2011-12-16

Close family ties keep cheaters in check: Why almost all multicellular organisms begin life as a single cell

How could the extreme degree of cooperation multicellular existence requires ever evolve? Why aren't all creatures unicellular individualists determined to pass on their own genes?

Joan Strassmann, PhD, and David Queller, PhD, a husband and wife team of evolutionary biologists at Washington University in St. Louis, provide an answer in the Dec. 16 issue of the journal Science. Experiments with amoebae that usually live as individuals but must also join with others to form multicellular bodies to complete their life cycles showed that cooperation depends on kinship.

If amoebae occur in well-mixed cosmopolitan groups, then cheaters will always be able to thrive by freeloading on their cooperative neighbors. But if groups derive from a single cell, cheaters will usually occur in all-cheater groups and will have no cooperators to exploit.

The only exceptions are brand new cheater mutants in all-cooperator groups, and these could pose a problem if the mutation rate is high enough and there are many cells in the group to mutate. In fact, the scientists calculated just how many times amoebae that arose from a single cell can safely divide before cooperation degenerates into a free-for-all.

The answer turns out to be 100 generations or more.

So population bottlenecks that kill off diversity and restart the population from a single cell are powerful stabilizers of cellular cooperation, the scientists conclude.

In other words our liver, blood and bone cells help our eggs and sperm pass on their genes because we passed through a single-cell bottleneck at the moment of conception.

The social amoebae

Queller, the Spencer T. Olin professor, and Strassmann, professor of biology, moved to WUSTL from Rice University this summer, bringing a truckload of frozen spores with them.

Although they worked for many years with wasps and stingless bees, Queller and Strassmann's current "lab rat" is the social amoeba Dictyostelium discoideum, known as Dicty for short.

The social amoebae can be found almost everywhere; in Antarctica, in deserts, in the canopies of tropical forests, and in Forest Park, the urban park that adjoins Washington University.

The amoebae spend most of their lives as tiny amorphous blobs of streaming protoplasm crawling through the soil looking for E. coli and other bacteria to eat.

Things become interesting when bacteria are scarce and the amoebae begin to starve. They then release chemicals that attract other amoebae, which follow this trail until they bump into one another.

A mound of some 10,000 amoebae forms and then elongates into a slug a few millimeters long that crawls forward (but never backward) toward heat and light.

The slug stops moving when it has reached a suitable place for dispersal, and then the front 20 percent of the amoebae die to produce a sturdy stalk that the remaining cells flow up and there become hardy spores.

Crucially, the 20 percent of the amoebae in the stalk sacrifice their genes so that the other 80 percent can pass theirs on.

When Strassmann and Queller began to work with Dicty in 1998, one of the first things they discovered was that the amoebae sometimes cheat.

Dennis Welker of Utah State University had given them a genetically diverse collection of wild-caught clones (genetically identical amoebae). They mixed amoebae from two clones together and then examined the fruiting bodies to see where the clones ended up. Each fruiting body included cells from both clones, but some clones contributed disproportionately to the spore body. They had cheated.

How can a blob of protoplasm cheat? The answer, it turns out, is many different ways.

"They might," Queller says, "have a mutation that makes an adhesion molecule less sticky, for example, so that they slide to the back of the slug, the part that forms spores."

"But there are tradeoffs," Strassmann says, "because if you're too slippery, you'll fall off the slug and lose all the advantages of being part of group."

Natural born cheaters

Mulling this over, Strassmann and Queller began to wonder if it would be possible to break the social contract among the amoebae by setting up conditions where relatedness was low and each clonal lineage encountered mostly strangers and rarely relatives.

Together with then-graduate student, Jennie Kuzdzal-Fick, they set up an experiment to learn what happened to cheating as heterogeneous (low relatedness) populations of amoebae evolved.

"At the end of the experiment, we assessed the cheating ability of the descendants by mixing equal numbers of descendants and ancestors and checking to see whether the descendants ended up in the stalks or the spores of the fruiting bodies," Strassmann says.

They found that in nearly all cases, the descendants cheated their ancestors. What's more, when descendent amoebae were grown as individual clones, about a third of them were unable to form fruiting bodies.

Many of the mutants, in other words, were "obligate" cheaters. Having lost the ability to form their own fruiting bodies, they were able to survive only by freeloading, or taking advantage of the amoebae that had retained the ability to cooperate.

This result, Queller and Strassmann say, shows that cheater mutations that threaten multicellularity occur naturally and are even favored -- as long as the population of amoebae remains genetically diverse.

What happens in the wild?

But the scientists were aware that obligate cheaters are either very rare or altogether missing among wild social amoebae. They had not found any obligate cheaters in the more than 2,000 wild clones they have sampled.

They also knew that in the wild, the amoebae in fruiting bodies are close kin, if not clones.

What prevents cooperation in wild populations from degenerating into the laboratory free-for-all? Could the difference be that the amoebae in the laboratory were distant relations and those in the wild are kissing kin?

Suppose, the scientists thought, one amoeba ventured alone into a pristine field of bacteria. As it grew and multiplied, making copies of itself, how long would it take for cheating mutations to appear (what was the mutation rate) and how successfully would these mutations proliferate (how strongly would they be selected)?

To establish the mutation rate, Strassmann and Queller together with graduate student Sara Fox ran what is called a mutation accumulation experiment.

In this experiment, amoebae that mutated didn't have to compete against amoebae that were faithful replicators. In the absence of selection, all but the most severe mutations were also reproduced and became a permanent part of the lineage's genome.

The scientists allowed 90 different lines of amoebae to accumulate mutations in this way.

"At the end," Queller says, "we found that among those 90 lines not a single one had lost the ability to fruit. So that's almost 100 lines, almost a thousand generations, so 100,000 opportunities to lose fruiting and none of them did.

"That allowed us, using statistics, to put an upper limit on the rate at which mutations turn a cooperator into an obligate cheater," he says.

The rate was low enough that if fruiting bodies were forming in the wild from amoebae that were all descended from one spore, cheating would never be an issue.

What this has to do with elephants and blue whales

But the scientists were inquisitive enough to ask another, bigger question. They used calculations invented for population genetics to ask how many times the amoeba could divide -- theoretically -- before cheating became a problem.

What if, they asked, we let an initial single amoebae divide until there were as many of amoebae as there are cells as a fruit fly and then transferred one amoeba and allowed it to divide until the daughter colony reached fruit-fly size, and so on?

What if we let the colonies grow to human size? To elephant size? To blue whale size? Would the cheaters bring down the whale-sized Dicty colony?

The answer, it turned out, was no.

A whale-sized Dicty colony is not the same thing as a whale, but nonetheless the experiments suggest how organisms, over the course of evolution, have sidestepped the cheating trap and maintained the levels of cooperation multicellular bodies demand.

"A multicellular body like the human body is an incredibly cooperative thing," Queller says, "and sociobiologists have learned that really cooperative things are hard to evolve because of the potential for cheating.

"It's the single-cell bottleneck that generates high relatedness among the cells that, in turn, allows them to cooperate, " he says.

Our liver cells have no kick against our sperm or egg cells, in other words, because they're all nearly genetically identical descendants of a single fertilized egg.

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Close family ties keep cheaters in check: Why almost all multicellular organisms begin life as a single cell

Scientists find microbes in lava tube living in conditions like those on Mars

The microbes tolerate temperatures near freezing and low levels of oxygen, and they can grow in the absence of organic food. Under these conditions their metabolism is driven by the oxidation of iron from olivine, a common volcanic mineral found in the rocks of the lava tube. These factors make the microbes capable of living in the subsurface of Mars and other planetary bodies, the scientists say.

The findings, supported by a grant from the National Aeronautics and Space Administration (NASA), are detailed in the journal Astrobiology.

"This microbe is from one of the most common genera of bacteria on Earth," said Amy Smith, a doctoral student at Oregon State University and one of the authors of the study. "You can find its cousins in caves, on your skin, at the bottom of the ocean and just about anywhere. What is different, in this case, is its unique qualities that allow it to grow in Mars-like conditions."

In a laboratory setting at room temperature and with normal oxygen levels, the scientists demonstrated that the microbes can consume organic material (sugar). But when the researchers removed the organic material, reduced the temperature to near-freezing, and lowered the oxygen levels, the microbes began to use the iron within olivine -- a common silicate material found in volcanic rocks on Earth and on Mars -- as its energy source.

"This reaction involving a common mineral from volcanic rocks just hasn't been documented before," said Martin Fisk, a professor in OSU's College of Earth, Ocean, and Atmospheric Sciences and an author on the study. "In volcanic rocks directly exposed to air and at warmer temperatures, the oxygen in the atmosphere oxidizes the iron before the microbes can use it. But in the lava tube, where the bacteria are covered in ice and thus sheltered from the atmosphere, they out-compete the oxygen for the iron.

"By mimicking those conditions, we got the microbes to repeat that behavior in the laboratory," Fisk added.

The microbes were collected from a lava tube near Newberry Crater in Oregon's Cascades Mountains, at an elevation of about 5,000 feet. They were within the ice on rocks some 100 feet inside the lava tube, in a low-oxygen, near-freezing environment. Scientists, including Fisk, have said that the subsurface of Mars could have similar conditions and harbor bacteria.

In fact, Fisk has examined a meteorite originating from Mars that contained tracks -- which could indicate consumption by microbes -- though no living material was discovered. Similar tracks were found on the rocks from the Newberry Crater lava tube, he said.

"Conditions in the lava tube are not as harsh as on Mars," Fisk said. "On Mars, temperatures rarely get to the freezing point, oxygen levels are lower and at the surface, liquid water is not present. But water is hypothesized to be present in the warmer subsurface of Mars. Although this study does not exactly duplicate what you would find on Mars, it does show that bacteria can live in similar conditions.

