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When reading popular-science books, what do you find most stimulating?

By James Dacey

Earlier this week we at Physics World revealed our top 10 popular-physics books of the year as we released this specially recorded podcast. I won’t spoil the surprise by mentioning any of the titles here, but I can say that the list spans a wide variety of books, including biographies, the history of physics and even a tome about cookery.

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As with any “best of” listing exercise, we fully expect that some listeners will disagree with our choices and some may feel strongly that other books have been cruelly overlooked. Of course, there is always going to be some degree of subjectivity in making these choices, and it is not always straightforward to explain what lifts a book from being great to being inspirational. But give the podcast a listen and let us know what you think about our choices by posting a comment on the accompanying article.

In the meantime, it would be great if you could share your thoughts on popular science in general writing by responding to our poll question.

When reading popular-science books, what do you find most stimulating?

The technical details underpinning the science
The personal stories of the scientists
The impact of the science on culture and society
The sense of wonder conveyed by the author

To cast your vote, please visit our Facebook page, and feel free to explain your answer by posting a comment.

In last week’s poll we wanted to gauge your opinion on a topic close to the hearts of both nuclear physicists and chemists. We asked whether you liked the names flerovium and livermorium, which have recently been proposed by the International Union of Pure and Applied Chemistry (IUPAC) for the two new elements 114 and 116, respectively.

Flerovium was devised because both elements were created in 2004 by researchers at the Joint Institute for Nuclear Research (JINR) in Dubna, Russia, which was founded by the prominent Soviet nuclear physicist Georgi Flerovm. Livermorium arose because both elements were confirmed by scientists at the Lawrence Livermore National Laboratory (LLNL) in California and the Centre for Heavy Ion Research (GSI) in Darmstadt, Germany. (The German contribution is not recognized because the element Darmstadtium already exists.)

Despite this relatively logical approach to naming, it seems that many respondents are not too impressed with the proposals. Just 30% selected “I like both”, while 49% opted for “they’re boring and unimaginative”. Some 13% said they “like flerovium but not livermorium”. And just 8% said the converse, they “like livermorium but not flerovium”. One pollster, Chandan Dasgupta based in Calcutta, India, took a particular dislike to flerovium, commenting that it “sounds like a health drink!”.

Thank you for all your responses and we look forward to hearing from you again in this week’s poll.

Let there be a year of light

Light plays a central role in science, technology and culture. The study of light and electromagnetism is fundamental to the evolution of essentially all modern science. Light underpins the existence of life itself through photosynthesis, and is our main messenger from investigating the large-scale universe to the infinitely small. Light-based technologies have already revolutionized medicine and opened up international communication via the Internet, and will continue to underpin the future development of human society.

Scientists, from physicists to astronomers and biologists, are, of course, well aware of the tremendous importance of optical science and technology for future development. But it is vital that this message is communicated more widely and that the brightest young minds continue to be attracted into careers in science and engineering. It is precisely for this reason that a proposal has been made for an International Year of Light to promote improved public and political understanding of the central role of light in the modern world.

Initiated by the European Physical Society (EPS), the call for an International Year of Light has assembled an impressive group of partners, including the Institute of Physics, which publishes Physics World. The EPS will now be approaching other international scientific unions and academies to involve them in the future development of the initiative. The proposal has also received a crucial endorsement from the International Union of Pure and Applied Physics (IUPAP) during its general assembly in London last month, which will allow the organizers to prepare a formal request next year to the UN and UNESCO – the UN’s educational, scientific and cultural organization. To make it a success, however, we will need the support of the whole scientific community.

Leading light

The UN has declared “international years” since 1959 to draw attention to topics deemed of worldwide importance, and these can only be granted by the UN’s general assembly. There have been a number of successful science-based themes in recent years, including physics in 2005, astronomy (2009) and chemistry this year. An International Year of Light in 2015 seems like a natural choice given that the year features a remarkable series of anniversaries, all of which have helped our understanding of light.

