Three days ago, the 2016 Nobel Prize in Physics was awarded to Michael Kosterlitz of Brown University:

David Thouless of the University of Washington:

and Duncan Haldane of Princeton University:

They won it for their “theoretical discovery of topological phase transitions and topological phases of matter”, which was later confirmed by many experiments.

Sadly, the world’s reaction was aptly summarized by *Wired* magazine’s headline:

Nobel Prize in Physics Goes to Another Weird Thing Nobody Understands

Journalists worldwide struggled to pronounce ‘topology’, and a member of the Nobel prize committee was reduced to waving around a bagel and a danish to explain what the word means:

That’s fine as far as it goes: I’m all for using food items to explain advanced math! However, it doesn’t explain what Kosterlitz, Thouless and Haldane actually did. I think a 3-minute video with the right animations would make the beauty of their work perfectly clear. I can see it in my head. Alas, I don’t have the skill to make those animations—hence this short article.

I’ll just explain the Kosterlitz–Thouless transition, which is an effect that shows up in thin films of magnetic material. Haldane’s work on magnetic wires is related, but it deserves a separate story.

I’m going to keep this very quick! For more details, try this excellent blog article:

• Brian Skinner, Samuel Beckett’s guide to particles and antiparticles, *Ribbonfarm*, 24 September 2015.

I’m taking all my pictures from there.

### The idea

Imagine a thin film of stuff where each atom’s spin likes to point in the same direction as its neighbors. Also suppose that each spin must point in the plane of the material.

Your stuff will be happiest when all its spins are lined up, like this:

What does ‘happy’ mean? Physicists often talk this way. It sounds odd, but it means something precise: it means that the energy is low. When your stuff is very cold, its energy will be as low as possible, so the spins will line up.

When you heat up your thin film, it gets a bit more energy, so the spins can do more interesting things.

Here’s one interesting possibility, called a ‘vortex’:

The spins swirl around like the flow of water in a whirlpool. Each spin is *fairly* close to being lined up to its neighbors, except near the middle where they’re doing a terrible job.

The total energy of a vortex is enormous. The reason is not the problem at the middle, which certainly contributes some energy. The reason is that ‘fairly’ close is not good enough. The spins fail to perfectly line up with their neighbors even far away from the middle of this picture. This problem is bad enough to make the energy huge. (In fact, the energy would be *infinite* if our thin film of material went on forever.)

So, even if you heat up your substance, there won’t be enough energy to make many vortices. This made people think vortices were irrelevant.

But there’s another possibility, called an ‘antivortex’:

A single antivortex has a huge energy, just like a vortex. So again, it might seem antivortices are irrelevant if you’re wondering what your stuff will do when it has just a little energy.

But here’s what Kosterlitz and Thouless noticed: the combination of *a vortex together with an antivortex* has much less energy than either one alone! So, when your thin film of stuff is hot enough, the spins will form ‘vortex-antivortex pairs’.

Brian Skinner has made a beautiful animation showing how this happens. A vortex-antivortex pair can appear out of nothing:

… and then disappear again!

Thanks to this process, at low temperatures our thin film will contain a dilute ‘gas’ of vortex-antivortex pairs. Each vortex will stick to an antivortex, since it takes a lot of energy to separate them. These vortex-antivortex pairs act a bit like particles: they move around, bump into each other, and so on. But unlike most ordinary particles, they can appear out of nothing, or disappear, in the process shown above!

As you heat up the thin film, you get more and more vortex-antivortex pairs, since there’s more energy available to create them. But here’s the really surprising thing. Kosterlitz and Thouless showed that as you turn up the heat, there’s a certain temperature at which the vortex-antivortex pairs suddenly ‘unbind’ and break apart!

Why? Because at this point, the density of vortex-antivortex pairs is so high, and they’re bumping into each other so much, that we can’t tell which vortex is the partner of which antivortex. All we’ve got is a thick soup of vortices and antivortices!

