Archive for November, 2009

A Shortcut for Detecting Alien Worlds

Evidence of water found on moon

Nanomaterial Being Produced By the Ton

New Technology May Cool The Laptop

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Finding new alien worlds may become a lot easier. Astronomers have discovered that stars containing low amounts of the element lithium tend to host solar systems, a result that could dramatically reduce the time it will take to detect another Earth-like planet.

Chemical clue. Stars that form solar systems tend to deplete their lithium content. Credit: ESO/L. Calcada

Thus far, attempting to determine whether other stars play host to planets has required great patience and painstaking measurements. Astronomers scan the skies for two stellar phenomena. One is the barely perceptible but regular dimming of a star’s brightness that occurs when an orbiting planet passes between the star and Earth. The other is the regular but minuscule variation in a star’s radial velocity–its speed through the galaxy relative to Earth’s speed–which indicates that the star is being tugged by an orbiting planet’s gravity. Astronomers casually refer to the two phenomena as blink and wobble. Efforts to detect planets via these methods can take months–and they often come up empty.

Enter lithium. Some young stars form inside a small rotating disk of dust and gas, whereas others coalesce inside a much larger rotating disk, called a protoplanetary disk. Astronomers think that in the former case, the star rotates much faster because it isn’t subject to the gravitational drag imposed by the larger disk. This faster rotation, the thinking goes, pushes the star’s lighter elements, such as lithium, closer to the surface, where they can persist for billions of years. The presence of a protoplanetary disk, on the other hand, could hinder the star’s rotation, thereby causing lithium and other lighter elements to sink deep inside the star’s nuclear furnace, where they are consumed. If these scenarios are correct, stars with low levels of lithium should be more likely to host planets.

That’s what astronomers have found. In today’s issue of Nature, a team led by Garik Israelian of the Instituto de Astrofisica de Canarias in Spain’s Canary Islands surveyed 46 stars in our galactic neighborhood that host planets, along with 116 stars where so far no planets have been detected. Analysis of the light from the 46 stars showed low lithium content, the team reports, whereas the 116 stars all had higher levels of lithium–with over half sporting about 10 times more than the planet-hosting stars.

Physicist Dejan Vinkovi?, of the University of Split in Croatia calls the paper exciting, but he says it’s still unclear exactly why stars that host planets have low lithium levels. It’s possible, he says, that something other than the protoplanetary disk is contributing to the chemical’s loss.

By Phil Berardelli

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Finding new alien worlds may become a lot easier. Astronomers have discovered that stars containing low amounts of the element lithium tend to host solar systems, a result that could dramatically reduce the time it will take to detect another Earth-like planet.

Chemical clue. Stars that form solar systems tend to deplete their lithium content. Credit: ESO/L. Calcada

Thus far, attempting to determine whether other stars play host to planets has required great patience and painstaking measurements. Astronomers scan the skies for two stellar phenomena. One is the barely perceptible but regular dimming of a star’s brightness that occurs when an orbiting planet passes between the star and Earth. The other is the regular but minuscule variation in a star’s radial velocity–its speed through the galaxy relative to Earth’s speed–which indicates that the star is being tugged by an orbiting planet’s gravity. Astronomers casually refer to the two phenomena as blink and wobble. Efforts to detect planets via these methods can take months–and they often come up empty.

Enter lithium. Some young stars form inside a small rotating disk of dust and gas, whereas others coalesce inside a much larger rotating disk, called a protoplanetary disk. Astronomers think that in the former case, the star rotates much faster because it isn’t subject to the gravitational drag imposed by the larger disk. This faster rotation, the thinking goes, pushes the star’s lighter elements, such as lithium, closer to the surface, where they can persist for billions of years. The presence of a protoplanetary disk, on the other hand, could hinder the star’s rotation, thereby causing lithium and other lighter elements to sink deep inside the star’s nuclear furnace, where they are consumed. If these scenarios are correct, stars with low levels of lithium should be more likely to host planets.

That’s what astronomers have found. In today’s issue of Nature, a team led by Garik Israelian of the Instituto de Astrofisica de Canarias in Spain’s Canary Islands surveyed 46 stars in our galactic neighborhood that host planets, along with 116 stars where so far no planets have been detected. Analysis of the light from the 46 stars showed low lithium content, the team reports, whereas the 116 stars all had higher levels of lithium–with over half sporting about 10 times more than the planet-hosting stars.

Physicist Dejan Vinkovi?, of the University of Split in Croatia calls the paper exciting, but he says it’s still unclear exactly why stars that host planets have low lithium levels. It’s possible, he says, that something other than the protoplanetary disk is contributing to the chemical’s loss.

By Phil Berardelli

Start uga_filter:

Scientists announced tonight that they have discovered “buckets” of water on the Moon following the analysis of data from a spacecraft that was deliberately crashed into a lunar crater last month.


The researchers said the evidence for the existence of significant bodies of water ice hidden in polar craters on the Moon is “definitive” and that the total quantities could be big enough to support a permanently-manned lunar base.

It is the first time that the US National Aeronautics and Space Administration (Nasa) has been so categorical about the discovery of water on the Moon. Previous studies had only suggested that the presence of water might be possible and then only in trace amounts.

However, a painstakingly detailed analysis of the data from the LCROSS spacecraft, which was deliberately crashed into the Cabeus crater near the Lunar South Pole, has revealed a definitive chemical signature of water vapour in the plume of dust and debris that was released on impact.

In just one crater, the team estimates that there was at least 100 kilograms of water, enough to fill a dozen, two-gallon buckets. If similar amounts of water exist in other polar craters permanently shaded from sunlight there could be enough water available on the Moon to be used as drinking water for a lunar base – or used as a source of rocket fuel.

Anthony Colaprete, the principal scientist of LCROSS (the Lunar Crater Observation and Sensing Satellite), said that the “eureka moment” came when the team saw a spectroscopic line indicating the presence of the OH water molecule, which could only exist if water was present in the crater.

“What we found was indeed water…We vetted it, vetted it, vetted it, vetted it and vetted it some more as a team…I’m pretty impressed by the amount of water we see in this small, 20-metre crater,” Dr Colaprete said at a press briefing from Nasa’s Ames Research Centre in California.

“It’s safe to say it’s not a frozen lake with a perfectly frozen surface. It was probably mixed in with the surface. It would be an interesting place to walk around,” Dr Colaprete said.

Mike Wargo from Nasa said: “We’ve discovered significant quantities of water in a permanently-shaded crater on the Moon. We’re not just talking of water on the Moon, but lots of water.”

When LCROSS was crashed into the Moon, it was expected to eject a visible plume of debris six-miles high that was supposed to have been visible from Earth. However, Nasa scientists said at the time that the absence of a visible plume did not mean that the mission was a failure.

Nasa’s Gregory Delory said that the discovery is one of the most exciting to be made in connection with lunar exploration. “If we find water in large enough amounts it could be used as a resource for human exploration,” Dr Delory said.

“Now we know there’s water there thanks to LCROSS we can go to the next set of questions. It’s a new picture of the Moon. It’s going to be a very exciting time,” he said.

One of the unresolved questions is how the water could have got to the Moon. One theory is that it arrived on a comet and never evaporated in the shaded polar craters where temperatures are minus 220C.