"We know from direct examination, as well as satellite imagery, that olivine is in Martian rocks," Fisk added. "And now we know that olivine can sustain microbial life."

The idea for exploring the lava tube came from Radu Popa, an assistant professor at Portland State University and lead author on the paper. Popa used to explore caves in his native Romania and was familiar with the environmental conditions. Because lava tubes are a sheltered environment and exist on both Earth and Mars, Popa proposed the idea of studying microbes from them to see if life may exist -- or could have existed -- on the Red Planet.

"When temperatures and atmospheric pressure on Mars are higher, as they have been in the past, ecosystems based on this type of bacteria could flourish," Popa said. "The fingerprints left by such bacteria on mineral surfaces can be used by scientists as tools to analyze whether life ever existed on Mars."

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Scientists find microbes in lava tube living in conditions like those on Mars

Discovery of a 'dark state' could mean a brighter future for solar energy

Zhu and his team have discovered that it's possible to double the number of electrons harvested from one photon of sunlight using an organic plastic semiconductor material.

"Plastic semiconductor solar cell production has great advantages, one of which is low cost," said Zhu, a professor of chemistry. "Combined with the vast capabilities for molecular design and synthesis, our discovery opens the door to an exciting new approach for solar energy conversion, leading to much higher efficiencies."

Zhu and his team published their groundbreaking discovery Dec. 16 in Science.

The maximum theoretical efficiency of the silicon solar cell in use today is approximately 31 percent, because much of the sun's energy hitting the cell is too high to be turned into usable electricity. That energy, in the form of "hot electrons," is instead lost as heat. Capturing hot electrons could potentially increase the efficiency of solar-to-electric power conversion to as high as 66 percent.

Zhu and his team previously demonstrated that those hot electrons could be captured using semiconductor nanocrystals. They published that research in Science in 2010, but Zhu says the actual implementation of a viable technology based on that research is very challenging.

"For one thing," said Zhu, "that 66 percent efficiency can only be achieved when highly focused sunlight is used, not just the raw sunlight that typically hits a solar panel. This creates problems when considering engineering a new material or device."

To circumvent that problem, Zhu and his team have found an alternative. They discovered that a photon produces a dark quantum "shadow state" from which two electrons can then be efficiently captured to generate more energy in the semiconductor pentacene.

Zhu said that exploiting that mechanism could increase solar cell efficiency to 44 percent without the need for focusing a solar beam, which would encourage more widespread use of solar technology.

The research team was spearheaded by Wai-lun Chan, a postdoctoral fellow in Zhu's group, with the help of postdoctoral fellows Manuel Ligges, Askat Jailaubekov, Loren Kaake and Luis Miaja-Avila. The research was supported by the National Science Foundation and the Department of Energy.

Science Behind the Discovery:

  • Absorption of a photon in a pentacene semiconductor creates an excited electron-hole pair called an exciton.
  • The exciton is coupled quantum mechanically to a dark "shadow state" called a multiexciton.
  • This dark shadow state can be the most efficient source of two electrons via transfer to an electron acceptor material, such as fullerene, which was used in the study.
  • Exploiting the dark shadow state to produce double the electrons could increase solar cell efficiency to 44 percent.

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Discovery of a 'dark state' could mean a brighter future for solar energy

'Fantastic voyage' through the body, with precision control

According to Dr. Gabor Kosa of TAU's School of Mechanical Engineering, the project is inspired by an endoscopic capsule designed for use in the small intestine. But unlike the existing capsule, which travels at random and snaps pictures every half second to give doctors an overall view of the intestines, the new "wireless" capsules will use the magnetic field of a magnetic resonance imaging (MRI) machine and electronic signals manipulated by those operating the capsule to forge a more precise and deliberate path.

It's a less invasive and more accurate way for doctors to get an important look at the digestive tract, where difficult-to-diagnose tumors or wounds may be hidden, or allow for treatments such as biopsies or local drug delivery. The technology, which was recently reported in Biomedical Microdevices, was developed in collaboration with Peter Jakab, an engineer from the Surgical Planning Laboratory at Brigham and Women's Hospital in Boston, affiliated with Harvard Medical School.

Swimming with the current

What sets this endoscope apart is its ability to actively explore the digestive tract under the direction of a doctor. To do this, the device relies on the magnetic field of the MRI machine as a "driving force," says Dr. Kosa. "An MRI has a very large constant magnetic field," he explains. "The capsule needs to navigate according to this field, like a sailboat sailing with the wind."

In order to help the capsules "swim" with the magnetic current, the researchers have given them "tails," a combination of copper coils and flexible polymer. The magnetic field creates a vibration in the tail which allows for movement, and electronics and microsensors embedded in the capsule allow the capsule's operator to manipulate the magnetic field that guides the movement of the device. The use of copper, a non-ferro magnetic material, circumvents other diagnostic challenges posed by MRI, Dr. Kosa adds. While most magnets interfere with MRI by obscuring the picture, copper appears as only a minor blot on otherwise clear film.

The ability to drive the capsule, Dr. Kosa says, will not only lead to better diagnosis capabilities, but patients will experience a less invasive procedure in a fraction of the time.

Microrobotics of the future

In the lab at the Brigham and Women's Hospital, Dr. Kosa and his fellow researchers have tested the driving mechanism of the capsule in an aquarium inside the MRI. The results have shown that the capsule can successfully be manipulated using a magnetic field. Moving forward, the researchers are hoping to further develop the capsule's endoscopic and signalling functions.

According to Dr. Kosa, a new faculty recruit to TAU, this project is part of a bright future for the field of microrobotics. At the university, his new research lab, called RBM2S, focuses on microsystems and robotics for biomedical applications, and an educational robotics lab, ERL, will teach future robotics experts studying at TAU's School of Mechanical Engineering.

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'Fantastic voyage' through the body, with precision control

First low-mass star detected in globular cluster

Until now, it was merely assumed that low-mass and therefore extremely faint stars must exist. However, in view of the vast distances and weak luminosity of low-mass stars, even the most modern telescopes fail. Together with a Polish-Chilean team of researchers, Swiss astrophysicist Philippe Jetzer from the University of Zurich has now detected the first low-mass star in the globular cluster M22 indirectly. As their recent article accepted in Astrophysical Journal Letters reveals, it involves a dwarf star that has less than a fifth of the mass of our sun and is 3.2 kiloparsecs from it (one kiloparsec corresponding to 3,210 light years).

The evidence, which enables the mass to be determined highly accurately, is based upon so-called gravitational microlensing and requires the highest technical standards available. The measurements were carried out on the ESO VLT 8-meter telescope with adaptive optics at the Paranal Observatory in Chile.

Major breakthrough in 2000

In August 2000 Polish astronomers discovered that the brightness of a star located at about two arcminutes from the center of the globular cluster M22 increased for twenty days. They suspected that the phenomenon was due to so-called gravitational microlensing, which is based on the fact that light spreads along a curved path near large masses as opposed to in a straight line. The brightness of the star increases briefly through the gravitation of an object crossing in front of it, which acts as a lens. The star -- the source, in other words -- appears brighter for a short time before fading again after passing by the lens. In order to confirm this supposition, the astronomers turned to gravitational microlensing specialist Philippe Jetzer from the University of Zurich. The control measurement carried out on July 17, 2011 at the Paranal Observatory confirmed the hypothesis. "The detailed analysis revealed that the source was outside M22," explains Jetzer. "A low-mass star acted as a lens within the globular cluster itself."

Low-mass stars instead of dark matter?

The first evidence of a low-mass star in a globular cluster is extremely important for astrophysics as it sheds new light on the structure of globular clusters. Until now, the overall mass of globular clusters could not be explained other than with dark matter, the existence of which, however, is unproven. "The overall mass or at least a significant proportion of globular clusters can now be explained through the presence of previously undetected low-mass, faint stars," says Jetzer.

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First low-mass star detected in globular cluster

Young star rebels against its parent cloud

Despite the celestial colours of this picture, there is nothing peaceful about star forming region Sh 2-106, or S106 for short. A devilish young star, named S106 IR, lies in it and ejects material at high speed, which disrupts the gas and dust around it. The star has a mass about 15 times that of the Sun and is in the final stages of its formation. It will soon quieten down by entering the main sequence, the adult stage of stellar life.

For now, S106 IR remains embedded in its parent cloud, but it is rebelling against it. The material spewing off the star not only gives the cloud its hourglass shape but also makes the hydrogen gas in it very hot and turbulent. The resulting intricate patterns are clearly visible in this Hubble image.

The young star also heats up the surrounding gas, making it reach temperatures of 10,000 degrees Celsius. The star's radiation ionises the hydrogen lobes, making them glow. The light from this glowing gas is coloured blue in this image.

Separating these regions of glowing gas is a cooler, thick lane of dust, appearing red in the image. This dark material almost completely hides the ionising star from view, but the young object can still be seen peeking through the widest part of the dust lane.

S106 was the 106th object to be catalogued by the astronomer Stewart Sharpless in the 1950s. It is a few thousand light-years distant in the direction of Cygnus (The Swan). The cloud itself is relatively small by the standards of star-forming regions, around 2 light-years along its longest axis. This is about half the distance between the Sun and Proxima Centauri, our nearest stellar neighbour.

This composite picture was obtained with the Wide Field Camera 3 on the NASA/ESA Hubble Space Telescope. It results from the combination of two images taken in infrared light and one which is tuned to a specific wavelength of visible light emitted by excited hydrogen gas, known as H-alpha. This choice of wavelengths is ideal for targetting star-forming regions. The H-alpha filter isolates the light emitted from hydrogen in gas clouds while the infrared light can shine through the dust that often obscures these regions.

