Pushing the limits – Light in the 21st Century

Guest post by Congcong Huang, Associated Editor, Nature Communications and Nicky Dean, Team Manager Physics, Nature Communications.

This week we conclude our series of ‘beautiful experiments with light’ featured in our poll and finally reach the new millennium in which lasers continue to enable powerful and diverse experiments.

Our story begins with the generation of ultrafast laser pulses. Following the invention of lasers in 1960 enormous efforts were made to shorten the pulse duration which led to femtosecond lasers in the late 1980s and finally in 2001 to the first reports of attosecond laser pulses. In one attosecond (10-18 s), light travels slightly more than the length of a water molecule, while molecules are essentially frozen during this time, with molecular vibration at femtosecond (10-15 s) and rotation at picosecond (10-12 s) timescales. This makes it possible to access the timescale of electron dynamics inside molecules.

As light pulses have been made ultrashort –short enough even to capture the motion of electrons – a natural question is whether the speed of light can be controlled to the same extent. It is not surprising that light slows down when it travels through glass or water, but this is only a modest effect. It was thus a stunning observation, made by Lene Hau and her group in Harvard in 1999, that light travels at a cycling speed – 7 orders of magnitude slower than c – in a sodium atom cloud right below its Bose-Einstein condensation temperature. The cold atoms alone cannot do the work; the use of a laser field that efficiently cancels light absorption, known as electromagnetically-induced transparency, makes the trick possible. The demonstration sparked a new chapter for laser controlled optical materials.

Meanwhile, more attempts at controlling the behavior of light were underway. As mentioned above, light slows down when it passes through a medium, an effect characterized by the medium’s refractive index. This index is normally positive, and it tells us how light rays will be bent when they move from one medium into another. You can see this effect by looking at a straw in a glass of water which appears to be sharply bent at the surface. In the late 1960s, Victor Veselago wondered what might happen if the refractive index was negative. He predicted that light entering such a medium should bend in the opposite sense to what we normally expect (as if the straw would bend the ‘wrong’ way). In 2001, David Smith and colleagues realized this prediction by constructing an artificial material, or ‘metamaterial’, made of an array of copper split-rings on circuit boards. Their metamaterial exhibited a negative refractive index at around 10 GHz. Following Smith’s demonstration, many more negative-index metamaterials have been made using all kinds of different structures, across a range of frequencies, including the visible spectrum.

Diffraction pattern of a virus particle, taken with an X-ray free electron laser.

Diffraction pattern of a virus particle, taken with an X-ray free electron laser.

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Back to light, back to reality

Guest post by Federico Levi, Associate Editor Nature Communications

The experiments in this week ’s blog entry accompanying our poll of ‘ the most beautiful experiment with light’ were carried out in the second half of the twentieth century, in which physicists were still struggling to accept the counter-intuitive implications of quantum physics.

One of the most bewildering embodiments of quantum theory is quantum entanglement.  When two particles are entangled, performing a measurement on one of them seems to instantaneously influence the other particle, even if it is light-years away. This paradox, famously termed ‘spooky action at a distance’ by Albert Einstein was formulated by Einstein, Podolsky and Rosen (EPR) in 1935. To restore reality, they argued that quantum physics could simply be our limited understanding of a deeper and less troubling theory, classically constructed over a set of ‘hidden variables’.

It took almost thirty years to devise a way to test their hypothesis. In 1964 John Stewart Bell demonstrated the famous theorem carrying his name, which showed how there would be an experimentally measurable difference between the prediction of quantum physics and that ‘less troubling theory’ imagined by EPR. Light provided the means to carry out this test. In 1972, by looking at the correlations in the linear polarization of photons emitted by an atomic cascade of calcium, Stuart J. Freedman and John F. Clauser tested Bell’s theorem at the Lawrence Berkeley Laboratory in California. The result was a landmark confirmation of quantum mechanics.

Jumping more than 10 years ahead, we find researchers dealing with the consequences of yet another quantum principle, namely the indistinguishability of fundamental particles. Two particles in exactly the same quantum state have to be considered essentially indistinguishable, and photons make no exception. In 1987 at Rochester University, New York, Chung Ki Hong, Zhe Yu Ou and Leonard Mandel showed what may be the most direct evidence of this principle. When a photon hits a beam splitter, it can continue in one of two ways with 50% probability. If two indistinguishable photons hit a beam splitter coincidentally, quantum interference forbids the outcome where they follow different output paths. The pronounced ‘dip’ in the measurement of simultaneous arrivals at the two outputs is a hallmark of the indistinguishability of a photon pair, a sought-after quality for quantum information applications.

Large-area metallic photonic crystal layer rolled onto a glass rod.

Large-area metallic photonic crystal layer rolled onto a glass rod.

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From the Big Bang to atomic clocks

Guest post by Amos Martinez, Associate Editor, Nature Communications

We kick off this week’s experiments for our poll with the discovery of a special kind of light: cosmic microwave background. The story of this discovery is a beautiful example of the fortuity of scientific discovery.

