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The return of supersolids

Predicted by Soviet scientists in the 1960s, supersolids possess the properties of solids and superfluids at the same time. New practical research from two independent groups suggests the hunt for this exotic state of matter may finally be up. Find out more here by reading this feature from the February issue of Physics World.

Hidden Figures behind NASA’s success, LEGO’s famous five women of space, seismic goal in Barcelona

Flight planner: NASA's Katherine Johnson now has a NASA computational facility named after her (Courtesy: NASA)

By Hamish Johnston

International Women’s Day was this week and to celebrate, we have published K Renee Horton’s review of the film Hidden Figures and the book by Margot Lee Shetterly that the film is based on. The book and film tell the true stories of African-American female mathematicians who worked at NASA and played a crucial role in America’s race into space during the Cold War. Indeed, they calculated the flight paths that would send Neil Armstrong to the Moon.

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Eco-friendly ultraviolet LEDs could zap disease

Light-emitting diodes (LEDs) that are efficient at producing deep-ultraviolet light have been created by Grace Xing, Debdeep Jena and colleagues at Cornell University in the US. The devices could be used to kill a wide range of harmful micro-organisms.

Deep-ultraviolet light has wavelengths between 200–280 nm and is particularly effective at penetrating tiny living organisms and killing them by disrupting their DNA. As a result, deep-ultraviolet light has been used for more than 100 years for controlling harmful viruses, bacteria, moulds and even dust mites. Today, most deep-ultraviolet sources are mercury vapour lamps. Although these devices are very good at what they do, mercury is a highly toxic substance and researchers are therefore trying to develop alternative sources of deep-ultraviolet light.

Low efficiencies

LEDs could offer a way forward, but creating sources that are bright enough to be of practical use has been a challenge. Boosting the efficiency of such devices involves making improvements in three main areas. The proportion of the electrical current passing through the device that makes it to the light-producing “active region” (the injection efficiency) could be increased. Once the electrons get to the right place, the proportion that actually creates light – the internal quantum efficiency (IQE) – could be improved. Finally, the amount of light that emerges from the device (the light extraction efficiency) could be boosted.

Conventional deep-ultraviolet LEDs are based on the compound semiconductor aluminium gallium nitride, but now the Cornell team has shown that devices made from atomically thin layers of gallium nitride and aluminium nitride have higher IQE and light-extraction efficiency. The team was also able to boost the injection efficiency of their LEDs by using a polarization-induced scheme for doping both the n and p regions of the device.

Record breaking

They made three different LEDs that create light with wavelengths of 232 nm, 246 nm and 270 nm. The 232 nm device is the shortest-wavelength gallium nitride LED ever made, beating the previous record of 239 nm set by a research group in Japan.

The next task for the team is to integrate their LEDs in a package that could form the basis of commercial deep-ultraviolet sources. “We do want to package it within the next few months and test it as if it was a product, and try to benchmark it against a product with one of the available technologies,” says Jena.

The devices are described in Applied Physics Letters.

Penguin spotting

Photograph of King penguins

By Louise Mayor

Those of you who enjoyed Peter Barham’s Physics World feature “Penguin physics” might have – like me – come away enamoured of these little creatures, but not imagining that you could contribute to penguin research yourself.

Imagine my delight then when I discovered that the team behind British Science Week (BSW), which starts today, has teamed up with Penguin Watch, a citizen-science Zooniverse project that is calling for volunteers. The volunteer activity involves looking at photographs and, in each one, marking penguins, chicks, eggs and other animals such as humans. These crowd-sourced data will then then help the University of Oxford project Penguin Lifelines to better understand how threats to the ecosystem disrupt the dynamics of resident wildlife.

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Flash Physics: Single-atom memory, black hole blew Fermi bubbles, polymer stabilizes ultrathin silicon

Single-atom memory is world’s smallest

Information has been stored in a single atom for the first time. The nascent binary memory was created by Andreas Heinrich at the Institute of Basic Science in South Korea and an international team. It uses a high-voltage signal from the tip of a spin-polarizing scanning tunnelling microscope (STM) to set the direction of the magnetic spin of a holmium atom on a nearby surface – so that spin-up corresponds to storing a “0” and spin-down to storing a “1”. The direction of the spin is read using a single iron atom that is located adjacent to the holmium atom. This involves using the STM tip to apply a radiofrequency signal to the spin of the iron atom, causing it to oscillate. The oscillation (Larmor) frequency of the iron atom is affected by the magnetic spin state of the nearby holmium atom, allowing the stored information to be read. Using this technique, the team showed that the direction of the spin is stable for several hours. Heinrich and colleagues were surprised to discover that two holmium atoms could be placed just 1 nm apart without their magnetic fields interfering. “There are no quantum mechanical effects between atoms of holmium,” says Henirich. “Now we want to know why.” This ability to pack the atoms close together could mean that the storage technique could be used to create high-density memories. The work is described in Nature.