What’s interesting is that this happens *suddenly* at some particular temperature. It’s a bit like how ice *suddenly* turns into liquid water when it warms above its melting point. A sudden change in behavior like this is called a **phase transition**.

So, the **Kosterlitz–Thouless transition** is the sudden unbinding of the vortex-antivortex pairs as you heat up a thin film of stuff where the spins are confined to a plane and they like to line up.

In fact, the pictures above are relevant to many other situations, like thin films of superconductive materials. So, these too can exhibit a Kosterlitz–Thouless transition. Indeed, the work of Kosterlitz and Thouless was the key that unlocked a treasure room full of strange new states of matter, called ‘topological phases’. But this is another story.

### Puzzles

What is the actual definition of a vortex or antivortex? As you march around either one and look at the little arrows, the arrows turn around—one full turn. It’s a **vortex** if when you walk around it clockwise the little arrows make a full turn *clockwise*:

It’s an **antivortex** if when you walk around it clockwise the little arrows make a full turn *counterclockwise*:

Topologists would say the vortex has ‘winding number’ 1, while the antivortex has winding number -1.

In the physics, the winding number is very important. Any collection of vortex-antivortex pairs has winding number 0, and Kosterlitz and Thouless showed that situations with winding number 0 are the only ones with small enough energy to be important for a large thin film at rather low temperatures.

Now for the puzzles:

**Puzzle 1:** What’s the mirror image of a vortex? A vortex, or an antivortex?

**Puzzle 2:** What’s the mirror image of an antivortex?

Here are some clues, drawn by the science fiction writer Greg Egan:

and the mathematician Simon Willerton:

### For more

To dig a bit deeper, try this:

• The Nobel Prize in Physics 2016, Topological phase transitions and topological phases of matter.

It’s a very well-written summary of what Kosterlitz, Thouless and Haldane did.

Also, check out Simon Burton‘s simulation of the system Kosterlitz and Thouless were studying:

In this simulation the spins start out at random and then evolve towards equilibrium at a temperature far below the Kosterlitz–Thouless transition. When equilibrium is reached, we have a gas of vortex-antivortex pairs. Vortices are labeled in blue while antivortices are green (though this is not totally accurate because the lattice is discrete). Burton says that if we raise the temperature to the Kosterlitz–Thouless transition, the movie becomes ‘a big mess’. That’s just what we’d expect as the vortex-antivortex pairs unbind.

I thank Greg Egan, Simon Burton, Brian Skinner, Simon Willerton and Haitao Zhang, whose work made this blog article infinitely better than it otherwise would be.

Thanks.

That’s fine as far as it goes, but how about enlightening us about the relevance of braid group reps?

That’s another story! For what Kosterlitz, Haldane and Thouless did, this is very good:

• The Nobel Prize in Physics 2016, Topological phase transitions and topological phases of matter.

You won’t see any braid group representations in here. However, you’ll see how they laid the groundwork, by showing how the first Chern class and U(1) Chern–Simons theory are important in 1-dimensional and 2-dimensional magnetic materials.

Thank you!

What do you mean by “mirror image”?

As far as I can tell from these pictures, mirroring a vortex will just cause it to change direction, i.e. it will still be a vortex but, if you look at it from above the thin film and it spun around clockwise, after mirroring (or, which should be equivalent, changing your perspective to looking at the same film from below), you’ll get a vortex which spins counterclockwise and vice versa.

Now for the anti-vortex, things seem a little bit more complicated. I can seemingly identify four different axes – a) two along the diagonals, b) two as far off them as possible – with two different outcomes:

Mirroring along a) will not change the system at all.

Mirroring along b) will also reverse direction.

And I’m currently not able to imagine what happens if you look at the same structure from below but I think it might end up reversing the direction just like for normal vortices.

Here is another puzzle: What about higher winding numbers?

