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Computing in a chilly Beijing

Peking University campus

By James Dacey

Today is my first day in Beijing and boy am I glad I packed my winter coat. Despite the clear blue skies, it was just above freezing point as I arrived at the Beijing Computational Science Research Center (CSRC) this morning, with an icy wind bringing an added chill factor. I was with my IOP Publishing colleague Tom Miller as we were delivering a presentation about scientific publishing and journalism and our taxi driver decided that 2 km from the venue was as far as he fancied going. So a brisk walk later we arrived with chattering teeth in need of a thorough thaw.

Located a few kilometres north-west of Beijing’s centre, the CSRC is within the Zhongguancun hi-tech zone. The majority of buildings within the technology hub are occupied by commercial firms, and our icy walk took us past the impressive modern offices of Baidu and Lenovo among other companies. The CSRC, however, is focused primarily on the application of computational modelling to fundamental science research. Its seven divisions include physical systems, quantum physics & quantum information, and materials & energy.

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3D cosmic-microwave background, iPhone paper and Dance Your PhD winner

https://youtu.be/3GSwl21-ZwI&rel=0

By Michael Banks

It might look like a kind of dumpling at first sight, but upon closer inspection the eagle eyed might spot that it is actually a 3D version of the cosmic microwave background (CMB) – the thermal remnant of the Big Bang that came into being when the universe was only 380 000 years old. The model was created by physicist Dave Clements from Imperial College London who says that detailed maps of the CMB – created by space telescopes such as the European Space Agency’s Planck satellite – are difficult to view in 2D. (more…)

Building-block metamaterials shape 3D acoustic holograms

Researchers in the US have created a printed array of metamaterials that can produce passive 3D acoustic holograms from a simple sound source, such as a single speaker. The device is made up of 3D-printed Lego-like blocks that can be put together in different configurations. The researchers say that their method is cheaper and simpler than other techniques and that they expect it to “open a new realm of holographic acoustic wave manipulation”.

A visual hologram manipulates electromagnetic waves in the visible part of the spectrum to create a 3D image. Because sound also travels in waves, it should be possible to create complex 3D fields of sound – acoustic holograms – in a similar way. While visual holograms can be made with physical structures that diffract light, it isn’t so easy with sound due to a lack of materials with the required acoustic properties. Generally, acoustic holograms use a transducer array controlled by complex phase shifting electronics.

Shifting sound

The new device created by Steve Cummer, an electrical and computer engineer at Duke University in North Carolina, US, and colleagues uses metamaterials to create a physical structure that can shift sound waves into the required 3D shapes. Metamaterials are engineered materials that have structural properties that don’t usually occur naturally. They are used to control and manipulate light, sound and other physical phenomena.

The device is made up of a range of 12 3D-printed plastic blocks, or “cells”. Each cell contains a different labyrinth pattern that is designed to modulate the phase of an acoustic wave. They work at a frequency of 4000 Hz and the 12 cells cover 180° of relative phase delay. A double layer of the cells can produce 360° of relative phase delay.

Cummer told physicsworld.com that although printing the cells was “time consuming,” fabricating each individual piece was “straightforward”. The more challenging part, he added, “was actually designing the components so that each one manipulates sound in precisely the way we need”.

Wave patterns

The cells slot together and can be rearranged to create different wave patterns. Once built, the array is placed in front of a single speaker and the acoustic hologram is produced on the other side. The construction of the array was aided by numerical simulations that show how the cells individually affect sound waves and how they act in combination. The researchers tested two different holograms. First, they used the array to project sound in a letter “A” pattern 30 cm from the hologram. Then they rearranged it to produce three circular hot spots of sound of different diameters.

Cummer says that although the goal was to “simply demonstrate a new concept”, now they have established that it is possible they are “thinking hard about where the idea might be deployed”. One possible application is the creation of “an acoustic hologram that converts the sound from a single speaker into the much more complex sound field created by an orchestra”.

It could also potentially be used for medical imaging. The transducer arrays used in ultrasound devices allow the acoustic field to be adjusted during imaging. While the new technique does not offer this level of control, it could be used for simple imaging if “you knew the depth of the object you were trying to image”, Cummer says. Such devices would not be as capable as current ultrasound imaging systems, but they would be cheaper and “orders of magnitude less complex”.

