middle is indeed the flag of Hungary, but as for the rest…

The islands together are called Zavikon island (I guess the smaller island is just considered an appendage of the larger one) and they are indeed in the Thousands Islands region. They are indeed owned by a Hungarian family. However, both islands are north of the international border, i.e., they are both in Canada. So the flags on this footbridge are really symbolic, they do not reflect political reality. And no, you cannot claim the “no man’s land”, even if it exists along the international border between two states, in the name of a third.

I was nonetheless astonished to see that this bridge actually exists and that at least the part about the flags is, indeed, true.

 Posted by at 11:59 am
Aug 032015
 

Here is one of the most mind-boggling animation sequences that I have ever seen:

This image depicts V838 Monocerotis, a red variable star that underwent a major outburst back in 2002.

Why do I consider this animation mind-boggling? Because despite all appearances, it is not an expanding shell of dust or gas.

Rather, it is echoes of the flash of light, reflected by dust situated behind the star, reaching our eyes several years after the original explosion.

In other words, this image represents direct, visual evidence of the finite speed of light.

The only comparable thing that I can think of is this video, created a few years ago using tricky picosecond photography, of a laser pulse traveling in a bottle. However, unlike that video, the images of V838 Monocerotis required no trickery, only a telescope.

And light echoes are more than mere curiosities: they actually make it possible to study past events. Most notably, a faint light echo of a supernova that was observed nearly half a millennium ago, in 1572, was detected in 2008.

 Posted by at 5:35 pm
Jul 202015
 

\(\renewcommand{\vec}[1]{\boldsymbol{\mathrm{#1}}}\)Continuing something I began about a month ago, I spent more of my free time than I care to admit re-deriving some of the most basic identities in quantum physics.

I started with the single-particle case of a harmonic oscillator. Such an oscillator is characterized by the classical Lagrangian

$$L=\frac{1}{2}m\dot{\vec{q}}^2-\frac{1}{2}k\vec{q}^2-V(\vec{q}),$$

and the corresponding Hamiltonian

$$H=\frac{\vec{p}^2}{2m}+\frac{1}{2}k\vec{q}^2+V(\vec{q}).$$

By multiplying this Hamiltonian with \(\psi=e^{i(\vec{p}\cdot\vec{q}-Ht)/\hbar}\), we basically obtain Schrödinger’s equation:

$$\left[i\hbar\partial_t+\frac{\hbar^2}{2m}\vec{\nabla}^2-\frac{1}{2}k\vec{q}^2-V(\vec{q})\right]e^{i(\vec{p}\cdot\vec{q}-Ht)/\hbar}=0.$$

The transition to the quantum theory begins when we accept that linear combinations of solutions of this equation (i.e., \(\psi\)-s corresponding to different values of \(\vec{p}\) and \(H\)) also represent physical states of the system, despite the fact that these “mixed” solutions are not eigenfunctions and there are no corresponding classical eigenvalues \(\vec{p}\) and \(H\).

Pure algebra can lead to an expression of \(\hat{H}\) in the form of “creation” and “annihilation” operators:

$$\hat{H}=\hbar\omega\left(\hat{a}^\dagger\hat{a}+\frac{1}{2}\right)+V(\vec{q}).$$

These operators have the properties

\begin{align*}
\hat{H}\hat{a}\psi_n&=\left([\hat{H},\hat{a}]+\hat{a}\hat{H}\right)\psi_n=(E_n-\hbar\omega)\hat{a}\psi_n,\\
\hat{H}\hat{a}^\dagger\psi_n&=\left([\hat{H},\hat{a}^\dagger]+\hat{a}^\dagger\hat{H}\right)\psi_n=(E_n+\hbar\omega)\hat{a}^\dagger\psi_n.
\end{align*}
where

$$E_n=\left(n+\frac{1}{2}\right)\hbar\omega.$$

This same derivation can be done in the relativistic single particle case as well.

