Archive for the The Universe and Stuff Category

For Your Listening Pleasure…

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

Well, this is blogging made easy. I’ve just cut-and-pasted the following item directly from the School’s news page with very few alterations, but it’s all done for a good reason, so please read on:

A leading member of the School of Physics and Astronomy at Cardiff University, whose research helped create one of the most powerful and ambitious astronomical satellites ever made will feature in a two-part Radio 4 programme.

The Herschel Space Telescope is a two-part series to be aired on Radio 4 on Wednesday 18th November, 11:00-11:30am and Wednesday 25th November, 11:00-11:30am. BBC science reporter Jonathan Amos follows the engineers and scientists working on the SPIRE instrument for the European Space Agency’s Herschel satellite. Herschel is one of the most important missions in the history of European spaceflight and was launched successfully on May 14 this year.

The SPIRE instrument was built by an international team led by Professor Matt Griffin, School of Physics and Astronomy. The programme tells the story of the UK SPIRE team, including several members from Cardiff, as they prepared for the launch of Herschel and as the first results came in.

As well as Professor Griffin, other members of staff in the School of Physics and Astronomy who contributed to the project are also featured. They include: Professor Steve Eales, Dr Jon Davies, Dr Kate Isaak, and Dr Pete Hargrave as well as post-doctoral researchers Dr Jason Kirk, Dr Michael Pohlen, and Dr Luca Cortese.

Professor Matt Griffin

Herschel carries the biggest mirror ever sent to space and is already giving astronomers their best view yet of the Universe at far-infrared and sub-millimetre wavelengths. It can peer through obscuring clouds of dust to look at the early stages of star birth and galaxy formation; it can examine the composition and chemistry of comets and planetary atmospheres in the Solar System; and it is able to study the star-dust ejected by dying stars into interstellar space which forms the raw material for planets like the Earth.

Professor Griffin said: “With its big telescope and sophisticated and sensitive instruments, including SPIRE, Herschel is a very powerful observatory for many studies from our own solar system to the most distant galaxies. Already we can see that its results will reveal how stars like the Sun are forming in our own galaxy today, how planetary systems can develop from the dust and gas around young stars, and how the galaxies grew and evolved over cosmic time.

“Astronomers from Cardiff are at the forefront in making these exciting scientific discoveries – we are delighted that the work of Cardiff scientists will be featured in such an important radio programme.”

I should also point out that BBC Radio 4 programmes can be listened to online, and are available to download for a week after the broadcast from the BBC website (even to foreigners).

PS. I should also mention that today’s “Material World” (another Radio 4 programme) was a special edition from Cardiff University and also featured an astronomy item. If you missed it, or if you want to hear it again, you can listen to it here.


Viva Voce

Posted in Biographical, The Universe and Stuff with tags , on November 11, 2009 by telescoper

Just back from a flying visit to the beautiful city of Edinburgh, where I was involved in the examination of a PhD candidate at the Institute for Astronomy, which is housed on the site of the Royal Observatory.

For those of you not familiar with how this works, a PhD involves doing research into a particular topic and then writing up what you’ve done in a thesis. The thesis is a substantial piece of work, often in the region of 100,000 words (200 pages or so), which is then assessed by two examiners (one internal to the university at which the research was done, and one external). They read copies of the thesis and then the candidate has to defend it in an oral examination, which was what happened today, after which they make a recommendation to the university about whether the degree should be awarded.

At most universities the supervisor does not attend the oral examination, but is not normally required to go into hiding for the day, which is what seemed to happen in this case…

There aren’t many rules for how a viva voce examination should be conducted or how long it should last, but the can be as short as, say, 2 hours and can be as long as 5 hours or more. The examiners usually ask a mixture of questions, some about the details of the work presented and some about the general background. The unpredictable content of a viva voce examination makes it very difficult to prepare for, and it can be difficult and stressful for the candidate (as well as just tiring, as it can drag on for a long time). However, call me old-fashioned but I think if you’re going to get to call youself Doctor of Philosophy you should expect to have to work for it. Some might disagree.