I tried scribbling on paper and I think I found a shape that basically traces out a lemniscate which should correspond to a vortex of winding number 2.

I think I, by a similar process, also found something with winding number -2 which seems to look like the above anti-vortex in its hyperbolic-plane-y pattern but with a total of six spokes instead of four, if that makes sense.

Do these also occur? Can it happen, that you, for instance, spontaneously get two anti-vortices and a 2-vortex, where the 2-vortex stays in place and the two anti-vortices fly apart?

Or alternatively, once you are in this new phase where these things become common, will two vortices or anti-vortices merge to become 2-vortices or -2-vortices respectively?

kram1032 wrote:

I mean that we take the picture, hold it in front of us facing away, and look at its image in a mirror. For example, the mirror image of this:

is this:

So then it’s exactly what I worked out in my reply above.

Oh, so “kram1032” is

you!Hi!Yes, your solutions seem correct. I just didn’t want to give away the answers prematurely.

One can certainly draw vector fields with larger winding number, either positive or negative. I’m fairly sure that, like the basic vortex and antivortex configurations, these ‘

n-vortices’ will have infinite energy unlessnis zero.I don’t really know anything about these

n-vortices. I would guess that below the Kosterlitz-Thouless transition there’s a pretty good description of the system as a gas of vortex-antivortex pairs, and above it as a dense plasma of vortices and antivortices, without any need to considern-vortices with |n| > 1. However, I could easily be wrong! I haven’t read any of the extensive literature on this subject!Oh whoops I forgot my name differs in g+, heh. Didn’t even think about how that could not have been clear, sorry.

Thank you for the excellent explanation!

Fascinating images.

Thanks. But we should thank Richard Skinner!

There are many more images that

shouldbe included here, which I can see in my mind. Let me describe two:1) Start with this:

Then, rotate each arrow about its tail at the same rate. At any moment in time we’ll have a picture that physicists would call a

vortex—but they’ll look dramatically different.2) Start with this:

Then, rotate each arrow about its tail at the same rate. At any moment in time we’ll have a picture that physicists would call an

antivortex—but they’ll look dramatically different.In case anyone wants to animate these, here’s the math. In the first case, at each point with polar coordinates we draw a unit vector pointing in the direction

at time In the second case, at each point with polar coordinates we draw a unit vector pointing in the direction

at time

Ah, so this is important because we are supposed to think of these vortices as being somehow the same: it’s the U(1) gauge degree of freedom.

Right, in the Landau–Ginzburg model of a 2d superconductor, the field usually called

is a unit complex number at the minimum of its potential, so we get a field of unit vectors on the plane. Rotating all these vectors by the same angle counts as a ‘global gauge transformation’: that is, we get a new field that counts as physically equivalent.

We can also take a continuum limit of the classical XY model, and get a simple model of a 2d ferromagnet in which the atom’s spins are described by a field of unit vectors on the plane, which we can think of as a field of unit complex numbers:

and the energy is

Rotating all the these unit complex numbers by the same angle gives a new field with the same energy. So, it’s a symmetry of the theory!

This symmetry also preserves the ‘winding number’, which is computed as an integral around a large circle in the plane: it’s a way to precisely define the number of vortices minus the number of antivortices.

The negative vortices look like the gradient of a scalar field with a saddle point, and using the U(1) symmetry we can transform the positive vortices into the gradient of a local minima or maxima. What’s going on here? If I keep thinking about this does it lead to something fancy like Chern-Simons theory?

Chern–Simons theory is certainly related to the work of Kosterlitz, Thouless and especially Haldane. Only U(1) Chern–Simons theory shows up, and that makes it a lot simpler than if we had a nonabelian gauge group. The easiest way to get started is to read this:

• The Nobel Prize in Physics 2016, Topological phase transitions and topological phases of matter.

It’s really quite well-written.

The connection to saddle points, local maxima and local minima is simpler. For that, try this:

• Wikipedia, Index of a vector field.

