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A tour de force of the cosmos

There is something rather strange about how physicists, both young and old, perceive science. I am sometimes confronted with the realization that I too am susceptible to a host of strange, if not pathological, notions: that science is pure and logical; that it is distant from the apparent caprice of more human-centred realms such as art or politics or sociology; and that this difference somehow makes science clean and ideal. However, the more I engage with the infrastructures of science – its reliance on both individuals and groups; its continuous need for advancing technologies; and the indelible effects of human rivalries, camaraderie and oversights – the more my notions of scientific idealism give way to a better understanding of scientific realism.

It is through this lens that I find Priyamvada Natarajan’s book, Mapping the Heavens: the Radical Scientific Ideas that Reveal the Cosmos, to be an instructive and thought-provoking exploration of the connections, tensions and mishaps that so often accompany scientific venture. The book delves into some of the most important and influential discoveries in cosmology – from exoplanets to dark energy and other universes. Through the stories of individuals and collaborations that have transformed cosmology, Natarajan – an astrophysicist at Yale University – attempts to blur the lines between the products of science and its human creators.

In doing so, she effectively renders modern physics and cosmology as an inherently anthropological search for answers to deep, fundamental questions. What is the Earth’s place in the universe? Is there a beginning and an end to all things? Is there more to our universe than we currently know? Indeed, Natarajan’s contemplations on various historical parables serve as a useful reference for today’s early-career scientists, who may find themselves in a state of uncertainty as they navigate the realms of “big science”, with its large collaborations and complex social structures.

On starting my first postdoctoral position at Cardiff University in the UK as part of the Laser Interferometric Gravitational-Wave Observatory (LIGO) collaboration, on 1 September 2015, I could not have predicted the historical observation we were to make a mere 13 days later. A gravitational wave, resulting from the collision of two black holes some 1.3 billion light-years away, rippled through the Earth and caused LIGO’s twin interferometers – in Livingston, Louisiana and Hanford, Washington – to squeeze and stretch by an infinitesimal but measurable amount.

It is expected that LIGO’s future observations will empower us to make novel contributions to many of the topics in astronomy and cosmology that the book explores. However, just as Natarajan traces the historical passage of astronomy and cosmology from fringe topics to venerated research fields, LIGO and its supporting communities are currently undergoing the process of mapping out an entirely new scientific subfield: gravitational-wave astronomy.

As LIGO scientists seek to define gravitational-wave astronomy with the insights gained from new observations, the field’s inherent ties to cosmology make Natarajan’s exploration valuable for any gravitational-wave enthusiast. This is perhaps not the most surprising claim, as gravitational physics – founded by Isaac Newton, and then reprised and strengthened by Albert Einstein – is the nexus for many stories in astronomy and cosmology. From the existence of black holes, to dark matter and dark energy, the impact of Einstein’s theory of gravity cannot easily be downplayed.

However, scientists may also often forget (either in exuberance over Einstein’s legacy or due to the seemingly deterministic nature of scientific progress) what Natarajan goes through a mildly repetitive exercise to reinforce: that not only do human biases impact the execution of science, but also they often impede and even obscure its progress as a whole.

Indeed, bias affects even the best of scientists, as Natarajan points out – Einstein’s long-held, incorrect belief in a static universe perfectly elucidates this point. The initial stubbornness of the astronomy community to accept the idea of dark matter, despite considerable observational evidence, shows how bias can affect entire groups. At the same time, Natarajan also describes how academic tensions and scientific scepticism go hand in hand with theory and evidence, to give way to and powerful consensus. Such agreement is the precursor to crucial, paradigm-changing discoveries that inevitably impact a scientific field, as well as the lives of every individual scientist.

Indeed, during my time at Cardiff, I have witnessed first-hand the changing trajectory of belief in a theory that results when heavy scepticism meets robust evidence. Looking back at an early staff meeting, a particular individual doubted the detectability of gravitational-wave signals and openly mocked the decades-long efforts of the group. It was quite interesting to see both heckler and advocate toast with champagne a few months later, after all arguments had been put to rest. Although I am certainly biased by my experiences as a gravitational-wave astronomer, I would recommend Mapping the Heavens to readers from middle-school level onwards and from a wide range of backgrounds. Any minor wrinkles in the text’s construction and style are outweighed by insights gained into modern physics’ history via Natarajan’s skilful writing.

