Archive for Physics

Perception, Piero and Pollock

Posted in Art, The Universe and Stuff with tags , , , , , on April 15, 2009 by telescoper

For some unknown reason I’ve just received an invitation to a private view at a small art gallery that’s about ten minutes’ walk from my house. Cocktails included. I shall definitely go and will blog about it next week. I’m looking forward to it already.

This invitation put me in an artistic frame of mind so, to follow up my post on randomness (and the corresponding parallel version on cosmic variance), I thought I’d develop some thoughts about the nature of perception and the perception of nature.

This famous painting is The Flagellation of Christ, by Piero della Francesca. I actually saw it many years ago on one of my many trips to Italy; it’s in an art gallery in Urbino. The first thing that strikes you when you see it is actually that the painting is surprisingly small (about 60cm by 80cm). However, that superficial reaction aside, the painting draws you into it in a way which few other works of art can. The composition is complicated and mathematically precise, but the use of linear perspective is sufficiently straightforward that your eye can quickly understand the geometry of the space depicted and locate the figures and actions within it. The Christ figure is clearly in the room to the left rear and the scene is then easily recognized as part of the story leading up to the crucifixion.

That’s what your eye always seems to do first when presented with a figurative representation: sort out what’s going on and fill in any details it can from memory and other knowledge.

But once you have made sense of the overall form, your brain immediately bombards you with questions. Who are the three characters in the right foreground? Why aren’t they paying attention to what’s going on indoors? Who is the figure with his back to us? Why is the principal subject so far in the background? Why does everyone look so detached? Why is the light coming from two different directions (from the left for the three men in the foreground but from the right for those in the interior)? Why is it all staged in such a peculiar way? And so on.

These unresolved questions lead you to question whether this is the straightforward depiction first sight led you to think it was. It’s clearly much more than that. Deeply symbolic, even cryptic, it’s effect on the viewer is eery and disconcerting. It has a dream-like quality. The individual elements of the painting add up to something, but the full meaning remains elusive. You feel there must be something you’re missing, but can’t find it.

This is such an enigmatic picture that it has sparked some extremely controversial interpretations, some of which are described in an article in the scientific journal Nature. I’m not going to pretend to know enough to comment on the theories, escept to say that some of them at least must be wrong. They are, however, natural consequences of our brain’s need to impose order on what it sees. The greatest artists know this, of course. Although it sometimes seems like they might be playing tricks on us just for fun, part of what makes art great is the way it gets inside the process of perception.

Here’s another example from quite a different artist.

This one is called Lavender Mist. It’s one of the “action paintings” made by the influential American artist Jackson Pollock. This, and many of the other paintings of its type, also get inside your head in quite a disconcerting way but it’s quite a different effect to that achieved by Piero della Francesca.

This is an abstract painting, but that doesn’t stop your eyes seeking within it some sort of point of reference to make geometrical sense of it. There’s no perspective to draw you into it so you look for clues to the depth in the layers of paint. Standing in front of one of these very large works – I find they don’t work at all in reduced form like on the screen in front of you now – you find your eyes constantly shifting around, following lines here and there, trying to find recognizable shapes and to understand what is there in terms of other things you have experienced either in the painting itself or elsewhere. Any order you can find, however, soon becomes lost. Small-scale patterns dissolve away into sea of apparent confusion. Your brain tries harder, but is doomed. One of the biggest problems is that your eyes keep focussing and unfocussing to look for depth and structure. It’s almost impossible to stop yourself doing it. You end up dizzy.

I don’t know how Pollock came to understand exactly how to make his compositions maximally disorienting, but he seems to have done so. Perhaps he had a deep instinctive understanding of how the eye copes with the interaction of structures on different physical scales. I find you can see this to some extent even in the small version of the picture on this page. Deliberately blurring your vision makes different elements stand out and then retreat, particularly the large darkish streak that lies to the left of centre at a slight angle to the vertical.

This artist has also been the subject of interest by mathematicians and physicists because his work seems to display some of the characteristic properties of fractal sets. I remember going to a very interesting talk a few years ago by Richard Taylor of the University of Oregon who claimed that fractal dimensions could be used to authenticate (or otherwise) genuine works by Pollock as he seemed to have his own unique signature.

I suppose what I’m trying to suggest is that there’s a deeper connection than you might think between the appreciation of art and the quest for scientific understanding.

Arrows and Demons

Posted in The Universe and Stuff with tags , , , , , on April 12, 2009 by telescoper

My recent post about randomness and non-randomness spawned a lot of comments over on cosmic variance about the nature of entropy. I thought I’d add a bit about that topic here, mainly because I don’t really agree with most of what is written in textbooks on this subject.