As it happens, my own PhD examination 20 years ago was quite long (about 4hrs 30 minutes) and my external examiner was John Peacock, who happened to be the supervisor of today’s candidate Berian James. It wasn’t a deliberate consequence of me wanting to take vicarious revenge as external examiner on John’s student, but this turned out to be a long examination too. We did break twice (once, briefly, for the remembrance day silence and then for a longer period for lunch), but it was still a lengthy affair.

Obviously I can’t give details of what went on in the examination except that it was long primarily because the thesis was very interesting and gave us lots to discuss. In the end internal examiner Philip Best and I agreed to recommend the award of a PhD. Berian then went off to celebrate while we completed the necessary paperwork. At Edinburgh as in most UK universities, the examiners simply make a recommendation to a higher authority (e.g. Board of Graduate Studies) to formally award the degree, but in the overwhelming majority of cases they follow the recommendation.

After doing the paperwork I still had time to join the party for a glass or two of fizzy. At the do and at various points during the day I had the chance to say hello to some old friends, including Andy Taylor, Bob Mann, and Alan Heavens who all work at the ROE and Richard Nelson who was there for a meeting that I hadn’t known about when we arranged the date and time of the viva.

All in all, it was a very pleasant trip. Although I had to dash around to and from airports a bit getting to and from Scotland, all the planes went on time and since it’s less than an hour flying time from Cardiff to Edinburgh, it was all remarkably hassle-free.

Just before I left to get a taxi to the airport I had a quick chat with one of the PhD students, Alina Kiessling, who joked that I must be rushing off to write about the day on my blog. I never had time to read blogs when I was a PhD student (but  they hadn’t been invented then).

Perhaps I should start charging people to put their name in lights on In the Dark

Planck’s Progress

Posted in The Universe and Stuff with tags , , on November 10, 2009 by telescoper

Only time for a very quick post today, so I thought I’d just pass on some news I got via Chris North about how Planck is doing. As it happens, the satellite has recently reached  the point where it has observed about half the sky. It spins on its axis in rather stately fashion (at about one revolution per minute) and, as it moves in its orbit, that sweeps the telescope across the celestial sphere. Each scan is almost a great circle, but  these gradually creep around over about a six month period to cover the whole sky.

The nice picture below, in ecliptic coordinates, shows how far it has got. You can also see the Galactic plane, arching across the sky and showing up clearly at the frequencies Planck is sensitive to.

Planck3NovSkyCoverage

The Planck Consortium had an official meeting last week in Bologna at which they drank lots of wine and ate lots of food, but other than that nobody who was there has told me anything.

It’s all very hush hush don’t you know.

I want it painted … beige?

Posted in The Universe and Stuff with tags , , , , , on November 4, 2009 by telescoper

I was quite pleased when I saw that Pass Notes No 2,677 in Today’s Guardian was about “the universe”. Like the other pieces in this series, it looks at the subject matter from a deliberately bizarre angle, focussing on the fact that it appears to be coloured beige, or at least if you blend the light from all the stars we can see in the right proportions, that’s the colour you would get.

Actually the work discussed in this item was done quite along time ago; it was featured in a New Scientist article in 2002. One of the authors, Karl Glazebrook had previously claimed that the colour produced by all the stars in all the galaxies that could be seen was in fact something like turquoise. For some reason, this trivial bit of science fluff captured the (obviously limited) imagination of journalists around the world. However it turned out to be have been wrong and a grave announcement was made pointing out that the Universe was actually more like beige. This story gave a few people their 15 minutes of fame, but I think the episode made cosmologists as a whole look very silly.

I had hoped this would be forgotten but, the Guardian decided to revive memories of the affair today, with obviously humorous intent. They also called Glazebrook an “astrologist”, although that appears to have been a mistake rather than a joke as it has now been changed to “astrophysicist”.

Anyway, this important observation requires a theoretical explanation and I now want to step into the limelight beigelight to offer a radical insight into the vexed issue of cosmological chromaticity.
My hypothesis has its inspiration in TV shows like House Doctor in which homeowners wishing to impress prospective purchasers are always advised to paint everything beige or magnolia. Since the Divine Creator appears to have decorated the Universe according to the same prescription, the obvious inference is that the cosmos is about to be put on the market. He might have had the courtesy to tell the sitting tenants.

