Category Archives: Misc

Visiting Brandeis

I gave a talk at Brandeis’s High Energy Theory Seminar this week. Brandeis is much easier to park at than Brown, but it’s proportionately easier to get lost in. While getting lost, I happened to run into this:

Many campuses have buildings that look like castles. Usen Castle is the only one I’ve seen that officially calls itself a castle. It’s a dorm, and the students there can honestly say that they live in a castle.

If I were a responsible, mature blogger, I’d tell you about the history of the place. I’d tell you who built it, and why they felt it was appropriate to make a literal castle the center of their college.

As I’m not a responsible, mature blogger, I’ll just leave you with this thought: they have a castle!

New Guide, Taking Suggestions

Hello readers!

Some of you have probably read the guide to N=4 super Yang-Mills theory linked at the top of my blog’s home page. A few of you even discovered this blog via the guide.

I’m thinking about doing another series of posts, like those, explaining a different theory. I’d like to get an idea of which theory you guys are most interested in seeing described. Whichever I choose, it will be largely along the same lines as the N=4 posts, so focused less on technical details and more on presenting something that a layman can understand.

Here are some of the options I’m considering:

  • N=8 Supergravity: Very broadly speaking, this is gravity’s equivalent of N=4 super Yang-Mills. It’s connected to N=4 in a variety of interesting ways, and it’s something I’d like to work more with at some point.
  • The (2,0) Theory: This was the motivation behind my first paper. It’s harder to explain than some of the other theories because it doesn’t have an easy analogy with the particles of the real world. It’s also even harder to work with, to the point that saying something rigorous about it is often worthy of a paper on its own.
  • String Theory/M Theory: This is a big topic, and there are many sites out there already that cover aspects of it. What I might try to do is look for an angle of approach that others haven’t covered, and try to explain some slightly more technical aspects of the situation in a popularly approachable way.

I could also give a more detailed description of some method from amplitudeology, like generalized unitarity or symbology.

Finally, I could always just keep posting like I have been doing. But this seems like a good time to add to my site’s utility. So what do you think? What should I talk about?

Shout-Out for a Fellow Blogger

This is a blog about explaining science. Science is for everybody!

In particular, science is not just for geeks/those into geek culture. Nevertheless, I’m willing to bet that a substantial fraction of you are into something nerdy, whether sci-fi, fantasy, or one of the many genres and subgenres that have sprung up in the crazy genre jungles of the internet.

As such, some of you may be aware of Geek and Sundry, the Felicia Day-headed geek media mini-empire. They’re adding a set of new Vloggers (like bloggers but with video), and they’re running a contest to determine their lineup. And of these Vloggers, you should definitely vote for Kiri Callaghan.

I know Kiri as a kickass director from way back when I used to do community theatre stuff. These days, she’s running an extra-mini geek media empire of her own, centered around her blog. This blog somehow manages to update every weekday (and used to update every day), which as someone who updates once a week I can tell you is physically impossible, especially while also holding down a real job which she apparently does. She almost certainly owns a Time Turner or something.  So yeah, very impressive, and the high quality nerd stuff attached (check out some of her parody songs, in particular I Dreamed a Dream of Firefly) adds to the picture.

So for those in the audience who are into this sort of thing, vote for her! Comment on the video (apparently the scoring for this stage is based on interaction with commenters)! Join the facebook group to keep tabs on the competition!

There’s something about Symmetry…

Physicists talk a lot about symmetry. Listen to an article about string theory and you might get the idea that symmetry is some sort of mysterious, mystical principle of beauty, inexplicable to the common man or woman.

Well, if it was inexplicable, I wouldn’t be blogging about it, now would I?

Symmetry in physics is dead simple. At the same time, it’s a bit misleading.

When you think of symmetry, you probably think of objects: symmetric faces, symmetric snowflakes, symmetric sculptures. Symmetry in physics can be about objects, but it can also be about places: symmetry is the idea that if you do an experiment from a different point of view, you should get the same results. In a way, this is what makes all of physics possible: two people in two different parts of the world can do the same experiment, but because of symmetry they can compare results and agree on how the world works.