The connection between thermodynamics (which deals with macroscopic quantities) and statistical mechanics (which explains these in terms of microscopic behaviour) is a fascinating but troublesome area.  James Clerk Maxwell (right) did much to establish the microscopic meaning of the first law of thermodynamics he never tried develop the second law from the same standpoint. Those that did were faced with a conundrum.  

 

The behaviour of a system of interacting particles, such as the particles of a gas, can be expressed in terms of a Hamiltonian H which is constructed from the positions and momenta of its constituent particles. The resulting equations of motion are quite complicated because every particle, in principle, interacts with all the others. They do, however, possess an simple yet important property. Everything is reversible, in the sense that the equations of motion remain the same if one changes the direction of time and changes the direction of motion for all the particles. Consequently, one cannot tell whether a movie of atomic motions is being played forwards or backwards.

This means that the Gibbs entropy is actually a constant of the motion: it neither increases nor decreases during Hamiltonian evolution.

But what about the second law of thermodynamics? This tells us that the entropy of a system tends to increase. Our everyday experience tells us this too: we know that physical systems tend to evolve towards states of increased disorder. Heat never passes from a cold body to a hot one. Pour milk into coffee and everything rapidly mixes. How can this directionality in thermodynamics be reconciled with the completely reversible character of microscopic physics?

The answer to this puzzle is surprisingly simple, as long as you use a sensible interpretation of entropy that arises from the idea that its probabilistic nature represents not randomness (whatever that means) but incompleteness of information. I’m talking, of course, about the Bayesian view of probability.

 First you need to recognize that experimental measurements do not involve describing every individual atomic property (the “microstates” of the system), but large-scale average things like pressure and temperature (these are the “macrostates”). Appropriate macroscopic quantities are chosen by us as useful things to use because they allow us to describe the results of experiments and measurements in a  robust and repeatable way. By definition, however, they involve a substantial coarse-graining of our description of the system.

Suppose we perform an idealized experiment that starts from some initial macrostate. In general this will generally be consistent with a number – probably a very large number – of initial microstates. As the experiment continues the system evolves along a Hamiltonian path so that the initial microstate will evolve into a definite final microstate. This is perfectly symmetrical and reversible. But the point is that we can never have enough information to predict exactly where in the final phase space the system will end up because we haven’t specified all the details of which initial microstate we were in.  Determinism does not in itself allow predictability; you need information too.

If we choose macro-variables so that our experiments are reproducible it is inevitable that the set of microstates consistent with the final macrostate will usually be larger than the set of microstates consistent with the initial macrostate, at least  in any realistic system. Our lack of knowledge means that the probability distribution of the final state is smeared out over a larger phase space volume at the end than at the start. The entropy thus increases, not because of anything happening at the microscopic level but because our definition of macrovariables requires it.

ham

This is illustrated in the Figure. Each individual microstate in the initial collection evolves into one state in the final collection: the narrow arrows represent Hamiltonian evolution.

 

However, given only a finite amount of information about the initial state these trajectories can’t be as well defined as this. This requires the set of final microstates has to acquire a  sort of “buffer zone” around the strictly Hamiltonian core;  this is the only way to ensure that measurements on such systems will be reproducible.

The “theoretical” Gibbs entropy remains exactly constant during this kind of evolution, and it is precisely this property that requires the experimental entropy to increase. There is no microscopic explanation of the second law. It arises from our attempt to shoe-horn microscopic behaviour into framework furnished by macroscopic experiments.

Another, perhaps even more compelling demonstration of the so-called subjective nature of probability (and hence entropy) is furnished by Maxwell’s demon. This little imp first made its appearance in 1867 or thereabouts and subsequently led a very colourful and influential life. The idea is extremely simple: imagine we have a box divided into two partitions, A and B. The wall dividing the two sections contains a tiny door which can be opened and closed by a “demon” – a microscopic being “whose faculties are so sharpened that he can follow every molecule in its course”. The demon wishes to play havoc with the second law of thermodynamics so he looks out for particularly fast moving molecules in partition A and opens the door to allow them (and only them) to pass into partition B. He does the opposite thing with partition B, looking out for particularly sluggish molecules and opening the door to let them into partition A when they approach.

The net result of the demon’s work is that the fast-moving particles from A are preferentially moved into B and the slower particles from B are gradually moved into A. The net result is that the average kinetic energy of A molecules steadily decreases while that of B molecules increases. In effect, heat is transferred from a cold body to a hot body, something that is forbidden by the second law.

All this talk of demons probably makes this sound rather frivolous, but it is a serious paradox that puzzled many great minds. Until it was resolved in 1929 by Leo Szilard. He showed that the second law of thermodynamics would not actually be violated if entropy of the entire system (i.e. box + demon) increased by an amount every time the demon measured the speed of a molecule so he could decide whether to let it out from one side of the box into the other. This amount of entropy is precisely enough to balance the apparent decrease in entropy caused by the gradual migration of fast molecules from A into B. This illustrates very clearly that there is a real connection between the demon’s state of knowledge and the physical entropy of the system.