Another possibility is that the water arrived on a solar wind, which is a stream of ionised hydrogen gas. A third theory is that is was dropped by a molecular cloud, or dropped by ice-laden cosmic dust. It might even be terrestrial water kicked up from Earth in a gigantic asteroid impact.

Nasa estimates that there are 12,500 square kilometres of permanently-shadowed terrain on the Moon and if the top 1 metre of this area were to hold just 1 per cent by mass of water, this would still produce thousands of litres of water.

It is not the first time that spacecraft have crashed into the Moon. In 1998, Nasa’s Lunar Prospector mission was deliberately crashed into a crater, which confirmed the presence of hydrogen, which may or may not have come from ancient stores of frozen water deposited in lunar craters over billions of years by passing comets.

By Steve Connor

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Scientists announced tonight that they have discovered “buckets” of water on the Moon following the analysis of data from a spacecraft that was deliberately crashed into a lunar crater last month.


The researchers said the evidence for the existence of significant bodies of water ice hidden in polar craters on the Moon is “definitive” and that the total quantities could be big enough to support a permanently-manned lunar base.

It is the first time that the US National Aeronautics and Space Administration (Nasa) has been so categorical about the discovery of water on the Moon. Previous studies had only suggested that the presence of water might be possible and then only in trace amounts.

However, a painstakingly detailed analysis of the data from the LCROSS spacecraft, which was deliberately crashed into the Cabeus crater near the Lunar South Pole, has revealed a definitive chemical signature of water vapour in the plume of dust and debris that was released on impact.

In just one crater, the team estimates that there was at least 100 kilograms of water, enough to fill a dozen, two-gallon buckets. If similar amounts of water exist in other polar craters permanently shaded from sunlight there could be enough water available on the Moon to be used as drinking water for a lunar base – or used as a source of rocket fuel.

Anthony Colaprete, the principal scientist of LCROSS (the Lunar Crater Observation and Sensing Satellite), said that the “eureka moment” came when the team saw a spectroscopic line indicating the presence of the OH water molecule, which could only exist if water was present in the crater.

“What we found was indeed water…We vetted it, vetted it, vetted it, vetted it and vetted it some more as a team…I’m pretty impressed by the amount of water we see in this small, 20-metre crater,” Dr Colaprete said at a press briefing from Nasa’s Ames Research Centre in California.

“It’s safe to say it’s not a frozen lake with a perfectly frozen surface. It was probably mixed in with the surface. It would be an interesting place to walk around,” Dr Colaprete said.

Mike Wargo from Nasa said: “We’ve discovered significant quantities of water in a permanently-shaded crater on the Moon. We’re not just talking of water on the Moon, but lots of water.”

When LCROSS was crashed into the Moon, it was expected to eject a visible plume of debris six-miles high that was supposed to have been visible from Earth. However, Nasa scientists said at the time that the absence of a visible plume did not mean that the mission was a failure.

Nasa’s Gregory Delory said that the discovery is one of the most exciting to be made in connection with lunar exploration. “If we find water in large enough amounts it could be used as a resource for human exploration,” Dr Delory said.

“Now we know there’s water there thanks to LCROSS we can go to the next set of questions. It’s a new picture of the Moon. It’s going to be a very exciting time,” he said.

One of the unresolved questions is how the water could have got to the Moon. One theory is that it arrived on a comet and never evaporated in the shaded polar craters where temperatures are minus 220C.

Another possibility is that the water arrived on a solar wind, which is a stream of ionised hydrogen gas. A third theory is that is was dropped by a molecular cloud, or dropped by ice-laden cosmic dust. It might even be terrestrial water kicked up from Earth in a gigantic asteroid impact.

Nasa estimates that there are 12,500 square kilometres of permanently-shadowed terrain on the Moon and if the top 1 metre of this area were to hold just 1 per cent by mass of water, this would still produce thousands of litres of water.

It is not the first time that spacecraft have crashed into the Moon. In 1998, Nasa’s Lunar Prospector mission was deliberately crashed into a crater, which confirmed the presence of hydrogen, which may or may not have come from ancient stores of frozen water deposited in lunar craters over billions of years by passing comets.

By Steve Connor

Start uga_filter:

Nano carbon Graphene is already being produced in decidedly non-nano quantities by Ohio-based Angstron. Yet the atom-thick nano-material was discovered so recently that researchers are still in the process of discovering what to use it for.


Graphene is an extremely low density material, almost an atomic-scale chicken wire made of carbon atoms and their bonds. It has been the focus of much research because of its exceptional electrical, mechanical and optical properties. It holds great promise in renewable energies.

Among the so far underutilized advantages Graphene offers are that it is fifty times stronger than steel, and it has five times the conductivity of copper, with only one quarter of the density.

There’s lots of possible uses for material with these properties, in renewable energy, aerospace, automotive, marine, electronics, construction, medical and telecommunications. And Graphene is a cost effective yet high quality alternative to carbon nanotubes, which were once the wonder nanomaterial, but which tended to stick together in clumps so was extremely difficult to form into composites.

Because of its light weight Graphene is the ideal substitute for copper for aerospace defense against emerging weapons technologies such as electromagnetic pulse as well as lightning strike protection for the aerospace market.

Graphene holds the promise of improving battery technology for hybrid cars and EVs. Adding Graphene to lithium batteries has recently been shown to prolong lithium battery life while increasing usable charge.

Angstron has a 22,000 square foot manufacturing facility in Dayton devoted to making this stuff, and is the first company to isolate single-layer and multi-layer graphene structures and successfully produce nano graphene sheets in large quantities.

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Nano carbon Graphene is already being produced in decidedly non-nano quantities by Ohio-based Angstron. Yet the atom-thick nano-material was discovered so recently that researchers are still in the process of discovering what to use it for.


Graphene is an extremely low density material, almost an atomic-scale chicken wire made of carbon atoms and their bonds. It has been the focus of much research because of its exceptional electrical, mechanical and optical properties. It holds great promise in renewable energies.

Among the so far underutilized advantages Graphene offers are that it is fifty times stronger than steel, and it has five times the conductivity of copper, with only one quarter of the density.

There’s lots of possible uses for material with these properties, in renewable energy, aerospace, automotive, marine, electronics, construction, medical and telecommunications. And Graphene is a cost effective yet high quality alternative to carbon nanotubes, which were once the wonder nanomaterial, but which tended to stick together in clumps so was extremely difficult to form into composites.

Because of its light weight Graphene is the ideal substitute for copper for aerospace defense against emerging weapons technologies such as electromagnetic pulse as well as lightning strike protection for the aerospace market.

Graphene holds the promise of improving battery technology for hybrid cars and EVs. Adding Graphene to lithium batteries has recently been shown to prolong lithium battery life while increasing usable charge.

Angstron has a 22,000 square foot manufacturing facility in Dayton devoted to making this stuff, and is the first company to isolate single-layer and multi-layer graphene structures and successfully produce nano graphene sheets in large quantities.

Start uga_filter:

By taking advantage of the vagaries of the natural world, Duke University engineers have developed a novel approach that they believe can more efficiently harvest electricity from the motions of everyday life.