In particular, in 2015 it will be 200 years since Augustin-Jean Fresnel’s seminal paper introducing the notion of the wave nature of light and 150 years since James Clerk Maxwell’s work on electromagnetism, which paved the way for technologies from lasers to mobile phones. The year also marks the centenary of the incorporation of the speed of light as an essential part of our description of space and time in Einstein’s equations of general relativity, as well as the 50th anniversary of Arno Penzias and Robert Woodrow Wilson’s discovery of the cosmic microwave background – the electromagnetic echo of the Big Bang.

Following the initiative of the EPS’s quantum electronics and optics division in 2009, the International Year of Light was launched by the EPS during the Passion for Light workshop held in Varenna, Italy, on 16 September. The workshop was attended by more than 100 distinguished physicists, including Nobel laureate Theodor Hänsch, IOP president and quantum-optics pioneer Peter Knight and Luciano Maiani, a former director-general of CERN. In addition, Mario Scalet, head of the science unit of the UNESCO Venice office, gave a talk outlining the general role of UNESCO in supporting science, culture and education, and Joseph Niemela, director of UNESCO’s optics education programme, provided an overview of UNESCO’s outreach activities.

By bringing together participants from so many different fields, the workshop clearly showed how light impacts on all areas of science. The general structure of the year, which was established at the Varenna meeting, will be focused around four broad themes: the fundamental science of light; the use of light as an enabling technology; the application of light to improve the quality of life in the developing world; and an educational theme covering the pioneering scientists who have studied light and optics throughout history.

An International Year of Light would have an almost unique potential to demonstrate that science is no longer made up of simple and disparate disciplines, and will highlight very strongly that the 21st century will see an increasing need for strong interactions between all areas in order to achieve the most ambitious scientific goals. With the backing of IUPAP, the project partners will now work through the necessary steps so that 2015 can be declared the International Year of Light.

But we should not forget that light touches upon much more than science. Given its central role in culture and art, an International Year of Light will not only be for scientists and physicists, but will be for all humanity.

  • If you are interested in being involved in the planning for the International Year of Light, e-mail light@eps.org

Physicists weigh up Higgs signals

Particle physicists are today digesting the news from yesterday’s special seminar at CERN, where potential glimpses of the Higgs boson were revealed. Based on nearly all the data collected so far – the debris of some 500 trillion proton–proton collisions – the Large Hadron Collider’s ATLAS and CMS experiments have now excluded the Higgs at pretty much all masses outside the narrow region between 115–130 GeV/c2 and 115–127 GeV/c2, respectively. The analyses represent a major reduction in the particle’s possible hiding places compared with the situation just a few months ago.

“We would like the Higgs to be in this range, but it’s too early to draw conclusions,” ATLAS spokesperson Fabiola Gianotti told the several hundred staff packed into CERN’s main auditorium. The Higgs is the observable upshot of a mathematical trick that preserves symmetry in the equations of fundamental particles as coded by the Standard Model of particle physics. Higgs bosons heavier than about 600 GeV/c2 have not yet been ruled out, but are disfavoured by indirect fits based on precision Standard Model measurements.

The two experimental collaborations also revealed what could be direct signs of the Standard Model Higgs lurking in the remaining low-mass region, which is where theory suggests it should appear. Although physicists stressed that the data are not sufficient to provide a conclusive statement either way on the existence of the Higgs, researchers could barely conceal their excitement about the tiny bumps in their plots. So is this finally the real thing, or are physicists being teased once again by the notorious, so far still imaginary, boson?

Hints and hopes

“It’s too early to be sure,” says theorist Matt Strassler of Rutgers University in the US. “But not too early to be hopeful.” Indeed, history would advocate caution. After all, in late 2000 the CERN auditorium was also the venue for a packed seminar on potential sightings of the Higgs from the forerunner to the LHC – the Large Electron–Positron (LEP) collider. Tantalizing hints were presented by LEP physicists of a Higgs at a mass of about 115 GeV/c2, but on further analysis of the data these eventually proved less significant and left physicists with the current lower bound on the Higgs mass.

