Friday 22 May 2015

Ants color vision may help march towards robot technology

Scientia — Researchers at The University of Western Australia have discovered how ants see in colour, a breakthrough that one day could help scientists create more autonomous robots.


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In a paper published today in Proceedings of the Royal Society B, researchers Dr Yuri Ogawa and Dr Jan Hemmi from UWA’s School of Animal Biology show for the first time that the Australian bull ants (like humans) have three types of photoreceptors that are sensitive to different colours (UV, Blue and Green) and therefore the potential for trichromatic colour vision.


Photoreceptors are the cells in the eye that are sensitive to light. This means that their colour vision is likely to be as good as that of humans and old world primates and significantly better than that of other mammals such as dogs, cats or wallabies.






Most mammals have only two types of photoreceptors they can use for colour vision, leading to poorer colour perception. However, in contrast to humans, the bull ants can also see UV light, which means they can see different colours than we do.


In addition, one of the two species investigated is completely nocturnal, so they only forage at night after dusk. That means they use their three different photoreceptors types at night, during light levels where humans are completely colour blind.


Dr Hemmi believes the driving force behind the sophistication of their colour vision is their need to navigate to and from their nest.


“In contrast to many other ant species, bull ants forage individually, do not lay pheromone trails like other ant species and use only vision to navigate,’ he said.


“The poor resolution of these ants means they see the world through an eye with only 2-3000 pixels and that must make it very difficult to accurately identify landmarks. Having accurate colour vision could therefore help with landmark identification. It is quite possible that navigation has played a major role in the early evolution of colour vision.”


The wider context of the research is to find out how animals see their world. With ants, the most interesting question is how miniaturisation affects their sensory systems and the researchers would like to know what strategies ants use to overcome miniaturisation effects such as small eyes and very limited processing power (small brains). The interest in miniaturisation comes from both biology and robotics.




Finding how animals navigate and see their world with very limited resources and how they use these resources to best effect could, in the long run, help scientists design more autonomous and effective robots and vehicles.



For loads more information about ants, and in particular the Bull dog ant, visit here







– Credit and Resource –


More information: Three spectrally distinct photoreceptors in diurnal and nocturnal Australian ants, rspb.royalsocietypublishing.org/lookup/doi/10.1098/rspb.2015.0673


Journal reference: Proceedings of the Royal Society B


Provided by University of Western Australia



Ants color vision may help march towards robot technology

WISE spacecraft discovers most luminous galaxy in universe

Scientia — A remote galaxy shining with the light of more than 300 trillion suns has been discovered using data from NASA’s Wide-field Infrared Survey Explorer (WISE). The galaxy is the most luminous galaxy found to date and belongs to a new class of objects recently discovered by WISE—extremely luminous infrared galaxies, or ELIRGs.


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This artist’s concept depicts the current record holder for the most luminous galaxy in the universe. The galaxy, named WISE J224607.57-052635.0, is erupting with light equal to more than 300 trillion suns. It was discovered by NASA’s Wide-Field Infrared Survey Explorer, or WISE. The galaxy is smaller than the Milky Way, yet puts out 10,000 times more energy. Scientists think that a supermassive black hole at the center of this dusty galaxy is busily consuming gaseous material in a colossal growth spurt. As the gas is dragged toward the black hole, it heats up and blasts out visible, ultraviolet and X-ray light. The dust swaddling the galaxy absorbs this light and heats up, radiating longer-wavelength, infrared light. The dust also blocks our view of shorter, visible-light wavelengths, while letting longer-wavelengths through. This is similar to what happens when sunlight streams through our dusty atmosphere, producing a brilliant red sunrise. In fact, more than 99 percent of the light escaping from this dusty galaxy is infrared. As a result, it is much harder to see with optical telescopes. Because light from the galaxy hosting the black hole has traveled 12.5 billion years to reach us, astronomers are seeing the object as it was in the distant past. During this epoch, galaxies would have been more than five times closer together than they are now, as illustrated in the background of the artist’s concept. This is due to the expansion of space — space itself and the galaxies in it are stretching apart from each other at ever-increasing speeds. Credit: NASA


“We are looking at a very intense phase of galaxy evolution,” said Chao-Wei Tsai of NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California, lead author of a new report appearing in the May 22 issue of The Astrophysical Journal. “This dazzling light may be from the main growth spurt of the galaxy’s black hole.”






The brilliant galaxy, known as WISE J224607.57-052635.0, may have a behemoth black hole at its belly, gorging itself on gas. Supermassive black holes draw gas and matter into a disk around them, heating the disk to roaring temperatures of millions of degrees and blasting out high-energy, visible, ultraviolet, and X-ray light. The light is blocked by surrounding cocoons of dust. As the dust heats up, it radiates infrared light.


Immense black holes are common at the cores of galaxies, but finding one this big so “far back” in the cosmos is rare. Because light from the galaxy hosting the black hole has traveled 12.5 billion years to reach us, astronomers are seeing the object as it was in the distant past. The black hole was already billions of times the mass of our sun when our universe was only a tenth of its present age of 13.8 billion years.


The new study outlines three reasons why the black holes in the ELIRGs could have grown so massive. First, they may have been born big. In other words, the “seeds,” or embryonic black holes, might be bigger than thought possible.


“How do you get an elephant?” asked Peter Eisenhardt, project scientist for WISE at JPL and a co-author on the paper. “One way is start with a baby elephant.”


The other two explanations involve either breaking or bending the theoretical limit of black hole feeding, called the Eddington limit. When a black hole feeds, gas falls in and heats up, blasting out light. The pressure of the light actually pushes the gas away, creating a limit to how fast the black hole can continuously scarf down matter. If a black hole broke this limit, it could theoretically balloon in size at a breakneck pace. Black holes have previously been observed breaking this limit; however, the black hole in the study would have had to repeatedly break the limit to grow this large.


Alternatively, the black holes might just be bending this limit.


“Another way for a black hole to grow this big is for it to have gone on a sustained binge, consuming food faster than typically thought possible,” said Tsai. “This can happen if the black hole isn’t spinning that fast.”


If a black hole spins slowly enough, it won’t repel its meal as much. In the end, a slow-spinning black hole can gobble up more matter than a fast spinner.


“The massive black holes in ELIRGs could be gorging themselves on more matter for a longer period of time,” said Andrew Blain of University of Leicester in the United Kingdom, a co-author of this report. “It’s like winning a hot-dog-eating contest lasting hundreds of millions of years.”


More research is needed to solve this puzzle of these dazzlingly luminous galaxies. The team has plans to better determine the masses of the central black holes. Knowing these objects’ true hefts will help reveal their history, as well as that of other galaxies, in this very crucial and frenzied chapter of our cosmos.




WISE has been finding more of these oddball galaxies in infrared images of the entire sky captured in 2010. By viewing the whole sky with more sensitivity than ever before, WISE has been able to catch rare cosmic specimens that might have been missed otherwise.


The new study reports a total of 20 new ELIRGs, including the most luminous galaxy found to date. These galaxies were not found earlier because of their distance, and because dust converts their powerful visible light into an incredible outpouring of infrared light.


“We found in a related study with WISE that as many as half of the most luminous galaxies only show up well in infrared light,” said Tsai.


JPL manages and operates WISE for NASA’s Science Mission Directorate in Washington. The spacecraft was put into hibernation mode in 2011, after it scanned the entire sky twice, thereby completing its main objectives. In September 2013, WISE was reactivated, renamed NEOWISE and assigned a new mission to assist NASA’s efforts to identify potentially hazardous near-Earth objects.






