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Do neutrinos move faster than the speed of light?

Can particles travel faster than the speed of light? Most physicists would say an emphatic “no”, invoking Einstein’s special theory of relativity, which forbids superluminal travel. But now physicists working on the OPERA experiment in Italy may have found tantalizing evidence that neutrinos can exceed the speed of light.

The OPERA team fires muon neutrinos from the Super Proton Synchrotron at CERN in Geneva a distance of 730 km under the Alps to a detector in Gran Sasso, Italy. The team studied more than 15,000 neutrino events and found that they indicate that the neutrinos travel at a velocity 20 parts per million above the speed of light.

Simple measurement

The principle of the measurement is simple – the physicists know the distance travelled and the time it takes, which gives the velocity. These parameters were measured using GPS, atomic clocks and other instruments, which gave the distance between source and detector to within 20 cm and the time to within 10 ns.

This is not the first time that a neutrino experiment has glimpsed superluminal speeds. In 2007 the MINOS experiment in the US looked at 473 neutrinos that travelled from Fermilab near Chicago to a detector in northern Minnesota. MINOS physicists reported speeds similar to that seen by OPERA, but their experimental uncertainties were much larger. According to the OPERA researchers, their measurement of the neutrino velocity is 10 times better than previous neutrino accelerator experiments.

‘Totally unexpected’

“This outcome is totally unexpected,” stresses Antonio Ereditato of the University of Bern and spokesperson for the OPERA experiment. “Months of research and verifications have not been sufficient to identify an instrumental effect that could explain the result of our measurements.” While the researchers taking part in the experiment will continue their work, they look forward to comparing their results with those of other experiments so as to fully assess the nature of this observation.

Although a measurement error could be the cause of the surprising result, some physicists believe that superluminal speeds could be possible. Its discovery could help physicists to develop new theories – such as string theory – beyond the Standard Model of particle physics. However, the OPERA measurements will have to be reproduced elsewhere before they are accepted by the physics community.

Jenny Thomas of University College London, who works on MINOS, said “The impact of this measurement, were it to be correct, would be huge. In fact it would overturn everything we thought we understood about relativity and the speed of light.”

Alexei Smirnov, a high-energy physicist at the Abdus Salam International Centre for Theoretical Physics, Italy, says that he finds the OPERA result “extremely surprising” as while some small deviation could have been expected, the observed deviation is very large – much larger than what is expected from even very exotic theories. “If this result is proved to be true, the consequences for modern science would undoubtedly be enormous,” he says. He agrees with the conclusion of the OPERA collaboration that currently unknown systematic effects should be looked for and they should continue observations. Smirnov was one of three researchers who discovered the “matter–mass” effect that modifies neutrino oscillations in matter.

Talking about neutrinos

On Friday afternoon, OPERA researcher Dario Autiero from the Institut de Physique Nucleaire de Lyon discussed the details of their experiment at a seminar at CERN. Autiero addressed possible reasons for the result that took into consideration everything from inherent errors during calibration of clocks, to tidal forces and the position of the Moon with respect to CERN and Gran Sasso at the time of the readings.

They considered the possibility of problems internal to the detector itself, the chances of which OPERA researchers say were reduced thanks to the independent external calibration methods they used. They also discussed if it would be possible to re-create the results at different energies. “We don’t claim energy dependence or rule it out with our level of precision and accuracy,” said Autiero. The final note of the seminar seemed to suggest that the real reason is indeed a mystery for the time being and further analysis will definitely be required.

The discovery is described in arXiv:1109.4897 (PDF).

Electrons surf between qubits

Two independent groups of physicists have taken an important step towards the creation of a practical quantum computer by showing how to transfer single electrons over relatively long distances between quantum dots. Both schemes involve using sound waves on the surface of a material to propel electrons between the quantum dots – which are sub-micron-sized pieces of semiconductor. The teams are confident that they will soon be able to show that electrons arrive at their destination with their quantum information intact, making the system a viable “quantum data bus” for a quantum computer.

Quantum computers, which exploit purely quantum phenomena such as superposition and entanglement, should in principle be able to outperform classical computers at certain tasks. But building a practical quantum computer remains a challenge because the physical entities that store and transfer quantum bits (qubits) of information are tricky to implement and are easily destroyed.

