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Through two mirrors, brightly

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Hubble’s “Rose of Galaxies” anniversary image
(Courtesy: NASA, ESA, A Riess (STScI/JHU), L Macri (Texas A&M University) and Hubble Heritage Team (STScI/AURA))

By Tushna Commissariat

Millions of people worldwide have exclaimed in awe and wonder at the images that the Hubble Space Telescope (HST) has been producing for more than two decades. The satellite has had a significant impact on all fields of science from planetary science to cosmology ever since it was launched on 24 April 1990 aboard Discovery’s STS-31 mission. In a bid to celebrate the 21st anniversary of the HST, astronomers at the Space Telescope Science Institute in Baltimore, Maryland, in the US pointed Hubble’s eye at a particularly magnificent cosmic phenomenon – a pair of interacting galaxies in the shape of a rose.

The newly released Hubble image shows two interacting galaxies known as Arp 273. The larger of the spiral galaxies – UGC 1810 – has a disc that is being distorted into a rose-like spiral thanks to the gravitational tidal pull of the companion galaxy below it, known as UGC 1813. The smaller companion shows signs of intense star formation at its nucleus, quite possibly triggered by the smaller galaxy actually passing through the disc of the larger galaxy. A veil of bright and hot young blue stars glows across the top of the dancing discs.

Arp 273 lies in the constellation Andromeda and is about 300 million light-years away from Earth. Though the galaxies are separated from each other by tens of thousands of light-years, they are connected by a tidal bridge of material between them that formed post interaction.

Take a look at the gorgeous image (above) and a video (below) zooming into the region of the galaxies.

In other space-related news, the final launch of the space shuttle Endeavour will take place tomorrow, 29 April, from Florida’s Space Coast in the US. So while Britons and many others all over the world will be watching the royal wedding, Kennedy Space Center is anticipating the arrival of an estimated half a million onlookers, eager to watch the space shuttle lift off one more time. Endeavour, first launched in May 1992, is expected to carry six astronauts, a cargo bay full of spare supplies and a $2bn astrophysics experiment to the International Space Station.

To look at some interesting images in the follow-up to the launch, look here: http://www.space.com/11221-photos-space-shuttle-endeavour-final-mission-sts134.html

Invisibility cloak offers a snug fit

An invisibility cloak that is less than five times bigger than the object it conceals has been unveiled by physicists in Denmark and the UK. They say that their device, which they built using semiconductor manufacturing techniques, offers the smallest cloak size relative to cloaked area to date.

First developed in 2006, invisibility cloaks can hide an object from view by bending light around it. The effect is similar to how a star’s immense gravity can warp space–time so that passing light is forced to take a curved path. In invisibility cloaks, however, the path of light is altered not by gravity, but by specially engineered variations in the refractive index of the devices.

Most invisibility cloaks have been able to hide objects the size of just a few microns, but earlier this year a group at the Singapore-MIT Alliance for Research and Technology Centre reported a cloak that could hide objects up to two millimetres big. Meanwhile, Jingjing Zhang and colleagues at the Technical University of Denmark in Lyngby, along with researchers at Imperial College London and the University of Birmingham, reported a cloak that could hide objects on the scale of centimetres. Yet both these cloaks had to be more than 10 times bigger than their cloaking area.

Hiding surface defects

Now Zhang and colleagues have worked out how to reduce this ratio. “In some applications where space is a critical issue, we need to design a cloak as small as possible for a given obstacle,” says Zhang. One of these applications might be in the optoelectronics industry, he adds, which sometimes needs to hide surface defects on microcircuits.

The cloak built by Zhang and colleagues is a carpet cloak, a type of cloak that uses a conducting sheet to flatten – or appear to flatten – the bulge of an object hidden beneath. In previous carpet cloaks, the design has been realized with a complex array of silicon holes or rods, varying in density everywhere to produce an anisotropic structure.

The cloak of Zhang’s group, however, is much simpler: a series of uniform slits (a grating) crafted into silicon using normal semiconductor manufacturing techniques. By changing the amount of silicon relative to air in the grating, the researchers could tune their cloak to be almost as anisotropic as they want. This is crucial to the design because keeping the cloak small relative to the cloaking area requires a lot of anisotropy.

In tests, the cloak could hide a bump in a surface that is the same width as the cloak (10 µm) and around four times shorter (the bump’s height is 1.84 µm and the cloak’s 8 µm). It worked over infrared light wavelengths between 1480 and 1580 nm, although the researchers say that in principle it should work over a broader range.

