October 2009 Archives

WSJ.com: The H1-B visa program that feeds skilled workers to top-tier US technology companies and universities is on track to leave thousands of spots unfilled for the first time since 2003, a sign of how the weak economy has eroded employment even among highly trained professionals.

Last year, even as the recession began to bite, employers snapped up the 65,000 visas available in just one day. This year, however, as of 25 September—nearly six months after the US government began accepting applications—only 46,700 petitions had been filed.

In addition to the weak economy, companies have curbed applications in the face of rising costs associated with hiring foreign-born workers.

While the number of visa holders is small compared with the US work force, their contribution is huge, employers say. For example, last year 35% of Microsoft's patent applications in the US came from new inventions by visa and green-card holders, according to company general counsel Brad Smith.

The first global map

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BBC news: Drawn half a millennium ago and then swiftly forgotten, one map made us see the world as we know it today... and helped name America. But, as BBC news reporter Toby Lester discovered, the first map that outlined the continents of the world as we know them today, also named America based on a pun.

early world maps_4.jpg
In late May 2003 the Library of Congress bought the only surviving copy of Martin Waldseemüller's monumental 1507 world map for $10 million (image credit: Library of Congress).


Related Link
The Map that named America

Wired.com: A cell in the eye may be worth two in the beak, at least when it comes to a migratory bird's magnetic compass.

180px-Robinwithfly.jpgIn European robins (right image), a visual center in the brain and light-sensing cells in the eye—not magnetic sensing cells in the beak—allow the songbirds to sense which direction is north and migrate correctly, a new study finds. The study published in Nature, may improve conservation efforts for migratory birds.

Related Link
Visual but not trigeminal mediation of magnetic compass information in a migratory bird

The Daily Telegraph: UK academics are calling on members of the public to use their mobile phones to record their local soundscape and send them the results.
 
It is hoped that the clips will then make up a detailed acoustic map of the noise environment around the country and help offset the growing menace of noise pollution.

The project—which will make the raw acoustic data available on the web—aims to get a better idea of why some sounds add to the atmosphere of a place and others detract and cause annoyance.

Nature: Forty years ago today the first message was sent between computers on the ARPANET. Vinton G. Cerf, who was a principal programmer on the project, reflects on how our online world was shaped by its innovative origins.

NPR: The NASA swift satellite has discovered the most distant γ-ray burst seen and the earliest astronomical object ever observed in cosmic history.

Two teams of scientists made the discovery, which they report in Nature.

Related Links
Astronomers detect most distant object ever seen

Related Nature Links
Most distant cosmic blast seen
A γ-ray burst at a redshift of z ≈ 8.2
An intergalactic race in space and time
GRB 090423 at a redshift of z ≈ 8.1

QinetiQ chief resigns

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guardian.co.uk: The chief executive of defense research technology firm QinetiQ has quit the company just hours after it was criticized by the official report into a 2006 Nimrod plane crash in Afghanistan, which claimed 14 lives.

Graham Love, who has run the company for the last four years, is departing on 30 November. His replacement, Leo Quinn, is the former chief executive of bank-note maker DeLaRue.

"We have been looking at succession planning for over a year," a company spokesman said. "[It is] mistaken to directly link the two events."

Science: The blogosphere has been having a field day with global warming's apparent decade-long stagnation. Negotiators are working toward an international global warming agreement to be signed in Copenhagen in December, yet there hasn't been any warming for a decade. What's the point, bloggers ask?

Climate researchers are beginning to answer back in their preferred venue, the peer-reviewed literature. The pause in warming is real enough, but it's just temporary, they argue from their analyses. A natural swing in climate to the cool side has been holding greenhouse warming back, and such swings don't last forever. "In the end, global warming will prevail," says climate scientist Gavin Schmidt of NASA's Goddard Institute for Space Studies (GISS) in New York City.

latimes.com: A big earthquake and resultant fire could trigger potentially deadly releases of radioactive materials from Los Alamos National Laboratory in New Mexico due to "major deficiencies" in the nuclear weapons lab's safety planning, federal safety experts warned Tuesday.

The warning from the Defense Nuclear Facilities Safety Board was sent to Energy Secretary Steven Chu, urging him to "execute both immediate and long-term actions."

The Daily Telegraph: A team of fluid dynamics experts have worked out what causes the so-called "teapot effect" and have come up with a way to put an end to it.

800px-A_tea_pot.jpgThey have deduced that at low pouring speeds tea starts to stick to the inside of the spout, causing the flow to momentarily stop and then start again—in other words to dribble.
 
By reducing the friction between the spout and the fluid, the dribble can be all but be eradicated even towards the end of a pour, claim the scientists at the University of Lyon in France.

Science: For the past 5 years, Jerry Nelson and his colleagues at University of California have been working on plans for the Thirty Meter Telescope (TMT)—whose primary mirror will be a glinting mosaic of 492 hexagonal segments.

tmt_primary_mirror.jpg
An artist's concept showing the segmented primary mirror, which has 492 hexagonal segments arranged into an f/1 hyperboloidal mirror (credit: TMT)

Meanwhile, Roger Angel and his collaborators have set their sights on building the Giant Magellan Telescope (GMTO)—whose seven monolithic 8.4-meter mirrors, arranged like flower petals, will function as a primary mirror 24.5 meters in diameter.

gmtdaytimemedium.jpg
Artist's concept showing the seven 8.4-meter mirrors. (credit: GMTO)

If the telescopes are built—TMT on Mauna Kea in Hawaii, GMT at Las Campanas—each will capture images up to 10 times sharper than today's best ground-based telescopes.

