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Posts Tagged light

Hawking radiation in the lab Marcus Wilson Oct 21

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A highlight of the recent NZ Institute of Physics conference was the Dan Walls medal talk given by Matt Visser. Matt has been working on general relativity. That's not desparately unusual for a physicist, but Matt has been successful in working on some of the crazier aspects of relativity and getting it published – wormholes, dumb holes and the like. He gave an entertaining talk – perfect for closing the conference.

I was particularly taken by the description of the analogies between light and sound. It's unsurprising that there should be analogies between the physics of light and the physics of sound in that both are waves, but the extent to which the analogy can go surprised me. For example, it is possible to get Hawking radiation with sound. 

Hawking radiation is predicted to be radiated from black holes. I say 'predicted' because experimental evidence is still scant. It allows black holes to 'evaporate' by emitting radiation from their event horizons (Within the event horizon nothing escapes the black hole – not even light. Once you've passed that boundary, you have a one-way ticket to a singularity). There's an analogy between the event horizon of the black hole and an acoustic shock-front (sonic boom) created by an object moving faster than sound. In the case of the former, once you are past the event horizon you can't get back out, and in the case of the latter, it's not possible for a perturbation that occurs behind the shock front to have an effect in front of it – in order to do so it would need to go faster than sound. 

It turns out that many of the equations governing the situations are similar, including those necessary to produce Hawking radiation. The implication is that one should be able to create Hawking radiation from shock fronts created with supersonic fluid flow. And indeed it has been done – what one might consider an effect of general relativity demonstrated in a fairly simple lab experiment. Quite beautiful. Black holes (well, OK, certain aspects of them) on your lab bench.

 

Precision Cosmology – Yeah, Right! Marcus Wilson Sep 27

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We've just had our first session at the NZ Institute of Physics Conference. The focus was on astrophysics, and we heard from Richard Easther about 'Precision Cosmology' – measuring things about the universe accurately enough to test theories and models of the universe. We ablso heard about binary stars and supernovae, and evidence for the existence of dark matter from observing high energy gamma rays.

Perhaps the most telling insight into cosmology was given in an off-the-cuff comment from one of our speakers, David Wiltshire. It went something like this. “In cosmology, if you have a model that fits all the experimental data then your model will be wrong, because you can guarantee that some of the data will be wrong.”

Testing models against experimental observation is a necessary step in their development. We call it validation. Take known experimental results for a situation and ask the model to reproduce them. If it can't (or can't get close enough) then the model is either wrong or it's missing some important factor.(s). Of course, this relies on your experimental observations being correct. And, if they're not, you're going to struggle to develop good models an good understanding about a situation.

The problem with astrophysics and cosmology is that experimental data is usually difficult and expensive to collect. There's not a lot of it – you don't tend to have twenty experiments sitting in orbit all measuring the same thing to offer you cross-checks of results – so if something goes wrong it might not be immediately apparent. And if you can't cross-check, you can't be terribly sure that your results are correct. It's a very standard idea across all of science – don't measure something just once, or just twice, (like so many of my students want to do), keep going until you are certain that you have agreement.

Little wonder why people have only very recently taken the words 'precision cosmology' at all seriously.

Hotspot and Silicone Tape Marcus Wilson Aug 09

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Well, today’s big story is just perfect for PhysicsStop. Cricket meets physics. What more could I ask for.

In case you’ve just arrived from Alpha Centauri,  there have been accusations flying that both English and Australian batsmen have been trying to defeat the ‘Hot Spot‘ detector by putting silicone tape on their bats. The allegations have been vigorously denied from both sides. 

Hot Spot is used as part of a decision review system in professional cricket. The idea is that it will provide evidence as to whether the ball has hit the bat or not when assessing possible dismissals. It uses thermal imaging (infra-red) technology to look for the heat left behind when the ball makes contact with a surface. As the cricket ball just skims the edge of the bat, friction between the two will generate a small amount of heat at the point of contact. The thermal imagers can detect this heat and therefore prove whether the ball hit the bat or not. At least, that is the intention.