Black hole blew Fermi bubbles six million years ago

Artist's impression of the two huge gaseous lobes on either side of the Milky Way

The supermassive black hole at the centre of the Milky Way had its last big meal roughly six million years ago. That’s the conclusion of a team of astronomers who used data from NASA’s Hubble Space Telescope to show that the last big object to be consumed by the black hole was a large clump of gas. The Milky Way’s supermassive black hole has the mass of 4.5 million suns and therefore any material that gets too close is drawn in by its powerful gravitational force. The material then swirls around the black hole until it is eventually consumed. However, the material can get so hot that some of the matter escapes along the black hole’s spin axis. Rongmon Bordoloi from the Massachusetts Institute of Technology in the US and colleagues believe that this happened to a large clump of gas six to nine million years ago, and the ejected matter created the huge lobes of material – called Fermi Bubbles – above and below the Milky Way. The team used observations from Hubble’s Cosmic Origins Spectrograph (COS) to analyse the ultraviolet light from 47 galaxy cores – called quasars – including the Milky Way. As the light travels through the bubbles it carries information about the gas speed, temperature and composition. The results provide a new insight into Fermi Bubbles, including how old they are. “We have traced the outflows of other galaxies, but we have never been able to actually map the motion of the gas,” says Bordoloi. The group also saw the presence of silicon and carbon – the fossil remnants of the stellar evolution. The research is described in The Astrophysical Journal.

Polymer coating stabilizes ultrathin silicon

Photograph of an extruded spiral made of polymer-coated silicon nanosheets

A new way of stabilizing sheets of silicon just one atom thick has been developed by researchers at the Technical University of Munich. Since it was first isolated in 2004, graphene has been shown to have a number of unique and potentially useful electronic properties. Many of these arise from the fact that the material is also just one atom thick, and as a result, physicists are keen to create other ultrathin materials with potentially useful properties. Silicon is an intriguing candidate because it is already widely used in electronic devices, and ultrathin sheets of the material have promising optoelectronic properties. Unfortunately, ultrathin sheets of silicon are extremely delicate and disintegrate when exposed to ultraviolet (UV) light. Now, Tobias Helbich, Bernhard Rieger and colleagues have embedded silicon nanosheets in a polymer to protect them from decay. “What makes our nanocomposite special is that it combines the positive properties of both of its components,” says Helbich. “The polymer matrix absorbs light in the UV domain, stabilizes the nanosheets and gives the material the properties of the polymer, while at the same time maintaining the remarkable optoelectronic properties of the nanosheets.” The team also created a photodetector by mounting several of the coated silicon sheets on a silicon-dioxide surface that is coated with gold contacts. The research is described in Journal of Physics D: Applied Physics.

 

  • You can find all our daily Flash Physics posts in the website’s news section, as well as on Twitter and Facebook using #FlashPhysics. Tune in to physicsworld.com later today to read today’s extensive news story on a new low-cost source of ultraviolet light.

‘Time crystals’ built in the lab

Two independent groups of physicists in the US have built what they describe as “time crystals” – systems of interacting particles that are driven by a periodic force but which appear to oscillate autonomously. These are not the same as the theoretical time crystal outlined by Nobel-prize-winner Frank Wilczek five years ago, which it was alleged could break time symmetry by oscillating indefinitely without any energy input. But the researchers report that their systems seem to break what is known as discrete time symmetry.

Wilczek put forward his idea in analogy with the highly ordered lattice structure seen in physical crystals such as salt or diamond. The laws of physics tell us that empty space exhibits a symmetry such that no point is different to any other, but crystals break this symmetry since their constituent atoms or molecules sit at very well-defined locations. Given that crystals exist in thermodynamic equilibrium, Wilczek wondered whether it might be possible for systems of particles to spontaneously form repeating structures in time, even in their lowest energy states.

In 2012, Wilczek argued that a time crystal could be created by applying a static magnetic field across a ring of quantum particles. These would then group together in clumps around the ring and rotate. But his proposal, which appears akin to a perpetual motion machine, proved controversial. Patrick Bruno, a theorist at the European Synchrotron Radiation Facility in France, published an analysis showing that the system would not be in its ground state, and that if it were, it wouldn’t rotate. Bruno’s critique was then generalized to show that such time crystals would be physically impossible.