Of course, if that was all there was to symmetry then it would hardly have the mystical reputation it does. The exciting, beautiful, and above all useful thing about symmetry is that, whenever there is a symmetry, there is a conservation law.

A conservation law is a law of physics that states that some quantity is conserved, that is, cannot be created or destroyed, but merely changed from one form to another. Energy is the classic example: you can’t create energy out of nothing, but you can turn the potential energy of gravity on top of a hill into the kinetic energy of a rolling ball, or the chemical energy of coal into the electrical energy in your power lines.

The fact that every symmetry creates a conservation law is not obvious. Proving it in general and describing how it works required a major breakthrough in mathematics. It was worked out by Emmy Noether, one of the greatest minds of her time, which given that her time included Einstein says rather a lot. Noether struggled for most of her life with the male-dominated establishment of academia, and spent many years teaching unpaid and under the names of male faculty, forbidden from being a professor because of her gender.

Why must women always be banished to the Noether regions of physics?

Noether’s proof is remarkable, but if you’re not familiar with the mathematics it won’t mean much to you. If you want to get a feel for the connection between symmetries and conservation laws, you need to go back a bit further. For the best example, we need to go all the way back to the dawn of physics.

Christiaan Huygens was a contemporary of Isaac Newton, and like Noether he was arguably as smart as if not smarter than his more famous colleague. Huygens could be described as the first theoretical physicist. Long before Newton first wrote his three laws of motion, Huygens used thought experiments to prove deep facts about physics, and he did it using symmetry.

In one of Huygens’ thought experiments, two men face each other, one standing on a boat and the other on the bank of a river. The men grab onto each other’s hands, and dangle a ball on a string from each pair of hands. In this way, it is impossible to tell which man is moving each ball.

Stop hitting yourself!

From the man on the bank’s perspective, he moves the two balls together at the same speed, which happens to be the same speed as the river. The balls are the same size, so as far as he can see they should have the same speed afterwards as well.

On the other hand, the man in the boat thinks that he’s only moving one ball. Since the man on the bank is moving one of the balls along at the same speed as the river, from the man on the boat’s perspective that ball is just staying still, while the other ball is moving with twice the speed of the river. If the man on the bank sees the balls bounce off of each other at equal speed, then the man on the boat will see the moving ball stop, and the ball that was staying still start to move with the same speed as the original ball. From what he could see, a moving ball hit a ball at rest, and transferred its entire momentum to the new ball.

Using arguments like these, Huygens developed the idea of conservation of momentum, the idea of a number related to an object’s mass and speed that can never be created or destroyed, only transferred from one object to another. And he did it using symmetry. At heart, his arguments showed that momentum, the mysterious “quantity of motion”, was merely a natural consequence of the fact that two people can look at a situation in two different ways. And it is that fact, and the power that fact has to explain the world, that makes physicists so obsessed with symmetry.

Valentine’s Day Physics Poem

In honor of Valentine’s Day, a physics-themed poem I wrote a few years ago, about unrequited love.

Measurement:

 

I once took a measurement

It was a simple, two-body problem,

Solvable. Not Poisson’s mess.

Two particles, drifting, perhaps entangled.

I wanted to know two things:

Position, and momentum:

Where they were, and where they might go.

 

I perturbed the system

Like a good scientist, I interacted, and observed,

Added input, caused change.

Then I knew their positions.

They became tightly entangled,

Bound together,

And there was no way of knowing

Any way they could change.

 

I should have remembered:

In quantum systems

The observer is always involved;

And a three-body problem

Has no solution.

Black Holes and a Superluminal River of Glass

If I told you that scientists have been able to make black holes in their labs for years, you probably either wouldn’t believe me, or would suddenly get exceptionally paranoid. Turns out it’s true, provided you understand a little bit about black holes.

A black hole is, at its most basic, an object that light cannot escape. That’s why it’s “black”: it absorbs all colors of light. That’s really, deep down, all you need in order to have a black hole.

Black holes out in space, as you are likely aware, are the result of collapsed stars. Gather enough mass into a small enough space and, according to general relativity, space and time begin to bend. Bend space and time enough and the paths that light would follow curve in on themselves, until inside the event horizon (the “point of no return”) the only way light can go is down, into the center of the black hole.