Energy harvesting is the process of converting one form of energy, such as motion, into another form of energy, in this case electricity. Strategies range from the development of massive wind farms to produce large amounts of electricity to using the vibrations of walking to power small electronic devices.

Although motion is an abundant source of energy, only limited success has been achieved because the devices used only perform well over a narrow band of frequencies. These so-called “linear” devices can work well, for example, if the character of the motion is fairly constant, such as the cadence of a person walking. However, as researchers point out, the pace of someone walking, as with all environmental sources, changes over time and can vary widely.

“The ideal device would be one that could convert a range of vibrations instead of just a narrow band,” said Samuel Stanton, graduate student in Duke’s Pratt School of Engineering, working in the laboratory of Brian Mann, assistant professor of mechanical engineering and materials sciences. The team, which included undergraduate Clark McGehee, published the results of their latest experiments early online in Applied Physics Letters.

“Nature doesn’t work in a single frequency, so we wanted to come up with a device that would work over a broad range of frequencies,” Stanton said. “By using magnets to ‘tune’ the bandwidth of the experimental device, we were able verify in the lab that this new non-linear approach can outperform conventional linear devices.”

Although the device they constructed looks deceptively simple, it was able to prove the team’s theories on a small scale. It is basically a small cantilever, several inches long and a quarter inch wide, with an end magnet that interacts with nearby magnets. The cantilever base itself is made of a piezoelectric material, which has the unique property of releasing electrical voltage when it is strained.

The key to the new approach involved placing moveable magnets of opposing poles on either side of the magnet at the end of the cantilever arm. By changing the distance of the moveable magnets, the researchers were able to “tune” the interactions of the system with its environment, and thus produce electricity over a broader spectrum of frequencies.

“These results suggest to us that this non-linear approach could harvest more of the frequencies from the same ambient vibrations,” Mann said. “More importantly, being able to capture more of the bandwidth makes it more likely that these types of devices could someday rival batteries as a portable power source.”

The range of applications for non-linear energy harvesters varies widely. For example, Mann is working on a project that would use the motion of ocean waves to power an array of sensors that would be carried inside ocean buoys.

“These non-linear systems are self-sustaining, so they are ideal for any electrical device that needs batteries and is in a location that is difficult to access,” Mann said.

For example, the motion of walking could provide enough electricity to power an implanted device, such as a pacemaker or cardiac defibrillator. On a larger scale, sensors in the environment or spacecraft could be powered by the everyday natural vibrations around them, Mann said.

Mann’s research is supported by the Office of Naval Research.

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By taking advantage of the vagaries of the natural world, Duke University engineers have developed a novel approach that they believe can more efficiently harvest electricity from the motions of everyday life.

Energy harvesting is the process of converting one form of energy, such as motion, into another form of energy, in this case electricity. Strategies range from the development of massive wind farms to produce large amounts of electricity to using the vibrations of walking to power small electronic devices.

Although motion is an abundant source of energy, only limited success has been achieved because the devices used only perform well over a narrow band of frequencies. These so-called “linear” devices can work well, for example, if the character of the motion is fairly constant, such as the cadence of a person walking. However, as researchers point out, the pace of someone walking, as with all environmental sources, changes over time and can vary widely.

“The ideal device would be one that could convert a range of vibrations instead of just a narrow band,” said Samuel Stanton, graduate student in Duke’s Pratt School of Engineering, working in the laboratory of Brian Mann, assistant professor of mechanical engineering and materials sciences. The team, which included undergraduate Clark McGehee, published the results of their latest experiments early online in Applied Physics Letters.

“Nature doesn’t work in a single frequency, so we wanted to come up with a device that would work over a broad range of frequencies,” Stanton said. “By using magnets to ‘tune’ the bandwidth of the experimental device, we were able verify in the lab that this new non-linear approach can outperform conventional linear devices.”

Although the device they constructed looks deceptively simple, it was able to prove the team’s theories on a small scale. It is basically a small cantilever, several inches long and a quarter inch wide, with an end magnet that interacts with nearby magnets. The cantilever base itself is made of a piezoelectric material, which has the unique property of releasing electrical voltage when it is strained.

The key to the new approach involved placing moveable magnets of opposing poles on either side of the magnet at the end of the cantilever arm. By changing the distance of the moveable magnets, the researchers were able to “tune” the interactions of the system with its environment, and thus produce electricity over a broader spectrum of frequencies.

“These results suggest to us that this non-linear approach could harvest more of the frequencies from the same ambient vibrations,” Mann said. “More importantly, being able to capture more of the bandwidth makes it more likely that these types of devices could someday rival batteries as a portable power source.”

The range of applications for non-linear energy harvesters varies widely. For example, Mann is working on a project that would use the motion of ocean waves to power an array of sensors that would be carried inside ocean buoys.

“These non-linear systems are self-sustaining, so they are ideal for any electrical device that needs batteries and is in a location that is difficult to access,” Mann said.

For example, the motion of walking could provide enough electricity to power an implanted device, such as a pacemaker or cardiac defibrillator. On a larger scale, sensors in the environment or spacecraft could be powered by the everyday natural vibrations around them, Mann said.

Mann’s research is supported by the Office of Naval Research.

Start uga_filter:

Does your laptop sometimes get so hot that it can almost be used to fry eggs? New technology may help cool it and give information technology a unique twist, says Jairo Sinova, a Texas A&M University physics professor.

Sinova and colleagues from Hitachi Cambridge Laboratory, Institute of Physics ASCR, University of Cambridge and University of Nottingham have had their research published in the renowned journal Nature Physics.

Laptops are getting increasingly powerful, but as their sizes are getting smaller they are heating up, so how to deal with excessive heat becomes a headache, Sinova explains.

“The crux of the problem is the way information is processed,” Sinova notes. “Laptops and some other devices use flows of electric charge to process information, but they also produce heat.

“Theoretically, excessive heat may melt the laptop,” he adds. “This also wastes a considerable amount of energy.”

Is there a solution?

One approach may be found in Sinova’s research — an alternative way to process information.

“Our research looks at the spin of electrons, tiny particles that naked eyes cannot detect,” the Texas A&M professor explains. “The directions they spin can be used to record and process information.”

To process information, Sinova says, it is necessary to create information, transmit the information and read the information. How these are done is the big question.

“The device we designed injects the electrons with spin pointing in a particular direction according to the information we want to process, and then we transmit the electrons to another place in the device but with the spin still surviving, and finally we are able to measure the spin direction via a voltage that they produce,” Sinova explains.

The biggest challenge to creating a spin-based device is the distance that the spins will survive in a particular direction.

“Transmission is no problem. You can think for comparison that if the old devices could only transmit the information to several hundred feet away, with our device, information can be easily transmitted to hundreds of miles away,” he says. “It is very efficient.”

Talking about its practical application, Sinova is very optimistic. “This new device, as the only all-semiconductor spin-based device for possible information processing, has a lot of real practical potential,” he says. “One huge thing is that it is operational at room temperature, which nobody has been able to achieve until now. It may bring in a new and much more efficient way to process information.”