Both will shoot for the same scientific goals, looking at the first stars and galaxies, studying the formation of planets and stars, the growth of black holes, and probe the nature of dark matter and dark energy. And both will cost between $700 million and $1 billion.

So far, neither telescope has come close to securing the total funding it needs, and if they are built with little federal support, the National Science Foundation would be hard pressed to provide the operating and maintenance costs.

Given the funding challenges, some astronomers say the two sides should join forces to build one telescope to rival the European Southern Observatory's proposed 42-meter segmented-mirror telescope, the European Extremely Large Telescope.

Storage ring dust-up

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Physical Review Focus: High-energy physicists have finally pinpointed their dust problem. Inside multi-million dollar storage rings, high-speed trains of electrons are often derailed by micron-sized specks of dust. Now a team has shown that dust grains arise from sparks inside a Japanese storage ring, the KEK Photon Factory Advanced Ring as they report in an upcoming paper in Physical Review Special Topics--Accelerators and Beams.

The team also caught on video, one of the tiny grains being swept along in the electron beam. The brief flashes of dust trapped in an invisible electron beam begin about halfway through the 10-second video.

Video courtesy of Y. Tanimoto, KEK.

Various: The launch of NASA's first new rocket in 25 years earlier today has given NASA a welcome boost while the agency grapples with a revised strategy for returning to the Moon and onto Mars under tighter budget conditions.

ares1x_launch.jpg
Above is the Ares I-X test rocket taking off from Launch Complex 39B at NASA's Kennedy Space Center in Florida. Liftoff occurred at 11:30 am. EDT. Credit: NASA/Jim Grossman

The Ares I-X test flight saw the first stage solid rocket boosters taking the vehicle to an altitude of 40km. The booster stage then parachuted down into the Atlantic for recovery, while the dummy second stage crashes into the ocean.

"It is a chance for the agency to remind itself what it takes to build a vehicle," said Robert Less, Ares I-X mission manager to the BBC.

The first stage is a highly modified version of a space shuttle rocket booster.

ares_mission_profile.jpg
The Ares I-X mission profile, Image credit: NASA.

The recent Augustine Panel that looked at manned spaceflight even questioned whether Ares I is the right vehicle for the job. NASA says Ares I will be ready in 2015, others told the panel it will be longer.

The Ares I-X was rolled to the launch pad early last week.

Space.com's Jeremy Hsu goes behind the scenes of Ares I-X booster and visits the group that built it.

It represents the culmination of years of work by the rocket-minded ATK Space Systems in Utah and almost 1,000 other NASA workers and private contractors across 17 states.

To ensure that they see the fruits of their labor, technicians have installed more than 700 sensors on the $445 million Ares I-X test vehicle.

It may be the only visible success of the program says New York Times reporter Kenneth Chang.

"Critics of the Ares I, which is part of NASA’s Constellation program intended to return astronauts to the Moon by 2020, have described it as too expensive, underpowered and technically flawed."

Thestar.com: What do Canada Post and the Mars Rover have in common with mammograms and video games? All use image sensors designed and made by the Canadian company DALSA Corp.

DALSA Corp was set up by Savvas Chamberlain, who also created the first microelectronics lab at the University of Waterloo in Canada shortly after the charge-coupled device was invented by Willard Boyle and George Smith in 1969.

Forty years later, Boyle and Smith were awarded the Nobel Prize for Physics.

Meanwhile, Chamberlain has built his company into a global leader in high-performance imaging, with 1000 employees worldwide and revenues of more than $200 million annually.

The Daily Telegraph: The mantis shrimps, found on the Great Barrier Reef in Australia, have the most complex vision systems known to science, researchers at Bristol University have found.

444px-Mantis_shrimp_from_front.jpgThe shrimps can see in 12 colors—humans see in only three—and can distinguish between different forms of light to give a sophisticated and vivid 3D image.

Related Update
A mantis shrimp's extraordinary eyes

Related Link
A biological quarter-wave retarder with excellent achromaticity in the visible wavelength region Nature Photonics

Making a scientific dessert

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Hindustan Times: Physicist Nicholas Kurti was at the forefront of molecular gastronomy—using science in cooking during the 1960s and 1970s.

In the 1960s Kurti used to wow crowds by demonstrating the then unfamiliar technology of microwaves. Microwaves are good for heating water but not for melting ice.

A hollowed out block of ice filled with water and heated for 30 seconds in an microwave oven would result in boiling water but the ice would remain frozen. (Editor's note: Do not try this experiment without supervision.)

A microwave oven produces an electric field that reverses direction billions of times a second, forcing the water molecules to keep realigning their orientation. As the molecules realign, they collide and that collision produces heat.

But frozen water molecules (the ones in ice) are trapped in a rigid lattice work so they can't flip back and forth and create heat. That's why the ice did not melt even when the water boiled. (Eventually of course, the heat from the water would have melted the ice.)

Kurti used that principle to create a dessert called Frozen Florida with a cold exterior and a hot interior (two
recipes can be found at the link "Continue reading Making a scientific dessert".)

Related Physics Today articles
The virtual cook: Modeling heat transfer in the kitchen November 1999
Obituary: Nicholas Kurti June 1999

Physics Today: At a packed auditorium at the Quantum to Cosmos: Ideas for the future festival held at the Perimeter Institute, in Waterloo, Canada, a panel of physicists was asked to respond to a single question: "What keeps you awake at night?"