Several potential sightings of the Higgs at other colliders have since come and gone. In 2007, for instance, the Tevatron proton–antiproton collider in Fermilab, Chicago, hinted at a Higgs with a mass of 160 GeV/c2, only for this and neighbouring masses to be ruled out a couple of years later by the same collider. In July this year, meanwhile, ATLAS and CMS both reported possible sightings of a roughly 140 GeV/c2 Higgs, but within weeks those hints had faded once more data were analysed, and yesterday the Large Hadron Collider (LHC) killed off any remaining hopes of finding a Higgs at this mass.

Statistical significance

The latest round of Higgs mania – some physicists had camped out in the auditorium from 8 a.m. to make sure they got a seat and security guards were turning away disgruntled staff more than two hours before the afternoon event began – concerns an excess of LHC collision “events” consistent with the production and decay of a Higgs with a mass of about 125 GeV/c2. “In the past we have seen similar fluctuations, but now it is different because the experiments are entering a region where the sensitivity is very high,” CMS spokesperson Guido Tonelli told reporters.

The statistical significance of the latest Higgs hints is not too different to that of previous sightings: around the 2σ mark, which means there is a probability of a few per cent that such bumps in the data would appear anyway in that mass region because of fluctuations in background processes. Less-conservative estimates – 3.6σ in the case of ATLAS – are obtained if one quotes the “local probability”, which represents the chance of getting such a fluctuation at a particular mass value. But there is good reason why many physicists think the latest bumps may grow rather than fade once collisions resume in the spring after the LHC’s scheduled winter shutdown.

Reasons to be cheerful

The first reason is that both experiments, which are physically independent and use different analysis techniques, see hints at similar masses: roughly 126 and 124 GeV/c2 for ATLAS and CMS, respectively. The second is that the experiments see an excess of events in more than one of the Higgs’ independent decay channels, which dictate the handful of ways in which a Higgs would reveal itself inside the detectors. The most striking signals at about 125 GeV/c2 come from events where the Higgs is presumed to have decayed into a pair of photons, but ATLAS also sees the effect in the channel where a Higgs decays into two Z bosons, which subsequently decay into leptons such as electrons.

Veteran Higgs hunter Sau Lan Wu from the ATLAS collaboration says that the fact that there is a potential signal in two channels is “most intriguing”, especially given that CMS also sees something at a similar mass. “I am excited and optimistic that there is a low-mass Higgs at about 126/125 GeV/c2, but the final judgement will come only in the second half of 2012,” she says. Indeed, having so far analysed more decay channels than ATLAS with the full 2011 dataset, CMS researchers say that the data across all channels provide a consistent picture. “We are observing exactly the significance that we would expect if we were to inject a Higgs with a mass of 124 GeV/c2 into the data,” Vivek Sharma of the CMS collaboration told physicsworld.com.

However, CMS also sees a small excess at about 119 GeV/c2 in the ZZ channel, and the fact that the main CMS and ATLAS bumps are not at precisely at the same masses does not sit well with some physicists. “The picture is somewhat confused,” explains Patrick Janot of the CMS experiment, who has been chasing the Higgs for the past 20 years. “We see something at 119, 126 and 124  GeV/c2, but everything is compatible with anything. People are being a bit too enthusiastic. These are not strong hints – LEP had a bigger Higgs significance. Let’s wait for more data.”

More work needed

Unlike LEP in 2000, when Higgs fever took hold just as the machine was scheduled to be shut down, the LHC is now at the very beginning of its life and is certain to either find the Standard Model Higgs or rule it out. If the Higgs does exist, it will take considerable time to understand precisely what it is, for example by measuring the many ways in which it interacts with other particles. Only then would physicists know whether the particle was the basic Higgs required to complete the Standard Model or something more complicated that could open the door to a more general theory beyond the Standard Model that, for instance, addresses the mystery of dark matter.