Start uga_in_feed Ending uga_in_feed: Start uga_track_user Start uga_get_option: ignore_users uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: ignore_users (1) Start uga_get_option: max_user_level uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: max_user_level (8) Tracking user with level Ending uga_track_user: 1 Calling preg_replace_callback: ]*?)href\s*=\s*['"](.*?)['"]([^>]*)>(.*?) Ending uga_filter:

Does your laptop sometimes get so hot that it can almost be used to fry eggs? New technology may help cool it and give information technology a unique twist, says Jairo Sinova, a Texas A&M University physics professor.

Sinova and colleagues from Hitachi Cambridge Laboratory, Institute of Physics ASCR, University of Cambridge and University of Nottingham have had their research published in the renowned journal Nature Physics.

Laptops are getting increasingly powerful, but as their sizes are getting smaller they are heating up, so how to deal with excessive heat becomes a headache, Sinova explains.

“The crux of the problem is the way information is processed,” Sinova notes. “Laptops and some other devices use flows of electric charge to process information, but they also produce heat.

“Theoretically, excessive heat may melt the laptop,” he adds. “This also wastes a considerable amount of energy.”

Is there a solution?

One approach may be found in Sinova’s research — an alternative way to process information.

“Our research looks at the spin of electrons, tiny particles that naked eyes cannot detect,” the Texas A&M professor explains. “The directions they spin can be used to record and process information.”

To process information, Sinova says, it is necessary to create information, transmit the information and read the information. How these are done is the big question.

“The device we designed injects the electrons with spin pointing in a particular direction according to the information we want to process, and then we transmit the electrons to another place in the device but with the spin still surviving, and finally we are able to measure the spin direction via a voltage that they produce,” Sinova explains.

The biggest challenge to creating a spin-based device is the distance that the spins will survive in a particular direction.

“Transmission is no problem. You can think for comparison that if the old devices could only transmit the information to several hundred feet away, with our device, information can be easily transmitted to hundreds of miles away,” he says. “It is very efficient.”

Talking about its practical application, Sinova is very optimistic. “This new device, as the only all-semiconductor spin-based device for possible information processing, has a lot of real practical potential,” he says. “One huge thing is that it is operational at room temperature, which nobody has been able to achieve until now. It may bring in a new and much more efficient way to process information.”

Start uga_filter:

High-performance energy storage technologies for the automotive industry or mobile phone batteries and notebooks providing long battery times — these visions of the future are being brought one step nearer by scientists from Graz University of Technology.

Stefan Koller. Researchers at the Institute for Chemistry and Technology of Materials have developed a new method that utilises silicon for lithium-ion batteries. Its storage capacity is ten times higher than the graphite substrate which has been used up to now, and promises considerable improvements for users.

Stefan Koller. Researchers at the Institute for Chemistry and Technology of Materials have developed a new method that utilises silicon for lithium-ion batteries. Its storage capacity is ten times higher than the graphite substrate which has been used up to now, and promises considerable improvements for users.

Researchers at the Institute for Chemistry and Technology of Materials have developed a new method that utilises silicon for lithium-ion batteries. Its storage capacity is ten times higher than the graphite substrate which has been used up to now, and promises considerable improvements for users.

The new findings — which came to light in the “NanoPoliBat” EU project — have been recently submitted to the patent office by researchers together with their co-operation partner Varta Microbattery.

Modern electronic devices need more energy and even the automotive industry is hankering after increasingly powerful energy storage systems. The technological development of battery research has been inadequate for some time now. “A real revolution is needed for the development of the next generation. We need new storage materials for lithium-ion batteries,” explains battery researcher Stefan Koller, who is familiar with the topic from his doctoral thesis. Together with colleagues from science and industry, he has managed to develop such a substrate material for electrochemical reactions at a low price.

Silicon gel on graphite

In the newly developed process, researchers utilise a silicon-containing gel and apply it to the graphite substrate material. “In this way the graphite works as a buffer, cushioning the big changes in volume of the silicon during the uptake and transfer of lithium ions,” explains Koller.

Silicon has a lithium-ion storage capacity some ten times higher than the up-to-now commercially used graphite. The new material can thus store more than double the quantity of lithium ions without changes to the battery lifetime.

This method is far cheaper than the previous ones in which silicon is separated in the gas phase. The challenge lies in the poor storage density of materials in the counter electrode in the whole battery, something which we have been doing intensive research on,” says Koller.

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High-performance energy storage technologies for the automotive industry or mobile phone batteries and notebooks providing long battery times — these visions of the future are being brought one step nearer by scientists from Graz University of Technology.

Stefan Koller. Researchers at the Institute for Chemistry and Technology of Materials have developed a new method that utilises silicon for lithium-ion batteries. Its storage capacity is ten times higher than the graphite substrate which has been used up to now, and promises considerable improvements for users.

Stefan Koller. Researchers at the Institute for Chemistry and Technology of Materials have developed a new method that utilises silicon for lithium-ion batteries. Its storage capacity is ten times higher than the graphite substrate which has been used up to now, and promises considerable improvements for users.

Researchers at the Institute for Chemistry and Technology of Materials have developed a new method that utilises silicon for lithium-ion batteries. Its storage capacity is ten times higher than the graphite substrate which has been used up to now, and promises considerable improvements for users.

The new findings — which came to light in the “NanoPoliBat” EU project — have been recently submitted to the patent office by researchers together with their co-operation partner Varta Microbattery.

Modern electronic devices need more energy and even the automotive industry is hankering after increasingly powerful energy storage systems. The technological development of battery research has been inadequate for some time now. “A real revolution is needed for the development of the next generation. We need new storage materials for lithium-ion batteries,” explains battery researcher Stefan Koller, who is familiar with the topic from his doctoral thesis. Together with colleagues from science and industry, he has managed to develop such a substrate material for electrochemical reactions at a low price.

Silicon gel on graphite

In the newly developed process, researchers utilise a silicon-containing gel and apply it to the graphite substrate material. “In this way the graphite works as a buffer, cushioning the big changes in volume of the silicon during the uptake and transfer of lithium ions,” explains Koller.

Silicon has a lithium-ion storage capacity some ten times higher than the up-to-now commercially used graphite. The new material can thus store more than double the quantity of lithium ions without changes to the battery lifetime.

This method is far cheaper than the previous ones in which silicon is separated in the gas phase. The challenge lies in the poor storage density of materials in the counter electrode in the whole battery, something which we have been doing intensive research on,” says Koller.

Start uga_filter:

Every year, scientists learn something new about the inner workings of lightning.

Central Africa receives the most flashes of lightning per square kilometer, while the polar regions receive the least. This global map of lightning flash density was created with data from the Lightning Imaging Sensor (LIS) aboard the Tropical Measuring Mission (TRMM) and the Optical Transient Detector (OTD) aboard the Microlab-1 spacecraft. (Credit: Jeff De La Beaujardiere, Scientific Visualization Studio)

Central Africa receives the most flashes of lightning per square kilometer, while the polar regions receive the least. This global map of lightning flash density was created with data from the Lightning Imaging Sensor (LIS) aboard the Tropical Measuring Mission (TRMM) and the Optical Transient Detector (OTD) aboard the Microlab-1 spacecraft. (Credit: Jeff De La Beaujardiere, Scientific Visualization Studio)

With satellites, they have discovered that more than 1.2 billion lightning flashes occur around the world every year. (Rwanda has the most flashes per square kilometer, while flashes are rare in polar regions.) Laboratory and field experiments have revealed that the core of some lightning bolts reaches 30,000 Kelvin (53,540 ºF), a temperature hot enough to instantly melt sand and break oxygen and nitrogen molecules into individual atoms.