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Young star rebels against its parent cloud

Analysts sees weaker chip sales in November


LONDON – The three-month average of global chip sales for November is going to be $25.6 billion flat compared to $25.74 billion reported for October by World Semiconductor Trade Statistics organization, according to Bruce Diesen, an analyst at Carnegie Group (Oslo, Norway).

This will be the result of actual November chip sales that will be 4 percent down year-on-year Diesen said.

"The world economy is slowing and the floods in Thailand have hurt the supply of key components for PC’s and smart phones in November. Automobile chips should outperform PC/handset chips in November," said Diesen in a note to clients.

In light of this Diesen expects global semiconductor sales to be the same in 2011 in U.S. dollar terms as in 2010, which is approximately $298 billion. Diesen forecasts 2012 global semiconductor sales to be up 2 percent on 2011.


Related links and articles:

October global chip sales fell back, says WSTS

Toshiba to close wafer fabs, slow IC production

WSTS drops 2012 chip market growth figure to 2.6 percent





Analysts sees weaker chip sales in November

2011-12-15

ST claims world first contactless wafer test


LONDON – European chip company STMicroelectronics NV has said it has produced the first wafer on which the die were fully tested wirelessly and without the use of contact probes.

The electromagnetic wafer sort (EMWS) technology was applied to a wafer of RFID (Radio Frequency Identification) ICs. It was developed in an R&D project called UTAMCIC (UHF TAG Antenna Magnetically Coupled to Integrated Circuit), led by Alberto Pagani, Giovanni Girlando and Alessandro Finocchiaro from STMicroelectronics, and Professor Giuseppe Palmisano from the University of Catania.

Electrical wafer sort is the last stage of wafer fabrication prior to assembly and test of packaged ICs. Conventional a probe card connected to automatic test equipment (ATE) makes contact with the bond pads on each die in turn and runs a series of tests. Under EMWS each die contains an antenna and the ATE supplies power and communicates with the IC wirelessly.

In some applications this can remove the need for dedicated test pads and reduce die area.

ST said that limitations in the amount of power that can be transmitted wirelessly means that some ICs will still require contact probes but that EMWS was applicable to low-power ICs.

EMWS make use of a focusing technique that can use multiple antenna to concentrate electromagnetic energy from across the wafer to the a small area, such as a single die. The Electromagnetic Concentrator/Expander allows the communication distance between the die and an external system such as the ATE to be increased by at least one order of magnitude.

Contactless testing also reduces the test cycle time because it reduces wafer movement and enables parallelism. Moreover, it increases yield by eliminating the pad damage that occasionally occurs during standard contact testing, ST said.


ST claims world first contactless wafer test

Rambus, ITRI to collaborate on 3-D packaging

SAN FRANCISCO—Technology licensor Rambus Inc. said Wednesday (Dec. 15) it is engaging Taiwan's Industrial Technology Research Institute (ITRI) on the development of interconnect and 3-D packaging technologies.

The work will initially focus on the development of system integration using silicon interposer technology, Rambus said.

Rambus (Sunnyvale, Calif.) also announced that it joined the Advanced Stacked-System Technology and Application Consortium (Ad-STAC), a multinational research association led by ITRI. Rambus and ITRI will work together as members of Ad-STAC on the development of system integration using silicon interposer technology, the company said.

According to Ramsbus, the collaboration combines ITRI’s strength in manufacturing and advanced process technologies with the system, package and signaling design experience of Rambus.

"Collaborating with leading research institutions, such as ITRI, is an effective way for us to advance 3-D packaging technology for the broader manufacturing community," said John Kent, vice president of technology development at Rambus, in a statement.

Rambus, ITRI to collaborate on 3-D packaging

Why buttercups reflect yellow on chins: Research sheds light on childrens game and provides insight into pollination

Their findings were published December 14, in the Royal Society journal Interface.

The researchers discovered that the buttercup petal's unique bright and glossy appearance is the result of the interplay between its different layers. In particular, the strong yellow reflection responsible for the chin illumination is mainly due to the epidermal layer of the petal that reflects yellow light with an intensity that is comparable to glass.

Scientists have been interested in how the buttercup flower works for over a century. They have previously shown that the reflected colour is yellow due to the absorption of the colours in the blue-green region of the spectrum by the carotenoid pigment in the petals. As the blue-green light is absorbed, the light in the other spectral regions (in this case, primarily yellow) is reflected. It has also been known for many years that the epidermal layer of the petals is composed of very flat cells, providing strong reflection.

This new study shows how the buttercup's exceptionally bright appearance is a result of a special feature of the petal structure. The epidermal layer of cells has not one but two extremely flat surfaces from which light is reflected. One is the top of the cells, the other exists because the epidermis is separated from the lower layers of the petal by an air gap. Reflection of light by the smooth surface of the cells and by the air layer effectively doubles the gloss of the petal, explaining why buttercups are so much better at reflecting light under your chin than any other flower.

The researchers also found that the buttercup reflects a significant amount of UV light. As many pollinators, including bees, have eyes sensitive in the UV region, this provides insight into how the buttercup uses its unique appearance to attract insects.

Dr Silvia Vignolini, from the University of Cambridge's Department of Physics (Cavendish Laboratory), explained the importance of the buttercup's unique appearance: "Although many different factors, such as scent and temperature, influence the relationships between pollinators and flowers, the visual appearance of flowers is one of the most important factors in this communication. Flowers develop brilliant colour, or additional cues, such as glossiness -- in the case of the buttercup -- that contribute to make the optical response of the flower unique. Moreover, the glossiness might also mimic the presence of nectar droplets on the petals, making them that much more attractive."

Dr Beverley Glover, Department of Plant Sciences, said: "This phenomenon has intrigued scientists and laymen alike for centuries. Our research provides exciting insight into not only a children's game but also into the lengths to which flowers will go to attract pollinators."

Professor Ulli Steiner, from the Nanophotonics Centre at the Cavendish Laboratory, the University of Cambridge's Department of Physics, said: "It is fun to revisit a problem that is more than one century old and, using modern methods, discover something new. The strong collaboration between Physics and the Plant Sciences has enabled this."

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Why buttercups reflect yellow on chins: Research sheds light on childrens game and provides insight into pollination

Lam to buy Novellus in $3.3B, all-stock deal

SAN FRANCISCO—Lam Research Corp. said Wednesday (Dec. 14) it would acquire rival semiconductor capital equipment maker Novellus Systems Corp. in an all-stock deal valued at about $3.3 billion.

Rumors about a possible Lam-Novellus deal have been circulating for years. The companies strengths within the capital equipment market are complementary, with Lam being especially strong in etch systems and Novellus in surface preparation and deposition technologies. According to Risto Puhakka, president of VLSI Research Inc., the two companies have virtually no products that compete head-to-head.

"It's a good fit," Puhakka said. "It's two really good companies getting together. It was just time to happen."

According to Puhakka, the timing of the deal is consistent with consolidation trends that have emerged over the past couple of years. "The playing field is narrowing down to two key suppliers for each [equipment] segment," Puhakka said. "This makes sense because Lam becomes a lot larger and gets huge economies of scale."

Lam, the No. 4 vendor in semiconductor equipment by sales in 2010, is likely to solidify its hold on that spot but unlikely to move higher in the vendor rankings. The combined revenue of Lam and Novellus in 2010 was about $3.55 billion. The top three vendors—Applied Materials Inc., ASML Holding NV and Tokyo Electron Corp.—had revenues of $5.95 billion, $5.04 billion and $4.12 billion in 2010, according to VLSI.

Puhakka said the deal might boost Lam's chances of doing more business with No. 1 semiconductor supplier Intel Corp., a longtime Novellus customer. Despite being the No. 1 vendor in etch systems, Lam has famously been unable to crack the Intel account with its etchers, he said.

"Novellus's strong capabilities and market leadership in deposition and surface preparation technologies enable Lam to become more deeply entrenched in critical semiconductor manufacturing processes that are important to our customers," said Steve Newberry, Lam's vice chairman and CEO, in a statement.

Under the terms of the agreement, Novellus stockholders will receive 1.125 shares of Lam Research common stock for each share of Novellus that they own, in a tax-free exchange, Lam said. Based on the closing price of Lam's stock Wednesday, the transaction values Novellus at a price of $44.42 per common share. Novellus' stock price closed at $34.70 Wednesday, prior to the acquisition announcement, making Lam's offer a 28 percent price premium over the stock's value.

Martin Anstice, who is set to become Lam's CEO on Jan. 1, will remain CEO of the combined company, Lam said. Timothy Archer, chief operating officer at Novellus, will become chief operating officer of the combined company, Lam said. Ernest Maddock, Lam's chief financial officer, will remain chief financial officer, Lam said. The board of directors of Lam will add four new directors jointly nominated by Lam and Novellus, Lam said.

Upon closing, Lam and Novellus stockholders will own approximately 59 percent and 41 percent, respectively, of the combined company, Lam said.

Lam said it expects total cost synergies between the two companies to be worth about $100 million per year. The firm said the combined company would be positioned to grow faster than either company could achieve individually through advancing technical benefits from owning adjacent technologies, optimizing and accelerating collective development of next-generation tools and further developing complementary customer relationships.

Lam also announced a $1.6 billion common stock repurchase program, which replaces its existing share repurchase program.
Lam to buy Novellus in $3.3B, all-stock deal

Intel announces mobile and wireless reorganization

MOUNTAIN VIEW, Calif--In a bid to tighten and hone its mobile technology focus, Intel Corp. has confirmed it has reorganized several business units to form a new mobile and communications group which will be responsible for all the firm’s smartphone, tablet and wireless communication efforts.

The reorganization fuses together the mobile communications, netbook/tablet, mobile wireless and ultra-mobility business units into one group headed by former Palm executive Mike Bell and former Infineon Wireless chief Hermann Eul.