The responses ranged from Why this universe? What is everything made of? How does complexity happen? Will string theory ever be proved correct? What is reality really? to How far can physics take us?

CERN: Ion and proton particles from CERN's Super Proton Synchrotron (SPS) were successfully injected into the Large Hadron Collider last weekend (23-25 October). It was the first time since September last year that particles were injected into the LHC.

TestWeekEnd_26October2009.png
The first ion beam entering point 2 of the LHC, just before the ALICE detector (23 October 2009. Image credit: CERN)


The particles did not travel along the whole circumference of the LHC because CERN is cautiously testing the new quench system—which will protect the magnets from similar damage to that experienced last year.

The LHC will operate at 450 GeV per beam when the machine becomes operational on 23 November, and eventually ramp up to 1.1 TeV per beam in December.

Using lower energies requires less current in the superconducting magnets and will get CERN some experience with the new safeguards before increasing the power output next year to 3.5 TeV per beam in February.

As Peter Woit at Columbia University points out on his blog.

This means that 2009 will not see physics collisions, but will perhaps see collisions at energies marginally higher than that of the Tevatron...

Meanwhile the Department of Energy is requesting extra funds for the Tevatron to keep the collider running through 2011.

Related News Picks

Related Physics Today articles
Mostly recovered, the LHC readies for restart October 2009
Mishap shuts down LHC until April November 2008
Multiple problems push LHC start to next spring September 2007

Article modified on 11/09/2009 to provide correct attribution of quote to Peter Woit.

Who owns an invention?

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USA Today: Ever since the 1980 Bayh-Dole Act, which gave federally funded university researchers the right to license their inventions as a way to spur innovation and economic growth, technology transfer offices have sprung up all over, with steady growth.

In 1991, US universities filed 1,335 patents and received $130 million in royalties. In 2005, they filed 9,306 patents and received $1.8 billion in royalties.

At some universities, the policy on who owns inventions created using university resources required researchers, at some future date, to "agree to assign" ownership rights to the university.

But contracts researchers have with industry may be worded slightly differently and state an inventor "will assign and do hereby assign" his or her rights to the funder, which can lead to court cases arising over who owns the innovation rights.

Related news story
Painful lesson on patents Inside Higher Ed

Cleaning up Los Alamos

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Various: No one knows for sure what is buried in the Manhattan Project-era dump at the Los Alamos National Laboratory in New Mexico says the New York Times.

...At the very least, there is probably a truck down there that was contaminated in 1945 at the Trinity test site, where the world’s first nuclear explosion seared the sky and melted the desert sand 200 miles south of here during World War II.

But now a team of workers is using $212 million in federal stimulus money to clean up the 65-year-old, six-acre dump, which was used by the scientists who built the world’s first atomic bomb.

They are approaching the job like an archeological dig—only with even greater care, since some of the things they unearth are likely to be radioactive, while others may be explosive...

Cheryl Rofer, a former Los Alamos scientist points out that some of the extra care concerning explosives may be unwarranted. LANL used to blow up old explosives on a frequent basis in the area close to the dump, and Rofer suspects that:

...that the 1970s interview contained a comment by the old-timer that they disposed of explosives out there. The interviewer, accustomed to the practice of burying things in pits, took this to mean that the explosives were buried and wrote that down. The Los Alamos environmental restoration program, and now the New York Times, live with that to this day.

Nature: More money for science is always good. Or is it? Six experts tell Nature what concerns them most about the US stimulus spending and suggest ways to ensure that it benefits research and society in the long term.

Science: Since the work of James Clerk Maxwell and Heinrich Hertz, we have known that light is an electromagnetic wave. An intricate mechanism generates magnetic fields around the electric fields, and vice versa. In the optical-wavelength range, experimental studies have been limited to probing only the electric-field components.

In Science, Matteo Burresi and colleagues report direct measurements of the magnetic-field components of light obtained with a nanostructured metallic probe at the tip of a sharp glass fiber.

Related Link
Probing the magnetic field of light at optical frequencies

Space.com: New maps reveal colorful patterns on the surfaces of Saturn's five innermost icy moons.

Some of the patterns have been seen before, but others took scientists by surprise, suggesting dynamic interactions between the moons and other particles orbiting around Saturn.

The maps of Mimas, Enceladus, Tethys, Dione, and Rhea were created from images taken by NASA's Cassini spacecraft and were presented by Paul Schenk of Houston's Lunar and Planetary Institute at a recent meeting of the American Astronomical Society.

NPR: The Kids' Science Challenge gives elementary school students the chance to work with biologists and engineers on real scientific problems. Jim Metzner, executive producer of the Challenge, discusses with NPR how kids can get involved, from developing low-gravity sports to building hopping robots.

guardian.co.uk: The UK government is poised to allow nuclear power generators to use ordinary landfill sites for dumping "hundreds of thousands of tons" of waste in an attempt to reduce the £73 billion ($140 bn) cost of decommissioning old reactors.

The move has triggered a swath of applications around the country from big corporations trying to cash in on this potential new business, but infuriated local governments and environmental campaign groups.

Various: A 180-km-diameter crater in Mexico called Chicxulub was formed by an object 10 km across that caused a 100-million-megaton explosion when it hit Earth. Until now, that event had generally been believed to have caused the extinction of the dinosaurs.

A bigger crater, named Shiva, which was found by Sankar Chatterjee of Texas Tech University, is 500 km across. The explosion that caused it may have been 100 times the size of the one that created Chicxulub.