– Credit and Resource –


More information: On Arxiv: arxiv.org/abs/1410.1751


Journal reference: arXiv search and more info & Astrophysical Journal


Provided by NASA’s Goddard Space Flight Center



WISE spacecraft discovers most luminous galaxy in universe

Thursday 21 May 2015

World's largest particle collider busts record

Scientia — The world’s largest particle smasher broke the record for energy levels late Wednesday in a test run after a two-year upgrade, CERN announced Thursday. “Last night, protons collided in the Large Hadron Collider (LHC) at the record-breaking energy of 13 TeV (teraelectronvolts) for the first time,” the European Organisation for Nuclear Research (CERN) said in a statement.


The LHC’s previous highest energy for collisions was eight TeV, reached in 2012. In April, it started up again after a two-year overhaul designed to pave the way to experiments at 13 TeV. It has the potential to be cranked up to 14 TeV.


Experiments at the collider are aimed at unlocking clues as to how the universe came into existence by studying fundamental particles, the building blocks of all matter, and the forces that control them. Before the upgrade, the LHC was used to prove the existence of the Higgs Boson, also known as the God particle, which confers mass.






That discovery earned the 2013 Nobel physics prize for two of the scientists who had theorised the existence of the Higgs back in 1964. Wednesday’s collisions at the giant lab, housed in a 27-kilometre (17-mile) tunnel straddling the French-Swiss border, are part of a recommissioning programme ahead of an even more ambitious roster of experiments, due to start next month.


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Presentation of the Large Hadron Collider


“These test collisions were to set up systems that protect the machine and detectors from particles that stray from the edges of the beam,” CERN said. The LHC allows beams containing billions of protons travelling at 99.9 percent the speed of light to shoot through the massive collider in opposite directions. Powerful magnets bend the beams so that they collide at points around the track where four laboratories have batteries of sensors to monitor the smashups.


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Workers check equipment at CERN in February, 2015


The sub-atomic rubble is then scrutinised for novel particles and the forces that hold them together. One teraelectronvolt is roughly equivalent to the energy of motion of a flying mosquito, CERN says on its website. But within the LHC, the energy is squeezed into an extremely small space—about a million, million times smaller than a mosquito. It is this intensity which causes the particles to be smashed apart.




First images of collisions at 13 TeV

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Test collisions continue today at 13 TeV in the Large Hadron Collider (LHC) to prepare the detectors ALICE, ATLAS, CMS, LHCb, LHCf, MOEDAL and TOTEM for data-taking, planned for early June (Image: LHC page 1)


Last night, protons collided in the Large Hadron Collider (LHC) at the record-breaking energy of 13 TeV for the first time. These test collisions were to set up systems that protect the machine and detectors from particles that stray from the edges of the beam.


A key part of the process was the set-up of the collimators. These devices which absorb stray particles were adjusted in colliding-beam conditions. This set-up will give the accelerator team the data they need to ensure that the LHC magnets and detectors are fully protected.


Today the tests continue. Colliding beams will stay in the LHC for several hours. The LHC Operations team will continue to monitor beam quality and optimisation of the set-up.


This is an important part of the process that will allow the experimental teams running the detectors ALICE, ATLAS, CMS, LHCb, LHCf, MOEDAL and TOTEM to switch on their experiments fully. Data taking and the start of the LHC’s second run is planned for early June.


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Protons collide at 13 TeV sending showers of particles through the ALICE detector (Image: ALICE)


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Protons collide at 13 TeV sending showers of particles through the CMS detector (Image: CMS)


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Protons collide at 13 TeV sending showers of particles through the ATLAS detector (Image: ATLAS)






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Protons collide at 13 TeV sending showers of particles through the LHCb detector (Image: LHCb)


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Protons collide at 13 TeV sending showers of particles through the TOTEM detector (Image: TOTEM)






– Credit and Resource –


CERN



World's largest particle collider busts record

Why you need one vaccine for measles and many for the flu

Scientia — While the influenza virus mutates constantly and requires a yearly shot that offers a certain percentage of protection, old reliable measles needs only a two-dose vaccine during childhood for lifelong immunity. A new study publishing May 21 in Cell Reports has an explanation: The surface proteins that the measles virus uses to enter cells are ineffective if they suffer any mutation, meaning that any changes to the virus come at a major cost.


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Credit: National Cancer Institute


The researchers used a high-throughput approach to mutate all of the genes in a virus in one experiment—a useful way to understand the future of viral evolution. They inserted mutations across the measles genome and looked to see whether the viruses were still capable of infection. They found that measles could not tolerate any mutations to the proteins that are recognized by the human immune system, making it very unlike influenza.






“We didn’t know what we were going to see when we started,” says senior study author Nicholas Heaton, a microbiologist at the Icahn School of Medicine at Mount Sinai, New York. “The almost complete lack of tolerance to insertional mutation of the measles proteins was surprising. We thought that they may be less tolerant than the influenza proteins, but we were surprised by the magnitude of the difference.”


It’s only possible to speculate why the measles virus would find an evolutionary advantage to being so rigid, but one hypothesis is that measles uses a more complex strategy to get into human cells than influenza. Influenza, for instance, simply requires the binding of one of the sugars that decorate the outside of cells as a means of getting inside. In contrast, measles requires binding to specific cellular protein receptors as its doorway.


“There are many potential explanations for why measles virus proteins can’t tolerate insertional mutations, from changing protein stability to changing the structure or function of the proteins,” Heaton says. “If we can better understand why flexibility or rigidity is imposed at a molecular level, we may be able to understand more about why we see different dynamics of viral evolution.”




– Credit and Resource –


More information: Cell Reports, Fulton et al.: “Mutational analysis of measles virus suggests constraints on antigenic variation of the glycoproteins” dx.doi.org/10.1016/j.celrep.2015.04.054



Why you need one vaccine for measles and many for the flu

Device may make converting waste heat to electricity industrially competitive

Scientia — Currently, up to 75% of the energy generated by a car’s engine is lost as waste heat. In theory, some of this waste heat can be converted into electricity using thermoelectric devices, although so far the efficiency of these devices has been too low to enable widespread commercialization.


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The proposed thermoelectric device consists of many parallel nanowires with an external gate voltage that can be tuned to optimize the efficiency and power output for different temperature differences between the leads and different loads. Credit: Muttalib and Hershfield. ©2015 American Physical Society


Now in a new study, physicists have demonstrated that a thermoelectric device made of nanowires may achieve a high enough efficiency to be industrially competitive, potentially leading to improvements in fuel economy and other applications.


The scientists, Khandker A. Muttalib and Selman Hershfield, both physics professors at the University of Florida in Gainesville, have published a paper on the new thermoelectric device in a recent issue of Physical Review Applied.






In addition to recovering energy from the waste heat in combustion engines in vehicles, thermoelectric devices could also perform similar functions in the engines of ships, as well as in power plants, manufacturing refineries, and other places that produce large amounts of waste heat.


In their paper, the scientists explain that using bulk materials in thermoelectric devices has turned out to be inherently inefficient, but nanoengineered materials appear to be more promising. The new device consists simply of two large leads at different temperatures connected by several noninteracting, very thin nanowires. Each nanowire transmits current from the hotter lead to the colder lead, and many nanowires in parallel can scale the power up to high levels.


One of the biggest challenges facing thermoelectric devices is that the conditions that optimize a device’s efficiency and power output are different for different temperature gradients between the two leads as well as for different electrical loads (how much power is being consumed at a given moment). Because of this complexity, the optimum device for a particular temperature gradient and load may not work nearly as well for a different temperature gradient or load.


The researchers here found a way around this issue by applying a voltage to the nanowires, which allows power to be transmitted along the nanowires only at energies above a certain value. This value depends on the temperature gradient and the load, which vary, but the applied voltage can also be varied in order to tune the power transmission and simultaneously optimize the device’s power and efficiency.


Using nanowires to connect the leads also has a practical advantage compared to using other materials. While many other candidate materials are difficult to manufacture reliably, nanowires can be manufactured reliably and controllably, which is important for realizing the precise optimum dimensions.