  • Yale University Press 288pp £16.99hb

Web life: ParticleBites

So what is the site about?

As you may guess from its name and strapline, ParticleBites – “The high-energy physics reader’s digest” – presents the latest research updates in high-energy particle physics. The blog, which serves as an online particle-physics journal club, covers both experimental and theoretical research, with each post based on a recently published research paper that is available on the arXiv preprint server. ParticleBites’ main aim, much like its sister website AstroBites, is to make research more accessible to those starting out in academia, by simplifying research papers and making the science more accessible to undergraduate students. “For most people, it takes years for scientific papers to become meaningful. Our goal is to solve this problem, one paper at a time,” claim the creators. Each post is written such that not only is the new research explained, but its importance in the field at large is also provided, giving some much-needed context to current research, especially for those who are new to particle physics. The website has about six to eight posts a month and topics range from dark matter and supersymmetry to neutrinos and nuclear physics. There is also the odd post about outreach, science policy and rumours, all with a particle-physics twist.

Who is behind it?

By particle physicists and for particle physicists, the posts are written and edited by a team of graduate students and postdoctoral researchers, including 10 regular authors and the occasional guest author. ParticleBites was founded in 2013 by Flip Tanedo, the website’s editor, following the Communicating Science 2013 workshop, which was organized by Harvard University’s Nathan Sanders, who co-founded AstroBites. Tanedo – an assistant professor in theoretical physics at the University of California, Irvine – also serves as director, together with Julia Gonski – a PhD student in the high-energy experimental group at Harvard. Tanedo also created the ParticleBites logo, which depicts a gauge boson (a force carrier) “eating” a Goldstone boson (spinless particles associated with the spontaneous symmetry) and becoming longitudinally polarized. According to Tanedo, the cartoon “represents the part of the phenomenon of electroweak symmetry breaking, which plays a central role in the Standard Model of particle physics.”

Can I get involved?

Yes – if you are a PhD student or postdoc in particle physics. The website has a “Write for us” section, which says that “if you’re a particle physicist (broadly defined) with a passion for writing and science outreach, feel free to contact us about writing opportunities with ParticleBites”. Potential authors are expected to have a solid background in particle physics and are selected on the basis of a sample blog post. Authors are expected to write a new post every two to four weeks, as well as edit fellow writers’ posts. The team is also looking for undergraduate and graduate students who can get involved in editing and proofreading posts.

Can you give me a sample quote?

From a post published in September 2016, titled “Horton hears a sterile neutrino?”: “Neutrinos, like the beloved Whos in Dr Seuss’ Horton Hears a Who!, are light and elusive, yet have a large impact on the universe we live in. While neutrinos only interact with matter through the weak nuclear force and gravity, they played a critical role in the formation of the early universe. Neutrino physics is now an exciting line of research pursued by the Hortons of particle physics, cosmology and astrophysics alike. While most of what we currently know about neutrinos is well described by a three-flavour neutrino model, a few inconsistent experimental results such as those from the Liquid Scintillator Neutrino Detector (LSND) and the Mini Booster Neutrino Experiment (MiniBooNE) hint at the presence of a new kind of neutrino that only interacts with matter through gravity. If this ‘sterile’ kind of neutrino does in fact exist, it might also have played an important role in the evolution of our universe.”

Seven Earth-like exoplanets orbit nearby star

Artist's impression of TRAPPIST-1

The largest known system of Earth-like exoplanets has been found orbiting a dwarf star in the Milky Way. At least three of the seven rocky exoplanets could have oceans of water, making it possible that the system could harbour life. The discovery lends weight to the growing belief among some astronomers that our galaxy could be teeming with Earth-like worlds.

The first exoplanet – a planet orbiting a star other than the Sun – was discovered 25 years ago, and since then, astronomers have identified thousands of such objects. Most are Jupiter-like gas giants because huge exoplanets are much easier to detect than smaller Earth-like worlds. However, improved techniques and new telescopes have led to the discovery of Earth-like exoplanets with the potential to harbour life.