Come to think of it, Glazebrook missed a trick here. We astrophysicists are always being castigated for not doing anything that leads to wealth creation. What he should have done was to produce a paint with the same colour as the Universe. Glazebrook Beige has a nice ring to it.

Highlights

Posted in Biographical, The Universe and Stuff with tags , , on November 2, 2009 by telescoper

Despite popular demand, here is more of the Unravelling the Universe show I posted a little bit from a few days ago. My total screen time on this programme only amounted to a couple of minutes, so I asked if it was possible to do an appropriate edit of the hour-long footage. Unfortunately, Ed got the wrong idea, so removed most of the highlights and left practically only the few minutes with me in them. You just can’t get the help these days.

The film  was shot in a studio in Greenford and I had to hang around there a long time before they even started shooting. I think that was because of the lights. I need a special form of  illumination if I am to present the illusion of having three dimensions. The director had insisted I wear my leather jacket for the sequence and under the very powerful lights I was sweating so much I had to wear make-up to stop me shining.

They reckon that there is a ratio of about 100:1 of film shot to film broadcast on programmes like this, and this is probably even higher when the subject is as inarticulate as me. In my memory it certainly took several hours just for my little bits.

If nothing else this tape gives you the chance to see Rocky Kolb in a splendid jumper that puts that of the new Lucasian professor well and truly in the shade. What was that about chromodynamics?

The Michael Green Experience

Posted in Biographical, The Universe and Stuff with tags , , , on October 30, 2009 by telescoper

It’s been a couple of weeks since the University of Cambridge announced that the successor to Stephen Hawking as Lucasian Professor  of Mathematics would be Michael Green, who is best known for his work on string theory. Heartiest congratulations to him for reaching a position of such eminence.

I was trying to think of a suitable way of marking the occasion of his election to this prestigious post when I suddenly remembered that we were actually on a TV programme together years ago. The show in question was called Unravelling the Universe and was first broadcast in December 1991 as part of a science documentary series called Equinox.

I eventually found my ancient VHS copy of the broadcast master tape of this show and persuaded Ed and Stephen, two of the excellent elves that work in the School of Physics & Astronomy here at Cardiff University, to transfer it to a digital format and put a bit on Youtube for all to see. Many thanks to them for their help.

Other people involved in the programme included Rocky Kolb, Chris Isham and Paul Davies but the short (2-and-a-half minute) clip below features just Michael Green (who basically put the show together) and myself (who was just there to make up the numbers), plus wonderful narration by the late great Peter Jones.

Michael Green hasn’t changed a bit in 18 years. In fact, I saw him last year and am sure he was even wearing the same sweater.

I, on the other hand….Oh dear.

The Edge of Darkness

Posted in The Universe and Stuff with tags , , , on October 29, 2009 by telescoper

I just picked up an item from the BBC Website that refers to news announced in this week’s edition of Nature of the discovery of a gamma-ray burst detected by NASA’s Swift satellite.  The burst itself was detected in April this year and I had a sneak preview that something exciting was going to be announced earlier this month at the Royal Astronomical Society meeting on October 9th. However, today’s press releases still managed to catch me on the hop owing to the fact that a rather different story had distracted my attention…

In fact, detections of gamma-ray bursts are not all that rare. Swift observes one every few days on average. Once such a source is found through its gamma-ray emission, a signal is sent to astronomers around the world who then work like crazy to detect an optical counterpart. If and when they find one, they try to measure the spectrum of light emitted in order to determine the source’s redshift. This is very difficult for the distant ones, and is not  always successful.

However, what happened in this case – called GRB 090423 – was that a spectrum was that not one but two independent teams obtained optical spectra of the  object in which the gamma-ray burst must have happened. What each time found was that their spectrum showed a sharp cut-off at wavelengths shorter than a given limiting value.

Hydrogen is very effective at absorbing radiation with wavelengths shorter than 91.2 nm (the so-called Lyman limit, which is in the ultraviolet part of the spectrum), and all galaxies contain large amounts of hydrogen; hence galaxies are virtually dark at wavelengths shorter than 91.2 nm in their rest-frame. The position of the break in an observed frame will be at a different wavelength owing to the effect of the cosmological redshift.