Although the physicists’ theoretical analysis suggests that the proposed device could have significant performance advantages over current devices, they caution that it’s too early to make any definite estimates.


“Any estimate at this point is going to be unreliable because there are so many ways to lose heat in any practical device that our theoretical proposal does not take into account,” Muttalib told Phys.org. “Even then, we gave a very crude estimate in our paper where both the efficiency and power output can be tuned (with a gate voltage) to be significantly larger than any commercial device currently available. Note that there are other theoretical proposals with large efficiency but without sufficient power, and therefore not practically usable.”




Most importantly, the physicists hope that the new ideas presented here may inspire new ways of thinking about thermoelectric technology.


“Perhaps the greatest significance is a possible shift in paradigm in the design of thermoelectric devices,” Muttalib said. “Currently, the focus of the community is overwhelmingly in the so-called ‘linear response’ regime (where the temperature and the voltage gradients across the material connecting the hot and the cold leads are small); the performance of such devices depends solely on the properties of the connecting material. This has kept the current efforts limited to finding or designing a ‘good’ thermoelectric material. Our work suggests that, in the ‘non-linear’ regime, the performance of the device also depends crucially on the parameters of the leads and the loads; the optimization of performance in such cases has many more interesting possibilities to be explored.”


Although this work offers many new possible directions for future research, Muttalib and Hershfield hope that it will be other scientists who move the technology forward.


“We are both theoretical physicists doing research in basic sciences, and in particular we are not experts in device technology,” Muttalib said. “We stumbled upon the current idea while trying to understand the effects of non-linear response on electron transport in nano systems. We hope that experimentalists and device engineers will find our work interesting and will pursue it to build an actual device. Our next plan in this general area is to understand, again at a very fundamental theoretical level, the effects of phonons or lattice vibrations in nano systems in general; these effects are known to be important for thermoelectric devices as well.”


The nanowire-based thermoelectric device isn’t the only new thermoelectric design to appear recently. In the same issue of Physical Review Applied, Riccardo Bosisio, et al., at Service de Physique de l’Etat Condensé in France have developed a thermoelectric device in which the electrons travel through the nanowires by “phonon-assisted hopping,” where the phonons are vibrations that carry heat.






– Credit and Resource –


More information: K. A. Muttalib and Selman Hershfield. “Nonlinear Thermoelectricity in Disordered Nanowires.” Physical Review Applied. DOI: 10.1103/PhysRevApplied.3.054003



Device may make converting waste heat to electricity industrially competitive

Wednesday 20 May 2015

Taking control of light emission

Researchers find a way of tuning light waves by pairing two exotic 2-D materials.

Scientia — Researchers have found a way to couple the properties of different two-dimensional materials to provide an exceptional degree of control over light waves. They say this has the potential to lead to new kinds of light detection, thermal-management systems, and high-resolution imaging devices.


Freedawn Scientia - Taking control of light emission Researchers find a way of tuning light waves by pairing two exotic 2-D materials.

Researchers have shown that a DC voltage applied to layers of graphene and boron nitride can be used to control light emission from a nearby atom. Here, graphene is represented by a maroon-colored top layer; boron nitride is represented by yellow-green lattices below the graphene; and the atom is represented by a grey circle. A low concentration of DC voltage (in blue) allows the light to propagate inside the boron nitride, forming a tightly confined waveguide for optical signals.
Image: Anshuman Kumar Srivastava and Jose Luis Olivares/MIT


The new findings — using a layer of one-atom-thick graphene deposited on top of a similar 2-D layer of a material called hexagonal boron nitride (hBN) — are published in the journal Nano Letters. The work is co-authored by MIT associate professor of mechanical engineering Nicholas Fang and graduate student Anshuman Kumar, and their co-authors at IBM’s T.J. Watson Research Center, Hong Kong Polytechnic University, and the University of Minnesota.






Although the two materials are structurally similar — both composed of hexagonal arrays of atoms that form two-dimensional sheets — they each interact with light quite differently. But the researchers found that these interactions can be complementary, and can couple in ways that afford a great deal of control over the behavior of light.


The hybrid material blocks light when a particular voltage is applied to the graphene, while allowing a special kind of emission and propagation, called “hyperbolicity,” when a different voltage is applied — a phenomenon not seen before in optical systems, Fang says. One of the consequences of this unusual behavior is that an extremely thin sheet of material can interact strongly with light, allowing beams to be guided, funneled, and controlled by voltages applied to the sheet.


“This poses a new opportunity to send and receive light over a very confined space,” Fang says, and could lead to “unique optical material that has great potential for optical interconnects.” Many researchers see improved interconnection of optical and electronic components as a path to more efficient computation and imaging systems.


Light’s interaction with graphene produces particles called plasmons, while light interacting with hBN produces phonons. Fang and his colleagues found that when the materials are combined in a certain way, the plasmons and phonons can couple, producing a strong resonance.


The properties of the graphene allow precise control over light, while hBN provides very strong confinement and guidance of the light. Combining the two makes it possible to create new “metamaterials” that marry the advantages of both, the researchers say.


Phaedon Avouris, a researcher at IBM and co-author of the paper, says, “The combination of these two materials provides a unique system that allows the manipulation of optical processes.”


The combined materials create a tuned system that can be adjusted to allow light only of certain specific wavelengths or directions to propagate, they say. “We can start to selectively pick some frequencies [to let through], and reject some,” Kumar says.


Freedawn Scientia - Taking control of light emission Researchers find a way of tuning light waves by pairing two exotic 2-D materials.

A higher concentration of electric charge in the graphene (in red) “repels” the light coming from the atom.
Image: Anshuman Kumar Srivastava and Jose Luis Olivares/MIT


These properties should make it possible, Fang says, to create tiny optical waveguides, about 20 nanometers in size — the same size range as the smallest features that can now be produced in microchips. This could lead to chips that combine optical and electronic components in a single device, with far lower losses than when such devices are made separately and then interconnected, they say.




Co-author Tony Low, a researcher at IBM and the University of Minnesota, says, “Our work paves the way for using 2-D material heterostructures for engineering new optical properties on demand.”


Another potential application, Fang says, comes from the ability to switch a light beam on and off at the material’s surface; because the material naturally works at near-infrared wavelengths, this could enable new avenues for infrared spectroscopy, he says. “It could even enable single-molecule resolution,” Fang says, of biomolecules placed on the hybrid material’s surface.


Sheng Shen, an assistant professor of mechanical engineering at Carnegie Mellon University who was not involved in this research, says, “This work represents significant progress on understanding tunable interactions of light in graphene-hBN.” The work is “pretty critical” for providing the understanding needed to develop optoelectronic or photonic devices based on graphene and hBN, he says, and “could provide direct theoretical guidance on designing such types of devices. … I am personally very excited about this novel theoretical work.”


The research team also included Kin Hung Fung of Hong Kong Polytechnic University. The work was supported by the National Science Foundation and the Air Force Office of Scientific Research.






– Credit and Resource –


David L. Chandler | MIT News Office



Taking control of light emission

Monday 18 May 2015

Computing at the speed of light

Team takes big step toward much faster computers

Scientia — University of Utah engineers have taken a step forward in creating the next generation of computers and mobile devices capable of speeds millions of times faster than current machines.


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The overhead view of a new beamsplitter for silicon photonics chips that is the size of one-fiftieth the width of a human hair. Credit: Dan Hixson/University of Utah College of Engineering


The Utah engineers have developed an ultracompact beamsplitter—the smallest on record—for dividing light waves into two separate channels of information. The device brings researchers closer to producing silicon photonic chips that compute and shuttle data with light instead of electrons. Electrical and computer engineering associate professor Rajesh Menon and colleagues describe their invention today in the journal Nature Photonics.