And then there is this: each of those billion lightning flashes produces a puff of nitrogen oxide gas (NOx) that reacts with sunlight and other gases in the atmosphere to produce ozone. Near Earth’s surface, ozone can harm human and plant health; higher in the atmosphere, it is a potent greenhouse gas; and in the stratosphere, its blocks cancer-causing ultraviolet radiation.

In 1827, the German chemist Justin von Liebig first observed that lightning produced NOx — scientific shorthand for a gaseous mixture of nitrogen and oxygen that includes nitric oxide (NO) and nitrogen dioxide (NO2). Nearly two centuries later, the topic continues to attract the attention of scientists.

Fossil fuel combustion, microbes in the soil, lightning, and forest fires all produce NOx. Scientists think lightning’s contribution to Earth’s NOx budget — probably about 10 percent — is relatively small compared to fossil fuel emissions. Yet they haven’t been sure whether global estimates of NOx produced by lightning are accurate.

“There’s still a lot of uncertainty about how much NOx lightning produces,” said Kenneth Pickering, an atmospheric scientist who studies lightning at NASA’s Goddard Space Flight Center in Greenbelt, Md. “Indeed, even recent published estimates of lightning’s global NOx production still vary by as much as a factor of four. We’re trying to narrow that uncertainty in order to improve the accuracy of both global climate models and regional air quality models.”

Using data gleaned from aircraft observations and satellites, Pickering and Goddard colleague Lesley Ott recently took steps toward a better global estimate of lightning-produced NOx and found that lightning may have a considerably stronger impact on the climate in the mid-latitudes and subtropics — and less on surface air quality — than previously thought.

According to a new paper by Ott and Pickering in the Journal of Geophysical Research, each flash of lightning on average in the several mid-latitude and subtropical thunderstorms studied turned 7 kilograms (15.4 pounds) of nitrogen into chemically reactive NOx. “In other words, you could drive a new car across the United States more than 50 times and still produce less than half as much NOx as an average lightning flash,” Ott estimated. The results were published July.

When the researchers multiplied the number of lightning strokes worldwide by 7 kilograms, they found that the total amount of NOx produced by lightning per year is 8.6 terragrams, or 8.6 million metric tons. “That’s somewhat high compared to previous estimates,” said Pickering.

More remarkable than the number, however, is where the NOx is produced. A decade ago, many researchers believed cloud-to-ground lightning produced far more NOx per flash than intracloud lightning, which occurs within a cloud and far higher in the atmosphere.

The new evidence suggests that the two types of lightning produce approximately the same amount of NOx per flash on average. But since most lightning is intracloud, this suggests a great deal more NOx is produced and remains higher in the atmosphere. Compounding this effect, the research also shows that strong updrafts within thunderstorms help transfer lower level NOx to higher altitudes in the atmosphere.

“We’ve really started to question some of our old assumptions as we’ve gotten better at measuring lightning in the field,” said Ott.

The observations spring out of field projects conducted in Germany, Colorado, Florida, Kansas, and Oklahoma between 1985 and 2002. For example, in a NASA field campaign called the Cirrus Regional Study of Tropical Anvils and Cirrus Layers Florida — Florida Area Cirrus Experiment (CRYSTAL-FACE) aircraft flew headlong through anvil-shaped thunderheads to measure the anatomy of the thunderstorms. Sensors sampled the pressure, humidity, temperature, wind, and the amount of trace gases such as NOx and ozone.

Later, Ott input this data, as well as additional data from the U.S. National Lightning Detection Network and NASA’s Total Ozone Mapping Spectrometer (TOMS), into a complex computer model that simulated the six storms and calculated the amount of NOx that the average flash of lightning produced. With that number, she could then estimate the amount of NOx that lightning produces globally each year.

“One of the things we’re trying to understand is how much ozone changes caused by lightning affect radiative forcing, and how that might translate into climate impacts,” said Pickering.

There’s a possibility that lightning could produce a feedback cycle that accelerates global warming. “If a warming globe creates more thunderstorms,” Pickering noted, “that could lead to more NOx production, which leads to more ozone, more radiative forcing, and more warming,” Pickering emphasizes that this is a theory, and while some global modeling studies suggest this is indeed the case, it has not yet been borne out by field observations.

The new findings also have implications for regional air quality models. Scientists from the U.S. Environmental Protection Agency (EPA), for example, are already plugging the new numbers into a widely-used air quality model called the Community Multi-scale Air Quality Model. “Lightning is one of the smaller factors for surface ozone levels, but in some cases a surge of ozone formed from lightning NOx could be enough to put a community out of compliance with EPA air quality standards during certain times of the year,” said Pickering.

Pickering offered one important caveat to the findings: The value of 7 kilograms per flash was derived without consideration of lightning from storms in the tropics, where most of the Earth’s lightning occurs. Only very recently have data become available for tropical regions, he noted.

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Every year, scientists learn something new about the inner workings of lightning.

Central Africa receives the most flashes of lightning per square kilometer, while the polar regions receive the least. This global map of lightning flash density was created with data from the Lightning Imaging Sensor (LIS) aboard the Tropical Measuring Mission (TRMM) and the Optical Transient Detector (OTD) aboard the Microlab-1 spacecraft. (Credit: Jeff De La Beaujardiere, Scientific Visualization Studio)

Central Africa receives the most flashes of lightning per square kilometer, while the polar regions receive the least. This global map of lightning flash density was created with data from the Lightning Imaging Sensor (LIS) aboard the Tropical Measuring Mission (TRMM) and the Optical Transient Detector (OTD) aboard the Microlab-1 spacecraft. (Credit: Jeff De La Beaujardiere, Scientific Visualization Studio)

With satellites, they have discovered that more than 1.2 billion lightning flashes occur around the world every year. (Rwanda has the most flashes per square kilometer, while flashes are rare in polar regions.) Laboratory and field experiments have revealed that the core of some lightning bolts reaches 30,000 Kelvin (53,540 ºF), a temperature hot enough to instantly melt sand and break oxygen and nitrogen molecules into individual atoms.

And then there is this: each of those billion lightning flashes produces a puff of nitrogen oxide gas (NOx) that reacts with sunlight and other gases in the atmosphere to produce ozone. Near Earth’s surface, ozone can harm human and plant health; higher in the atmosphere, it is a potent greenhouse gas; and in the stratosphere, its blocks cancer-causing ultraviolet radiation.

In 1827, the German chemist Justin von Liebig first observed that lightning produced NOx — scientific shorthand for a gaseous mixture of nitrogen and oxygen that includes nitric oxide (NO) and nitrogen dioxide (NO2). Nearly two centuries later, the topic continues to attract the attention of scientists.

Fossil fuel combustion, microbes in the soil, lightning, and forest fires all produce NOx. Scientists think lightning’s contribution to Earth’s NOx budget — probably about 10 percent — is relatively small compared to fossil fuel emissions. Yet they haven’t been sure whether global estimates of NOx produced by lightning are accurate.