So how might silicone tape (a fairly innocuous medical product) give the batsman an advantage? The allegation being made is that a batsman would put tape on the outside edge of the bat, which reduces or eliminates the ‘hot spot’ left by a ball grazing the edge. Presumably they’d leave off the tape from the inside edge, so as to make sure that a fine edge on to their pads gets detected to counter any appeal for leg-before-wicket. (I admit that anyone who doesn’t know cricket will not have a clue what I’m talking about at this point, but hopefully you can still follow the physics part.)

Presumably the thinking is that silicone tape reduces the frictional forces between bat and ball, and therefore reduces the heat generated during a collision between the two. Would it work? One would need to try it out to be sure. But a quick glance at some values for coefficients of friction (e.g. here) will show that there is a vast range of values depending on the two materials. Some combinations surfaces have much more potential for friction (and therefore heating) than others. So it’s plausible that a low friction tape might have the effect. (Though one would think there might be more effective methods – e.g. spraying the edge of the bat with a lubricant spray. The thinking might be that applying tape to a bat is, bizarrely as it might sound,  actually legal in cricket.)

There’s been some discussion on the blogs that it has to do with thermal conductivity, though I’m not convinced by this argument. To defeat Hot Spot in this manner, one would need a material that gets rid of the heat very quickly by spreading it to other areas, so a noticeable hot spot doesn’t persist. The problem is that the thermal diffusivities of everyday materials are too low for this to happen. Thermal diffusivity controls how quickly heat spreads out by conduction. Even the very highly diffusive materials, with thermal diffusivities of around 100 mm2/s or so, would have a spot of heat spread out by only 10 mm in a second (The square-root of the product of thermal diffusivity and time tells you roughly how far heat will spread in that time). The Hot Spot frame rate is much shorter than this so there’s not time for the heat to diffuse away.

But I can think of another mechanism by which the tape might fool Hot Spot. The amount of infra-red light emitted by a surface doesn’t just depend on its temperature. Some surfaces are better emitters than others. A perfect emitter is called a ‘black-body’ in physics. However, be warned – an object that emits infra-red really well doesn’t necessarily look black to the eye – and conversely don’t think that because something is white that it doesn’t emit infra-red well. Some materials have properties that are very dependent on wavelength. It is possible (I don’t know) that silicone tape has a lower emissivity than wood, and therefore the effect, as viewed by an infra-red camera, would be reduced. Possibly it’s a combination of reduced friction and reduced emissivity.

Then again, possibly this is just a media propaganda stunt to try to get some interest back into the last two Ashes tests. (Again, non-cricketers won’t have a clue about that sentence).

All this would make a great student project. I’m sure there’d be physics graduates queuing up to do a PhD in defeating cricket technology. 

 

 

 

What’s in a colour? Marcus Wilson Jul 23

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When I was young (about six-ish)  I had a variety of ambitions. Some of them I shared with a lot of other boys of my age, such as being a train driver and playing cricket for England. Some were more particular to me, such as becoming a biologist and discovering a new colour. 

Needless to say I failed on all accounts. One I got close to – being a physicist is not so far away from being a biologist.  I’ve at least watched England play cricket (including an England v India match at Lord’s – in the members’ guests area – that was rather neat) and stood on the footplate of a steam engine. Discovering a new colour, however, is something I was not likely to achieve from the outset.

I had a vague idea that if I mixed enough paints together I’d hit on a combination that no-one had tried before (maybe purple and green with just a hint of orange) and, hey-presto, they’d mix together to some entirely colour previously unknown to science. The colour would naturally be named after me, and become an instant hit with home decorators. Out would go ‘Magnolia’, in would come ‘Wilurple’. 