In 2010, an international team of astronomers began using the TRAPPIST telescope in Chile to search for Earth-like exoplanets orbiting small stars nearby in the Milky Way. They were looking for tiny drops in the intensity of a star that occur when an exoplanet’s orbit takes it between the star and Earth. Such “transits” of small exoplanets are much easier to see with dwarf stars because the change in intensity is large.

Rocky compositions

Just 40 light-years from Earth, they spotted a star they called TRAPPIST-1 that appeared to be transited by several exoplanets. Now, further observations – including 20 days of continuous monitoring using NASA’s Spitzer Space Telescope – have revealed seven exoplanets in the TRAPPIST-1 system. The exoplanets have orbital periods ranging from 1.5–20 days. All seven objects appear to be similar in size to Earth, with radii ranging from 0.77–1.13 Earth radii. The team was able to determine the mass and density of six of the exoplanets, which suggests that they have rocky compositions.

TRAPPIST-1 is about 80 times more massive than Jupiter. So instead of resembling the Sun and its planets, the system is similar to Jupiter and its four Galilean moons – according to team member Michaël Gillon of the University of Liege in Belgium. Gillon says that three of the planets orbit within the habitable zone of the star, which means that they could have liquid water and even life.

TRAPPIST-1’s nearness to Earth combined with the fact that the exoplanets are relatively large compared with the star means that it should be possible to study the exoplanet atmospheres. This would provide important information about chemical composition and the possibility of life.

Climate studies

According to Amaury Triaud of the University of Cambridge in the UK, the team is now trying to work out if the exoplanets are shrouded in envelopes of hydrogen – which would suggest that they are not Earth-like. The James Webb Space Telescope – to be launched in 2018 – will have the capability to study the composition of the exoplanet’s atmospheres and even their climates. “We could know if there is life in TRAPPIST-1 within a decade,” says Triaud.

TRAPPIST-1 is described in Nature. Hear Sara Seager explain how astronomers are searching for life on exoplanets in this podcast: Searching for life on other planets.

Flash Physics: ‘Queen of Carbon’ dies, LHCb spots rare B-meson decay, antineutrino detector is portable

“Queen of Carbon” Mildred Dresselhaus dies

The solid-state physicist Mildred Dresselhaus from the Massachusetts Institute of Technology (MIT) has died at the age of 86. Dresselhaus was born in 1930 in New York City and completed a bachelor degree in physics from Hunter College in New York in 1951. Following an MA from Radcliffe College in 1953, Dresselhaus was awarded a PhD in physics in 1958 from the University of Chicago, where she studied under the Nobel laureate Enrico Fermi. After a couple of years at Cornell University, she headed to MIT in 1960 where she remained for the rest of her career. Known as the “Queen of Carbon”, Dresselhaus made fundamental discoveries in solid-state physics, in particular studying the electronic structure of materials, including carbon, and was noted for her work on graphite, graphite intercalation compounds, fullerenes and carbon nanotubes. In 1985, she was the first woman to become a full-tenured professor at MIT, and Dresselhaus continued to promote gender equality in science and engineering throughout her career, co-organizing the first Women’s Forum at MIT in 1971. Dresselhaus won many awards including the National Medal of Science in 1990 and the Presidential Medal of Freedom in 2014 – the highest award bestowed by the US government on US civilians. In 2014, Dresselhaus spoke to Physics World about her career in science.

LHCb observes rare B-meson decay

Photograph at LHCb at CERN

The rare decay of a neutral B meson to two oppositely charged kaons has been observed for the first time by physicists working on the LHCb experiment at CERN. B mesons are created when protons collide in the Large Hadron Collider and the observed decay happens to fewer than one in 10 million B mesons. This is the rarest decay ever observed that involves just hadrons. Particle physicists study the decays of heavy-quark hadrons such as B mesons because these events could reveal new particles and interactions that are not described in the Standard Model of particle physics. In this case, however, the decay appears to proceed as predicted by several different schemes for performing quantum chromodynamics (QCD) calculations. The decay was measured with a statistical significance greater than 5σ and is reported in Physical Review Letters. In the same paper, the LHCb team also reports observing the decay of a strange B meson to two oppositely charged pions. This measurement differs somewhat from that predicted by some QCD calculations.