“If the Higgs is light as the data now suggest, then this is very important theoretically because it means there must be new physics,” Gigi Rolandi of CMS told physicsworld.com. “If the Higgs is lighter than 127 GeV/c2, the Standard Model breaks at [energies of] about 108 GeV/c2.”

In the spotlight

Another difference in today’s Higgs search compared with a decade ago is the huge interest from outside CERN – more than 110 000 people hooked up to the webcast of yesterday’s seminar. “Journalists are picking up on the chase and reporting real science in the making,” CERN’s head of communications James Gillies told physicsworld.com.

Few physicists who spoke to physicsworld.com were convinced, however, by CERN’s decision to invite the media to an interim report on the Higgs search yesterday, although most accepted that it was inevitable given the amount of speculation on physics blogs in recent weeks. Although those blogs proved fairly accurate, Dave Charlton of ATLAS says that the rumours were “not helpful”, arguing that they could have harmed the scientific process by alerting ATLAS or CMS to each others’ search results before independent conclusions have been reached. Dave Barney of CMS goes further. “The only people talking up the significance of these latest Higgs hints were the [bloggers],” he told physicworld.com. “CERN had no choice [but to hold a press conference to clarify the situation].”

One thing is certain: yesterday will not be the last time physicists pack into CERN’s main auditorium to hear a special seminar on the Higgs. “The CERN seminar has a very positive effect on the young physicists here,” adds Wu. ” More than ever, they are excited about their work hunting the Higgs.”

Top 10 books of 2011

You will hear a little about each of our top 10 books in the podcast, including a short explanation of why we liked them so much. There are a few detours as well, as the three of us seize opportunities to discuss bad physics in films, Richard Feynman’s legacy and the unusual career of one of Stephen Hawking’s postdocs. You will also find out which very well-publicized physics book did not make our list (and why!).

Our selections (see below for a full list) include books on condensed matter, biophysics, astrophysics and astronomy, as well as science history and policy. Regardless of their subject matter, though, all of the choices are well written, scientifically interesting and novel – and we think this year’s winner is a worthy successor to The Strangest Man and The Edge of Physics, which scooped our number-one honours in 2009 and 2010, respectively.

We hope you enjoy hearing about these books as much as we enjoyed reading them. Look out for more books podcasts in 2012!

2011 Books of the Year – alphabetical by author

Engineering Animals Mark Denny and Alan McFadzean

Measure of the Earth: the Enlightenment Expedition that Reshaped the World Larrie Ferreiro

The Hidden Reality: Parallel Universes and the Deep Laws of the Cosmos Brian Greene

Lab Coats in Hollywood: Science, Scientists and Cinema David Kirby

Quantum Man: Richard Feynman’s Life in Science Lawrence Krauss

Rising Force: the Magic of Magnetic Levitation James Livingston

Modernist Cuisine Nathan Myhrvold, Chris Young and Maxime Bilet

The 4% Universe: Dark Matter, Dark Energy, and the Race to Discover the Rest of Reality Richard Panek

Radioactive: Marie and Pierre Curie, A Tale of Love and Fallout Lauren Redniss

Hindsight and Popular Astronomy Alan Whiting

Hear all about it

<img width="500" height="273" src="https://physicsworld.com/wp-content/uploads/2011/12/PW-2011-12-14-team.jpg" alt="Recording the Physics World Book of the Year podcast “>
The Physics World podcasters. Left to right: Margaret Harris, James Dacey and
Matin Durrani.

By Margaret Harris

’Tis the season of “Top 10” lists here at physicsworld.com, and to kick off our commemorations of the year in physics, my colleagues James Dacey, Matin Durrani and I have recorded a special podcast on our choices for the 10 best popular-physics books of 2011. You can listen to the podcast here or by subscribing to our podcast service.

