Skip to main content

To solidify, just add water

Scientists in Germany have shown that a suspension of particles can be transformed from a viscous fluid to an elastic gel by adding a small quantity of a second liquid – as long as the second liquid does not mix with the bulk fluid. They say that the second liquid binds the particles more tightly together, and found that this enhanced binding takes place even when the liquid itself adheres poorly to the particles. Applications of this work, say the researchers, include lighter and cheaper foams as well as improved manufacturing of paints and other suspensions.

Being able to control the flow of suspensions – small, solid particles dispersed in a fluid – is important in the manufacture of many commercial products, such as coatings and foodstuffs. For example, it is better if paint is less viscous when it is being mixed during production, but more viscous when in its finished state so that it sticks to walls and does not drip.

In the latest research Erin Koos and Norbert Willenbacher of the Karlsruhe Institute of Technology have demonstrated a new and practical method for adjusting the viscosity of a suspension. In their experiment, they first dispersed hydrophilic (or water-attracting) glass beads, each about 25 µm in diameter, into an organic solvent. Then they added water to this suspension so that it made up just 1% of the suspension by weight. When they stirred, the initially viscous fluid transformed into a gel-like material.

Water builds bridges

This transformation has been known about for many years, and occurs because the water wets the particles – in other words, it tends to adhere to the surface of the hydrophilic particles more readily than does the organic liquid and so forms a thin film around them. When two particles get close enough, the water’s surface tension then dictates that it becomes energetically favourable for the coatings of water to join up and form a bridge, so binding the particles together and creating a network that makes the suspension more rigid.

What the researchers also found, however, was that the reverse can happen. When dispersing hydrophobic (water-repelling) glass beads into the solvent and then adding 1% water, they discovered that the initially viscous suspension becomes gel-like upon stirring. In other words, adding a small quantity of a substance that wets less well than the solvent, rather than better, also binds the beads together to form a more-or-less rigid network.

This process has also been observed before. For example, adding water to melted chocolate causes the latter to solidify even though the solvent in the chocolate – cocoa butter – wets the cocoa particles more readily. What Koos and Willenbacher have done is to demonstrate that this is a general phenomenon, having subsequently found that the process occurs in a wide variety of fluid and particle combinations. They were also able to pin down the mechanism responsible, and show that it is essentially the same process as occurs when introducing a superior wetter, but in reverse.

Rotating plates

In their experiment, the researchers measured the amount of force needed to set two parallel metal plates rotating relative to one another when a suspension is placed between them. They found that the force required increased markedly as the second, non-mixable fluid was added to the suspension – in other words the “yield point” of the suspension increased – and they found that this increase is just what would be expected were the particle binding determined by surface-tension, or “capillary”, effects. In this case, however, the water does not coat the particles but instead seeks to minimize its total area of contact with the particles and the bulk fluid, which leaves the water enclosed by particles (see figure).

Koos says that this effect can also be seen when building sandcastles. Adding a little water makes sand firmer because it creates bridges between the sand particles. The inter-particle binding increases as more water is added but when the sand finally becomes saturated with water, and there is no longer any air present, the sand particles simply slosh around in the water. But adding back in a small amount of air – the inferior wetting fluid – provides nuclei around which the sand particles can agglomerate.

According to Koos, this ability to enhance rigidity by adding small quantities of either a superior or inferior wetter could improve the industrial manufacture of suspensions. For example, she says, they found that foam can be made by dispersing PVC particles in water and then adding a tiny amount of oil. This requires less PVC than the traditional approach of dispersing PVC directly into oil, meaning that the process is cheaper and the resulting foam is lighter, which could make it attractive in the manufacture of lightweight building materials and insulating foams.