0954-ShivaCrater.jpg
Above is an image that shows a three-dimensional reconstruction of the submerged Shiva crater at the Mumbai Offshore Basin—part of the western shelf of India—from different cross-sectional and geophysical data. The overlying strata and water were removed to show the morphology of the crater (credit: Sankar Chatterjee, Texas Tech University).

Chatterjee presented his latest findings on Shiva to the annual meeting of the Geological Society of America in Portland, Oregon, on 18 October.

The late era of the dinosaurs was a period in which volcanic activity was frequent and common, yet the dinosaurs were thriving until the two objects hit Earth.

According to the Economist:

The picture that is emerging, then, is of a strange set of coincidences. First, two of the biggest impacts in history happened within 300,000 years of each other—a geological eyeblink. Second, they coincided with one of the largest periods of vulcanicity in the past billion years. Third, one of them just happened to strike where these volcanoes were active. Or, to put it another way, what really killed the dinosaurs was a string of the most atrocious bad luck.

Related Links
I am become Death, destroyer of worlds The Economist
Dinosaurs 'could have been wiped out by 25 mile wide meteor' The Daily Telegraph
Giant impact near India—not Mexico—may have doomed dinosaurs GSA
The significance of the contemporaneous Shiva impact structure and Deccan volcanism at the KT boundary

BBC News: Art experts at the Science Museum think they may have found the world's oldest painting to feature a watch in a hitherto unknown picture of a member of the influential Medici family.

The picture forms part of a new exhibit on measuring time.

Related News story
Science Museum consults Italian experts in bid to reveal owner of earliest portrayed watch Culture 24

HARP finds new planets

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Physics Today: Thirty-two new planets have been discovered using the High Accuracy Radial Velocity Planet Searcher (HARPS), attached to the European Southern Observatory's 3.6-meter telescope at La Silla, Chile.

The findings, presented at a conference in Porto, Portugal, raise the number of known so-called exoplanets to more than 400, of which HARPS has discovered 75.

HARPS has facilitated the discovery of 24 of the 28 planets known with masses below 20 Earth masses. As with the previously detected super-Earths, most of the new low-mass candidates reside in multi-planet systems, with up to five planets per system.

HARPS, which was installed in 2003, measures small changes in a star’s radial velocity—as small as 3.5 km/hour. The radial velocity fluctuates under the gravitational pull of an unseen exoplanet.

HARPS has already discovered the first super-Earth (around µ Ara); the trio of Neptune-sized planets around HD 69830; Gliese 581d, the first super-Earth in the habitable zone of a small star; and earlier this year, the lightest exoplanet so far detected around a normal star, Gliese 581e. More recently, they found a potentially lava-covered world, with density similar to that of Earth’s.

“These observations have given astronomers a great insight into the diversity of planetary systems and help us understand how they can form,” says HARPS team member Nuno Santos.

The team found three candidate exoplanets around stars that are metal-deficient. Such stars were originally thought to be less favorable for the formation of planets, which form in the metal-rich disk around the young star.

However, now that planets up to several Jupiter masses have been found orbiting metal-deficient stars, planet formation models will have to be revised.

Related press release
32 new exoplanets found

A portable black hole

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Nature News: Physicists have created a black hole for light that can fit in your coat pocket. Their device, which measures just 22 centimeters across, can suck up microwave light and convert it into heat

Various: Updated 10/26/09: A lawyer for the Justice Department said in court on Tuesday that Stewart Nozette, a scientist who worked for NASA and the Defense Department before being arrested on 19 October 2009 on espionage charges, had been willing to sell some of America’s “most guarded secrets” to a man he believed to be an Israeli intelligence officer but was in fact an undercover FBI officer writes New York Times reporter Robert Mackey.

290528main_stewart_nozette.jpgStewart Nozette (Credit: NASA)

Recently, Nozette, who had worked on the Clementine spacecraft in the 1990s, had been working on NASA instrument that was on board India's Chandrayaan-1 spacecraft, which recently found evidence of water on the Moon.

The Washington Post reported on 26 October that Nozette had pleaded guilty in January to over-billing NASA and the Defense Department more than $265,000 for contracting work. The court documents were sealed because Nozette was cooperating with authorities in unrelated investigations into government corruption.

Nozette admitted that he used that money to help pay personal credit card bills, car loans and maintenance costs for his swimming pool. He faced at least two years in prison under federal sentencing guidelines, according to the plea papers.

The Justice Department in a statement announcing his arrest said that Nozette had worked at the Lawrence Livermore National Laboratory from approximately 1990 to 1999. Nozette held a special security clearance equivalent to the Defense Department Top Secret and Critical Nuclear Weapon Design Information clearances. Department of Energy clearances apply to access to information specifically relating to atomic or nuclear-related materials

"Those who would put our nation’s defense secrets up for sale can expect to be vigorously prosecuted," said Channing D. Phillips, Acting U.S. Attorney for the District of Columbia. "This case reflects our firm resolve to hold accountable any individual who betrays the public trust by compromising our national security for his or her own personal gain."

Related news story
FBI arrests US scientist on spying charges The Guardian
Espionage suspect had guilty plea in fraud Washington Post

latimes.com: Three federal agencies—the Food and Drug Administration, the Defense Department and the National Eye Institute—announced last week that they are launching a three-year effort to gauge how many, and which, patients suffer troubling symptoms after undergoing the vision correction procedure called Lasik.

Space.com: NASA scientists have finally seen in their data a debris plume created by the impact of a moon probe last week onto the Cabeus crater, at the lunar south pole.