Here’s an animation of the rotating version John described:

this looks really neat!

It’s a little weird, though, that the arrows seem to not only rotate, they also shift around.

I think that “shifting” is an optical illusion. Knowing Greg, he would have firmly nailed the tail of each arrow to a fixed location. The tails would still

seemto shift, since our eyes’ main way of locating an object is relative to other objects, and the heads of the arrows are moving around.Is there a specific reaon for rotating the arrows around their tail? Greg’s animations made me dizzy! Here’s my attempt where I rotate the arrows around their centre.

Nice! Okay, now I get it. Rotating the arrows around their midpoints rather than their tails is less creepy—it feels less like a drug trip scene in an old 1950’s movie, where the walls are bending.

Here’s the anti-vortex version with arrows spinning around their centre.

Thanks, Simon. Very nice!

Puzzle 3:As these unit vectors rotate, at what moments do we get a vector field that’s obtained by normalizing a vector field with curl zero?Puzzle 4:As these unit vectors rotate, at what moments do we get a vector field that’s obtained by normalizing a vector field with curl zero?I thought of these puzzles because at certain moments, these unit vector fields are obtained by normalizing rather famous curl-free vector fields. I don’t know of any deep significance, but there could be one.

Very interesting.

Can you say some words about what your cobordism hypothesis is (or was before it became a theorem) and whether and how it fits in here?

The cobordism hypothesis arose from attempts to classify topological quantum field theories. Very roughly, a field theory is called “topological” if it’s invariant under all diffeomorphisms of spacetime. The theory studied by Kosterlitz and Thouless is not topological in this sense. However, it introduced topological considerations into condensed matter physics in a way that ultimately led to a very fruitful interaction between that subject and topological quantum field theory.

As for what the cobordism hypothesis

is, my best explanation is here:• John Baez and James Dolan, Higher-dimensional algebra and topological quantum field theory,

Jour. Math. Phys.36(1995), 6073–6105.Ah …. so many meanings of “topological”. Thank you for the clarification.

It turns out that the most exciting qualitative properties of topological phases are often summarized by topological quantum field theories, even for phases arising from theories that are not themselves topological.

Looking at the mirror for helical vortices/antivortices is the same as rotating the picture around x or y axes. So here, parity is changed by a 180 deg rotation.

I had a bit of fun trying to simulate this system. Here is what I ended up with:

Positive vortices are blue, and negative vortices are green (it’s not totally accurate because the lattice is discrete.) It looks like vortices attract, which makes sense given your description of the infinite energy of an isolated vortex. The temperature is way below the Kosterlitz–Thouless transition. Raising the temperature to that point it just becomes a big mess.

Excellent! Yes, a vortex will attract an antivortex, since their total energy goes to infinity as you pull them apart taking their distance to infinity.

Now that I think of it, this is similar to how a quark-antiquark pair in a meson increases in energy roughly linearly as you pull them apart. In that situation the field energy is concentrated in a ‘flux tube’ connecting the quarks. Eventually there’s enough energy to create a new quark-antiquark pair: the flux tube gets cut into two shorter flux tubes.

(I don’t have a good mental image of where the field energy lies when you have a distant vortex-antivortex pair, so I don’t know if it mainly lies in a ‘tube’ connecting the two.)

I wonder if there’s

visibledramatic change near the Kosterlitz–Thouless transition. Google leads me to this picture:but I don’t know exactly what it means. The lower right looks like the ‘big mess’ you mentioned.

I did some more experimenting and came up with this:

I added a “heat map” to show how much energy each compass needle has, and also varied the temperature so that you can see the onset of the KT transition. It does look like there are tendrils of excitation extending between the vortices, but it’s hard to see.

Nice! One can start to see how fascinating this model is. It’s on that nice cusp between being simple enough to understand and complex enough to be deeply interesting.