Wilson Poon at the University of Edinburgh in the UK points out that while other groups are studying the effects of adding a small amount of a second, unmixable liquid to suspensions, this latest work provides a striking demonstration of the potential of such an approach. And he agrees that the results obtained by Koos and Willenbacher indicate that capillary forces play a dominant role. “Since it is very difficult to eliminate moisture entirely from oil-based systems, or oily impurities from aqueous systems, it is possible that the effects presented here are widespread, but not widely recognized as such,” he says. “It is always tempting to think that the odd 0.3% impurity doesn’t really matter. In fact, it may matter, and matter hugely, either for good or for ill.”

The work is described in Science 331 897.

Freebies galore

freebies.jpg
Conference collectables

By Michael Banks in Washington, DC

No conference trip is complete without hoarding freebies from exhibitor stands.

So above is the result of my 30-minute sweep through the exhibition hall at the 2011 American Association for the Advancement of Science (AAAS) meeting here in Washington, DC.

Kudos to the Nanyang Technological University in Singapore who were providing USB hubs to conference goers (bottom left item in the image above). No expense spared there.

The AAAS yo-yo was a particular hit with delegates, with many people walking through the exhibition doing yo-yo tricks. The strangest item has to be the EurekAlert! sticky brain – not sure what I am going to do with that.

My favourite freebie has to be the big red “Canada” mittens. Next year’s AAAS conference is in Vancouver, Canada, so they just might come in handy then.

conferencehall.jpg
Gateway to conference freebies

Carbon concerns

cow.jpg
How much carbon is coming out?

By Michael Banks in Washington, DC

“Carbon is the most important element, but we are deeply ignorant of its effect on the Earth,” says Robert Hazen from the Carnegie Institution of Washington.

Hazen is the principal investigator of the deep carbon observatory – a 10-year programme funded by the Alfred Sloan Foundation to better understand the Earth’s carbon cycle.

It’s a wide-ranging study and speaking at the 2011 American Association for the Advancement of Science meeting in Washington, DC, Hazen spelled out the many questions that remain unanswered about carbon. These include how much of the element is stored in the Earth, especially in the core, and how much of the material is released when a volcano erupts.

In the case of a volcanic eruption, Hazen says some scientists conclude carbon makes up around 2% of the material ejected, while others say it is more like 75% – a big discrepancy that the programme will hope to reduce.

The programme only started in 2009 so Hazen is issuing a call to arms for scientists of different backgrounds to come together and join the project.

You will have to be quick as proposals for research activities must be submitted by 11 March.

Read more about the programme here.

Eye-catching exhibits

cow.jpg
Science on a sphere

By Margaret Harris in Washington, DC

No trip to the AAAS meeting would be complete without a tour of the exhibit hall, which for the past two days has been buzzing with visitors to “Family Science Days”, a public outreach-oriented event running in parallel with the more technical seminars.

One of the most eye-catching exhibits was the National Oceanic and Atmospheric Administration’s Science on a Sphere, which pretty much does what it says on the tin. The Sphere is the brainchild of Alexander McDonald, director of NOAA’s Earth Systems Research Laboratory, and there are now over 250 datasets that can be displayed on it. In this photo, it’s illustrating the shock waves that spread around the globe after the Boxing Day tsunami of 2004, but I also saw depictions of ocean currents, aeroplane flight paths, global temperatures and the past week’s weather. According to exhibitor Jana Goldman, there’s even one in a science fiction museum in Seattle, Washington that displays the (hypothetical) features of a (fictional) alien planet – so it’s definitely a versatile beast!

Another exhibit that got a lot of traffic was the US Department of Energy’s set of bicycle-powered light bulbs, which is designed to teach kids (and maybe some adults) about the differences between voltage and current, and to demonstrate in a very physical way how much power it takes to light up an incandescent 50 W bulb compared with fluorescent and LED bulbs. The young gentleman in this photo, for example, was having real trouble getting the incandescent bulb to give off any light, but despite being a little too short for the pedals, he managed the LED bulb just fine.

cow.jpg
Bicycle-powered light bulbs

For the bigger kids, exhibitor Steve Eckstrand keeps a 12 V, 300 W hairdryer on hand. “They can usually get the 50 W bulb working just fine, and one girl did manage to pedal hard enough to get a faint glow out of the 100 W bulb,” he says. “But nobody can do more than get the hairdryer sort of gently warm.”