394495main_MIR-camera-image-false-color-1_full.pngA thermal image of the impact (credit: NASA)


The faint plume was seen in the data from the engineered crash one week after the impact of the LCROSS probe in the ultraviolet/visible and near infra-red wavelengths.


lunarplume.jpgA image of a plume of debris. NASA estimates the dust went up about a mile. (credit: NASA)


"There is a clear indication of a plume of vapor and fine debris," said Anthony Colaprete, LCROSS principal investigator and project scientist.

Related news story
NASA moon crash did kick up debris plume as hoped LA Times

Cambridge News: Michael Green has been elected as the 18th Lucasian Professor of Mathematics, an academic chair founded in 1663 and previously held by such luminaries as Sir Isaac Newton, Charles Babbage, and James Lighthill. Stephen Hawking retired from the post earlier this year.

Hawking has been appointed to a new role as director of research in the Department of Applied Mathematics and Theoretical Physics, and will continue to lead research efforts in cosmology and gravitation.

Various: In a talk entitled Higgs, dark matter and supersymmetry, what the Large Hadron Collider will tell us, given to science writers attending the Council for the Advancement of Science Writing’s annual symposium, Nobel laureate Steven Weinberg of the University of Texas at Austin gave his opinion of what the LHC will discover.

The LHC will eventually attain sufficient energy to produce the Higgs boson, he says, but evidence of supersymmetry is a much more speculative possibility.

"If the Congress had not had the imbecility to cancel the Superconducting Super Collider [in 1993], it would have been discovered long ago here in Texas," says Weinberg in comments reported by Tom Siegfried of Science News.

"Many of us are terrified that the LHC will discover a Higgs particle and nothing more," Weinberg said. That would just confirm the standard model, which everybody believes already. It would not point the way to further progress in solving a deeper problem that physics faces—how to add gravity to the unified theory of the other forces.

Peter Woit of "Not Even Wrong" says that what he found interesting about Weinberg’s talk was that, "whatever Weinberg’s views on more speculative theories in physics such as extra dimensions or string theory landscape, he decided not to mention these at all in his talk."

"As a result, both questioners wanted to ask Weinberg about string theory, which he hadn’t talked about, not about the solid science he did talk about," says Woit.

String theory or superstring theory, is one of the candidates for unifying all the forces in the universe into one theory.

If the LHC creates new particles generated by supersymmetry, then clues to what makes up the bulk of dark matter in the universe would be found, which may give some tangible evidence to whether string theory is correct.

But string theory to this point has not produced a cohesive and clear guide to testing its fit with all the observable features of physical existence. Weinberg said:

"It’s developed mathematically, but not to the point where there is any one theory, or to the point that even if we had one theory we would know how to do calculations to predict things like the mass of the electron, or the masses of the quarks. So, I would say, although there has been theoretical progress... I find it disappointing. One of the hopes would be that the LHC would provide a clue to something we’re missing in superstring theory and I think that supersymmetry is the most likely place to look."

"One of the troubles with superstring theory is that although in a sense the theorists think there is only one theory, there are an infinite number of approximate solutions of it and we don’t know which one corresponds to our world. But at least in a large variety of the solutions of superstring theory there is supersymmetry visible at low energies, and if we see supersymmetry at low energies, superstring theorists may be able to derive from it some kind of clue as to how to solve these theories. But I haven’t talked about it in this lecture because I don’t see how that would work... I mean I couldn’t say that it was likely with any degree of sincerity, and certainly the LHC and any other accelerator that we can imagine being built will not get up to energies which are high enough so that we can directly see the structures that are described by superstring theory, the strings or the D-branes or whatever it is. Those will not be accessible at the LHC, so any clue we get will be very indirect."

"I myself, well I was working on superstring theory in the 80s and gave it up because... I moved into cosmology, which in the last couple of decades has had the excitement that elementary particle physics had in the 60s and 70s, a wonderful coming together of theory and observation. Cosmology now reminds me of the excitement that I felt when I was younger and doing particle physics... and it’s a pity that superstring hasn’t developed better. I still think it’s the best hope we have, I don’t know of anything else. My own work very recently has been trying to develop an alternative to superstring theory as a way of making sense out of quantum gravity at very high energies. But even though I’m working on this I still find superstring theory more attractive, but not attractive enough…"


Nature: Science communication today remains firmly wedded to its print origins says Cameron Neylon in Nature and yet there are opportunities that could "allow scientists to wire their research and publications into an interactive data web."

...Beyond ease of delivery, we take very little advantage of the potential of the World Wide Web to transform the way we store and transfer knowledge. We rarely take the opportunity to update material with new data, or to provide a record of how a document or data set has changed.
...Very few companies worldwide have both the expertise and resources to take on the task of stitching [scientific data] together. So it is with great interest that I have watched Google develop its product, Google Wave.

Neylon points out that Google Wave documents can use automated agents that can "look through your paper checking for Protein Data Bank codes or gene names, for example, and putting in links to the [associated] databases."

These agents can also help create a dashboard in your inbox to monitor and control instruments in the lab.

Google Wave also has version control, that notes every change to a data or record collection.

"This would allow a reader to step through an analysis to see where conclusions have come from, and would make detecting fraud —or honest mistakes—much easier," he says.

Physics Today: Batteries can power anything from small sensors to large systems. University of Missouri researchers are developing a nuclear energy source that is smaller, lighter and more efficient.

"To provide enough power, we need certain methods with high energy density," said Jae Kwon, assistant professor of electrical and computer engineering at MU. The radioisotope battery can provide power density that is six orders of magnitude higher than chemical batteries.

