Archive for Physics

Lincoln – Green Shoots for Maths and Physics?

Posted in Education with tags , , , , on March 3, 2014 by telescoper

I noticed over the weekend that there’s a job being advertised at the University of Lincoln designated Founding Head of the School of Mathematics and Physics. It seems the powers that be at Lincoln University (which is in the Midlands) have decided to set up an entire new activity in Mathematics and Physics. I’m pointing this out not because of any personal connection with the position, but because it’s refreshing to see a new(ish) Higher Education Institute apparently willing to take the plunge and invest in a new venture, particularly because it includes Physics. It wasn’t at all long ago that UK Physics departments were being closed down – the University of Reading being a prominent example, in 2006. I think Reading is thinking of starting up Physics again, in fact. Perhaps these are the green shoots that presage a new spring for Physics in this country? I do hope so.

It won’t be an easy task to start up a new department from scratch in Lincoln: grant funding is tight and the competition for students among established institutions is already so intense that it will be very difficult for a brand new outfit to break through. Nevertheless, I think it’s a praiseworthy initiative and I wish it well.

Sussex University – the Place for Undergraduate Physics Research!

Posted in Education, The Universe and Stuff with tags , , , , , , , on February 27, 2014 by telescoper

One of the courses we offer in the School of Physics & Astronomy here at the University of Sussex is the integrated Masters in Physics with a Research Placement. Aimed at high-flying students with ambitions to become research physicists, this programme includes a paid research placement as a Junior Research Associate each summer vacation for the duration of the course; that means between Years 1 & 2, Years 2 & 3 and Years 3 & 4 . This course has proved extremely attractive to a large number of very talented students and it exemplifies the way the Department of Physics & Astronomy integrates world-class research with its teaching in a uniquely successful and imaginative way.

Here’s a little video made by the University that features Sophie Williamson, who is currently in her second year (and who also in the class to whom I’m currently teaching a module on Theoretical Physics:

This week we had some very good news about another of our undergraduate researchers, Talitha Bromwich, who is now in the final year of her MPhys degree, and is pictured below with her supervisor Dr Simon Peeters:

Talitha Bromwich with her JRA supervisor Dr Simon Peeters at 'Posters in Parliament' event 25 Feb 14

Talitha spent last summer working on the DEAP3600 dark-matter detector after being selected for the University’s Junior Research Associate scheme. Her project won first prize at the University’s JRA poster exhibition last October, and she was then chosen to present her findings – alongside undergraduate researchers from 22 other universities – in Westminster yesterday as part of the annual Posters in Parliament exhibition, organized under the auspices of the British Conference of Undergraduate Research (BCUR).

A judging panel – consisting of Ben Wallace MP, Conservative MP for Wyre and Preston North; Sean Coughlan, Education Correspondent for the BBC; and Professor Julio Rivera, President of the US Council of Undergraduate Research; and Katherine Harrington of the Higher Education Academy – decided to award Talitha’s project First Prize in this extremely prestigious competition.

Congratulations to Talitha for her prizewinning project! I’m sure her outstanding success will inspire future generations of Sussex undergraduates too!

Galaxies, Glow-worms and Chicken Eyes

Posted in Bad Statistics, The Universe and Stuff with tags , , , , , , , , on February 26, 2014 by telescoper

I just came across a news item based on a research article in Physical Review E by Jiao et al. with the abstract:

Optimal spatial sampling of light rigorously requires that identical photoreceptors be arranged in perfectly regular arrays in two dimensions. Examples of such perfect arrays in nature include the compound eyes of insects and the nearly crystalline photoreceptor patterns of some fish and reptiles. Birds are highly visual animals with five different cone photoreceptor subtypes, yet their photoreceptor patterns are not perfectly regular. By analyzing the chicken cone photoreceptor system consisting of five different cell types using a variety of sensitive microstructural descriptors, we find that the disordered photoreceptor patterns are “hyperuniform” (exhibiting vanishing infinite-wavelength density fluctuations), a property that had heretofore been identified in a unique subset of physical systems, but had never been observed in any living organism. Remarkably, the patterns of both the total population and the individual cell types are simultaneously hyperuniform. We term such patterns “multihyperuniform” because multiple distinct subsets of the overall point pattern are themselves hyperuniform. We have devised a unique multiscale cell packing model in two dimensions that suggests that photoreceptor types interact with both short- and long-ranged repulsive forces and that the resultant competition between the types gives rise to the aforementioned singular spatial features characterizing the system, including multihyperuniformity. These findings suggest that a disordered hyperuniform pattern may represent the most uniform sampling arrangement attainable in the avian system, given intrinsic packing constraints within the photoreceptor epithelium. In addition, they show how fundamental physical constraints can change the course of a biological optimization process. Our results suggest that multihyperuniform disordered structures have implications for the design of materials with novel physical properties and therefore may represent a fruitful area for future research.

The point made in the paper is that the photoreceptors found in the eyes of chickens possess a property called disordered hyperuniformity which means that the appear disordered on small scales but exhibit order over large distances. Here’s an illustration:

chicken_eyes

It’s an interesting paper, but I’d like to quibble about something it says in the accompanying news story. The caption with the above diagram states

Left: visual cell distribution in chickens; right: a computer-simulation model showing pretty much the exact same thing. The colored dots represent the centers of the chicken’s eye cells.

Well, as someone who has spent much of his research career trying to discern and quantify patterns in collections of points – in my case they tend to be galaxies rather than photoreceptors – I find it difficult to defend the use of the phrase “pretty much the exact same thing”. It’s notoriously difficult to look at realizations of stochastic point processes and decided whether they are statistically similar or not. For that you generally need quite sophisticated mathematical analysis.  In fact, to my eye, the two images above don’t look at all like “pretty much the exact same thing”. I’m not at all sure that the model works as well as it is claimed, as the statistical analysis presented in the paper is relatively simple: I’d need to see some more quantitative measures of pattern morphology and clustering, especially higher-order correlation functions, before I’m convinced.

Anyway, all this reminded me of a very old post of mine about the difficulty of discerning patterns in distributions of points. Take the two (not very well scanned)  images here as examples:

points

You will have to take my word for it that one of these is a realization of a two-dimensional Poisson point process (which is, in a well-defined sense completely “random”) and the other contains spatial correlations between the points. One therefore has a real pattern to it, and one is a realization of a completely unstructured random process.

I sometimes show this example in popular talks and get the audience to vote on which one is the random one. The vast majority usually think that the one on the right is the one that is random and the left one is the one with structure to it. It is not hard to see why. The right-hand pattern is very smooth (what one would naively expect for a constant probability of finding a point at any position in the two-dimensional space) , whereas the  left one seems to offer a profusion of linear, filamentary features and densely concentrated clusters.

In fact, it’s the left picture that was generated by a Poisson process using a Monte Carlo random number generator. All the structure that is visually apparent is imposed by our own sensory apparatus, which has evolved to be so good at discerning patterns that it finds them when they’re not even there!

The right process is also generated by a Monte Carlo technique, but the algorithm is more complicated. In this case the presence of a point at some location suppresses the probability of having other points in the vicinity. Each event has a zone of avoidance around it; the points are therefore anticorrelated. The result of this is that the pattern is much smoother than a truly random process should be. In fact, this simulation has nothing to do with galaxy clustering really. The algorithm used to generate it was meant to mimic the behaviour of glow-worms (a kind of beetle) which tend to eat each other if they get too close. That’s why they spread themselves out in space more uniformly than in the random pattern. In fact, the tendency displayed in this image of the points to spread themselves out more smoothly than a random distribution is in in some ways reminiscent of the chicken eye problem.

The moral of all this is that people are actually pretty hopeless at understanding what “really” random processes look like, probably because the word random is used so often in very imprecise ways and they don’t know what it means in a specific context like this. The point about random processes, even simpler ones like repeated tossing of a coin, is that coincidences happen much more frequently than one might suppose. By the same token, people are also pretty hopeless at figuring out whether two distributions of points resemble each other in some kind of statistical sense, because that can only be made precise if one defines some specific quantitative measure of clustering pattern, which is not easy to do.