I gave up on the ambition long before I found out why it was unlikely to work. The CIE colour chart encapsulates the situation neatly. There are only three different colour receptors (‘cones’)  in the human eye. By having the ‘red’, ‘green’ and ‘blue’ cones stimulated differently, one sees different colours. The CIE chart puts all possible colours onto a 2d grid. One defines the variable ‘x’ as being the fraction of the total stimulation that is accounted for by the red cones; the variable ‘y’ as the fraction of the total that is accounted for by the green cones. (One could define ‘z’ in a similar way for the blue cones, but it is redundant since x plus y plus z must equal 1.) Then ‘x’ and ‘y’ defines a colour. The chart shows it. 

All possible colours are shown on this chart. The outside of the curved space shows the colours of the spectrum – those stimulated by a pure wavelength of light. The others are due to combinations of wavelengths. At x=1/3, y=1/3 (and so z=1/3) there is white. It isn’t possible to go outside this chart, and therefore it contains all possible colours. D’oh.

But, there is hope. The response of the green cones of the eye is entirely overlapped by those of the red and the blue. This means it isn’t possible to find a wavelength of light that stimulates JUST the green cones. If, somehow, one could stimulate cells artificially, one might be able to trigger green cones to fire without any response from red and blue. And then the person would be seeing a colour they’ve never experienced before. 

 

Seeing circular polarization Marcus Wilson Nov 22

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Physicsworld magazine is doing a ‘special feature’ this month on animal superheroes – those with rather unusual physical abilities.

The best of the lot (in my subjective opinion) is the featured-on-the-cover mantis shrimp. Not because of its ‘dactyl clubs’ that can produce a force of 700 N, but because of its eyesight.

The mantis shrimp can see circularly polarized light - something that no other animal is known to do. Polarization describes how the electric and magnetic fields in the light wave are oriented. For example, a horizontally-travelling light wave (say in the x- direction) might have its electric field pointing in the z-direction (vertically) and the magnetic field in the negative y direction. In an electromagnetic wave, the electric field, magnetic field and direction of travel are all mutually perpendicular. We could call that a vertical, plane polarization.

In circular polarization, the electric field moves in a corkscrew-like shape as the wave travels. The corkscrew can spiral one of two ways – hence there are two distinct polarizations which we call left-handed and right-handed. The mantis shrimp can distinguish between the two. It does this by using its own version of a quarter-wave plate – made of a birefringent material – one that has a different refractive index in different directions. That converts a circular polarization to a linear polarization, which it detects via more conventional methods. (There are several animals that can ‘see’ linear polarization – bees are a famous example. There are plenty that don’t distinguish one  polarization from another at all, such as humans.)

The mysterious question is why? Bees use linear polarization to assist navigation (light from the sky is linearly polarized), but what use is distinguishing left-handed and right-handed circular polarizations to a shrimp? There’s a cool research question for someone’s PhD thesis.

 

Pinhole cameras and eclipses Marcus Wilson Nov 15

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Well, the eclipse yesterday was fun. There were enough patches of sky between the clouds to get some good views. I was pleased that the pinhole cameras I made out of miscellaneous cardboard tubes, tins, paper and tinfoil worked really well. Also, the trees around the front of the sciences building gave some nice natural pinholes as the sunlight worked it’s way through the gaps between the foliage – we could see lots of crescents projected onto the wall of the building. Not something you see everyday.

The trick with the pinhole camera is to get the combination of length between pinhole and screen and size of pinhole correct. (Basically – the f-number in photography-speak) A long length means a larger image – but also a fainter one. To increase the brightness, we need to let more light through (a bigger pinhole) but the drawback of this is that it blurs the image. It takes a bit of experimenting – best done well before the eclipse that you want to see.

On the subject of which…if you live in New Zealand…you don’t have a lot of opportunity for a while. We northerners get an iddy-biddy eclipse next May (10th) – sorry Mainlanders – you miss out – and then it’s nothing for ages before we get a few more feeble partials in the 2020s. BUT, as I said earlier, it’s then non-stop eclipse mayhem from 2028, with THREE total and THREE annular eclipses before 2045, for those of us who are still alive to see them. Details are all here courtesy of RASNZ.