Kwon and his research team have been working on building a small nuclear battery, currently the size and thickness of a penny, intended to power various micro/nanoelectromechanical systems. Although nuclear batteries can pose concerns, they are safe are already powering a variety of devices, such as pace-makers, space satellites and underwater systems.

Kwon's innovation is not only in the battery's size, but also in its semiconductor. Kwons battery uses a liquid semiconductor rather than a solid semiconductor.

The critical part of using a radioactive battery is that when you harvest the energy, part of the radiation energy can damage the lattice structure of the solid semiconductor, said Kwon. By using a liquid semiconductor, we believe we can minimize that problem.

Kwon has been collaborating with J. David Robertson, chemistry professor and associate director of the MU Research Reactor, and is working to build and test the battery at the facility.

In the future, they hope to increase the battery's power, shrink its size and try with various other materials. Kwon said that the battery could be thinner than the thickness of human hair.

NYTimes.com: Two cases involving CT scans are under scrutiny in California—one involving a large, well-known Los Angeles hospital, the other a tiny hospital in the northern part of the state—underscoring the risks that powerful CT scans pose when used incorrectly.

Raven Knickerbocker, then an X-ray technologist at Mad River Community Hospital in Arcata, activated a CT scan 151 times on the same area of the head of 2 ½-year-old Jacoby Roth, investigators concluded.

A week ago, Cedars-Sinai Medical Center in Los Angeles disclosed that it had mistakenly administered up to eight times the normal radiation dose to 206 possible stroke victims over an 18-month period during a procedure intended to get clearer images of the brain.

Although CT scans are useful in determining internal injuries, there are major risks associated to patients because of the intensity of the X-rays used in the device, either through human error, or through too frequent exposure to X-rays.

In 2000-2001, CT scans constituted 7% of all radiologic examinations, but contributed 47% of the total collective dose from medical X-ray examinations.

BBC News: The Large Hadron Collider (LHC) experiment has once again become one of the coldest places in the Universe.

All eight sectors of the LHC have now been cooled to their operating temperature of 1.9 kelvin (-271°C)—colder than deep space.

The large magnets that bend particle beams around the LHC are kept at this frigid temperature using liquid helium.

The magnets are arranged end-to-end in a 27km-long circular tunnel straddling the Franco-Swiss border.

The cool-down is an important milestone ahead of the collider's scheduled re-start in the latter half of November as leaks earlier in the year delayed the restart of the LHC.

Science News: Although the impact of a published study can be measured many ways, the most common tactic has been to tally how often, over the years, others cite the study in their published works. A small industry has emerged over the past half century to quantify these citations. A new analysis has now compared citation counts from three different companies and shown that their performance differs. At least when it comes to published biomedical studies, some citation indices may make a given piece of work appear substantially more—or less—influential than do others. Related Links Comparisons of citations in Web of Science, Scopus, and Google Scholar for articles published in general medical journals The journal impact factor denominator: Defining citable (counted) items

Various: NASA launched the Interstellar Boundary Explorer (IBEX) spacecraft last year to investigate the edges of the heliosphere—the insulating bubble the sun creates around the solar system. IBEX principal investigator David McComas talks to NPR's Ira Flatow on the first surprising results that were published by Science on Friday.

What did IBEX discover?

At the boundary of our Solar System, the interactions between solar wind particles and interstellar medium particles create Energetic Neutral Atoms (ENAs), particles with no charge that move very fast.

Some of the ENAs happen to be travel inwards through the Solar System toward Earth where IBEX can collect them. This region emits no light and so cannot be observed by conventional telescopes.

The five maps released by the group on Friday show that ENA's are not uniformly spread across the sky, which was the opposite of what was expected with the existing theoretical models of the heliosphere's behavior.

ibex_data_map.jpg

Instead there is there is an arc-shaped region in the sky that is creating a large amount of ENAs, showing up as a bright, narrow ribbon on the maps.

IBEX is also observing many more ENAs from smaller regions in the sky than researchers thought they would.

The ribbon appears to be produced by the alignment of magnetic fields outside our heliosphere. "These observations suggest that the interstellar environment has far more influence on structuring the heliosphere than anyone previously believed," says McComas on the IBEX site.

Related Science papers
Tying up the Solar System with a ribbon of charged particles
Global observations of the interstellar interaction from the Interstellar Boundary Explorer (IBEX)
Width and variation of the ENA flux ribbon observed by the Interstellar Boundary Explorer
Structures and spectral variations of the outer heliosphere in IBEX energetic neutral atom maps
Comparison of Interstellar Boundary Explorer observations with 3-D global heliospheric models
Direct observations of Interstellar H, He, and O by the Interstellar Boundary Explorer

Hindustan Times: An alumnus from Vadodara’s Maharaja Sayajirao University may have given India its latest Nobel laureate, but the department of physics, where V. Ramakrishnan learnt the basics, is struggling to attract students.

“While we are happy that our students has achieved a global honor, the declining interest for basic sciences among students is a cause for worry,” the head of the physics department AC Sharma, head told the Hindustan Times.

Six years back, Sharma said, the department attracted more than 400 applications for 52 seats in MSc Physics. Today, the number has dropped to 150.

Nature News: Construction at the site of ITER—the multibillion-euro project to prove controlled nuclear fusion—has been at a standstill since April.

The stoppage comes as European contributors negotiate how to pay for their share of ITER, a collaboration between Europe, Japan, South Korea, Russia, the United States, China and India.