You’ll find a list of all 10 featured books below, along with links to their reviews on physicsworld.com. However, to find out which of them gets our vote for the 2011 Book of the Year – and why we thought all of them were worth including in the top 10 – you’ll have to listen to the podcast.

If your favourite didn’t make the shortlist, keep in mind that there were many other good physics books published this year – including several that featured in our previous podcast – and also some promising ones that we haven’t had a chance to review yet. Look out for them in 2012!

2011 Books of the Year – alphabetical by author

Engineering Animals Mark Denny and Alan McFadzean

Measure of the Earth: the Enlightenment Expedition that Reshaped the World Larrie Ferreiro

The Hidden Reality: Parallel Universes and the Deep Laws of the Cosmos Brian Greene

Lab Coats in Hollywood: Science, Scientists and Cinema David Kirby

Quantum Man: Richard Feynman’s Life in Science Lawrence Krauss

Rising Force: the Magic of Magnetic Levitation James Livingston

Modernist Cuisine Nathan Myhrvold, Chris Young and Maxime Bilet

The 4% Universe: Dark Matter, Dark Energy, and the Race to Discover the Rest of Reality Richard Panek

Radioactive: Marie and Pierre Curie, A Tale of Love and Fallout Lauren Redniss

Hindsight and Popular Astronomy Alan Whiting

Other-worldy tales

The 5th Dimensional Camera


The artwork The 5th Dimensional Camera, which explores the theme of parallel worlds. (Courtesy: EPSRC Press Office)

By Matin Durrani

I’m sure we’ve all go our own personal wishes for a parallel universe – perhaps it’s a world where physicists are flush with cash, the Superconducting Super Collider had never been cancelled and CERN press conferences discussing the search for the Higgs had a bit more oomph about them.

But writing in the December issue of Physics World magazine, Stony Brook University philosopher and historian Robert P Crease examines how the idea of parallel universes and parallel worlds also appear frequently in art and literature.

We’ve all heard of Lewis Carroll’s beloved story Alice’s Adventures in Wonderland, of course, but did you know that Jorge Luis Borges described the concept of a “multiverse” in his 1941 anthology The Garden of Forking Paths? Or that Alan Ayckbourn wrote a series of plays called “Intimate Exchanges”, in which a single opening scene branches out into 16 different endings?

As Crease points out, the idea that parallel worlds should attract novelists is “perhaps not surprising” – after all, as he puts it, they deal with “events shaped by contingencies that unfold over time”.

But the theme of alternative worlds that are similar (but not identical) to our own, branching off from each other, has featured in films as well, including last year’s Rabbit Hole, starring Nicole Kidman, which was based on the celebrated 2005 play of the same name by David Lindsay-Abaire.

It also crops up in the new film Another Earth, which was released earlier this year. Examining the consequences of a promising student who causes a fatal car crash, the film has unfortunately received a bit of a panning, being dubbed by the Daily Mail as “pretentious twaddle” and by the Guardian as “ponderous and contrived”.

Still, let’s not forget that multiple worlds have even inspired some sculptors, including Jon Ardern and Anab Jain of the Superflux studio in London, who created an interesting work called The 5th Dimensional Camera, pictured above, which appeared last year in an exhibition called “Talk to Me” at the Museum of Modern Art in New York.

Members of the Institute of Physics (IOP) can read the article “Other-worldly tales” online free of charge via the digital version of the magazine by following this link or by downloading the Physics World app onto your iPhone or iPad or Android device, available from the Apple store and Android Marketplace, respectively.

If you’re not yet a member, you can join the IOP as an imember for just £15, €20 or $25 a year via this link. Being an imember gives you access to a digital version of Physics World both online and through the apps.

Higgs hunters close in on their quarry

 

The first solid experimental evidence for the existence of the Higgs boson has been unveiled today by physicists working on the Large Hadron Collider (LHC) at CERN in Geneva. Members of the ATLAS experiment revealed evidence that the Higgs particle has a mass of about 126 GeV/c2. Physicists working on the rival CMS experiment released similar – albeit weaker – evidence for a Higgs with a mass of about 124 GeV/c2.