Mobile antineutrino detector could monitor nuclear reactors

Photograph of MiniCHANDLER being assembled

An 80 kg antineutrino detector called MiniCHANDLER will hit the road in April, when it will become the world’s second mobile antineutrino detector, after a similar device was unveiled in Japan in 2014. Built by Jon Link and colleagues at Virginia Tech in the US, The detector uses a solid scintillator that allows it to detect about 100 antineutrinos per day. Antineutrinos are discriminated from much more common background radiation by looking for both the proton and neutron that are produced when an antineutrino interacts with an atom in the detector. MiniCHANDLER is deployed in a trailer that could be parked next to a nuclear facility, where it would monitor the huge flux of antineutrinos created by nuclear fission within the reactor. Such measurements could, in principle, be used to determine what type of nuclear fuel is being used. This information could be used to ensure that a reactor is not being used clandestinely to create weapons-grade material. If MiniCHANDLER is successful, the team plans to build much larger portable neutrino detectors that could weigh as much as 1 tonne.

 

  • 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 exoplanets.

Brooklyn’s pioneering approach to art and science

After spending four days in Boston at the annual meeting of the American Association for the Advancement of Science, I travelled down by train to New York (gotta love those comfy Amtrak seats and free WiFi). I first hooked up with mathematical physicist Peter Woit at Columbia University and then with science philosopher Bob Crease from Stony Brook University, who’s been a long-time columnist for Physics World.

I was keen to find out if they’d be interested in writing for the new Physics World Discovery series of ebooks and, while at Columbia, I had also hoped to put the same question to astrophysicist and author Janna Levin, who’s based in the physics department. Turns out, however, that Levin is on sabbatical, spending a year as “director of sciences” at Pioneer Works in Brooklyn’s Red Hook district. Curious to find out more about a centre that seeks to “make culture accessible to all”, I accepted her invitation to pay a visit.

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Parents’ enthusiasm for science boosts teens’ exam scores

Teenagers with parents who conveyed the importance of science, technology, engineering and mathematics (STEM) had higher scores in mathematics and science-college preparatory examinations, a long-term US study has found. Talking to teenagers about the benefits of science boosted their exam results by as much as 12%, which in turn increased the number pursuing STEM-based careers.

The research was part of a longitudinal study that recruited families in the state of Wisconsin in 1990 and 1991 when mothers were pregnant. The STEM part of the analysis, led by psychologist Judith Harackiewicz from the University of Wisconsin–Madison, looked at 181 families from that cohort with students attending 108 different high schools.

Utility and relevance

These families were randomly assigned to either an “intervention” group or a control group. Parents in the intervention group were sent information about the utility and relevance of mathematics and science for high-school students. They received a brochure in the 10th grade – when students are 15–16 years old – and another brochure and access to a website in the 11th grade. Families in the control group received no material.

Previously, Harackiewicz and colleagues found that students in the intervention group took nearly an extra semester – half a school year – of mathematics or science classes in the last two years of high school, compared with the control group.

Parents are an untapped resource for promoting STEM motivation
Judith Harackiewicz, University of Wisconsin–Madison

In their latest study, the researchers found that the intervention increased mathematics and science scores in a standardized test for high-school achievement and college applications by 12%. They also found that at 20 years old, the students in the intervention group were more likely to take STEM classes in college, major in a STEM subject, desire a STEM career and value STEM, compared with the control group.

The researchers argue that the intervention improved STEM preparation, which influenced post-high-school choices. “Parents are an untapped resource for promoting STEM motivation – they know their teens and can help them connect course material to their lives,” says Harackiewicz, adding that parents “can have a major impact on their teens’ academic trajectories by helping them understand the importance of taking math and science courses in high school”.

The study is described in Proceedings of the National Academy of Sciences.