Moreover, it is possible to define a classical scalar field in the form

$${\cal L}=\frac{1}{2}\rho(\partial_t\phi)^2-\frac{1}{2}\rho c^2(\vec{\nabla}\phi)^2-\frac{1}{2}\kappa\phi^2-V(\phi),$$

which leads to the Hamiltonian density

$${\cal H}=\pi\partial_t\phi-{\cal L}=\frac{\pi^2}{2\rho}+\frac{1}{2}\rho c^2(\vec{\nabla}\phi)^2+\frac{1}{2}\kappa\phi^2+V(\phi).$$

The transitioning to the quantum theory occurs by first expressing \(\phi\) as a Fourier integral and then promoting the Fourier coefficients to operators that satisfy a commutation relation in the form

$$[\hat{a}(\omega,\vec{k}),\hat{a}^\dagger(\omega,\vec{k}’)]=(2\pi)^3\delta^3(\vec{k}-\vec{k}’).$$

This leads to a commutation relation for the field and its canonical momentum in the form

$$[\hat{\phi}(t,\vec{x}),\hat{\pi}(t,\vec{x}’)]=i\hbar\delta^3(\vec{x}-\vec{x}’),$$

and for the Hamiltonian,

$$\hat{H}=\hbar\omega\left\{\frac{1}{2}+\int\frac{d^3\vec{k}}{(2\pi)^3}\hat{a}^\dagger(\omega,\vec{k})\hat{a}(\omega,\vec{k})\right\}+\int d^3xV(\hat{\phi}).$$

More details are provided on my Web site, at https://www.vttoth.com/CMS/physics-notes/297.

So why did I find it necessary to capture here something that can be found in first chapter of every semi-decent quantum field theory textbook? Several reasons.

  • First, I wanted to present a consistent treatment of all four cases: the nonrelativistic and relativistic case for both the particle and the field theory.
  • Second, I wanted to write down all relevant equations without omitting dimensions. I wanted to write down a Lagrangian density that has the dimensions of energy density, consistent with a scalar field that has the dimensions of length (i.e., a displacement).
  • Third, I wanted to spell out some of the details of the derivation that are omitted from nearly all textbooks yet, I am obliged to admit, almost stumped me. That is, once you see the derivation the steps are reasonably trivial, but it is still hard to stumble upon exactly the right way to apply the relevant identities related to Fourier transforms and Dirac deltas.
  • Lastly, I find it revealing how this approach can highlight exactly where a quantum theory is introduced. In the particle theory case, it is when we assume that “mixed states”, that is, linear combinations of eigenstates also represent physical states of a system, despite the fact that they do not correspond to classical eigenvalues. In the case of a field theory, the transition occurs when we replace Fourier coefficients with operators: implicit in the transition is that once again, mixed states are included as representing actual physical states of the system.

Note also how none of this has anything to do with interpretations. There is no “collapse of the wave function” or any such nonsense. That stuff happens when we introduce into our consideration a “measurement event”, effectively an interaction between the quantum system and a classical instrument, which forces the quantum system into an eigenstate. This eigenstate cannot be predicted from the initial conditions alone, precisely because the classical idealization of the measurement apparatus effectively amounts to an admission of ignorance about its true quantum state.

 Posted by at 6:27 pm
Jul 152015
 

For the past ten years, I have been thinking about NASA’s New Horizons probe as the space probe that will eventually fly by Pluto if all goes well and its systems perform as expected.

Well, that historic flyby happened today, and New Horizons sent back pictures to prove it. Best of all, it successfully re-established contact after performing its flyby observations. Now we will have to wait many months (more than a year, as a matter of fact) before all the collected data is radioed back to the Earth.

But we already have amazing photos. A sight never seen by a human being up until just over a day ago.

 Posted by at 1:35 am
Jul 062015
 

I like New Scientist. This weekly British popular science publication was able to maintain reasonably high standards. More or less.

But not last week. Typos or the occasional excess hype on the cover page are one thing, but what is the excuse for this?

For the record, the solar system is not traveling at two-thirds the speed of light in its voyage around the center of the Milky Way.

To their credit, it has since been corrected on the Web site, but still. Very disappointing.

newscicor

 Posted by at 12:08 pm
Jun 212015
 

There is a particularly neat way to derive Schrödinger’s equation, and to justify the “canonical substitution” rules for replacing energy and momentum with corresponding operators when we “quantize” an equation.

