World's smallest solar panel, or should that be wire?US scientists have taken solar cell technology a step further with the development of the solar nanowire - a solar device 200 times smaller than a human hair.
21st Oct 2007 Scientists mussel-in on sticky surfacesUS reseachers studying how mussels anchor themselves to rocks, stones and jetties have stumbled upon a trick that can chemically coat any surface with something so sticky that it will even bind to Teflon. "We were able to remove mercury from water by passing it down a column containing beads treated with our polydopamine coating," says Messersmith. "So this could be very useful in cleaning up water in countries with heavy metal pollution." 21st Oct 2007 Researchers get to the bottom of coral clockWorking on the Great Barrier Reef, researchers at the University of Queensland in Australia have lifted the lid on one of the great marine mysteries of our time - how corals synchronise their spawning and ensure that it takes place on just a few nights of the year and always when there is a full moon. They found that the genes encode proteins which respond to blue-green light, which fits perfectly because water absorbs red light very strongly. Then, by growing coral samples in tanks with either a normal light-dark cycle to simulate day and night, or by keeping the coral just in the dark for an extended period, the team found that the levels of the genes peaked in the daylight and dropped off in the dark. Next they collected RNA samples from corals on the reef when there was a full moon, and again when there was a new moon (i.e. no moon) and compared the levels of the two genes. Intriguingly at the time of the full moon the levels of one of the genes - cry2 - were much higher, suggesting that this gene is the linchpin which links the coral's behaviour to moonlight and therefore the spawning pattern. 21st Oct 2007 Magnets and TVsIn a 'only do at home if you don't like your TV' experiment find out what a TV has in common with a particle physics experiment. What you needAn old fashioned CRT TV or Monitor (one of the ones that are almost as deep as they are wide) One that you are not overly attached to as there is a possibility this may permanently damage the picture. A magnet, the stronger the better the effect. What to DoTurn on the TV or monitor and tune it into a picture. If you can lift the TV comfortably turn it upside down very carefully, and see if it has any effect on the picture. The take your magnet and move it close to the TV, move it around, what effect does it have. Warning: The second part of this experiment may permanently damage the colour on some TVs - you have been warned so don't do it on a TV that is important to you! What may HappenYou will find that if you turn the TV upside down the colours will go strange. If you turn the TV off and on while it is upside down they go back to normal. If you put the magnet near the TV, if it is strong enough you will see strange patterns appearing on the screen, that move with the magnet.
What is going on?To understand what is going on you have to understand how a CRT (Cathode Ray Tube) TV works.
The beams of electrons are scanned across the screen very quickly and as they do this they are turned on and off by the signal sent from the TV station. This allows them to build up a picture of your (least) favourite celebrity on the screen. What is the magnet doing?A magnetic field deflects the electrons so they end up going to the wrong place. This has the effect of both moving the whole picture and sometimes moving the electron beam that should be forming the red part of the picture onto another colour, so everything looks the wrong colour.
Magnets are so good at deflecting electron beams that electromagnets near the electron guns are used to scan the beams across the screen to form the picture. It is very hard to get the steering electromagnets to bend the beams through a large angle accurately which is why CRT TVs have to be so deep and take up so much space. Why does turning it upside affect it?The earth has a magnetic field, and the TV is set up to expect this, when you turn the TV upside down the magnetic field is coming from the wrong direction and so it is just like putting a magnet near the screen, the picture moves slightly making the picture go a bit strange. How can magnets damage the TV.
Why does turning the TV off and on affect it?When you turn the TV on you will probably hear a mixture between a thump and a buzz, this is caused by the degaussing coil. This is an electromagnet which is made to apply a large magnetic field that is changing too fast for the metal in the mask to keep up with it, and has the effect of demagnetising the metal so it cancels out the earth's magnetic field. So with any luck it will fix any damage you have done. What has this go to do with particle physics?First of all electrons are sub-atomic particles, the same sort of thing that are created at CERN and other large particle physics experiments, although mostly they make more exotic particles. Also in CERN they do exactly the same experiment as you have just done in order to identify particles coming out of the collisions. The detectors apply a magnetic field to the particles, which makes them travel on a curved path if they are charged. If you know how much energy they have how curved these paths are tells you how heavy the particles are and so helps you find out what they are. Why is an old fashioned TV called a Cathode Ray tube?Beams of electrons are emitted from the -ve electrode which is also known as the cathode so the beams are also known as cathode rays. 'Tube' is just a contraction of vacuum tube, as the whole of the TV has to have the air pumped out to stop it interfering with the electron beam. Valves which are also a form of vacuum tube were fundamental to the first forms of electronics in the beginning of the 20th century because you can interfere with the progress of electron beams by applying electric and magnetic fields, so you can use them to amplify signals and other cunning things. So valves were used to amplify the radio signals in both radios and TVs before transistors were invented.