The advantage of using quantum dots as qubits is that they can hold zero, one or two electrons, thereby defining the “logic state” of the qubit data. Furthermore, two electrons in a dot are entangled – a condition that persists even if one electron is carefully removed and transported some distance away. This process, which is known as “quantum teleportation”, can play an important role in quantum computers.

Avoiding decoherence

While physicists can reliably transfer a single electron short distances between adjacent quantum dots, moving it around an integrated circuit containing hundreds or thousands of qubits is a significant challenge. The problem is that an electron in a metal or semiconductor travels through a vast “sea” of other electrons that can destroy the entanglement. One way to avoid this “decoherence” is to essentially drain the sea of electrons from the appropriate channels in the circuit – effectively making them insulating. The challenge is then how to give the electron enough energy to send it flying through the channel without causing decoherence.

Now, however, Tristan Meunier and colleagues at the Institut Néel in Grenoble, the University of Tokyo and the University of Bochum in Germany – and, independently, Rob McNeil and colleagues at the University of Cambridge in the UK – have devised a way to deliver that kick. Both teams fabricated similar semiconductor devices, each with two quantum dots separated by several microns. In both cases the dots are connected by a narrow semiconductor channel between two electrodes.

To deplete the channel of all its conduction electrons, both teams applied a negative voltage to both electrodes. The kick is supplied by a piezoelectric actuator that injects a surface acoustic wave (SAW) pulse along the channel. A SAW is a sound wave that travels on the surface of a material, where it causes the positive ions in the channel to oscillate back and forth. The result is a changing electric field that drives the electron forward.

Extremely fast transfer

Meunier and colleagues employed one piezoelectric actuator, which was able to drive an electron the 3 µm between the two dots in just 1 ns. This is much quicker than the several microseconds it takes for decoherence to destroy a quantum dot qubit, something that is essential for a practical quantum computer, according to Meunier. Meanwhile, in Cambridge, McNeil and colleagues used two opposing piezoelectric actuators to bounce an electron back and forth between quantum dots separated by 4 µm. Indeed, McNeil said that they were able to do this up to 60 times, which means that the electron travelled a total of 0.25 mm.

Both experiments were carried out at extremely low temperature, which means that there are few random sound waves in the channel that would cause decoherence. The SAW wave itself is coherent and should not destroy entanglement, according to McNeil. However, neither team has confirmed that the electron does not suffer decoherence on its journey – something that both labs are currently investigating.

The work of both teams is described in two separate papers in Nature.

Is Sheldon an inspiration or a grotesque parody?

By James Dacey

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Earlier this week US actor Jim Parsons picked up an Emmy Award for his portrayal of Sheldon Cooper, the socially inept physics postdoc, on the hit CBS TV comedy show The Big Bang Theory. Parsons picked up the award for “outstanding lead actor in a comedy series” at the awards ceremony in Los Angeles on Saturday night, as reported by my colleague Matin Durrani. A large appeal of the comedy smash hit stems from the relationship between Sheldon and his friends and colleagues (two other physicists and an engineer), and their interactions with “near-normal” neighbour Penny (played by Kaley Cuoco).

The idea of humour on screen being derived from a geeky scientist is not particularly new: Eddy Murphy in The Nutty Professor and Christopher Lloyd in the Back to the Future series are two obvious examples that spring to mind. But the thing that strikes me as novel about the Big Bang Theory is that the vast majority of the humour comes from the geeks’ responses to everyday situations, outside of their work. A rich source of humour, for instance, derives from Sheldon’s excessively analytical approach to social situations, where he is aware of what “people” do in given situations but he is not sure why.

On the one hand, it is refreshing to see that people have accepted Sheldon and his crew into their hearts and people seem to love him because all of his physics geekiness. But on the other hand, it is rarely clear whether we are laughing with Sheldon or at him. The extreme view is that Sheldon is a grotesque parody of a socially inept physicist who simply does not fit in with everyday life.

We’d like to hear your thoughts about this. Which of the following statements best describes your feelings about Sheldon?

He’s got me down to a tee!
He’s an exaggerated version of a physicist for comic effect
He’s a grotesque parody that insults physicists
Who is Sheldon?

Have your say by taking part in our Facebook poll. And please feel free to explain your answer by posting a comment on the poll.