Drawbacks from very large anisotropy?

Won Park, an engineer specializing in invisibility cloaks at the University of Colorado, says the cloak’s very large anisotropy might have drawbacks. “Some unintended effects such as diffraction may occur at some wavelengths,” he says.

Zhang says her group is now looking to extend the design for bigger objects and for microwaves. “In microwave frequencies…we [may be] able to achieve even bigger object-to-cloak ratios,” she says.

The research is published in Optics Express 19 8625.

Keeping a close eye on the future

The Optical Society of America (OSA) was founded in 1916 with the mission “To promote the generation, application, archiving and worldwide dissemination of knowledge in optics and photonics.” Based in Washington, DC, it has a staff of about 130 and an annual operating budget of around $30m (€21m). With more than 16,000 members in 95 countries, including some 220 active student chapters in 48 countries, the OSA serves about 100,000 optics professionals globally. Christopher Dainty is the society’s current president; he is also professor of applied physics at the National University of Ireland in Galway. In recent years his research has focused on adaptive optics and other aspects of imaging.

How would you assess the current state of optics science and technology, both in academia and industry?

Very healthy indeed! Optical science ranges from the fundamental to the highly applied, and there have been many examples in recent decades of fundamental science leading to applications – think of lasers, fibre optics and detectors. There is a huge optics and photonics industry, with sales estimated by the industrial association Photonics 21 to be about €270bn a year. In Europe, photonics has recently been elevated to the status of a “key enabling technology”, along with the usual suspects of nanotechnology and biotechnology. In short, optics is thriving.

What do you see as the OSA’s role within the international optics community?

The OSA publishes some of the world’s top-rated journals in optics and photonics, and with 80% of our authors coming from outside the US, it is de facto a global organization. More than half of our student members are also from countries other than the US. In fact, students and recent graduates are particularly well served by the OSA, with many grants, leadership and global networking opportunities available.

What do you see as the main challenges facing those involved with optics science and technology? How can the OSA’s initiatives help address those goals?

The challenges facing those working in optics are really the same as for those working in many other fields of science: keeping up to date with the latest developments; and effective publishing, networking and collaboration on a global scale. And as in many other fields, professional societies such as the OSA help to meet these goals. The OSA focuses in particular on its peer-reviewed journals and publishes or co-publishes 15 titles in different sub-fields of optics, including the leading open-access journal Optics Express. We are leading the way in many new developments in publishing – for example, “interactive science publishing”, where authors can publish multidimensional data sets that readers can interact with and interrogate. The OSA also organizes a limited number of high-quality peer-reviewed topical meetings around the world and co-organizes major conferences such as the Optical Fibre Conference (OFC) and the Conference on Lasers and Electro-Optics (CLEO).

How does the OSA plan to develop?

At present the OSA is working to serve optics professionals more effectively wherever they may be in the world. China, India and South America are three areas where the growth of all science and technologies is advancing rapidly. The OSA wants to help everyone in optics realize their potential for personal development, whether it is in teaching, research, industry or government. We try to do everything to the highest possible standards. In publishing we are focusing on new technologies, such as XML, and on the challenges of open-access publishing, where we already have a lot of experience.

What aspects of basic science do you think will have the biggest impact on optical science and technology over the next 20 years?

That’s a difficult one. During my 40-year career in optics, I’ve been wrong so many times I am probably the last person you should ask. But since you do ask, new optical materials have got to come near the top of the list. These will lead to new technologies and devices, which in turn will lead to new discoveries – I am a firm believer that science and technology feed into each other and are complementary. The laser was 50 years old last year, but I still think that new tunable low-cost lasers (costing a few euros) will emerge and enable all kinds of new applications. Imaging detectors, such as those based on CMOS technology, are also dropping in price and I believe that ubiquitous imaging (i.e. imaging every-where) will be with us in a decade. And who knows, even quantum computation might produce new consumer devices. One thing I am certain of is that basic physics, chemistry and maths are key disciplines that will underpin advances in optics in the foreseeable future.

Optical sensors boost space science

Andor Technology and e2v are two firms that excel in the design and manufacture of optical sensors. While e2v has carved a niche in space science, Andor has made great strides in developing imaging systems for the biological sciences.