Reconfigurable holograms

Bruce Drinkwater, professor of ultrasonics at the University of Bristol in the UK, says that “this is a really nice idea. Arrays are expensive, particularly the electronics required to drive them. This paper makes beam-forming much easier and cheaper.” Discussing its potential application for medical ultrasound, Drinkwater says that “[transducer] arrays are still the gold standard” but “if you want to perform a fixed beam-forming operation – e.g focus on a specific tumour on a specific patient – this idea is perfect.”

The device as tested does not work at ultrasound frequencies, but Cummer says that scaling it up or down to work at different frequencies “should be pretty straightforward”. “The challenge of scaling down for higher frequencies like ultrasound is simply manufacturing the components in a much smaller size. 3D manufacturing approaches are evolving very quickly, and we are working with colleagues with experience in this area to do exactly this.”

Cummer adds that they would also like to “be able to show the same kind of dynamic sound-field manipulation with a single source and reconfigurable hologram” as has been shown with transducer arrays. “We are working towards that.”

The work is published in Scientific Reports.

Flash Physics: Particle pioneers bag J J Sakurai Prize, Brian Bowsher appointed new head of STFC, colliding light waves may create magnetic monopoles

Particle-physics pioneers bag J J Sakurai Prize

The American Physical Society’s J J Sakurai Prize for Theoretical Particle Physics has been awarded to Sally Dawson of Brookhaven National Laboratory, Gordon Kane of the University of Michigan, Howard Haber of the University of California, Santa Cruz, and John Gunion of the University of California, Davis, all in the US, for “instrumental contributions to the theory of the properties, reactions, and signatures of the Higgs boson”. All four winners also authored The Higgs Hunter’s Guide, an important book first published in 1989 that detailed the physics of the then-elusive Higgs particle. “It’s a great honour to receive this award with such distinguished scientists,” says Dawson. She also highlighted the importance of theoretical work, saying that “you never would have found the Higgs if you didn’t know what you were looking for. The searches were based on years of calculations and the detectors were designed to find this thing based on that theoretical work, which is still ongoing.” The quartet will receive their award, which consists of $10,000 to be shared and certificates citing their achievements, at a ceremony next January in Washington, DC.

Brian Bowsher appointed new head of Science and Technology Facilities Council

Brian Bowsher has been appointed as the chief executive of the UK Science and Technology Facilities Council (STFC) and will take up the post from next month. Bowsher will replace current head John Womersley, who has been appointed the next director-general of the European Spallation Source research facility. Bowsher was previously the managing director of the National Physical Laboratory, for more six years. “Bowsher is a highly respected scientist, with extensive experience leading world-class science laboratories, managing major science facilities and representing the UK on an international stage,” says science-minister Jo Johnson. “As a member of the STFC Council, he is already familiar with the organization, making him the ideal person to promote the UK’s scientific expertise and extend our international collaborations.” Bowsher received his PhD in inorganic chemistry from the University of Southampton in 1981, and has published extensively on materials, chemistry and nuclear-fuel issues. “It is an honour to be asked to lead the STFC and drive scientific research with our partners, both in the UK and internationally,” says Bowsher, who was first appointed to the STFC Council in May 2013.

Could colliding light-waves create magnetic monopoles?

Magnetic monopoles may form via wave-wave collisions

Ever since famous physicist Paul Dirac first predicted the existence of magnetic monopoles in 1931, physicists have looked high and low for these elusive particles. Dirac predicted the existence of a monopole as a way of explaining electric-charge quantization and finding them could help researchers to move towards unifying fundamental forces. Indeed, scientists have looked everywhere from particle accelerators to polar rocks to “spin ices” and have even tried creating them in the lab – all of the searchers in nature have ended in vain. Now, theorist Tanmay Vachaspati from Arizona State University in the US says that monopoles may form via wave collisions of force-carrying particles like photons. He calculated that it may be possible to see signatures of monopoles emerging from the collisions of two circularly polarized, high-intensity laser beams. Vachaspati’s simulations showed that monopoles formed as cratered peaks in the energy density in the wake of a head-on collision and that isolated North- or South-Pole magnetic fields formed around the peaks. The research is published in Physical Review Letters.

 

  • 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 creating acoustic holograms.

Liquid flow in capillaries contradicts conventional wisdom

Fill a narrow glass capillary tube with water, then turn it horizontal. Conventional wisdom says that the water will remain inside the tube. But a group of scientists in Spain and the UK has found that when the internal cross-section of the tube has a certain shape – triangular or a squashed ellipse – the tube will empty, however narrow it is. This phenomenon could represent a new way to control flow in microfluidics. It might even already be exploited in nature, for example in plants or blood vessels.

