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Physicists propose ‘wireless’ solar cells

A new type of solar cell that relies on a surprising property of certain insulators has been proposed by physicists in Austria, the US and Germany. The design relies on the discovery a decade ago that the interface between two insulating oxides can become metallic, which could eliminate the need for metal wires in solar cells. If the cost of producing layered structures of the oxides can be reduced, the research could lead to a new type of highly efficient photovoltaic cell.

In 2004 Harold Hwang and Akira Ohtomo made the remarkable discovery that when a layer of the insulator lanthanum titanate was grown on the insulator strontium titanate, a 2D electron gas forms at the interface causing it to become metallic. The phenomenon is caused by the accumulation of charge at the edge of a polar oxide as it meets a non-polar oxide. It has since been seen in other oxide interfaces and has been investigated by multiple research groups trying to develop new and improved electronic devices.

Conducting interfaces

Now, an independent team of researchers at the Vienna University of Technology, the Oak Ridge National Laboratory and the University of Würzburg has done calculations that suggest that the effect could be used to create a new type of solar cell – one in which the generated current is extracted via conducting interfaces rather than with metal wires.

Solar cells rely on the photoelectric effect, where a photon striking an electron in the valence band of a material promotes it to the conduction band, leaving a positively charged “hole”. The electrons and holes must be removed from the photovoltaic material without recombining or dissipating their energy into lattice vibrations.

Polar oxides such as lanthanum titanate contain an internal electric field and positively and negatively charged planes of atoms. Oak Ridge’s Satoshi Okamoto and colleagues reasoned that this polarization would help separate the electrons and the holes before they could recombine. If such a polar oxide is paired with the appropriate non-polar oxide, the interfaces would be metallic. As a result, electrons and holes could be extracted from either side of the device without covering the surface with wires, which block some of the light from reaching the active region of the cell.

Maximizing absorption

The researchers first needed a polar oxide that would absorb as much solar energy as possible. A material’s band gap is the energy difference between its valence and conduction bands. Photons with energies less than the band gap cannot create electron–hole pairs, whereas photons with energies greater than the band gap will create pairs. In the latter case, however, energy in excess of the band gap is lost as heat. As a result, the band gap should therefore be low enough to absorb plenty of solar photons, but high enough to extract as much energy as possible from the photons absorbed.

The researchers settled on lanthanum vanadate, which has an band gap of 1.1 eV – visible light is in the 1.5–3.5 eV energy range. They used density functional theory to model the behaviour of a solar cell constructed of a layer of lanthanum vanadate grown on a strontium titanate substrate. While they were unable to make precise predictions about device efficiency based on their results, the researchers suggest that the inherent advantages of the design deserve further investigation.

Capturing higher-energy photons

The researchers also suggest that the efficiency of the solar cell could be increased further by incorporating a layer of lanthanum ferrate on top of the lanthanum vanadate. Lanthanum ferrate has a band gap of 2.2 eV, so higher-energy photons could be captured in this layer, leaving the lower-energy photons to be captured by the lanthanum vanadate. A project to produce prototype solar cells is under way at the University of Würzburg.

Optimistic but cautious

Okamoto is cautiously optimistic about whether the solar cells could ever be efficient enough to make them economically viable. “They could become competitive, but it will take quite a long time,” he says. “Currently, only a limited number of facilities can grow this kind of heterostructure using very advanced thin-film growth methods. I hope that when people fully understand how best to grow these solar cells the cost will come down.”

Neil Greenham, who works on novel solar cells at the University of Cambridge, describes the research, published in Physical Review Letters, as “an interesting theory paper” but emphasizes it will be impossible to assess whether or not the solar cells will have any practical advantages over current designs until working prototypes are produced. He also questions the assertion that simply incorporating two epitaxial layers could allow electron–hole pairs to be collected with two different energies, suggesting that, unless the electron–hole pairs could be extracted separately, any extra energy captured by an electron in lanthanum ferrate would be dumped into the lattice as it passed through the lanthanum vanadate.

Okamoto responded that photogenerated electrons and holes should cross a thin film of lanthanum vanadate in “a few femtoseconds”, which is less than the time it would take to lose energy to the lattice.

Hunting the Higgs

By Michael Banks in Boston

“It looks like a Standard Model Higgs,” remarks Christopher Hill from Ohio State University. “Everything we have measured has strengthened that position.”

Last year, researchers working at the Large Hadron Collider (LHC) at CERN reported they had found a Higgs-like particle with an energy of around 126 GeV.

Yet while the Higgs looks like that predicted by the Standard Model of particle physics, further measurements were needed before researchers could be sure.

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Why are carbon nanotubes so strong?

In less than 100 seconds, Michael Strano explains how carbon nanotubes get their strength.

Shining a light on dark energy

Dust is annoying, particularly when you want to obtain a precise measurement of the expansion of the universe.

Today, Robert Kirshner from Harvard University gave a plenary lecture at the 2013 AAAS meeting in Boston giving participants a tour of the latest in dark-energy research.

Kirshner is a member of the High-Z team that some 15 years ago used observations of supernovae to discover that the expansion of the universe is accelerating.

Indeed, his former students – Brian Schmidt and Adam Riess – shared the 2011 Nobel Prize for Physics together with Saul Perlmutter for this discovery.

Riess, a graduate student at the time, played an important part in figuring out how to account for dust when measuring supernovae distances. This dust surrounding a supernovae is annoying as it absorbs light, which introduces uncertainties in deducing how far away supernovae are.

Reiss managed to account for this well enough to measure the brightness of supernovae to a reasonable precision that could then be used to deduce the accelerating expansion of the universe; but now Kirshner’s team is planning to go a few steps further by doing better measurements.