In 1996 the UK-based optoelectronics company e2v entered the space race when it created digital cameras for the Envisat mission of the European Space Agency (ESA). Envisat was launched in 2002 with two charge-coupled devices (CCDs) from e2v and since then the firm’s sensors have been launched aboard an impressive list of space missions. These include NASA’s Messenger mission to Mercury, which uses e2v’s sensors in its Mercury Dual Imaging System (MDIS).

Comprising a multispectral wide-angle camera and a monochrome narrow-angle camera, MDIS is used to map the surface of the planet in monochrome, colour and stereo. It has been used to acquire 1200 images during each of Messenger’s three fly-bys of the planet since the mission launched in 2004. In March Messenger began to orbit Mercury and e2v’s cameras supplied the first close-up images of the planet.

Beyond our solar system, much of what we know about planets orbiting stars other than the Sun (exoplanets) comes from e2v devices on ESA’s COROT and NASA’s Kepler satellites. Also, the latest dramatic images of the Sun from NASA’s STEREO mission were obtained in part using e2v’s CCD devices.

Founded in 1947 and based in Chelmsford, e2v is a publicly traded company with 1600 employees, a third of whom are scientists and engineers. The firm has annual sales of about £201m (€227m) and 13 major locations worldwide. The company first started making CCD sensors about 30 years ago, and according to Jean-Francois Bruyeres from the firm’s Space & Defence Imaging division, e2v specializes in customizing CCD technology for use in space. This involves removing nearly all of the semiconductor material from the back of the CCD device, allowing light to enter via the back and straight into the optically sensitive region.

Special coatings

The CCDs are also coated with different films, making them sensitive to light at different wavelengths from the near-infrared through the visible and ultraviolet up to soft X-rays. So where will the next images be coming from? Bruyeres says e2v has signed a major contract to supply 100 sensors for the ESA’s Gaia mission, which will launch in 2013. Gaia will study about a billion stars and also look for exoplanets.

Back on Earth, UK-based Andor Technology has created devices that allow scientists to watch the inner workings of living cells at a length scale of about 100 nm – which is not possible with conventional optical microscopes. Belfast-based Andor spun out of Queens University in 1989 and employs more than 200 people in 15 offices worldwide. It had a turnover of £42.7m in 2010. The firm makes more than 70 products, including its electron multiplying charge-coupled device (EMCCD) optical sensors. The EMCCDs can be used as part of a system that can resolve tiny features in living cells. It works by firing a beam of light at the boundary of two media with different indices of refraction – say a glass slide and water. The angle of incidence is chosen such that all of the light reflects back through the glass.

The electromagnetic field of the reflected light extends about 100 nm into the water, where its intensity decays exponentially. This “evanescent” light forms the basis of total internal reflection fluorescence (TIRF) microscopy. This evanescent light penetrates a very short distance into a single-cell organism placed on the glass slide. Organelles within the cell are labelled using special fluorescent molecules that emit light when bathed in the evanescent light. The fluorescent light can be detected some distance away using a microscope. As a result, the technique can be used to make high-spatial-resolution studies of the movement of organelles.

The fluorescent light is extremely dim and is therefore very difficult to pick out from background light and noise. Andor makes the technique possible thanks to its new iXon3 EMCCD camera. A CCD works by converting light to electrical charge. In an EMCCD the amount of charge is multiplied over several stages to enhance very weak signals. Andor and e2v have enjoyed success by pushing the limits of optical sensors in very different directions – showing how important such devices have become across a broad range of science and technology.

Optoelectronics: a green explosion

Green photonics is booming according to the US-based Optoelectronic Industry Development Association, which reckons this incredibly diverse global industry netted a colossal $57.9bn (€40bn) in 2008. In 2021 this is expected to rise to nearly $300bn and encompass just over half of the optoelectronic industry, says the association.

This rapid growth looks set to make the world a better place. For example, it promises to aid increased solar-cell deployment to boost clean energy generation, cut greenhouse-gas emissions and pollution, and ultimately lead to a more environmentally sustainable approach to producing electricity. Another consequence of the green photonics revolution could be improved public health, with light-emitting diodes (LEDs) starting to purify water and improve the treatment of skin conditions.