A modest proposal

Undeterred, Wilczek and others recast the idea in a more modest form, such that the particles in the system do not exist in a true state of equilibrium. Such a “discrete time crystal” involves applying a set of periodic forces to a set of spins, such that the orientation of the spins oscillate at an integer multiple of the driving period. Rather than breaking time symmetry per se, this breaks the “discrete” symmetry already created by the driving fields. This is analogous to placing atoms of a different element at, say, every second or third atomic site on the surface of a crystal, which breaks the surface’s existing symmetry.

According to Christopher Monroe of the University of Maryland, who led one of the two experimental teams, these time crystals must have two particular properties if they are to be considered real, self-contained entities. One is “rigidity”, the ability to maintain a fixed oscillation period while external parameters – such as the driving period – vary. The other condition is that the system must not heat up, even though it requires energy to oscillate. “This allows us to drive the system, but have it remain in quasi-equilibrium,” he says.

These time crystals tick in a reliable way and have long-range correlations
Frank Wilczek, MIT

To create their time crystal, Monroe and colleagues used trapped ions. They exposed around a dozen strongly interacting ytterbium-ion spins to a sequence of periodic laser pulses. These pulses drove the system at a particular rate, while additional laser beams added randomness to each spin’s rotation – creating disorder that prevented the system from heating up. The researchers found that the oscillation period of the spins remained at the expected, fixed value – and, crucially, that it did so even when the pulse period changed slightly. “That is the smoking gun,” says Monroe. “It is a property of the system, like the fixed lattice of a crystal.”

Natural set-up

The other experiment, led by Mikhail Lukin of Harvard University, involved a less precise but more natural set-up. It consisted of nearly a million spins formed by impurities in diamond known as nitrogen-vacancy centres. The driving field in this case came in the form of microwave pulses, while the heat-suppressing noise arose naturally as a result of a random variation in the dipole interaction between vacancy centres. Here too, the researchers were able to oscillate spins at integer multiples of the driving period – twice and three times as long, in this case – which remained unaffected by changes to the driving parameters.

Chetan Nayak of Microsoft Station Q in California – who wrote a commentary to accompany two papers in Nature describing the work – says that the “rigidity” observed by the two groups provides evidence of discrete time crystals. But he says that the case will only become watertight when they show that the spin oscillations remain in phase for a period of time that is exponentially long compared with some parameter of the system, such as its physical length. “The next generation of experiments would have to overcome some technical hurdles to see this,” he says. “But I think that these hurdles can be overcome.”

Bruno, meanwhile, has a more basic objection. He argues that the latest results provide useful information in the study of non-equilibrium quantum systems, but that they fall a long way short of what he says would have been the “radical change of paradigm” accompanying a confirmation of Wilczek’s original theory. “For systems out-of-equilibrium, the spontaneous breaking of time-translation invariance, per se, is neither new, nor surprising, nor mysterious,” he says.

Wilczek, however, describes himself as “ecstatic” at the latest research. He concedes that the results do not constitute a “fundamental breakthrough in physics in the sense of rewriting the Standard Model, for example”. But he argues that being able to “spontaneously break discrete time symmetry” is “qualitatively new”. And he adds that the research could lead to practical applications, such as the development of a clock for quantum computers. “These time crystals tick in a reliable way and have long-range correlations,” he says.

Decoding the quantum horizon

At a fundamental level, the physical universe can be thought of as information. All the stuff we observe arises from chains of yes-or-no questions. This “it from bit” concept was introduced in 1990 by the theoretical physicist John Wheeler. Now, however, a new idea has arrived that is even more fundamental, where the universe is conceptualized in terms of quantum bits of information – “qubits”.

This radical “it from qubit” was the subject of a feature in the January issue of Physics World. Authors Patrick Hayden and Robert Myers describe how collaborations between the high-energy physics and quantum-information communities may hold the key to a unified theory of quantum gravity. Find out how to access that article here.

Proton therapy: the benefits and the challenges

By Tami FreemanPWebook-cover

Proton therapy is an increasingly popular treatment technique that uses beams of protons to accurately target and destroy cancerous tumours. A new Physics World Discovery ebook, Proton Beam Therapy, takes a close look at the physics of this cancer treatment, its benefits and the challenges associated with bringing this approach into the clinical mainstream.