Excavations for the buildings, slated to begin this autumn, will not start until spring 2010—roughly a year after site preparations were completed.

Various: A series of papers in Science and Nature report new results on spin ices and monopoles.

The Nature paper

Spin ices are an exotic class of crystalline solids that are rare, three-dimensional systems in which the magnetic moments (spins) of the ions remain disordered even at the lowest temperatures available writes Shivaji Sondhi in Nature. This means that the geometrical layout of the atoms are such that the norths and souths are never able to align in a satisfactory way and so the magnets continually flip up and down trying to find a stable position says Hannah Delvin in the London Times.

The material has a second property, at regular intervals on the lattice the magnetic fields of individual atoms add up to produce essentially isolated north or south charges, behaving as point-like objects that are the condensed-matter versions of Paul Dirac's theoretical magnetic monopoles—particles that, unlike iron magnets, have a single magnetic pole and hence carry an overall magnetic charge.

Initially, it was not evident that their charge could be measured in a straightforward way. Magnetic monopoles live in a lattice at a moderate density under normal laboratory conditions—not the sort of setting in which you could carry out a magnetic version of Millikan and Fletcher's oil-drop experiment to determine the electric charge of the electron.

But Steve Bramwell of the London Centre for Nanotechnology and colleagues in Nature report a measurement of the magnetic charge of the monopoles in spin ice that is in surprisingly good agreement with the theoretical prediction.

"It is not often in the field of physics you get the chance to ask, ‘How do you measure something?’, and then go on to prove a theory unequivocally," said Bramwell to Delvin. "This is a very important step to establish that magnetic charge can flow like electric charge."

The Science papers

In Science, two groups also report measurements from neutron-scattering experiments showing that the low-energy excitations in spin ices are reminiscent of magnetic monopoles writes Michel J. P. Gingras.

These dissociated north and south poles diffuse away from each other in these oxides and leave behind a "Dirac string" of reversed spins that can be seen as patterns in the intensity of scattered neutrons.

Related Links
Discovery of ‘magnetricity’ marks important advance in physics London Times
Measurement of the charge and current of magnetic monopoles in spin ice Nature
Observing Monopoles in a Magnetic Analog of Ice Science
Magnetic Coulomb Phase in the Spin Ice Ho2Ti2O7 Science
Dirac Strings and Magnetic Monopoles in the Spin Ice Dy2Ti2 Science

Physics Today: Johns Hopkins University is again the leading US academic institution in total research and development spending for the 30th year in a row, according to a new the latest annual NSF Survey of Research and Development Expenditures at Universities and Colleges.

The total funding ranking includes research support not only from federal agencies, but also from foundations, industry and other sources.

The university pulled in $1.68 billion in medical, science and engineering research in fiscal 2008, half of which was based at the Applied Physics Laboratory. Since NSF changed its methodology in 1979 to include spending by the Applied Physics Laboratory in the university’s totals, the university has remained top of the list.

APL employs 4,300 people working specifically on some 400 R&D projects with annual funding of about $800 million.

The institutions ranked second through fifth—University of California at San Francisco; University of Wisconsin at Madison; University of Michigan and UCLA—all reported spending in the $800 million to $900 million range.

Top of the federal list

Johns Hopkins also ranked first on the NSF’s separate list of federally funded research and development, spending $1.42 billion in FY2008 on research supported by NSF, NASA, the National Institutes of Health and the Department of Defense.

"More than half of our annual expenditures is invested in research," said Lloyd Minor, provost and senior vice president of academic affairs at Johns Hopkins. "Our success in attracting external research support is a testament to the talent, dedication and leadership of the faculty, staff and students."

In FY2010, positions on the list may change slightly due to the heavy investment in R&D as part of the administration's billion dollar stimulus package.

Virginia Tech dropped from 42nd to 46th out of 679 universities, not because of a lack of funding—which increased by $7 million to $373 million in 2008—, but because funding increased more dramatically at other institutions.

"While our overall growth was below our goals, the areas that account for competitive research awards continued to grow," said Robert Walters, vice president for research. "We increased our external federal funding by more than 5 percent and our industry funding by almost 20 percent. In the current economy, those numbers are encouraging."

Paul Guinnessy

CNN.com: Building's connected to Rome's ancient Mediterranean port "Portus" have been discovered after being buried for 1800 years.

The site consists of an amphitheater, a Roman warehouse and the ruins of an Imperial palace by University of Southampton archaeologists owes much to modern technology.

"It's true I think also to say that we have kind of rediscovered it because the great Italian archaeologist Rodolfo Lanciani reported the discovery of a theater in the 1860s but nobody could actually find it," said Simon Keay, a leading expert on Roman Archaeology to CNN.


The site is less than a mile from Rome's Fumicino International Airport, and was discovered using modern sensors, ground-penetrating radar and probes to compile a digital underground map of the area.

"So we then played around with it on the computer screen, we did a virtual reconstruction of it and amphitheater shape grew out of the screen and we knew that we were on to something very special," said Keay.

Physics Today: The next generation of energy efficient houses appeared in Washington this week as part of the Department of Energy's 2009 solar decathlon competition (pdf).

The competition, held on the Washington Mall, judged 20 homes based on aesthetics, functionality and energy measurements.

The University of Minnesota's 565 sq. ft solar home called ICON cost half a million dollars to build and came 5th in the competition.

Student's have to design in factors such as is there enough solar thermal hot water for the big and small dishwashers in the kitchen and the clothes washer in a cabinet next to the small bathroom? Was the temperature in the house just right? What about the humidity? Exactly how much power would the appliances, along with the lights—mostly LEDs—draw from the photovoltaic cells that covered the roof and south-facing wall?