Silicon photonics could significantly increase the power and speed of machines such as supercomputers, data center servers and the specialized computers that direct autonomous cars and drones with collision detection. Eventually, the technology could reach home computers and mobile devices and improve applications from gaming to video streaming.


“Light is the fastest thing you can use to transmit information,” says Menon. “But that information has to be converted to electrons when it comes into your laptop. In that conversion, you’re slowing things down. The vision is to do everything in light.”


Photons of light carry information over the Internet through fiber-optic networks. But once a data stream reaches a home or office destination, the photons of light must be converted to electrons before a router or computer can handle the information. That bottleneck could be eliminated if the data stream remained as light within computer processors.


“With all light, computing can eventually be millions of times faster,” says Menon.


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Credit: Dan Hixson/University of Utah College of Engineering


To help do that, the U engineers created a much smaller form of a polarization beamsplitter (which looks somewhat like a barcode) on top of a silicon chip that can split guided incoming light into its two components. Before, such a beamsplitter was over 100 by 100 microns. Thanks to a new algorithm for designing the splitter, Menon’s team has shrunk it to 2.4 by 2.4 microns, or one-fiftieth the width of a human hair and close to the limit of what is physically possible.




The beamsplitter would be just one of a multitude of passive devices placed on a silicon chip to direct light waves in different ways. By shrinking them down in size, researchers will be able to cram millions of these devices on a single chip.


Potential advantages go beyond processing speed. The Utah team’s design would be cheap to produce because it uses existing fabrication techniques for creating silicon chips. And because photonic chips shuttle photons instead of electrons, mobile devices such as smartphones or tablets built with this technology would consume less power, have longer battery life and generate less heat than existing mobile devices.


The first supercomputers using silicon photonics—already under development at companies such as Intel and IBM—will use hybrid processors that remain partly electronic. Menon believes his beamsplitter could be used in those computers in about three years. Data centers that require faster connections between computers also could implement the technology soon, he says.






– Credit and Resource –


More information: An integrated-nanophotonics polarization beamsplitter with 2.4 x 2.4µm2 footprint, Nature Photonics, DOI: 10.1038/nphoton.2015.80


Journal reference: Nature Photonics


Provided by University of Utah



Computing at the speed of light

Sunday 17 May 2015

What happens when Newton's third law is broken?

Scientia — Even if you don’t know it by name, everyone is familiar with Newton’s third law, which states that for every action, there is an equal and opposite reaction. This idea can be seen in many everyday situations, such as when walking, where a person’s foot pushes against the ground, and the ground pushes back with an equal and opposite force. Newton’s third law is also essential for understanding and developing automobiles, airplanes, rockets, boats, and many other technologies.


Freedawn Scientia - What happens when Newton's third law is broken?

In the new experiments, two layers of microparticles levitating at two different heights above an electrode have allowed researchers to investigate the statistical mechanics of nonreciprocal interactions, which violate Newton’s third law. Credit: A. V. Ivlev, et al. CC-BY-3.0


Even though it is one of the fundamental laws of physics, Newton’s third law can be violated in certain nonequilibrium (out-of-balance) situations. When two objects or particles violate the third law, they are said to have nonreciprocal interactions. Violations can occur when the environment becomes involved in the interaction between the two particles in some way, such as when an environment moves with respect to the two particles. (Of course, Newton’s law still holds for the complete “particles-plus-environment” system.)






Although there have been numerous experiments on particles with nonreciprocal interactions, not as much is known about what’s happening on the microscopic level—the statistical mechanics—of these systems.


In a new paper published in Physical Review X, Alexei Ivlev, et al., have investigated the statistical mechanics of different types of nonreciprocal interactions and discovered some surprising results—such as that extreme temperature gradients can be generated on the particle scale.


“I think the greatest significance of our work is that we rigorously showed that certain classes of essentially nonequilibrium systems can be exactly described in terms of the equilibrium’s statistical mechanics (i.e., one can derive a pseudo-Hamiltonian which describes such systems),” Ivlev, at the Max Planck Institute for Extraterrestrial Physics in Garching, Germany, told Phys.org. “One of the most amazing implications is that, for example, one can observe a mixture of two liquids in detailed equilibrium, yet each liquid has its own temperature.”


One example of a system with nonreciprocal interactions that the researchers experimentally demonstrated in their study involves charged microparticles levitating above an electrode in a plasma chamber. The violation of Newton’s third law arises from the fact that the system involves two types of microparticles that levitate at different heights due to their different sizes and densities. The electric field in the chamber drives a vertical plasma flow, like a current in a river, and each charged microparticle focuses the flowing plasma ions downstream, creating a vertical plasma wake behind it.


Although the repulsive forces that occur due to the direct interactions between the two layers of particles are reciprocal, the attractive particle-wake forces between the two layers are not. This is because the wake forces decrease with distance from the electrode, and the layers are levitating at different heights. As a result, the lower layer exerts a larger total force on the upper layer of particles than the upper layer exerts on the lower layer of particles. Consequently, the upper layer has a higher average kinetic energy (and thus a higher temperature) than the lower layer. By tuning the electric field, the researchers could also increase the height difference between the two layers, which further increases the temperature difference.




“Usually, I’m rather conservative when thinking on what sort of ‘immediate’ potential application a particular discovery (at least, in physics) might have,” Ivlev said. “However, what I am quite confident of is that our results provide an important step towards better understanding of certain kinds of nonequilibrium systems. There are numerous examples of very different nonequilibrium systems where the action-reaction symmetry is broken for interparticle interactions, but we show that one can nevertheless find an underlying symmetry which allows us to describe such systems in terms of the textbook (equilibrium) statistical mechanics.”


While the plasma experiment is an example of action-reaction symmetry breaking in a 2D system, the same symmetry breaking can occur in 3D systems, as well. The scientists expect that both types of systems exhibit unusual and remarkable behavior, and they hope to further investigate these systems more in the future.


“Our current research is focused on several topics in this direction,” Ivlev said. “One is the effect of the action-reaction symmetry breaking in the overdamped colloidal suspensions, where the nonreciprocal interactions lead to a remarkably rich variety of self-organization phenomena (dynamical clustering, pattern formation, phase separation, etc.). Results of this research may lead to several interesting applications. Another topic is purely fundamental: how one can describe a much broader class of ‘nearly Hamiltonian’ nonreciprocal systems, whose interactions almost match with those described by a pseudo-Hamiltonian? Hopefully, we can report on these results very soon.”






– Credit and Resource –


More information: A. V. Ivlev, et al. “Statistical Mechanics where Newton’s Third Law is Broken.” Physical Review X. DOI: 10.1103/PhysRevX.5.011035


Journal reference: Physical Review X



What happens when Newton's third law is broken?

DARPA Aims to Accelerate Memory Function for Skill Learning

Research may accelerate rehabilitation post trauma or memory impairment, enable warfighter training

Scientia — A new DARPA program aims to investigate the role of neural “replay” in the formation and recall of memory, with the goal of helping individuals better remember specific episodic events and learned skills. The 24-month fundamental research program, Restoring Active Memory Replay or RAM Replay, is designed to develop novel and rigorous computational methods to help investigators determine not only which brain components matter in memory formation and recall but also how much they matter. To ensure real-world relevance, those assessments will be validated through performance on DoD-relevant tasks instead of conventional computer-based behavioral paradigms commonly used to assess memory in laboratory settings. New knowledge and paradigms for memory assessment and formation could translate into improved rehabilitation and recovery for injured warfighters challenged by impaired memory.