Last week’s poll addressed the issue of money, given that the worsening economic conditions on either side of the Atlantic have kept fiscal affairs in the headlines of late. We asked you: “Can ideas borrowed from physics lead us to financial recovery?”

80% of respondents said yes and 20% said no. This suggests that there is still faith in the ability of science to predict “the madness of men”, as Newton once described stock trading after losing a lot of money in the South Sea Bubble. Luis Rico, one of the respondents who voted yes, believes that one of the main advantages of applying physics ideas to economics is “the lack of both political bias and conflicts of interest”. He believes that economics needs to develop more sophisticated systems to better reflect the real world. “Working with a single model of a complex system that has already proven to fail seems unnatural to me and the inability to question axioms makes impossible any real advance.”

Thanks you for all your responses. And check physicsworld.com next Thursday for the results to our latest poll.

Searching for a star

By Matin Durrani

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I learned earlier today that Lord Sainsbury – the former UK science minister – is launching a search for the UK’s “most inspirational technician”.

It seems a worthwhile initiative, given how important lab technicians are for the smooth running of science. (We can all probably speak from experience – I recall some fabulous technicians during my time at the Cavendish Laboratory in Cambridge, including Dick the glassblower, who once saved my bacon after I blew up a mercury thermometer that I’d left too long in a beaker on a hot plate. The beaker dried out and the thermometer exploded. Fortunately the embarrassing incident took place inside a fume cupboard and was not witnessed by anyone else.)

Supported by Sainsbury’s Gatsby Foundation and STEMNET – a charity that tries to get young people involved in science, technology, engineering and medicine (STEM) – the award seeks to recognize “the excellent work of technicians who inspire young people to follow technical careers” and to improve the image of a profession in “high demand by employers”. It is one of five categories in the National STEMNET Awards 2011, sponsored by the Science and Technology Facilities Council (STFC), the others being for best teacher, best employer, best STEM club and best STEM ambassador.

There is no limit to the number of categories you can nominate in and all finalists will be decided by an expert panel. The deadline for nominations is Monday 3 October – more information is available via this link

The top technician – and the other award winners – will win a day trip to the CERN particle-physics lab in Geneva, sponsored by the STFC. Winners will be announced at an awards ceremony at the House of Lords in December.

If he were alive today, I reckon in the running for an award would be veteran Cavendish lab technician Ebenezer Everett, who by all accounts did some fabulous work that played a key role in J J Thomson’s discovery of the electron in the late 1890s.

The reason I mention Everett is that I recently came across the following passage in Robin Strutt’s biography of Thomson, which appeared in the Cavendish magazine CavMag last year, concerning the switching on of a powerful electromagnet surrounding a discharge tube.

JJ: “Put the magnet on.”

There followed a click as Everett closed the large switch.

JJ: “Put the magnet on.”

Everett: “It is on.”

JJ: (eye still to the microscope) “No, it isn’t on. Put it on.”

Everett: “It is on.”

A moment later JJ called for a compass needle. Everett returned with a large needle 10 inches long. JJ took it, and approached the electromagnet. When about a foot away the needle was so strongly attracted to the electromagnet that it swung round and flew off its pivot, crashing into the bulb (which burst with a loud report) and coming to rest between
the poles of the magnet. Everett was glowing with triumph, and JJ looking at the wreck with an air of dejection.

“Hmm,” he said. “It was on.”

Neutrons for the future at the Institut Laue-Langevin

Since its reactor first went critical 40 years ago, the Institut Laue-Langevin (ILL) in Grenoble, France, has maintained it reputation as Europe’s leading centre for neutron scattering. In this audio interview, ILL’s scientific director Andrew Harrison explains how the lab is in the middle of a major upgrade that aims to maintain its position as one of the world’s leading neutron centres.

Neutrons for the future

This effort is particularly important now that construction of the European Spallation Source (ESS) in Sweden is set to get under way. The ESS is an accelerator-based facility that will offer a wide range of researchers, from biologists to engineers, neutron beams that are not available at ILL. However, Harrison insists that ILL will not become a white elephant when the ESS comes online in 2025 and explains how the two facilities will in fact complement each other.

Indeed, physicists at ILL have plenty of experience of working with other major science facilities because Grenoble is also home to the European Synchrotron Radiation Source (ESRF) and several other major research institutes. Harrison explains how this brings the best science and scientists to ILL and continues to encourage the development of other facilities in Grenoble.