Flash Physics: Stellar family history, extremely sensitive electron camera, full-body PET scanner planned

Stellar family history

The family tree of nearby stars has been mapped by astronomers. Paula Jofré from the University of Cambridge and colleagues have applied biological principles to map how 22 stars are related to each other. In evolutionary biology, the DNA of living organisms allows scientists to map the route of evolution and determine the relationships between different species. While stars are very different to living creatures, they carry the chemical signature of the gas cloud they formed in, and will therefore share “chemical DNA” with other stars formed from the same cloud. Looking at 22 stars in our galactic neighbourhood including the Sun, the astronomers analysed chemical spectra taken by large telescopes in Chile, alongside data from the European Space Agency’s Earth orbiter, Hipparcos. Using computer algorithms, the team identified 3 groups of stars that share a common ancestor and six stars that were not statistically viable for any group. The researchers suggest that the thicker part of the Milky Way’s disc forms new stars more rapidly than other parts of the galaxy. Meanwhile, they also found that some stars may have originated from another galaxy that collided with the Milky Way in the distant past. The work, published in Monthly Notices of the Royal Astronomical Society, is a proof-of-concept study. Further datasets from Hipparcos’ replacement Gaia, more advanced telescopes and sky surveys, should allow astronomers to build a detailed stellar family history.

Electron camera images fragile metal–organic frameworks

Transmission electron microscope image of ZIF-8

An extremely sensitive electron camera has been used to obtain transmission electron microscope images of fragile crystals called metal–organic frameworks (MOFs). Comprising metal atoms connected by organic molecules, MOFs are highly porous materials that can be engineered to store or transport specific gases. Determining the structure of a MOF is crucial to optimizing its performance, but doing so using electron microscopy is challenging because electron beams intense enough to create a useful image will destroy most MOFs. Now, an international team of researchers led by Yu Han at KAUST in Saudi Arabia have imaged a MOF using an electron-counting camera developed by US-based Gatan, which was also involved in the study. According to Gatan, the camera is able to detect individual electrons – making it possible to take microscope images under extremely low electron illumination. The team acquired images of ZIF-8, which is a MOF made of zinc atoms connected by 2-methylimidazole molecules. The images have a spatial resolution of 0.21 nm, which allowed the team to see individual zinc atoms in columns as well as the organic linking molecules. Han says that the research has already revealed new information about the porosity of the material, “which influences gas molecules transport in ZIF-8 crystals”. The research is described in Nature Materials.

Consortium will build full-body PET scanner

Photograph of positron emission tomography scanner

Researchers at the University of California, Davis, are leading a collaboration to build a prototype total-body positron-emission-tomography (PET) scanner. The EXPLORER consortium hopes to have a small-scale version ready for testing by July and the full-sized prototype by mid-2018. PET scanners use radioactive tracers attached to molecules of interest to show how organs and tissues are functioning. PET scans are mostly used to diagnose and monitor cancer, heart disease and forms of dementia. To gain multiple organ views of diseases such as measuring the spread of cancer, for example, it is necessary to scan the whole body because metastatic cancer can appear at many different sites. The detector in conventional PET scanners only covers a small part of the body, so imaging the whole body involves moving the patient through the scanner. The small detectors also mean that only about 1% of the available signal is actually collected. Another limitation of existing scanners is that they cannot collect dynamic data showing how the radio tracer distributes throughout the body. The new full-body PET scanner should provide a 40 fold gain in effective signal, compared with current scanners. This, say the researchers, will dramatically improve imaging capabilities and quality, revolutionizing the ability to study and diagnose disease as well as also reducing patient radiation exposure, which would allow more frequent use of PET scans. “Total-body PET is going to allow the interactions between different systems to be studied, providing a whole-body system view of disease that is not readily provided by other technologies,” says project leader Simon Cherry.

 

  • 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 to encourage teenagers to study physics.

Optical clocks hit the road

Two independent groups of physicists in Germany and China have built portable optical clocks that are more accurate than the best caesium devices. They say that their instruments could be used to compare the timekeeping of different optical clocks distributed across the globe, and so take us closer to an overhaul of the SI definition of the second. They also reckon their compact clocks could be used by geodesists to determine the height difference between two widely spaced points on the Earth’s surface.

