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Fuel cells are often touted as one method to help decrease society’s addiction to fossil fuels. But there is still a lot of work to be done before fuel cells will be ready for mass market to be used in transportation, home heating and portable power for emergencies.

U of C chemists Jeff Hurd and George Shimizu have taken the science behind a specific type of fuel cell towards a higher level of design. They have discovered a new material that allows a PEM fuel cell, known as a polymer electrolyte membrane fuel cell, to work at a higher temperature. This discovery is extremely important in terms of increasing the efficiency and decreasing the cost of PEM fuel cells.

“This research will alter the way researchers have to this point perceived candidate materials for fuel cell applications,” says Shimizu a professor in the Department of Chemistry at the University of Calgary.

A research paper by Shimizu, Hurd, Ramanathan Vaidhyanathan and Venkataraman Thangadurai of the University of Calgary, and Christopher Ratcliffe and Igor Moudrakovski of the Steacie Institute for Molecular Sciences, National Research Council, has just been published in Nature Chemistry online. Shimizu filed a patent with the US patent office last year.

A fuel cell is an electrochemical energy conversion device which converts the chemicals hydrogen and oxygen into water and electrical energy. Water usually carries the ions (protons) in a hydrogen fuel cell but this research uses higher boiling molecules trapped in a molecular scaffolding.

Currently, PEM fuel cells can produce energy from hydrogen below 90 °C, just under the boiling point of water. With Shimizu’s material, energy can be produced at a higher temperature, up to 150 °C. This could ultimately make the fuel cell cheaper to produce because at a higher temperature less expensive metals can be used to convert hydrogen into energy. Currently, platinum is used which is extremely expensive. Also, reactions at a higher temperature would be faster thus increasing efficiency.

“Ours is an entirely new approach that strikes a balance between having a regular molecular structure and mobile components all while showing genuine promise of application,” says co-author Hurd, a PhD candidate studying chemistry at the U of C.

Kevin Colbow, director of research and development at Ballard Power Systems, a company that designs and manufactures clean energy hydrogen fuel cells, calls the work significant. “We believe that further improvement on conductivity and robustness of these materials could provide next generation membranes for PEM fuel cells.”

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Fuel cells are often touted as one method to help decrease society’s addiction to fossil fuels. But there is still a lot of work to be done before fuel cells will be ready for mass market to be used in transportation, home heating and portable power for emergencies.

U of C chemists Jeff Hurd and George Shimizu have taken the science behind a specific type of fuel cell towards a higher level of design. They have discovered a new material that allows a PEM fuel cell, known as a polymer electrolyte membrane fuel cell, to work at a higher temperature. This discovery is extremely important in terms of increasing the efficiency and decreasing the cost of PEM fuel cells.

“This research will alter the way researchers have to this point perceived candidate materials for fuel cell applications,” says Shimizu a professor in the Department of Chemistry at the University of Calgary.

A research paper by Shimizu, Hurd, Ramanathan Vaidhyanathan and Venkataraman Thangadurai of the University of Calgary, and Christopher Ratcliffe and Igor Moudrakovski of the Steacie Institute for Molecular Sciences, National Research Council, has just been published in Nature Chemistry online. Shimizu filed a patent with the US patent office last year.

A fuel cell is an electrochemical energy conversion device which converts the chemicals hydrogen and oxygen into water and electrical energy. Water usually carries the ions (protons) in a hydrogen fuel cell but this research uses higher boiling molecules trapped in a molecular scaffolding.

Currently, PEM fuel cells can produce energy from hydrogen below 90 °C, just under the boiling point of water. With Shimizu’s material, energy can be produced at a higher temperature, up to 150 °C. This could ultimately make the fuel cell cheaper to produce because at a higher temperature less expensive metals can be used to convert hydrogen into energy. Currently, platinum is used which is extremely expensive. Also, reactions at a higher temperature would be faster thus increasing efficiency.

“Ours is an entirely new approach that strikes a balance between having a regular molecular structure and mobile components all while showing genuine promise of application,” says co-author Hurd, a PhD candidate studying chemistry at the U of C.

Kevin Colbow, director of research and development at Ballard Power Systems, a company that designs and manufactures clean energy hydrogen fuel cells, calls the work significant. “We believe that further improvement on conductivity and robustness of these materials could provide next generation membranes for PEM fuel cells.”

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A magnetic charge can behave and interact just like an electric charge in some materials, according to new research led by the London Centre for Nanotechnology (LCN).

The magnetic equivalent of electricity in a spin ice material: atom sized north and south poles in spin ice drift in opposite directions when a magnetic field is applied.

The magnetic equivalent of electricity in a 'spin ice' material: atom sized north and south poles in spin ice drift in opposite directions when a magnetic field is applied.

The findings could lead to a reassessment of current magnetism theories, as well as significant technological advances.

The research, published in Nature, proves the existence of atom-sized ‘magnetic charges’ that behave and interact just like more familiar electric charges. It also demonstrates a perfect symmetry between electricity and magnetism – a phenomenon dubbed ‘magnetricity’ by the authors from the LCN and the Science and Technology Facility Council’s ISIS Neutron and Muon Source.

In order to prove experimentally the existence of magnetic current for the first time, the team mapped Onsager’s 1934 theory of the movement of ions in water onto magnetic currents in a material called spin ice. They then tested the theory by applying a magnetic field to a spin ice sample at a very low temperature and observing the process using muons at ISIS.

The experiment allowed the team to detect magnetic charges in the spin ice (Dy2Ti2O7), to measure their currents, and to determine the elementary unit of the magnetic charge in the material. The monopoles they observed arise as disturbances of the magnetic state of the spin ice, and can exist only inside the material.

Professor Steve Bramwell, LCN co-author of the paper, said: “Magnetic monopoles were first predicted to exist in 1931, but despite many searches, they have never yet been observed as freely roaming elementary particles. These monopoles do at least exist within the spin ice sample, but not outside.

“It is not often in the field of physics you get the chance to ask ‘How do you measure something?’ and then go on to prove a theory unequivocally. This is a very important step to establish that magnetic charge can flow like electric charge. It is in the early stages, but who knows what the applications of magnetricity could be in 100 years time.”