The area where green photonics is tipped to generate its biggest sales is flat-panel displays. Recently, TVs with liquid-crystal and plasma displays have nudged up household electricity bills. These technologies do not need any more juice than the cathode-ray tube per unit of screen area, but their screens are often larger, making them more power hungry. Customers can save energy by investing in laser-projection TVs: for 60–65 inch screens, plasma and liquid-crystal display (LCD) TVs typically consume 525 W, while an equivalent based on projection technology requires just 135 W. A cheaper green option is also tipped for huge growth: an LCD screen backlit with an array of LEDs rather than the conventional cold compact fluorescent lamp. This cuts electrical consumption by up to 60% for a 42 inch TV, according to Chinese screen manufacturer Chi Mei Optoelectronics.

Revolution in lighting

LEDs will also drive a revolution in general lighting. LED devices on sale today can deliver up to twice the efficiency of a compact fluorescent, and unlike this incumbent they are free from mercury. High prices are holding back sales – a 40 W equivalent with a good hue retails for $20 or more – but prices could plummet to $5 by 2014.

A robust evaluation of the environmental impact of any lighting source must consider the energy required for product manufacture. For LEDs, compact fluorescents and incandescents this equals about 2% of energy used during the entire life cycle, according to calculations made by German firm Osram Opto Semiconductors. “But you have to compare the lifetimes,” says Osram’s Berit Wessler. “LED lamps last 25,000 hours – two-and-a-half times as long as a compact fluorescent and 25 times that of an incandescent,” he explains.

An LED that is on for 4 hours a day should last 15 years, which means that lighting sources need no longer be thought of as consumables. This has already led developers of LED products to blur the distinction between the lamp and the light fixture – or luminaire. “At some time in the future people will buy luminaires, and due to the extremely long lifetimes they will not exchange the lamp anymore, because the LEDs are connected directly to the luminaires,” says Wessler.

Lightweight spectrometers

Photonics can also help to create a greener world by monitoring air quality. One company making such a product is Ocean Optics of Dunedin, Florida, which builds lightweight spectrometers that were widely used during the 2008 Olympics. “You can put an optical sensor inside a factory, traversing the smoke stack, and monitor emissions – we were a big part of that in Beijing,” says Jason Eichenholz from Ocean Optics.

Eichenholz says that one of the strengths of spectroscopy, compared with more traditional technologies for atmospheric monitoring, is the small size. “In the UK we are working with customers to do mobile sensing. They are able to put something that used to be the size of a small trailer into something the size of a briefcase,” he says. The spectrometer can be fitted on the top of a car, enabling comparisons of sulphur-dioxide and nitrous-oxide levels on different parts of the road.

To reduce emissions produced by cars and improve manufacturing throughput, Swedish car maker Volvo has been replacing its resistance spot-welding systems for assembling car body frames with laser-based versions. The optical approach cuts downtime because of greater reliability, and less metal is scrapped thanks to less variation in weld quality.

Reducing carbon-dioxide emissions

Volvo’s Johnny Larson says it is possible to shave a few kilograms off the weight of a car’s metal frame by optimizing its design for a laser process. This has knocked up to 2 kg off the XC60, and for every one of these models that clocks up 100 000 km, 24 kg of carbon-dioxide emissions will be saved.

Lighter cars that are less polluting, air that is monitored for public health, and LEDs that power more efficient displays and lighting are sure to drive up revenues in green photonics. But making more money will not be the only outcome – a better quality of life for all of us is also on the horizon.

African Astronomical Society debuts in Cape Town

The first astronomical society encompassing all of Africa has been formally launched at a meeting of the International Astronomical Union (IAU) in Cape Town, South Africa. The African Astronomical Society (AfAS) debuted at the Second Middle East-Africa Regional IAU Meeting on 14 April – just three years after the society was first proposed.

The ceremony was attended by astronomers from each of five regions of Africa: Northern, Southern, Eastern, Western and Central. There were also representatives from a sixth region designated as the African Diaspora. This society follows in the wake of the African Physical Society (AfPS), which launched last year.

Organize and connect

The aims of the AfAS are to organize and connect a community of astronomers, and to develop resources for astronomy and astrophysics throughout Africa. The American physicist Hakeem Oluseyi has been elected interim president of the society. Oluseyi is at the Department of Physics and Space Sciences, Florida Institute of Technology and has worked in Africa to promote astronomy.

According to its constitution, the main vision of the society is “to be the voice of the astronomy profession in Africa in order to promote and support research on the continent and to facilitate the use of astronomy in addressing the challenges faced by Africa”.

The AfAS will promote astronomy as a tool for socioeconomic development in Africa and plans to further the study of mathematics and physics at a school level in order to encourage students to pursue careers in astronomy. It will also advocate the production and dissemination of scientific works by African astronomers. To achieve these goals the society will collaborate with institutions like the IAU, AfPS, UNESCO and the US-based National Society of Black Physicists.