The Brightest Diamond; Synchrotron, that is...Richard Walker & Sanjeet Dhesi, Diamond Synchrotron; Tim Wess, Cardiff UniversityEarlier this week, HM the Queen and the Duke of Edinburgh opened the Diamond Synchrotron in Oxfordshire. Now this very expensive device creates very high energy electromagnetic radiation (that’s known as synchrotronic light) and it’s filtered to give you and extremely intense x-ray beam which is hundreds of times more powerful that the one you’d get in hospital. We sent Meera down to the site this week to find out how it works and the benefits of using such high-energy light. Meera - Hello, this week I’m at Diamond Light-Source out at Didcot, Oxfordshire to find out about the giant particle accelerator located out here known as the synchrotron. Now the building itself is huge, silver and doughnut-shaped. And to give you an idea of just how big it is, it apparently covers the area of five football pitches. What I’m here to find out about is, ‘what is a synchrotron, what does it actually do and how does it work?’ I’m also going to be finding out just how this technology is being used to benefit everyday life and even to uncover ancient messages hidden in parchment such as the Dead Sea Scrolls. To answer the first of my questions is Richard Walker who’s the Technical Director of Diamond Lightsource. We’re actually here inside the synchrotron now. What exactly is a synchrotron?
Meera - We’re inside the synchrotron itself, where are we standing? Richard - Well, we’re actually stood in the linear accelerator which is the first part of the acceleration system. Right at the beginning, where the electrons come to life and they’re liberated from the atoms in an electron gun. The electron gun fires the electrons into the linear accelerator where they’re accelerated up to 100 million volts. From there they’re transferred into another synchrotron, a booster synchrotron where they’re accelerated up to the final energy of 3000 million volts before they’re injected into the storage ring. Meera - They’re bent round. Is this done using magnets? Richard - We use a large array of electromagnets, both to bend the electrons that form the circular orbit and also to focus them and keep them very tightly compressed. It’s the small size of the electron beam that gives rise to very bright synchrotron light that we want to generate and use in our experiments. Meera - So now I know how the synchrotron actually runs, but what benefit does this high beam of light actually provide? I’m with Sanjeet Dhesi who’s a principle beam-line scientist here at Diamond. What, exactly, is a beam-line? Sanjeet - A beam-line is a series of x-ray optics that helps channel the light that’s produced in the machine all the way down to the sample where we have an electron microscope that we use to study anything from magnetism to chemical reactions on a surface. Meera - So we’re outside your nano-science beam-line now. What is this in front of us? How is this beam line being channelled? Sanjeet - If you take light into a camera you use a series of lenses to focus the light onto your film. If you try to do that with x-rays, the x-rays just go straight through the lens. Instead of using lenses you have to use mirrors. The beam-line is actually a series of half a dozen mirrors that take the light and channel the light and focus the light down to our sample where the light is only a tenth of the width of your hair but it has about 1000 billion times the intensity of a hospital x-ray source. Meera - How many beam-lines are there here at Diamond? Sanjeet - In phase 1 of Diamond there were seven beam-lines that were constructed. You can do anything on a beam-line from looking at the structure of a protein to understand how a virus attacks your body to looking at structures under extremely high pressure and extremely high temperatures. That’s important, for instance, for understanding how iron behaves at the Earth’s core. There’s a whole host of ways that x-rays interact with matter to work out exactly what’s happening at the fundamental level of the atomic scale. Meera - So extremely variable fields of science are being explored using this synchrotron light but it’s not only science that’s benefiting. Scientists are also trying to learn more about history. Professor Tim Wess and his team at Cardiff University have been using synchrotron light to understand the texts of ancient parchments such as the Dead Sea Scrolls: potentially enabling them to read the scrolls without having to unravel them. I’ve got Tim here with me now. Hello Tim. Tim - Hello Meera. Meera - What made you start working with ancient parchments? Tim - Well, what a lot of people don’t actually know is that parchment’s actually made out of dried skin and therefore that’s made out of collagen. I’ve been working with synchrotron radiation to understand the structure of collagen for about the last 20 years. What we’ve been trying to do is see how intact the collagen is in a piece of parchment because what happens to parchment as it gets older and the control mechanisms of repair are lost when we’re looking at something which is no longer in an animal, you begin to see that the collagen deteriorates into gelatine. Collagen is really like a little rope molecule which really gives us the strength in our tissues, tendons, our bones and our skin. When it deteriorates into gelatine usually in our body it’s taken away and recycled but in a document like an historical parchment the gelatine just sits there. It’s lost its strength; it likes to take up water which means the gelatine actually becomes a jelly. Therefore, the parchment becomes very fragile, brittle and very, very difficult to unfold and read or handle. Meera - So how are you using synchrotron light to overcome this problem?