Take a particle in a potential. Its energy is given by

$$E=\frac{{\bf p}^2}{2m}+V({\bf x}),$$

or

$$E-\frac{{\bf p}^2}{2m}-V({\bf x})=0.$$

Now multiply both sides this equation by the formula \(e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}\). We note that this exponential expression cannot ever be zero if the part in the exponent that’s in parentheses is real:

$$\left[E-\frac{{\bf p}^2}{2m}-V({\bf x})\right]e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}=0.$$

So far so good. But now note that

$$Ee^{i({\bf p}\cdot{\bf x}-Et)/\hbar}=i\hbar\frac{\partial}{\partial t}e^{i({\bf p}\cdot{\bf x}-Et)/\hbar},$$

and similarly,

$${\bf p}^2e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}=-\hbar^2{\boldsymbol\nabla}e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}.$$

This allows us to rewrite the previous equation as

$$\left[i\hbar\frac{\partial}{\partial t}+\hbar^2\frac{{\boldsymbol\nabla}^2}{2m}-V({\bf x})\right]e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}=0.$$

Or, writing \(\Psi=e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}\) and rearranging:

$$i\hbar\frac{\partial}{\partial t}\Psi=-\hbar^2\frac{{\boldsymbol\nabla}^2}{2m}\Psi+V({\bf x})\Psi,$$

which is the good old Schrödinger equation.

The method works for an arbitrary, generic Hamiltonian, too. Given

$$H({\bf p})=E,$$

we can write

$$\left[E-H({\bf p})\right]e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}=0,$$

which is equivalent to

$$\left[i\hbar\frac{\partial}{\partial t}-H(-i\hbar{\boldsymbol\nabla})\right]\Psi=0.$$

So if this equation is identically satisfied for a classical system with Hamiltonian \(H\), what’s the big deal about quantum mechanics? Well… a classical system satisfies \(E-H({\bf p})=0\), where \(E\) and \({\bf p}\) are eigenvalues of the differential operators \(i\hbar\partial/\partial t\) and \(-i\hbar{\boldsymbol\nabla}\), respectively. Schrödinger’s equation, on the other hand, remains valid in the general case, not just for the eigenvalues.

 Posted by at 6:29 pm
Jun 182015
 

Having just finished work on a major project milestone, I took it easy for a few days, allowing myself to spend time thinking about other things. That’s when I encountered an absolutely neat problem on Quora.

pi

Someone asked a seemingly innocuous number theory question: are there two positive integers such that one is exactly the π-th power of the other?

Now wait a minute, you ask… We know that π is a transcendental number. How can an integer raised to a transcendental power be another integer?

But then you think about \(\alpha=\log_2 3\) and realize that although \(\alpha\) is a transcendental number, \(2^\alpha=3\). So why can’t we have \(n^\pi=m\), then?

As it turns out, we (probably) cannot, but the reason is subtle and it relies on a very important, but unproven conjecture from transcendental number theory.

But first, let us rewrite the equation by taking its logarithm:

$$\pi\log n = \log m.$$

We can also divide both sides by \(\log n\), which leads to

$$\pi = \frac{\log m}{\log n}=\log_n m,$$

but it turns out to be not very helpful. However, squaring the equation will help, as we shall shortly see:

$$\pi^2\log^2 n=\log^2 m.$$

Can this equation ever by true for positive integers \(n\) and \(m\), other than the trivial solution \(n=m=1\), that is?

To see why it cannot be the case, let us consider the following triplet of numbers:

$$(i\pi,\log n,\log m),$$

and their exponents,

$$(e^{i\pi}=-1, e^{\log n}=n, e^{\log m}=m).$$

The three numbers \((i\pi,\log n,\log m)\) are linearly independent over \({\mathbb Q}\) (that is, the rational numbers). What this means is that there are no rational numbers \(A, B, C, D\) such that \(Ai\pi+B\log n+C\log m + D=0\). This is easy to see as the ratio of \(\log n\) and \(\log m\) is supposed to be transcendental but both numbers are real, whereas \(i\pi\) is imaginary.