The recent trend towards accelerator-based neutron sources, such as the ESS, is, however, leading to a fall in the number of research reactors worldwide, which is a concern to the medical community as it could threaten the supply of medical isotopes. Nevertheless, Harrison has some good news for medical physicists because, as he explains, the ILL has several pilot projects to look at how it could produce isotopes – particularly those that are not easily made elsewhere. Harrison also discusses how ILL is working with a commercial isotope supplier to work out how the institute’s high flux reactor could serve the medical community.

The flawed multiverse

According to the quantum-information theorist David Deutsch, our modern understanding of how the world works has provided us with "good explanations" that open up essentially infinite possibilities for future progress. One of these explanations is the idea of the quantum multiverse, which Deutsch discussed in the May issue of Physics World (pp34–38, print version only) and to which he devotes a chapter in his book The Beginning of Infinity.

In 1957 Hugh Everett III noted that if quantum mechanics is a universal theory, then it should be applicable to particle detectors, and indeed observers, as well as to individual particles. Consider an experiment where a photon interacts with a partially reflecting surface, and separate photon detectors are positioned to register transmitted and reflected photons. A straightforward quantum-mechanical calculation predicts that the resulting quantum state of this whole set-up should be a linear combination of one where the photon has been detected in the transmitted (but not the reflected) direction, and another where the reverse is true. Experimentally, of course, a photon is found in one or other of the detectors at random, with probabilities that depend on the properties of the reflecting surface.

To get agreement with experiment, we normally employ a further postulate, known as the Born rule, which states that a measurement causes the wavefunction of the system to "collapse", which means that only one of the above outcomes actually occurs. The relative probabilities of the possible outcomes are given by the modulus squared of the corresponding parts of the wavefunction.

However, Everett proposed that the collapse postulate is unnecessary, thanks to decoherence. Once a photon has been detected, its quantum state becomes entangled with the state of the detector, and to perform an interference experiment, coherence would have to be maintained for all the phases associated with the huge number of particles making up the detectors. This is a practical impossibility; so even though the two outcomes coexist, they cannot affect each other in any way. This means that both can continue while unaware of each other's existence. In other words, the photon has gone both ways, and the detectors and everything that interacts with them have two different futures: one in which the photon was reflected and another in which it was transmitted.

An inevitable consequence of Everett's theory is that this splitting occurs even if a human observer records the result of the experiment. The observer also evolves into a superposition of two states, each of which is completely unaware of the other, leading them to assume that collapse has occurred and only their branch exists. As Deutsch explains, this splitting spreads out from the experimental apparatus in what he calls a "wave of differentiation" until it eventually encompasses everything – hence the terms "parallel universes" or "many worlds".

Because the assumption of collapse is no longer required, it has been said that the many-worlds interpretation is "economical with postulates although extravagant with universes". This should surely be sufficient reason not to dismiss the idea out of hand. However, I believe the many-worlds theory is open to criticism for reasons other than extravagence. One of these concerns probabilities in a situation where both outcomes occur in parallel. If both options are happening, how can it be meaningful to say that one is more probable than the other – as is experimentally the case if the reflector is not exactly 50/50?

As he described in his Physics World article, Deutsch's response is to propose that before the measurement, the photon is not just a single particle but is actually an (uncountable) infinity of identical or "fungible" particles. After interacting with the reflector, an infinite number of fungible photons exist in both output channels, but the ratio of these numbers is finite, so that each has a "measure" proportional to the squared modulus of the wavefunction. Even though an observer knows they are going to evolve into two copies of themself, they can apparently assign relative probabilities to which copy they expect to become. These probabilities are given by the Born rule.

Whether Deutsch's fungibility formulation successfully resolves the question of probabilities is a moot point, but it seems to me that the multiverse concept raises another problem, which other supporters of many-worlds theories thought they had resolved some time ago. This is known as the "preferred basis" problem, and it arises from the fact that there is no unique way to express a quantum state as a superposition of two component states.