Innocent question

The authors of a new paper first began thinking about the behaviour of liquid in a horizontal capillary tube about eight years ago, when mathematician Carlos Rascón of the University Carlos III de Madrid, Spain, and theoretical physicist Andrew Parry of Imperial College London, UK visited Dirk Aarts at the University of Oxford, UK.

Aarts was experimenting on the behaviour of colloid–polymer mixtures in slit-like capillaries, and he commented that at the end of the day’s work they’d turn the capillaries horizontal and see the meniscus slump. He asked his visitors the innocent question “Do you know what shape it is?” And the trio realized that none of them knew how to work that out.

Keeping it simple

The equilibrium shape of the meniscus comes from minimizing the total free energy of the liquid confined by the solid walls of the tube. It can have a range of shapes, from a simple sloped meniscus, to an s-shaped cross-section in which a “tongue” of liquid extends along the base of a capillary.

The 3D shape is not easy to calculate and so, in 2012, the researchers’ first step was to calculate a reduced-dimension solution. They showed that for a simple 2D slit (with a 1D meniscus) there is a critical slit width at which the meniscus length becomes infinite, meaning that the slit-like pore empties.

Solving the problem in 3D for an arbitrary capillary shape is much harder. Rascón and colleagues simplified the calculation by considering the energy needed to form a meniscus with a constant cross-sectional shape all along the tube: that is, one where the liquid “flattens out” and the tube empties. When this energy falls to zero, such a tube-emptying meniscus becomes stable. Using this method, the researchers could find the “emptying conditions” for a tube, which depend on parameters such as the contact angle of the bulk liquid with the wall (a measure of how strongly the wall attracts or repels the liquid), and the shape and width of the tube.

Surprise result

To the researchers’ surprise, they found that changing the liquid type and what the vessel is made of – which affects the contact angle – doesn’t have a big effect on whether a tube empties or not. Only for a narrow range of tube sizes does it matter at all; outside of this range, the tube will be filled or empty for any liquid.

The shape, on the other hand, matters a lot. For sufficiently flattened ellipse-shaped cross-sections, the tube will always empty, both for very small and very large contact angles, regardless of the tube width. In the former (hydrophilic) case, the strong liquid–wall interactions “pull” the liquid along the tube and out of the ends, while in the latter (hydrophobic) case, the very weak interactions mean that the liquid just “slips out”. This behaviour contradicts the conventional wisdom that very narrow horizontal capillaries will always hold onto their contents. “We could not believe what we were seeing in the maths,” says Parry.

“We all thought we understood how liquid can clog a very narrow tube, being incapable of flowing out no matter how we orient the capillary,” says Joseph Indekeu, a specialist on wetting at the Catholic University of Leuven in Belgium. But these results suggest that very narrow tubes may always empty for particular shapes of cross-section.

Capillaries with an equilateral triangular cross-section may also empty spontaneously, the researchers find, but the precise conditions for it depend on the orientation. Such behaviour has been discussed previously by applied-mathematician Robert Finn of Stanford University in California, US, who in 2011 showed that a tube with an “ice-cream-cone” cross-section – round at the top, sharply V-shaped at the bottom – will empty even in the absence of gravity, thanks to capillary forces alone. He and others have a patent on an “astronaut’s drinking cup” based on this principle. There is, says Finn, a “moderately substantive” body of work on the question of capillary emptying in the fluid-dynamics literature, partly to understand the question of how liquid “plugs” might block flow down narrow tubes.

Shape-based switches

The researchers say that such findings might be put to use in microfluidic technology. A change in shape of the tube (such as flattening of a circular cross-section) might induce flow – a kind of “pumping” – without requiring any change in fluid pressure. “I like very much the possibility of ‘lock and go’ switches, akin to traffic lights, for directing liquids in networks of capillaries, operated by simply rotating non-cylindrical tubes around their axes,” says Indekeu.

It’s possible too, says Parry, that examples of flow controlled by geometry might appear in nature, for example through changes in the shape of blood vessels or the v-like grooves of leaves and folded membranes.

The research is published in PNAS.