On the other hand, their exponents are all rational numbers (\(-1, n, m\)). And this is where the unproven conjecture, Schanuel’s conjecture, comes into the picture. Schanuel’s conjecture says that given \(n\) complex numbers \((\alpha_1,\alpha_2,…,\alpha_n)\) that are linearly independent over the rationals, out of the \(2n\) numbers \((\alpha_1,…,\alpha_n,e^{\alpha_1},…,e^{\alpha_n})\), at least \(n\) will be transcendental numbers that are algebraically independent over \({\mathbb Q}\). That is, there is no algebraic expression involving roots and powers of the \(\alpha_i\), \(e^{\alpha_i}\), and rational numbers that will yield 0.

The equation \(\pi^2\log^2 n=\log^2 m\), which we can rewrite as

$$(i\pi)^2\log^2 n + \log^2 m=0,$$

is just such an equation, and it can never be true.

I wish I could say that I came up with this solution but I didn’t. I was this close: I was trying to apply Schanuel’s conjecture, and I was of course using the fact that \(\pi=-i\log -1\). But I did not fully appreciate the implications and meaning of Schanuel’s conjecture, so I was applying it improperly. Fortunately, another Quora user saved the day.

Still I haven’t had this much fun with pure math (and I haven’t learned this much pure math all at once) in years.

 Posted by at 8:25 pm
May 242015
 

John Forbes Nash Jr. is dead, along with his wife Alicia. They were killed on the New Jersey Turnpike when the taxi, taking them home from the airport, crashed into a guardrail and another vehicle after the driver lost control while trying to pass.

Nash and his wife were returning from Norway, where Nash was one of the recipients of the 2015 Abel prize.

News of this accident made me shudder for another reason. Less than two weeks ago, when I was returning from Dubai, my taxi driver not only answered a call on his cell phone, he even responded to a text while driving. I was too tired to say anything at first and then thankfully he came to his senses… but his behavior made me feel decidedly uncomfortable in his vehicle. Next time, I will not hesitate to tell the taxi driver to stop immediately or call another taxi for me.

 Posted by at 1:38 pm
Apr 302015
 

OK, I have had some sad good-byes in my blog this month, so here is a bittersweet one.

Earlier this afternoon, NASA’s Messenger probe, the first planetary probe to orbit Mercury, crashed into Mercury’s surface.

Although this means the end of Messenger, it also means that this particular probe fulfilled all expectations and then some: it worked flawlessly until it ran out of fuel and could no longer maintain a stable orbit around Mercury. The information it provided about the Solar System’s innermost planet will no doubt be studied for many years to come.

Good-bye, Messenger, and thanks for all the good work.

 Posted by at 4:50 pm
Mar 232015
 

Emmy Noether… not exactly a household name, at least outside of the community of theoretical physicists and mathematicians.

Which is why I was so surprised today when I noticed Google’s March 23 Doodle: a commemoration of Emmy Noether’s 133rd birthday.

Wow. I mean, thank you, Google. What a nice and deserving tribute to one of my heroes.

 Posted by at 11:36 pm
Mar 052015
 

Last month, something happened to me that may never happen again: I had not one but two papers accepted by Physical Review D in the same month, on two completely different topics.

The first was a paper I wrote with John Moffat, showing how well his scalar-tensor-vector gravity theory (STVG, also called MOG) fits an extended set of Milky Way rotational curve data out to a radius of nearly 200 kpc. In contrast, the archetypal modified gravity theory, MOND (Mordehai Milgrom’s MOdified Newtonian Dynamics) does not fare so well: as it predicts a flat rotation curve, its fit to the data is rather poor, although its advocates suggest that the fit might improve if we take into account the “external” gravitational field due to other galaxies.

The other paper, which I wrote together with an old friend and colleague, Eniko Madarassy, details a set of numerical simulations of self-gravitating Bose-Einstein condensates, which may form exotic stars or stellar cores. There has been some discussion in the literature concerning the stability of such objects. Our simulation shows that they are stable, which confirms my own finding, detailed in an earlier paper (which, curiously, was rejected by PRD), namely that the perceived instability arises from an inappropriate application of an approximation (the Thomas-Fermi approximation) used to provide a simplistic description of the condensate.

allcases

Oh, and we also had another paper accepted, not by Physical Review D, but by the International Journal of Modern Physics D, but still… it is about yet another topic, post-Galilean coordinate transformations and the analysis of the N-body problem in general relativity. Unlike the first two papers, this one was mostly the work of my co-author, Slava Turyshev, but I feel honored to have been able to contribute. It is a 48-page monster (in the rather efficient REVTeX style; who knows how many pages it will be in the style used by IJMPD) with over 400 equations.