In 1964, Arno Penzias and Robert Wilson were looking for radio emission from the Milky Way using an antenna originally built for radio-wave satellite communications. They soon noticed a noise in the microwave region evenly spread in all directions of space. After eliminating every known noise source, including a pigeon’s nest in the 6m antenna, they reached the conclusion that the noise could only be coming from outside this galaxy.

Elsewhere, cosmologists were debating whether the universe had a beginning and had been created by a Big Bang or had always existed. Advocates of the big bang theory Robert H. Dicke, Jim Peebles, and David Wilkinson had predicted that had the big bang taken place it would have generated an enormous blast of radiation that should still be detectable in the microwave region with a sensitive enough device. Sure enough, that persistent noise measured by Penzias and Wilson turned out not to be caused by pigeons but by radiation generated during the creation of the Universe. This discovery represented the first solid experimental proof of the Big Bang and, as Stephen Hawking put it, the final nail in the coffin of the steady-state theory.

Cosmic microwave background: Big Bang’s afterglow. (Credit: ESA, HFI & LFI consortia.)

Cosmic microwave background: Big Bang’s afterglow. (Credit: ESA, HFI & LFI consortia.)

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Into the laser era

Guest post by Rachel Won International Editor, Nature Photonics

This week’s set of experiments featured in our poll  are all about the advent of the maser (microwave amplification by stimulated emission of radiation) and the optical maser, now known as the laser, and the remarkable wide impact these inventions had in science, technology and society.

The concept of stimulated emission was introduced in 1917 by Einstein, who found that the process of absorption by atoms must be accompanied by an amplification process such that the received radiation can stimulate the emission of the same kind of radiation. It was not until 1953 that the effect was experimentally demonstrated by Charles Townes and his two graduate students at Columbia University in New York. Their maser used stimulated emission in a stream of energized ammonia molecules to produce amplification of microwaves at a frequency of about 24.0 GHz. The development of a maser was simultaneously carried out by Nikolay Basov and Alexander Prokhorov at the Lebedev Institute in Moscow.

The achievements led to the award of the Nobel Prize in Physics in 1964 to Townes, Basov and Prokhorov.

The invention of the maser kicked off a race to create a similar device for visible light, now known as a laser (with ‘microwave’ replaced by ‘light’). In 1958 Townes, together with Arthur Schawlow, then at Bell Labs, published a paper extending the maser techniques to the infrared and optical region. The first working laser, however, was built by Theodore Maiman at Hughes Research Laboratories in 1960. His laser used a solid-state synthetic ruby crystal pumped by a flashlamp to produce red laser light at 694 nm.

Theodore Maiman and his invention, the first laser. (Photo credit: HRL Laboratories, LLC)

Theodore Maiman and his invention, the first laser. (Photo credit: HRL Laboratories, LLC)

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Betwixt and between

Guest post by Leonie Mueck, Associate Editor, Nature

In last week’s post you heard about beautiful experiments with light featured in our poll from the turn of the century. This week, we will talk about the time until the 1950s. And, while so many turning points in politics and history fall into that period, advances in optics and photonics were a bit betwixt and between. Scientists were modernizing their methods and instruments but still didn’t have modern-day tools like the laser, which in the 1960s would completely transform light-related research.

They did have highly advanced telescopes. When Edwin Hubble arrived at Mount Wilson Observatory in California it was 1919. By a lucky coincidence something else arrived there at around the same time: the Hooker Telescope, which allowed Hubble to perform detailed investigations on spiral nebulae. Thanks to his measurements, we now know that those nebulae are in fact distant galaxies. As jaw dropping as this finding was to his contemporaries, Hubble went on to show something even more ground-breaking. Looking at the Doppler shift of as many galaxies as possible, he found that the shift was proportional to the galaxies’ distance in 1929. The only plausible explanation for this phenomenon was that we live in an expanding Universe!

Andromeda Galaxy taken by Spitzer in infra-red, 24 micrometres. (Image: NASA/JPL–Caltech/K. Gordon, University of Arizona)

Andromeda Galaxy taken by Spitzer in infra-red, 24 micrometres. (Image: NASA/JPL–Caltech/K. Gordon, University of Arizona)

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Flash forward: new surprises with light

Guest post by Maria Maragkou, Associate Editor at Nature Materials

This week’s entries for the poll of the most beautiful experiments with light occurred around the turn of the 19th century.

Wilhelm Roentgen, a physics professor in Wurzburg, changed the course of medicine when he accidentally discovered X-rays, energy waves at frequencies from 0.1 – 10 nanometres. In November 1895, while experimenting with an electron-discharge tube covered with black cardboard, he noticed that a fluorescent screen further away was illuminated. Eventually he realised that the tube emitted a type of ray – marked X for unknown – that was blocked by dense material, such as lead or bones, but could penetrate other objects. As he held a piece of lead in front of the X-rays, he could see the contrast between bones and flesh on the fluorescent screen. A few weeks later, Roentgen took an X-ray picture of his wife’s hand, who allegedly claimed “I have seen my death” upon seeing it. With the discovery of X-rays, it became possible to look inside the human body without surgery and Roentgen earned the first ever Nobel Prize in Physics in 1901 for this remarkable invention.