A spokesperson said Intel was looking to “speed up and improve development of Intel-based mobile devices,” from streamlining the software development efforts for tablets and phones to fine tuning the SoCs for mobile usage.

Back in March 2011, Intel announced that Anand Chandraskher, GM of the former ultra-mobility group, would be leaving the company to "pursue other interests," with many analysts positing that he had been ousted for failing to deliver on Intel’s long held mobile aspirations.

An Intel spokesman said Bell and Eul’s role would be bigger than Chandraskher’s, with the pair boasting numerous years of wireless industry experience between them.

Though Palm was never a big player in the mobile market, Bell also has previous experience at Apple Inc. where he worked on the Macintosh and the early iPhone model. Eul, on the other hand, will be instrumental to helping Intel integrate wireless baseband onto its Atom chips, putting the firm in direct competition with rival Qualcomm.

It’s generally believed that Atom products with integrated baseband could emerge within the next two years.

Intel has said publicly it hopes to have a viable smartphone offering on the market within the first half of 2012, and has made much of its partnership with Google for Android x86 development. Whether Intel’s engineers are able to reduce Atom power levels significantly enough to compete seriously with ARM’s chip architecture, however, remains to be seen.
Intel announces mobile and wireless reorganization

Dinosaurs with killer claws yield new theory about evolution of flight

In a paper published Dec. 14 in PLoS ONE, MSU researchers Denver W. Fowler, Elizabeth A. Freedman, John B. Scannella and Robert E. Kambic (now at Brown University in Rhode Island), describe how comparing modern birds of prey helped develop a new behavior model for sickle-clawed carnivorous dinosaurs like Velociraptor.

"This study is a real game-changer," said lead author Fowler. "It completely overhauls our perception of these little predatory dinosaurs, changing the way we think about their ecology and evolution."

The study focuses on dromaeosaurids; a group of small predatory dinosaurs that include the famous Velociraptor and its larger relative, Deinonychus. Dromaeosaurids are closely related to birds, and are most famous for possessing an enlarged sickle-claw on digit two (inside toe) of the foot. Previous researchers suggested that this claw was used to slash at prey, or help climb up their hides, but the new study proposes a different behavior.

"Modern hawks and eagles possess a similar enlarged claw on their digit 2's, something that hadn't been noted before we published on it back in 2009," Fowler said. "We showed that the enlarged D-2 claws are used as anchors, latching into the prey, preventing their escape. We interpret the sickle claw of dromaeosaurids as having evolved to do the same thing: latching in, and holding on."

As in modern birds of prey, precise use of the claw is related to relative prey size.

"This strategy is only really needed for prey that are about the same size as the predator; large enough that they might struggle and escape from the feet," Fowler said. "Smaller prey are just squeezed to death, but with large prey all the predator can do is hold on and stop it from escaping, then basically just eat it alive. Dromaeosaurs lack any obvious adaptations for dispatching their victims, so just like hawks and eagles, they probably ate their prey alive too."

Other features of bird of prey feet gave clues as to the functional anatomy of their ancient relatives; toe proportions of dromaeosaurids seemed more suited for grasping than running, and the metatarsus (bones between the ankles and the toes) is more adapted for strength than speed.

"Unlike humans, most dinosaurs and birds only walk on their toes, so the metatarsus forms part of the leg itself," Fowler said. "A long metatarsus lets you take bigger strides to run faster; but in dromaeosaurids, the metatarsus is very short, which is odd."

Fowler thinks that this indicates that Velociraptor and its kin were adapted for a strategy other than simply running after prey.

"When we look at modern birds of prey, a relatively short metatarsus is one feature that gives the bird additional strength in its feet," Fowler continued. "Velociraptor and Deinonychus also have a very short, stout metatarsus, suggesting that they had great strength but wouldn't have been very fast runners."

The ecological implications become especially interesting when dromaeosaurids are contrasted with their closest relatives: a very similar group of small carnivorous dinosaurs called troodontids, Fowler said.

"Troodontids and dromaeosaurids started out looking very similar, but over about 60 million years they evolved in opposite directions, adapting to different niches," Fowler said. "Dromaeosaurids evolved towards stronger, slower feet; suggesting a stealthy ambush predatory strategy, adapted for relatively large prey. By contrast, troodontids evolved a longer metatarsus for speed and a more precise, but weaker grip, suggesting they were swift but probably took relatively smaller prey."

The study also has implications for the next closest relatives of troodontids and dromaeosaurids: birds. An important step in the origin of modern birds was the evolution of the perching foot.

"A grasping foot is present in the closest relatives of birds, but also in the earliest birds like Archaeopteryx," Fowler said. "We suggest that this originally evolved for predation, but would also have been available for use in perching. This is what we call 'exaptation:' a structure evolved originally for one purpose that can later be appropriated for a different use."

The new study proposes that a similar mechanism may be responsible for the evolution of flight.

"When a modern hawk has latched its enlarged claws into its prey, it can no longer use the feet for stabilization and positioning," Fowler said. "Instead the predator flaps its wings so that the prey stays underneath its feet, where it can be pinned down by the predator's bodyweight."

The researchers suggest that this 'stability flapping' uses less energy than flight, making it an intermediate flapping behavior that may be key to understanding how flight evolved.

"The predator's flapping just maintains its position, and does not need to be as powerful or vigorous as full flight would require. Get on top, stay on top; it's not trying to fly away," Fowler said. "We see fully formed wings in exquisitely preserved dromaeosaurid fossils, and from biomechanical studies we can show that they were also able to perform a rudimentary flapping stroke. Most researchers think that they weren't powerful enough to fly; we propose that the less demanding stability flapping would be a viable use for such a wing, and this behavior would be consistent with the unusual adaptations of the feet."

Another group of researchers has proposed that understanding flapping behaviors is key to understanding the evolution of flight, a view with which Fowler agrees.

"If we look at modern birds, we see flapping being used for all sorts of behaviors outside of flight. In our paper, we are formally proposing the 'flapping first' model: where flapping evolved for other behaviors first, and was only later exapted for flight by birds."

The researchers believe their new ideas will open multiple new lines of investigation into dinosaur paleobiology, and the evolution of novel anatomical structures.

"As with other research conducted at the Jack Horner paleo lab, we're looking at old paleontological questions with a fresh perspective, taking a different angle," Fowler said. "Just as you have to get beyond the idea that feet are used just for walking, so we are coming to realize that many unusual structures in modern animals originally evolved for quite different purposes. Revealing the selection pathways that mold and produce these structures helps us to better understand the major evolutionary transitions that shaped life on this planet."

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Dinosaurs with killer claws yield new theory about evolution of flight

New method for enhancing thermal conductivity could cool computer chips, lasers and other devices

The finding was made by a group of engineers headed by Deyu Li, associate professor of mechanical engineering at Vanderbilt University, and published online in the journal Nature Nanotechnology on Dec. 11.

Li and his collaborators discovered that the thermal conductivity of a pair of thin strips of material called boron nanoribbons can be enhanced by up to 45 percent depending on the process that they used to stick the two ribbons together. Although the research was conducted with boron nanoribbons, the results are generally applicable to other thin film materials.

An entirely new way to control thermal effects

"This points at an entirely new way to control thermal effects that is likely to have a significant impact in microelectronics on the design of smart phones and computers, in optoelectronics on the design of lasers and LEDs, and in a number of other fields," said Greg Walker, associate professor of mechanical engineering at Vanderbilt and an expert in thermal transport who was not directly involved in the research.

According to Li, the force that holds the two nanoribbons together is a weak electrostatic attraction called the van der Waals force. (This is the same force that allows the gecko to walk up walls.)

"Traditionally, it is widely believed that the phonons that carry heat are scattered at van der Waals interfaces, which makes the ribbon bundles' thermal conductivity the same as that of each ribbon. What we discovered is in sharp contrast to this classical view. We show that phonons can cross these interfaces without being scattered, which significantly enhances the thermal conductivity," said Li. In addition, the researchers found that they could control the thermal conductivity between a high and a low value by treating the interface of the nanoribbon pairs with different solutions.

The enhancement is completely reversible

One of the remarkable aspects of the effect Li discovered is that it is reversible. For example, when the researchers wetted the interface of a pair of nanoribbons with isopropyl alcohol, pressed them together and let them dry, the thermal conductivity was the same as that of a single nanoribbon. However, when they wetted them with pure alcohol and let them dry, the thermal conductivity was enhanced. Then, when they wetted them with isopropyl alcohol again, the thermal conductivity dropped back to the original low value.

"It is very difficult to tune a fundamental materials property such as thermal conductivity and the demonstrated tunable thermal conductivity makes the research especially interesting," Walker said.

One of the first areas where this new knowledge is likely to be applied is in thermal management of microelectronic devices like computer chips. Today, billions to trillions of transistors are jammed into chips the size of a fingernail. These chips generate so much heat that one of the major factors in their design is to prevent overheating. In fact, heat management is one of the major reasons behind today's multi-core processor designs.

"A better understanding of thermal transport across interfaces is the key to achieving better thermal management of microelectronic devices," Li said.

Discovery may improve design of nanocomposites

Another area where the finding will be important is in the design of "nanocomposites" -- materials made by embedding nanostructure additives such as carbon nanotubes to a host material such as various polymers -- that are being developed for use in flexible electronic devices, structural materials for aerospace vehicles and a variety of other applications.

Collaborators on the study were post-doctoral research associate Juekan Yang, graduate students Yang Yang and Scott Waltermire from Vanderbilt; graduate students Xiaoxia Wu and Youfei Jiang, post-doctoral research associate Timothy Gutu, research assistant professor Haitao Zhang, and Associate Professor Terry T. Xu from the University of North Carolina; Professor Yunfei Chen from the Southeast University in China; Alfred A. Zinn from Lockheed Martin Space Systems Company; and Ravi Prasher from the U.S. Department of Energy.