By now it should be clear why there is some sense of the word subjective that does apply to entropy. It is not subjective in the sense that anyone can choose entropy to mean whatever they like, but it is subjective in the sense that it is something to do with the way we manage our knowledge about nature rather than about nature itself. I know from experience, however, that many physicists feel very uncomfortable about the idea that entropy might be subjective even in this sense.

On the other hand, I feel completely comfortable about the notion:. I even think it’s obvious. To see why, consider the example I gave above about pouring milk into coffee. We are all used to the idea that the nice swirly pattern you get when you first pour the milk in is a state of relatively low entropy. The parts of the phase space of the coffee + milk system that contain such nice separations of black and white are few and far between. It’s much more likely that the system will end up as a “mixed” state. But then how well mixed the coffee is depends on your ability to resolve the size of the milk droplets. An observer with good eyesight would see less mixing than one with poor eyesight. And an observer who couldn’t perceive the difference between milk and coffee would see perfect mixing. In this case entropy, like beauty, is definitely in the eye of the beholder.

The refusal of many physicists to accept the subjective nature of entropy arises, as do so many misconceptions in physics, from the wrong view of probability.

Easter Physics Quiz

Posted in Uncategorized with tags on April 10, 2009 by telescoper

Over the Easter holidays the newspapers seem to be full of quizzes and other distractions, so I thought I’d join in with a little quiz of my own.

So for a negligible prize can anyone point out the mathematical connection between these two pictures?

 

 

 

 

 

 

 

Answers via the comments box please.

Post Mortem

Posted in Science Politics with tags , , , , on April 6, 2009 by telescoper

Finally the full details of the Physics panel’s deliberations during the 2008 Research Assessment Exercise have been published in the form of sub-profiles, showing the breakdown of the overall scores into various components, including the rating attached to “outputs” (i.e. papers), “environment” and “esteem”; for the jargon see the RAE guidelines for submissions.

 I’ve blogged about the RAE results before: here, there, elsewhere, et cetera and passim. Andy Lawrence (e-astronomer) has now written a blog post about the latest publications from HEFCE  (commenting on the Cardiff situation with a generosity that contrasts with the offensive attitude displayed by one of my former colleagues).  Andy has also produced a graph which makes for very interesting reading:

rae_21

I’ve used my meagre graphical skills to indicate the location of Cardiff on the figure between the thick solid lines. Note the enormous gap between the panel’s assessment of our outputs (2.22) compared to the score for esteem (2.74).

I’ve mentioned before that apparently not a single one of the papers submitted by Cardiff’s excellent Astronomy Instrumentation Group was graded as 4* (world leading). Among the papers submitted by this group were several highly cited ones relating to an important Cosmic Microwave Background experiment called BOOMERANG. The panel probably judged that Cardiff hadn’t played a sufficiently prominent role in this collaboration to merit a 4*, which seems to be a completely perverse conclusion. The experiment wouldn’t have been possible at all without the Cardiff group.

Notwithstanding my disgruntlement at the particularly and peculiarly harsh assessment of Cardiff’s physics submission, there is also an indication of a more general problem. Notice how at the top right, a large number of departments has an output score seriously lagging their other score (by about 0.4 or more).

The counterexample to this trend is Loughborough, which has a very small but clearly good research activity in physics, and which scored 2.66 on its outputs but only 1.1 on environment. They are easily identified on the graph as an extreme outlier below the general trend.

Although there is no reason to expect a perfect correlation between the different elements of the overall assessment, it looks to me like the Physics panel decided to let the output score for the strong departments saturate at a level of about 2.8 whereas other panels were much more generous.

Why did they do this?

Answers on a postcard (or, better, via the comments box), please.

Clover and Out

Posted in Science Politics, The Universe and Stuff with tags , , , , , , , , , on March 31, 2009 by telescoper

One of the most exciting challenges facing the current generation of cosmologists is to locate in the pattern of fluctuations in the cosmic microwave background evidence for the primordial gravitational waves predicted by models of the Universe that involve inflation.

Looking only at the temperature variation across the sky, it is not possible to distinguish between tensor  (gravitational wave) and scalar (density wave) contributions  (both of which are predicted to be excited during the inflationary epoch).  However, scattering of photons off electrons is expected to leave the radiation slightly polarized (at the level of a few percent). This gives us additional information in the form of the  polarization angle at each point on the sky and this extra clue should, in principle, enable us to disentangle the tensor and scalar components.