From Real Time to Imaginary Time

Posted in Brighton, Education, The Universe and Stuff with tags , , , , , , , , , , , on February 24, 2014 by telescoper

Yesterday, after yet another Sunday afternoon in my office on the University of Sussex campus, I once again encountered the baffling nature of the “real time boards” at the bus-stop at Falmer Station (just over the road from the University). These boards are meant to show the expected arrival times of buses; an example can be seen on the left of the picture below, taken at Churchill Square (in the City Centre).

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The real-time board system works pretty well in central Brighton, but it’s a very different story at Falmer, especially for the Number 23 which is my preferred bus home. Yesterday provided a typical illustration of the problem: the time of the first bus on the list, a No. 23, was shown as “1 min” when I arrived at the stop. It then quickly moved to “due” (a word which I’ll comment about later). It then moved back to “2 mins” for about 5 minutes and then back to “due” again. It stayed like that for over 10 minutes at which point the bus that was second on the list (a No. 28 from Lewes) appeared. Rather than risk waiting any longer for the 23 I got on the 28 and had a slightly longer walk home from the stop at the other end. Just as well I did because the 23 vanished entirely from the screen as soon as I boarded the other bus. This apparent time-travel isn’t unusual at Falmer, although I’ve never really understood why.

By sheer coincidence when I got to the bus stop to catch a bus to campus this morning there was a chap from Brighton and Hove buses there. He was explaining what sometimes goes wrong with the real time boards to a lady, so I joined in the conversation and asked him if he knew why Falmer is so unreliable. He was happy to oblige. It turns out that the way the real-time boards work depends on each bus having a GPS system that communicates to a central computer via a radio link. If the radio link drops out for some reason – as it apparently does quite often up at Falmer (mobile phone connectivity is poor here also) – the system looks up the expected time of the bus after the one that it has lost contact with. Thus it is that a bus can apparently be “due” and then apparently go back in time. Also, if a bus has to divert from the route programmed into the GPS tracker then it is also removed from the real-time boards.

However, there is another system in operation alongside the GPS tracker. When a bus actually stops at a stop and opens its doors the onboard computer communicates this to the central system at the same time as the location signs inside the bus are updated. At this point the real-time boards are reset.

The unreliability I’ve observed at Falmer is in fact caused by two problems: (i) the patchy radio coverage as the bus wanders around the hilly environs of Falmer campus; and (ii) the No. 23 is on a new route around the back of campus which means that it vanishes from the system entirely when it wanders off the old route, as would happen if the bus were to break down.

Mystery solved then, in a sense, but it means there’s a systematic problem that isn’t going to be fixed in the short-term. Would it be better to switch off the boards than have them show inaccurate information? Perhaps, but only if it were always wrong. In fact the boards seem to work OK for the more frequent bus, the No. 25. My strategy is therefore never to rely on the information provided concerning the No. 23 and just get the first bus that comes. It’s not a problem anyway during the week because there’s a bus every few minutes, but on a Sunday evening it is quite irksome to see apparently random times on the screens.

All this talk about real-time boards reminds me of a question I was asked in a lecture last week. I was starting a new section of my Theoretical Physics module for 2nd Year students on Complex Analysis: the Cauchy-Riemann equations, Conformal Transformations, Contour Integrals and all that Jazz. To start the section I went on a bit of a ramble about the ubiquity of complex numbers in physics and whether this means that imaginary numbers are, in some sense, real. You can find an enjoyable polemic on this subject, given the answer “no” to the question here.