The research was performed with financial support from the National Science Foundation, Lockheed Martin's Engineering and Technology University Research Initiatives program and the Office of Naval Research.

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New method for enhancing thermal conductivity could cool computer chips, lasers and other devices

The ability to love takes root in earliest infancy

While those attitudes can change with new relationships, introspection, and therapy, in times of stress old patterns often reassert themselves. The mistreated infant becomes the defensive arguer; the baby whose mom was attentive and supportive works through problems, secure in the goodwill of the other person.

This is an "organizational" view of human social development. Explains Simpson: "People find a coherent, adaptive way, as best as they can, to respond to their current environments based on what's happened to them in the past." What happens to you as a baby affects the adult you become: It's not such a new idea for psychology -- but solid evidence for it has been lacking.

Simpson, Collins, and Salvatore have been providing that evidence: investigating the links between mother-infant relationships and later love partnerships as part of the Minnesota Longitudinal Study of Risk and Adaptation. Their subjects are 75 children of low-income mothers whom they've been assessing from birth into their early 30s, including their close friends and romantic partners. When the children were infants, they were put into strange or stressful situations with their mothers to test how securely the pairs were bonded. Since then, the children -- who are now adults -- have returned regularly for assessments of their emotional and social development. The authors have focused on their skills and resilience in working through conflicts with school peers, teenage best friends, and finally, love partners.

Through multiple analyses, the research has yielded evidence of that early encoding -- confirming earlier psychological theories. But their findings depart from their predecessors' ideas, too. "Psychologists started off thinking there was a lot of continuity in a person's traits and behavior over time," says Simpson. "We find a weak but important thread" between the infant in the mother's arms and the 20-year-old in his lover's. But "one thing has struck us over the years: It's often harder to find evidence for stable continuity than for change on many measures."

The good news: "If you can figure out what those old models are and verbalize them," and if you get involved with a committed, trustworthy partner, says Simpson, "you may be able to revise your models and calibrate your behavior differently." Old patterns can be overcome. A betrayed baby can become loyal. An unloved infant can learn to love.

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How granular materials become solid: Discovery may be boon to engineers, manufacturers

In a study out this week in the journal Nature, researchers at Brandeis in collaboration with Duke University explain how granular materials are transformed from a loose state to a solid state when force is applied at a particular angle, in a process known as shearing. "Traditionally people thought of shearing as a mechanism for breaking up materials," says Dapeng Bi, a graduate student in the Martin Fisher School of Physics. "In this case, we find shear actually drives solidification."

Bulbul Chakraborty, the Enid and Nate Ancell Professor of Physics, and Bi, analyzed an experiment performed at Duke which used photo-elastic discs of two different sizes to represent granular materials such as rice or sand. The discs were placed into a plastic box whose shape could be precisely manipulated and measured. The box was illuminated from the bottom, forcing light through the discs. A polarized lens placed on top of the box revealed the photo-elastic discs creating colorful patterns -- called force chains -- caused by the pressure they received when the sides of the box were moved to create a rectangle. Using a computer program the Duke researchers were able to determine the amount of force that was exerted by the discs on each other.

"The polarized light changes the index of refraction of the materials and makes the patterns non-uniform," says Bi. "We then use those numbers to calculate the forces and the geometry of the contact ​network that the discs formed."

The researchers found that when the shape of the box changed due to shear, the discs exhibited a solid state even without the density changing. This, Chakraborty says, is remarkable because usually it is an increase in density that transforms loose material to a solid. "For theorists like us, these experiments are wonderful because we can see exactly what this system is doing," says Chakraborty. "How these patterns change as the discs are pushed and altered gives us information such as how many contacts each grain makes, and the force at every contact."

Chakraborty says that using this data she and Bi constructed a theory that explains how the solid is being formed. "It's possible that if there was no friction between the discs that they would have been able to slide past each other and not get jammed," says Chakraborty. "We now are performing computer simulations to see if shear jamming will occur without friction."

In an abstract written in 2008 in Jamming of Granular Matter, Chakraborty and Robert P. Behringer of Duke University explained that jamming is the extension of the concept of freezing to the transition from a fluid state to a jammed state. Understanding jamming in granular systems, they say, is important from a technological, environmental, and basic science perspective. A jamming of grains in silos can cause catastrophic failures. Avalanches are examples of unjamming, which need to be understood in order to prevent and control, such as the avalanche that killed pro skier Jamie Pierre on November 13, 2011.

Shearing is a major force in nature, explains Chakraborty. When wind blows over the earth, shearing occurs in the sand. Understanding what shear does, she says, is very important.

"We have a very good theoretical framework as to how water behaves, or ice or air," says Chakraborty. "We don't have any fundamental theoretical framework to predict how sand behaves when the wind is blowing fast or slow."

This information could potentially be used to further understand​ things like avalanches and earthquakes and erosion. "Those are effects of shearing of granular materials," says Chakraborty. "What we're trying to do is get at a basic understanding of how sand responds to shear. Most natural forces are shearing forces."

The behavior seen here is similar to "shear thickening," which has been used when manufacturing bulletproof vests that present as a soft material when worn, but hardens upon impact of a bullet.

"The research shows that friction can fundamentally change the nature of granular materials in intriguing ways," says Daryl Hess, program director for condensed matter and materials theory at the National Science Foundation. "Friction and shear reveal the richness of possible states of granular matter, pointing us down a road paved with new discoveries. These may expose deeper connections between jamming and seemingly unrelated phenomena spanning from earthquakes to transformations occurring in other kinds of matter, like water to ice."

In industries where hoppers are used, like loading rice grains onto a truck for example, jamming can be a problem. One possible solution, says Chakraborty, is to change the traditional shape in order to both prevent and break up jams.

"We need these sort of laboratory-based experiments to construct and test theories," says Chakraborty. "Once you get into an industrial situation things are not controlled enough to understand."

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How granular materials become solid: Discovery may be boon to engineers, manufacturers

Alzheimer's drug candidate may be first to prevent disease progression, mouse study suggests

When given to mice with Alzheimer's, the drug, known as J147, improved memory and prevented brain damage caused by the disease. The new compound, developed by scientists at the Salk Institute for Biological Studies, could be tested for treatment of the disease in humans in the near future.

"J147 enhances memory in both normal and Alzheimer's mice and also protects the brain from the loss of synaptic connections," says David Schubert, the head of Salk's Cellular Neurobiology Laboratory, whose team developed the new drug. "No drugs on the market for Alzheimer's have both of these properties."

Although it is yet unknown whether the compound will prove safe and effective in humans, the Salk researchers' say their results suggest the drug may hold potential for treatment of people with Alzheimer's.

As many as 5.4 million Americans suffer from Alzheimer's, according to the National Institutes of Health. More than 16 million will have the disease by 2050, according to Alzheimer's Association estimates, resulting in medical costs of over $1 trillion per year.

The disease causes a steady, irreversible decline in brain function, erasing a person's memory and ability to think clearly until they are unable to perform simple tasks such as eating and talking, and it is ultimately fatal. Alzheimer's is linked to aging and typically appears after age 60, although a small percentage of families carry a genetic risk for earlier onset. Among the top ten causes of death, Alzheimer's is the only one without a way to prevent, cure or slow down disease progression.

Scientists are unclear what causes Alzheimer's, which appears to emerge from a complex mix of genetics, environment and lifestyle factors. So far, the drugs developed to treat the disease, such as Aricept, Razadyne and Exelon, only produce fleeting memory improvements and do nothing to slow the overall course of the disease.

To find a new type of drug, Schubert and his colleagues bucked the trend within the pharmaceutical industry of focusing exclusively on the biological pathways involved in the formation of amyloid plaques, the dense deposits of protein that characterize the disease. To date, Schubert says, all amyloid-based drugs have failed in clinical trials.

Instead, the Salk team developed methods for using living neurons grown in laboratory dishes to test whether or not new synthetic compounds were effective at protecting the brain cells against several pathologies associated with brain aging. Based on the test results from each chemical iteration of the lead compound, which was originally developed for treatment of stroke and traumatic brain injury, they were able to alter its chemical structure to make a much more potent Alzheimer's drug.

"Alzheimer's is a complex disease, but most drug development in the pharmaceutical world has focused on a single aspect of the disease--the amyloid pathway," says Marguerite Prior, a research associate in Schubert's lab, who led the project along with Qi Chen, a former Salk postdoctoral researcher. "In contrast, by testing these compounds in living cell cultures, we can determine what they do against a range of age-related problems and select the best candidate that addresses multiple aspects of the disease, not just one."

With a promising compound in hand, the researchers shifted to testing J147 as an oral medication in mice. Working with Amanda Roberts, a professor of molecular neurosciences at The Scripps Research Institute, they conducted a range of behavioral tests that showed that the drug improved memory in normal rodents.

The Salk researchers went on to show that it prevented cognitive decline in animals with Alzheimer's and that mice and rats treated with the drug produced more of a protein called brain-derived neurotrophic factor (BDNF), a molecule that protects neurons from toxic insults, helps new neurons grow and connect with other brain cells, and is involved in memory formation.

Because of the broad ability of J147 to protect nerve cells, the researchers believe that it may also be effective for treating other neurological disorders, such as Parkinson's disease, Huntington's disease and amyotrophic lateral sclerosis (ALS), as well as stroke.

The research was funded by the Fritz B. Burns Foundation, the National Institutes of Health, the Bundy Foundation and the Alzheimer's Association.