All atomic clocks rely on counting the oscillations of an electromagnetic wave with a frequency that is locked to that of a known atomic transition. Traditional atomic clocks use a microwave transition in caesium-133 to fix the output of a crystal oscillator, whereas optical clocks use much higher optical frequencies generated when a monochromatic laser beam interacts with various species of trapped ions or with clouds of cold atoms. These clocks now have accuracies and stabilities that are nearly two orders of magnitude higher than those of the best caesium devices – at levels of a few parts in 1018 rather than 1 part in 1016.

These improvements have led to calls for a change in the definition of the second within the SI system of units, from one based on the caesium-133 transition to another based on an optical standard. However, such a move requires a way of comparing the ticking rate of optical clocks located in different laboratories around the world – which is harder to do than a comparison of microwave frequencies.

Clock in a caravan

Now, Christian Lisdat and colleagues at the Physikalisch-Technische Bundesanstalt (PTB) in Braunschweig have shown how this could be done by making a compact optical clock that can be transported in an air-conditioned trailer. Their clock consists of several thousand neutral strontium-87 atoms that are held in place, cooled and excited by lasers. Lisdat says that among the main challenges involved in building the portable system were shrinking the laser systems for cooling and preparation of the atoms. Also difficult was to build a vacuum system for holding the atoms that is compact but at the same time doesn’t cause the lasers to misalign when it is transported.

Another major hurdle the group had to overcome, says Lisdat, was holding in place the optical cavity used to stabilize the frequency of the monochromatic laser that excites the strontium atoms. The kind of soft pads used to support the cavity in a laboratory, he explains, would not survive the clock’s journey by road. The solution, developed by group member Uwe Sterr, was to mount the cavity inside a 3D arrangement of wires that squeeze the cavity to keep its length set to a very precise value. “If you don’t make these corrections, even a tiny vibration will degrade the quality of the laser,” says Sterr.

As Lisdat and colleagues used their clock to carry out two measurement campaigns on the road, and by comparing its performance against that of a stationary optical clock, they showed it was accurate to 7.4 parts in 1017. In particular, they found it was an order of magnitude more accurate and two orders of magnitude more stable than the best portable caesium clock. They are now working to improve the clock’s accuracy by better understanding the behaviour of the lasers used to trap the strontium atoms, and describe their current clock in a paper in Physical Review Letters.

Single ion

Meanwhile in China, a team led by Xueren Huang of the Wuhan Institute of Physics and Mathematics has obtained a similar uncertainty (7.7 parts in 1017) from its own transportable optical clock. The system is based on a transition of a single ion of calcium-40 and is described in a preprint on arXiv.

According to Rachel Godun of the National Physical Laboratory in the UK, the Chinese system has the advantage of simplicity, which, she says, makes it smaller – at just half a cubic metre (minus the electronics) – and cheaper. Writing in an article in Physics that accompanies the Physical Review Letters paper, she says that the PTB set-up benefits from having more atoms and therefore a better signal-to-noise ratio. This, she explains, means it can reach a given statistical uncertainty much more quickly – allowing it to make measurements in minutes rather than days.

Comparisons between atomic clocks in different parts of the world are often carried out using satellites, but noise limits the sensitivity of such comparisons. Optical-fibre networks offer a better method of comparison, but these need special amplifiers at intervals of about 100 km to compensate for lost power. While this can be done on land, creating a similar link between continents would be far costlier. It is here, according to Godun, that the new transportable optical clocks would be very useful. They “could travel between laboratory clocks located anywhere in the world”, she says, so enabling “significant progress towards a redefinition of the SI second”.

Height differences

Godun points out that these portable clocks could also have other applications, including in geodesy. General relativity tells us that time runs more quickly further away from a massive object, which means that clocks on Earth will tick at very slightly different rates, depending on how high up they are. Optical clocks with accuracies of one part in 1017 could resolve height differences of a mere 10 cm, she says, so making them competitive when it comes to comparing the heights of sites that are separated by hundreds of kilometres – a time-consuming task when using the traditional technique of spirit levelling.

Godun adds that optical clocks transported to remote locations could also be used for “long-term environmental monitoring by measuring height changes in ice sheets and ocean levels”.

