Tension

A D-braneIt was a fun week in the string theory class this week, as we got to some major landmarks that are always fun to teach. We’ve uncovered the extended objects called D-branes (see numerous previous posts for how useful and important these objects are in string theory research) in all their glory in the lectures before, and deduced lots of their properties, such as the form of the action that determines how a D-brane moving in spacetime responds to the various fields (including the geometry) created by the string theory. That’s all fun, but then the key thing to do next is to compute the mass of these dynamical objects, or the mass per unit volume – the tension. Computing it fully, with no hand-wavy factors. Your mass measures how strongly you interact with gravity. So you can measure it by studying the gravitational interaction between masses. (You do that when you step on a scale to measure your weight… well the scale does it by showing how much force it takes to stop you from falling through the floor toward the center of the earth…)

d-brane_emit_absorbSo in class this is when we go all Polchinski and unpack the tension computation, stopping to admire the various features of string theory you learn along the way, and seeing how simply beautifully the various basic features of the superstring theories that we’ve met in the last few lectures encode themselves in one nice object – the vacuum amplitude  {\cal A } from the cylinder diagram representing either exchange of closed strings (including quanta like the graviton – this is what you focus on to learn what the mass is) between a pair of D-branes, or an open string with its ends tethered to a pair of D-branes going in a closed loop. That there are two ways of looking at the diagram, an open string way (running time around the cylinder) and a closed string way (running time along the cylinder) is a hugely powerful thing, and is at the heart of so very much of what we do in string theory these days especially – including a lot of what I’ve told you in previous posts (see e.g. here and here) about applications to things of interest in current experiments.

One of the fun things about all this is that the answer is actually {\cal A}=0. It is zero because all the infinite modes of oscillation of the string gather themselves up nicely to give a factor:

<br />
q^{-\frac{1}{6}}\prod_{n=1}^{\infty}(1+q^{n-\frac{1}{2}})^8-q^{-\frac{1}{6}}\prod_{n=1}^{\infty}(1-q^{n-\frac{1}{2}})^8-16q^{\frac{1}{3}}\prod_{n=1}^{\infty}(1+q^{n})^8=0\ .<br />

Think of q as a book-keeping device that lets one track energy contributions (in the power of it that appears in a term if one expanded this expression), and how many things contribute with that energy (the coefficient in an expansion)… and so on and so forth. This expression has, in principle, an infinite number of terms at higher and higher powers of q representing more and more contributions from higher frequency oscillations of the string. The vanishing of this somewhat bizarre combination of things was noticed in the middle of the nineteenth Century by Jacobi (he called it an “abstruse” relation, and it keeps this name in the present day…!) We understand why this combination is zero in the present physics context because every term in the expansion of that expression has an interpretation in terms of various oscillations of strings with both bosonic and fermionic modes (states with integer and half-integer spin respectively) involved. The vanishing is due to there being a large amount of supersymmetry present in spacetime that ensures that all bosonic contributions are cancelled by fermionic ones (if you interpret it from the open string point of view). Put differently (the closed string point of view), the attraction of the branes due to exchange of gravitons (and other attractive quanta exchange) is exactly cancelled by repulsion due to exchange of quanta associated to them being like-charged under generalizations of Maxwell’s electromagnetism.

Well, anyway, I’m babbling (you can look up the details in the books and papers by Joe Polchinski, or in my book, references therein, etc)… It’s fun seeing how highly non-trivial mathematics and physics (old and new) are in dialogue with each other over the centuries.

Oh, the best thing that happens when I teach this is when someone interjects with the question “but if the answer is zero, how are we going to extract an answer for the tension from it?!”… I love that question. I did get it this time, happily. And I respond “Aha! Exactly!…”

And off we go.

Next class: Black holes. Hurrah!

-cvj

On this day on Asymptotia...

Some Related Asymptotia Posts (not exhaustive):

Bookmark the permalink.