Nice! Can you try if a temperature gradient across the critical temperature makes a difference?

Also, do you think you could host a video file somewhere? YouTube makes quite a mess out of the video due to compression. It really doesn’t like lots of small, fast-changing objects.

Many thanks for your fascinating insights on this phenomenon, John. Please forgive my naivete, but what minimum temperature is required to spontaneously create a vortex-antivortex pair? Can it occur at 0 K? Is there any connection to the creation of electron-positron pairs?

At absolute zero any physical system will definitely be in its lowest-energy state, or a randomly chosen lowest-energy state if there is more than one. Since a vortex-antivortex pair has more energy than a state in which all the spins are aligned, you’ll never see a vortex-antivortex pair at absolute zero.

For any physical system as soon as the temperature exceeds absolute zero, there’s

somenonzero probability to find that system in any state. Thus, there’ssomenonzero probability to find a vortex-antivortex pair in any given large region of the magnet as soon as the temperature exceeds zero, but this probability will be low for low temperatures.Kosterlitz and Thouless won the Nobel for discovering that this particular system has a

phase transitionat some positive temperature This means that the probability of finding vortex-antivortex pair in any given large region of the magnet is not analytic as a function of temperature at the point The system ‘changes phase’, a bit like ice melting or water vaporizing: vortex-antivortex pairs become common and the system is qualitatively different.This is the famed

Kosterlitz–Thouless transition.It’s slightly similar: as you heat up any system, high-energy states become more probable. Thus as you heat up a box of gas, or a box of radiation, to a sufficiently high temperature, electron-positron pairs will eventually become common. I happen to have worked out the temperature a few weeks ago, and it’s roughly 12 billion kelvin.

To estimate this, take the mass of the electron and convert it into units of energy. The answer is 0.511 MeV, where MeV or ‘million electron volts’ is a common unit of energy in particle physics. Multiply by two to get the energy of a positron-electron pair: roughly 1 MeV. Convert this to a temperature using the formula where is Boltzmann’s constant. In other words, let It’s convenient to note that is about 12,000 kelvin per eV. Thus, 1 MeV divided by Boltzmann’s constant is about 12,000,000,000 kelvin.

So, at a temperature of about 12 billion kelvin, electron-positron pairs become common. This is not an all-or-nothing thing, and I don’t know if there’s a phase transition. Someone must know.

Temperatures were this high in the early Universe, and also in the jets produced by black holes, and some other extreme situations. Here’s a jet coming out of the supermassive black hole at the center of the galaxy M87, where this is happening:

If I knew the energy of a vortex-antivortex pair, I could do a similar calculation to give a

rough estimateof the temperature at which the Kosterlitz–Thouless transition occurs. But I’m sure people have worked out the details in a much more precise: there’s even a whole book on the Kosterlitz-Thouless transition.Somewhat related: https://en.wikipedia.org/wiki/Pair-instability_supernova

Cool! If spontaneous creation of lots of electron-positron pairs could suddenly cause a star to collapse and go supernova, it sounds like there

isa phase transition at work here… at least if the pressure is high.These curl equations are fascinating and are of course endemic in applications from electromagnetics to fluid dynamics. Perhaps there is some overlap with the model of the QBO equatorial winds that we are working on at John’s Azimuth Forum (see sidebar) and at my blog. Have some notes here:

http://contextearth.com/2016/09/23/compact-qbo-derviation/#comment-199906

Paul Pukite

A closely related topological phase transition is described by the Quantum Hall Effect and Fractional Quantum Hall Effect. That was a hot topic when I was in grad school growing GaAs quantum well structures. Stormer and Tsui eventually won a Nobel Prize after they experimentally discovered the fractional effect that Laughlin had predicted.

I mention this because in last month’s blog post linked in my comment above, I stated that I applied knowledge of the Hall effect in solving the QBO problem. The two phenomenon share similar curl terms. The math is the common tie between these systems.

from “Modeling water waves beyond perturbations”

Making progress in one area certainly has application in other disciplines.