Flash Physics: CubeSats could soon self-propel, ALMA unveils the birth of stellar siblings, patent award for US plasma lab

CubeSats could soon have on-board propulsion

CubeSats – small, low-cost satellites – could soon become self-propelled, thanks to a rocket-motor concept developed by researchers at Los Alamos National Laboratory in the US. While CubeSats are a cheap and easy way for relatively small research groups to launch satellites and access space, they traditionally do not have any on-board propulsion system – the nanosatellites are usually launched via a larger satellite and simply released into a specific orbit. “The National Academy of Sciences recently convened a meeting to look at science missions in CubeSats,” says Bryce Tappan, lead researcher of the CubeSat Propulsion Concept team, “and identified propulsion as one of the primary categories of technology that needs to be developed.” Recently, the Los Alamos researchers successfully tested a six-motor CubeSat-compatible propulsion array and according to Tappan, they are very close to being able to take the next step and show that the propulsion system works on a satellite in space. One of the main problems with CubeSat propulsion is that of safety – the fuels used in any such system are intrinsically hazardous ones such as hydrazine, and as multiple CubeSats are deployed by piggybacking on a larger mission, even a small margin of risk can be disastrous. To avoid these issues, Tappan’s team is developing a solid-based chemical-fuel technology – called a “segregated fuel oxidizer” system – that is completely non-detonable and where the solid fuel and solid oxidizer are kept completely separate inside the rocket assembly. The ability to self-propel would expand the capabilities of CubeSats, allowing them to enter higher orbits and achieve multiple orbital-planes in a single mission, and could also be used to make them “de-orbit” when their mission ends, reducing space junk.

ALMA unveils the birth of stellar siblings

Astronomers have spotted a relatively rare triple-star system surrounded by a disc with a spiral structure, using the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile. The discovery lends support to a proposed process known as “disc fragmentation”, which allows for the formation of young binary and multiple star systems – such a triple-star system forming in a disc has never been observed until now. “What is important is that we discovered that companion stars can form in disc material surrounding a dominant star,” says team-leader John Tobin at the University of Oklahoma in the US. “We had observed this system in the past with ALMA’s predecessors, but this is the first time we have been able to clearly analyse the disc and the newborn stars within it,” he explains, adding that “triple systems like this one are rare, and this is the only one with a configuration like this, but we are actively searching for more.” The work may help to explain how binary star systems form – something that astronomers are still not sure about. The research is published in Nature.

Patent award for US plasma lab

The Princeton Plasma Physics Laboratory team that invented a new way to produce technetium 99m

Researchers at the Princeton Plasma Physics Laboratory (PPPL) have won the 2016 Edison Patent Award for developing a new technique to create isotopes for medical imaging. The refrigerator-sized device can produce the radioactive element Technetium 99m (Tc-99m) – a substance with a half-life of six hours that is used in more than 60% of nuclear medical diagnostic procedures. Tc-99m results when Molybdenum 99 (Mo-99) decays – an isotope typically produced in a nuclear reactor. However, there has been a shortage of Tc-99m due to the closure or aging nuclear reactors worldwide. The technique developed by the PPPL researchers can produce Tc-99m from naturally occurring Molybdenum 100 (Mo-100). It involves firing neutrons at a metal plate to produce gamma rays that then strike a Mo-100 nucleus turning it into Mo-99. Due to the device’s size, the researchers say that that technique could allow many other countries to have access to Tc-99m imaging. “There was a lot of work that went into this and we’re just happy that we can potentially make a positive impact on helping people in the world who would not necessarily have access to this diagnostic technology,” says PPPL researcher Charles Gentile, who worked on the device. The prize will be awarded at a ceremony at the Liberty Science Center in Hoboken, New Jersey, on 3 November.

 

  • 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 the strange behaviour of liquids flowing in capillaries.

A toe-tally terrific trio

Photo of three Chatty Feet socks

By Matin Durrani

It’s not even Halloween yet and Physics World HQ has already received its first gift ideas for the Christmas season. Now most of us might roll our eyes if we were given a pair of socks for Christmas, but the footwear sent to us by UK firm ChattyFeet – slogan “Let the socks do the talkin'” – are sure to bring a smile to any physicist’s face.

The company has three different physics-related sock designs on offer, each depicting a cartoon image of a famous physicist and branded with a toe-totally amusing name. First up is a fetching blue number dubbed “Stephen Toeking” with the washing instruction: “Choose a slow spinning cycle to avoid a black hole.”