The polarization signal can be decomposed into two basic types depending on whether the pattern has  odd or even parity, as shown in the nice diagram (from a paper by James Bartlett)

The top row shows the E-mode (which look the same when reflected in a mirror and can be produced by either scalar or tensor modes) and the bottom shows the B-mode (which have a definite handedness that changes when mirror-reflected and which can’t be generated by scalar modes because they can’t have odd parity).

The B-mode is therefore (in principle)  a clean diagnostic of the presence of gravitational waves in the early Universe. Unfortunately, however, the B-mode is predicted to be very small, about 100 times smaller than the E-mode, and foreground contamination is likely to be a very serious issue for any experiment trying to detect it.

An experiment called Clover (involving the Universities of  Cardiff, Oxford, Cambridge and Manchester) was designed to detect the primordial B-mode signal from its vantage point in Chile. You can read more about the way it works at the dedicated webpages here at Cardiff and at Oxford. I won’t describe it in more detail here, for reasons which will become obvious.

The chance to get involved in a high-profile cosmological experiment was one of the reasons I moved to Cardiff a couple of years ago, and I was looking forward to seeing the data arriving for analysis. Although I’m primarily a theorist, I have some experience in advanced statistical methods that might have been useful in analysing the output.  It would have been fun blogging about it too.

Unfortunately, however, none of that is ever going to happen. Because of its budget crisis, and despite the fact that it has spent a large amount (£4.5M) on it already,  STFC has just decided to withdraw the funding needed to complete it (£2.5M)  and cancel the Clover experiment.

Clover wasn’t the only B-mode experiment in the game. Its rivals include QUIET and SPIDER, both based in the States. It wasn’t clear that Clover would have won the race, but now that we know  it’s a non-runner  we can be sure it won’t.

Honoured amongst bloggers…

Posted in Uncategorized with tags , , , on March 25, 2009 by telescoper

I only have time for a quickie today as I have to spend this evening getting things together for my forthcoming trip to the Irish Republic for a talk in Dublin (which I’ll no doubt ramble on about when I get back).

I hear dark rumblings about the STFC financial crisis turning into a full-scale disaster owing to inept management, but I’ll refrain from going into details until it all becomes official. Suffice to say for now that, if you thought things were bad already, just watch this space…

Anyway, at least today brought some news that flattered my ego. Ian Douglas at the Daily Telegraph has seen fit to put this blog on his list of five great physics blogs. He’s obviously a man of great taste. Quite cute too. I’ll have to revise my opinion of the Daily Telegraph.

But no.

They have boring crosswords.

Late Arrivals at the Physics Ball

Posted in The Universe and Stuff, Uncategorized with tags , , on March 13, 2009 by telescoper

Today is the day we have to endure Comic Relief, an event which happens mercifully only once a year. The idea is to raise money for charity by doing something funny. If only.

I’ve also recently been persuaded to part with £30 to buy a ticket for the annual Physics Ball, organized by Chaos (Cardiff University Physics student-staff society). In the light of this I thought I’d add yet another item of debatable comic value to Comic Relief. My old friend Bryn Jones and I have been taking a leaf out of the I’m Sorry I Haven’t a Clue book of appalling puns.

Without further ado, therefore, it gives us great pleasure to announce the late arrivals at the Physics Ball:

Mr. and Mrs. Sirquashens and their son Maxwell
Mr and Mrs Rowave and their son Mike
Mr and Mrs Ofmotion and their daughter Constance
Mr and Mrs Destate and their son Solly
And from Ireland, Mr and Mrs O’genesis and their son Barry who has brought his two pet newts (Ron and Reno).
Mr and Mrs Yabatick and their daughter Ada.
Mr and Mrs Dardtemperatureandpressure and their son, Stan.
Mr and Mrs Hertz and their son Terry.
Mr and Mrs Avolt and their energetic daughter Meg
Mr and Mrs Persymmetry and their daughter Sue
Mr and Mrs Mentum and their daughter Mo.
Mr and Mrs Sticity and their daughter Ella.
Mr and Mrs Ryovrelativity and their son, Theo, who has a successful career in the military, yes it’s General Theo Ryovrelativity. He’s brought a couple of friends too: Chris Toffle-Cymbals and Joe Desick. Oh, and have you met Rick Tensor?

Here’s Mr and Mrs Zeinstein-Condensate with their son Bo.
Mr and Mrs Gular-velocity and their daughter Anne.
And now we have Mr. and Mrs. Ihilation and their destructive daughter Ann.
Here are Mr. and Mrs. Barr and their highly pressured daughter Millie.

