Archive for July, 2011

Villanelle for the News of the World

Posted in Poetry with tags , , , , , on July 8, 2011 by telescoper

Time will say nothing but I told you so,
News International knows the price  to pay;
If I could tell you I would let you know.

If we should weep when Murdoch flaunts his dough,
If we should care what other papers say,
Time will say nothing but I told you so.

There are no fortunes to be told, although,
Because I hate you more than I can say,
If I could tell you I would let you know.

The winds must come from Wapping when they blow,
The Press Commission doesn’t know which way;
Time will say nothing but I told you so.

Perhaps the readers really want it so,
The tabloids seriously intend to stay;
If I could tell you I would let you know.

Suppose the hacks all get up and go,
And all the Brooks and Coulsons run away?
Will time say nothing but I told you so?
If I could tell you I would let you know.

(with apologies to W.H. Auden)

Feynman on Computers

Posted in The Universe and Stuff with tags , on July 8, 2011 by telescoper

This is a special one for all those people who prefer fiddling about with computers to actually doing science with them!

Well, Mr. Frankel, who started this program, began to suffer from the computer disease that anybody who works with computers now knows about. It’s a very serious disease and it interferes completely with the work. The trouble with computers is you *play* with them. They are so wonderful. You have these switches – if it’s an even number you do this, if it’s an odd number you do that – and pretty soon you can do more and more elaborate things if you are clever enough, on one machine.

After a while the whole system broke down. Frankel wasn’t paying any attention; he wasn’t supervising anybody. The system was going very, very slowly – while he was sitting in a room figuring out how to make one tabulator automatically print arc-tangent X, and then it would start and it would print columns and then bitsi, bitsi, bitsi, and calculate the arc-tangent automatically by integrating as it went along and make a whole table in one operation.

Absolutely useless. We *had* tables of arc-tangents. But if you’ve ever worked with computers, you understand the disease – the *delight* in being able to see how much you can do. But he got the disease for the first time, the poor fellow who invented the thing.

Richard Feynman (1918-1988)

JWST: Too Big to Fail?

Posted in Finance, Science Politics, The Universe and Stuff with tags , , , , , on July 7, 2011 by telescoper

News emerged last night that the US Government may be about to cancel the  James Webb Space Telescope, which is intended to be the successor to the Hubble Space Telescope. I’m slow out of the blocks on this one, as I had an early night last night, but there’s already extensive reaction to the JWST crisis around the blogosphere: see, for example, Andy Lawrence, Sarah Kendrew, and Amanda Bauer; I’m sure there are many more articles elsewhere.

The US House Appropriations Committee has released its Science Appropriations Bill for the Fiscal Year 2012, which will be voted on tomorrow. Among other announcements (of big cuts to NASA’s budget) listed in the accompanying press release we find

The bill also terminates funding for the James Webb Space Telescope, which is billions of dollars over budget and plagued by poor management.

It is undoubtedly the case that JWST is way over budget and very late. Initial estimates put the cost of the at $1.6 billion and that it would be launched this year (2011). Now it can’t launch until at least 2018,  and probably won’t fly until as late as 2020, with an estimated final price tag of $6.8 billion. I couldn’t possibly comment on whether that is due to poor management or just that it’s an incredibly challenging project.

There’s a very informative piece on the Nature News Blog that explains that this is an early stage of the passage of the bill and that there’s a long way to go before JWST is definitely axed, but it is a worrying time for all those involved in it. There are serious implications for the European Space Agency, which is also involved in JWST, to STFC, which supports UK activity in related projects, and indeed for many groups of astronomers around the world who are currently engaged in building and testing instruments.

One of the arguments against cancelling JWST now is that all the money that has been spent on it so far would have been wasted, in other words that it’s “too big to fail”, which is an argument that obviously can’t be sustained indefinitely. It may be now it’s so far over budget that it’s become a political liability to NASA, i.e. it’s too big to succeed. It’s too early to say that JWST is doomed – this draft budget is partly a political shot across the bows of the President by the Republicans in the House – but it does that the politicians are prepared to think what has previously been unthinkable.

UPDATE: A statement has been issued by the American Astronomical Association.

 

Feynman on Poetry

Posted in Poetry, The Universe and Stuff with tags , on July 6, 2011 by telescoper

Poets say science takes away from the beauty of the stars – mere globs of gas atoms. I too can see the stars on a desert night, and feel them. But do I see less or more? The vastness of the heavens stretches my imagination – stuck on this carousel my little eye can catch one – million – year – old light. A vast pattern – of which I am a part… What is the pattern, or the meaning, or the why? It does not do harm to the mystery to know a little about it. For far more marvelous is the truth than any artists of the past imagined it. Why do the poets of the present not speak of it? What men are poets who can speak of Jupiter if he were a man, but if he is an immense spinning sphere of methane and ammonia must be silent?

Richard Feynman (1918-1988)

After Summer Rain

Posted in Poetry with tags , , on July 6, 2011 by telescoper

All day the rain has filled the apple-trees,
And stilled the orchard grasses of their mirth,
Turning these acres green and silvered seas
That drowned the summer musics of the earth.
Now that this clearer twilight takes the hill,
This thin, belated radiance, moving by,
Bird-calls return, and odours, rainy still,
And colours glinting through the earth and sky.

