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Celebrating 50 years of the diode laser

By Hamish Johnston

Semiconductor diode lasers are everywhere. They created the light pulses that raced along the fibres between our server and yours – allowing you to read this article – and if you stop at the supermarket on the way home, their light will read the barcodes on your purchases.

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A few years ago I would have also pointed out that CD and DVD players rely on diode lasers, but those once-revolutionary technologies have already become passé while diode lasers have gone on to new and exciting applications such as healthcare.

So what does the image on the right – which looks more like a bent paperclip than a state-of-the-art laser – have to do with this revolutionary technology? It is the first diode laser (also called an “injection laser”) and was made in 1962 at the Lebedev Institute in Moscow. The institute was home to a group of scientists formed in 1957 by Nikolay Basov with the aim of creating a semiconductor laser. The team succeeded, and Basov’s pioneering efforts in the development of lasers earned him a share of the 1964 Nobel Prize for Physics – along with his institute colleague Aleksandr Prokhorov and Charles Townes of the Massachusetts Institute of Technology.

One member of Basov’s team was Yuri Popov, who is still at the institute and who has written a historical account of the group’s effort for a special issue of the journal Semiconductor Science and Technology – published by IOP Publishing, which also produces Physics World.

As well as historical papers documenting the development of the diode laser, the special issue also contains a number of invited papers that look at a range of contemporary research, including quantum-dot-based lasers and cascade lasers for the generation of terahertz radiation.

And if you can’t get enough about diode lasers, the Institute of Physics is putting on a conference in Leicester in September called The Celebration of the 50th Anniversary of the Diode Laser.

What is supersymmetry?

In less than 100 seconds, Helen Heath explains why SUSY is so beautiful.

What is dark energy?

In less than 100 seconds, Luke Davies explains how we know dark energy exists.

Metamaterial switches on to the tune of light

An international team of researchers has created the first metamaterial where its properties can be controlled with light. The material – made of metallic resonators with electronic circuits incorporating photodiodes – might find use in radar and communications applications, say the researchers.

Metamaterials, which were first made around 10 years ago, are artificial sub-wavelength patterned structures containing arrays of tiny elements such as rods and rings that respond to light and other electromagnetic waves in unusual ways. For example, a metamaterial can be designed to have a negative refractive index so that it bends light in the opposite direction to normal materials. Such a unique property means that metamaterials have already been used to make “superlenses” that are able to focus light to a point smaller than its wavelength, allowing optical microscopes to view much smaller objects than is possible today. They can also be used to make “invisibility cloaks” for electromagnetic waves.

Light sensitive

Up to now, however, most metamaterials had fixed architectures and their properties could not be tuned across the structure. A team led by Ilya Shadrivov and Yuri Kivshar, from the Australian National University and the University of Information Technologies, Mechanics and Optics in Russia, has now come up with a new idea that overcomes this problem. The researchers decided to build a metamaterial lattice not just with simple metal tracks as in previous experiments, but one that contains electronic circuits incorporating light-sensitive photodiodes.

“The voltage generated by this photodiode when it is illuminated with light can be used to change the resonance of the metamaterial structure,” explains Shadrivov. “This means that we can control the refractive properties of the structure at will and bend the microwave light beams passing through the material in whichever direction we like.”

Illuminated array

The metamaterials used in this study were made in much the same way as a conventional printed circuit board with a lattice of engineered copper tracks. In this case, the tracks comprise 24 so-called broadside-coupled split-ring resonators (SRRs) placed in front of a metallic screen. The components in this structure interact with microwaves like ordinary glass atoms in a lens interact with light. The SRR itself is made of two broken copper rings placed on the opposite sides of 1.6 mm printed circuit board. The inner radius of the SRR is 3.25 mm, the width of the metal strip is 0.5 mm, the copper thickness is 30 μm and the gap between them is 1 mm. Each ring has an extra gap of 0.4 mm in which an electronic circuit with photodiodes is placed. These diodes generate a voltage that increases as the intensity of the incoming light increases.