Fascinating. So how about three dimensions? I guess point like singularities are out of the question if the analogy with vortices still holds. Is there such a thing as an anti vortex ring?

In a Type II superconductor, the magnetic field is confined in ‘flux tubes’, also known as Abrikosov vortices. They act like vortice in the following sense: the vector potential is a vector field with

where is the magnetic field, but except inside these tubes. Thus, the is curl-free outside these tubes— but it curls around inside these tubes! So, you can roughly imagine a flux tube as a little tornado but where the wind is the vector potential

But it gets better. Thanks to quantum mechanics, each tube carries one ‘quantum of magnetic flux’. That is, the integral of the field over a disk cutting one of these tubes is a certain fixed value depending only on fundamental constants of nature: the magnetic flux quantum!

If you have a fairly thin film made of a type II superconductor, these flux tubes tend to line up at right angles to the film. In a homogeneous material, they’re happiest forming a lattice! Here’s an actual picture of what they look like, created in a lab in 1989:

So far this is all sounding fairly similar to what Kosterlitz and Thouless were studying. However, I believe that in

thissituation, the antiparticle of a vortex is a vortex spinning the other way—that is, a mirror-image vortex.John,

Your wording is a bit confusing about the appearance of the KT pairs. As Simon Burton’s excellent video shows they appear at far below the transition temperature , as the pairing reduces the activation energy to a finite number. However they stay bound together below and only break at above (or in Simon’s words “become a big mess”). This is what the Nobel committee has to say:

However in your blog and comments you termed it as “the Kosterlitz–Thouless transition is the sudden appearance of large numbers of vortex-antivortex pairs as you heat up”, which while maybe true (in the sense that more pairs certainly will appear as the temperature rises) is not quite the same as what the Nobel committee is saying. So which one is correct?

Thanks for the excellent illustrations (and amazing contributions from commenters).

The Nobel committee is, unsurprisingly, correct. In my blog article I was trying to say, in a very nontechnical way, that various quantities depend on the temperature in a way that fails to be analytic (i.e., given by a convergent Taylor series) at the phase transition. I

guessedthat the density of vortices is one of these quantities. I do not actually know this to be true. Since I was in a rush, I made the mistake of stating my guess as a fact. Then I made the further mistake of trying to express my guess in simple terms by saying there’s a “sudden appearance of large numbers of vortex-antivortex pairs” as the temperature passes through the phase transition.I knew full well that the vortex density could fail to be non-analytic even without a sudden increase in the density as we increase the temperature past the phase transition. I felt mildly guilty about this, but you’ve simultaneously pointed out the problem and pointed to a good expository solution—that is, a nice way to explain what’s really happening!

Briefly: in the Kosterlitz–Thouless transition, the vortex-antivortex pairs “unbind” and we get a messy soup of vortices and antivortices.

This reminds me a bit of a quark-gluon plasma. In neutronium that’s not too hot, quarks, antiquarks and gluons are bound into nucleons, perhaps with some mesons hopping around between them. But when we heat it up enough, we go through a phase transition called ‘deconfinement’, leading to a new state of matter called a quark-gluon plasma. In fact the full story here is more complicated, more interesting, and not fully understood. Click on the image for more:

So, I’ll fix my blog article. However, I would also love to see a graph of the density of

Great. Thanks for the quark-gluon plasma analogy. Very interesting! BTW, I remember reading your physics newsgroup posts before there was the web in the early 90s when I was a physics grad student. I couldn’t really follow back then but I am glad that I can understand this post and was even able to contribute a little.

P.S. Thanks for fixing the formatting issues in my comment. And please feel free to delete my other duplicate comment (which I wasn’t sure was going through).

I’m glad you survived my physics posts from the early 90’s! It’s nice to hear from people who remember that ancient era. Thanks again for helping me improve my article. It’s a lot better now, and I think it’s still comprehensible by ordinary folks.