The Lyman break for the host of  GRB 090423 appears not in the ultraviolet but in the infrared, indicating a very large redshift. In fact, it’s a truly spectacular  8.2.

Together with the direct observations of galaxies at high redshifts I blogged about a month or so ago, this discovery helps push back the frontiers of our knowledge of the Universe not just in space but also in time. A quick calculation reveals that in the standard cosmological model, light from a source at redshift 8.2 has taken about 13.1 billion light years to reach us. The gamma-ray burst therefore exploded about 600 million years after the Big Bang.

Another interesting thing about this source is its duration. The optical afterglow of a gamma-ray burst  decays with time. Gamma-ray bursts are usually classified as either short or long, depending on the decay time with the dividing line between the two classes being around 2 seconds. The optical afterglow of GRB 090423 lasted about ten seconds. But that doesn’t make it a long burst. We actually see the afterglow stretched out in time by the same redshift factor as an individual photon’s wavelength. So in the rest frame of the source the optical glow was only a bit over a second in duration, i.e. it was a short burst.

Long gamma-ray bursts are thought to be associated with core-collapse supernovae which arise from the self-destruction of very massive stars with very short lifetimes. The fact that such things die young means that they are only found where star formation has happened very recently. One might expect the earliest gamma-ray bursts to therefore be of this type.

I don’t think anyone is really sure what the shorter ones really are, but they  seem to happen in regions without active star formation in which the stellar populations are quite old, such as in elliptical galaxies. The fact that the most distant GRB yet discovered happens to be a short burst is very interesting. How can there be an old stellar population at a time when the  Universe itself was so young?

If the Big Bang theory is correct, astronomers  should eventually be able to reach back so far in time that the Universe was so young that no stars had had time to form. There would be no sources of light to detect so we would have reached the edge of darkness. We’re not there yet, but we’re getting closer.

A Random Walk

Posted in The Universe and Stuff with tags , , , , , on October 24, 2009 by telescoper

In 1905 Albert Einstein had his “year of miracles” in which he published three papers that changed the course of physics. One of these is extremely famous: the paper that presented the special theory of relativity. The second was a paper on the photoelectric effect that led to the development of quantum theory. The third paper is not at all so well known. It was about the theory of Brownian motion.  In fact, Einstein spent an enormous amount of time and energy working on problems in statistical physics, something that isn’t so well appreciated these days as his work on the more glamorous topics of relativity and quantum theory.

 Brownian motion, named after the botanist Robert Brown,  is the perpetual jittering observed when small particles such as pollen grains are immersed in a fluid. It is now well known that these motions are caused by the constant bombardment of the grain by the fluid molecules. The molecules are too small to be seen directly, but their presence can be inferred from the visible effect on the much larger grain.

Brownian motion can be observed whenever  any relatively massive particles (perhaps large molecules) are immersed in a fluid comprising lighter particles. Here is a little video showing the Brownian motion observed by viewing smoke under a microscope. There is a small coherent “drift” motion in this example but superimposed on that you can clearly see the effect of gas atoms bombarding the (reddish) smoke particles:

The mathematical modelling of this process was pioneered by Einstein (and also Smoluchowski), but has now become a very sophisticated field of mathematics in its own right. I don’t want to go into too much detail about the modern approach for fear of getting far too technical, so I will concentrate on the original idea.

Einstein took the view that Brownian motion could be explained in terms of a type of stochastic process called a “random walk” (or sometimes “random flight”). I think the first person to construct a mathematical model to describethis type of phenomenon was the statistician Karl Pearson. The problem he posed concerned the famous drunkard’s walk. A man starts from the origin and takes a step of length L in a random direction. After this step he turns through a random angle and takes another step of length L. He repeats this process n times. What is the probability distribution for R, his total distance from the origin after these n steps? Pearson didn’t actually solve this problem, but posed it in a letter to Nature in 1905. Only a  week later, a reply from Lord Rayleigh was published in the same journal. He hadn’t worked it all out, written it up and sent it within a week though. It turns out that Rayleigh had solved essentially the same problem in a different context way back in 1880 so he had the answer readily available when he saw Pearson’s letter.