“There’s still a lot of uncertainty about how much NOx lightning produces,” said Kenneth Pickering, an atmospheric scientist who studies lightning at NASA’s Goddard Space Flight Center in Greenbelt, Md. “Indeed, even recent published estimates of lightning’s global NOx production still vary by as much as a factor of four. We’re trying to narrow that uncertainty in order to improve the accuracy of both global climate models and regional air quality models.”

Using data gleaned from aircraft observations and satellites, Pickering and Goddard colleague Lesley Ott recently took steps toward a better global estimate of lightning-produced NOx and found that lightning may have a considerably stronger impact on the climate in the mid-latitudes and subtropics — and less on surface air quality — than previously thought.

According to a new paper by Ott and Pickering in the Journal of Geophysical Research, each flash of lightning on average in the several mid-latitude and subtropical thunderstorms studied turned 7 kilograms (15.4 pounds) of nitrogen into chemically reactive NOx. “In other words, you could drive a new car across the United States more than 50 times and still produce less than half as much NOx as an average lightning flash,” Ott estimated. The results were published July.

When the researchers multiplied the number of lightning strokes worldwide by 7 kilograms, they found that the total amount of NOx produced by lightning per year is 8.6 terragrams, or 8.6 million metric tons. “That’s somewhat high compared to previous estimates,” said Pickering.

More remarkable than the number, however, is where the NOx is produced. A decade ago, many researchers believed cloud-to-ground lightning produced far more NOx per flash than intracloud lightning, which occurs within a cloud and far higher in the atmosphere.

The new evidence suggests that the two types of lightning produce approximately the same amount of NOx per flash on average. But since most lightning is intracloud, this suggests a great deal more NOx is produced and remains higher in the atmosphere. Compounding this effect, the research also shows that strong updrafts within thunderstorms help transfer lower level NOx to higher altitudes in the atmosphere.

“We’ve really started to question some of our old assumptions as we’ve gotten better at measuring lightning in the field,” said Ott.

The observations spring out of field projects conducted in Germany, Colorado, Florida, Kansas, and Oklahoma between 1985 and 2002. For example, in a NASA field campaign called the Cirrus Regional Study of Tropical Anvils and Cirrus Layers Florida — Florida Area Cirrus Experiment (CRYSTAL-FACE) aircraft flew headlong through anvil-shaped thunderheads to measure the anatomy of the thunderstorms. Sensors sampled the pressure, humidity, temperature, wind, and the amount of trace gases such as NOx and ozone.

Later, Ott input this data, as well as additional data from the U.S. National Lightning Detection Network and NASA’s Total Ozone Mapping Spectrometer (TOMS), into a complex computer model that simulated the six storms and calculated the amount of NOx that the average flash of lightning produced. With that number, she could then estimate the amount of NOx that lightning produces globally each year.

“One of the things we’re trying to understand is how much ozone changes caused by lightning affect radiative forcing, and how that might translate into climate impacts,” said Pickering.

There’s a possibility that lightning could produce a feedback cycle that accelerates global warming. “If a warming globe creates more thunderstorms,” Pickering noted, “that could lead to more NOx production, which leads to more ozone, more radiative forcing, and more warming,” Pickering emphasizes that this is a theory, and while some global modeling studies suggest this is indeed the case, it has not yet been borne out by field observations.

The new findings also have implications for regional air quality models. Scientists from the U.S. Environmental Protection Agency (EPA), for example, are already plugging the new numbers into a widely-used air quality model called the Community Multi-scale Air Quality Model. “Lightning is one of the smaller factors for surface ozone levels, but in some cases a surge of ozone formed from lightning NOx could be enough to put a community out of compliance with EPA air quality standards during certain times of the year,” said Pickering.

Pickering offered one important caveat to the findings: The value of 7 kilograms per flash was derived without consideration of lightning from storms in the tropics, where most of the Earth’s lightning occurs. Only very recently have data become available for tropical regions, he noted.

Start uga_filter:

It may look like little more than fishing line, but plastic optical fibre or POF promises to revolutionise high-speed last-mile communications networks. Its evolution is being aided by groundbreaking research in Europe.

Plastic optical fibre (POF) for data transmission is often described as the “consumer” version of glass optical fibre, the kind that makes up the long-distance trunk routes of telecommunications networks. Flexible plastic fibres, with a core diameter of 1mm and made from polymethyl methacrylate (PMMA), are cheap to produce, easy to install and transmit light in the visible range as opposed to infrared, making maintenance easier and safer. But those properties typically come at the expense of lower bandwidth and high attenuation, restricting their use to sending data over short distances at relatively low speeds.

As a result, POF networks have mostly been used as an alternative to copper wires for short-distance — or so-called last-mile — data transmission. In offices and homes, POF has become a popular alternative for setting up local area networks (LANs), while in cars plastic fibres have replaced copper for sending video signals to onboard entertainment systems or obtaining data from sensors. That, however, is but a fraction of the potential uses for the technology.

Groundbreaking research by a team of European scientists working in the EU-funded POLYCOM project has helped put POF on track for use in optical computing, ultra-high-speed LANs, new sensing devices and even clothing that lights up for safety or simply fashion.

“The range of applications for POF and the optical technology that underlies it is extensive… and its development beyond the current state of the art could benefit a wide range of sectors over the coming years,” explains Guglielmo Lanzani, a researcher at Milan Technical University and coordinator of POLYCOM.

World first in all-optical, high-speed switching

One of the key achievements of the POLYCOM team is the world’s first all-optical high-speed switch for POF networks, a crucial step towards blisteringly fast optical data transmission. The technique, tested at the 520-nanometer wavelength (at which light appears green), involves using two beams of light from a single pulsed laser source in a special plastic optical fibre, the physical properties of which have been chemically modified, or doped, with photoactive polymers to change the way it transmits photons.

By overlapping the light pulses in space and time it is possible to use one light pulse to cancel out the other, thus switching it from on to off and transmitting a data signal. And because of the specific properties of the doped POF the cancellation of the light is reversed within only a few hundred femtoseconds (one femtosecond is one billionth of one millionth of a second).

“Not only will this increase data transmission rates in POF networks, but it could be used for time division multiplexing (TDM) to increase the bandwidth of optical networks beyond what is possible with current wavelength division multiplexing (WDM) techniques,” Lanzani says.

Whereas WDM uses light pulses of different colours to create different channels and therefore carry more data along a single fibre, TDM, as its name suggests, separates the pulses by time, allowing two or more signals to be carried as asynchronous sub-channels within a single fibre.

With bandwidth demands set to continue increasing, separating the signals at the transmission end and sorting them at the receiving end will require switching at rates that only an all-optical — as opposed to an optical-electronic solution — will be able to achieve.

The doped-POF used by the POLYCOM team for the all-optical switch is a polyfluorene called F8BT, one of several different materials studied by the group to test their optical properties. Several new types of doped POF were also developed by the researchers.

“In all, we developed and tested five or six new generations of materials, using different chemical agents to dope them in order to improve their optical properties and achieve very good dispersion of the doping agent in the polymer in several cases,” Lanzani says. “Each of the materials has different characteristics that may make them suitable for different applications.”