‘Outpouring of support’

“The AfAS has received an outpouring of support from astronomical societies, institutions and organizations worldwide,” said Oluseyi who is eager to usher in a new era for astronomy in Africa. “Of course there are still challenges despite the support that we have received,” he added. “One issue is that although computers are ubiquitous across Africa, high-speed Internet is not.” Regarding the popularization of astronomy, “a big challenge is in reaching students and the public in Africa’s rural areas”.

Oluseyi acknowledges that the current global financial scenario could make fundraising difficult. “Our approach is to put together the right people, do the good work, and continuously seek support and cooperation,” he told physicsworld.com. “As an individual, I worked in Africa for many years with several others and we had virtually no support. We have made progress, and we believe that ultimately we will win support and achieve even more.”

The AfAS has six different types of membership categories that extend from student memberships to honorary memberships to memberships for non-professional astronomers that any person interested in astronomy could apply for. As there are already a number of local astronomy groups and societies that exist in Africa, members of such groups have been encouraged to join the society. For example, the Ghana Association of Astronomy (GAOA) has been active since 2009 and some of its members have already joined the AfAS.

Supporting SKA

South Africa is currently one of the nations contending to be the site of the Square Kilometer Array (SKA), which will be a giant network of thousands of radio telescopes. “Supporting Africa’s SKA bid is a primary objective of the society and played a role in its inception” explained Oluseyi. “The impact of Africa’s selection as the host site of the SKA can not be overstated,” he added.

Would Africa not being chosen as the primary site for SKA affect the society in any way? “I’m sure that the AfAS membership and leadership will continue to work as hard as possible to support astronomy research and education in Africa regardless of the SKA outcome,” said Oluseyi. “The one thing that I can assure you, which will probably surprise most people in the Western world, is that the African people are as scientifically literate and talented as any people on Earth. However, the full potential of Africa’s minds is not being tapped. Having the SKA on African soil will raise the visibility of Africa’s many bright scientists and students at home and abroad.”

Transparent material opens a new window on solar energy

Researchers in the US have developed a new kind of organic solar cell that converts a small but significant fraction of the sunlight that falls onto it into electricity, while still allowing most of the visible part of that light to pass through. Thanks to this transparency, the team says that the cell could be mounted onto windows in buildings or cars in order to tap a currently under-exploited source of energy.

Most of today’s commercial solar cells are made from the semiconductor silicon. When photons with sufficient energy strike the silicon they create pairs of electrons and holes. An electric field created by adding impurities to the silicon splits the electron–hole pairs apart, which results in an electric current. However, the costs involved in processing the silicon mean that photovoltaic cells remain very expensive compared to other forms of electricity generation.

One alternative is plastic – or organic – semiconductors, which are much cheaper to work with and are also flexible and lightweight. However, in plastic solar cells the liberated electrons and holes bind strongly to one another, forming particle-like entities known as excitons. These excitons only break apart when they reach a “heterojunction”, which is the interface formed by making cells from two different organic materials. But because excitons tend to travel only very short distances before they self-annihilate, cells must be very thin for significant numbers of excitons to reach the heterojunction and generate a measurable current. This need for thinness makes the cells inefficient.

Exploiting excitons

Now, Richard Lunt and Vladimir Bulovic of Massachusetts Institute of Technology have turned the exciton problem on its head. They exploit the fact that the formation of excitons alters a material’s absorption properties. So rather than absorbing wavelengths more or less equally across a broad spectrum, as is the case in silicon, their prototype cell instead displays distinct absorption peaks. By combining the organic molecules chloroaluminium phthalocyanine and carbon-60, their cell absorbs light at infrared and ultraviolet wavelengths but has limited absorption at visible wavelengths. In other words, it is able to extract energy from the non-visible parts of the spectrum while leaving most of the visible light free to propagate.

The fact that the new device does not absorb appreciably at visible wavelengths makes it less efficient than opaque organic cells. However, say Lunt and Bulovic, it is more efficient that other kinds of transparent cell that absorb across the spectrum. As they point out, these other cells must be made very thin if they are not to become opaque and as a result have efficiencies of less than 1% when at least partially transparent. In contrast, they achieved efficiencies of up to 1.3% when transmitting at least 65% of the incident visible light and up to 1.7% for transparencies greater than 55%.