LHC ready for new physics

By Michael Banks in Washington, DC

If you are reading this blog in the hope that physicists at CERN have announced the discovery of new physics at the Large Hadron Collider (LHC) then you may be a little disappointed.

At a session this morning at the 2011 annual meeting of the American Association for the Advancement of Science, CERN researchers reflected on the past year of LHC data.

The bottom line is that the LHC has taken enough measurements to verify the Standard Model of particle physics and is now on the verge of searching for new physics.

“We are opening a door to a new landscape, starting an exploration in physics for the next 20 years.” was one of the take-home soundbites from the opening talk given by Felicitas Pauss, head of international relations at CERN.

One area of research at CERN is whether quarks – the building blocks of particles such as protons and neutrons – have any substructure.

Thomas LeCompte, from Argonne National Laboratory, told delegates that the ATLAS detector at the LHC had so far not yet spotted any evidence for quark substructure. But the emphasis is on the “yet”. CERN researchers are continously narrowing down the search.

LeCompte used a nice analogy to describe the LHC’s current limit. “If an atom is the size of an Earth, then we have not seen any evidence of substructure down to the relative size of a pea,” he says.

Indeed, LeCompte says that over the next few years, the search will narrow down to the order of a “single hundreds and thousands sprinkle”. Quite a feat.

Likewise, CERN researcher Joe Incandela noted that the CMS detector has not yet found any evidence for supersymmetry, which predicts that each fermion has a partner boson and each boson has a partner fermion – that are all known as “sparticles”. Again the emphasis is on the yet: “In 2011 we will have more than 50 times the data we have now,” he says.

Monica Pepe Altarelli from the LHCb experiment told delegates about the hunt for the a rare B-meson decay (into a muon and antimuon), which other experiments such as CDF and D0 detectors at Fermilab have searched for but not yet seen.

Altarelli notes that even with the LHC’s limited run, the collider will have recorded the production of more B-mesons than the Fermilab accelerator has managed in its whole lifetime. Altarelli also says the collaboration will publish some results in the coming days but by the end of this year they should have enough statistics to probably see glimpses of the event.

The final slide Pauss flashed up on the screen in her summary talk was an image of the Particle Physics Booklet that is published by the Institute of Physics Publishing, which owns physicsworld.com.

Pauss wondered if by the end of 2011 we will need to publish another separate book – the “sparticle physics booklet”. CERN physicists will certainly be hoping so.

A fun way of learning lab safety

test.bmp

By Margaret Harris

As a veteran of many stupendously boring – but mandatory – safety training sessions, I was initially tempted to give a wide berth to a booth in the AAAS exhibit hall on lab safety.

However, two things persuaded me to linger at this particular kiosk, which had been set up by the National Institute of Health (NIH) Division of Occupational Health and Safety. One was a statistic related to me by Kersten Haskell, a science communicator at the NIH. “We have a lot of students who come into NIH labs as interns in the summer, and what we found was that of all the injuries that were happening during that time, around 75% were to students,” she said. “So we figured we had to find a way to train them better.”

The NIH’s solution to this problem was to put essential elements of safety training into a video game. This brings me to my second reason for stopping: the row of monitors displaying scenes from the Safe Techniques Advance Research – Laboratory Interactive Training Environment (STAR-LITE). This visually appealing, easy-to-use game allows students (and visiting journalists) to guide avatars through typical lab-safety situations, solving problems and receiving points (or injuries) in the process – and I couldn’t resist giving it a quick test.