Glow in the dark clubbers?

An offshoot of the research was work on optofluidic channels in which the researchers exploited the optical properties of conjugated polymers in a fluid solution inside a microfluidic channel in order to produce a compact photonic device. Such a device could be used as the basis for a biochip for health applications in which optical sensors could be used to identify bacteria, viruses and even DNA strands in body fluids.

Though a commercial optofluidic device is probably some way off, Lanzani notes that the team’s research is likely to feed into a variety of commercial applications over the coming years, particularly as interest grows in the range of uses to which POF can be put.

“The auto industry will continue to demand faster and higher capacity POF networks as cars become more complex, while interest in using POF for LANs and telecommunications is continuing to grow,” Lanzani notes.

In addition, some research groups and companies are looking to use POF to create new sensing devices, relying on changes in the way the fibres carry light to measure liquid levels or humidity. And given its low cost and, with the right materials, dazzling luminescent properties, it is also being considered for safety clothing and probably even by clubbers looking to stand out in the crowd!

POLYCOM received funding from the FET Open strand of the EU’s Sixth Framework Programme for research.

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It may look like little more than fishing line, but plastic optical fibre or POF promises to revolutionise high-speed last-mile communications networks. Its evolution is being aided by groundbreaking research in Europe.

Plastic optical fibre (POF) for data transmission is often described as the “consumer” version of glass optical fibre, the kind that makes up the long-distance trunk routes of telecommunications networks. Flexible plastic fibres, with a core diameter of 1mm and made from polymethyl methacrylate (PMMA), are cheap to produce, easy to install and transmit light in the visible range as opposed to infrared, making maintenance easier and safer. But those properties typically come at the expense of lower bandwidth and high attenuation, restricting their use to sending data over short distances at relatively low speeds.

As a result, POF networks have mostly been used as an alternative to copper wires for short-distance — or so-called last-mile — data transmission. In offices and homes, POF has become a popular alternative for setting up local area networks (LANs), while in cars plastic fibres have replaced copper for sending video signals to onboard entertainment systems or obtaining data from sensors. That, however, is but a fraction of the potential uses for the technology.

Groundbreaking research by a team of European scientists working in the EU-funded POLYCOM project has helped put POF on track for use in optical computing, ultra-high-speed LANs, new sensing devices and even clothing that lights up for safety or simply fashion.

“The range of applications for POF and the optical technology that underlies it is extensive… and its development beyond the current state of the art could benefit a wide range of sectors over the coming years,” explains Guglielmo Lanzani, a researcher at Milan Technical University and coordinator of POLYCOM.

World first in all-optical, high-speed switching

One of the key achievements of the POLYCOM team is the world’s first all-optical high-speed switch for POF networks, a crucial step towards blisteringly fast optical data transmission. The technique, tested at the 520-nanometer wavelength (at which light appears green), involves using two beams of light from a single pulsed laser source in a special plastic optical fibre, the physical properties of which have been chemically modified, or doped, with photoactive polymers to change the way it transmits photons.

By overlapping the light pulses in space and time it is possible to use one light pulse to cancel out the other, thus switching it from on to off and transmitting a data signal. And because of the specific properties of the doped POF the cancellation of the light is reversed within only a few hundred femtoseconds (one femtosecond is one billionth of one millionth of a second).

“Not only will this increase data transmission rates in POF networks, but it could be used for time division multiplexing (TDM) to increase the bandwidth of optical networks beyond what is possible with current wavelength division multiplexing (WDM) techniques,” Lanzani says.

Whereas WDM uses light pulses of different colours to create different channels and therefore carry more data along a single fibre, TDM, as its name suggests, separates the pulses by time, allowing two or more signals to be carried as asynchronous sub-channels within a single fibre.

With bandwidth demands set to continue increasing, separating the signals at the transmission end and sorting them at the receiving end will require switching at rates that only an all-optical — as opposed to an optical-electronic solution — will be able to achieve.

The doped-POF used by the POLYCOM team for the all-optical switch is a polyfluorene called F8BT, one of several different materials studied by the group to test their optical properties. Several new types of doped POF were also developed by the researchers.

“In all, we developed and tested five or six new generations of materials, using different chemical agents to dope them in order to improve their optical properties and achieve very good dispersion of the doping agent in the polymer in several cases,” Lanzani says. “Each of the materials has different characteristics that may make them suitable for different applications.”

Glow in the dark clubbers?

An offshoot of the research was work on optofluidic channels in which the researchers exploited the optical properties of conjugated polymers in a fluid solution inside a microfluidic channel in order to produce a compact photonic device. Such a device could be used as the basis for a biochip for health applications in which optical sensors could be used to identify bacteria, viruses and even DNA strands in body fluids.

Though a commercial optofluidic device is probably some way off, Lanzani notes that the team’s research is likely to feed into a variety of commercial applications over the coming years, particularly as interest grows in the range of uses to which POF can be put.

“The auto industry will continue to demand faster and higher capacity POF networks as cars become more complex, while interest in using POF for LANs and telecommunications is continuing to grow,” Lanzani notes.

In addition, some research groups and companies are looking to use POF to create new sensing devices, relying on changes in the way the fibres carry light to measure liquid levels or humidity. And given its low cost and, with the right materials, dazzling luminescent properties, it is also being considered for safety clothing and probably even by clubbers looking to stand out in the crowd!

POLYCOM received funding from the FET Open strand of the EU’s Sixth Framework Programme for research.

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Researchers at the Kavli Institute for Nanosciences at Delft University of Technology, have succeeded in getting hold of the environment of a quantum particle. This allows them to exercise greater control over a single electron, and brings the team of researchers, led by Vidi winner and FOM workgroup leader Lieven Vandersypen, a step closer still to the super-fast quantum computer.

Their results were published in Nature Physics on 16 August.

One of the unique properties of quantum particles is that they can be in different states at the same time. An atom or electron is then in what is termed a ’superposition’ of two conditions. For instance, this means that the ’spin’ of an electron can be pointing in two different directions at once. A particle like this can therefore be 0 and 1 at the same time, and not just 0 or 1 as in an ordinary computer connection. This permits super-fast calculations. Until now, however, it has not proved possible to keep a particle in one specific state for any real length of time, because the environment — which also consists of quantum particles — is constantly disrupting the state. Researchers have been unable to get to grips with this until now.

Stabilising the pull and push

The researchers in Delft tackled the problem by stabilising the environment. They had already shown that it was possible to direct the spin of an electron using a quantum dot — a quantum scale box. The problem, however, is that the nuclei in the material of the box also have their own spins. Because spins operate like miniscule magnets, they pull and push the spin of the electron in the box. But that electron is also pushing and pulling in return.

The interaction between the spin of the electron and the spins of the surrounding nuclei was precisely what allowed the researchers to pin down the nuclear spins. They directed an electrical current through the nano-box and thus influenced the spin direction of the nuclei. The interaction between the spin of the electron and the nuclear spins in the environment finally allowed a situation to be created where the nuclear spins no longer varied at random, but actually became relatively stable. This stable environment now makes it possible to preserve the fragile but important superposition for a longer period.

