Landon Lehman

Updates on my interests/research

Integrating the Kuramota-Sivashinsky Equation in Mathematica

I recently was reading this paper by Jaideep Pathak, Brian Hunt, Michelle Girvan, Zhixin Lu, and Edward Ott (because I read this article by Natalie Wolchover), and got interested in trying to reproduce the numerical integration of the Kuramota-Sivashinsky equation as shown in Figure 2 of the paper (sorry, I know the paper is paywalled):

KS_plotThe top plot is the numerical integration, the middle one is the prediction using reservoir computing, and the bottom is the difference. For now, I am just interested in the top plot.

I found a nice paper by Aly-Khan Kassam and Lloyd Trefethen that contains Matlab code for doing this integration (using a method they developed called exponential time-differencing). I reproduced this code in Mathematica. There were a few annoying differences; the worst one being a difference in the Fourier conventions between Matlab and Mathematica.

Here is the Mathematica code initializing things:

carbon

The initial profile looks like this:

Untitled

Then code for calculating some things used in the integration loop:

carbon2.png

And finally the full numerical integration loop:

carbon3.png

The result can be plotted using ListPlot3D:

listplot3d

I should emphasize that this is nothing original; I just changed a few small things to make the Matlab code given by Kassam and Trefethen work in Mathematica. I put the full Mathematica code on my github in case anyone finds it useful. I’m sure the code could be shortened and made more efficient by using some of Mathematica’s functional programming capabilities.

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Wave Animations

I’m teaching a “General Physics 3” course this semester, and in looking for materials I came across this excellent page by Dan Russell: http://www.acs.psu.edu/drussell/demos.html. I only wish I had discovered this before I taught the chapters on mechanical and sound waves!

I especially like the discussion and animations on the difference between displacement and pressure in standing sound waves: http://www.acs.psu.edu/drussell/Demos/StandingWaves/StandingWaves.html. Students found this confusing in lecture and I think seeing the animations would have really helped.

The Difference Between 6 and 7

A ring system consists of n  “light” point masses orbiting around a “heavy” central mass. Assume that the orbit is circular and the light masses are equally spaced around the circle. The relevant physical force is Newtonian gravity.

Here is a ring system with n = 6:

6_rings

And here is a ring system with n = 7:

7_rings

 

The ring system with n = 6 is always linearly unstable, while the ring system with n = 7 can be stable (if the central mass satisfies a certain condition).

See the detailed analysis here: https://arxiv.org/abs/astro-ph/0606510, by Robert J. Vanderbei and Egemen Kolemen.

This is closely related to work done by Maxwell (yes, the electromagnetism Maxwell) on the stability of the rings of Saturn. Speaking of which, some amazing pictures have been taken of Saturn’s rings:

PIA21628_-_B_Ring_fine_structure_in_color

The above is a high-resolution image in the Solar System sense – each pixel corresponds to about 3 square kilometers! The image was taken by the Cassini Orbiter. (More info here: https://photojournal.jpl.nasa.gov/catalog/PIA21628).

 

Physics Has Changed

Ok, physics hasn’t changed (with the exception of exciting new discoveries of course).

But the way we teach and present physics to students has changed.

21 pages into the 1937 book An Outline of First Year College Physics (by Dr. Clarence Bennett):

physics_book

Most modern textbooks that I am familiar with would take 5-6 times as many pages to reach the same point. One that I just pulled off of my shelf takes over 10 times as many pages.

An Outline of First Year College Physics is available on the Internet Archive: https://archive.org/details/outlineoffirstye00benn.

 

Entropy of a d-dimensional ideal gas

I’m slowly reading through Kittel and Kroemer to refresh my knowledge of basic statistical mechanics and thermodynamics. They have a nice little problem at the end of Chapter 3 (Problem 11), which is to calculate the entropy of a one-dimensional ideal gas (using the methods outlined in that chapter). It is only a brief step further to calculate the general expression for the entropy of a {d}-dimensional ideal gas, which I do here.