Anyway, I got the class to suggest examples of the use of complex numbers in physics. The things you’d expect came up such as circuit theory, wave propagation etc. Then somebody mentioned that somewhere they had heard of imaginary time. The context had probably been provided Stephen Hawking who mentioned this in his book A Brief History of Time. In fact the trick of introducing imaginary time is called a Wick Rotation and the basic idea is simple. In special relativity we deal with four-dimensional space-time intervals of the form

ds^2 = -c^2dt^2 + dx^2 + dy^2 +dz^2,

i.e. the metric describing Minkowski space. The minus sign in front of the time bit is essential to the causal structure of space-time but it causes quite a few mathematical difficulties. However if we make the substitution

\tau \rightarrow i c t

then the metric becomes

ds^2 = d\tau^2 + dx^2 + dy^2 +dz^2,

which corresponds to a four-dimensional Euclidean space which is in many situations much easier to handle mathematically.

Complex variables and complex functions provide the theoretical physicist with a host of extremely elegant techniques for solving tricky problems. But does that mean they are somehow “built in” to nature? I don’t think so. I don’t think the Brighton & Hove Bus company uses imaginary time on its display boards either, although it does sometimes seem that way.

 

POSTSCRIPT. I forgot to include my planned rant about the use of the word “due”. The boards displaying train times at railway stations usually give the destination and planned departure time of the train, e.g. “Brighton 11.15”. If things are running to schedule this information is supplemented by the phrase “On Time”. If not, which is sadly a more likely contingency in the UK, this changes to “due 11.37” or some such. This really annoys me.: the train is due at 11.15. If it doesn’t come until after then, it’s overdue or, in other words, late.

The most beautiful equation?

Posted in The Universe and Stuff with tags , , , , on February 13, 2014 by telescoper

There’s an interesting article on the BBC website today that discusses the way mathematicians’ brains appear to perceive “beauty”. A (slightly) more technical version of the story can be found here. According to functional magnetic resonance imaging studies, it seems that beautiful equations excite the same sort of brain activity as beautiful music or art.

The question of why we think equations are beautiful is one that has come up a number of times on this blog. I suspect the answer is a slightly different one for theoretical physicists compared with pure mathematicians. Anyway, I thought it might be fun to invite people offer suggestions through the comments box as to the most beautiful equation along with a brief description of why.

I should set the ball rolling myself, and I will do so with this, the Dirac Equation:

dirac_equation

This equation is certainly the most beautiful thing I’ve ever come across in theoretical physics, though I don’t find it easy to articulate precisely why. I think it’s partly because it is such a wonderfully compact fusion of two historic achievements in physics – special relativity and quantum mechanics – but also partly because of the great leaps of the imagination that were needed along the journey to derive it and my consequent admiration for the intellectual struggle involved. I feel it is therefore as much an emotional response to the achievement of another human being – such as one feels when hearing great music or looking at great art – as it is a rational response to the mathematical structure involved. But it’s not just that, of course. The Dirac Equation paved the way to many further developments in particle physics. It seems to encapsulate so much about the behaviour of elementary particles in so few symbols. Some of its beauty also derives from its compactness.

Anyway, feel free to suggest formulae or equations through the comments box, preferably with a brief explanation of why you think they’re so beautiful.

Big Trouble with Big G

Posted in The Universe and Stuff with tags , , on February 4, 2014 by telescoper

An Antonymous email correspondent this morning drew my attention to an interesting article in the latest Physics World about the trials and tribulations of groups of physicists trying to measure Newton’s Gravitational Constant,  G. This is probably the first physical constant that most of us encounter when we’re learning the subject so it might seem strange that it’s the one which is known to the lowest accuracy. That’s not for want of trying to make the measurements more precise, just that gravity is such a very weak force that it’s very difficult to eliminate systematic effects down to the necessary level.

Just how difficult it is to measure Big G is demonstrated by the following graphic which shows the latest measurements:

Big_G

Here’s the caption, so you can identify the various groups responsible for the various measurements:

Disagreeing over “big G” This chart shows wildly differing values of the gravitational constant, G, as measured by various high-profile research groups (blue). The values do not agree even within their error bars. Also shown are two values of G adopted by the Committee on Data for Science and Technology (CODATA) as international standards (red). The groups are based at the National Institute of Standards and Technology (NIST), the University of Washington (UWASH), the International Bureau of Weights and Measures (BIPM), the Measurement Standards Laboratory of New Zealand (MSL), the University of Zurich (UZURICH), the Huazhong University of Science and Technology (HUST) and the Joint Institute for Astrophysics (JILA).