Freedawn Scientia - DARPA Aims to Accelerate Memory Function for Skill Learning


“Military personnel carry a growing responsibility to recount, report and act upon knowledge gleaned from previous experiences, and how well those experiences are recalled can make all the difference in how well these individuals perform in combat and other challenging situations,” said Dr. Justin Sanchez, DARPA program manager. But stored memories are not inert, Sanchez noted, and are subject to subtle forces over time. “The timeframe between a given experience and subsequent reporting or use of the memory can range from hours to months to years. During this time, physiological, environmental and behavioral factors can affect the process by which an individual’s representation of the experience is consolidated into memory, potentially affecting the accessibility and accuracy of the memory and one’s ability to make use of ‘lessons learned’ later on.”






Human memory is the result of biological processes that culminate in the formation or strengthening of neural connections in the brain. Multiple mechanisms are involved in memory formation and recall, including brain networks that govern perception, attention and emotion. Through a process known as consolidation, representations of experiences are stored in long-term memory and integrated with older knowledge and memories.


Studies investigating the mechanisms of memory formation, consolidation and retrieval have suggested that memory representations in the brain are repeatedly “reactivated”—albeit often unconsciously—following initial encoding, during both wakefulness and sleep. Moreover, memory reactivation has been linked to the process of neural replay, during which patterns of neural activity reflect the patterns of activity that had occurred during initial encoding of the memory.


The engagement of the replay process, frequency of activation and the time during which replay occurs can affect subsequent performance on behavioral tasks designed to assess memory recall and performance of learned skills. Additionally, some human studies have investigated modulation of subsequent memory recall via presentation of sensory cues or transcranial stimulation during specific phases of sleep. Of particular interest, there is growing evidence that various physiological or environmental factors may affect the degree to which replay strengthens memory circuits—and the accuracy with which it does so. That suggests the possibility of developing evidence-based means of harnessing the brain’s own replay system to improve the strength and fidelity of memory.


“Unconventional memory aids are everywhere today, from simple mnemonics to sophisticated smartphone apps. But many of these techniques focus on just a few of the many aspects that influence memory,” said Sanchez. “In the long run, we hope RAM Replay will identify core memory-strengthening mechanisms and give rise to a generalizable set of solutions applicable to the challenge of memory reliability in an increasingly information-dense world. That could benefit civilians and Service members alike in areas as diverse as general education, job retraining and battlefield awareness.”




– Credit and Resource –


DARPA



DARPA Aims to Accelerate Memory Function for Skill Learning

“100x Zoom Lens” for Seeing Distant Space Objects

Brainstorm with DARPA on a “100x Zoom Lens” for Seeing Distant Space Objects More Clearly. Request for Information seeks ideas for revolutionary telescope systems that could provide the first-ever ability to closely inspect objects in geosynchronous Earth orbit from the ground

Scientia — Imaging of Earth from satellites in space has vastly improved in recent years. But the opposite challenge—using Earth-based systems to find, track and provide detailed characterization of satellites and other objects in high orbits—has frustrated engineers even as the need for space domain awareness has grown. State-of-the-art imagery of objects in low Earth orbit (LEO), up to 2,000 km (1,200 miles) high, can achieve resolution of 1 pixel for every 10 cm today, providing relatively crisp details. But image resolution for objects in geosynchronous Earth orbit (GEO), a favorite parking place for space assets roughly 36,000 km (22,000 miles) high, drops to just 1 pixel for every 2 meters, meaning many GEO satellites appear as little more than fuzzy blobs when viewed from Earth. Enabling LEO-quality images of objects in GEO would greatly enhance the nation’s ability to keep an eye on the military, civilian and commercial satellites on which society has come to depend, and to coordinate ground-based efforts to make repairs or correct malfunctions when they occur.


Freedawn Scientia - Brainstorm with DARPA on a “100x Zoom Lens” for Seeing Distant Space Objects More Clearly Request for Information seeks ideas for revolutionary telescope systems that could provide the first-ever ability to closely inspect objects in geosynchronous Earth orbit from the ground

Imagery of objects in low Earth orbit (LEO) (left) can achieve much higher resolution than images of objects in geosynchronous Earth orbit (GEO) (right), which appear only as rough blobs. To improve space domain awareness, DARPA has issued a Request for Information (RFI) seeking specific technological information and innovative ideas to achieve high-resolution imaging of objects in GEO.


Achieving that goal will require radical technological advances because traditional or “monolithic” telescopes designed to provide high-resolution images of objects in GEO would be too physically and financially impractical to construct. For instance, achieving image resolution of 1 pixel to 10 cm for objects at GEO would require the equivalent of a primary imaging mirror 200 meters in diameter—longer than two football fields. To overcome these limitations and expedite the possible development of revolutionary benefits, DARPA has issued a Request for Information (RFI) (http://go.usa.gov/3Buvx) seeking specific technological information and innovative ideas demonstrating the potential for high-resolution imaging of GEO objects.






The RFI envisions a ground-based system that would be a sparse-aperture interferometer, which instead of relying upon one primary imaging mirror would measure the interference patterns of light detected by multiple smaller telescopes, from which a composite image could be derived. The GEO-imaging interferometer would rely on only passive (solar) illumination or thermal self-emission from imaged objects and could require the use of many telescopes, quite likely in a reconfigurable array. Responses to the RFI may inform a potential future program.


“We’re looking for ideas on how to create ground-based sparse aperture telescope systems that would provide GEO imagery as clear as current LEO imagery,” said Lindsay Millard, DARPA program manager. “This ‘100x zoom lens’ would provide the first ground-based capability to quickly assess anomalies that happen to GEO satellites, such as improperly deployed antennas or partially unfurled solar panels. With that capability, satellite owners could identify and fix problems more effectively and increase their satellites’ operating lifetimes and performance.”


“The image resolution this RFI envisions—down to a milli-arcsecond, or approximately one-3.6-millionth of a degree—would be up to 100 times more powerful than the current state of the art,” Millard continued. “Beyond helping us achieve our immediate needs on orbit, that improvement could significantly advance astronomy research, helping us learn about black holes and galaxy dynamics, as well as characterizing nearby exoplanets and detecting more-distant ones.”




The RFI invites short responses (3 pages or fewer) that explore some or all of the following technical areas:


> Direct atmospheric phase measurement: Information on methods to directly and locally measure atmospheric conditions to enable collection of clear data at the distances between apertures envisioned for the system, as well as decrease system complexity and infrastructure requirements


> Meter-class replicated optics and compensation of low-quality optics: Information about replicated optics technology applicable to telescopes 0.5 meter to 5 meters in diameter to potentially mitigate the need for high-precision fabrication, and reduce fabrication cost and timescales by an order of magnitude over conventional optical manufacturing methods


> Image-formation algorithms: Ideas on novel image formation algorithms and post-processing techniques that would enable reliable image reconstruction from sparse aperture or similar imaging systems


> Interferometry demonstration testbeds: Information about existing facilities that may provide economical and expedient means of demonstrating such technologies by utilizing existing infrastructure


To maximize the pool of innovative proposal concepts, DARPA strongly encourages participation by non-traditional performers, including small businesses, academic and research institutions and first-time government contractors. For this RFI, DARPA particularly seeks expertise in astronomy, novel optical design and quantum optics as it applies to long-baseline interferometry.






– Credit and Resource –
DARPA



“100x Zoom Lens” for Seeing Distant Space Objects

Defects in atomically thin semiconductor emit single photons

Researchers create optically active quantum dots in 2D semiconductor for the first time; may have applications for integrated photonics

Scientia–Researchers at the University of Rochester have shown that defects on an atomically thin semiconductor can produce light-emitting quantum dots. The quantum dots serve as a source of single photons and could be useful for the integration of quantum photonics with solid-state electronics – a combination known as integrated photonics.


Freedawn Scientia - Defects in atomically thin semiconductor emit single photons

Optical micrograph of electrically contacted tungsten diselenide. This atomically thin semiconductor is the host of an new type of quantum dot that exhibits voltage controlled single photon emission. Image courtesy of Chakraborty et al


Scientists have become interested in integrated solid-state devices for quantum information processing uses. Quantum dots in atomically thin semiconductors could not only provide a framework to explore the fundamental physics of how they interact, but also enable nanophotonics applications, the researchers say.