Mr. and Mrs. Farparticull with their son Al.
Mr. and Mrs. Diantflucks and their bright son Ray.
And the coach party has arrived from Ireland with Mr. and Mrs. O’Moshun and their important son Newt Onslow.
Mr. and Mrs. O’Lissforss and their daughter rotating daughter Kerry.
From the Institute of Electrical Engineers we have Mr. and Mrs. Arrsirkitt and their pulsating daughter Elsie.
We now have Mr. and Mrs. Rectcurrant and their son Dai.
Mr and Mrs Hair-Theorem and their son Noah.
Mr and Mrs Mix and their daughter Dinah
Mr and Mrs Clotron and their son Si
Mr and Mrs Yaolis and, doing her best to circulate, their daughter Cora
Mr and Mrs Daze-Lore and their Daughter Farrah
From the Ruritanian principality of Energee we have Prince Ippilocon-Servashun of Energee.
Mr. and Mrs. Jeenslaw and their far-from-energetic son Ray Lee.
Mr. and Mrs. Minnusflucks and their bright son Lou.
Mr. and Mrs. Litonian and their dynamic son Hammy.
Mr. and Mrs. Shuoffheet-Capassitees and their son Ray.
And more arrivals from Ireland: Mr. O’Savar-Law and his attractive wife Bea.
Mr. and Mrs. O’Watt and their powerful daughter Meg.
Mr. and Mrs. O’Particull and their petite daughter Nan
Mr and Mrs Ear-accelerator and their daughter Lynne

And although I don’t think they were invited here are Mr and Mrs Osoficklenonsense and their son Phil along with Mr and Mrs Logicaldistraction and their son Theo.

And a definitely unwelcome are Mr and Mrs Thropic-principle and their daughter Anne

Sorry you can’t come in wearing those jeans. You might not like it, but we do have a Jeans criterion.

Mr and Mrs Ittifluctuation and their son Dennis
Mr and Mrs Punovexponent and their rather chaotic daughter, Leah
Mr and Mrs Stransition and their daughter Fay
Mr and Mrs Trope with their children Polly and Barry.
And we now welcome Mr. and Mrs. Way-Veckwashunn and their canny daughter Inga; that’s the shrewd Inga Way-Veckwashunn.
Mr. and Mrs. Broywavelength and their daughter Deb.
Please welcome Mr. and Mrs. Noldsnumber and their turbulent son Ray.

And now it’s Cabaret time!

First we’ve got sensational pop in the form of singer Larry Tee, followed by a quick burst of Pump up the Volume, folllowed by Norwegian artist Lars Kattering, then chillout with the smooth background sounds of The Three Degrees and ending up with a number of fading stars performing Back to Black.

For those of you wanting something more traditional, we’ve got folk music by The Spinors.

Mr. and Mrs. Helmholtz-Instability and their unstable son Kelvin.
Mr. and Mrs. Tensor and their son Richie
From Wales, Mr and Mrs Menshanalanalissis and their son Dai
Mr and Mrs Eyelength and their daughter Deb Eyelength
Mr and Mrs Notanotherloadofbolloxaboutstringtheory and their son Gordon Bennett Notanotherloadofbolloxaboutstringtheory
Mr and Mrs Dingo-Flyte and their son Ben
From Norway, Mr and Mrs Tableorbit and their son Lars
Mr and Mrs Sonscattering and their son Tom.
Mr. Skelleration and his rapidly moving wife Constance.
Mr. and Mrs. Vennspeed and their son Alf.
And the Welsh electrician, Dai Electric.
From Germany we have Herr Diffraction and his wife Frau Enhofer Diffraction.
Mr. and Mrs. Offslaw and their electrical engineer son Kirk.
Mrs and Mrs Ginvariance and their daughter Gay
Mr and Mrs Terry-Matrix and their daughter Una
And here is Solly, the only member of the Ton family who could make it, but then he always comes on his own
Mr and Mrs On and their daughter Kay and son Barry
Mr and Mrs Roscopic-quantity and their son Mac.
Mr. and Mrs. Moment and their bipolar son Dai Paul.
Mr. and Mrs. Covraydiashonn and their glowing daughter Cherry Ann.
Mr. and Mrs. Arisation and their son Paul.
Mr. and Mrs. Onsprinkippiah and their very important son Newt.
Mr. and Mrs. Cannsoyldropp-Experryment and their very practical daughter Millie.
Mr. and Mrs. Sonnmorlie-Experryment, and here comes their son Michael with no positive result.
Mr. Menterryparticalls and his fundamentally important wife Ellie.
Mr. and Mrs. Swelldeemon and their problematic son Max.
Mr. and Mrs. Defect and their slightly spolit daughter Crystal.
Mr. Formmotion and his constant wife Una.
And here are the Tonn children with their father Newt, and their father’s unmarried sister Prue – that’s Auntie Prue Tonn.
The coach party has arrived from Wales, with Mr. and Mrs. Nammicks and their fast-moving son Dai.
Mr. and Mrs. Vergance-Theorem and their son Dai.
Mr. and Mrs. Oolie-Ekwayshonn and their son Bernie.
From America, Mr and Mrs Chure and their spaced-out son Cosmic Tex Chure
Mr and Mrs Wurld and their son Brian
Mr and Mrs Theory and their Daughter Emma
and here are the Structive-interference family, with brother and sister Des and Connie
Mr and Mrs Medes-Principle with their son Archie
Mr and Mrs Fishalsatellites and their son Artie
In a bit of a whirl here’s Mr and Mrs Currants and their son Eddy