Consider a spin-half particle in an eigenstate of the x component of spin. This can be expressed as an equally weighted superposition of the positive and negative eigenstates of the z component – or of the y component, or, indeed, as an appropriately weighted superposition of any two linearly independent spin states. Together, these states constitute a "basis". Suppose now that we pass such a particle through an apparatus oriented to measure some component of spin. According to the multiverse model, before the measurement, the ratio of the (infinite) numbers of instances of the particle that will appear in the two possible output channels corresponds to the relative probabilities given by the Born rule.

However, this ratio is a function of the direction chosen for the measurement, so the initial state of the particle must depend on the nature of the measurement that is still to be performed. Choosing the basis beforehand to suit the properties of the subsequent measurement seems to me to destroy the objectivity of the description of the initial state and, indeed, of the multiverse. This process also implies an additional assumption, which means that we have lost the multiverse's economy with postulates, while the extravagance with universes remains. Deutsch appears to recognize this difficulty to some extent; he indicates that it is related to the quantum electron "field", but he does not explain how this could resolve the problem.

Deutsch's belief in the existence of the multiverse inspired his ground-breaking contributions to quantum computing, and he believes that a successful implementation of a quantum computer would constitute incontrovertible evidence for it. He argues that the reason a quantum computer can carry out some tasks very much faster than a classical one is because the former performs a large number of calculations simultaneously in parallel universes. However, I believe that this idea is also challenged by the preferred-basis problem.

To see how, let us take as an example the quantum Fourier transform, which is the core operation in Shor's algorithm for efficiently obtaining the prime factors of large numbers using a quantum computer. This operation subjects a set of qubits – quantum objects such as spin-half particles that have two possible states – to a series of "unitary" operations, which in the spin-half example amount to subjecting the spins to a series of rotations. This creates an entangled state that is a linear superposition of binary representations of the components of the Fourier transform of whichever function was represented by the original configuration of qubits. These separate components certainly form a basis, but there is no obvious reason why this basis should be preferred over any other, or why this quantum process should not occur in a single universe.

Criticisms of many-worlds theories in general and of the quantum multiverse in particular have been around for a long time now, and it is a pity that Deutsch does not recognize and address some of them in his book. Instead, he devotes a chapter to attacking the "bad philosophy" underlying alternative interpretations, particularly the conventional "Copenhagen" interpretation, which relies on making a distinction between the quantum world of particles and the classical world of detectors and observers. Many of us can certainly see weaknesses in the Copenhagen approach, but this does not mean that the multiverse is immune to criticism.

Quantum physics occupies only two of the 18 chapters of this book, which also surveys a wide range of modern science and philosophy. Deutsch's main theme is the possibilities for future progress that the ongoing scientific revolution has generated. As well as allegedly explaining quantum physics, these possibilities include the evolution of a culture based on a democratic political system and our ability to achieve anything that is not forbidden by the laws of nature – including immortality. Illness and old age, he writes, "are going to be cured ...certainly within the next few lifetimes".

Deutsch's ideas are expressed very clearly and the text is enlivened by a number of amusing anecdotes. This is a book that should interest anyone who likes thinking about the deep issues that underlie our understanding of the modern world – provided they maintain some scepticism over its dogmatic tone and reluctance to countenance alternative viewpoints. Deutsch willingly accepts that much of his inspiration comes from the work of Karl Popper, whose mantra "we have a duty to be optimistic" clearly underlies his thinking. However, he would have done well to remember that Popper was often dogmatic, to the point where some wags said that his book The Open Society and its Enemies should have been called "The Open Society by one of its Enemies"!

The geek shall inherit the Earth

"India was once one of the most powerful scientific nations of all," writes Angela Saini in the preface to Geek Nation. She bases her claim on the fact that Indians were using algebra, the zero and square roots centuries before the West, and that Indian astronomers are believed to have been the first to realize that day and night are caused by the Earth's rotation. Then Indian science went into a slump, Europe had its Enlightenment and modern science ended up being shaped mostly in the West. But now, Saini writes, "this impoverished tea- and cotton-growing backwater is starting to reclaim the scientific legacy that it lost thousands of years ago", and she is "here to learn about this rediscovered nation of geeks".

Unfortunately, this highlights one of the problems with Geek Nation, which is that Saini, a UK-based science journalist, seems to know from the outset what she wants to find in India. In her first interview on arriving in the country, she tells one of the pioneers of India's space programme that her book is to be titled Geek Nation and explains that, to her, "geekiness is all about passion. It's about choosing science and technology or another intellectual pursuit...and devoting your life to it."