Quantum dots are often referred to as artificial atoms. They are artificially engineered or naturally occurring defects in solids that are being studied for a wide range of applications. Nick Vamivakas, assistant professor of optics at the University of Rochester and senior author on the paper, adds that atomically thin, 2D materials, such as graphene, have also generated interest among scientists who want to explore their potential for optoelectronics. However, until now, optically active quantum dots have not been observed in 2D materials.






In a paper published in Nature Nanotechnology this week, the Rochester researchers show how tungsten diselenide (WSe2) can be fashioned into an atomically thin semiconductor that serves as a platform for solid-state quantum dots. Perhaps most importantly the defects that create the dots do not inhibit the electrical or optical performance of the semiconductor and they can be controlled by applying electric and magnetic fields.


Vamivakas explains that the brightness of the quantum dot emission can be controlled by applying the voltage. He adds that the next step is to use voltage to “tune the color” of the emitted photons, which can make it possible to integrate these quantum dots with nanophotonic devices.


A key advantage is how much easier it is to create quantum dots in atomically thin tungsten diselenide compared to producing quantum dots in more traditional materials like indium arsenide.


“We start with a black crystal and then we peel layers of it off until we have an extremely thin later left, an atomically thin sheet of tungsten diselenide,” said Vamivakas.


The researchers take two of these atomically thin sheets and lay one over the other one. At the point where they overlap, a quantum dot is created. The overlap creates a defect in the otherwise smooth 2D sheet of semiconductor material. The extremely thin semiconductors are much easier to integrate with other electronics.




The quantum dots in tungsten diselenide also possess an intrinsic quantum degree of freedom – the electron spin. This is a desirable property as the spin can both act as a store of quantum information as well as provide a probe of the local quantum dot environment.


“What makes tungsten diselenide extremely versatile is that the color of the single photons emitted by the quantum dots is correlated with the quantum dot spin,” said first author Chitraleema Chakraborty. Chakraborty added that the ease with which the spins and photons interact with one another should make these systems ideal for quantum information applications as well as nanoscale metrology.


The paper, “Voltage controlled quantum light from an atomically thin semiconductor,” was published by Nature Nanotechnology on May 4, 2015. Apart from Vamivakas and Chakraborty, the team also included Laura Kinnischtzke, Kenneth M. Goodfellow, and Ryan Beams from the University of Rochester.






– Credit and Resource –


Provided by: University of Rochester



Defects in atomically thin semiconductor emit single photons

When an electron splits in two

Scientia – As an elementary particle, the electron cannot be broken down into smaller particles, at least as far as is currently known. However, in a phenomenon called electron fractionalization, in certain materials an electron can be broken down into smaller “charge pulses,” each of which carries a fraction of the electron’s charge. Although electron fractionalization has many interesting implications, its origins are not well understood.


Freedawn, Scientia, elementary particle, the electron cannot be broken down into smaller particles, at least as far as is currently known. However, in a phenomenon called electron fractionalization, in certain materials an electron can be broken down into smaller "charge pulses," each of which carries a fraction of the electron's charge. Although electron fractionalization has many interesting implications, its origins are not well understood.

An artistic illustration of electron fractionalization. When an electron travels along the outer 1D wire in an interferometer, the Coulomb interaction between the outer and inner 1D wires produces two types of excitation pairs, as shown here: two pulses of the same sign (carrying a net charge) and two pulses of opposite signs (which together are neutral). Because the two different excitation pairs travel at different velocities, the original electron eventually splits into two distinct charge pulses in the inner wire. Credit: Freulon, et al. ©2015 Nature


Now in a new paper published in Nature Communications, a team of physicists led by Gwendal Fève at the Ecole Normale Supérieure in Paris and the Laboratory for Photonics and Nanostructures in Marcoussis have applied an experiment typically used to study photons to investigate the underlying mechanisms of electron fractionalization. The method allows the researchers to observe single-electron fractionalization on the picosecond scale.






“We have been able to visualize the splitting of an electronic wavepacket into two fractionalized packets carrying half of the original electron charge,” Fève told Phys.org. “Electron fractionalization has been studied in previous works, mainly during roughly the last five years. Our work is the first to combine single-electron resolution—which allows us to address the fractionalization process at the elementary scale—with time resolution to directly visualize the fractionalization process.”


The technique that the researchers used is called the Hong-Ou-Mandel experiment, which can be used to measure the degree of resemblance between two photons, or in this case electron charge pulses, in an interferometer. This experiment also requires a single-electron emitter, which some of the same researchers, along with many others, have recently been developing.


The researchers first analyzed the propagation of a single electron in the interferometer’s outer one-dimensional wire, and then when that electron fractionalized, they could observe the interaction between its two charge pulses in the inner one-dimensional wire. As the researchers explain, when the original electron travels along the outer wire, Coulomb interactions (interactions between charged particles) between excitations in the outer and inner wires produce two types of excitation pairs: two pulses of the same sign (carrying a net charge) and two pulses of opposite signs (which together are neutral). The two different excitation pairs travel at different velocities, again due to Coulomb interactions, which causes the original electron to split into two distinct charge pulses.


Freedawn, Scientia, elementary particle, the electron cannot be broken down into smaller particles, at least as far as is currently known. However, in a phenomenon called electron fractionalization, in certain materials an electron can be broken down into smaller "charge pulses," each of which carries a fraction of the electron's charge. Although electron fractionalization has many interesting implications, its origins are not well understood.

(a) An electron on the outer channel fractionalizes into two pulses. (b) A modified scanning electron microscope picture of the sample. Credit: Freulon, et al. ©2015 Nature


The experiment reveals that, when a single electron fractionalizes into two pulses, the final state cannot be described as a single-particle state, but rather as a collective state composed of several excitations. For this reason, the fractionalization process destroys the original electron particle. Electron destruction can be measured by the decoherence of the electron’s wave packet.


Gaining a better understanding of electron fractionalization could have a variety of implications for research in condensed matter physics, such as controlling single-electron currents in one-dimensional wires.


“There has been, during the past years, strong efforts to control and manipulate the propagation of electrons in electronic conductors,” Fève said. “It bears many analogies with the manipulations of the quantum states of photons performed in optics. For such control, one-dimensional conductors are useful, as they offer the possibility to guide the electrons along a one-dimensional trajectory. However, Coulomb interactions between electrons are also very strong in one-dimensional wires, so strong that electrons are destroyed: they fractionalize. Understanding fractionalization is understanding the destruction mechanism of an elementary electron in a one-dimensional wire. Such understanding is very important if one wants to control electronic currents at the elementary scale of a single electron.”




In the future, the researchers plan to perform further experiments with the Hong-Ou-Mandel interferometer in order to better understand why fractionalization leads to electron destruction, and possibly how to suppress fractionalization.


“The Hong-Ou-Mandel interferometer can be used to picture the temporal extension (or shape) of the electronic wavepackets, which is what we used to visualize the fractionalization process,” Fève said. “It can also be used to capture the phase relationship (or phase coherence) between two components of the electronic wavepacket.


“This combined information fully defines the single-electron state, offering the possibility to visualize the wavefunction of single electrons propagating in a one-dimensional conductor. This would first provide a complete understanding of the fractionalization mechanism and in particular how it leads to the decoherence of single-electron states. It would also offer the possibility to test if single electrons can be protected from this decoherence induced by Coulomb interaction. Can we suppress (or reduce) the fractionalization process by reducing the strength of the Coulomb interaction? We would then be able to engineer and visualize pure single-electron states, preserved from Coulomb interaction.


“The next natural step is then to address few-particle states and electron entanglement in quantum conductors. Again, the question of the destruction of such states by Coulomb interaction effects will be a crucial one.”