“Our set-up also allows us to change the properties of the metamaterial non-uniformly by illuminating the array with light beams of varying intensities,” says Shadrivov. “This concept of being able to tune a metamaterial’s optical properties could potentially be used to make reconfigurable satellite dishes or reflectors for antennas that can operate at different light wavelengths,” he told physicsworld.com. “We could change the properties of such a dish (for example its focal length or reflectivity) without changing its physical shape in any way and could, for instance, create a satellite dish that is not a dish at all but a flat disc.”

Such structures might also be designed to become strong absorbers of light or they could be used to make the first invisibility cloaks that are fully reconfigurable. “These devices might find use in both military and civilian applications,” he adds.

The research is published in Physical Review Letters.

What steps have you taken to pursue your career in physics?

By Margaret Harris
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In last week’s Facebook poll, we asked for your views on the most important criterion for choosing a postdoc position. The results weren’t quite what I had expected. While it makes sense that “institutional resources” came out on top – you can’t do much experimental physics without lab space and equipment, and theory is certainly easier if you’ve got a good bunch of colleagues – I was surprised by how much it outpaced the other poll options. A whopping 65% of voters rated “institutional resources” as the most important factor, with “prestige” of the supervisor and institution coming a distant second and third at 17% and 13%, respectively.

But the thing that really puzzled me was the low emphasis placed on “location”, which picked up a measly 5% (three votes out of 63). Are physicists really not that fussy about where they go to do postdoctoral research?

To find out, I’ve constructed this week’s Facebook poll so that it focuses on mobility – both geographic and intellectual.

What steps have you taken to pursue your career in physics?

Moved to a new location (less than 500 miles away)
Moved to a new location (more than 500 miles away)
Changed my field of research or expertise
Switched to a different sector (e.g. from academia to industry)
Two of the above
Three or more of the above

Have your say by visiting our Facebook page, and please feel free to explain your response or give us more suggestions by posting a comment below the poll or by e-mailing us at pwld@iop.org.

How does quantum teleportation work?

In less than 100 seconds, John Rarity explains why it is tricky to copy quantum information.

US telescopes faced with closure

A committee of the National Science Foundation (NSF) has recommended closing six major astronomy facilities in favour of building and supporting new telescopes. The observatories under threat include two leading radio telescopes – the Green Bank Telescope (GBT) in West Virginia and the Very Large Base Array (VLBA), which comprises 10 radio-dish antennas spread across the US from Hawaii to the US Virgin Islands. They are joined by four others based at Kitt Peak in Arizona – the Mayall Telescope, the Wisconsin-Indiana-Yale-National Optical Astronomy Observatory, a 2.1 m telescope and the McMath-Pierce Solar Telescope. US astronomers fear that if the telescopes close it will jeopardize the country’s position as a world leader in astronomy.

The NSF’s astronomy portfolio review, chaired by astronomer Daniel Eisenstein from Harvard University, calls for the NSF to stop supporting the six facilities within the next five years. Given tougher budget conditions for the NSF, the money saved from such closures would go towards supporting newer facilities such as Atacama Large Millimeter/submillimeter Array (ALMA), the Advanced Technology Solar Telescope and eventually the Large Synoptic Survey Telescope.

The VLBA, with a “baseline” of more than 5000 miles, makes it the largest in the world, with the GBT sporting the largest steerable radio dish at 100 m across. However, the 17-person NSF committee believes that other radio telescopes could take on the workload of the GBT and that the capabilities of the VLBA to precisely measure the position and movements of stars has not been deemed a priority in the recent Astrophysics Decadal Survey. “We were charged to recommend the best possible overall portfolio in light of the budget constraints and the Decadal Survey science priorities,” says Einsenstein. “Hard choices have to be made.”

“A huge surprise”

Many astronomers, however, are not satisfied with the committee’s recommendations. “The loss of the GBT and the VLBA will be a blow to astronomers within the US and around the world,” says GBT site director Karen O’Neil. “Implementation of the recommendations will have a serious impact on the accessibility of major astronomy facilities to US observers as competition for those facilities becomes extremely high.”