The single-particle partition function is calculated using the “particle-in-a-box” solution from quantum mechanics, and the end result is that

\displaystyle  	Z_1 = \left( \int_0^\infty \text{d}n\, e^{-\alpha^2 n^2} \right)^d = \left( 	\frac{ \sqrt{\pi}}{2\alpha}\right)^d, \ \ \ \ \ (1)

where

\displaystyle  	\alpha = \left( \frac{\hbar^2 \pi^2}{2 M L^2 \tau} \right)^{1/2}. \ \ \ \ \ (2)

Define the {d}-dimensional quantum concentration as {n_{Q_d} = Z_1/L^d}, then by plugging in we get

\displaystyle  	n_{Q_d} = \left( \frac{M\tau}{2\pi \hbar^2} \right)^{d/2}. \ \ \ \ \ (3)

The free energy is (using the Stirling approximation)

\displaystyle  	F = - \tau N \log{(Z_1)} + \tau (N \log{(N)} - N), \ \ \ \ \ (4)

and thus the entropy is

\displaystyle  	\sigma = - \left( \frac{\partial F}{\partial \tau} \right)_V = N 	\left( \log{\left(\frac{Z_1}{N}\right)} + 1 + \tau \frac{\partial \log{Z_1}}{\partial 	\tau} \right). \ \ \ \ \ (5)

Now, we can use the properties of the logarithm to make taking the derivative really easy, since

\displaystyle  	\log{Z_1} = \frac{d}{2} \log{\tau} + \cdots 	 \ \ \ \ \ (6)

where I have dropped all of the terms that don’t depend on the temperature. So

\displaystyle  	\frac{\partial \log{Z_1}}{\partial \tau} = \frac{d}{2\tau}, 	 \ \ \ \ \ (7)

and the final result for the entropy is

\displaystyle  	\sigma = N \left( \log{\left( \frac{n_{Q_d}}{n}\right)} + \frac{d}{2} + 1 \right). \ \ \ \ \ (8)

Here I have defined {n = N/L^d}.

For 1,2, and 3 dimensions, we have

\displaystyle  	\sigma_1 = N \left( \log{\left( \frac{n_{Q_1}}{n} \right)} + \frac{3}{2} 	\right), \ \ \ \ \ (9)

\displaystyle  	\sigma_2 = N \left( \log{\left(\frac{n_{Q_2}}{n} \right)} + 2 	\right), \ \ \ \ \ (10)

and

\displaystyle  	\sigma_3 = N \left( \log{\left(\frac{n_{Q_3}}{n} \right)} + \frac{5}{2} 	\right). \ \ \ \ \ (11)

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Anatomy of an “Anomaly”

On Tuesday, December 15 of last year, the LHC experimental collaborations ATLAS and CMS released the first results from the 13 TeV run. The most exciting news was a bump in the diphoton spectrum at about 750 GeV. This could be a sign of new physics (finally), or it might just be a fluctuation (the statistical significance is not very high). We will probably have to wait until at least late summer to find out whether or not the bump disappears with more statistics (this an optimistic estimate as far as magnet issues go).

Of course this “anomaly” is exciting and gives theorists something to think about. But I want to focus on the amount of thinking that has been done already, measured in part by the papers that have been written. (Of course, one could argue that the number of papers written is not a good proxy variable for the amount of real, hard thinking that has been done. One might have a point.)

Seven papers citing the ATLAS or CMS papers were submitted on the day of the announcement (i.e. the same day the ATLAS and CMS papers were released). Obviously a good number of theorists had advance warning. Here is a plot of the number of papers versus the date of their arXiv submissions from Dec. 15 until today (not counting the papers that just showed up on the arXiv tonight).

diphoton_stats

The vertical orange lines are for Mondays, the day when diphoton papers were most likely to be submitted. There is an idea that your paper is most likely to be read if you submit in on a Monday (so it shows up on the arXiv on Tuesday). So far there have been 172 papers!

For those interested in how I made the plot, I used inspire and searched for papers citing either the ATLAS results or the CMS results, and sorted by the earliest date recorded (“de”). I didn’t use both/and, because sometimes it takes a while for inspire to correctly catch all of the citations.