Thank you for a very nice explanation of the KT transition. Most of the time I don’t have a clue about who the Nobel prize winners are, but this is something that I actually knew something about, even if it was a long time ago I learned about it and my memory is hazy. Let me just point out that the phase diagram of the XY model is really weird, because there is no ordered phase below the KT transition.

The point is that domain walls destroy long-range order in low dimensions. In 1D a domain wall consists of a single pair of opposite spins, which can be excited at any non-zero temperature. In 2D you can only have long-range order in systems with discrete symmetry, like the Ising model. In systems with continuous symmetry, the energy of a domain wall decreases with its thickness. The cost of exciting a very thick domain wall is neglible, so again this will happen at any non-zero temperature.

However, the XY model is a bordering case, because below the KT transition the correlation length is infinite although there is no long-range order (this is called quasi-long-range order). Instead correlation functions decay with a power law, and the power depends on temperature. So there is a continuum of inequivalent critical systems up to the KT transition. Above that, the correlation length becomes finite.

Being 2D critical systems, this continuum is described by a continuum of inequivalent CFTs, all with c = 1.

That’s cool! I hadn’t heard of ‘quasi-long-range order’. I have the feeling that these technical subtleties about the XY model are part of why experts got so excited about the Kosterlitz–Thouless transition: it opened up new worlds that hadn’t been considered before.

I’ve updated my blog article thanks to help from Greg Egan, Simon Burton, Simon Willerton and Haitao Zhang, and credited them for their work. It’s much better now!

There is some substantial information on the Nobel prize home page: https://www.nobelprize.org/nobel_prizes/physics/laureates/2016/advanced.html.

Yes, that’s what I recommended that people read in my blog article above:

I have a problem near the phase transition; if the temperature is near the phase transition (for an infinitesimal difference in the temperature), and the material is homogeneus and without imperfections (so that the vortex-antivortex are uniform), then is there a temperature where the vortex-antivortex collide in a single singularity (in the form of a eight) for an overlap of vortices? I was thinking that a superconductive nanomaterial like a sphere, or a torus (without borders) could contain colliding singularities, or is it all too simple?

My first remark is that a phase transition can only occur in this kind of magnet—or indeed, almost any commonly studied physical system—when it has infinite spatial extent. Only in this limit do the expected values of physical quantities cease to be smooth functions of temperature! (For a large but finite system, these functions will be smooth, but some of their derivatives may become huge.)

So, a spherical or torus-shaped magnet of this sort won’t have a true phase transition. Nonetheless it’s very interesting to study vortices and antivortices on these topologies.

[…] Empezamos por el “Premio Nobel de Física 2016: Los físicos teóricos Thouless, Haldane y Kosterlitz por los materiales topológicos 2D”, LCMF, 04 Oct 2016; puedes ver algunas animaciones de vórtices, antivórtices y de la transición de fase BKT en John Baez, “Kosterlitz–Thouless Transition”, Azimuth, 07 Oct 2016. […]

This article got a bunch of hits from readers of the financial news magazine

Bloomberg View, thanks to:• Mark Buchanan, A Nobel that helps explain why a bagel always has hole,

Bloomberg View, 13 October 2016.The title and lead picture plays up the “topology as the science of bagels” theme that I was mocking, but the article gets past that in a nice way, while remaining utterly non-technical.

And Bob Dylan beats out Joan Baez for the Nobel Prize in Literature. Who’d a thunk?

[…] But add even more energy and there is a critical level where the vortex and antivortex can separate. This is named the “Kosterlitz-Thouless transition” after two of the Nobel Prize awardees. It is a phase transition, meaning an abrupt change of state like the melting of ice into water at around 0°C or the evaporation of water into steam at around 100°C. (My summary is based on the very readable introduction by John Baez, who is also an internet relativity personality by the way.) […]