The first few people she meets do not live up to her expectations. One of them is a physics prodigy who turns out not to be curious or brilliant but just hard-working and dreary. She spends a week in one of the most selective engineering colleges in India, the Indian Institute of Technology, Delhi (IITD), but finds the place dilapidated and the students uncreative and unresponsive. She visits India's largest software company, Tata Consultancy Services, and finds no trace of innovation. Saini is disappointed at not finding any geeks: "All I can see are drones."

Then, just when Saini wonders if "India is genuinely turning into a geeky, scientific society, or whether it's just hype", she visits IBM's India research lab and sees the development of the Spoken Web, a voice-based version of the Internet that can be accessed through a phone call by the underprivileged or illiterate. She visits a start-up in Bangalore where she finds innovation. And she goes back to IITD and finds that things there are not as bad as she initially thought. She even finds a student who is interested in design and is writing a novel about robots, and enthusiastically hails him as "a real geek".

Despite her (belated) success in finding someone who conforms to it, this narrative created around "geekiness" feels forced. Even Saini's constant use of the word "geek" – perhaps to justify the book's title – becomes tiresome. Hers is a "geeky mission"; the founder of India's space programme, Vikram Sarabhai, was a "good-looking geek"; and a tuberculosis researcher whose work may have damaged her health is saluted as a "true geek".

A bigger problem, though, is Saini's grasp of the facts. In her introductory chapter, for example, she writes that the first Indian prime minister, Jawaharlal Nehru, "even wedged a plea into the Indian constitution, announcing, 'It shall be the duty of every citizen of India to develop the scientific temper'." She repeats this claim in a later chapter, but although this line does appear in the Indian constitution, it was introduced more than a decade after Nehru's death. Elsewhere, an environmental activist tells Saini that "quantum theory teaches you that things are connected". Saini guesses that the activist is mixing up unrelated branches of science by invoking the idea of quantum entanglement, "which says that every particle in the universe is connected to every other, however distant it is, on a fundamental level" – yet this quasi-mystical definition is scarcely better than the activist's claim. Then there is a stray factoid that turns out to be only three-quarters true: "[Tuberculosis] killed Chekhov, Kafka, Keats and Napoleon."

In other places, Saini comes across as fanciful in her perceptions, writing of one interviewee that he "spends so much time designing computer programs that he speaks in peculiarly clipped sentences". When she meets a professor who has chosen science over religion, and comes across as calm and well adjusted, Saini even appears to indulge in a bit of "hot reading" when she says that behind his "happy, baggy eyes, I can see how hard the tension between the two must have been for him".

There are too many instances of error and imprecision in Geek Nation to list, but a particularly flagrant episode is Saini's description of India's first Moon mission. According to Saini, the probe Chandrayaan-1 was launched from "a remote island" and it "wandered the lunar surface for months" before being "forced to come back to Earth". But the launch site, Sriharikota, is just off the Indian coast and is easily accessible by road. Chandrayaan-1 was an orbiter with an impact probe, had no rover capable of wandering and only its radio signals ever came back to Earth. These errors end up compromising the wider argument they are part of. In addition to factual errors, the book contains unattributed perceptions about the Chandrayaan-1 mission, such as this (p5): "Nobody was sure whether the project would be a success or a waste of time, but the reputation of Indian science depended on it. Many in the scientific community had always assumed that India would never be able to afford a space mission." Statements such as these call upon the reader to trust Saini's command of relevant facts and judgement, but this becomes increasingly difficult as the book progresses.

Despite its limitations, Geek Nation does manage to provide a broadly impressionistic view of Indian science today. The book's sub-title, "How Indian Science is Taking Over the World", is debatable, but there is no doubt that steady progress is being made. Saini has chosen material that is rich in its potential to yield insights about science and technology in India and the cultural battles being fought around it: the education system; genetically modified crops; the sometimes overlapping boundaries between science, superstition and religion; the possibilities created by electronic governance in a country reeling from corruption; open-source drug discovery; and nuclear power. She also meets an array of people – industrialists, scientists, students, academics and traditional scholars – whose ideas are often interesting or insightful. With some better fact-checking and with a less predetermined view, Geek Nation might have been a very good book.