There are a few videos up already from the Cairns region – here’s one. However, video does not do an eclipse justice, partly because of the difficulty in video capturing parts of the corona at different luminances simultaneously. If you want to see the fainter, whispy stuff at the far edge of the corona, you end up well overexposing the brighter area nearer the moon.  The naked eye does a far better job of capturing the totality phase than a camera. 

http://www.youtube.com/watch?v=CTbIufApsSk

I note a fair amount of pink on the video – this is the chromosphere – a thin, cooler area of the sun, between the photosphere (the bright yellow bit that we normally see) and the corona.

 

 

 

 

Pepper’s Ghost Marcus Wilson Nov 01

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 Have a good look at the photo. The pretty rhododendron to the left of the chair looks a bit odd. That’s because it’s a ghost shrub. No, our garden isn’t haunted, and neither have I doctored the photo; it’s an example of Pepper’s Ghost – an illusion caused by reflections. The bush in question is off to the right, out of frame, and the camera is seeing its reflection in the window. Because the bush is well lit, but the background isn’t, it appears to be ‘real’. The effect looked even more stunning with polarizing sunglasses on.

 

 

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Distant galaxies and hobbits Marcus Wilson Oct 01

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I haven’t read ALL of Tolkien’s work, but I suspect space-travelling hobbits don’t feature anywhere. However, what do feature are hole-dwelling hobbits, and I had the fun of seeing their holes in the countryside near Matamata yesterday. The original set for Lord of the Rings was mostly removed after filming, and rebuilt for the filming of the Hobbit trilogy.  (Trilogy? Since when was The Hobbit a trilogy? This is just milking money out of Tolkien fans, isn’t it?) But this time the set will remain, for all to see, for an appropriate fee of course. It certainly was fun to have a look around – what made it was the commentary provided by our excellent guide.

One of the fascinating things pointed out was the perspective tricks that were used. For The Hobbit, there are three different versions of some of the holes.  One, a ‘large’ version, appropriate for a normal-sized actor, dressed as a hobbit, to walk through. One, a smaller version, to make the dwarfs look bigger than the hobbits. And another, an even smaller version, to make Gandalf look bigger than the dwarfs. And the three had to be identical.

And then there are the perspective tricks. To make the view look like it is over a longer distance, the more distant holes are of smaller size than the nearer ones. On a 2d movie it works – your mind interprets what you see as being of equal-sized holes spread over a larger distance. But being there in 3d you see it more as it is.  

That’s the problem that’s faced when determining the distance to distant stars and galaxies. Just how far are they away?  The moon, and anything further away, we perceive as 2 dimensional. We can’t get any 3-dimensional cues and so we have no idea, just by looking, of how far away they are.  So how can we measure distance to the stars? 

One way, which works for the nearest stars, is parallax. The earth orbits the sun, and six months from now it will be about 300 million km away from where it is now. That gives a different viewpoint. The nearest stars, therefore, appear to move against the background of stars that are further away. We can therefore use a bit of simple trigonometry to work out the distance to the star. Indeed, one of the units of distance in astronomy is the parsec – one parsec being the distance over which the diameter of the earth’s orbit subtends a parallax angle of one arc-second.  Essentially, using parallax in this manner is like viewing the situation with two eyes – 300 million km apart.

Parallax, however, only works for our nearest stars, since the distances to our neighbours are so huge. To work out distances further away, there are other methods – such as looking at the intensity of Cephid Variable stars, and, for really long distances, the famous redshift. However, somewhat disappointingly, neither of these are exemplified by the Hobbiton movie set.