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The struggle for convergence

“Young man, if I could remember the names of these particles, I would have been a botanist.” Enrico Fermi’s reply to the unfortunate student who asked him the name of a certain subatomic particle came in the mid-1950s, when only a dozen such particles were known to exist. Within a decade, the number had swelled to nearly 100 as ever more powerful accelerators and detectors came online. But as Peter Watson explains in his latest book Convergence, although this proliferation in the number of particles “seemed counterintuitive at first, [it] would also help unify our understanding of certain aspects of the universe that had been beyond comprehension beforehand”. Indeed, it was not long before Murray Gell-Mann managed to turn what had become a nightmarish particle jungle into an ordered particle zoo, by devising a classification scheme called the Eightfold Way that grouped certain particles (the hadrons) into families of eight. In the process, this reorganization allowed the existence of undiscovered particles to be predicted.

Watson, a former journalist and a prolific (but always thought-provoking) historian of ideas, calls Convergence “a history of modern science but with a distinctive twist”. This twist, he claims, “has been there for all to see but so far it has not been set out as clearly as it deserves”. His main argument is that the various disciplines – despite their very different beginnings and apparent areas of interest – have in fact been gradually coming together over the past 150 years. Like Gell-Mann’s particle zoo in the early 1960s, these disciplines are “Converging and coalescing to identify one extraordinary master narrative, one overwhelming interlocking coherent story: the history of the universe.”

The two great unifying topics of the 19th century, Watson argues persuasively, were the conservation of energy and Darwin’s theory of evolution by natural selection. Each was the “fruit” of the coming together of the sciences: of heat, optics, electricity, magnetism and blood chemistry in the case of energy conservation; of geology, palaeontology, anthropology, geography and biology in the case of evolution.

Given this impulse to unite and simplify, Watson points out that physics has advanced when seemingly diverse phenomena have turned out to be different aspects of the same thing. Newton’s great discovery was that the same force that pulled the apple to the ground also held the Moon in its orbit around the Earth, and the Earth in orbit around the Sun. Magnetism, electricity and light were thought to be completely disparate phenomena until James Clerk Maxwell and Michael Faraday found that all were just different manifestations of electromagnetism. Albert Einstein’s theory of relativity grew out of his efforts to reconcile electromagnetism with classical mechanics.

It is hard to argue with Watson’s choice of Einstein’s unification of mass and energy and space and time as “the first great convergence event after the 1850s”. Max Born described Einstein’s masterwork as “the greatest feat of human thinking about nature, the most amazing combination of philosophical penetration, physical intuition and mathematical skill”. However, I do wonder how many would have chosen, as Watson has, Linus Pauling and his work on the nature of the chemical bond as one of their top three unifiers of the 20th century.

Watson also makes much of the Nobel laureate Steven Weinberg’s claim that convergence is “the deepest thing about the universe”. However, I find it remarkable that the “convergence of the sciences” (or, as Watson puts it “their synthesis, symphysis and coherence”) should be accorded such an accolade in the face of what those sciences have revealed to us about the nature of the universe and our place within it. It is widely accepted that when the universe was born in the Big Bang there was only a single force that soon shattered into four. Far from converging, these four forces have played largely separate roles ever since. The strong force holds the quarks together in the atomic nucleus. The weak force transmutes matter and makes the different elements. The electromagnetic force binds atoms and controls their chemical reactions. And then there is gravity, which has so far defeated all attempts to make it converge with the other three.

Weinberg was one of those responsible, in the late 1960s, for unifying electromagnetism and the weak force into the electroweak. Even so, I am surprised by his claim about convergence, which allows Watson to assert that “the most exciting intellectual breakthrough of all time” is “the way one science supports and interconnects with another, the beginning of a form of understanding like no other in history”.

Wherever experimental evidence can be coaxed out of nature, it suffices to corroborate or refute a theory and serves as the sole arbiter of validity. But where evidence is sparse or absent, other criteria, including aesthetic ones, have been allowed to come into play – both in formulating a theory and evaluating it. Watson believes that because of this, in some ways “physics has become mathematics”, arguing that we are currently “living in an in-between time, and have no way of knowing whether many of the ideas current in physics will endure and be supported by experiment”.

This, Watson explains, deeply worries the likes of cosmologists Joseph Silk and George Ellis. At the end of 2014, Silk and Ellis argued in a Nature comment piece that some scientists appear to have “explicitly set aside” the need for experimental confirmation of our most ambitious theories, “so long as those theories are sufficiently elegant and explanatory”. They further complain that we are at the end of an era, “breaking with centuries of philosophical tradition” of defining scientific knowledge as empirical.