Pearson’s problem is a restricted case of a random walk, with each step having the same length. The more general case allows for a distribution of step lengths as well as random directions. To give a nice example for which virtually everything is known in a statistical sense, consider the case where each component of the step, i.e. x and y, are independent Gaussian variables, which have zero mean so that there is no preferred direction:

p(x)=\frac{1}{\sigma\sqrt{2\pi}} \exp \left(-\frac{x^2}{2\sigma^2}\right)  

A similar expression holds for p(y). Now we can think of the entire random walk as being two independent walks in x and y.  After n steps the total displacement in x, say, xn is given by

 p(x_n)=\frac{1}{\sigma\sqrt{n 2\pi }} \exp \left(-\frac{x_n^2}{2n\sigma^2}\right)

and again there is a similar expression for the distribution of yn . Notice that each of these distribution has a mean value of zero. On average, meaning on average over the entire probability distribution of realizations of the walk, the drunkard doesn’t go anywhere. In each individual walk he certainly does go somewhere, of course, but he is equally likely to move in any direction the probabilistic mean has to be zero. The total net displacement from the origin, rn , is just given by Pythagoras’ theorem:

r_n^2=x_n^2+y_n^2

 from which it is quite easy to establish that the probability distribution has to be

 p(r_n)=\frac{r_n}{n\sigma^2} \exp \left(-\frac{r_n^2}{2n\sigma^2}\right)

 This is called the Rayleigh distribution, and this kind of process is called a Rayleigh “flight”. The mean value of the displacement is just σ√n. By virtue of the ubiquitous central limit theorem, this result also holds in the original case discussed by Pearson in the limit of very large n. So this gives another example of the useful rule-of-thumb that quantities arising from fluctuations among n entities generally give a result that depends on the square root of n.

The figure below shows a simulation of a Rayleigh random walk. It is quite a good model for the jiggling motion executed by a Brownian particle. 

 sp003196

The step size resulting from a collision of a Brownian particle with a molecule depends on the mass of the molecule and of the particle itself. A heavier particle will be relatively unaffected by each bash and thus take longer to diffuse than a lighter particle. Here is a nice video showing three-dimensional simulations of the diffusion of sugar molecules (left) and proteins (right) that demonstrates this effect.

Of course not even the most inebriated boozer will execute a truly random walk. One would expect each step direction to have at least some memory of the previous one. This gives rise to the idea of a correlated random walk.  Such objects can be used to mimic the behaviour of geometric objects that possess some stiffness in their joints, such as proteins or other long molecules. Nowadays theory of Brownian motion and related stochastic phenomena is now considerably more sophisticated than the simply random flight models I have discussed here. The more general formalism can be used to understand many situations involving phenomena such as diffusion and percolation, not to mention gambling games and the stock market. The ability of these intrinsically “random” processes to yield surprisingly rich patterns is, to me, one of their most fascinating aspects. It takes only a little tweak to create order from chaos.

 

Nox Nocti Indicat Scientiam

Posted in Poetry, The Universe and Stuff with tags , on October 23, 2009 by telescoper

According to my blog access statistics, some of the poems I post on here seem to be fairly popular so I thought I’d put up another one by another poet  from the Metaphysical tradition, William Habington. He belonged to a prominent Catholic family and lived in England from 1605 to 1654, during a time of great religious upheaval.

The title of this particular poem is taken from the Latin (Vulgate) version of Psalm 19, the first two lines of which are

Caeli enarrant gloriam Dei et opus manus eius adnuntiat firmamentum.
Dies diei eructat verbum et nox nocti indicat scientiam.

The King James Bible translates this as

The heavens declare the glory of God; and the firmament sheweth his handywork.
Day unto day uttereth speech, and night unto night sheweth knowledge.

Some translations I have seen give “night after night” rather than the form above. My distant recollection of  Latin learnt at school tells me that nocti is the dative case of the third declension noun nox, so I think think “night shows knowledge to night” is indeed the correct sense of the Latin. Of course I don’t know what the sense of the original Hebrew is!

The original Psalm is the text on which one of the mightiest choruses of Haydn’s  Creation is based, “The Heavens are Telling” and Habington’s poem is a meditation on it. It seems to me to be a natural companion to the poem by John Masefield I posted earlier in the week, but I don’t know whether they share a common inspiration in the Psalm or just in the Universe itself.