This will be done by using the Hawaii-based Pan-STARRS telescope to find candidate supernovae and then follow up the measurement in the infra-red to “see” through the dust cloud and get a better measure of the supernova’s brightness.

Kirshner’s team has just started to use the Hubble Space Telescope to do this kind of  measurement in the infra-red.

Dark energy is thought to account for around 73% of the total mass-energy of the universe, but Kirshner thinks this new technique will give researchers a more precise measure.

Further ahead, Kirshner is looking forward to more enhanced infra-red observations of the universe by using the James Webb Space Telescope as well as the ground-based Giant Magellan Telescope, which he is involved in constructing.

Japan 101

Stand from Japanese research bodies at the 2013 AAAS meeting

By Michael Banks in Boston

There is certainly a big presence from Japanese research bodies at the 2013 AAAS meeting in Boston.

In the exhibitors’ hall, the World Premier Institutes (WPI), RIKEN and the Okinawa Institute for Science and Technology all share a large central stall plugging their research and facilities.

Indeed, this presence may well be part of Japan’s drive to increase the number of foreign researchers and students in the country by actively highlighting its top research and facilities, a topic Physics World touched upon in a special report published last September.

After a brief chat at the WPI’s stall, I was handed a book called The Challenging Daily Life, which is published by the WPI’s International Center for Material Nanoarchitechtonics (MANA).

The 136-page book, featuring Japanese-style cartoons, introduces problems that foreigners in Japan come across in their everyday lives, and gives information and hints about how these problems can be solved.

The book features 34 different “episodes” – all based on real experiences of MANA staff – such as the “nightmarish bad weather” in Japan or how to deal with an invitation to a wedding.

My favorite case study, though, is “don’t overeat”, which seems to basically tell people that if you eat too much you will get fat and that while Japanese food is healthy, eating too much will result in weight gain.

I guess as long as it plays a role in making researchers from abroad more comfortable in Japan then it will have done its job.

First results due from AMS

By Michael Banks in Boston

The first results from the $1.5bn Alpha Magnetic Spectrometer (AMS) are expected to be released in the coming two weeks, according to AMS principal investigator Samuel Ting.

Ting, who shared the 1976 Nobel Prize for Physics, was speaking at the 2013 AAAS meeting in Boston.

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A factor of two

conference image

By Michael Banks in Boston

“A factor of two is not a small thing, it is quite a challenge,” says Robert McCory from the University of Rochester in New York.

McCory was speaking about the latest in laser-based fusion research (known as inertial confinement fusion) at the 2013 AAAS conference.

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Infinite BBQs

By Michael Banks in Boston

Here is a good quiz question. What contains more water: a cucumber or a glass of milk?

If you happened to guess the humble cucumber then you would be correct.

At least that is, according to Nathan Myhrvold, who says the water content of a glass of milk is around 85%, while for a cucumber it is more like 95%.  This is because milk is made up of other things such as proteins and fat.

Myhrvold, who has a PhD in physics, was speaking at the 2013 AAAS meeting in Boston where he gave a plenary lecture to a packed audience on the science of cooking.

Myhrvold is the brains behind the recently published six-volume, 2400-page tome  Modernist Cuisine that took him and his staff of eight researchers around five years to put together.

Apart from talking about the novel cooking techniques he has developed such as making crispy chips in an ultrasonic bath and spinning peas in a centrifuge to bring out more flavour, Myhrvold had some tidbits of information we could all put to use.

One is how to make wine taste better. Usually when wine goes from a bottle into a decanter the taste improves. However, if you don’t fancy using a decanter then you can just put the wine in a food processor and give it a quick blitz. According to Myhrvold this produces just the same effect.

Another is creating what Myhrvold says is an infinite BBQ. In a BBQ the food is cooked by infrared radiation emerging from the hot coals. As this radiation is emitted in all directions the centre of the grill is much warmer while the outer sections are cooler. His solution is to put foil around the inside of the BBQ to reflect some of the radiation back from the coals that are on the edge of the BBQ. This then acts to cook the outer section just the same as inner part.

Food for thought, indeed.

A trip to MIT

By Michael Banks in Boston

It may have been the prospect of free pizza that led me to hop on a bus heading to the Massachusetts Institute of Technology (MIT).

But apart from a free lunch, we were also promised a tour of MIT’s fusion facilities, which are based at institute’s Plasma Science and Fusion Center (PSFC).

So after a few slices of pepperoni pizza, we donned the hard hats and moved on to the tour, which included a look at MIT’s main experimental fusion facility – the Alcator C-Mod fusion tokamak.

Operating since 1991 and with a budget of around $25m per year, Alcator C-Mod is a magnetic-confinement fusion device. It heats up a plasma of deuterium and tritium atoms to millions of degrees kelvin, which causes the hydrogen isotopes to fuse and release energy.

However, Alcator C-Mod faces an uncertain future. Last year Congress slated the facility for closure after increasing the budget for the ITER fusion reactor in France. Given no increase in the Department of Energy’s budget for fusion – standing at around $450m per year – the cut had to then come from the domestic fusion programme.

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Curiosity on Mars

Mars

By Michael Banks in Boston

John Grotzinger, project scientist for NASA’s Curiosity mission, might be best known for whipping up a media frenzy in late November when he told NPR that data from one of the probe’s 10 instruments was “gonna be one for the history books”.

While the news that the probe had discovered evidence of organic molecules in the soil but more tests were needed was less than earth shattering, today at the 2013 AAAS meeting in Boston, Grotzinger gave an update on the mission that touched down on Mars on 6 August 2012.

If you don’t fancy reading any more, the bottom line is that everything is working as expected.

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