Tim - First of all, we can begin to detect without hopefully damaging the piece of parchment how intact it is. Using the synchrotron, we have a very fine beam of x-rays we put through the parchment sample. The way that the x-rays interact with the matter tells us about the state of the matter that’s present. We get a very distinct signal for the way the x-rays are scattered with collagen and a different one for gelatine. We can begin to tell the difference between those two and then advise on the collagen-to-gelatine ratio in any of these samples. We have looked at the Dead Sea Scrolls here using the scattering to try and understand the damage that’s occurred to the Dead Sea Scrolls because what we’re finding is that the caves that the different samples were coming from seem to have affected how stable they are and how they’ve managed to stay intact. When we find that a sample has been so badly damaged that it shouldn’t be displayed or unfurled, there’s a second approach with the synchrotron that we can begin to use which really relates to a process called tomography. We pass an x-ray beam through an object then the picture we get depends on presence of things like writing on the surface of the parchment so from that we can take lots and lots of pictures at different angles of the piece of parchment. Whether it’s a rolled up piece of parchment as a scroll, we can then reconstruct on a computer from all the different absorption patterns that we have what the original object was. And that’s where we’ve begun to realise that using the ink on parchment, on the surface of it, we can read objects which we would really not be able to unroll. Meera - So there you have it. Irony at its best. This giant silver doughnut is enabling scientists to probe matter down to tiny atomic scales and this extremely new technology is going to provide answers to questions and beliefs that go back thousands of years.
October 2007 Inside the AtomDr Ben Allanach, Cambridge UniversityChris - We’re looking at the origins of the universe, what’s inside matter, what are atoms made of this week. Let’s kick off by talking first of all to Ben Allanach, a theoretical physicist at the University of Cambridge. So when we’re talking about atoms I think even the ancient Greeks (sort of Democritus’ time) had a concept of the atom, as this tiny particle which you can link lots together and you’ve got something. How do we actually know what’s inside them? Ben - A hundred years ago Earnest Rutherford, down in the Cavendish lab, here in Cambridge fired radioactive particles into atoms and you can tell from that roughly speaking what’s going on inside. One in about every eight thousand of these particles came back at him. He measured those with a Geiger-Counter. That led him to completely throw away the model at the time which was the ‘plum pudding’ model of some sort of squishy stuff which was positive with little electrons dotted around it. What he realised was that most of the atom is actually empty space, with light electrons flying around the outside. Inside there’s a very small, hard, dense core called the nucleus. Chris - It’s interesting, what you say about the empty space Ben, I’ve got an email here from Jack Dao who says, ‘Hi guys I’m listening in Brooklyn, New York and I like your program. I’ve heard there’s a vast empty space between the orbiting electrons and the nucleus of an atom but I’ve been told that if all the empty space was taken away so that every single electron touched another electron and the nucleus then the size of the world would theoretically be the size of a melon. Ben - That could actually be true. I’d have to do a calculation on the back of an envelope to be absolutely sure but it is a huge amount of space and the particles inside are tiny. Chris - What are the actual particles that make up an atom? Ben - Around the outside you have electrons, they’re light, negatively charged particles and inside you have the nucleus which is made up of protons and neutrons. They’re kind of heavier stuff that stick together quite well. Chris - And how big are these things? Ben - An atom is roughly 10-10m so that’s a tenth of a billionth of a metre across and the tiny constituents in the middle are almost a million times smaller than that so they’re just unimaginably tiny really. Chris - And the nucleus is positively charged because it’s got the protons in it and the electrons are negatively charged. Now I can understand why the electrons would be clung-on to by the positive core of each atom. Why is it that all those protons with that big positive charge can be stuffed together and they stay there? They don’t fly apart… Ben - There’s an additional force keeping them together that’s called the strong nuclear force. They’re stuck in there with neutrons as well and this thing just sticks them together. Chris - And so how do we work out what the different atoms are because if I’ve got an atom of oxygen which I’m breathing, how is that different from say the atom of carbon that I’m burning to make the energy in my body? Ben - You can weigh them through indirect means and you can work it out through chemical reactions and so on to work out how many of the different atoms make different substances up. Kat - Delving a bit more deeply into the structure of matter, you hear about things like quarks and neutrinos and all these kinds of things. How do they fit in and how do we know that they’re there? Ben - Well, as far as we know they’re the smallest bits of matter and so if we go deeper into the nucleus, for instance, every proton and neutron is made up of three smaller particles and they’re quarks. They’re stuck together with this strong nuclear force so by breaking up protons you can actually detect these things indirectly.