While these efficiencies are very low compared to the 22% of the best commercial silicon cells, the MIT researchers claim that they should be able to up the efficiency of their cell to around 12% by increasing the length of the heterojunction interface. They will do this by blending the two organic materials, and also by stacking a series of cells together, each absorbing at a slightly different position within the infrared spectrum (ultraviolet absorption provides a very small fraction of the cell’s output).

Rolling onto existing windows

They say that their cell could be coated directly onto the glass in new windows or onto a flexible substrate that is then rolled onto existing windows, pointing out that exploitation of existing window structures would lower installation costs compared with conventional solar cells. They estimate that they will need between five and ten years to commercialize their technology because uncertainties remain regarding the durability of organic cells.

Lunt acknowledges that while the new cell could allow private individuals and companies to exploit more of the sunlight that falls on their buildings, it will not avoid the need for other energy sources. “It will be one of the tools in the clean-energy tool box,” he says.

Martin Green, of the University of New South Wales in Australia, believes that organic photovoltaic cells will be used in niche applications, but he does not think that they can compete with mainstream cell technologies even if they are cheaper to manufacture. He argues that the savings obtained in the manufacturing process will be nullified by the extra costs, common to all photovoltaic technologies, needed to “field-safe, professional systems with a long field life.”

Green’s position is backed up by a recent report from US technology analysts Lux Research, which concluded that the low efficiencies and short lifetimes of organic photovoltaic cells will make them uncompetitive with crystalline silicon and inorganic thin-film technologies over the next decade.

The work is described in App. Phys. Lett. 98 113305.

Cleaning oil spills drop by drop

By Matin Durrani

If you want to get your research results noticed by us here at Physics World headquarters, you can always try e-mailing us a copy of your paper, preferably well before it’s about to be published.

But Burak Eral from the physics of complex fluids group at the University of Twente in the Netherlands has taken a novel approach in flagging his research to us — he’s sent us a three-minute Youtube video consisting of a series of Powerpoint slides put to music.

As you can see, his tactic has worked. The video describes how Eral and his pals have studied the morphology of a drop clinging to a cylindrical fibre — a problem first studied by Joseph Fourier in the late 19th century.

If you can bear Eral’s rather soporiphic choice of music, you’ll find that the drops can either surround the fibre symmetrically, like a barrel, or attach themselves to one side of the fibre, rather like a clam-shell. By using the technique of “electrowetting”, Eral’s team was then able to reversibly change which form the drops adopt — with what they claim is “previously unachieved precision”.

The work has its practical side too as it could potentially lead to a way to clean oil spills in the world’s oceans. Eral envisages creating special fibres that could be dropped into the affected, oil-damaged region. Although the oil would naturally tend to form barrell-shaped drops around the fibre, the drops could be forced into adopting the clam-shell shape, which are much easier to wash off from the fibre. The result: cleaner oceans with the oil drained safely away.

Eral is not, of course, the first physicist to find the lure of creating an educational video about their work. In fact, you can find plenty of these “video abstracts” at the New Journal of Physics — an open-access journal published by the Institute of Physics, which also publishes physicsworld.com.

Eral’s full paper about his work appears in the journal Soft Matter

Between the lines

Apocalypse eventually

The list of disasters that threaten life on Earth is long and varied. The list of books that have been written about such disasters, however, is even longer. With what is, in retrospect, spectacularly bad timing, we picked this month to review a trio of recent books that explores the science of disasters. Of the three, Armageddon Science: the Science of Mass Destruction is the most conventional. In it, the science writer Brian Clegg presents a tour of the science and history behind numerous possible doomsday scenarios, ranging from the unlikely (antimatter bombs and planet-eating black holes) to the all too real (climate change). Not all of them are covered in the same depth. For example, tsunamis, earthquakes, asteroid impacts, supervolcano eruptions, alien invasions and irradiation by interstellar gamma-ray bursts are all crammed into a mere 26 pages. In contrast, the chapter on nuclear weapons takes up almost a quarter of the book, and sections on nanotechnology and climate change are also relatively meaty. One reason for this emphasis may be the author’s own background: Clegg is a physicist by training, and he seems more at home with physics-related disasters than he does with geological ones. However, as the book’s thoughtful introduction and conclusion make clear, Clegg is also primarily interested in disasters that are in some sense caused by science, not merely explained by it. Noting that Marie Curie died of radiation-induced leukaemia, he observes that “scientists don’t always have a great track record in keeping themselves and others safe”. Apparently callous attitudes such as these – which Clegg links, tenuously, to the fact that many scientists exhibit mild symptoms of autism – have a detrimental effect on the way outsiders perceive the scientific community.