Professor Keith Mason, Chief Executive of STFC said: “The unequivocal proof that magnetic charge is conducted in spin ice adds significantly to our understanding of electromagnetism. Whilst we will have to wait to see what applications magnetricity will find in technology, this research shows that curiosity driven research will always have the potential to make an impact on the way we live and work. Advanced materials research depends greatly on having access to central research labs like ISIS allowing the UK science community to flourish and make exciting discoveries like this.”

Dr Sean Giblin, instrument scientist at ISIS and co-author of the paper, added: “The results were astounding, using muons at ISIS we are finally able to confirm that magnetic charge really is conducted through certain materials at certain temperatures – just like the way ions conduct electricity in water.”

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A magnetic charge can behave and interact just like an electric charge in some materials, according to new research led by the London Centre for Nanotechnology (LCN).

The magnetic equivalent of electricity in a spin ice material: atom sized north and south poles in spin ice drift in opposite directions when a magnetic field is applied.

The magnetic equivalent of electricity in a 'spin ice' material: atom sized north and south poles in spin ice drift in opposite directions when a magnetic field is applied.

The findings could lead to a reassessment of current magnetism theories, as well as significant technological advances.

The research, published in Nature, proves the existence of atom-sized ‘magnetic charges’ that behave and interact just like more familiar electric charges. It also demonstrates a perfect symmetry between electricity and magnetism – a phenomenon dubbed ‘magnetricity’ by the authors from the LCN and the Science and Technology Facility Council’s ISIS Neutron and Muon Source.

In order to prove experimentally the existence of magnetic current for the first time, the team mapped Onsager’s 1934 theory of the movement of ions in water onto magnetic currents in a material called spin ice. They then tested the theory by applying a magnetic field to a spin ice sample at a very low temperature and observing the process using muons at ISIS.

The experiment allowed the team to detect magnetic charges in the spin ice (Dy2Ti2O7), to measure their currents, and to determine the elementary unit of the magnetic charge in the material. The monopoles they observed arise as disturbances of the magnetic state of the spin ice, and can exist only inside the material.

Professor Steve Bramwell, LCN co-author of the paper, said: “Magnetic monopoles were first predicted to exist in 1931, but despite many searches, they have never yet been observed as freely roaming elementary particles. These monopoles do at least exist within the spin ice sample, but not outside.

“It is not often in the field of physics you get the chance to ask ‘How do you measure something?’ and then go on to prove a theory unequivocally. This is a very important step to establish that magnetic charge can flow like electric charge. It is in the early stages, but who knows what the applications of magnetricity could be in 100 years time.”

Professor Keith Mason, Chief Executive of STFC said: “The unequivocal proof that magnetic charge is conducted in spin ice adds significantly to our understanding of electromagnetism. Whilst we will have to wait to see what applications magnetricity will find in technology, this research shows that curiosity driven research will always have the potential to make an impact on the way we live and work. Advanced materials research depends greatly on having access to central research labs like ISIS allowing the UK science community to flourish and make exciting discoveries like this.”

Dr Sean Giblin, instrument scientist at ISIS and co-author of the paper, added: “The results were astounding, using muons at ISIS we are finally able to confirm that magnetic charge really is conducted through certain materials at certain temperatures – just like the way ions conduct electricity in water.”

Start uga_filter:

Rutgers researchers have discovered novel electronic properties in two-dimensional sheets of carbon atoms called graphene that could one day be the heart of speedy and powerful electronic devices.

Graphene sample with electrodes, fabricated using electron beam lithography

Graphene sample with electrodes, fabricated using electron beam lithography

The new findings, previously considered possible by physicists but only now being seen in the laboratory, show that electrons in graphene can interact strongly with each other. The behavior is similar to superconductivity observed in some metals and complex materials, marked by the flow of electric current with no resistance and other unusual but potentially useful properties. In graphene, this behavior results in a new liquid-like phase of matter consisting of fractionally charged quasi-particles, in which charge is transported with no dissipation.

In a paper issued online by the journal Nature and slated for print publication in the coming weeks, physics professor Eva Andrei and her Rutgers colleagues note that the strong interaction between electrons, also called correlated behavior, had not been observed in graphene in spite of many attempts to coax it out. This led some scientists to question whether correlated behavior could even be possible in graphene, where the electrons are massless (ultra-relativistic) particles like photons and neutrinos. In most materials, electrons are particles that have mass.

“Our work demonstrated that earlier failures to observe correlated behavior were not due to the physical nature of graphene,” said Eva Andrei, physics professor in the Rutgers School of Arts and Sciences. “Rather, it was because of interference from the material which supported graphene samples and the type of electrical probes used to study it.”

This finding should encourage scientists to further pursue graphene and related materials for future electronic applications, including replacements for today’s silicon-based semiconductor materials. Industry experts expect silicon technology to reach fundamental performance limits in a little more than a decade.

The Rutgers physicists further describe how they observed the collective behavior of the ultra-relativistic charge carriers in graphene through a phenomenon known as the fractional quantum Hall effect (FQHE). The FQHE is seen when charge carriers are confined to moving in a two-dimensional plane and are subject to a perpendicular magnetic field. When interactions between these charge carriers are sufficiently strong they form new quasi-particles with a fraction of an electron’s elementary charge. The FHQE is the quintessential signature of strongly correlated behavior among charge-carrying particles in two dimensions.

The FHQE is known to exist in semiconductor-based, two-dimensional electron systems, where the electrons are massive particles that obey conventional dynamics versus the relativistic dynamics of massless particles. However, it was not obvious until now that ultra-relativistic electrons in graphene would be capable of exhibiting collective phenomena that give rise to the FHQE. The Rutgers physicists were surprised that the FHQE in graphene is even more robust than in standard semiconductors.

Scientists make graphene patches by rubbing graphite – the same material in ordinary pencil lead – onto a silicon wafer, which is a thin slice of silicon crystal used to make computer chips. Then they run electrical pathways to the graphene patches using ordinary integrated circuit fabrication techniques. While scientists were able to investigate many properties of the resulting graphene electronic device, they were not able to induce the sought-after fractional quantum Hall effect.

Andrei and her group proposed that impurities or irregularities in the thin layer of silicon dioxide underlying the graphene were preventing the scientists from achieving the exacting conditions they needed. Postdoctoral fellow Xu Du and undergraduate student Anthony Barker were able to show that etching out several layers of silicon dioxide below the graphene patches essentially leaves an intact graphene strip suspended in mid-air by the electrodes. This enabled the group to demonstrate that the carriers in suspended graphene essentially propagate ballistically without scattering from impurities. Another crucial step was to design and fabricate a probe geometry that did not interfere with measurements as Andrei suspected earlier ones were doing. These proved decisive steps to observing the correlated behavior in graphene.