From Germany, Mr and Mrs Duranium and their son Heinrich
Mr and Mrs Photon and their son Virgil
Mr and Mrs Velocity and their typical son Aramis
Mr and Mrs Gadrowsnumber and their daughter Ava
Mr and Mrs Experryment and their son Jules
Mr and Mrs Psimeson and their son Jay
Mr and Mrs Dington-Limit and their son Ed.
Mr. and Mrs. Eslaw and their son Charles.

From the Institution of Electrical Engineers we have Mr. and Mrs. Acksialcabell and their shielded son Carl.
We are pleased to receive Mr. Tennar and his wife Ann.
And from the Science and Technology Facilities Council we have their chief accountants, Mrs. Nanshall-Dissastar and Mr. Jettery-Kayoss: that’s Fi Nanshall-Dissastar and Bud Jettery-Kayoss.

Mr. Motiff-Forss and his magnetic wife Elektra.
Here from the left come Mr. and Mrs. Saslaw and their charged son Guy, and in the opposite direction their son Len.
Mr. and Mrs. Annicall-Annerjee and their son Mike.
Mr. and Mrs. Tamass and their son Rhys.
Mr. and Mrs. Statickpotenshall and their daughter Elektra.
Mr. Jenner-Ait-Annerjee-Levell and his wife Dee.
Mr. and Mrs. Mental-Constance and their humorous, light-hearted son Dai. That’s fun Dai Mental-Constance

Feel free to add more via the comments if you get the idea! The more excruciating the better…

Doctor Atomic

Posted in Opera with tags , , , , on March 1, 2009 by telescoper

It’s not often that my interest in Opera overlaps significantly with my career in Physics, but this Saturday night (28th March) was a definite example, with English National Opera‘s production of Doctor Atomic by John Adams providing the opportunity. I even went with a group of six physicists to see it.

The piece is, of course, centred around the personality of J Robert Oppenheimer “The Father of the Atomic Bomb” and is set in Los Alamos in the runup to the first “Trinity” test detonation of an atomic bomb in July 1945. Other physicists feature in the story, especially Edward Teller and Robert Wilson, and images of many more taken from their security passes are projected onto the set at the opening of Scene 1.

According to what I was told, John Adams originally engaged a librettist to write the text for the Opera but this didn’t work out, and a libretto was instead stitched together by Peter Sellars from a variety of sources, including the poetry of John Donne, the Bhagavad Gita, scientific documents, and assorted memoranda from Los Alamos.

This means that the work doesn’t really have a real narrative trajectory, and there is very little in the way of character development, but instead it resolves itself into a series of impressionist tableaux. Rather than attempting to provide the coherence that the libretto lacks through the music, Adams chose to work with what he had and not try to impose a larger structure on it via the score.

The result is fascinating but it’s not without its problems. I greatly admire John Adams’ music, which manages to be both innovative and accessible. There certainly are many places in Doctor Atomic where the music, words and drama come together to make wonderful Opera. Frankly, though, there are also some passages where it gets becalmed, especially in the domestic scenes between Oppenheimer and his wife which didn’t seem to me to add any special insight into the character of either. The Opera ends with the countdown to the detonation of the Trinity Test, but I thought this was also too long, robbing the event of some of its power, although the last moments and the explosion itself were brilliantly done.

This is a new Opera, first performed as recently as 2005 in San Francisco. This production is only the second, as it has moved directly to London from a successful run at the Metropolitan Opera in New York. Many of the great operas which we now regard as standards went through several iterations before they arrived at their final version. This may happen to Doctor Atomic too. The running time of around three hours is by no means excessive by opera standards, but I do think it would work even better on stage if it were shortened quite a bit and tightened up to remove the longueurs from both acts and focus on building the tension as the test approaches.

I hope all this doesn’t sound too negative. It really is a fascinating and compelling piece. The ending, involving an empty stage and a tape recording of the words of a dying Japanese woman asking for water, moved at least one of our little group to tears.