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Alzheimer's drug candidate may be first to prevent disease progression, mouse study suggests

Globalfoundries announces 20-nm chip tape out

MOUNTAIN VIEW, Calif--ARM Holdings plc. and Globalfoundries Inc. have announced the tape out of a 20nm chip and have demoed a Cortex-A9 SoC operating at more than 2.5GHz on 28nm technology.

Globalfoundries said the tape out was a milestone for its Technology Qualification Vehicle (TQV), which it has worked closely on with ARM, and that it was “more than a standard test chip.”

TQV is what Globalfoundries is calling a strategy to develop process technology specifically optimized for ARM Cortex-A series processors.

The fab said each TQV was designed to emulate a full specification SoC and aimed to improve performance, lower power consumption and facilitate a faster path to market for its customers.

Mojy Chian, senior vice president of design enablement at Globalfoundries said it was clear the firm’s TQV strategy was “paying dividends” at 32-nm and 28-nm HKMG technology by delivering on its goals for performance and energy efficiency.

Chian added that the fab would continue to work closely with ARM on TQV “as an integral part of 20nm process technology development” allowing customers to ramp more rapidly to next-generation designs based on ARM Cortex-A series processors in high-volume production.

Globalfoundries has said its 20-nm platform is designed to improve performance by up to 35 percent and almost halve power consumption compared with its 28nm technologies.

As to the firm’s 2.5GHz performance on 28-nm, Globalfoundries said the result had been achieved at the company’s Dresden, Germany fab on its high performance offerings. A further performance increase is expected on the firm’s 28nm High Performance Plus (HPP) platform targeted at the wired networking applications market, owing to its low active power and an operating point of 0.85V.

Analysts have said the announcement is a positive sign from Globalfoundries in a year that has been both difficult and turbulent for the firm.

“It’s a good proof point that they are moving forward for other customers, but they still need to answer the doubts about being able to handle their existing issues with existing customers,” said InStat’s Jim McGregor.
Globalfoundries announces 20-nm chip tape out

Disaster looms for gas cloud falling into Milky Way's central black hole

Many, if not all, galaxies have massive black holes at their centers. But this supermassive black hole is the only one close enough for astronomers to study in detail, so the violent encounter is a unique chance to observe what until now has only been theorized: how a black hole gulps gas, dust and stars as it grows ever bigger.

"When we look at the black holes in the centers of other galaxies, we see them get bright and then fade, but we never know what is actually happening," said Eliot Quataert, a theoretical astrophysicist and University of California, Berkeley professor of astronomy. "This is an unprecedented opportunity to obtain unique observations and insight into the processes that go on as gas falls into a black hole, heats up and emits light. It's a neat window onto a black hole that's actually capturing gas as it spirals in."

"The next two years will be very interesting and should provide us with extremely valuable information on the behavior of matter around such massive objects, and its ultimate fate," said Reinhard Genzel, professor of physics at both UC Berkeley and the Max Planck Institute for Extraterrestrial Physics (MPE) in Garching, Germany.

The discovery by Genzel; Stefan Gillessen of the MPE; Quataert and colleagues from Germany, Chile and Illinois will be reported online on Dec. 14, in advance of the Jan. 5 publication of the news in the British journal Nature.

Since 2008. Genzel, Gillessen, Quataert and their team have seen the gas cloud about three times the mass of Earth speeding up as it has fallen deeper into the gravitational whirlpool of the black hole. Its edges are already beginning to fray.

"It is not going to survive the experience," said first author Gillessen. He built the infrared detector on the European Southern Observatory's Very Large Telescope in Chile used to observe the movement of stars and gas in the center of the Milky Way, 27,000 light years from Earth.

By 2013, scientists should see outbursts of X-rays and radio waves as the cloud -- composed mostly hydrogen and helium gas gets hotter and is torn asunder. The light emitted around the black hole could increase by a hundredfold to a thousandfold, Quataert calculated.

The Chandra X-ray satellite has already scheduled its largest single chunk of observation time in 2012 near the Milky Way's central black hole.

Black hole normally quiet

Astronomers have long observed clouds of gas streaming toward the center of our Milky Way Galaxy, presumably destined to fall into the 4.3 million solar-mass black hole lurking there. But this black hole "has a surprisingly low amount of matter falling inward at the moment," Quataert said.

Since MPE astronomers began observing the black hole in 1992, they have seen only two stars as close as this gas cloud to the black hole. The crucial difference is that those stars "passed unharmed through their closest approach, (while) the gas cloud will be completely ripped apart by the tidal forces around the black hole," Gillessen said.

This particular cold cloud (about 550 Kelvin or 280 degrees Celsius) may have formed when gas pushed by stellar winds from two nearby stars collided, and is glowing under the strong ultraviolet radiation from surrounding hot stars. As the cloud skirts the gravitational influence of the black hole, it will come within about 40 billion kilometers ‑ 250 times the distance between Earth and the sun ‑ of the event horizon, the limit beyond which nothing, not even light, can escape.

Even at that distance, the gas will get stretched out, with probably half spiraling into the black hole and the rest flung outward.

As the cloud falls towards the black hole -- its current velocity is about 2,350 kilometers per second, twice what it was seven years ago -- it will interact with the hot gas present in the accretion flow around the black hole and become disrupted by turbulent interaction.

Thanks to the Very Large Telescope's years of observations of the black hole at many different wavelengths, the scientists were able simulate the time evolution of the cloud and predict that the temperature of the gas cloud should increase rapidly to several million Kelvin near the black hole, dramatically increasing X-ray emissions.

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Disaster looms for gas cloud falling into Milky Way's central black hole

'Supernova of a generation' shows its stuff: Astronomers determine how brightest and closest stellar explosion in 25 years happened

"What caused these explosions has divided the astronomical community deeply," says Shri Kulkarni, the John D. and Catherine T. MacArthur Professor of Astronomy and Planetary Sciences. But this new supernova -- dubbed SN2011fe -- can help astronomers solve this longstanding mystery. "SN2011fe is like the Rosetta Stone of Type Ia supernovae," says Kulkarni, who is also the principal investigator on the Palomar Transient Factory (PTF). Led by the California Institute of Technology (Caltech), the PTF is designed to survey the skies for transient flashes of light that last for a few days or months, such as those emitted by exploding stars.

On August 24, the PTF team discovered the supernova in one of the arms of the Pinwheel Galaxy (also called M101), 21 million light years away. They caught the supernova just 11 hours after it exploded.

"Never before have we seen a stellar thermonuclear explosion so soon after it happened," says Lars Bildsten, professor of theoretical astrophysics at the Kavli Institute for Theoretical Physics at UC Santa Barbara, and member of the PTF team, which described its supernova findings in the December 15 issue of the journal Nature.

The PTF team uses an automated system to search for supernovae, and because they were able to point their telescopes at SN2011fe so quickly after its detonation, the astronomers were able to put together a blow-by-blow analysis of the explosion, determining that the supernova involves a dense, Earth-sized object called a white dwarf and, most likely, a main-sequence star (a star in the main stage of its life).

Scientists have long suspected that Type Ia supernovae involve a binary system of two stars in orbit around each other, with one of those stars being a white dwarf. The white dwarf, which is made out of carbon and oxygen, explodes when matter from its companion star spills over onto its surface. But no one is sure what kind of star the companion is. Scientists have suggested that it's another white dwarf, a main-sequence star, a helium star, or a star in a late life stage that's puffed up into a red giant.

Still, because the explosion always involves a white dwarf, its overall brightness and behavior is relatively predictable, making it a useful tool for measuring distances. Since all Type Ia supernovae produce about the same amount of light, those that appear dimmer must be farther away. In this way, by measuring the brightness of supernovae, astronomers can use them as cosmic meter sticks to determine the size of the universe -- and how fast it's expanding. In fact, the work that earned the 2011 Nobel Prize in physics -- the discovery that expansion of the universe is speeding up -- was based on observations using Type Ia supernovae.

"This discovery is exciting because the supernova's infancy and proximity allows us to directly see what the progenitor system is," explains Mansi Kasliwal, an astronomer at the Carnegie Institution for Science who is a recent Caltech doctoral graduate and a coauthor on the paper. "We have expected for a while that a Type Ia supernova involves a carbon-oxygen white dwarf, but now we have direct evidence."

In the case of SN2011fe, the researchers were also able to deduce, by process of elimination, that the companion star is most likely a main-sequence star. How do they know?

If the companion was a red giant, the explosion of the white dwarf would send a shock wave through the red giant, heating it. This scenario would have generated several tens of times more light than the astronomers observed. Additionally, it happens that the Hubble Space Telescope took images of the location where SN2011fe lived before it blew up. When the researchers looked at the data, they found no evidence of red giants or helium stars.

If the companion was another white dwarf, the interactions between the companion and the explosion would produce light in the optical and ultraviolet wavelengths. Since none of this sort of radiation was seen coming from SN2011fe, it is less likely that the companion was a white dwarf.

These results -- which they describe in a companion paper in the same issue of Nature -- along with X-ray and radio observations that also fail to see any evidence for red giants or helium stars, rule those out as the companion. Caltech postdoc Assaf Horesh is the lead author on the paper describing the X-ray and radio data, which will be published in The Astrophysical Journal.

The astronomers have also observed, in unprecedented detail, the material that's blown off during the explosion. In particular, the team detected oxygen hurtling out from the supernova at speeds of over 20,000 kilometers per second -- the first time anyone has seen high-speed oxygen coming from a Type Ia supernova, according to the researchers. "These observations probe the thin, outermost layers of the explosion," Bildsten says. "These are the parts that are moving the fastest, for which we have never been able to see this mix of atomic elements."