• 2010 St Martins Press £18.99/$25.99hb 304pp

A scientific conspiracy?

Large-scale US government support of scientific research was born in the Second World War. To keep federal dollars flowing in peacetime, scientists have repeatedly spread alarms about natural disasters such as asteroid impacts and climate change – the solutions to which, inevitably, involve more government-funded research. This, at least, is the argument put forward by James Bennett in The Doomsday Lobby: Hype and Panic from Sputniks, Martians, and Marauding Meteors. As this synopsis indicates, Bennett, a political scientist at George Mason University in Virginia, is actively hostile to government support of scientific research – or, as he terms it, “the federal appropriation dole”. However, readers who are thick-skinned enough to withstand repeated insults will find a few atoms of truth inside Bennett’s layers of anti-government ideology. As he points out, state-funded science is not always a benign matter: it has also meant despoiling large swathes of the American West with dams, subsidized mining and weapons testing. Moreover, it is true that in former times, science functioned tolerably well without state support. As Bennett describes in the book’s opening chapters, the rise of US astronomy in the early 20th century was funded almost entirely by philanthropists. Yet his privately funded scientific utopia has a fundamental flaw. One of the anecdotes he uses to describe it concerns a 19th-century “Society for the Diffusion of Useful Knowledge”, which built itself an observatory after selling more than 300 memberships at $25 each. That may sound commendably egalitarian, but it is worth noting (as Bennett does not) that when the observatory opened in 1845, $25 was worth as much to the average person as $12,300 is today, as measured by per capita GDP. The fact is that before the late 19th century, scientists were, overwhelmingly, either aristocrats or people who could persuade aristocrats to back them financially. Is that really a better system?

• 2010 Springer £22.99/$24.95pb 200pp

Things fall apart

What do the Tay Bridge disaster, a tense family game of Monopoly and the loss of vegetation in the Sahara have in common? According to Bristol University physicist Len Fisher, who uses each of them as examples in his book Crashes, Crises and Calamities, they all have something to tell us about “critical transitions”, which occur when a system “abruptly, without apparent warning…jump[s] to a very different state”. Sometimes, such transitions are obvious, as in the 1879 collapse of the rail bridge across Scotland’s Tay estuary, or a player overturning a Monopoly board in frustration. Others, such as desertification, are more subtle, and are preceded by characteristic signs that can – if properly interpreted – alert observers to impending change. The key point, Fisher writes, is that “to anticipate and deal with such disasters, we need to be able to predict the changeover point”. His book outlines three overlapping approaches for doing this. One of them, catastrophe theory, classifies transition-prone systems into distinct mathematical types – including one, the “cusp catastrophe”, that has variously been used to explain love–hate relationships and the behaviour of cornered dogs. The second approach, computer modelling, is useful for predicting the outcome of complex situations, while the third focuses on early-warning signs such as fluctuations in the population of an animal species. It is all fascinating stuff, even if the threads that bind Fisher’s examples together sometimes seem weak.

• 2011 Basic Books £13.99/$23.95hb 256pp

The dark-energy game

The universe is not like a clock, where well-understood parts tick in predictable ways, nor like a balloon expanding or contracting. It is in fact pushing itself apart with a strange kind of energy, and 96% of it is made of an unknown kind of matter. How we discovered this is the subject of The 4% Universe, which condenses the complex, messy and startling tale – people, science, instruments, events – into an easily digestible, fast-paced 243 pages. That is a startling achievement in itself. To the connoisseur of popular science, indeed, the way author Richard Panek tells the tale is as interesting as the events: half drama, half detective story.

The prologue begins with a one-page “wow!” moment. On 5 November 2009 scientists at 16 institutions around the world dropped their collective jaws as they seemed to catch a first-ever glimpse of an entirely new structure of the universe. Two pages follow explaining its significance. Referring to the year when Galileo first used the telescope to reveal entire new worlds previously unknown to humankind, Panek writes “It’s 1610 all over again.”