Classic Nature Paper 1896.

Roentgen’s first X-ray image featured in Nature in 1896.

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Electrifying light

Guest post by Nicky Dean, Team Manager Physics, Nature Communications.

For this week’s set of experiments in our poll we will stick to the 19th century. Our first entry is from 1839, when Alexandre Edmond Becquerel invented the photovoltaic cell at the tender age of 19. While playing around in his father’s lab, Becquerel created an electrolytic cell from silver chloride in acid. After connecting it to platinum electrodes, he found that exposing it to light generated an electrical current. Currently, photovoltaics is one of the most active themes in materials research, as it may be key in our challenge to produce enough clean energy for the world for generations ahead.

Skipping ahead to 1887, our next experiment also unveiled some of the intricacies of the interaction between light and matter. While testing Maxwell’s theory of electromagnetic waves, Heinrich Hertz constructed a receiver device based around a gap between two metallic electrodes across which a spark could propagate. He realised that light promoted spark production but also found that this could be suppressed by inserting a piece of glass between the light source and his receiver. Crucially, this wasn’t the case for a sheet of quartz and from this, Hertz deduced that ultraviolet light, which glass absorbs but quartz does not, was responsible for easing the ejection of electrons from the metal electrodes, forming his sparks. Thus he discovered the photoelectric effect, in which electrons can be emitted from a metal by light.

Later on, Albert Einstein would explain this effect as arising from the quantum nature of light. Hertz didn’t think his findings were of any practical use and that they merely served to support Maxwell’s theories. Ironically, his investigations would eventually lead to such world-changing inventions as telegraphy, radio, and television.

While Hertz was busy submitting his findings to the Annalen der Physik, our final experiment was taking place on the other side of the Atlantic. The growing understanding of light throughout the 19th century led people to believe that light needed a medium to transit through, much as sound travels through air and waves ripple across water. Scientists called this medium the “luminiferous aether” and it was believed to permeate all of space. As such, while the Earth was whizzing around the Sun, it must be moving relative to the aether and so it must surely be possible to detect its presence.

Michael Morley interferometer (Wikimedia)

Michelson interferometer (Wikimedia)

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Theory of light and colours

Guest post by Iulia Georgescu, Senior Editor, Nature Physics

The next couple of experiments with light listed in our ‘beautiful experiments’ poll come from, well, the age of enlightenment.

First up is Christian Huygens. Although Galileo first used a telescope to make detailed observations of celestial objects, it was Huygens who by 1655 had crafted a telescope with a refracting lens powerful enough to resolve the ring structure of Saturn.

A decade later, in 1665, Isaac Newton discovered that a beam of white light is decomposed by a prism into its component colours, which another prism would combine back into white. At the time, the origin of colours was still debated and Newton’s experiment confirmed that it is light that gives colour to the world. His work influenced art and Newton also came up with the colour circle he described in his book Optiks.

Around the same time the Dutch merchant Antonie van Leeuwenhoek  was indulging into lens-making. He crafted powerful lenses and was the first to create a microscope with sufficient magnification to see single-celled organisms. He later dedicated himself to the characterization of tissues and micro-organisms, becoming the father of microbiology.

In 1679 Ole Rømer, working at the Royal Observatory in Paris, determined the speed of light by cataloguing the eclipses of Jupiter’s moon Io. Rømer was in fact trying to calculate the orbital period of the moon, but noticed time differences depending on the relative positions of Earth and Jupiter and realized that these could only be explained by the finite speed of light. He estimated that light would take 22 minutes to cross the diameter of the Earth’s orbit – not a bad estimate given his rough data.

Dispersive Prism.

Dispersive Prism (Wikimedia)

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Years of Light – Vote for your most beautiful light experiment

Guest post by Liesbeth Venema, Senior Physics Editor, Nature

We are basking in light. In our daily lives we encounter a multitude of light-based technologies from basic lighting, optical fibre communication, television and computer screens, to diagnostic techniques in healthcare. Sunlight energy harvesting will almost certainly be essential to match the world’s growing energy needs. The International Year of Light 2015, which is celebrating these achievements, and more, is now in full swing.

Of course, light plays a key role in scientific inquiry and discovery. To take a closer look, we have opened up a poll to find out what are the most striking, beautiful experiments with light. To have your say, please click here and simply select three experiments from the list of candidates that would be top of your list. Over the next few weeks, we will introduce the candidate experiments on this blog, in chronological order. The results of the poll will be announced here at the beginning of May.

So let us start – with Greek philosophers who of course already pondered the nature of light. They debated for example how we can see: with light emitted by our own eyes or by absorbing rays that reflect from objects?

Lighthouse Lens By Tonya Cook (Own work) [CC BY-SA 3.0 (https://creativecommons.org/licenses/by-sa/3.0)], via Wikimedia Commons)

Lighthouse Lens by Tonya Cook (Own work) (CC BY-SA 3.0, via Wikimedia Commons)

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