And of course there’s that aria. At the end of Act 1, just before the interval, Oppenheimer is alone on stage while the prototype bomb is suspended behind him. His thoughts are expressed by the words of a Sonnet Batter my Heart, by John Donne:

Batter my heart, three-person’d God, for you
As yet but knock, breathe, shine, and seek to mend;
That I may rise and stand, o’erthrow me, and bend
Your force to break, blow, burn, and make me new.
I, like an usurp’d town to’another due,
Labor to’admit you, but oh, to no end;
Reason, your viceroy in me, me should defend,
But is captiv’d, and proves weak or untrue.
Yet dearly’I love you, and would be lov’d fain,
But am betroth’d unto your enemy;
Divorce me,’untie or break that knot again,
Take me to you, imprison me, for I,
Except you’enthrall me, never shall be free,
Nor ever chaste, except you ravish me.

Coming back to Cardiff on the train this morning I read a glowing review of Doctor Atomic in the Observer by Fiona Maddocks which referred to this aria as the greatest written since Puccini. I’m not sure I’d go as far as that, but it is truly wonderful, especially when sung as it was last night by the flawless Gerald Finley. It also struck me that it has many parallels with, and is as at least as good as, the aria When the Great Bear and Pleiades in Peter Grimes by Benjamin Britten. Whether Doctor Atomic eventually comes to be regarded as a great Opera in the way Peter Grimes has remains to be seen, but I would bet my bottom dollar that this aria will anyway be performed many many times as a concert piece.

Fortunately, though, you don’t have to take my word for how good  it is. Since the Met version of this production has been released on video, I can end with Batter my Heart just as we saw and heard it last night, with John Adams great music stuttering uneasily at the start but taking on a radiant quality as the aria develops. Superb.

Executive Roast

Posted in Science Politics with tags , , , on February 6, 2009 by telescoper

The Chief Executive of the Science and Technology Facilities Council (Keith Mason) was recently summoned to the House of Commons Select Committee on Innovation, Universities and Skills. The video of his inquisition is now available for your enjoyment (but not his) here.

(I tried embedding this using vodpod but it didn’t work, so you’ll just have to click the link…)

Notice how in traditional fashion the light was shining in his eyes throughout. I suppose I should really feel sorry for him, but somehow I don’t. He may not be entirely responsible for the budgetary crisis currently engulfing STFC, but he handled the aftermath so badly that the damage done to relations between STFC and the community of physics researchers that rely on it for funding will take a long time to fix.

Anyway, if you can’t be bothered to watch the whole show here are some of the salient points in a summary that was passed to me by an anonymous source; I was too busy laughing to make my own notes, but I’ve added a few comments in italics. For those of you not up with acronyms, DIUS is the Department for Innovation, Universities and Skills and CSR stands for the Comprehensive Spending Review.

KM insisted that STFC had been successful in giving the UK unprecedented opportunities for doing world class science, and by the end (though by that stage his most aggressive interlocutor, Ian Gibson, had left) appeared to have earned the committee’s grudging respect (though I suspect that was for the way he played a tricky wicket as much as because he had persuaded them out of their deep concerns about his management of the STFC)

Among the many issues raised were the following:

  • KM agreed to hand over the letter detailing the Science and Technology Facilities Council’s 2007 spending review allocation to MPs for scrutiny.
  • He denied that the external review of STFC had been a “total
    whitewash” on the grounds that it had not been given sufficient time to thoroughly interview a cross section of staff during the review or to do other than take the STFC’s self-assessment document, upon which their work was based, at “face value” without being able to find out if the majority of STFC staff actually agreed with its content. On the contrary staff had made their views known ‘vociferously’.
  • Challenged about the perceived overrepresentation of the executive council on the STFC council KM said that, while it had affected the perception held in the community, it made “no difference” to the outcomes (a point which the committee repeatedly contested). He added that STFC takes full account of community input via the advisory panels and science board. It’s simply not true, he insisted, that the executive dominates the Council;  rather it ensures it is properly informed so that decisions are well founded. However he acknowledged that communications had not been good – hence the new arrangements (Director of Communications appointment); Great, another spin doctor – PC .
  • An extra GBP 9M had been freed up by DIUS reducing STFC’s liabilities to exchange rate variations from the first 6 to 3 m pa over the triennium. Of this 6 would go to exploitation grants and 3 to HEIs to promote knowledge transfer. So 6M will be used properly and the rest wasted – PC .
  • He stated that Jodrell Bank had no long term future in radio astronomy since its location exposed it to too much ‘noise’ – but that was for Manchester University (which STFC would continue to support via E-MERLIN and SKA) to determine. It will take a silver bullet to kill that particular zombie -PC
  • KM also voiced the opinion that here was no tension between being simultaneously responsible for developing STFC labs/campuses and funding HEIs through grants; on the contrary it enabled better utilisation of resources bearing in mind the role of STFC which is BOTH to promote science AND its societal /economic benefits. In other words he wants the flexibility to continue robbing Peter to pay Paul – PC
  • For this reason (as well as reasons of administrative complexity)
    STFC had rejected Wakeham’s recommendation to ring fence the ex-PPARC budget line in the forthcoming CSR. Ditto
  • KM argued that  Daresbury was not being treated unfairly in relation to Harwell (there was a good deal of probing about this by North West MPs) .