The game is clearly designed with health research in mind. In fact, it’s dedicated to the memory of a biology student, Beth Griffin, who died after contracting the rare macaque-borne B virus in a laboratory. However, I was pleasantly surprised to find that many of the hazards addressed in the game could apply equally well to physics. For example, my avatar spent a happy five minutes securing gas bottles and labelling hazardous chemicals (something I did many times while working in real-life physics labs) before I reluctantly turned the game back over to Haskell and her colleagues.

STAR-LITE is principally aimed at secondary-school students and new undergraduates, but if anyone wants to have a go, it’s free to download – and it’s a heck of an improvement over the grainy videos from the 1980s that made up the backbone of my own safety training.

Watching out for space weather

By Michael Banks in Washington, DC

Last week a hiccup from the Sun resulted in travel misery. Flights that were due to travel over the poles had to be rerouted when material from a solar flare was expected to impact on the Earth’s magnetosphere.

The result would be a geomagnetic storm and the airlines couldn’t risk their craft suffering electrical interference that the storm – the strongest for four years – would bring. It resulted in frustrated passengers and added costs for airlines.

You probably do not think that space weather would affect your daily life, but a huge coronal mass ejection (CME) from the Sun would have untold consequences on Earth, potentially damaging electrical transmission lines that would result in power outages.

A CME releases a plasma of electrons and protons into space and the shock wave of the traveling plasma causes a geomagnetic storm.

Today at the 2011 annual American Association for the Advancement of Science meeting in Washington, DC a panel of distinguished scientists spoke about the effects of space weather and what to do to mitigate its effects.

Jane Lubchenco, head of the National Oceanic and Atmospheric Association, told delegates that space weather is a “serious concern”. “We are going to be seeing more space weather”, says Lubchenco. “10 years ago the world was a different place, fewer aircraft were flying, now space weather is everyone’s business.”

John Beddington, chief scientific adviser to the UK government, said that countries need to invest in “predication facilities” and learn how to characterize space weather better so when it does arrives we know how to deal with it.

Unfortunately, mitigation at the moment mostly means turning off transformers until the storm passes. This would mean a temporary blackout. However, the alternative is the possible destruction of infrastructure that would take years to replace.

As Lubchenco noted about future solar storms: “it’s not a matter of if, but when and by how much.”

Hunting for exomoons

boss.jpg
Planet hunter Alan Boss from the Carnegie Institution in Washington (courtesy: the University of Virginia)

By Michael Banks in Washington, DC

Could NASA’s Kepler mission be able to spot the first moon outside our solar system? Astronomer Alan Boss from the Carnegie Institution in Washington thinks so.

Sitting down for a chat today at the 2011 annual meeting of the American Association for the Advancement of Science in Washington, Boss told me that evidence of an exomoon could be buried in Kepler data.

Kepler is designed to study exoplanets – planets outside our solar system – and in particular planets that have a similar size to Earth. It has so far found around 1235 planet candidates since its launch in March 2009.

Boss says finding a moon would be difficult but not impossible. “If a large enough gas planet is found it may have an Earth-sized moon and that could be potentially seen in the Kepler data,” says Boss. “I am sure folks are combing through the data looking for signs.”

I also asked Boss about naming planets. Currently they are named after the craft that found them, such as Kepler 9b, CoRoT-7b etc, so is the time right to start a more robust classification for naming them?

“I think astronomers are quite comfortable naming them Kepler b, Kepler c etc,” says Boss. “But that doesn’t mean that a creative astronomer who wants to call a planet Cleopatra shouldn’t do that.”

Look out for an upcoming audio interview with Boss on physicsworld.com about the search for exoplanets with Kepler.

The atomic detectives

068_05.10.06.jpg

By Margaret Harris in Washington DC

One July day not so long ago, a shipment of scrap metal entered an EU seaport from somewhere outside the EU. No-one who watched the shipment being unloaded saw anything out of the ordinary. But when it went through the port’s radiation detector, alarm bells began to ring – and they rang again the next month with another shipment, and for a third time in October the same year. What was going on?