Here where I watch the robins from the lane,
That pirouette and preen among the leaves,
These swift, wet-winged arrivals in the rain
Have spilled a wisdom from their dripping eaves,–
And beauty still is more than daily bread,
For fevered minds, and hearts discomforted.

by David Morton (1886-1957)

Late Talking

Posted in Biographical, Education with tags , , , , , , on July 5, 2011 by telescoper

In the course of linking my previous post to Richard Feynman’s wikipedia page, I happened upon an interesting fact:

Feynman (in common with the famous physicists Edward Teller and Albert Einstein) was a late talker; by his third birthday he had yet to utter a single word.

I therefore have something in common with these famous physicists. I didn’t learn to speak until I was well past my third birthday, as my mum never tires of reminding me.  In fact, as I have blogged about before,  I was a very slow developer in other ways and when I started school was immediately earmarked as an educational basket case.

I subsequently discovered that

Neuroscientist Steven Pinker postulates that a certain form of language delay may be associated with exceptional and innate analytical prowess in some individuals, such as Albert Einstein, Richard Feynman and Edward Teller.

Which is obviously where the similarity between me and these chaps ends, as I certainly don’t have “exceptional and innate analytical prowess”. I am however intrigued by the fact that I at least shared their  failure to develop language abilities on the same timescale as “normal” infants. I don’t know very much at all about this field, even to the extent of not knowing at what age most children learn to talk…

So here’s a couple of questions for my readers out there in blogoland. Were any of you late talkers? And how unusual is it for a child not to speak until they’re three years old?

Contributions welcomed through the comments box!

Feynman on Wine

Posted in Poetry, The Universe and Stuff with tags , on July 5, 2011 by telescoper

A poet once said, ‘The whole universe is in a glass of wine.’ We will probably never know in what sense he meant it, for poets do not write to be understood. But it is true that if we look at a glass of wine closely enough we see the entire universe. There are the things of physics: the twisting liquid which evaporates depending on the wind and weather, the reflection in the glass; and our imagination adds atoms. The glass is a distillation of the earth’s rocks, and in its composition we see the secrets of the universe’s age, and the evolution of stars. What strange array of chemicals are in the wine? How did they come to be? There are the ferments, the enzymes, the substrates, and the products. There in wine is found the great generalization; all life is fermentation. Nobody can discover the chemistry of wine without discovering, as did Louis Pasteur, the cause of much disease. How vivid is the claret, pressing its existence into the consciousness that watches it! If our small minds, for some convenience, divide this glass of wine, this universe, into parts — physics, biology, geology, astronomy, psychology, and so on — remember that nature does not know it! So let us put it all back together, not forgetting ultimately what it is for. Let it give us one more final pleasure; drink it and forget it all!

Richard Feynman (1918-1988)

 

Cool Columbo

Posted in Columbo with tags , on July 4, 2011 by telescoper

I thought I’d post a quick update about ye olde Columbo because last week I mentioned that I was a bit concerned about his health. I’m glad to report that there’s been no re-occurrence of sickness (that I’ve seen). I started him back on the anti-inflammatory drug and that, probably together with the warm weather we’ve been having recently, has improved his mood considerably. He’s been spending most of his time outdoors lately, in the shade among the bushes at the end of the garden, emerging only to answer the call of nature or to cadge some food. Despite the fact that he’s not exactly Speedy Gonzalez these days it’s still quite difficult to take a picture of him, as he won’t look at the camera, and when I do manage to get a snap he always seems to look grumpy.

 

False Convergence and the Bandwagon Effect

Posted in The Universe and Stuff with tags , , , , , , on July 3, 2011 by telescoper

In idle moments, such as can be found during sunny sunday summer afternoons in the garden, it’s  interesting to reminisce about things you worked on in the past. Sometimes such trips down memory lane turn up some quite interesting lessons for the present, especially when you look back at old papers which were published when the prevailing paradigms were different. In this spirit I was lazily looking through some old manuscripts on an ancient laptop I bought in 1993. I thought it was bust, but it turns out to be perfectly functional; they clearly made things to last in those days! I found a paper by Plionis et al. which I co-wrote in 1992; the abstract is here

We have reanalyzed the QDOT survey in order to investigate the convergence properties of the estimated dipole and the consequent reliability of the derived value of \Omega^{0.6}/b. We find that there is no compelling evidence that the QDOT dipole has converged within the limits of reliable determination and completeness. The value of  \Omega_0 derived by Rowan-Robinson et al. (1990) should therefore be considered only as an upper limit. We find strong evidence that the shell between 140 and 160/h Mpc does contribute significantly to the total dipole anisotropy, and therefore to the motion of the Local Group with respect to the cosmic microwave background. This shell contains the Shapley concentration, but we argue that this concentration itself cannot explain all the gravitational acceleration produced by it; there must exist a coherent anisotropy which includes this structure, but extends greatly beyond it. With the QDOT data alone, we cannot determine precisely the magnitude of any such anisotropy.