What follows in Act One is the story of how cosmology went from speculation to science: how astronomers discovered that the furniture of the universe was more than planets and stars, and was on the move to boot. The universe “had a story to tell”, Panek writes. “Instead of a still life, it was a movie,” he says. We learn how scientists uncovered this movie’s plot by peering over the shoulders of Act One’s two main characters: theoretical physicist Jim Peebles, author of the classic textbook Physical Cosmology on the physics of the early universe; and astronomer Vera Rubin, whose work on the galaxy-rotation problem pointed the way to the idea that the universe contains some amount of “dark” matter, invisible to present-day instruments.

Act Two introduces more characters and “the game”, in which two different teams of scientists vie to unravel the plot by finding distant “Type 1a” supernovae. The game is played with telescopes equipped with charge-coupled devices, which revolutionized astronomical photography, and with the Hubble Space Telescope, which peered into hitherto invisible corners of the universe, among other equipment. The first team, the Supernova Cosmology Project (SCP), was led by Saul Perlmutter and Carl Pennypacker, particle physicists at the Lawrence Berkeley National Laboratory who applied the tools of their trade to astronomy. In doing so, Panek observes, “[T]hey weren’t drifting towards a new discipline. The discipline was drifting towards them.”

The second team was known as High-Z, where Z is a term for redshift. Highly redshifted objects are among the oldest and most distant in the universe, meaning that they would bear the clearest traces of any expansion or contraction. High-Z‘s main members were Adam Reiss and Brian Schmidt, who hailed from Harvard University and viewed supernovae as their area of expertise. They saw the Berkeley group as being out to “beat them at their own game”. While SCP had a six-year head start, High-Z recruited the “old-boy network” to, in effect, beat the Berkeley group at beating them at their own game.

In 1997 the two teams converged – simultaneously, yet reluctantly – on two wild, toothfairy-like ideas: that the universe contained “dark matter they couldn’t see and [a] new force they couldn’t imagine”. In Act Three, all the main characters introduced so far in the drama gather at a meeting where the SCP’s results (picked up by discerning newspaper reporters) suggest that “SCP was beating [High-Z] at beating the SCP at beating [High-Z] at their own game”. Then High-Z outdid that by securing full credit in the media. The discovery of this new force – soon dubbed “dark energy” – became Science magazine’s “breakthrough of the year” in 1998.

The new idea – that the universe’s expansion is accelerating – both simplifies things, by explaining a lot of puzzling data, and makes them more complex, by raising a lot of questions.

In Act Four, SCP and High-Z make plans to hunt for answers to one question – dark matter – while struggling over credit for the other, dark energy. The existing picture of the universe turns “preposterous”. But as Perlmutter remarks on the final page of the book, what usually attracts physicists to their field is “not the desire to understand what we already know but the desire to catch the universe in the act of doing really bizarre things”. And so, at the book’s conclusion, while one chapter in astronomy ends, another begins.

Panek tells the story briskly yet warmly, capturing personalities and not overlooking controversies. He chooses characters carefully. Through Rubin, for instance, we not only learn about dark matter, but also what it is like to be a woman in science, literally balancing child and career: textbook in one hand, pram in the other. Panek also has a knack for summarizing developments concisely and efficiently, such as in the following passage about how astronomy became more specialized over time:

You couldn’t just study the heavens anymore; you studied planets, or stars, or galaxies, or the Sun. But you didn’t study just stars anymore, either; you studied only the stars that explode. And you didn’t study just supernovae; you studied only one type. And you didn’t study just Type 1a; you specialized in the mechanism leading to the thermonuclear explosion, or you specialized in what metals the explosion creates, or you specialized in how to use the light from the explosion to measure the deceleration of the expansion of the universe – how to perform the photometry or do the spectroscopy or write the code.

Inevitably, Panek makes some compromises, and the seams of his crisp storytelling occasionally show. Galileo is mentioned once too often, and Panek’s apothegmatic style can ring precious, as in this remark about the signal from a radio antenna: “[T]his time the source wasn’t a radio broadcast from the West Coast. It was the birth of the universe.” The reader sometimes feels manipulated, too. That “wow!” moment that kicks things off so dramatically in the prologue? You don’t find out until page 197 that it was phoney – not a discovery after all.

Another author might have explored why it initially seemed to be a discovery, why its announcement was hyped even after problems were uncovered, and what this says about science and scientists. But by this time, you are so absorbed in the story that you do not care that much. And the book does convey a good picture of scientists in the act of catching the universe doing really bizarre things – while also showing that this is why they took the job. Give this book to your non-scientist friends to show them what it is all about – and to fellow scientists as a model of how to write popular science.

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