Ben - That’s right yeah. So Rutherford’s initial experiments of the radioactive atom are now being done at much higher energies in order to delve deeper and deeper into the protons. Kat - So tell us a bit more about what you’re doing. I sort of understand it as you do the maths and then the particle accelerator people try and work out if it’s right or not. Ben - Yeah, it gets a blurred around the edges though. We both do bits of each other’s jobs. That’s right, I do a lot of theory and there’s a lot of sums. I try and work out models of the early universe to explain facts about the universe that you see today and then most importantly, to work out ways of testing these theories by looking at the data coming out of the experiments. Kat - So this is working out what you should see if you smash two particles together? Ben - If the theory is right, yeah. Chris - So why do you want to smash things together? How does that actually help? Ben - Because we can’t actually see with the naked eye or even with a microscope we can’t actually see these particles. They’re much too small so the only way to probe them at all is to have something very high in energy that breaks them apart and you can see what they decay into, for instance. You can get a picture of what happens after those collisions. That’s the only way you have, really, of probing them. Chris - What’s new about the large hadron collider? What have we done in the past and how does this differ? Ben - Plenty of different collisions have been happening in the past and basically the energy gets higher and higher and higher every time. In Einstein’s equation E=MC2, if you’re got more energy you can make heavier particles. So particles that were previously undiscovered, when you pass an energy threshold, all of a sudden you’ll be able to produce them. That’s what’s hoped particularly for the Higgs boson hypothetical particle that’s hoped will show up there. Chris - So up until now people have been slamming things together the same way as they will do in the LHC but now they’re gonna be able to do it even more powerfully? Ben - Yeah, basically that’s right. The technology’s come on a lot and that’s why they’re able now to do such high energy collisions. Kat - Where’s this gonna stop? If we’ve got this new, exciting, huge particle accelerator, what if you do some sums you’ll find some evidence that means you’ll have to build an even bigger one to get even higher energies? Do you think that the LHC would be the answer to everything? Ben - Not necessarily. You might need to build one more, actually. Kat - An even bigger one? Ben - Well, it won’t necessarily be bigger. Chris - Don’t these things consume energy on the scale of a national grid just for one experiment? Ben - It’s not as much as that, actually. It is a lot of power, its 100MW or so. Chris - That’s about 20% of a reasonable nuclear power station. So that’s quite a lot isn’t it? Ben - It’s a lot of power so you do have to weigh up the cost of these things and decide whether the science you’re gonna get out of it is actually worth the cost. It was decided, and I think rightly, that for the LHC, the answer to that question is yes. It will be that that decides whether the next one is built. October 2007 The Search for Sub-Atomic BeautyDr Cristina Lazzeroni, Birmingham UniversityChris - Now we’ve heard from Ben Allanach about some of these collisions and the huge energy that are going to be produced. Presumably from those collisions there are particles produced or evidence that particles get produced so we can try and understand what’s inside atoms. What are you actually looking for in your experiments?