When I survey the bright
Celestial sphere;
So rich with jewels hung, that Night
Doth like an Ethiop bride appear:

My soul her wings doth spread
And heavenward flies,
Th’ Almighty’s mysteries to read
In the large volumes of the skies.

For the bright firmament
Shoots forth no flame
So silent, but is eloquent
In speaking the Creator’s name.

No unregarded star
Contracts its light
Into so small a character,
Removed far from our human sight,

But if we steadfast look
We shall discern
In it, as in some holy book,
How man may heavenly knowledge learn.

It tells the conqueror
That far-stretch’d power,
Which his proud dangers traffic for,
Is but the triumph of an hour:

That from the farthest North,
Some nation may,
Yet undiscover’d, issue forth,
And o’er his new-got conquest sway:

Some nation yet shut in
With hills of ice
May be let out to scourge his sin,
Till they shall equal him in vice.

And then they likewise shall
Their ruin have;
For as yourselves your empires fall,
And every kingdom hath a grave.

Thus those celestial fires,
Though seeming mute,
The fallacy of our desires
And all the pride of life confute:–

For they have watch’d since first
The World had birth:
And found sin in itself accurst,
And nothing permanent on Earth.


Another take on cosmic anisotropy

Posted in Cosmic Anomalies, The Universe and Stuff with tags , , , on October 22, 2009 by telescoper

Yesterday we had a nice seminar here by Antony Lewis who is currently at Cambridge, but will be on his way to Sussex in the New Year to take up a lectureship there. I thought I’d put a brief post up here so I can add it to my collection of items concerning cosmic anomalies. I admit that I had missed the paper he talked about (by himself and Duncan Hanson) when it came out on the ArXiv last month, so I’m very glad his visit drew this to my attention.

What Hanson & Lewis did was to think of a number of simple models in which the pattern of fluctuations in the temperature of the cosmic microwave background radiation across the sky might have a preferred direction. They then construct optimal estimators for the parameters in these models (assuming the underlying fluctuations are Gaussian) and then apply these estimators to the data from the Wilkinson Microwave Anisotropy Probe (WMAP). Their subsequent analysis attempts to answer the question whether the data prefer these anisotropic models to the bog-standard cosmology which is statistically isotropic.

I strongly suggest you read their paper in detail because it contains a lot of interesting things, but I wanted to pick out one result for special mention. One of their models involves a primordial power spectrum that is intrinsically anisotropic. The model is of the form

P(\vec{ k})=P(k) [1+a(k)g(\vec{k})]

compared to the standard P(k), which does not depend on the direction of the wavevector. They find that the WMAP measurements strongly prefer this model to the standard one. Great! A departure from the standard cosmological model! New Physics! Re-write your textbooks!

Well, not really. The direction revealed by the best-choice parameter fit to the data is shown in the smoothed picture  (top). Underneath it are simulations of the sky predicted by their  model decomposed into an isoptropic part (in the middle) and an anisotropic part (at the bottom).

lewis2

You can see immediately that the asymmetry axis is extremely close to the scan axis of the WMAP satellite, i.e. at right angles to the Ecliptic plane.

This immediately suggests that it might not be a primordial effect at all but either (a) a signal that is aligned with the Ecliptic plane (i.e. something emanating from the Solar System) or (b) something arising from the WMAP scanning strategy. Antony went on to give strong evidence that it wasn’t primordial and it wasn’t from the Solar System. The WMAP satellite has a number of independent differencing assemblies. Anything external to the satellite should produce the same signal in all of them, but the observed signal varies markedly from one to another. The conclusion, then, is that this particular anomaly is largely generated by an instrumental systematic.

The best candidate for such an effect is that it is an artefact of a asymmetry in the beams of the two telescopes on the satellite. Since the scan pattern has a preferred direction, the beam profile may introduce a direction-dependent signal into the data. No attempt has been made to correct for this effect in the published maps so far, and it seems to me to be very likely that this is the root of this particular anomaly.

We will have to see the extent to which beam systematics will limit the ability of Planck to shed further light on this issue.