– Credit and Resource –


More information: V. Freulon, et al. “Hong-Ou-Mandel experiment for temporal investigation of single-electron fractionalization.” Nature Communications. DOI: 10.1038/ncomms7854


Journal reference: Nature Communications



When an electron splits in two

New Theories on Dark Matter

Tom Broadhurst, the Ikerbasque researcher in the Department of Theoretical Physics of the UPV/EHU, together with Sandor Molnar of the National Taiwan University and visiting Ikerbasque researcher at the UPV/EHU in 2013, have conducted a simulation that explains the collision between two clusters of galaxies. Clusters of galaxies are the biggest objects that exist in the universe. They are collections of hundreds of thousands of galaxies pulled together by gravity.


Freedawn Scientia - Fresh theories about dark matter, comparing the data showing the many galaxies and the X-ray emission from the hot gas (left) with the model of the hot gas (right). The "comet" shape of the X-ray data is well reproduced by the model

An image comparing the data showing the many galaxies and the X-ray emission from the hot gas (left) with the model of the hot gas (right). The “comet” shape of the X-ray data is well reproduced by the model


In general, galaxy clusters grow in size by merging with each other to become increasingly larger. Gravitational forces cause them to slowly come together over time despite the expansion of the universe. The system known as “El Gordo”, the biggest known cluster of galaxies, is in turn the result of the collision between two large clusters. It was found that the collision process compresses the gas within each cluster to very high temperatures so that it is shining in the Xray region of the spectrum. In the Xray spectrum this gas cloud is comet shaped with two long tails stretching between the dense cores of the two clusters of galaxies. This distinctive configuration has allowed the researchers to establish the relative speed of the collision, which is extreme (~2200km/second), as it puts it at the limit of what is allowed by current theory for dark matter.






These rare, extreme examples of clusters caught in the act of colliding seem to be challenging the accepted view that dark matter is made up of heavy particles, since no such particles have actually been detected yet, despite the efforts being made to find them by means of the LHC (Large Hadron Particle Collider) accelerator in Geneva and the LUX (Large Underground Xenon Experiment), an underground dark matter detector in the United States. In Tom Broadhurst’s opinion, “it’s all the more important to find a new model that will enable the mysterious dark matter to be understood better”. Broadhurst is one of the authors of a wave-dark-matter model published in Nature Physics last year.


This new piece of research has entailed interpreting the gas observed and the dark matter of El Gordo “hydrodynamically” through the development of an in-house computational model that includes the dark matter, which comprises most of the mass, and which can be observed in the Xray region of the visible spectrum because of its extremely high temperature (100 million kelvin). Dr Broadhurst and Dr Molnar have managed to obtain a unique computational solution for this collision because of the comet-like shape of the hot gas, and the locations and the masses of the two dark matter cores that have passed through each other at an oblique angle at a relative speed of about 2200 km/s. This means that the total energy release is bigger than that of any other known phenomenon, with the exception of the Big Bang.




– Credit and Resource –


More information: “Hydrodynamical Solution for the ‘Twin-Tailed’ Colliding Galaxy Cluster ‘El Gordo.'” Astrophysical Journal, ApJ 800 37. DOI: 10.1088/0004-637X/800/1/37


Journal reference: Astrophysical Journal and Nature Physics


Provided by University of the Basque Country



New Theories on Dark Matter

Polysis is marketing a plastic that turns to clay

Polysis is showing a plastic that can turn to clay when heated, according to a story on DigInfo TV. Polysis is described as a specialist developer of polyurethane resins and resin products, and they are marketing haplafreely, presented with a lower-case “h,” as a plastic that turns to clay when heated to temperatures above 60 degrees Centigrade.


Freedawn Scientia - Polysis is marketing a plastic that turns to clay


Immerse the product in hot water—or heat it with a heat gun—and you find that the plastic is easy to shape, yet hardens again as it cools—and returns to its original hardness by the time it reaches room temperature.






Takato Mori, development division of Polysis, said the product remains in its clay state—staying malleable— five to 10 times longer than other products.”It also has a tensile strength,” he said, “three times greater than ordinary rubber, making it hard to break.”


It’s not difficult to peel off haplafreely; it won’t stick easily to other materials, according to DigInfo TV. It is softer than other plastics. As a cover material, it will not damage the product to which it is applied.


Promoted benefits include cutting costs. One does not have to think about thermal design or processing; the product can be formed into different shapes without them. “When heated, it will return to clay time and time again, making it ideal as a way of reducing costs in production line jigs.”


Real-world uses? The presentation suggested haplafreely as a cover for various components. Mori said haplafreely can be used to form bases on which to place unstable objects. For example, engine components need to be placed on a base for stability. Another case, he said, might be where motorcycle handlebars need to be worked on with a screwdriver. Haplafreey can be used in large quantities for protective covering.





Polysis is currently selling haplafreely in sheets measuring 40cm x 40cm and 4mm in thickness, and is aiming for monthly sales of 1,000 sheets, but haplafreely is also available in roll form, in thicknesses ranging from 0.6mm to 1.0mm.


The DigInfo TV report stated that “Polysis has received many requests from users for products that become soft at 70, 80 or 100°C, and will begin developing these this year.”


Commenting, Lee Mathews in Geek.com said the product was “noteworthy for its ability to become malleable with a minimal amount of heat applied.” He said haplafreely could make a difference on production lines. “If parts can be molded at a lower temperature, that means reduced energy use and shorter production times, which ultimately turns into either savings for you and me or higher profit margins for the producer. Or maybe even both.”







Polysis is marketing a plastic that turns to clay

NASA Challenges Designers to Construct Habitat for Deep Space Exploration

Freedawn Scientia - NASA Challenges Designers to Construct Habitat for Deep Space Exploration

Credits: NASA


NASA and the National Additive Manufacturing Innovation Institute, known as America Makes, are holding a new $2.25 million competition to design and build a 3-D printed habitat for deep space exploration, including the agency’s journey to Mars.


The multi-phase 3-D Printed Habitat Challenge, part of NASA’s Centennial Challenges program, is designed to advance the additive construction technology needed to create sustainable housing solutions for Earth and beyond.


Shelter is among the most basic and crucial human needs, but packing enough materials and equipment to build a habitat on a distant planet would take up valuable cargo space that could be used for other life-sustaining provisions. The ability to manufacture a habitat using indigenous materials, combined with material that would otherwise be waste from the spacecraft, would be invaluable.






The first phase of the competition, announced Saturday at the Bay Area Maker Faire in San Mateo, California, runs through Sept. 27. This phase, a design competition, calls on participants to develop state-of-the-art architectural concepts that take advantage of the unique capabilities 3-D printing offers. The top 30 submissions will be judged and a prize purse of $50,000 will be awarded at the 2015 World Maker Faire in New York.


“The future possibilities for 3-D printing are inspiring, and the technology is extremely important to deep space exploration,” said Sam Ortega, Centennial Challenges program manager. “This challenge definitely raises the bar from what we are currently capable of, and we are excited to see what the maker community does with it.”


The second phase of the competition is divided into two levels. The Structural Member Competition (Level 1) focuses on the fabrication technologies needed to manufacture structural components from a combination of indigenous materials and recyclables, or indigenous materials alone. The On-Site Habitat Competition (Level 2) challenges competitors to fabricate full-scale habitats using indigenous materials or indigenous materials combined with recyclables. Both levels open for registration Sept. 26, and each carries a $1.1 million prize.


Winning concepts and products will help NASA build the technical expertise to send habitat-manufacturing machines to distant destinations, such as Mars, to build shelters for the human explorers who follow. On Earth, these capabilities may be used one day to construct affordable housing in remote locations with limited access to conventional building materials.