In the past few months, other academic and corporate research groups have reported streamlined graphene production techniques, which will propel further research and potential applications.

Andrei’s collaborators were Xu Du, now on faculty at Stony Brook University; Ivan Skachko, a post-doctoral fellow; Fabian Duerr, a master’s student; and Adina Luican, a doctoral student. The research was supported by the Department of Energy, the National Science Foundation, the Institute for Complex Adaptive Matter and Alcatel-Lucent.

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Rutgers researchers have discovered novel electronic properties in two-dimensional sheets of carbon atoms called graphene that could one day be the heart of speedy and powerful electronic devices.

Graphene sample with electrodes, fabricated using electron beam lithography

Graphene sample with electrodes, fabricated using electron beam lithography

The new findings, previously considered possible by physicists but only now being seen in the laboratory, show that electrons in graphene can interact strongly with each other. The behavior is similar to superconductivity observed in some metals and complex materials, marked by the flow of electric current with no resistance and other unusual but potentially useful properties. In graphene, this behavior results in a new liquid-like phase of matter consisting of fractionally charged quasi-particles, in which charge is transported with no dissipation.

In a paper issued online by the journal Nature and slated for print publication in the coming weeks, physics professor Eva Andrei and her Rutgers colleagues note that the strong interaction between electrons, also called correlated behavior, had not been observed in graphene in spite of many attempts to coax it out. This led some scientists to question whether correlated behavior could even be possible in graphene, where the electrons are massless (ultra-relativistic) particles like photons and neutrinos. In most materials, electrons are particles that have mass.

“Our work demonstrated that earlier failures to observe correlated behavior were not due to the physical nature of graphene,” said Eva Andrei, physics professor in the Rutgers School of Arts and Sciences. “Rather, it was because of interference from the material which supported graphene samples and the type of electrical probes used to study it.”

This finding should encourage scientists to further pursue graphene and related materials for future electronic applications, including replacements for today’s silicon-based semiconductor materials. Industry experts expect silicon technology to reach fundamental performance limits in a little more than a decade.

The Rutgers physicists further describe how they observed the collective behavior of the ultra-relativistic charge carriers in graphene through a phenomenon known as the fractional quantum Hall effect (FQHE). The FQHE is seen when charge carriers are confined to moving in a two-dimensional plane and are subject to a perpendicular magnetic field. When interactions between these charge carriers are sufficiently strong they form new quasi-particles with a fraction of an electron’s elementary charge. The FHQE is the quintessential signature of strongly correlated behavior among charge-carrying particles in two dimensions.

The FHQE is known to exist in semiconductor-based, two-dimensional electron systems, where the electrons are massive particles that obey conventional dynamics versus the relativistic dynamics of massless particles. However, it was not obvious until now that ultra-relativistic electrons in graphene would be capable of exhibiting collective phenomena that give rise to the FHQE. The Rutgers physicists were surprised that the FHQE in graphene is even more robust than in standard semiconductors.

Scientists make graphene patches by rubbing graphite – the same material in ordinary pencil lead – onto a silicon wafer, which is a thin slice of silicon crystal used to make computer chips. Then they run electrical pathways to the graphene patches using ordinary integrated circuit fabrication techniques. While scientists were able to investigate many properties of the resulting graphene electronic device, they were not able to induce the sought-after fractional quantum Hall effect.

Andrei and her group proposed that impurities or irregularities in the thin layer of silicon dioxide underlying the graphene were preventing the scientists from achieving the exacting conditions they needed. Postdoctoral fellow Xu Du and undergraduate student Anthony Barker were able to show that etching out several layers of silicon dioxide below the graphene patches essentially leaves an intact graphene strip suspended in mid-air by the electrodes. This enabled the group to demonstrate that the carriers in suspended graphene essentially propagate ballistically without scattering from impurities. Another crucial step was to design and fabricate a probe geometry that did not interfere with measurements as Andrei suspected earlier ones were doing. These proved decisive steps to observing the correlated behavior in graphene.

In the past few months, other academic and corporate research groups have reported streamlined graphene production techniques, which will propel further research and potential applications.

Andrei’s collaborators were Xu Du, now on faculty at Stony Brook University; Ivan Skachko, a post-doctoral fellow; Fabian Duerr, a master’s student; and Adina Luican, a doctoral student. The research was supported by the Department of Energy, the National Science Foundation, the Institute for Complex Adaptive Matter and Alcatel-Lucent.

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Could sustainable architecture address pollution, climate change and resource depletion by helping us build self-sufficient, off-grid, housing from “waste”, including vehicle tires and metal drinks containers? That’s the question researchers at the University of South Australia address in a new paper appearing in the International Journal of Sustainable Design.

Martin Freney of the department of Art, Architecture and Design has taken a critical look at the work of architect, Michael Reynolds of Taos, New Mexico, USA, who has experimented with radical house designs, and construction techniques over the past three and half decades. Reynolds designs incorporate passive heating and cooling, water catchment and sewage treatment, renewable energy, and even food production. These houses, which Reynolds calls “Earthships” are essentially independent of external utilities and waste disposal. On the face of it, they offer, an environmentally benign approach to housing.

A common method of responding to unsustainable housing is to design an energy-efficient home using “natural building” methods, Freney points out. He adds that Reynolds has already demonstrated that essentially free building materials resulted in greater financial independence for the owner-occupiers of his houses and when he added off-the-grid power and water systems he found that it was possible to reduce his utilities bills to practically zero.

Freney, while enthusiastic about the potential of Reynolds’ approach is also more realistic about the actual sustainability of Earthships that are off the utility grids. After all, he says, to a certain degree, Earthships are still locked into potentially unsustainable systems because they rely on a technological society for the production of the vehicle tires and aluminum can bricks from which they are constructed and the high-tech components such as solar panels, electronics, pumps, tanks, glass and cement that allow them to go off-grid.

Freney, however, has studied the approach in more detail and suggests that the design of the Earthship could allow precious resources to be used more efficiently, effectively and durably than is possible with conventional housing. They could, he argues, “provide shelter for many decades, possibly even centuries, regardless of what happens to the infrastructure that is essential to the operation of a typical home in the developed world.”