Not only was the supernova detected quickly, but the data processing -- performed by researchers led by Peter Nugent, staff scientist at Lawrence Berkeley National Laboratory -- was also done within hours. The machine-learning algorithms developed by Joshua Bloom, an associate professor at UC Berkeley, also helped make the fast find possible. And because the astronomers caught the blast so soon after it ignited, and because it's so close, the researchers say SN2011fe will become one of the best-studied supernovae ever.

"The rapid discovery and classification of SN2011fe -- all on the same night -- is a testament to the great teamwork between all the researchers from over a half a dozen institutions," Kulkarni says. "The future looks very bright. Soon we should be finding supernovae at an even younger age and thereby better understand how these explosions happen."

Nugent is the lead author on the Nature paper, which is titled, "Supernova 2011fe from an exploding carbon-oxygen white dwarf star." The lead author on the companion paper, "Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe," is Weidong Li of UC Berkeley. The Astrophysical Journal paper is titled, "Early radio and X-ray observations of the youngest nearby type Ia supernova PTF11kly (SN 2011fe)."

The Palomar Transient Factory (PTF) uses the 48-inch Oschin Schmidt telescope and the 60-inch telescope of the Palomar Observatory of Caltech for its observations and is a collaboration between Caltech, Columbia University, Las Cumbres Observatory Global Telescope, Lawrence Berkeley National Laboratory, Oxford University, UC Berkeley, and the Weizmann Institute of Science.

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'Supernova of a generation' shows its stuff: Astronomers determine how brightest and closest stellar explosion in 25 years happened

The 'supernova of a generation' shows its stuff

"What caused these explosions has divided the astronomical community deeply," says Shri Kulkarni, the John D. and Catherine T. MacArthur Professor of Astronomy and Planetary Sciences. But this new supernova -- dubbed SN2011fe -- can help astronomers solve this longstanding mystery. "SN2011fe is like the Rosetta Stone of Type Ia supernovae," says Kulkarni, who is also the principal investigator on the Palomar Transient Factory (PTF). Led by the California Institute of Technology (Caltech), the PTF is designed to survey the skies for transient flashes of light that last for a few days or months, such as those emitted by exploding stars.

On August 24, the PTF team discovered the supernova in one of the arms of the Pinwheel Galaxy (also called M101), 21 million light years away. They caught the supernova just 11 hours after it exploded.

"Never before have we seen a stellar thermonuclear explosion so soon after it happened," says Lars Bildsten, professor of theoretical astrophysics at the Kavli Institute for Theoretical Physics at UC Santa Barbara, and member of the PTF team, which described its supernova findings in the December 15 issue of the journal Nature.

The PTF team uses an automated system to search for supernovae, and because they were able to point their telescopes at SN2011fe so quickly after its detonation, the astronomers were able to put together a blow-by-blow analysis of the explosion, determining that the supernova involves a dense, Earth-sized object called a white dwarf and, most likely, a main-sequence star (a star in the main stage of its life).

Scientists have long suspected that Type Ia supernovae involve a binary system of two stars in orbit around each other, with one of those stars being a white dwarf. The white dwarf, which is made out of carbon and oxygen, explodes when matter from its companion star spills over onto its surface. But no one is sure what kind of star the companion is. Scientists have suggested that it's another white dwarf, a main-sequence star, a helium star, or a star in a late life stage that's puffed up into a red giant.

Still, because the explosion always involves a white dwarf, its overall brightness and behavior is relatively predictable, making it a useful tool for measuring distances. Since all Type Ia supernovae produce about the same amount of light, those that appear dimmer must be farther away. In this way, by measuring the brightness of supernovae, astronomers can use them as cosmic meter sticks to determine the size of the universe -- and how fast it's expanding. In fact, the work that earned the 2011 Nobel Prize in physics -- the discovery that expansion of the universe is speeding up -- was based on observations using Type Ia supernovae.

"This discovery is exciting because the supernova's infancy and proximity allows us to directly see what the progenitor system is," explains Mansi Kasliwal, an astronomer at the Carnegie Institution for Science who is a recent Caltech doctoral graduate and a coauthor on the paper. "We have expected for a while that a Type Ia supernova involves a carbon-oxygen white dwarf, but now we have direct evidence."

In the case of SN2011fe, the researchers were also able to deduce, by process of elimination, that the companion star is most likely a main-sequence star. How do they know?

If the companion was a red giant, the explosion of the white dwarf would send a shock wave through the red giant, heating it. This scenario would have generated several tens of times more light than the astronomers observed. Additionally, it happens that the Hubble Space Telescope took images of the location where SN2011fe lived before it blew up. When the researchers looked at the data, they found no evidence of red giants or helium stars.

If the companion was another white dwarf, the interactions between the companion and the explosion would produce light in the optical and ultraviolet wavelengths. Since none of this sort of radiation was seen coming from SN2011fe, it is less likely that the companion was a white dwarf.

These results -- which they describe in a companion paper in the same issue of Nature -- along with X-ray and radio observations that also fail to see any evidence for red giants or helium stars, rule those out as the companion. Caltech postdoc Assaf Horesh is the lead author on the paper describing the X-ray and radio data, which will be published in The Astrophysical Journal.

The astronomers have also observed, in unprecedented detail, the material that's blown off during the explosion. In particular, the team detected oxygen hurtling out from the supernova at speeds of over 20,000 kilometers per second -- the first time anyone has seen high-speed oxygen coming from a Type Ia supernova, according to the researchers. "These observations probe the thin, outermost layers of the explosion," Bildsten says. "These are the parts that are moving the fastest, for which we have never been able to see this mix of atomic elements."

Not only was the supernova detected quickly, but the data processing -- performed by researchers led by Peter Nugent, staff scientist at Lawrence Berkeley National Laboratory -- was also done within hours. The machine-learning algorithms developed by Joshua Bloom, an associate professor at UC Berkeley, also helped make the fast find possible. And because the astronomers caught the blast so soon after it ignited, and because it's so close, the researchers say SN2011fe will become one of the best-studied supernovae ever.

"The rapid discovery and classification of SN2011fe -- all on the same night -- is a testament to the great teamwork between all the researchers from over a half a dozen institutions," Kulkarni says. "The future looks very bright. Soon we should be finding supernovae at an even younger age and thereby better understand how these explosions happen."

Nugent is the lead author on the Nature paper, which is titled, "Supernova 2011fe from an exploding carbon-oxygen white dwarf star." The lead author on the companion paper, "Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe," is Weidong Li of UC Berkeley. The Astrophysical Journal paper is titled, "Early radio and X-ray observations of the youngest nearby type Ia supernova PTF11kly (SN 2011fe)."

The Palomar Transient Factory (PTF) uses the 48-inch Oschin Schmidt telescope and the 60-inch telescope of the Palomar Observatory of Caltech for its observations and is a collaboration between Caltech, Columbia University, Las Cumbres Observatory Global Telescope, Lawrence Berkeley National Laboratory, Oxford University, UC Berkeley, and the Weizmann Institute of Science.

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The 'supernova of a generation' shows its stuff

Qualcomm becomes Imagination Technologies licensee

MOUNTAIN VIEW, Calif--Qualcomm Inc. has become a new Imagination Technologies licensee, along with MStar, Ricoh and Rockchip, joining existing partners like Sony, Intel, Mediatek, Renesas, Samsung, Sigma and Realtek.

Imagination Technologies confirmed that Qualcomm was licensing the display IP from its PowerVR portfolio.
Several months back, Wall Street pundits were speculating that Qualcomm might be readying itself to make an investment in Imagination’s GPU solution for use with Windows 8 devices.

Qualcomm has its own mobile graphics unit, and Adreno GPUs, purchased from AMD several years ago, but has been slow to integrate the offering in any meaningful way. Analysts posited that Qualcomm could invest in Imagination’s Rogue technology instead, in order to better capitalize on Windows 8 momentum, while continuing to work on its own graphics at a slower pace.

Imagination’s Rogue graphics supports a higher class of DX than Adreno, which only supports DX9, a technology soon to be two generations old.

While DX9 will work on Windows 8, it’s widely felt that users would have a better visual experience on devices supporting a higher class of DX, like Rogue which purports to support from DirectX 10 up to DirectX 11.

Imagination is one of very few companies that has the experience of delivering DirectX for SoCs, encompasses both 3D graphics capabilities and a variety of video playback features.

Qualcomm rival Texas Instruments is already licensing Imagination’s PowerVR core for future OMAP system-on-a-chip products to use with Windows 8, and Nvidia supports DX11 on its Tegra chips, meaning that Qualcomm desperately needs to up its graphical game in order to stay at the front of the mobile processing pack.

If Qualcomm were to license Imagination’s graphics technology, it would also mean that the British firm’s GPU would become the most widely adopted graphics offering for Windows 8 devices. It would also be a blow to ARM, which has been trying to license its Mali graphics IP to partners, with little success.

Currently, however, there is no solid indication that Qualcomm will be taking its license any further than simply display IP, though an Imagination spokesman said his firm now had “high hopes.”

“We really like them as a customer, we’re delighted to have Qualcomm’s business and hope it leads to something more. At least they’re a customer now,” he said.
Qualcomm becomes Imagination Technologies licensee

Broadcom raises fourth quarter revenue guidance


LONDON – Wireless and broadband fabless chip company Broadcom Corp. has raised its financial guidance for the fourth quarter of 2011. The company has increased it net revenue guidance to high-end of the previous range to approximately $1.8 billion.

"Broadcom's Q4 is coming in stronger than expected driven by solid shipments and tight operational management," said Scott McGregor, CEO of Broadcom, in a statement.

Broadcom's raised guidance differs from many other companies' behavior including Intel, Texas Instruments, Altera, FormFactor, Sequans, which have all lowered guidance often citing weak demand. Nonetheless Broadcom's net revenue is forecast to show a sequential decline from $1.96 billion in the third quarter of 2011.