Clearly there’s quite a lot of disagreement between recent results, with some a long way outside each other’s error bars. They can’t all be right, but who’s most likely to be wrong? Answers on a postcard.

I’m by no means an expert on experimental gravity so I won’t attempt to suggest who is right and who is wrong. What I will say is that although this kind of research is clearly extremely important it is clearly also fiendishly difficult. I’m not really surprised that the pieces of the puzzle haven’t fallen into place yet. The dedicated teams who have been tackling this problem for many decades deserve the deep admiration as well as the continued support of the physics community. Theoretical physics is generally perceived to be more glamorous and exciting than its experimental counterpart, but the subject as a whole is nothing without its empirical foundations. That said, I’m glad it’s not my job to measure Big G. I have neither the practical skill nor the patience to cope with so many frustrations!

Methods of Images

Posted in Biographical, Cute Problems, Education with tags , , , , on January 29, 2014 by telescoper

I’ve had a very busy day today including giving a lecture on Electrostatics and the Method of Images and, in an unrelated lunch-hour activity, filing my tax return (and paying the requisite bill). The latter was the most emotionally draining.

With no time for a proper post, I thought I’d give some examples of the images produced by yesterday’s graduands, including some who used a particular approach called the Method of Selfies. Unfortunately some of these are spoiled by having a strange bearded person in the background.

But first you might like to try the following example using the actual Method of Images:

Given two parallel, grounded, infinite conducting planes a distance a apart, we place a charge +q between the plates, a distance x from one of them. What is the force on the charge?

This is, in fact, from Griffiths, David J. (2007) Introduction to Electrodynamics, 3rd Edition; Prentice Hall – Problem 3.35.

Solutions via the comments box as usual, please.

And now here are some of the official pictures from yesterday

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How to Address Gender Inequality in Physics

Posted in Education, The Universe and Stuff with tags , , , , on January 26, 2014 by telescoper

Last night I was drinking a glass or several of wine while listening to the radio and thinking about a brainwave I’d had on Friday. Naturally I decided to wait until I reconsidered it in the cold light and sobriety of day before posting it, which I have now done, so here it is.

The idea that came to me simply joins two threads of discussion that have appeared on this blog before. The first is that, despite strenuous efforts by many parties, the fraction of female students taking A-level Physics has flat-lined at 20% for over a decade. This is the reason why the proportion of female physics students at university is the same, i.e. 20%. In short, the problem lies within our school system.

The second line of argument is that A-level Physics is not a useful preparation for a Physics degree because it does not develop the sort of problem-solving skills or the ability to express physical concepts in mathematical language on which university physics depends. Most physics admissions tutors that I know care much more about the performance of students at A-level Mathematics than Physics.

Hitherto, most of the effort that has been expended on the first problem has been directed at persuading more girls to do Physics A-level. Since all universities require a Physics A-level for entry into a degree programme, this makes sense but it has not been successful.

I now believe that the only practical way to improve the gender balance on university physics course is to drop the requirement that applicants have A-level Physics entirely and only insist on Mathematics (which has a much more even gender mix). I do not believe that this would require many changes to course content but I do believe it would circumvent the barriers that our current school system places in the way of aspiring female physicists.

Not all UK universities seem very interested in widening participation, but those that are should seriously consider this approach.

The Russell Groupies

Posted in Education, Politics with tags , , , on November 29, 2013 by telescoper

There’s an interesting article in Research Professional upon which I thought a brief comment would be appropriate. The article is mainly about the recent demise of the 1994 Group of universities, made inevitable when some of its larger members jumped ship to climb on board the much posher Russell Group. I’ve always felt that mission groups of this type were of little interest or value, but the growth of the Russell Group has, in my view, become rather sinister because it involves a cynical attempt to manufacture status when none is justified by performance.