Further research is now needed to investigate thoroughly all aspects of sustainable architecture but the early indicators suggest that the Earthship model could be entirely viable “Earthship owners start to appreciate relief from financial stresses and from knowing that they have acted to address environmental problems,” concludes Freney.

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Could sustainable architecture address pollution, climate change and resource depletion by helping us build self-sufficient, off-grid, housing from “waste”, including vehicle tires and metal drinks containers? That’s the question researchers at the University of South Australia address in a new paper appearing in the International Journal of Sustainable Design.

Martin Freney of the department of Art, Architecture and Design has taken a critical look at the work of architect, Michael Reynolds of Taos, New Mexico, USA, who has experimented with radical house designs, and construction techniques over the past three and half decades. Reynolds designs incorporate passive heating and cooling, water catchment and sewage treatment, renewable energy, and even food production. These houses, which Reynolds calls “Earthships” are essentially independent of external utilities and waste disposal. On the face of it, they offer, an environmentally benign approach to housing.

A common method of responding to unsustainable housing is to design an energy-efficient home using “natural building” methods, Freney points out. He adds that Reynolds has already demonstrated that essentially free building materials resulted in greater financial independence for the owner-occupiers of his houses and when he added off-the-grid power and water systems he found that it was possible to reduce his utilities bills to practically zero.

Freney, while enthusiastic about the potential of Reynolds’ approach is also more realistic about the actual sustainability of Earthships that are off the utility grids. After all, he says, to a certain degree, Earthships are still locked into potentially unsustainable systems because they rely on a technological society for the production of the vehicle tires and aluminum can bricks from which they are constructed and the high-tech components such as solar panels, electronics, pumps, tanks, glass and cement that allow them to go off-grid.

Freney, however, has studied the approach in more detail and suggests that the design of the Earthship could allow precious resources to be used more efficiently, effectively and durably than is possible with conventional housing. They could, he argues, “provide shelter for many decades, possibly even centuries, regardless of what happens to the infrastructure that is essential to the operation of a typical home in the developed world.”

Further research is now needed to investigate thoroughly all aspects of sustainable architecture but the early indicators suggest that the Earthship model could be entirely viable “Earthship owners start to appreciate relief from financial stresses and from knowing that they have acted to address environmental problems,” concludes Freney.

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As manufacturers of consumer digital cameras compete in increments, adding one or two megapixels to their latest models, David Brady of Duke University is thinking much bigger. Working with the U.S. Department of Defense’s Defense Advanced Research Projects Agency, he is designing and building a camera that could achieve resolutions 1,000 or even 1 million times greater than the technology on the market today

The goal of reaching giga- or terapixels, says Brady, is currently being held back by the difficulty of designing a spherical lens that will not distort small areas of a scene. His idea is not only to modify the shape of the camera lens — making it aspherical — but to link together thousands of microcameras behind the main lens. Each of these cameras would have its own lens optimized for a small portion of the field of view.

“Now, when you use a camera, you’re looking through a narrow soda straw,” says Brady. “These new cameras will be able to capture the full view of human vision.”

The final result of the three-year project should be a device about the size of a breadbox, though Brady hopes to scale the technology down to create a single-lens reflex camera with a resolution of 50 gigapixels.

Reference: Paper CWB2, “Multiscale Optical Systems” is at 2 p.m. Wednesday, Oct. 14.

The latest technology in optics and lasers will be on display at the Optical Society’s (OSA) Annual Meeting, Frontiers in Optics (FiO), which takes place Oct. 11-15 at the Fairmont San Jose Hotel and the Sainte Claire Hotel in San Jose, Calif.


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As manufacturers of consumer digital cameras compete in increments, adding one or two megapixels to their latest models, David Brady of Duke University is thinking much bigger. Working with the U.S. Department of Defense’s Defense Advanced Research Projects Agency, he is designing and building a camera that could achieve resolutions 1,000 or even 1 million times greater than the technology on the market today

The goal of reaching giga- or terapixels, says Brady, is currently being held back by the difficulty of designing a spherical lens that will not distort small areas of a scene. His idea is not only to modify the shape of the camera lens — making it aspherical — but to link together thousands of microcameras behind the main lens. Each of these cameras would have its own lens optimized for a small portion of the field of view.

“Now, when you use a camera, you’re looking through a narrow soda straw,” says Brady. “These new cameras will be able to capture the full view of human vision.”

The final result of the three-year project should be a device about the size of a breadbox, though Brady hopes to scale the technology down to create a single-lens reflex camera with a resolution of 50 gigapixels.

Reference: Paper CWB2, “Multiscale Optical Systems” is at 2 p.m. Wednesday, Oct. 14.

The latest technology in optics and lasers will be on display at the Optical Society’s (OSA) Annual Meeting, Frontiers in Optics (FiO), which takes place Oct. 11-15 at the Fairmont San Jose Hotel and the Sainte Claire Hotel in San Jose, Calif.


Start uga_filter:

NASA’s Interstellar Boundary Explorer, or IBEX, spacecraft has made it possible for scientists to construct the first comprehensive sky map of our solar system and its location in the Milky Way galaxy. The new view will change the way researchers view and study the interaction between our galaxy and sun.

The Interstellar Boundary Explorer (IBEX) mission science team has used data from NASAs IBEX spacecraft to construct the first-ever all-sky map of the interactions occurring at the edge of the solar system, where the suns influence diminishes and interacts with the interstellar medium. Among the findings is an unexpectedly bright ribbon-like emission. (Credit: NASA/Goddard Space Flight Center Scientific Visualization Studio)

The Interstellar Boundary Explorer (IBEX) mission science team has used data from NASA's IBEX spacecraft to construct the first-ever all-sky map of the interactions occurring at the edge of the solar system, where the sun's influence diminishes and interacts with the interstellar medium. Among the findings is an unexpectedly bright ribbon-like emission. (Credit: NASA/Goddard Space Flight Center Scientific Visualization Studio)

The sky map was produced with data that two detectors on the spacecraft collected during six months of observations. The detectors measured and counted particles scientists refer to as energetic neutral atoms.

The energetic neutral atoms are created in an area of our solar system known as the interstellar boundary region. This region is where charged particles from the sun, called the solar wind, flow outward far beyond the orbits of the planets and collide with material between stars. The energetic neutral atoms travel inward toward the sun from interstellar space at velocities ranging from 100,000 mph to more than 2.4 million mph. This interstellar boundary emits no light that can be collected by conventional telescopes.