“America Makes is honored to be a partner in this potentially revolutionary competition,” said Ralph Resnick, founding director of America Makes. “We believe that 3D printing/Additive Manufacturing has the power to fundamentally change the way people approach design and construction for habitats, both on earth and off, and we are excitedly awaiting submissions from all types of competitors.”


America Makes is a public/private partnership of organizations focused on accelerating the capabilities and adoption of additive manufacturing technology.


The Centennial Challenges Program is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama for the agency’s Space Technology Mission Directorate in Washington.


For more information about the 3-D-Printed Habitat Challenge, visit: http://AmericaMakes.us/Challenge




– Credit and Resource –


NASA



NASA Challenges Designers to Construct Habitat for Deep Space Exploration

Researchers build new fermion microscope

Instrument freezes and images 1,000 individual fermionic atoms at once.

Freedawn Scientia - Researchers build new, fermion microscope, Instrument freezes and images 1,000, individual fermionic atoms


Fermions are the building blocks of matter, interacting in a multitude of permutations to give rise to the elements of the periodic table. Without fermions, the physical world would not exist.


Examples of fermions are electrons, protons, neutrons, quarks, and atoms consisting of an odd number of these elementary particles. Because of their fermionic nature, electrons and nuclear matter are difficult to understand theoretically, so researchers are trying to use ultracold gases of fermionic atoms as stand-ins for other fermions.


But atoms are extremely sensitive to light: When a single photon hits an atom, it can knock the particle out of place — an effect that has made imaging individual fermionic atoms devilishly hard.


Now a team of MIT physicists has built a microscope that is able to see up to 1,000 individual fermionic atoms. The researchers devised a laser-based technique to trap and freeze fermions in place, and image the particles simultaneously.




The new imaging technique uses two laser beams trained on a cloud of fermionic atoms in an optical lattice. The two beams, each of a different wavelength, cool the cloud, causing individual fermions to drop down an energy level, eventually bringing them to their lowest energy states — cool and stable enough to stay in place. At the same time, each fermion releases light, which is captured by the microscope and used to image the fermion’s exact position in the lattice — to an accuracy better than the wavelength of light.


Freedawn Scientia - Researchers build new, fermion microscope, Instrument freezes and images 1,000, individual fermionic atoms, MIT

Laser beams are precisely aligned before being sent into the vacuum chamber.
Photo: Jose-Luis Olivares/MIT


With the new technique, the researchers are able to cool and image over 95 percent of the fermionic atoms making up a cloud of potassium gas. Martin Zwierlein, a professor of physics at MIT, says an intriguing result from the technique appears to be that it can keep fermions cold even after imaging.


“That means I know where they are, and I can maybe move them around with a little tweezer to any location, and arrange them in any pattern I’d like,” Zwierlein says.


Zwierlein and his colleagues, including first author and graduate student Lawrence Cheuk, have published their results today in the journal Physical Review Letters.


Seeing fermions from bosons

For the past two decades, experimental physicists have studied ultracold atomic gases of the two classes of particles: fermions and bosons — particles such as photons that, unlike fermions, can occupy the same quantum state in limitless numbers. In 2009, physicist Markus Greiner at Harvard University devised a microscope that successfully imaged individual bosons in a tightly spaced optical lattice. This milestone was followed, in 2010, by a second boson microscope, developed by Immanuel Bloch’s group at the Max Planck Institute of Quantum Optics.


These microscopes revealed, in unprecedented detail, the behavior of bosons under strong interactions. However, no one had yet developed a comparable microscope for fermionic atoms.


“We wanted to do what these groups had done for bosons, but for fermions,” Zwierlein says. “And it turned out it was much harder for fermions, because the atoms we use are not so easily cooled. So we had to find a new way to cool them while looking at them.”


Techniques to cool atoms ever closer to absolute zero have been devised in recent decades. Carl Wieman, Eric Cornell, and MIT’s Wolfgang Ketterle were able to achieve Bose-Einstein condensation in 1995, a milestone for which they were awarded the 2001 Nobel Prize in physics. Other techniques include a process using lasers to cool atoms from 300 degrees Celsius to a few ten-thousandths of a degree above absolute zero.


A clever cooling technique

And yet, to see individual fermionic atoms, the particles need to be cooled further still. To do this, Zwierlein’s group created an optical lattice using laser beams, forming a structure resembling an egg carton, each well of which could potentially trap a single fermion. Through various stages of laser cooling, magnetic trapping, and further evaporative cooling of the gas, the atoms were prepared at temperatures just above absolute zero — cold enough for individual fermions to settle onto the underlying optical lattice. The team placed the lattice a mere 7 microns from an imaging lens, through which they hoped to see individual fermions.


However, seeing fermions requires shining light on them, causing a photon to essentially knock a fermionic atom out of its well, and potentially out of the system entirely.


“We needed a clever technique to keep the atoms cool while looking at them,” Zwierlein says.


His team decided to use a two-laser approach to further cool the atoms; the technique manipulates an atom’s particular energy level, or vibrational energy. Each atom occupies a certain energy state — the higher that state, the more active the particle is. The team shone two laser beams of differing frequencies at the lattice. The difference in frequencies corresponded to the energy between a fermion’s energy levels. As a result, when both beams were directed at a fermion, the particle would absorb the smaller frequency, and emit a photon from the larger-frequency beam, in turn dropping one energy level to a cooler, more inert state. The lens above the lattice collects the emitted photon, recording its precise position, and that of the fermion.


Zwierlein says such high-resolution imaging of more than 1,000 fermionic atoms simultaneously would enhance our understanding of the behavior of other fermions in nature — particularly the behavior of electrons. This knowledge may one day advance our understanding of high-temperature superconductors, which enable lossless energy transport, as well as quantum systems such as solid-state systems or nuclear matter.


Freedawn Scientia - Researchers build new, fermion microscope, Instrument freezes and images 1,000, individual fermionic atoms, MIT

Sodium atoms diffuse out of an oven to form an atomic beam, which is then slowed and trapped using laser light.
Photo: Jose-Luis Olivares/MIT






“The Fermi gas microscope, together with the ability to position atoms at will, might be an important step toward the realization of a quantum computer based on fermions,” Zwierlein says. “One would thus harness the power of the very same intricate quantum rules that so far hamper our understanding of electronic systems.”


Freedawn Scientia - Researchers build new, fermion microscope, Instrument freezes and images 1,000, individual fermionic atoms, MIT

A Quantum gas microscope for fermionic atoms. The atoms, potassium-40, are cooled during imaging by laser light, allowing thousands of photons to be collected by the microscope.
Credit: Lawrence Cheuk/MIT


Zwierlein says it is a good time for Fermi gas microscopists: Around the same time his group first reported its results, teams from Harvard and the University of Strathclyde in Glasgow also reported imaging individual fermionic atoms in optical lattices, indicating a promising future for such microscopes.


Zoran Hadzibabic, a professor of physics at Trinity College, says the group’s microscope is able to detect individual atoms “with almost perfect fidelity.”


“They detect them reliably, and do so without affecting their positions — that’s all you want,” says Hadzibabic, who did not contribute to the research. “So far they demonstrated the technique, but we know from the experience with bosons that that’s the hardest step, and I expect the scientific results to start pouring out.”


This research was funded in part by the National Science Foundation, the Air Force Office of Scientific Research, the Office of Naval Research, the Army Research Office, and the David and Lucile Packard Foundation.


Freedawn Scientia - Researchers build new, fermion microscope, Instrument freezes and images 1,000, individual fermionic atoms, MIT

The Fermi gas microscope group: (from left) graduate students Katherine Lawrence and Melih Okan, postdoc Thomas Lompe, graduate student Matt Nichols, Professor Martin Zwierlein, and graduate student Lawrence Cheuk.
Photo: Jose-Luis Olivares/MIT






– Credit and Resource –


Jennifer Chu | MIT News Office



Researchers build new fermion microscope