However, ATLAS spokesperson Fabiola Gianotti cautions that the measurements are not good enough yet to claim the discovery of the particle.

Physicists are keen to discover the Higgs boson to complete the Standard Model of particle physics. The particle and its associated field are needed to explain how electroweak symmetry broke just after the Big Bang – which gave certain elementary particles the property of mass. The Standard Model does not, however, actually predict the mass of the Higgs, and successive experimental programmes at CERN’s Large Electron–Positron Collider, Fermilab’s Tevatron and now the LHC have sought to measure its mass.

If the current glimpse of the Higgs proves to be an illusion, and it – or a similar symmetry-breaking entity – is never found, all would not be lost, as physicists would be forced to concede that the Standard Model is incomplete and to look for “new physics” beyond it.

Evidence versus discovery

The ATLAS measurement was made at a confidence level of about 3.6σ, which means that the measurement could be the result of a random fluke just 0.1% of the time. While these might sound like fantastic odds, particle physicists normally wait until they have a confidence of 5σ or greater before they call it a “discovery”. Anything above 3σ is described as “evidence”.

There are several reasons why particle physicists require such high confidence levels. One is the “look elsewhere” effect that arises because the data are sorted into mass/energy bins to create a histogram – which could concentrate fluctuations. After the look elsewhere effect is considered in the ATLAS result, the confidence level drops to 2.3σ, according to Gianotti.

Another potential problem is that there could be unknown systematic errors lurking in the experiment that could be responsible for the apparent result, and therefore requiring a very high confidence could help avoiding such errors.

Despite the preliminary results announced at CERN today, unravelling the mystery of the Higgs will take some time. Assuming that the signal at 126 GeV/c2 survives further analysis, the next step for physicists will be to tease out the precise nature of the Higgs they have discovered. According to Matt Strassler of Rutgers University in the US, a mass of about 126 GeV/c2 could indicate many different things. These include a Standard Model Higgs, a Higgs that is best described by theories beyond the Standard Model such as supersymmetry (SUSY), a “little Higgs” or various other theories.

Different reactions

To gain a better understanding of the Higgs, Strassler says that several different reactions that produce the Higgs at the LHC must be studied, as well as several different decay channels of the particle. In particular, physicists must find out how closely the Higgs is described by the Standard Model, which involves studying interactions involving W and Z particles, top and bottom quarks, and tau leptons.

In total, he believes that seven or eight different measurements are required before physicists will have a handle on the Higgs. “Next year we could be in a position to say that we have a particle that’s reasonably consistent with the Standard Model,” says Strassler. This would allow physicists to eliminate theories – such as technicolor – that do not include the Higgs particle.

“By 2014/2015 we could have enough additional data to eliminate large classes of theories that attempt to explain the Higgs,” adds Strassler, although he warns that it could take as long as 10 years to gain a full understanding of the particle.

However, not all physicists believe that the road to understanding the Higgs will be a long one. Gordon Kane of the University of Michigan and colleagues have recently published a preprint on the arXiv server that calculates the mass of the Higgs using string theory – calculations that put the Higgs mass in the 122–129 GeV/c2 range. Kane told physicsworld.com that physics beyond the Standard Model has “jumped out as string theory”. “The game is over and we have won – we have landed on the shores of a new world,” he adds.

For more information about the search for the Higgs, watch our video with Guido Tonelli, spokesperson for the CMS experiment, and ATLAS researcher Pippa Wells.

Are pulsars giant ‘neutromagnets’?

Pulsars are created when a star collapses to form a neutron star in which the magnetic moments of the neutrons are frozen in a particular direction – much like the atomic moments in a permanent magnetic. That is the claim of two physicists in Sweden, who believe that their theory can account for many of the unexplained properties of these astronomical oddities.