The new map reveals the region that separates the nearest reaches of our galaxy, called the local interstellar medium, from our heliosphere — a protective bubble that shields and protects our solar system from most of the dangerous cosmic radiation traveling through space.

“For the first time, we’re sticking our heads out of the sun’s atmosphere and beginning to really understand our place in the galaxy,” said David J. McComas, IBEX principal investigator and assistant vice president of the Space Science and Engineering Division at Southwest Research Institute in San Antonio. “The IBEX results are truly remarkable, with a narrow ribbon of bright details or emissions not resembling any of the current theoretical models of this region.”

NASA released the sky map image Oct. 15 in conjunction with publication of the findings in the journal Science. The IBEX data were complemented and extended by information collected using an imaging instrument sensor on NASA’s Cassini spacecraft. Cassini has been observing Saturn, its moons and rings since the spacecraft entered the planet’s orbit in 2004.

The IBEX sky maps also put observations from NASA’s Voyager spacecraft into context. The twin Voyager spacecraft, launched in 1977, traveled to the outer solar system to explore Jupiter, Saturn, Uranus and Neptune. In 2007, Voyager 2 followed Voyager 1 into the interstellar boundary. Both spacecraft are now in the midst of this region where the energetic neutral atoms originate. However, the IBEX results show a ribbon of bright emissions undetected by the two Voyagers.

“The Voyagers are providing ground truth, but they’re missing the most exciting region,” said Eric Christian, the IBEX deputy mission scientist at NASA’s Goddard Space Flight Center in Greenbelt, Md. “It’s like having two weather stations that miss the big storm that runs between them.”

The IBEX spacecraft was launched in October 2008. Its science objective was to discover the nature of the interactions between the solar wind and the interstellar medium at the edge of our solar system. The Southwest Research Institute developed and leads the mission with a team of national and international partners. The spacecraft is the latest in NASA’s series of low-cost, rapidly developed Small Explorers Program. NASA’s Goddard Space Flight Center manages the program for the agency’s Science Mission Directorate at NASA Headquarters in Washington.

The Cassini-Huygens mission is a cooperative project of NASA and the European and Italian Space Agencies. NASA’s Jet Propulsion Laboratory in Pasadena, Calif., provides overall management for Cassini and the Voyagers for the Science Mission Directorate.

To view the sky map and for more information about IBEX, visit: http://www.nasa.gov/ibex

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NASA’s Interstellar Boundary Explorer, or IBEX, spacecraft has made it possible for scientists to construct the first comprehensive sky map of our solar system and its location in the Milky Way galaxy. The new view will change the way researchers view and study the interaction between our galaxy and sun.

The Interstellar Boundary Explorer (IBEX) mission science team has used data from NASAs IBEX spacecraft to construct the first-ever all-sky map of the interactions occurring at the edge of the solar system, where the suns influence diminishes and interacts with the interstellar medium. Among the findings is an unexpectedly bright ribbon-like emission. (Credit: NASA/Goddard Space Flight Center Scientific Visualization Studio)

The Interstellar Boundary Explorer (IBEX) mission science team has used data from NASA's IBEX spacecraft to construct the first-ever all-sky map of the interactions occurring at the edge of the solar system, where the sun's influence diminishes and interacts with the interstellar medium. Among the findings is an unexpectedly bright ribbon-like emission. (Credit: NASA/Goddard Space Flight Center Scientific Visualization Studio)

The sky map was produced with data that two detectors on the spacecraft collected during six months of observations. The detectors measured and counted particles scientists refer to as energetic neutral atoms.

The energetic neutral atoms are created in an area of our solar system known as the interstellar boundary region. This region is where charged particles from the sun, called the solar wind, flow outward far beyond the orbits of the planets and collide with material between stars. The energetic neutral atoms travel inward toward the sun from interstellar space at velocities ranging from 100,000 mph to more than 2.4 million mph. This interstellar boundary emits no light that can be collected by conventional telescopes.

The new map reveals the region that separates the nearest reaches of our galaxy, called the local interstellar medium, from our heliosphere — a protective bubble that shields and protects our solar system from most of the dangerous cosmic radiation traveling through space.

“For the first time, we’re sticking our heads out of the sun’s atmosphere and beginning to really understand our place in the galaxy,” said David J. McComas, IBEX principal investigator and assistant vice president of the Space Science and Engineering Division at Southwest Research Institute in San Antonio. “The IBEX results are truly remarkable, with a narrow ribbon of bright details or emissions not resembling any of the current theoretical models of this region.”

NASA released the sky map image Oct. 15 in conjunction with publication of the findings in the journal Science. The IBEX data were complemented and extended by information collected using an imaging instrument sensor on NASA’s Cassini spacecraft. Cassini has been observing Saturn, its moons and rings since the spacecraft entered the planet’s orbit in 2004.

The IBEX sky maps also put observations from NASA’s Voyager spacecraft into context. The twin Voyager spacecraft, launched in 1977, traveled to the outer solar system to explore Jupiter, Saturn, Uranus and Neptune. In 2007, Voyager 2 followed Voyager 1 into the interstellar boundary. Both spacecraft are now in the midst of this region where the energetic neutral atoms originate. However, the IBEX results show a ribbon of bright emissions undetected by the two Voyagers.

“The Voyagers are providing ground truth, but they’re missing the most exciting region,” said Eric Christian, the IBEX deputy mission scientist at NASA’s Goddard Space Flight Center in Greenbelt, Md. “It’s like having two weather stations that miss the big storm that runs between them.”

The IBEX spacecraft was launched in October 2008. Its science objective was to discover the nature of the interactions between the solar wind and the interstellar medium at the edge of our solar system. The Southwest Research Institute developed and leads the mission with a team of national and international partners. The spacecraft is the latest in NASA’s series of low-cost, rapidly developed Small Explorers Program. NASA’s Goddard Space Flight Center manages the program for the agency’s Science Mission Directorate at NASA Headquarters in Washington.

The Cassini-Huygens mission is a cooperative project of NASA and the European and Italian Space Agencies. NASA’s Jet Propulsion Laboratory in Pasadena, Calif., provides overall management for Cassini and the Voyagers for the Science Mission Directorate.