All in all, a productive month insofar as my nonexistent second career as a theoretical physicist is concerned. Now I have to concentrate on my first job, the one that feeds the cats…

 Posted by at 3:21 pm
Feb 082015
 

cat-dead-aliveI have some half-baked ideas about the foundations of quantum physics (okay, who doesn’t.) When I say half-baked, I don’t mean that they are stupid (I sure hope not!) I simply mean I am not 100% sure about them, and there is more to learn.

But, I am allowed to have opinions. So when I came across this informal 2013 poll among (mostly) quantum physicists, I decided to answer the questions myself.

Question 1: What is your opinion about the randomness of individual quantum events (such as the decay of a radioactive atom)?

a. The randomness is only apparent: 9%
b. There is a hidden determinism: 0%
c. The randomness is irreducible: 48%
d. Randomness is a fundamental concept in nature: 64%

(“Jedenfalls bin ich überzeugt, daß [der Alte] nicht würfelt.”)

Question 2: Do you believe that physical objects have their properties well defined prior to and independent of measurement?

a. Yes, in all cases: 3%
b. Yes, in some cases: 52%
c. No: 48%
d. I’m undecided: 9%

(Note that the question does not say that “well-defined” is a synonym for “in an eigenstate”.)

Question 3: Einstein’s view of quantum mechanics

a. Is correct: 0%
b. Is wrong: 64%
c. Will ultimately turn out to be correct: 6%
d. Will ultimately turn out to be wrong: 12%
e. We’ll have to wait and see: 12%

(Einstein’s views are dated, but I feel that he may nonetheless be vindicated because his reasons for holding those views would turn out to be valid. But, we’ll have to wait and see.)

Question 4: Bohr’s view of quantum mechanics

a. Is correct: 21%
b. Is wrong: 27%
c. Will ultimately turn out to be correct: 9%
d. Will ultimately turn out to be wrong: 3%
e. We’ll have to wait and see: 30%

(If I said “wait and see” on Einstein’s views, how could I possibly answer this question differently?)

Question 5: The measurement problem

a. A pseudoproblem: 27%
b. Solved by decoherence: 15%
c. Solved/will be solved in another way: 39%
d. A severe difficulty threatening quantum mechanics: 24%
e. None of the above: 27%

(Of course it’s a pseudoproblem. It vanishes the moment you look at the whole world as a quantum world.)

Question 6: What is the message of the observed violations of Bell’s inequalities?

a. Local realism is untenable: 64%
b. Action-at-a-distance in the physical world: 12%
c. Some notion of nonlocality: 36%
d. Unperformed measurements have no results: 52%
e. Let’s not jump the gun—let’s take the loopholes more seriously: 6%

(I don’t like how the phrase “local realism” is essentially conflated with classical eigenstates. Why is a quantum state not real?)

Question 7: What about quantum information?

a. It’s a breath of fresh air for quantum foundations: 76%
b. It’s useful for applications but of no relevance to quantum foundations: 6%
c. It’s neither useful nor fundamentally relevant: 6%
d. We’ll need to wait and see: 27%

(I wish there was another option: e. A fad. Then again, it does have some practical utility, so b is my answer.)

Question 8: When will we have a working and useful quantum computer?

a. Within 10 years: 9%
d. In 10 to 25 years: 42%
c. In 25 to 50 years: 30%
d. In 50 to 100 years: 0%
e. Never: 15%

(The threshold theorem supposedly tells us what it takes to avoid decoherence. What I think it tells us is the limits of quantum error correction and why decoherence is unavoidable.)

Question 9: What interpretation of quantum states do you prefer?

a. Epistemic/informational: 27%
b. Ontic: 24%
c. A mix of epistemic and ontic: 33%
d. Purely statistical (e.g., ensemble interpretation): 3%
e. Other: 12%

(Big words look-up time, but yes, ontic it is. I may have remembered the meaning of “ontological”, but I nonetheless would have looked up both, just to be sure that I actually understand how these terms are used in the quantum physics context.)