First discovered in 1967, pulsars are astronomical objects that emit radiation pulses with astonishing regularity. Astronomers believe pulsars are rapidly rotating neutron stars that have very large magnetic fields. Just like the Earth, the magnetic dipole moment of the star is believed to be offset from its rotational axis. Jets of radiation are emitted from the star along its magnetic poles. Because the star is rotating about a different axis, the jet sweeps round like a lighthouse beam that appears as a regular pulse if it happens to strike Earth.

Beyond this basic description, however, little is known about the physics of pulsars and how they formed. One important question is the origin of the magnetic field, which can range from about 104 to 1011 T. That is huge compared with the Sun’s magnetic field, which is about 100 µT. Furthermore, the regular nature of the pulses suggests that a pulsar’s magnetic field must be extremely stable. In contrast, the Sun’s magnetic field is notoriously unstable because it is generated by the rotation of the star’s plasma, which is prone to instabilities.

Nuclear force favours alignment

“There is no good explanation for how the magnetic field is generated,” explains Johan Hansson of Lulea University of Technology, who put forward this latest theory with colleague Anna Ponga. Hansson and Ponga suggest that the magnetic moments of all the neutrons in the star point in the same direction in a state of matter called a “neutromagnet”. This is similar to the alignment of atomic magnetic moments in a ferromagnetic material. The researchers point out that the nuclear force that binds protons and neutrons together in nuclei favours the alignment of spins – an effect that they say could be enhanced in neutron stars, where neutrons are packed even more tightly together.

Hansson and Ponga assumed that the energy gained by two neutrons by aligning their spins in the same direction is about 10% of the total nuclear binding energy of the pair. This gives a Curie temperature – below which all the neutrons in the star align to become a giant magnet – of about 1010 K.

Because neutron stars all seem to have about the same mass, the maximum magnetic field that could result is about 1012 T. This would occur when all the neutrons are aligned in the same direction. However, just like everyday magnets, it is possible that different regions of the star have domains of neutrons – with each domain pointing in a different direction. This would reduce the overall magnetic field and could explain why some neutron stars have much smaller magnetic fields. According to Hansson, this maximum value of the magnetic field provides astronomers with a simple way of falsifying the theory.

Moment is frozen in

Hansson told physicsworld.com that their model also explains the fixed misalignment between the magnetic moment and the rotational axis of a pulsar. “The orientation of the magnetic field is set by the direction of the star’s magnetic field at the moment it collapses to form the neutron star,” he explains. “The direction is then ‘frozen in’ by the nuclear force”.

However, not all astronomers are convinced. “I don’t claim that the current ‘understanding’ is complete or free of contradiction – the problem is very hard – but I believe that the concept presented in this paper is not nearly as good as the standard models,” says Michael Kramer of the University of Manchester in the UK.

The work is described in arXiv:1111.3434.

Corrosion carves out 3D nanostructures

Researchers in Spain have invented a new technique for making hollow nanoparticles with sophisticated shapes and compositions. The method, which combines two well-known corrosion processes into a single step, modifies the shape of tiny nanoparticles after they have been created. The resulting nanostructures could find use in drug delivery, catalysis and even as structural components for nanorobots.

Nanobjects can be assembled from the bottom up, atom by atom or molecule by molecule, but this is usually a tedious process that generally involves picking up individual atoms or molecules with the tip of a scanning-electron or atomic-force microscope. The technique is also fiddly because the microscope tip has a tendency to “stick” to the nano-objects.

Now, Edgar Gonzàlez and colleagues at the Institut Català de Nanotecnologia have overcome this so-called sticky nanofinger problem using chemistry. The researchers have shown that corrosion processes such as galvanic replacement and the Kirkendall effect can be used to attack and pit nanoparticles from the “inside out”. The result being complex geometric interconnected multicavity hollow nanostructures. Corrosion is much more aggressive for nanoparticles – compared with larger structures – because the tiny particles have larger surface areas relative to their volume.