The piece in Research Professional says:

Vice-chancellors and principals are not the only ones playing the status game. Students, employers, academics and government ministers—who seem to love visiting Russell Group universities—all want to be associated with high-status universities, even if those institutions do not necessarily provide better education or research. A 2009 analysis of the results of the 2008 Research Assessment Exercise, carried out by the Higher Education Policy Institute, found that Russell Group institutions performed only half a percentage point better than the overall average, and that when universities in the golden triangle were excluded the score fell to below average. Truly, this is an emperor with very modest clothes.

This echoes my experience. Before moving to the University of Sussex earlier this year I worked in two Russell Group universities (and one which wasn’t in the Russell Group when I worked there but is now). All these institutions have much to recommend them – and I have no desire whatsoever to say negative things about former colleagues – but it is clear to me that they (or at least their Physics Departments) can’t claim to be any better than the one in which I currently work. Indeed the Physics department that performed best in the 2008 Research Assessment Exercise was Lancaster, which is also not in the Russell Group.

It’s also noticeable that the primary characteristic of Russell Group universities in the National Student Survey tables is that they generally do quite poorly relative to non-members. Does Russell Group status mean promoting research at the expense of teaching and the student experience generally?

There’s no doubt that by many metrics there is a group of “elite” English universities – Oxford, Cambridge, UCL, and Imperial. The Russell group comprises these and a few other excellent institutions. But the later additions are simply a group of fairly average universities who thought the £500,000 joining fee was worth paying to try to convince students and others that they had elite status too. Worryingly, it seems that the Russel Brand Group Group Brand has been marketed so effectively that politicians are starting to talk as if “research intensive” and “Russell Group” mean one and the same thing.

Six (very) bad things about the REF

Posted in Education, Science Politics with tags , , , , on November 22, 2013 by telescoper

I see that Jon Butterworth has written a piece on the Grauniad website, entitled Six good things about the REF, the REF in question not being a black-clad figure of questionable parentage and visual acuity responsible for supervising a game of association football, but the Research Excellence Framework.

I agree with some of Jon’s comments and do believe that past Research Assessment Exercises have generally raised the quality of research in UK universities. I do however think that there are some very bad things about the way the REF is being implemented, and that these far outweigh the positives Jon mentions. In the interest of balance, therefore, I thought I’d respond with a list of six (very) bad things about the REF, and particularly how it applies to physics. I’ll keep them brief because I’ve blogged about most of them before:

  1. The rules positively encouraged universities to play games with selectivity. This is absurd. All academic staff on teaching and research contracts should be submitted if a true indication of research quality is to be obtained.
  2. The criteria for what constitutes 3* or 4* publications are vague and subjective, leaving everything in the hands of the panels. Worse, all paperwork will be shredded after the panel’s deliberations leaving no possibility for appeal. This absolutely stinks.
  3. How QR funding will be allocated on the basis of the REF is not made clear in advance of the submission. Nobody knows how heavily the funding will be skewed towards 4* and 3* submissions. Having encouraged departments to play games, therefore, the REF refuses to disclose the rules. It’s not even clear there will be any QR funding.
  4. The panels will be unable to perform a detailed peer review of submissions simply because there will be too many papers. Each panel will be expected to make decisions on many hundreds of papers, leaving time only for a cursory reading of each.
  5. Limiting the physics submission to 4 papers per person is ridiculous. This corresponds to a tiny fraction of the outputs of a typical physics researcher. If someone has written ten 4* publications in the REF period, why should these not be counted?
  6. Impact counts for a sizable fraction (20%) of the funding, but the rules governing what counts as “impact” are absurdly restrictive and clearly encourage short-term commercially-oriented boilerplate stuff at the expense of genuine long-term “blue skies” research.

 

Well, I got to six in just a few minutes and could easily get to sixty, but that will do for now. Perhaps you’d like to contribute your own bad things through the comments box?