Flash Physics: Liquid drops explode, developing world scientists honoured, star breaks X-ray emission record

Liquid drops explode

Drops of a water–alcohol mixture exploding into millions of tiny droplets have been observed by Etienne Reyssat and colleagues at the Institute of Industrial Physics and Chemistry in Paris. The explosions occur when the liquid is placed on a layer of oil and the physicists say that the process is driven by a combination of evaporation, surface tension and fluid flow. The relative concentrations of water and alcohol in the mixture determine the surface tension of the fluid – the more water, the greater the surface tension. When a high-alcohol mixture is placed on an oily surface, it will spread out to create a film, whereas a high-water mixture will form drops. However, as alcohol evaporates from the high-alcohol mixture, the increasing surface tension causes the liquid to form puddle-like drops. The rate of alcohol evaporation is greatest at the edge of the drops, causing fluid to flow rapidly towards the edge, where liquid bursts out creating thousands or even millions of droplets. The size of the ejected droplets can be adjusted from a few microns to a fraction of a millimetre by changing the ratio of alcohol to water in the mixture. The study is described in Physical Review Letters.

Award celebrates women for their pioneering research in developing countries

Photograph of the award sculpture

Five early-career researchers from developing countries have been honoured for their work in engineering sciences. The OWSD-Elsevier Foundation Awards for Early-Career Women Scientists in the Developing World celebrates the achievements of female researchers who have made a significant contribution to their field and encouraged young women in science in their respective countries. The 2017 winners are Tanzima Hashem of the University of Engineering and Technology in Bangladesh for her work developing computational methods to the protect privacy of people accessing location-based services; María Fernanda Rivera Velásquez of the Universidad Nacional de Chimborazo in Ecuador for her research on decontaminating industrial areas using native materials; Felycia Edi Soetaredjo of Widya Mandala Catholic University Surabaya in Indonesia for her work on using biomass for renewable energy and environmental decontamination applications; Grace Ofori-Sarpong of the University of Mines and Technology in Ghana for her work on extracting gold-bearing minerals and free particles from mine water; and Rania Mokhtar of Sudan University of Science and Technology in Sudan for her research into advanced security systems for mobile devices. The Elsevier Foundation award is run in partnership with The Academy of Sciences for the Developing World (TWAS) and the Organization for Women in Science for the Developing World (OWSD). The winners were rewarded $5000 each and an all-expenses-paid trip to the 2017 American Association for the Advancement of Science (AAAS) Annual Meeting in Boston, where they were honoured during a ceremony on 18 February.

Neutron star breaks X-ray emission record

The XMM-Newton space telescope

A neutron star that emits X-rays at 1000 times greater intensity than predicted by theory has been discovered by astronomers working on the EXTraS X-ray observation programme. Located in NGC 5907 – a spiral galaxy 50m light-years from Earth, the ultraluminous X-ray source (ULX) is far too bright to be explained by the balance between the force of radiation acting outward on a neutron star and the gravitational force acting inward. This balance is called the “Eddington limit” and had led astronomers to assume that ULXs were driven by small black holes. Instead, observations using the XMM-Newton space telescope suggest that the X-rays are emitted by a spinning neutron star that is accelerating rapidly as it sucks in surrounding matter. While the intense X-ray emission cannot be explained if the star has a simple dipole magnetic field, the team writes in Science that the emissions could be driven by a magnetic field with strong multipolar components.

 

  • 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 an atomic clock in a van.

Science supporters protest in Boston

Stand up for Science rally in Boston, 19 February 2017

By Matin Durrani in Boston, US

Hundreds of scientists and science supporters gathered in Copley Square in Boston earlier today in a rally to underline the importance of science. The “Stand up for Science” event was organized to coincide with the annual meeting of the American Association for the Advancement of Science, which is taking place a few blocks away.

To find out more about the aims and purpose of the rally, I hooked up with Geoffrey Supran (picutred below), who helped to organize the event. Having originally studied physics at the University of Cambridgein the UK, Supran obtained a PhD in materials science at the Massachussetts Institute of Technology and is now doing a postdoc in the history of science with Naomi Oreskes at nearby Harvard University.

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