A variety of nano-objects

The structures produced by the team range in shape from molecular labyrinths or nanomazes (made from silver and gold or platinum) to gold fullerenes. Other structures, such as nanoboxes, porous nanotubes and nanoframes, can also be fashioned from silver and gold nanoparticles (see figure).

The Kirkendall effect occurs when there is a movement of vacancies in a metal that is in the opposite direction to that of natural atom diffusion. This flux leads to voids being produced in the material. Galvanic replacement is also a simple way to make hollow nanostructures of noble metals when silver nanostructures are used as sacrificial templates. It is a one-step process that dissolves metallic nanostructures to produce constructs that are enclosed by continuous or porous walls the thicknesses of which can be controlled.

Corroding objects in such a way would be impossible on the macroscale, says team leader Victor Puntes. “In the nanoworld, however, the effect occurs spontaneously if the corrosion ingredients and nanoparticles are mixed together properly,” he says. “The nanoworld is a billion times smaller than the ordinary world, and phenomena occurring there seem like pure miracles when compared with those happening on our everyday scale.”

Carrying cargo

The hollow nanoparticle capsules or cages can protect and carry different types of payload. They could be used to safely transport a drug to a target in the body – for instance to treat a tumour – or carry a specific catalyst to a reaction site. The capsules can also be open or closed, heated and manipulated by electromagnetic fields.

The researchers observed the structures they made using high-resolution transmission electron microscopy, which allowed them to analyse and visualize different shapes atom by atom.

The technique can also be readily adapted to industrial-scale production levels, adds Puntes.

Details of the work can be found in Science.

New ink prints graphene electronics

A new ink based on graphene has been used to print high-performance, transparent, thin-film transistors and interconnects. The ink was invented by researchers at the UK’s University of Cambridge, who say that the work could lead to better printed electronics, including flexible displays, solar cells and electronic paper.

Flexible electronics looks set to change the way we use technology in our everyday lives, with a wide range of devices already having been made. Inkjet printing is one of the best ways of making large amounts of plastic electronics, and a variety of components, such as transistors, photovoltaic devices, organic light-emitting diodes and displays, can be fabricated using this technique. Inkjet printing is also simple and only has a few processing steps.

The technique has been used to print thin-film transistors based on organic and semiconducting inks. However, these devices do not offer the same performance and reliability as standard silicon-based electronics.

Better transistors

Now, Andrea Ferrari and colleagues have taken an important step towards creating better devices. They have developed an ink based on graphene – sheets of carbon just one atom thick with unique electronic and mechanical properties. The ink is made by separating graphene flakes from pieces of graphite in a liquid. The process begins with treating graphite flakes in a sonic bath containing the solvent N-methylpyrrolidone for several hours. The flakes are then left to settle for a few minutes. Next, the team decants the dispersions and centrifuges the samples for an hour to filter out any flakes bigger than 1 µm across that might clog the printer nozzle.

The ink can then be used to print electronic devices such as thin-film transistors (TFTs) on a variety of substrates, including silicon dioxide and quartz. The first TFTs printed using this ink already seem to perform better than state-of-the-art inkjet-printed devices. The preliminary devices have electron mobilities of up to 95 cm2 V–1 s–1 for example. In comparison, inkjet-printed TFTs based on organic semiconducting polymers have mobilities ranging from just 0.01 to 0.5 cm2 V–1 s–1, but better on/off ratios of up to 105.

Compatible with existing technology

“Our technique is not new and the graphene ink produced should therefore be compatible with existing standard inkjet machines,” says Ferrari. “This will hopefully allow the ink to be used in existing printed electronics.”

The researchers – who report their work on the arXiv preprint server – now plan to optimize the process parameters. “We shall also be making contact with the major players in the printed-electronics industry to try and implement the ink in useful devices,” reveals Ferrari.

The work is described in arXiv:1111.4970.

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