(I’ve added a link to the Rowan-Robinson et al. paper for reference). This was  a time long before the establishment of the current standard model of cosmology (“ΛCDM”) and in those days the favoured theoretical paradigm was a flat universe, but one without a cosmological constant but with a critical density of matter, corresponding to a value of the density parameter \Omega_0 =1.

In the late eighties and early nineties, a large number of observational papers emerged claiming to provide evidence for the (then) standard model, the Rowan-Robinson et al. paper being just one. The idea behind this analysis is very neat. When we observe the cosmic microwave background we find it has a significant variation in temperature across the sky on a scale of 180°, i.e. it has a strong dipole component

There is also some contamination from Galactic emission in the middle, but you can see the dipole in the above map from COBE. The interpretation of this is that the Earth is not at rest. The  temperature variation causes by our motion with respect to a frame in which the cosmic microwave background (CMB) would be isotropic (i.e. be the same temperature everywhere on the sky) is just \Delta T/T \sim v/c. However, the Earth moves around the Sun. The Sun orbits the center of the Milky Way Galaxy. The Milky Way Galaxy orbits in the Local Group of Galaxies. The Local Group falls toward the Virgo Cluster of Galaxies. We know these velocities pretty well, but they don’t account for the size of the observed dipole anisotropy. The extra bit must be due the gravitational pull of larger scale structures.

If one can map the distribution of galaxies over the whole sky, as was first done with the QDOT galaxy redshift survey, then one can compare the dipole expected from the distribution of galaxies with that measured using the CMB. We can only count the galaxies – we don’t know how much mass is associated with each one but if we find that the CMB and the galaxy dipole line up in direction we can estimate the total amount of mass needed to give the right magnitude. I refer you to the papers for details.

Rowan-Robinson et al. argued that the QDOT galaxy dipole reaches convergence with the CMB dipole (i.e. they line up with one another) within a relatively small volume – small by cosmological standards, I mean, i.e. 100 Mpc or so- which means that  there has to be quite a lot of mass in that small volume to generate the relatively large velocity indicated by the CMB dipole. Hence the result is taken to indicate a high density universe.

In our paper we questioned whether convergence had actually been reached within the QDOT sample. This is crucial because if there is significant structure beyond the scale encompassed by the survey a lower overall density of matter may be indicated. We looked at a deeper survey (of galaxy clusters) and found evidence of a large-scale structure (up to 200 Mpc) that was lined up with the smaller scale anisotropy found by the earlier paper. Our best estimate was \Omega_0\sim 0.3, with a  large uncertainty. Now, 20 years later, we have a  different standard cosmology which does indeed have \Omega_0 \simeq 0.3. We were right.

Now I’m not saying that there was anything actually wrong with the Rowan-Robinson et al. paper – the uncertainties in their analysis are clearly stated, in the body of the paper as well as in the abstract. However, that result was widely touted as evidence for a high-density universe which was an incorrect interpretation. Many other papers published at the time involved similar misinterpretations. It’s good to have a standard model, but it can lead to a publication bandwagon – papers that agree with the paradigm get published easily, while those that challenge it (and are consequently much more interesting) struggle to make it past referees. The accumulated weight of evidence in cosmology is much stronger now than it was in 1990, of course, so the standard model is a more robust entity than the corresponding version of twenty years ago. Nevertheless, there’s still a danger that by treating ΛCDM as if it were the absolute truth, we might be closing our eyes to precisely those clues that will lead us to an even better understanding.  The perils of false convergence  are real even now.

As a grumpy postscript, let me just add that Plionis et al. has attracted a meagre 18 citations whereas Rowan-Robinson et al. has 178. Being right doesn’t always get you cited.

Lucia’s Mad Scene

Posted in Opera with tags , , on July 2, 2011 by telescoper

I came across this little clip of the great Maria Callas on youtube, and couldn’t resist sharing it for the benefit of those (apparently many) people out there who think she was an overrated singer. I’m a devout Callas fan, but I also freely admit that many of the performances she recorded later in her career (especially in the 60s) weren’t all that good and it’s unfortunate that most of her famous performances were in an era when audio technology wasn’t really up to the task of recording live opera.

However, you can get an idea of how very special Maria Callas was in this little clip recorded live at La Scala in Milan in 1954. It’s a poor quality recording but her voice has a stunning radiance to it despite the distortions. This is the very end of the lengthy Act III “Mad Scene” from Donizetti‘s Opera Lucia di Lammermoor. It’s a tremendously demanding piece, which Callas sings with flawless technical accuracy and extraordinary expressive power leading up to a ringing top E♭ at the end. Her approach to the vocal gymnastics required by the bel canto repertoire was uniquely full-on and, without a safety net, the sense of danger surrounding these performances made them truly electrifying.

Only some of the music  made it onto the recording, but there’s enough there to convince the doubters that this was a very special artist. And, listening to the applause at the end, the notoriously demanding audience at La Scala were clearly convinced too!

Incidentally, some argue that Callas’ voice was in decline after her substantial weight loss (she lost 80lbs between 1953 and 1954), but this was the slim Callas and her voice sounds pretty good to me!