Question 10: The observer

a. Is a complex (quantum) system: 39%
b. Should play no fundamental role whatsoever: 21%
c. Plays a fundamental role in the application of the formalism but plays no distinguished physical role: 55%
d. Plays a distinguished physical role (e.g., wave-function collapse by consciousness): 6%

(Of course the observer is a complex quantum system. I am surprised that some people still believe this new age quantum consciousness bull.)

Question 11: Reconstructions of quantum theory

a. Give useful insights and have superseded/will supersede the interpretation program: 15%
b. Give useful insights, but we still need interpretation: 45%
c. Cannot solve the problems of quantum foundations: 30%
d. Will lead to a new theory deeper than quantum mechanics: 27%
e. Don’t know: 12%

(OK, I had to look up the papers, as I had no recollection of the word “reconstruction” used in this context. As it turns out, I’ve seen papers in the past on this topic and they left me unimpressed. My feeling is that even as they purport to talk about quantum theory, what they actually talk about are (some of) its interpretations. And all too often, people who do this leave QFT completely out of the picture, even though it is a much more fundamental theory than single particle quantum mechanics!)

Question 12: What is your favorite interpretation of quantum mechanics?

a. Consistent histories: 0%
b. Copenhagen: 42%
c. De Broglie–Bohm: 0%
d. Everett (many worlds and/or many minds): 18%
e. Information-based/information-theoretical: 24%
f. Modal interpretation: 0%
g. Objective collapse (e.g., GRW, Penrose): 9%
h. Quantum Bayesianism: 6%
i. Relational quantum mechanics: 6%
j. Statistical (ensemble) interpretation: 0%
k. Transactional interpretation: 0%
l. Other: 12%
m. I have no preferred interpretation 12%

(OK, this is the big one: which camp is yours! And the poll authors themselves admit that it was a mistake to leave out n. Shut up and calculate. I am disturbed by the number of people who opted for Everett. Information-based interpretations seem to be the fad nowadays. I am surprised by the complete lack of support for the transactional interpretation, and also by the low level of support for Penrose. I put myself in the Other category, because my half-baked ideas don’t precisely fit into any of these boxes.)

Question 13: How often have you switched to a different interpretation?

a. Never: 33%
b. Once: 21%
c. Several times: 21%
d. I have no preferred interpretation: 21%

(I am not George W. Bush. I don’t “stay the course”. I change my mind when I learn new things.)

Question 14: How much is the choice of interpretation a matter of personal philosophical prejudice?

a. A lot: 58%
b. A little: 27%
c. Not at all: 15%

(I put my mark on a. because that’s the way it is today. If you asked me how it should be, I’d have answered c.)

Question 15: Superpositions of macroscopically distinct states

a. Are in principle possible: 67%
b. Will eventually be realized experimentally: 36%
c. Are in principle impossible: 12%
d. Are impossible due to a collapse theory: 6%

(Of course it’s a. Quantum physics is not about size, it’s about the number of independent degrees of freedom.)

Question 16: In 50 years, will we still have conferences devoted to quantum foundations?

a. Probably yes: 48%
b. Probably no: 15%
c. Who knows: 24%
d. I’ll organize one no matter what: 12%

(Probably yes but do I really care?)

OK, now that I answered these poll questions myself, does that make me smart? I don’t feel any smarter.

 Posted by at 2:52 pm
Jan 162015
 

Beagle 2 has been found.

Beagle 2 was the British lander component of the European Space Agency’s Mars Express mission. It was supposed to land on Mars on Christmas Day, 2003; however, no radio signal was ever received from the spacecraft. Beagle 2 was considered lost, its fate unknown.

But now, it has been found. Beagle 2, together with its parachute and rear cover, have been spotted by the High Resolution Imaging Science Experiment (HiRISE) camera on board the Mars Reconnaissance Orbiter (MRO) spacecraft, which itself has been orbiting Mars since March 10, 2006.

Imagine: a spacecraft orbiting another planet was able to spot an object barely more than a square meter in size, on that planet’s surface.