To view the sky map and for more information about IBEX, visit: http://www.nasa.gov/ibex

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In the past 5 years, no material has excited more interest from condensed matter physicists than graphene, a sheet of carbon only one atom thick. Electrons zing through the stuff in an unusual way, and they flow so easily that graphene could someday replace silicon and other semiconductors as the material of choice for microchips. Now, a team of physicists has taken a key step in fulfilling graphene’s promise as a hotbed of exotic physics by showing that the electrons within it can team up to behave like particles with a fraction of the electron’s charge.

The effect is called the fractional quantum Hall effect, and it’s an esoteric embellishment of an already esoteric phenomenon known as the Hall effect. Discovered in 1879, the Hall effect works like this: Suppose you take a horizontal bar of metal and apply a voltage from one end to the other. A current will run down the length of the bar. If you then apply a strong vertical magnetic field, the flowing electrons will experience a sideways shove that will cause them to crowd to the side of the bar as they go so that a voltage develops across the width of the bar too. Sideways Hall voltage increases in proportion to the strength of the magnetic field.

Things get weirder if the bar is made of semiconductor and is extremely thin top to bottom. In that case, the electrons can flow in only a few quantum channels that close one by one as the magnetic field increases. The Hall voltage climbs as the magnetic field increases in a series of even steps whose spacing is set by the electron’s charge. The discovery of that quantum Hall effect won the Nobel Prize in physics in 1985. Weirder still, if the slab of semiconductor is made very pure and cold, then the electrons can gang up to act like “quasiparticles” with fractional charges–say, 1/3 of an electron’s charge–adding more steps to the Hall-voltage stairway. That’s the fractional quantum Hall effect, which bagged a Nobel in 1988.

The fractional effect is a sign of very strong interactions among the electrons, a condition that can lead to a variety of surprising phenomena and which marks the conceptual frontier in condensed matter physics. Many physicists had hoped to see the fractional effect in graphene as proof that it would be an especially fruitful material to study. But they couldn’t be entirely sure it would appear. Because of the arrangement of the atoms in graphene, the electrons zip through less like ordinary massive particles that can stop and start and more like massless and always-moving particles of light. Nobody was sure such “relativistic” electrons would interact strongly enough to produce the effect, though several groups had looked for it. “It was the biggest disappointment in this really hot field, that it hadn’t been seen,” says Eva Andrei of Rutgers University in Piscataway, New Jersey.

Fret no more, physicists. Andrei and her team have finally spotted electrons in graphene getting together in the right way. To do it, the team suspended micrometer-sized bits of graphene to avoid interference from the underlying substrate. The researchers then used a special arrangement of electrodes to keep from shorting out their own measurements, they report online this week in Nature. They observed quasiparticles with 1/3 an electron’s charge. In fact, Andrei says, the researchers saw the effect at higher temperatures and lower magnetic fields than are needed to see it in semiconductors, suggesting that the electrons in graphene interact especially strongly.

“It’s absolutely convincing,” says physicist Kostya Novoselov of the University of Manchester, U.K. “It definitely proves it’s reasonable to study electron-electron interactions in graphene.” Andrei says now that physicists have spotted this effect, they may see electrons in graphene joining together in completely new and even weirder ways. And if researchers can produce quasiparticles with charge 5/2, then in principle they could make a type of quantum computer that would work by braiding the particles’ paths together.

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In the past 5 years, no material has excited more interest from condensed matter physicists than graphene, a sheet of carbon only one atom thick. Electrons zing through the stuff in an unusual way, and they flow so easily that graphene could someday replace silicon and other semiconductors as the material of choice for microchips. Now, a team of physicists has taken a key step in fulfilling graphene’s promise as a hotbed of exotic physics by showing that the electrons within it can team up to behave like particles with a fraction of the electron’s charge.

The effect is called the fractional quantum Hall effect, and it’s an esoteric embellishment of an already esoteric phenomenon known as the Hall effect. Discovered in 1879, the Hall effect works like this: Suppose you take a horizontal bar of metal and apply a voltage from one end to the other. A current will run down the length of the bar. If you then apply a strong vertical magnetic field, the flowing electrons will experience a sideways shove that will cause them to crowd to the side of the bar as they go so that a voltage develops across the width of the bar too. Sideways Hall voltage increases in proportion to the strength of the magnetic field.

Things get weirder if the bar is made of semiconductor and is extremely thin top to bottom. In that case, the electrons can flow in only a few quantum channels that close one by one as the magnetic field increases. The Hall voltage climbs as the magnetic field increases in a series of even steps whose spacing is set by the electron’s charge. The discovery of that quantum Hall effect won the Nobel Prize in physics in 1985. Weirder still, if the slab of semiconductor is made very pure and cold, then the electrons can gang up to act like “quasiparticles” with fractional charges–say, 1/3 of an electron’s charge–adding more steps to the Hall-voltage stairway. That’s the fractional quantum Hall effect, which bagged a Nobel in 1988.

The fractional effect is a sign of very strong interactions among the electrons, a condition that can lead to a variety of surprising phenomena and which marks the conceptual frontier in condensed matter physics. Many physicists had hoped to see the fractional effect in graphene as proof that it would be an especially fruitful material to study. But they couldn’t be entirely sure it would appear. Because of the arrangement of the atoms in graphene, the electrons zip through less like ordinary massive particles that can stop and start and more like massless and always-moving particles of light. Nobody was sure such “relativistic” electrons would interact strongly enough to produce the effect, though several groups had looked for it. “It was the biggest disappointment in this really hot field, that it hadn’t been seen,” says Eva Andrei of Rutgers University in Piscataway, New Jersey.

Fret no more, physicists. Andrei and her team have finally spotted electrons in graphene getting together in the right way. To do it, the team suspended micrometer-sized bits of graphene to avoid interference from the underlying substrate. The researchers then used a special arrangement of electrodes to keep from shorting out their own measurements, they report online this week in Nature. They observed quasiparticles with 1/3 an electron’s charge. In fact, Andrei says, the researchers saw the effect at higher temperatures and lower magnetic fields than are needed to see it in semiconductors, suggesting that the electrons in graphene interact especially strongly.

“It’s absolutely convincing,” says physicist Kostya Novoselov of the University of Manchester, U.K. “It definitely proves it’s reasonable to study electron-electron interactions in graphene.” Andrei says now that physicists have spotted this effect, they may see electrons in graphene joining together in completely new and even weirder ways. And if researchers can produce quasiparticles with charge 5/2, then in principle they could make a type of quantum computer that would work by braiding the particles’ paths together.