El Niño marches to the same beat as seasonal change

The El Niño–Southern Oscillation (ENSO) occurs in the Pacific Ocean every few years and the resulting weather conditions can wreak havoc on people and the environment, particularly in Latin America and South East Asia. Predicting when an ENSO event will occur has confounded scientists because the phenomenon does not appear at regular intervals. But a new study by researchers at institutions in the US could provide an important step in our understanding of this phenomenon, by establishing a direct link between ENSO and the annual global weather cycle.

El Niño, meaning "the Christ child", is so-called because the first signs of its appearance are marked by a warm current off the coast of Ecuador just after Christmas. These rising sea temperatures are related to a weakening of the trade winds that usually transport warm surface waters to the western margin of the Pacific. During an ENSO phase – which occur every 2–7 years – these warmer waters accumulate in the eastern tropical Pacific.

Individual ENSO episodes can last up to two years and lead to severe flooding in Latin America and droughts in South East Asia. One extreme cycle in 1997–1998 had far-reaching consequences, including extensive fires in the Indonesian rainforests and mudslides in California. Another impact of El Niño is that the accumulated warm water acts to block cold-water currents, which usually transport nutrients from the deep ocean to ecosystems along the Latin American coast. This can have a devastating effect on the fish stocks that form an important part of the economy in countries such as Peru and Colombia.

Mysterious origins

Despite El Niño's familiarity, scientists still do not fully understand what triggers these events, how they are sustained or what finally causes an ENSO cycle to subside. One thing that has been noted is that once ENSO episodes are under way, they all tend to follow a similar pattern of developing during summer or autumn in the northern hemisphere, then peaking during the northern winter. This interaction between ENSO and the annual cycle has now been more firmly established by a numerical study by Karl Stein and his colleagues at the University of Hawaii at Manoa.

Stein’s team has analysed observations of sea-surface temperature from the UK Met Office Hadley Centre spanning the period 1964–2007 and covering 20°S–20°N and 120–290°E. The extensive numerical analysis showed that ENSO events and the annual variation in temperature in the eastern Pacific are synchronized in a "2:1 Arnold tongue". In simple terms, this means that during a positive phase, ENSO and the annual cycle run according to the same beat but the seasonal cycle is moving twice as fast as ENSO.

Stein told physicsworld.com that one of the ultimate goals in characterizing ENSO is to develop a means of predicting when the next large warming event might occur. "Understanding the relative importance of amplitude versus phase modulation should lead to a better understanding of the physics involved in synchronizing ENSO to the annual cycle, which should hopefully lead to better predictions," he says. Stein believes that given the complexity of the climate system, realistically we could hope to predict the state of the equatorial Pacific only months or a year ahead of time at best.

Numerical connection

Rameshan Kallummal, a climate scientist at the Centre for Mathematical Modelling and Computer Simulation in Bangalore, India, is impressed by the fact that the new research establishes a quantative relationship between ENSO and the annual cycle. However, he feels that to gain a better understanding of El Niño will also require improved climate monitoring. "The main limitations to our understanding come from the various practical constraints in setting up well-distributed observing systems capable of making measurements continuously," he says.

Stein says that he and his colleagues intend to develop their research by investigating the influence that the tropical convergence zones have on the timing of ENSO events. He believes that the main outstanding questions relate to how ENSO will respond to future changes in the global climate. "The ENSO cycle is always going on; right now, we're observing La Niña [cold] conditions that are likely to persist through the winter," he says.

This latest research in published in Physical Review Letters.

Cyclotrons could boost technetium supply

 

The medical isotope technetium-99m (Tc-99m) could be made in hospitals rather than nuclear reactors. That is the conclusion of researchers in Canada, who have done theoretical modelling of how the material could be produced and processed in medical cyclotrons. Today Tc-99m is made centrally in a few nuclear reactors and cyclotron-based production could help to alleviate shortages that can occur when a reactor shuts down.

Although Tc-99m is used in a wide range of nuclear medicine procedures, the isotope is produced at only five nuclear reactors worldwide. The fragility of supply was highlighted recently by a global shortage brought about by the unscheduled shutdown of a reactor in Canada. As a result, physicists are keen to develop alternative methods for making the material.