That’s not the only way to get a “point of no return” though. Imagine flying a glider above a fast-moving river. If the plane is slower than the river, then any object placed in the river is like a “point of no return”:  once the object passes you, you can never fly back and find it again.

Of course, trying to apply this to light runs into a difficulty: you can have a river faster than a plane, but it’s pretty hard to have a river faster than light. You might even say it’s impossible: nothing can travel faster than light, after all, right?

The idea that nothing can travel faster than light is actually a common misconception, held because it makes a better buzzword than the truth: nothing can travel faster than light in a vacuum. Light in a vacuum goes straight to its target, the fastest thing in the universe. But light in a substance, moving through air or water or glass, gets deflected: it runs into atoms, gets absorbed, gets released, and overall moves slower. So in order to make a black hole, all we need is some substance moving faster than light moves in that substance: a superluminal river of glass.

(By the way, is that not an amazingly evocative phrase? Sounds like the title of a Gibson novel.)

Now it turns out that literally making glass move faster than light moves inside it is still well beyond modern science. But scientists can get around that. Instead of making the glass move, they  make the properties of the glass change, using lasers to alter the glass so that the altered area moves faster than the light around it. With this sort of setup, they can test all sorts of theoretical black hole properties up close, in the comfort of a university basement.

That’s just one example of how to create an artificial black hole. There are several others, and all of them rely on various ingenious manipulations of the properties of matter. You live in a world in which artificial black holes are routine and diverse. Inspiring, no?

Wormholes and Donut Holes

I’ve heard people claim that in order to understand wormholes, you need to understand five-dimensional space.

Well that’s just silly.

A wormhole is often described as a hole in space-time. It can be imagined as a black hole where instead of getting crushed when you fall in to the center, you emerge somewhere else (or even some-when else: wormholes are possibly the only way to get time travel). They’re a staple of science fiction, even if they aren’t always portrayed accurately.

Probably not what a wormhole looks like

How does this work? Well like many things in physics, it’s helpful to imagine it with fewer dimensions first:

Suppose that you live on the surface of a donut. You can’t get up off the surface; you’re stuck to its gooey sugary coating. All you can do is slide around it.

It’s a simple life

Let’s say that one day you’re sitting on the pink side of the donut, near the center. Your friend lives on the non-frosted side, and you want to go see her. You could go all the way back to the outside edge of the donut, around the side, and down to the bottom, but you’re tired and the frosting is sticky. Luckily, you can use your futuristic pastry technology, the donut hole! Instead of going around the outside, you dive in through the inside hole, getting to your friend’s house much faster.

That’s really all a wormhole is. Instead of living on a two-dimensional donut surface, you live in a world with three space dimensions and one time dimension. A wormhole is still just like a donut hole: a shortcut, made possible by space being a non-obvious shape.

Now earlier I said that you don’t need to understand five-dimensional space to understand wormholes, and that’s true. Yes, real donuts exist in three dimensions…but if you live on the surface only, you only see two: inward versus outward, and around the center. It’s like a 2D video game with a limited map: the world looks flat, but if you go up past the top edge you find yourself on the bottom. Going from the top edge directly to the bottom is easier than going all the way down the screen: it’s just the same as a wormhole. You don’t need extra dimensions to have wormholes, just rules: when you go up far enough, you come back down. Go to the center of the wormhole, and come out the other side. And as one finds in physics, it’s the rules, not naïve intuitions, that determine how the world works. Just like a video game.

Who Am I?

I call myself a String Theorist, someone who describes the world in terms of subatomic lengths of string that move in ten dimensions (nine of space and one of time),

But in practice I’m more of a Particle Theorist, describing the world not in terms of short lengths of string but rather with particles that each occupy a single point in space,

More specifically, I’m an Amplitudeologist, part of a trendy new tribe including the likes of Zvi Bern, Lance Dixon, Nima Arkani-Hamed, John Joseph Carrasco (jjmc on twitter), and sometimes Sheldon Cooper,

In terms of my career, I’m a Graduate Student, less like a college student and more like an apprentice, learning not primarily through classes but rather through working to advance my advisor’s research,

And what do I work on? Things like this.