Chris - So what you’re trying to do is to simulate, in a laboratory environment, the Big Bang? Cristina - Kind of. Chris - So you’re turning a pinpoint of energy into the stuff, the matter that is the stuff we see around us today. Cristina - Yes, that’s quite the idea, yes. Chris - I guess the question is though, is that safe? Are we going to spawn a new universe in CERN in Geneva where people do say it’s the centre of the universe in some respects but is that a good idea? Cristina - Yes it is actually, it’s a very good idea and no, we are not creating an entire universe. Previously, for example in CERN, we have been smashing particles together for years. In fact, CERN has been celebrating its 50th year quite recently. Nothing of such catastrophe ever happened. There are reasons for that. The idea that we’ve got higher and higher energy is because we want somehow to go more and more back in time. We want to see the particles that were produced farther back in time. That doesn’t mean that it’s dangerous because these particles live so shortly and is not dangerous in itself that there will be no harm for anybody. Chris - How can you really have faith that you’ve recreated what was going on at the Big Bang? Cristina - Let’s be honest, we will not create the exact condition of the Big Bang but what we want to do is to get a very similar condition as much as we can. That doesn’t matter if it’s not a perfect condition to try to understand how these particles were formed and the new particles that may come over and try to build more complete pictures from that. Chris - So, theorising for a minute and straying into Ben’s territory – what do you think actually happened then, when the universe was born? There was a lot of energy around then so can you just talk us through what you think, on paper at least, probably happened? Cristina - Right, yes at the very beginning we think that there was a new state of matter which is called Plasma. This, in fact is one of the main topics of one of the experiments at LHC. You know that in quarks, quarks are confined in protons and neutrons so in fact we never see quarks free so far. We see protons and neutrons but not quarks. We believed at the very beginning there was such a hot and dense state of matter that the quarks were actually free. So it’s all together some sort of big, hot and dense soup of quarks and gluons. From there the things started to freeze out and our model has to be somehow the kinds of studies that we do with gases and with liquid, that sort of thing. At some point somehow matter formed as atoms. Also light was released and went out forever. That is what we observed. From atoms we got bigger matter and so on. Chris - So when you designed an experiment for the LHC as it will be, when it switches on next week in CERN, what’s going to be happening is a stream of protons is gonna be whipping round this circle (27km long) at nearly the speed of light. Tremendously high energy and that beam will then be brought into collision course with a second beam going the other way. The two will then cannon into each other at a point, presumably you know where that collision will happen. So what are you looking for? Cristina - At that point, in fact, there’s going to be four places of collision along the ring. We place at these collision points some huge cameras. They take almost photographic pictures of what’s going on. So from these pictures you try to use some sort of forensic science to go back and see from the traces that they left in the detector what was actually happening in the first collision. Chris - That doesn’t sound too complicated. The price tag is huge. How long are you going to have to do this for to see the kind of evidence that you need to know what’s going on? Cristina - Well, it depends what people are looking for. If you look for very rare processes, for things that you know are very, very rare you have to look for longer. There might be other things that you spot immediately. We hope to see the Higgs boson quite fast but, you know, you never know until you see it. Chris - Ben mentioned it; you mentioned it. What is the Higgs boson? Cristina - The Higgs boson is supposed to be the thing that gives everybody mass so we could imagine it’s a sort of gelatine that fills the space. The bigger you are the bigger resistance this gelatine offers to you. So somehow the Higgs mass is this sort of gelatine that fills up the entire space. Somehow it gives you more mass because it gives you a measure of the resistance that you have going through it. Chris - So this is what Ben tells us should exist? Cristina - If it doesn’t exist in fact, the whole theory needs to be revised quite fundamentally, yes. October 2007
RNA-away HepatitisScientists in the US have uncovered how the body tackles certain viral infections, and the results might help to produce better ways to treat Hepatitis C. Hepatitis C is a blood-bourne viral infection spread by needle sharing, use of contaminated blood products and by sex, and it affects about 1% of the population in the western world. 80% of individuals who catch it develop a chronic infection which causes liver injury and can lead to cirrhosis in about 20% of cases. Recently doctors have found that long-term therapy with a immune-regulating hormone called alpha-interferon can enable the immune system to overcome the virus and eliminate it from the body, although exactly how remained a mystery. This approach could hold the key to effective new therapies for hepatitis C in the future, and may also spare patients the unpleasant flu-like side effects of interferon therapy. 21st Oct 2007 When you've got to go...It's become traditional that Dr Chris nips to the little boys' room five minutes before every show, but scientists in Belgium have found a gene that may be partly responsible for the urge to spend a penny. Normally, when our bladder gets full, then this sends signals to the muscles around it telling them to contract, meaning a trip to the toilet is in order.
The TRPV4 gene makes a protein that sits in the wall of cells that line the bladder, and helps to send signals that tell the bladder muscles to contract. The researchers think that it has an important role in translating the signals that the bladder is full into muscle contraction that allows a controlled trip to the loo. Although these are just experiments in mice, there is the possibility that TRPV4 might be a target for treatments to help with bladder problems such as incontinence. 21st Oct 2007 |
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