This latest study was done by Anna Celler of the University of British Columbia and colleagues and is part of a C$35 million initiative by the Canadian government to look for alternative manufacturing techniques for Tc-99m.

Unwanted isotopes

In principle, Tc-99m can be made using a hospital's medical cyclotron to bombard molybdenum with a proton beam, causing the transmutation of some of the molybdenum-100 nuclei into Tc-99m. However, molybdenum targets are expensive and the technique produces other unwanted isotopes that reduce the diagnostic benefit for the patient. The viability of the technique must therefore be carefully scrutinized – however, doing experiments is extremely expensive.

Now Celler and colleagues have developed a theoretical model that predicts the viability of the method and estimates logistical parameters, such as the number of cyclotron runs needed to meet the daily demands of a typical nuclear medicine department. The reaction conditions needed for optimal yields, such as beam energy and target geometry, were also identified.

The researchers used the nuclear-reaction model code EMPIRE-3 to calculate the cross-section, or probability, of each of the possible molybdenum–proton reactions, across an energy range of 6–30 MeV. The simulation confirmed that the numerous molybdenum–proton reactions produced multiple contaminants, including several technetium, molybdenum, niobium and zirconium isotopes. Together with the yield calculations, the EMPIRE-3 simulation also demonstrated that only molybdenum targets enriched with molybdenum-100 were viable for efficient Tc-99m production. Natural molybdenum, with its composition of several isotopes, produced significant amounts of contaminant isotopes.

Ideal proton energy

The researchers also identified 16–19 MeV as the optimal proton energy range for Tc-99m production. In this range, relative Tc-99m yields were greatest when compared with contaminant isotopes. Shorter, multiple molybdenum -100 irradiation cycles per day, each 3–6 hours long, also proved to be the most efficient production schedule.

"We are very happy with these results: not only are our theoretical calculations in agreement with the existing experimental data, but also they provide us with guidance for future experiments and suggest what could be the optimal conditions for technetium production," said Celler. "The yields are sufficient, so that even cyclotrons designed to produce [positron emission tomography] PET radionuclides can produce sufficient quantities of Tc-99m to meet local needs."

The researchers are now using their results to calculate radiation doses to patients that will result from the cyclotron-produced technetium. "These dose calculations can then be compared with those related to reactor-produced technetium and will serve as guidance for the selection of target enrichment," explained Celler.

The research is described in Phys. Med. Biol. 56 5469.

The rhythm is gonna get you – where you want to go

Cell in the entorhinal cortex


Cell in the entorhinal cortex (Credit:Journal of Neuroscience )

By Tushna Commissariat

Last week I wrote about physicists in Europe who have developed a model to better understand the neuron activity in the brain that occurs when we listen to music. Their simulations suggest that certain notes sound harmonious because of the consistent rhythmic firing of neurons in the auditory system. They quantified this effect by showing that neural signals are regularly spaced for frequencies that are pleasant sounding, but are erratic for those that are not. The same researchers also said that their model may also provide insights into other senses, such as vision, that employ similar neural processing systems. Hot on the heels of that statement, this week I came across a paper in the Journal of Neuroscience discussing how neurons work to “code position in space” – simply put, the team looked at what mental processes occur while your brain perceives the space you are in and helps you to navigate within it.

Motoharu Yoshida and colleagues at Boston University in the US investigated how the rhythmic activity of nerve cells supports spatial navigation. The scientists showed that cells in the entorhinal cortex – which is located in the medial temporal lobe of the brain and acts as the main interface between the hippocampus and neocortex, playing an essential role in episodic and spatial memory formation – oscillate with individual frequencies, with the frequencies depending upon the positions of the cells within that cortex. Until now, it was believed that the frequency was modulated by the interaction with neurons in other brain regions, but in the light of these new data, this may be incorrect.

“The brain seems to represent the environment like a map with perfect distances and angles” explains Yoshida. “However, we are not robots with GPS in our head. But the rhythmic activity of the neurons in the entorhinal cortex seems to create a kind of map.” The activity of individual neurons in this region of the brain represents different positions in space, according to the researchers. The rhythmic activity of each cell may enable us to code a set of positions, forming a regular grid in the brain. Researching the capacity that most animals and mammals have for spatial navigation is always of interest, as a through understanding of it could lead to a clear picture of how our brains function in general.

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