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Follow your nose: Compared to Neanderthals, modern humans have a better sense of smell

In a study published this week by Nature Communications, led by Markus Bastir and Antonio Rosas, of the Spanish Natural Science Museum (CSIC), high-tech medical imaging techniques were used to access internal structures of fossil human skulls. The researchers used sophisticated 3D methods to quantify the shape of the basal brain as reflected in the morphology of the skeletal cranial base. Their findings reveal that the human temporal lobes, involved in language, memory and social functions as well as the olfactory bulbs are relatively larger in Homo sapiens than in Neanderthals. "The structures which receive olfactory input are approximately 12% larger in modern humans than in Neanderthals," the authors explain.

These findings may have important implications for olfactory capacity and human behaviour. In modern humans the size of the olfactory bulbs is related to the capacity of detection and discrimination of different smells. Olfaction is among the oldest sense in vertebrates. "Also, it is the only one that establishes a direct connection between the brain and its environment," says Markus Bastir, the lead author of the study. While other senses must pass through different cortical filters, olfaction goes from the environment right into the highest centres of the brain. What is more, "olfaction never sleeps," adds Antonio Rosas, "because we always breathe and perceive smells." The neuronal circuitry of olfaction coincides with that of memory and emotion (the limbic system), "which explains the enormous memory retention and vital intensity of olfaction-mediated life events."

Researchers at the Max Planck Institute for Evolutionary Anthropology in Leipzig, who also contributed to the current publication, could recently show differences in the patterns of brain development between modern humans and Neanderthals during a critical phase for cognitive development. "In the first year of life the brains of Neanderthals and modern humans develop differently," says Philipp Gunz from the Max Planck Institute of Evolutionary Anthropology in Leipzig. "Modern humans have smaller faces and smaller noses than their Neanderthal cousins. However, the part of the brain that processes smells, is bigger in modern humans than in Neanderthals." "Evidence is accumulating that Neanderthals and modern humans independently evolved large brains and that their brains might have worked differently. Our new study offers a glimpse into the functional significance of these developmental differences," adds Jean-Jacques Hublin, who heads the Department of Human Evolution at the Max Planck Institute of Evolutionary Anthropology in Leipzig.

Olfactory information projects to brain regions directly responsible for processing of emotion, motivation, fear, memory, pleasure and also attraction. Neuroscientists have coined the term "higher olfactory functions" to describe those brain functions which combine cognition (memory, intuition, perception, judgment) and olfaction. The greater olfactory bulbs and relatively larger temporal lobes in H. sapiens compared to any other human species may point towards improved and different olfactory sense possibly related to the evolution of behavioural aspects and social functions.

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Follow your nose: Compared to Neanderthals, modern humans have a better sense of smell

2011-12-14

Report: TSMC reserves land for 450-mm fab


LONDON – A 50-hectare (about 120 acres) plot of land is being appropriated by the Central Taiwan Science Park in Taichung, Taiwan, on which foundry Taiwan Semiconductor Manufacturing Co. Ltd. (TSMC) could build a 450-mm wafer fab, according a Taiwan Economic News report.

The report added that the projected cost of the 450-mm wafer fab would involve an investment exceeding NT800 billion (about $26 billion), or nearly three times the cost of TSMC's Fab 15 Gigafab currently being built on the science park.

The report referenced TSMC as saying Tuesday (Dec. 12) that the earliest it would start building the fab would be 2015 to 2016 but that once the 450-mm diameter wafer size becomes mainstream it planned to also build 450-mm wafer fabs in Hsinchu and Tainan.

TSMC is expected to bring up 450-mm wafer processing at two of its established wafer fabs, built for 300-mm wafer processing, before building a dedicated 450-mm wafer fab.

A 450-mm pilot line is expected to go into Fab 12 in Hsinchu, Taiwan and be running the 20-nm process technology node by 2013 to 2014. Following that TSMC plans to bring up 450-mm volume production within Fab 15 on the Central Taiwan Science Park in Taichung. This would process devices at the 14-nm node, the node at which TSMC is expected to switch from planar transistors in bulk CMOS to FinFET structures.http://cms.eetimes.com/ContentCreator/SelectContentItemType


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Redpine tips Gbit/s Wi-Fi design

SAN JOSE, Calif. – Redpine Signals, Inc. completed the design of a low power Wi-Fi block based on the 802.11ac standard that supports up to a Gbit/second of throughput over 5 GHz spectrum. The Quali-Fi block uses approximately the same amount of power as its previous 802.11n design, the company claims.

Redpine (San Jose) will license the technology to one mobile applications processor vendor, the company's third licensing deal in ten years following agreements with Portal Player and Infineon. It also will embed the block in its own multi-mode wireless chip slated for mid-2012.

The new block can support MIMO (multiple input, multiple output) antennas in configurations ranging from 1x1 to 3x3. It dissipates less than 1 milliwatt in standby mode and has been implemented both as an FPGA and ASIC.

Venkat Mattela, chief executive of Redpine, said he expects companies to start volume shipments of .11ac chips probably late in 2012. One startup recently started limited sampling of its .11ac design.

Analysts and vendors expect .11ac, will become the next iteration of Wi-Fi. It is being implemented in combo chips that also support .11n and are now starting to sample with production expected next year.


Redpine tips Gbit/s Wi-Fi design

Intel weakness not just about HDDs, says Nomura


LONDON – Investment broker Nomura Equity Research reckons the $1 billion that Intel shaved off its forecast for its 4Q11 sales revenue is about more than just a shortage of hard disk drives hurting PC sales and thereby Intel's sales of microprocessors.

Nomura has reduced its own estimate of Intel's 4Q11 sales by $800 million to the same figure as Intel; $13.7 billion. But it does not see the hard disk drive situation being as being the only reason that the reduction is requred.

In a note to clients entitled: Intel finally blows up and subtitled: Change in outlook may highlight issues beyond HDDs, Nomura said that problems at Intel are based on a wider set of challenges. "HDD shortages are a concern, but we think weak sell-through is also contributing to the $1 billion shortfall. We see softness in China, continued demand for ARM-based more power-efficient devices, and low volumes for ultrabooks," the note said.

In other words demand for PCs and ultrabooks is weak, but demand for ARM-based processors to go in smartphones and tablet computers is high. The ultrabook is Intel's favored form factor that it hopes will take market share from tablet computers just as tablet computers have taken market share from the notebook computer and killed the netbook at birth.

Nor does Nomura hold out much hope for Intel in the first half of 2012. "We would not be surprised to see below-seasonal growth in Q1 and Q2 given lack of PC catalysts (Windows 8 likely Q3 event), increasing ASP pressure, and slowing China and Europe," the report said.

As a result Nomura has cut its forecast for Intel sales revenue in 2012 by $3 billion to $53.4 billion, which would be a fall from its estimate for Intel's 2011 sales revenue of $53.8 billion.


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Intel, Inside make NFC deal


LONDON – Inside Secure SA, a fabless supplier of near field communications (NFC) chips, has signed a technology transfer agreement to provide Intel Corp. with NFC designs and technologies.

The agreement has a five-year term and gives Intel access to Inside's software, firmware and core hardware technology for development of future Intel products. In addition, Inside will provide Intel’s Mobile Wireless Group with access to scalable NFC solutions based on Inside's MicroRead, SecuRead and Open NFC products.

Intel recently upgraded its membership of the NFC Forum to take on a seat on its board of directors and now has the right to integrate Inside's technology within its SoCs.

Remy de Tonnac, CEO of Inside (Aix-en-Provence, France), said his company would make money out of the deal by way of licensing payments, royalties and development contracts with Intel but declined to say how much the deal might be worth to Inside. "It's no secret that it [NFC technology] will go into PCs and other mobile products such as smartphones and tablets."

While Intel will have the right to develop and integrate Inside's technology into its SoCs the deal is non-exclusive, allowing Inside to cut a similar deal with another company, and Inside will also continue to sell stand-alone NFC chips, de Tonnac said. "The industry has debated how and when NFC integration should happen, but both patterns will co-exist for some time."

"We are building a partnership with Intel," said de Tonnac.
Next: Going to smaller geometry
Intel, Inside make NFC deal

2011-08-10

New Enterprise Associates, Lithium-Ion Battery, Leyden Energy, Battery Battery developer Leyden Energy recharges with $20M

Battery technology developers continue to attract venture funding.

Among them is Leyden Energy Inc. (Fremont, Calif.), which recently announced Series B funding totaling $20 million. The round was led by New Enterprise Associates (Menlo Park, Calif.) along with current investors Lightspeed Ventures, Sigma Partners and Walden Capital.

Leyden said it will use it latest infusion of capital to add manufacturing capacity for its next-generation lithium-ion batteries as well as for future development of advanced battery technologies. The production boost is tied to growing demand from customers in the "smaller consumer electronics sector," the company said.

Leyden's core technology includes thermal properties that address shortfalls in Li-ion battery performance at high temperatures. Chemical reactions in batteries speed up at high temperature, degrading performance and reducing the number of charging cycles. The company said it is offering a three-year warranty on its Li-ion batteries as compared to a standard one-year warranty.

“Market demand for high-performance, long-lasting batteries in consumer electronics is growing," Leyden Energy CEO Aakar Patel said in a statement.

The company also said Ron Bernal of New Enterprise Associates will  join its board of directors. “What [Leyden] has introduced is really an energy storage platform that can be applied to a number of different product markets in order to increase the value that those applications bring to end customers," Bernal said in a statement.

Along with consumer electronics, Leyden Energy is also targeting the electric vehicle, smart grid and backup storage markets.
New Enterprise Associates, Lithium-Ion Battery, Leyden Energy, Battery Battery developer Leyden Energy recharges with $20M