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The National Institute for Computational Sciences’ (NICS’s) Cray XT5 supercomputer—Kraken—has been upgraded to become the first academic system to surpass a thousand trillion calculations a second, or one petaflop, a landmark achievement that will greatly accelerate science and place Kraken among the top five computers in the world.


Managed by the University of Tennessee (UT) for the National Science Foundation (NSF), the system came online Oct. 5 with a peak performance of 1.03 petaflops. It features more than 16,000 six-core 2.6-GHz AMD Istanbul processors with nearly 100,000 compute cores.

In addition, an upgrade to 129 terabytes of memory (the equivalent of more than 13 thousand movies on DVD) effectively doubles the size of Kraken for researchers running some of the world’s most sophisticated 3-D scientific computing applications. Simulation has become a key tool for researchers in a number of fields, from climate change to materials.

“At over a petaflop of peak computing power, and the ability to routinely run full machine jobs, Kraken will dominate large-scale NSF computing in the near future,” said NICS Project Director Phil Andrews. “Its unprecedented computational capability and total available memory will allow academic users to treat problems that were previously inaccessible.”

For example, understanding the mechanism behind the explosion of core-collapse supernovas will reveal much about our universe (these cataclysmic events are responsible for more than half the elements in the universe). Essentially three phenomena are being simulated to explore these explosions: hydrodynamics, nuclear burning or fusion, and neutrino transport, said UT astrophysicist Bronson Messer.

At the terascale, or trillions of calculations per second, Messer and his team were forced to simulate the star in 1-D as a perfect sphere and with unrealistic fusion physics. “Now, however, we are getting closer to physical reality,” said Messer. “With petascale capability, we can simulate all three phenomena simultaneously with significant realism. This brings us closer to understanding the explosion mechanism and being able to make meaningful predictions.”

From the physical makeup of the universe to the causes of global warming to the roles of proteins in disease, Kraken’s increased computing muscle will reach far and wide.

As the main computational resource for NICS, the new system is linked to the NSF-supported TeraGrid, a network of supercomputers across the country that is the world’s largest computational platform for open scientific research.

The system and the resulting NICS organization are the result of an NSF Track 2 award of $65 million to the University of Tennessee and its partners to provide for next-generation high-performance computing (HPC). The award was won in an open competition among HPC institutions vying to guarantee America’s continued competitiveness through the next generation of supercomputers (systems greater than 10 teraflops and into the petascale).

“While reaching the petascale is a remarkable achievement in itself, the real strides will be made in the new science that petascale computing will enable,” said Thomas Zacharia, NICS principal investigator, professor in electrical and computer engineering at the University of Tennessee and deputy director for science and technology at Oak Ridge National Laboratory. “Kraken is a game changer for research.”

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The National Institute for Computational Sciences’ (NICS’s) Cray XT5 supercomputer—Kraken—has been upgraded to become the first academic system to surpass a thousand trillion calculations a second, or one petaflop, a landmark achievement that will greatly accelerate science and place Kraken among the top five computers in the world.


Managed by the University of Tennessee (UT) for the National Science Foundation (NSF), the system came online Oct. 5 with a peak performance of 1.03 petaflops. It features more than 16,000 six-core 2.6-GHz AMD Istanbul processors with nearly 100,000 compute cores.

In addition, an upgrade to 129 terabytes of memory (the equivalent of more than 13 thousand movies on DVD) effectively doubles the size of Kraken for researchers running some of the world’s most sophisticated 3-D scientific computing applications. Simulation has become a key tool for researchers in a number of fields, from climate change to materials.

“At over a petaflop of peak computing power, and the ability to routinely run full machine jobs, Kraken will dominate large-scale NSF computing in the near future,” said NICS Project Director Phil Andrews. “Its unprecedented computational capability and total available memory will allow academic users to treat problems that were previously inaccessible.”

For example, understanding the mechanism behind the explosion of core-collapse supernovas will reveal much about our universe (these cataclysmic events are responsible for more than half the elements in the universe). Essentially three phenomena are being simulated to explore these explosions: hydrodynamics, nuclear burning or fusion, and neutrino transport, said UT astrophysicist Bronson Messer.

At the terascale, or trillions of calculations per second, Messer and his team were forced to simulate the star in 1-D as a perfect sphere and with unrealistic fusion physics. “Now, however, we are getting closer to physical reality,” said Messer. “With petascale capability, we can simulate all three phenomena simultaneously with significant realism. This brings us closer to understanding the explosion mechanism and being able to make meaningful predictions.”

From the physical makeup of the universe to the causes of global warming to the roles of proteins in disease, Kraken’s increased computing muscle will reach far and wide.

As the main computational resource for NICS, the new system is linked to the NSF-supported TeraGrid, a network of supercomputers across the country that is the world’s largest computational platform for open scientific research.

The system and the resulting NICS organization are the result of an NSF Track 2 award of $65 million to the University of Tennessee and its partners to provide for next-generation high-performance computing (HPC). The award was won in an open competition among HPC institutions vying to guarantee America’s continued competitiveness through the next generation of supercomputers (systems greater than 10 teraflops and into the petascale).

“While reaching the petascale is a remarkable achievement in itself, the real strides will be made in the new science that petascale computing will enable,” said Thomas Zacharia, NICS principal investigator, professor in electrical and computer engineering at the University of Tennessee and deputy director for science and technology at Oak Ridge National Laboratory. “Kraken is a game changer for research.”

Start uga_filter:

Solar Roads are the future power houses of the world. We all know that there are many million miles of roads built in the world, what if all those roads were able to harness sun’s energy?

Well, considering the massive network of roads and highways, a huge amount of power would be generated even if solar panels with just 15% efficiency are used. These roads could also have embedded LED lights in them which can provide navigation to the travelers and tell them about any road blockages due to accidents etc. These roads would also be able to re-route the entire traffic.

US Department of Energy recognized the huge potential in this concept and gave a $100,000 contract to a company named “Solar Roadways”. The firm will build a prototype 12 x 12 feet solar panel which could be fixed into roads.

If this experiment turns out to be successful then who knows one day we forget about Nuclear or any other energy and just rely on Solar Roads because they have a huge potential.

See the video below for some detailed information.

httpv://www.youtube.com/watch?v=J3PeSm6_hTE

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Solar Roads are the future power houses of the world. We all know that there are many million miles of roads built in the world, what if all those roads were able to harness sun’s energy?