Time travel Marcus Wilson Aug 24

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On Monday evening this week I managed to do a bit of time travelling while driving back home. I was driving back through one of those heavy showers that have been marauding around the place recently, with windscreen wipers full pelt on a rather wet road. However, these showers don’t last for very long, and the rain soon began to ease. As it did so, I noticed the road was getting drier.  Then the rain stopped all together, and I was left driving on an absolutely dry road.

That’s not what usually happens. Usually, the more rain there is, the wetter the road gets. I’m sure you’ve worked out what was happening.  I was heading in the same direction as the shower, but going faster than it. So I had overtaken it, as it were, and emerged from the rain ahead of the shower. There was a dry road, because the shower hadn’t got there yet.  Sure enough, I got home in the dry but within a few minutes it was raining – the same shower that I’d just driven through.

So I was experiencing the events of the rain shower backwards, because I was travelling faster than it. In one sense it was time travel. I was seeing events happen in a different order from what someone stationary on the ground would have seen.

Of course, it wasn’t really time travel. My clock was still going forward, as was everyone else’s. Now, if I’d been travelling faster than light, things might have been a little different. Special relativity says that time slows down for an observer travelling quickly  (from the point of view of someone who isn’t).   As this traveller approaches the speed of light, special relativity says that the passing of time for him becomes very slow indeed. In fact, at the speed of light, time wouldn’t pass at all for him. That’s one of the reasons that photons, light ‘particles’, behave very oddly.

What about beyond the speed of light? Physics as we know it doesn’t let us go there, not even with those neutrinos at Gran Sasso. If that result had been true, our understanding of physics would have been shaken up quite severely. The possibility of really travelling backwards in time might then have become a reality.

[ For those who are more mathematically inclined, the rain shower's also an example of why the partial derivative is not the same as the full derivative.  The full derivative for the rate of change of road wetness with respect to time was negative here - the road was getting dryer as I went alogn, but the partial derivative of road wetness with respect to time at constant position was still positive.  ]

 

 

Equipment failure Marcus Wilson Aug 13

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In the last couple of weeks, I’ve been working with one of our technicians tracking down what has been going wrong with one of the experiments we get our third year physics students to do. It’s on Brownian Motion. Specifically, analyze the movement of small particles suspended in water by scattering of laser light. By studying the way in which the scattered light varies in intensity with time, we can work out the size of the particles in the suspension.

So says the theory. However, in practice the pattern of scattered light is nothing like what we’d expect in this situation. There was clearly something going wrong, but working out what hasn’t been straightforward.

In the end, we just went through piece by piece through all the equipment, and the interfaces between the equipment, checking each was doing what it should have been. In the end Stewart worked it out – we had a dodgy oscilloscope. It’s rather easy to trust your instrumentation, especially that you’ve paid a lot of money for, but it is worth remembering that sometimes it breaks, and, when it breaks, it might not do so in a manner that is obvious. A piece of equipment that spits out the dummy and refuses to do anything is rather less dangerous than one that, on the face of it, is doing its job, but actually is getting it wrong. In this case the consequences of the fault are hardly serious – we’ve just had an experiment that was clearly giving puzzling and unbelievable results. In fact, for the last couple of years, I haven’t had the students even attempt it, because I’ve known something’s been amiss with it. However, that’s not always the case.

There are similarities I think with those faster-than-light neutrinos that hit the headlines last year. It was a crazy result – hence the attention – but on the face of it the experimental results appeared to be real. But, very careful checking of the apparatus highlighted a couple of glitches with the equipment. It wasn’t doing exactly what it was supposed to be doing. The problem was small, but it was big enough to produce a sensational result.

Fortunately, science has ways of correcting itself, and in due course the problem was tracked down by some careful investigation. It’s interesting that this is a skill we often overlook in teaching our students. In an effort to illustrate the theory, we present them with experiments that actually work (or at least try to). We never (certainly not here) deliberately give students dodgy equipment and then teach them how to find out what’s going wrong. Given that it is a skill that any experimentalist needs to have, it should be one we teach. Something to try in the future with another class of guinea pigs.

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