As Silk and Ellis point out, this situation has come about because particle physicists have struggled to go beyond the Standard Model. Their most prominent attempt has been the theory of supersymmetry, but the problem is that no supersymmetric particles have been found, and Silk and Ellis fear that its advocates will simply “retune” their models “to predict particles at masses beyond the reach of the LHC’s power of detection”.

The result, Watson writes, is “a discernible sense of crisis”. The problem with a process of convergence, as he acknowledges, is that it presupposes a final end point. So while it may be true that “convergence is happening all over the sciences”, he admits, “The problem in physics is that it may be just too expensive to build the equipment that might bring that final convergence about.”

  • 2016 Simon & Schuster £25.00hb 544pp

Web life: Precarious Physicist

So what is this site about?

If teaching physics to undergraduate students strikes you as a secure, well-respected and at least somewhat highly paid job, the Precarious Physicist blog will challenge your assumptions. Its author, Andrew Robinson, is one of a large and growing number of university lecturers who work on short-term contracts with relatively poor pay, high teaching loads and little prospect of permanent employment. Or, as Robinson puts it: “Hello. My name is Andrew. I am 54 years old, have a PhD and I have a crap job in academia.”

That’s…blunt.

Indeed. But it’s also hard to disagree. As Robinson explains, his job as a contract instructor in physics at Carleton University in Ottawa, Canada, is “completely casualized labour. I have to reapply for my own job every four months; I have very poor benefits compared to tenured staff; I have no promotion or career development prospects at all”. By his calculation, Robinson also teaches “twice as many courses as tenured staff for around a third of their salary”, and although he has won awards for his teaching, he feels that his opinions on pedagogy “do not matter” to the university.

If it’s that terrible, why doesn’t he quit?

In part, it’s the students, who Robinson describes on his blog as “wonderful…the only reason I still do this job”. But there are personal factors, too. Robinson is originally from the UK, but he moved to Canada after his Canadian wife got a tenure-track job in physics at the University of Saskatchewan. “We had the classic two-body problem,” Robinson told Physics World. “I got into teaching by accident.” Asked to cover his wife’s physics course when she went on maternity leave, he discovered that he liked teaching and was good at it. Later, Saskatchewan gave him annual contracts to teach large lecture courses for first-year students – a job he describes as “a good match”. After a few years, however, their second child’s health problems forced them to move to be near family in Ottawa. Once there, Robinson found that conditions for contract teaching staff were much less favourable than those he’d experienced previously, but “there aren’t really any other jobs for a 50-something PhD scientist in Ottawa”, he says. In Canada, he adds, “a PhD is regarded much more as training to be a professor than it is in the UK or Europe”.

What topics does it cover?

In addition to the “crap job in academia” post quoted above, Robinson has analysed how his stipend and benefits stack up against those of his tenured or tenure-track colleagues (badly); skewered an essay that advised faculty to step away from the “frantic pace” of modern academia (“I don’t have this luxury”); and discussed the financial disincentives of trying new things in his classroom (“a huge uncompensated task”). But he also regularly writes about physics teaching, and his posts on this topic are as kind and patient as his diatribes against his employer are pointed and sarcastic.

Why should I visit?

Numbers of “contingent” (that is, neither permanent nor potentially permanent) faculty have been rising for years in many parts of the world. According to the American Association of University Professors, more than 70% of university-level instructors in the US are now in non-tenure-track jobs. Looking at it from the university’s point of view, this trend makes perfect sense: contract or adjunct faculty are cheap, well qualified and often very good at what they do, so why would they hire anyone else? Economic arguments aside, though, Precarious Physicist makes a powerful case that the current system is both unfair and unsustainable, and Robinson is taking a risk by writing it. As he repeatedly points out, his employer could decide at any moment not to renew his contract. Under the circumstances, paying attention seems like the very least the rest of us can do.

What can we learn from ultrahigh energy cosmic rays?

Cosmic rays are streams of highly energetic particles arriving at the Earth from sources beyond the Milky Way galaxy. In this video, Gordon Thomson from the University of Utah in the US explains what this phenomenon can teach us about the nature of the cosmos. Specifically, Thomson introduces the Telescope Array experiment in Millard County, Utah, which observes the secondary radiation produced by cosmic rays interacting with particles in the Earth’s atmosphere. The experiment is being used to create a map of the sky to identify cosmic ray sources and investigate how they might be able to accelerate particles to such high energies.

This video is part of our 100 Second Science series, in which researchers give concise presentations covering the spectrum of physics.

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