Well, considering the massive network of roads and highways, a huge amount of power would be generated even if solar panels with just 15% efficiency are used. These roads could also have embedded LED lights in them which can provide navigation to the travelers and tell them about any road blockages due to accidents etc. These roads would also be able to re-route the entire traffic.

US Department of Energy recognized the huge potential in this concept and gave a $100,000 contract to a company named “Solar Roadways”. The firm will build a prototype 12 x 12 feet solar panel which could be fixed into roads.

If this experiment turns out to be successful then who knows one day we forget about Nuclear or any other energy and just rely on Solar Roads because they have a huge potential.

See the video below for some detailed information.

httpv://www.youtube.com/watch?v=J3PeSm6_hTE

Start uga_filter:

Biomolecular computers, made of DNA and other biological molecules, only exist today in a few specialized labs, remote from the regular computer user. Nonetheless, Tom Ran and Shai Kaplan, research students in the lab of Prof. Ehud Shapiro of the Weizmann Institute’s Biological Chemistry, and Computer Science and Applied Mathematics Departments have found a way to make these microscopic computing devices ‘user friendly,’ even while performing complex computations and answering complicated queries.

Shapiro and his team at Weizmann introduced the first autonomous programmable DNA computing device in 2001. So small that a trillion fit in a drop of water, that device was able to perform such simple calculations as checking a list of 0s and 1s to determine if there was an even number of 1s. A newer version of the device, created in 2004, detected cancer in a test tube and released a molecule to destroy it. Besides the tantalizing possibility that such biology-based devices could one day be injected into the body – a sort of ‘doctor in a cell’ locating disease and preventing its spread – biomolecular computers could conceivably perform millions of calculations in parallel.

Now, Shapiro and his team, in a paper published online August 3 in Nature Nanotechnology, have devised an advanced program for biomolecular computers that enables them to ‘think’ logically.

The train of deduction used by this futuristic device is remarkably familiar. It was first proposed by Aristotle over 2000 years ago as a simple if…then proposition: ‘All men are mortal. Socrates is a man. Therefore, Socrates is mortal.’ When fed a rule (All men are mortal) and a fact (Socrates is a man), the computer answered the question ‘Is Socrates Mortal?’ correctly. The team went on to set up more complicated queries involving multiple rules and facts, and the DNA computing devices were able to deduce the correct answers every time. At the same time, the team created a compiler – a program for bridging between a high-level computer programming language and DNA computing code. Upon compiling, the query could be typed in something like this: Mortal(Socrates)?. To compute the answer, various strands of  DNA representing the rules, facts and queries were assembled by a robotic system and searched for a fit in a hierarchical process. The answer was encoded in a flash of green light: Some of the strands had a biological version of a flashlight signal – they were equipped with a naturally glowing fluorescent molecule bound to a second protein which keeps the light covered. A specialized enzyme, attracted to the site of the correct answer, removed the ‘cover’ and let the light shine. The tiny water drops containing the biomolecular data-bases were able to answer very intricate queries, and they lit up in a combination of colors representing the complex answers.

Prof. Ehud Shapiro’s research is supported by the Clore Center for Biological Physics; the Arie and Ida Crown Memorial Charitable Fund; the Phyllis and Joseph Gurwin Fund for Scientific Advancement; Sally Leafman Appelbaum, Scottsdale, AZ; the Carolito Stiftung, Switzerland; the Louis Chor Memorial Trust Fund; and Miel de Botton Aynsley, UK. Prof. Shapiro is the incumbent of the Harry Weinrebe Chair of Computer Science and Biology.

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Biomolecular computers, made of DNA and other biological molecules, only exist today in a few specialized labs, remote from the regular computer user. Nonetheless, Tom Ran and Shai Kaplan, research students in the lab of Prof. Ehud Shapiro of the Weizmann Institute’s Biological Chemistry, and Computer Science and Applied Mathematics Departments have found a way to make these microscopic computing devices ‘user friendly,’ even while performing complex computations and answering complicated queries.

Shapiro and his team at Weizmann introduced the first autonomous programmable DNA computing device in 2001. So small that a trillion fit in a drop of water, that device was able to perform such simple calculations as checking a list of 0s and 1s to determine if there was an even number of 1s. A newer version of the device, created in 2004, detected cancer in a test tube and released a molecule to destroy it. Besides the tantalizing possibility that such biology-based devices could one day be injected into the body – a sort of ‘doctor in a cell’ locating disease and preventing its spread – biomolecular computers could conceivably perform millions of calculations in parallel.

Now, Shapiro and his team, in a paper published online August 3 in Nature Nanotechnology, have devised an advanced program for biomolecular computers that enables them to ‘think’ logically.

The train of deduction used by this futuristic device is remarkably familiar. It was first proposed by Aristotle over 2000 years ago as a simple if…then proposition: ‘All men are mortal. Socrates is a man. Therefore, Socrates is mortal.’ When fed a rule (All men are mortal) and a fact (Socrates is a man), the computer answered the question ‘Is Socrates Mortal?’ correctly. The team went on to set up more complicated queries involving multiple rules and facts, and the DNA computing devices were able to deduce the correct answers every time. At the same time, the team created a compiler – a program for bridging between a high-level computer programming language and DNA computing code. Upon compiling, the query could be typed in something like this: Mortal(Socrates)?. To compute the answer, various strands of  DNA representing the rules, facts and queries were assembled by a robotic system and searched for a fit in a hierarchical process. The answer was encoded in a flash of green light: Some of the strands had a biological version of a flashlight signal – they were equipped with a naturally glowing fluorescent molecule bound to a second protein which keeps the light covered. A specialized enzyme, attracted to the site of the correct answer, removed the ‘cover’ and let the light shine. The tiny water drops containing the biomolecular data-bases were able to answer very intricate queries, and they lit up in a combination of colors representing the complex answers.

Prof. Ehud Shapiro’s research is supported by the Clore Center for Biological Physics; the Arie and Ida Crown Memorial Charitable Fund; the Phyllis and Joseph Gurwin Fund for Scientific Advancement; Sally Leafman Appelbaum, Scottsdale, AZ; the Carolito Stiftung, Switzerland; the Louis Chor Memorial Trust Fund; and Miel de Botton Aynsley, UK. Prof. Shapiro is the incumbent of the Harry Weinrebe Chair of Computer Science and Biology.

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