We may not yet have humans walking on Mars, but nonetheless, we live in amazing times. Now if only we somehow managed to stop murdering and hating each other, I might even begin to believe that there is hope for us yet…

 Posted by at 11:27 pm
Jan 042015
 

Courtesy to a two-part article (part 1 and part 2, in Hungarian) of the Hungarian satirical-liberal magazine Magyar Narancs (Hungarian Orange), I now have a much better idea of what happened at Hungary’s sole nuclear generating station, the Paks Nuclear Power Plant, in 2003. It was the most serious nuclear incident to date in Hungary (the only INES level 3 incident in the country.)

At the root of the incident is a characteristic issue with these types of Soviet era nuclear reactors leading to magnetite contamination of the fuel elements and control rods. To deal with this contamination and prolong the life of fuel elements, cleaning ponds are installed next to the reactor blocks, where under roughly 30 feet of water, in a specially designed cleaning tank, fuel bundles can be cleaned.

As the problem of contamination became increasingly acute, the power plant ordered a new type of cleaning tank. On April 10, 2003, this cleaning tank was used for the first time on fuel bundles that were freshly removed from the reactor. The cleaning of the fuel bundles was completed successfully by 5 PM in the afternoon; however, the crane that was supposed to replace the fuel bundle in the reactor was used for another task and was not going to be available before midnight. The situation was complicated by language issues, as the technicians attending the new cleaning tank were from Germany and could not speak Hungarian. Nonetheless, the German crew assured the plant’s management that the delay would not represent a problem and that cooling of the fuel bundle inside the cleaning tank was adequate.

Shortly before 10 PM, an alarm system detected increased radiation and noble gas levels in the hall housing the cleaning pond. Acting upon the suspicion that a fuel rod assembly was leaking (the German crew suggested that the fuel bundles may have been incorrectly placed in the cleaning tank) the crew proceeded with a plan to open the cleaning tank. When the lid of the cleaning vessel was unlocked, a large steam bubble was released, and radiation levels spiked. Indeed, the crane operator received a significant dose of radiation contamination on his face and arms. The hall was immediately evacuated and its ventilation system was turned on. However, as the system had no adequate filtering systems installed (despite a regulation that six years prior mandated their installation) some radiation was released into the environment.

As it turns out, the culprit was the new type of cleaning tank. A model that, incidentally, was approved using an expedited process, due to the urgency of the situation at the power plant. The fact that the supplier was a proven entity also contributed to a degree of complacency.

Both the new and the old tank had a built-in pump that circulated water and kept the fuel bundle cool. However, in the old tank, the water inlet was at the bottom, whereas the outlet was near the top. This was not the case in the new tank: both inlet and outlet were located at the bottom, which allowed the formation of steam inside the cleaning vessel near the top. Combined with the lack of instrumentation, and considering that the fuel bundle released as much as 350 kW of heat, this was a disaster in the making.

And that is exactly what happened: due to the delay with the crane, there was enough time for the heat from the fuel bundle to cause most of the water inside the vessel to turn into steam, and the fuel elements heated to 1,000 degrees Centigrade. This caused their insulation to crack, which led to the initial detection of increased radiation levels. When the cleaning tank’s lid was opened, a large bubble of steam was released, while cold water rushed in causing a minor steam explosion and breaking up the fuel elements inside, contaminating the entire pond.

It took another ten years before the last remaining pieces of broken-up fuel elements were removed from the power plant, taken by train through Ukraine to a reprocessing plant in Russia. The total cost of the incident was in the $100 million range.

As nuclear incidents go, Paks was by no means among the scariest: after all, no lives were lost, there was only one person somewhat contaminated, and there was negligible environmental damage. This was no Chernobyl, Fukushima or Three Mile Island. There was some economic fallout, as this reactor block remained inoperative for about a year, but that was it.

Nonetheless, this incident is yet another example how inattention by regulatory agencies, carelessness, or failure to adhere to regulations can lead to catastrophic accidents. Despite its reputation, nuclear power remains one of the safest (and cleanest!) ways to generate electricity but, as engineers are fond of saying, there are no safeguards against human stupidity.

 Posted by at 4:25 pm
Dec 242014
 

Year after year, I can find no better way to wish Merry Christmas to all my family, my friends, and all good people on Earth, than with the immortal words of Apollo 8 astronaut Frank Borman from 46 years ago: “And from the crew of Apollo 8, we close with good night, good luck, a Merry Christmas and God bless all of you – all of you on the good Earth.

 Posted by at 3:57 pm