The ebook is written by Harald Paganetti, director of physics research at Massachusetts General Hospital and professor of radiation oncology at Harvard Medical School. He is a pioneer in advanced Monte Carlo dose calculations for proton therapy, and is considered the world expert on the relative biological effectiveness of proton beams.

In the last few decades, proton therapy has transitioned from research laboratories into the clinical setting – making this publication particularly timely. There are currently around 60 proton therapy facilities worldwide, and this number is increasing rapidly. “Proton therapy is becoming a standard treatment option but there are still many challenges in terms of the physics, biology and clinical use of protons, which are summarized in this ebook,” Paganetti explains.

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Guest presenter shakes up the Physics World podcast

By James Dacey

 

Physics World podcast: Neutrino tour

 

Regular listeners of the Physics World podcast will have noticed that things have been a little different for the past couple of months. That’s because we’ve handed over the presenter mic to science communicator Andrew Glester, who has brought his own unique style to proceedings. Based in Bristol, UK, just a few kilometres from the Physics World HQ, Glester is a presenter and co-founder of Cosmic Shed – a podcast about science and storytelling, recorded in Andrew’s garden shed.

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Flash Physics: Women still under-represented in physics, paint-drying mystery solved, LIGO’s Ronald Drever dies

Women are still under-represented in physics

Internationally, women only represent 25% of researchers in the physical sciences, compared with 40% in health and life sciences. This is the finding of a new study published by Elsevier that examines the gender trends across 27 research areas in 12 countries during the periods 1996–2000 and 2011–2015. According to the work, while the past 20 years has seen a significant increase in the percentage of women in scientific research, with nine of the 12 countries now over 40%, the physical sciences are still dominated by men. For physics and astronomy in both the UK and US, around 22% of researchers were women in 2011–2015. Although this is an increase from 15% during 1996–2000, women are still under-represented. Portugal, meanwhile, has the best ratio of women to men in physics and astronomy, with 37% of researchers being female. The team behind the study hopes that the empirical evidence will help governments, funders and institutions worldwide as they develop gender-balance initiatives. "[The report] will enable us to explore ideas about the causes of gender inequality in science," explains Uta Frith of University College London in the UK, who provided guidance for the report. The study, which is freely available online, used high-quality data sources including Elsevier's SciVal and Scopus, and the World Intellectual Property Organization (WIPO).

Mystery of drying paint cracked by new calculations

Diagram showing how larger particles eschew the air interface as paint dries

Last year, physicists made the surprising discovery that smaller particles in a layer of drying paint tend to move towards the air–paint interface, whereas larger particles move towards the surface being painted. This upended conventional wisdom, which suggested that smaller particles (which experience more random motion than larger particles) are more likely to diffuse away from the air interface. This response was expected to be driven by increased particle concentration near the air interface that is caused by evaporation. Now, Jiajia Zhou, Ying Jiang and Masao Doi at Beihang University in Beijing have come up with an explanation for why particles stratify in the opposite way. Writing in Physical Review Letters, they describe a model system that contains particles of two different sizes. The system is governed by the standard diffusion equation as well as an interaction between particles of different sizes. Their calculations suggest that the large particles do not tend to move towards the air interface because their size makes it difficult for them to push their way through the region of high particle concentration. This restricted mobility also features in a popular explanation of the "Brazil-nut effect", whereby larger nuts in a shaken tin of mixed nuts tend to congregate at the top of the tin. The research could lead to the development of new techniques for creating layered structures – and better paint.

Gravitational-wave pioneer Ronald Drever dies

Photograph of Ronald Drever

The Scottish physicist Ronald Drever, a key person behind the direct detection of gravitational waves, has died at the age of 85. Drever was born in 1931 in Bishopston, Scotland, and after studying a BSc in physics at the University of Glasgow, he graduated with a PhD from the same institution in 1958. Drever continued to work at Glasgow, setting up a research group on gravitational-wave physics and began building a prototype detector. In 1979, Drever then moved to the California Institute of Technology, where he worked on a gravitational-wave programme with the theorist Kip Thorne. Together with Rainer Weiss from the Massachusetts Institute of Technology, the trio co-founded the Laser Interferometer Gravitational-wave Observatory (LIGO), which is located in Hanford, Washington and Livingston, Louisiana. Drever retired in 2002 and his death comes just a year after LIGO announced the first direct detection of gravitational waves.

 

  • You can find all our daily Flash Physics posts in the website's news section, as well as on Twitter and Facebook using #FlashPhysics. Tune in to physicsworld.com later today to read today's extensive news story on how a time crystal has been created in the lab.
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