My own view having watched most of the video is that Professor Mason must have an incredibly thick skin to shrug off such a sustained level of antipathy. Some of it is crude and abusive, but it’s quite impressive how well informed some of the members are.

Physics Funding by Numbers

Posted in Science Politics with tags , , , , , on January 29, 2009 by telescoper

I just read today that HEFCE has decided on the way funds will be allocated for research following the 2008 Research Assessment Exercise. I have blogged about this previously (here, there and elsewhere), but to give you a quick reminder the exercise basically graded all research in UK universities on a scale from 4* (world-leading) to 1* (nationally recognized), producing for each department a profile giving the fraction of research in each category.

HEFCE has decided that English universities will be funded according to a formula that includes everything from 2* up to 4* but with a weighting 1:3:7.  Those graded 1* and unclassified get no funding at all. How they arrived at this formula is anyone’s guess. Personally I think it’s a bit harsh on 2* which is supposed to be internationally recognized research, but there you go.

Assuming there is also a multiplier for volume (i.e. the number of people submitted) we can now easily produce another version of the physics research league table which reveals the relative amount of money each will get. I don’t know the overall normalisation, of course.

The table shows the number of staff submitted (second column) and the overall fundability factor based on a 7:3:1 weighting of the published profile multiplied by the figure in column 2. This is like the “research power” table I showed here, only with a different and much steeper weighting (7,3,1,0) versus (4,3,2,1).

1. University of Cambridge 141.25 459.1
2. University of Oxford 140.10 392.3
3. Imperial College London 126.80 380.4
4. University College London 101.03 298.0
5. University of Manchester 82.80 227.7
6. University of Durham 69.50 205.0
7. University of Edinburgh 60.50 184.5
8. University of Nottingham 44.45 144.5
9. University of Glasgow 45.75 135.0
10. University of Warwick 51.00 130.1
11. University of Bristol 46.00 128.8
12. University of Birmingham 43.60 126.4
13. University of Southampton 45.30 120.0
14. Queen’s University Belfast 50.00 115.0
15. University of Leicester 45.00 114.8
16. University of St Andrews 32.20 104.7
17. University of Liverpool 34.60 96.9
18. University of Sheffield 31.50 92.9
19. University of Leeds 35.50 88.8
20. Lancaster University 26.40 88.4
21. Queen Mary, University of London 34.98 85.7
22. University of Exeter 28.00 77.0
23. University of Hertfordshire 28.00 72.8
24. University of York 26.00 67.6
25. Royal Holloway, University of London 27.96 67.1
26. University of Surrey 27.20 65.3
27. Cardiff University 32.30 64.6
28. University of Bath 20.20 63.6
29. University of Strathclyde 31.67 60.2
30. University of Sussex 20.00 55.0
31. Heriot-Watt University 19.50 51.7
32. Swansea University 20.75 48.8
33. Loughborough University 17.10 41.9
34. University of Central Lancashire 22.20 41.1
35. King’s College London 16.40 38.5
36. Liverpool John Moores University 16.50 35.5
37. Aberystwyth University 18.33 23.8
38. Keele University 10.00 18.0
39. Armagh Observatory 7.50 13.1
40. University of Kent 3.00 4.5
41. University of the West of Scotland 3.70 4.1
42. University of Brighton 1.00 1.8

It looks to me that the fraction of funds going to the big three at the top will probably be reduced quite significantly, although apparently there are  funds set aside to smooth over any catastrophic changes. I’d hazard a guess that things won’t change much for those in the middle.

I’ve left the Welsh and Scottish universities in the list for comparison, but there is no guarantee that HEFCW and SFC will use the same formula for Wales and Scotland as HEFCE did for England. I have no idea what is going to happen to Cardiff University’s funding at the moment.

Another bit of news worthing putting in here is that HEFCE has protected funding for STEM subjects (Science, Technology and Medicine) so that the apparently poor showing of some science subjects (especially physics) compared to, e.g., Economics will not necessarily mean that physics as a whole will suffer. How this works out in practice remains to be seen.

Apparently also the detailed breakdowns of how the final profiles were reached will go public soon. That will make for some interesting reading, although apparently everything relating to individual researchers will be shredded to prevent problems with the data protection act.