Michael Kramer of the Max Planck Institute for Radio Astronomy in Bonn, which operates the German-based Effelsberg 100-m Radio Telescope, says that the GBT is one of the most important radio telescopes in the world, as its location in a radio quiet zone in the northern hemisphere is unique. “The report has come as a huge and unpleasant surprise,” says Kramer. “I cannot follow the arguments of the report and find it particularly difficult to accept the report’s conclusions.”

That view is shared by Tony Beasley who is director of the National Radio Astronomy Observatory, which operates the GBT and the VLBA. “We are pleased that ALMA and the Very Large Array were highly ranked, but the loss of the GBT and VLBA would break up the quartet of the best radio facilities in the world, which cover nearly the entire range of resolution, wavelength coverage and imaging capability,” he adds.

However, there may still be a lifeline for the VLBA and GBT as well as the other four telescopes affected in the committee’s report. Although the recommendation calls for the NSF to cease funding of the observatories, other funding sources could be found to keep them running in the long-term, such as private investment. “The report recommends divestment, which need not be the same as closure,” says Eisenstein. “We are recommending an end to NSF funding but there are many possible implementations of that.”

Integrated quantum chip may help close quantum metrology triangle

Researchers in Germany have moved one step closer to closing the “quantum metrology triangle”, by fabricating a proof-of-principle circuit that links two quantum electrical devices in series, for the first time. A closed triangle – something scientists have been chasing for more than 20 years – would finally allow standardized units of voltage, current and resistance to be defined solely in terms of fundamental constants of nature.

Metrology – the science of measurement – has evolved as new and more accurate ways of standardizing measurements have been found. For example, the metre is nowadays defined in terms of the speed of light, rather than by the old platinum–iridium prototype, because even though it was held in a controlled environment, the prototype was susceptible to tiny chemical and structural changes over long timescales. Quantum metrologists seek to improve upon traditional metrological methods by looking for ways of making high-resolution measurements of physical parameters using quantum theory and trying to link measurements to nature’s fixed fundamental constants.

Uncomplicated relationships?

In the 1960s Brian Josephson discovered that when a junction between two superconductors is irradiated with microwaves, the voltage that appears across the junction is proportional to Plank’s constant (h) and inversely proportional to the electron charge (e) – two fundamental constants of nature. Since the voltage is not affected by the dimensions of the junction or the materials it is made of, this voltage standard can be reproduced anywhere at any time and will always be the same.

Similarly, a quantum standard for resistance, known as the quantum Hall effect, was defined by Klaus von Klitzing 15 years later. He found that putting a superconducting material at a temperature of almost absolute zero in a magnetic field 100,000 times stronger than the Earth’s renders the superconductor’s resistance independent of the properties of the material, and again only dependent on e and h.

But, explains Bernd Kaestner of the Physikalisch-Technische Bundesanstalt, Germany, who helped build the new chip, “There is an uncertainty to e and h that is still quite large, so one can never be sure whether the quantum Hall effect and the Josephson effect are absolutely determined by these quantum relations or whether there are small corrections to them.”

Trouble with triangles

For the last 20 years, scientists have been attempting to link these two quantum-electrical standards in a triangle, defining a quantum-current standard in terms of e and h – the single-electron transport effect – as the third arm. If realized, this quantum metrological triangle would be able to test the consistency of the three electrical standards and work out whether any of the relations are in need of some fine-tuning.

“Any renormalizing factor would be incredibly small,” explains J T Janssen of the UK’s National Physical Laboratory, who was not involved in the research, “but it would also be incredibly important, because it would undermine the existing theory.”

Single chip approach

Kaestner and colleagues designed a chip that would generate discrete quantized voltages, by placing a semiconducting single-electron pump and a quantum Hall device in series. The voltage generated was dependent only on the current, which in turn was dependent only on the frequency of the single-electron pump.

“So you have now two sides of the triangle, if you like, combined in one device,” explains Kaestner. This offers an independent check on the Josephson voltage, because the Josephson effect relies on superconductor physics, and the new device on semiconductor physics. “Now one can [try to] produce exactly the same voltage with two fundamentally different physics…This is one elegant way of closing the triangle.”