 

 

New books

“To those of my colleagues who predict that computers will soon replace human mathematicians by virtue of their superior skill and reliability in proving theorems, I am inclined to respond that the goal of mathematics is to convert rigorous proofs to heuristics. The latter are, in turn, used to produce new rigorous proofs, a necessary input (but not the only one) for new heuristics.”

– Michael Harris, Mathematics without Apologies: Portrait of a Problematic Vocation, 2015

Also, a Princeton Companion to Physics is scheduled to come out in 2018, with Wilczek as editor. The Princeton Companion to Mathematics – edited by Gowers, is quite nice, so I will be anticipating the physics one.

Firenze and amplitudes

I am headed to Firenze (Florence), Italy this weekend to attend a 3-week-long winter school at the Galileo Galilei Institute for Theoretical Physics. It should be a good place to meet some new people and perhaps come up with new ideas to explore. Perhaps there will be time to explore the city as well!

In December I thought about calculating Yang-Mills amplitudes in 6 dimensions by using the formalism outlined in a paper by Cheung and O’Connell. In the paper, they calculate the the 4- and 5-point amplitudes by using BCFW recursion on the 3-point amplitude. The interesting thing about 6-dimensional amplitudes is that all of the 4-dimensional helicity structures can be obtained from a single expression in 6 dimensions. For example, 4D MHV amplitudes are contained in the “general” 6D expression. So if there were a simple expression for an n-point 6D amplitude, like there is a simple expression for a 4D MHV n-point amplitude, it would contain all of the 4D tree-level amplitudes.

Unfortunately the 6D amplitudes become complicated very quickly. The 3-point amplitude must be written using special kinematic variables, and using these the 4-point amplitude can be deduced from BCFW. The 4-point Einstein gravity amplitude can also be obtained by using the KLT relations. The 4-point amplitude has a relatively simple structure, but applying BCFW to this structure and calculating the 5-point amplitude gives a very complicated expression (at least I think it is complicated!). Perhaps some new notation is needed in order to see the underlying structure. Or maybe 6D is just inherently more complicated than 4D, and it would be easy to just directly attack the 4D problem instead of solving it in 6D and reducing to 4D.

I also thought about the application of on-shell methods to effective field theories. This possibility has been explored for the nonlinear sigma model using “semi-on-shell” amplitudes. In general, adding masses to the spinor-helicity formalism makes it more complicated, and I am not sure what it means to integrate out a particle in this formalism. And since integrating out heavy particles from a Lagrangian is the most common form of generating an effective field theory, it would be useful to have a way to translate this procedure into spinor helicity language.

Update

Almost done with my second year of classes (I will be done by Wednesday).  I will probably sit in on some classes next year, but this marks the likely end of my formal coursework. Now research starts “for real,” which is exciting (and somewhat frightening)!

On the research side of things, a couple of my fellow graduate students and I just had a paper accepted for publication!

On the more formal, coursework side of things, I feel that I still have only a marginal grasp of quantum field theory. I want to work through Weinberg’s trilogy on the subject, but it is proving to be a very slow and arduous task. Perhaps by the end of this summer I will have finished Volume 1.  One of my goals for this year was to finish the entire trilogy, and that is looking unlikely unless I really pick up the pace.

Other books I want to read in the near future: QFT in a Nutshell by Zee and Dynamics of the Standard Model by Donoghue, Golowich, and Holstein. Also, a new book by Schwartz just came out that looks good.  Between reading and research I should have a busy summer!

 

Galileo

Go look at the last 12 or so slides in this presentation.  I hope this will be released soon – it should be fun to play around with.  I am especially interested to see how it works out the problem of finding invariants in general tensor products of Lie group representations.  At this point I am not sure how to do this in an algorithmic manner. After seeing the slides, I was inspired to write a short Mathematica function that finds the terms of a given dimension allowed by some collection of scalar fields with different U(1) charges. This was relatively easy – the hard part would be finding all the independent singlets of, for example, SU(2) that can then be formed once the U(1) constraint is satisfied.  Automatically generating the terms in, for example, the Higgs potential in this paper, would be impressive.

And here is the mandatory comment on BICEP2: I don’t understand inflationary physics nearly well enough to offer anything original – and if I did, I would probably be writing a paper on it right now.