The article by Ivo Vink, Lieven Vandersypen and collegues was published as an Advance Online Publication on the website of Nature Physics on 16 August 2009. A detailed theory about the mechanism behind these experimental observations was elaborated by PhD student Jeroen Danon and collegues, and published recently in the journal Physical Review Letters. The research was funded by NWO and the Foundation for Fundamental Research on Matter (FOM).

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Researchers at the Kavli Institute for Nanosciences at Delft University of Technology, have succeeded in getting hold of the environment of a quantum particle. This allows them to exercise greater control over a single electron, and brings the team of researchers, led by Vidi winner and FOM workgroup leader Lieven Vandersypen, a step closer still to the super-fast quantum computer.

Their results were published in Nature Physics on 16 August.

One of the unique properties of quantum particles is that they can be in different states at the same time. An atom or electron is then in what is termed a ’superposition’ of two conditions. For instance, this means that the ’spin’ of an electron can be pointing in two different directions at once. A particle like this can therefore be 0 and 1 at the same time, and not just 0 or 1 as in an ordinary computer connection. This permits super-fast calculations. Until now, however, it has not proved possible to keep a particle in one specific state for any real length of time, because the environment — which also consists of quantum particles — is constantly disrupting the state. Researchers have been unable to get to grips with this until now.

Stabilising the pull and push

The researchers in Delft tackled the problem by stabilising the environment. They had already shown that it was possible to direct the spin of an electron using a quantum dot — a quantum scale box. The problem, however, is that the nuclei in the material of the box also have their own spins. Because spins operate like miniscule magnets, they pull and push the spin of the electron in the box. But that electron is also pushing and pulling in return.

The interaction between the spin of the electron and the spins of the surrounding nuclei was precisely what allowed the researchers to pin down the nuclear spins. They directed an electrical current through the nano-box and thus influenced the spin direction of the nuclei. The interaction between the spin of the electron and the nuclear spins in the environment finally allowed a situation to be created where the nuclear spins no longer varied at random, but actually became relatively stable. This stable environment now makes it possible to preserve the fragile but important superposition for a longer period.

The article by Ivo Vink, Lieven Vandersypen and collegues was published as an Advance Online Publication on the website of Nature Physics on 16 August 2009. A detailed theory about the mechanism behind these experimental observations was elaborated by PhD student Jeroen Danon and collegues, and published recently in the journal Physical Review Letters. The research was funded by NWO and the Foundation for Fundamental Research on Matter (FOM).

Start uga_filter:

An international team of astronomers have found an unexpected link between mysterious ‘dark matter’ and the visible stars and gas in galaxies that could revolutionise our current understanding of gravity.


One of the astronomers, Dr Hongsheng Zhao of the SUPA Centre of Gravity, University of St. Andrews, suggests that an unknown force is acting on dark matter. The findings are published this week in the scientific journal Nature.

Only 4% of the universe is made of known material. Stars and gas in galaxies move so fast that astronomers have speculated that the gravity from a hypothetical invisible halo of dark matter is needed to keep galaxies together. However, a solid understanding of dark matter as well as direct evidence of its existence has remained elusive.

Now the team believes that the interactions between dark and ordinary matter could be more important and more complex than previously thought, and even speculate that dark matter might not exist and that the anomalous motions of stars in galaxies are due to a modification of gravity on extragalactic scales.

Dr. Benoit Famaey (Universities of Bonn and Strasbourg) explains: “The dark matter seems to ‘know’ how the visible matter is distributed. They seem to conspire with each other such that the gravity of the visible matter at the characteristic radius of the dark halo is always the same. This is extremely surprising since one would rather expect the balance between visible and dark matter to strongly depend on the individual history of each galaxy.”

Dr. Zhao at the SUPA Centre of Gravity notes, “The pattern that the data reveal is extremely odd. It’s like finding a zoo of animals of all ages and sizes miraculously having identical, say, weight in their backbones or something. It is possible that a non-gravitational fifth force is ruling the dark matter with an invisible hand, leaving the same fingerprints on all galaxies, irrespective of their ages, shapes and sizes.”

Such a force might solve an even bigger mystery, known as ‘dark energy’, which is ruling the accelerated expansion of the Universe. A more radical solution is a revision of the laws of gravity first developed by Isaac Newton in 1687 and refined by Albert Einstein’s theory of General Relativity in 1916. Einstein never fully decided whether his equation should add an omnipresent constant source, now called dark energy.

Dr Famaey added, “If we account for our observations with a modified law of gravity, it makes perfect sense to replace the effective action of hypothetical dark matter with a force closely related to the distribution of visible matter.”

The implications of the new research could change some of the most widely held scientific theories about the history and expansion of the universe.

Lead researcher Dr. Gianfranco Gentile at the University of Ghent concludes, “Understanding this puzzling conspiracy is probably the key to unlock the formation of galaxies and their structures.”

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An international team of astronomers have found an unexpected link between mysterious ‘dark matter’ and the visible stars and gas in galaxies that could revolutionise our current understanding of gravity.


One of the astronomers, Dr Hongsheng Zhao of the SUPA Centre of Gravity, University of St. Andrews, suggests that an unknown force is acting on dark matter. The findings are published this week in the scientific journal Nature.

Only 4% of the universe is made of known material. Stars and gas in galaxies move so fast that astronomers have speculated that the gravity from a hypothetical invisible halo of dark matter is needed to keep galaxies together. However, a solid understanding of dark matter as well as direct evidence of its existence has remained elusive.

Now the team believes that the interactions between dark and ordinary matter could be more important and more complex than previously thought, and even speculate that dark matter might not exist and that the anomalous motions of stars in galaxies are due to a modification of gravity on extragalactic scales.

Dr. Benoit Famaey (Universities of Bonn and Strasbourg) explains: “The dark matter seems to ‘know’ how the visible matter is distributed. They seem to conspire with each other such that the gravity of the visible matter at the characteristic radius of the dark halo is always the same. This is extremely surprising since one would rather expect the balance between visible and dark matter to strongly depend on the individual history of each galaxy.”

Dr. Zhao at the SUPA Centre of Gravity notes, “The pattern that the data reveal is extremely odd. It’s like finding a zoo of animals of all ages and sizes miraculously having identical, say, weight in their backbones or something. It is possible that a non-gravitational fifth force is ruling the dark matter with an invisible hand, leaving the same fingerprints on all galaxies, irrespective of their ages, shapes and sizes.”

Such a force might solve an even bigger mystery, known as ‘dark energy’, which is ruling the accelerated expansion of the Universe. A more radical solution is a revision of the laws of gravity first developed by Isaac Newton in 1687 and refined by Albert Einstein’s theory of General Relativity in 1916. Einstein never fully decided whether his equation should add an omnipresent constant source, now called dark energy.

Dr Famaey added, “If we account for our observations with a modified law of gravity, it makes perfect sense to replace the effective action of hypothetical dark matter with a force closely related to the distribution of visible matter.”

The implications of the new research could change some of the most widely held scientific theories about the history and expansion of the universe.

Lead researcher Dr. Gianfranco Gentile at the University of Ghent concludes, “Understanding this puzzling conspiracy is probably the key to unlock the formation of galaxies and their structures.”

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