Simplifying and scaling

“It is certainly a nice experiment to make these two quantum standards in one device,” comments Janssen. But the voltages it generates are only of the order of microvolts. Because quantum Hall devices produce noise in the region of nanovolts, he cautions “You would have to measure for a very long time to get any sort of resolution.”

The researchers, on the other hand, suggest that their device is easily scalable, which would allow the signal-to-noise ratio to be brought down significantly. Kaestner argues that an integrated circuit is also the most logical approach, since each micron-sized chip must be kept at a given temperature – about 1 K in this case – by cryostats that occupy several cubic metres of lab space.

But Janssen questions the practicality of connecting 10 current sources and 100 quantum Hall devices in series on one tiny chip, as the researchers propose. His team favour a current amplifier, which ramps the current from a separate single-electron device by a factor of about 10,000 without introducing much error.

“It is a nice experiment they have done, it is a nice device, but it would be very difficult for this device to compete with the traditional technology that we are using at the moment…there would have to be a significant breakthrough in device replication to make this competitive,” he says.

Kaestner hopes that this initial proof-of-principle work will prompt others to think of new and innovative combinations of integrated quantum devices. “Single-electron sources are very new, and I think the semiconductor industry is not aware of the possibilities,” he explains, adding “this is really a new circuit component.”

The research is published in Physical Review Letters.

How can you use X-rays to explore the nanoworld?

In less than 100 seconds, Annela Seddon explains why X-rays are such a useful imaging tool.

Thomas Kuhn's paradigm shift 50 years on

Thomas Kuhn book.jpg

By Hamish Johnston

“Great books are rare. This is one. Read it and you will see.”

That’s the opening paragraph of an introductory essay included in the 50th anniversary edition of Thomas Kuhn’s book The Structure of Scientific Revolutions, which was first published in August 1962 by University of Chicago Press. About 1.4 million copies of the book have been sold and it was recently described by the Observer as “one of the most influential books of the 20th century”.

The introductory essay is written by the Canadian philosopher Ian Hacking, who explores how Kuhn’s ideas have changed our view of the scientific process over the past five decades – and how controversial they were when the book was first published.

Kuhn was an American physicist who was born in 1922 and died in 1996. His career took an important turn in the 1950s when he taught a course at Harvard University on the history of science.

At the time, science was seen as a cumulative process in which knowledge is built up gradually. As such, it should have been possible for Kuhn to look back over the ages and conclude that the ancient Greeks understood X% of mid-20th century physics, while Newton understood Y%.

Instead, he realized that the way he understood physics was fundamentally different from how an ancient Greek philosopher understood physics. Indeed, he found it impossible to compare the science of ancient Greece with that of the mid-20th century – a property he later called “incommensurability”.

Fascinated by these ideas, Kuhn gave up physics and focused first on the history of science and then its philosophy.

Central to Kuhn’s analysis is the idea that our understanding of the universe has evolved in a series of discontinuities in which an intellectual framework (or paradigm) is built up, only to be brought crashing down in a crisis in which it becomes clear that theory is incapable of describing nature. An example familiar to physicists is the failure in the early 20th century of classical mechanics and electromagnetics to explain what we now understand as quantum physics. The two paradigms are incommensurate because quantum concepts such as superposition and entanglement simply do not exist in classical physics.

The intervals between these “paradigm shifts” – a much used and abused phrase popularized by Kuhn – are dubbed as periods of “normal science”, in which scientists work within a paradigm and solve “puzzles” that are thrown up when observation doesn’t quite agree with theory. This is exactly where particle physicists have been for the last 50 years with the Standard Model. Although many hope the Large Hadron Collider (LHC) will deliver observations that will put particle physics into a period of crisis, so far it has discovered exactly what it was expected to discover.

Indeed, it must be the fear of some particle physicists that the LHC will end up being an extremely expensive puzzle solver rather than a shifter of paradigms.

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