This is the story of “Find 33,” a case study from the emerging science of nuclear forensics that formed the basis of Klaus Mayer’s talk at an AAAS session on combating nuclear terrorism. Mayer, a scientist at the Institute for Transuranium Elements (ITU) in Karlsruhe, Germany, was called to investigate Find 33 after national authorities had isolated which particular bits of scrap were setting off the detectors.

The initial data were puzzling. The amount of enriched uranium in the four pieces of suspicious scrap ranged from a few percent to over 90% – values that suggested a mixture of commercial-grade and weapons- or research-reactor grade contamination. Could they have a common origin? Or were Mayer and his team dealing with multiple uncontrolled sources of radioactive and nuclear material?

After more detailed tests, a clearer picture began to emerge. A sample from the first piece of scrap – an extremely dirty funnel-shaped object – was found to contain 0.33% uranium by weight, of which the fraction of enriched uranium (U-235, the isotope used in both nuclear weapons and reactor fuel) was 9%. This was unusual: 9% is too high for a commercial reactor, which typically uses fuel that is 90%). However, after grinding the sample into powder, Mayer and his team were able to show that it was actually a mixture of 3.6%-enriched and 20%-enriched particles. Radiochemical tests also showed that the uranium in it was old – it hadn’t been chemically purified since 1962.

ITU_Find33pic.jpgA piece of contaminated scrap from Find 33. (Courtesy: VROM-Inspectorate)

The other three scraps were analysed in a similar fashion, turning up a mixture of ages (June 1959, June 1972, October 1983) and enrichment fractions that ranged from a few percent for the second scrap to a sobering 89% for the fourth. This indicated that wherever these scraps had come from, it had to be someplace that had been producing a mixture of light-water reactor fuel, fast-breeder reactor fuel, submarine fuel and material for research reactors or weapons for at least 30 years, between the late 1950s and early 1980s.

And there were only two sites that fit the bill.

Sadly for this story’s narrative arc, Mayer declined to provide any further information on the two candidate facilities, citing an ongoing investigation. One thing, however, is certain: with 207 illicit trafficking incidents recorded in 2010 alone, the atomic detectives are keeping busy.

Kepler basks in its success

By Michael Banks in Washington, DC

It was all things exoplanets this morning at the 2011 annual meeting of the American Association for the Advancement of Science here in Washington, DC.

It’s quite amazing what NASA’s planet hunter – the Kepler mission – has managed to find. So far, in data released in February, the Kepler probe has discovered 1235 planet candidates. 68 of them are Earth-sized planets with 54 thought to be in the habitable zone of a star – an orbit that is not too close or far away from the star so the conditions are ideal for life.

Maybe one of the most interesting potential planets is “KOI 326.01”. It is actually smaller than Earth and is in the habitable zone of its star. However, like most of the planets Kepler has so far spotted, the planet has yet to be confirmed.

When asked further about the planet, William Borucki, from the NASA Ames Research Centre, who gave an overview of the mission, would not single it out for special attention.

The next speaker in the session was Matthew Holman from the Harvard-Smithsonian Centre for Astrophysics, who told delegates that Kepler has found 45 three-planet systems, eight systems with four planets in them, one with five and one with six planets.

Even though Kepler will be studying exoplanets for another three years, astronomers are also thinking about what comes next.

Sara Seager from MIT is planning to send a host of Cubesats into orbit in the next few years to study exoplanets. These small-sized satellites – each around 20 × 20 × 20 cm – would each study a single star to look for planets orbiting them.

Only a few years ago, exoplanet science was thought of as a “cottage industry” according to Seager. “No-one thought how dominating the field of exoplanet research would now be,”she says. As the planets found by Kepler are confirmed and studied further over the coming years, that dominance is likely to continue.

Copyright © 2025 by IOP Publishing Ltd and individual contributors