"We build [ICON] specifically for the Minnesota climate," said Shona Mosites, a senior studying interior design at the University of Minnesota.


Like all of the houses in the competition, the Minnesota house is compact—about the size of a large house trailer. It is extremely energy efficient, producing more electricity during the day than it uses and feeding the excess into the regional power grid. At night, when the sun is down, the house draws from the grid, but less than it feeds into the system during the day.

And like all of the other houses, the ICON house makes extensive use of green materials.

"The sliding panels are made of recycled material, and the maple flooring is two-thirds reclaimed wood," Mosites said.

A difficult road trip


At the other end of the Mall, the team from the University of Wisconsin-Milwaukee was struggling. The team was in last place, and were struggling to get the house's sliding doors to move smoothly on their tracks. Their house, valued at $485,000, had tabletops made out of pressed paper and cashew shells and the ability to warm up just from the heat of the people inside.

But its last-place standing reflected a 3-inch problem in the design.

"The west end of the house was 3 inches too tall to go through Indiana [on the transport trailer]," said Eric Davis, the project's chief engineer. "So we had to go down through Illinois, then cross Kentucky."

There was another height regulation problem when they got to the edge of Washington, and it took another 20 hours to finally get their structure to the National Mall. While the other teams were fine tuning their home's systems, the Wisconsin team was still wearing hard hats and putting their house together.

"We missed the metering contest, so our score is down," Davis said.

The houses that make up the high-tech Solar Village are mostly from universities, shipped in multiple pieces from around the world. Germany, Spain and two teams from consortiums of Canadian universities also have entries in the competition. And the event is drawing crowds, with long lines of people waiting to tour the houses.

"About 2,000 people come through our house each day," said Thomas Rauch, media liaison and team member of Penn State University's Natural Fusion house.

The energy produced by these small structures, each limited to 800 square feet, powers all of the lighting, appliances and air conditioning within. And on sunny days, when the houses produce more electricity than is needed, they pump the extra energy directly into the regional electrical grid that powers the metro area.

The German team's house often gives back twice as much energy as it uses—enough in one day to light 400 incandescent light bulbs for one hour.


solar_kickoff.jpg

Home improvement

US Secretary of Energy Steven Chu helped to kick-off the event on Oct 8 (see picture left. Chu is on the right. Photo credit: DOE) by describing his own home-improvement experiences while working to make his home more energy efficient. "I started doing this long before I knew about climate change. And I have to confess the only reason I was doing that is because I'm fundamentally cheap," he said.

Chu said that during his time at Lawrence Berkeley National Laboratory in California he became convinced that houses could be made 75 or 80 percent more efficient in terms of energy usage—before adding any solar panels. He also announced an additional $87 million in DOE funding to further the solar research on display in the homes.

Several of the houses are smart phone-enabled—the interior lighting and temperature can be changed remotely with an iPhone application. Others adjust interior conditions automatically, using sensors that monitor time and weather data to tint electrochemical windows and dim light levels.

But the point of the contest isn't just to showcase new technology. Each team is scored in ten different categories. The buildings must provide all the basics of daily life. Several times a day, they must pump out 15 gallons of hot water that could be used for showering. Solar energy also powers a host of appliances that include dishwashers, clothes washers, refrigerators and televisions.

Teams that score well overall are those that focus not only on the individual pieces of the house, but on how the pieces fit together to create a the houses focus on a systems approach—designing a house not piece by piece, but as a giant system.

"As we went through the 70s and the 80s, we had terribly unreliable systems that gave solar a black eye," said Richard King, director of the Solar Decathlon. "As we move into the future, to do it right we have to start from the ground up and make the whole house a system, so it's all integrated."

King, who launched the first Solar Decathlon in 2002, said that the contest is designed not to be too restrictive, to give students a blank page and see what they come up with. This promotes a wide variety of engineering approaches and aesthetic designs, he said.

The team from Iowa State University in Ames built a house designed specifically to appeal to older, retired couples. It was the only structure to be certified under the Americans with Disabilities Act, and the unfinished white maple exterior is intended to feel comfortable and familiar.

"A lot of people have been saying that they could see themselves eating breakfast in this corner, that the house feels livable," said Melissa Sander of Iowa State University as she guided visitors through the house. Their house placed 3rd in market viability.

The average cost of a home on this solar-powered block is $490,000, but teams can spend as much on their project as they can afford. The cheapest house Rice University's ZEROW House—is intended for lower-income inner-city neighborhoods and is built with walls of galvanized metal that could retail for $140,000. The customized electronics and solar panels in the North House help contribute to a cost upwards of $800,000, a sum that Team Ontario/British Columbia from the University of Waterloo, Ryerson University and Simon Fraser University aim to target at young urban professionals.

Team California's house,—a collaboration between Silicon Valley's Santa Clara University and the Bay Area's California College of the Arts—was in 1st place throughout the first several days of the competition and featured a design utilizing bamboo as an alternative building material for its rafters, while Team Spain—from the Polytechnic University of Madrid—had constructed their walls from the solar panels themselevs.

Patents and prototypes

Many of the design elements have led to patents, and new prototypes from several companies were on display—from a heat-absorbing lining made of the same materials as insulating pizza boxes by Phase Change Energy Solutions of Asheboro, N.C., to a solar water heater that creates miniature hot geysers and collects the overflow by Sunnovations in Reston, Va.

On Tuesday, scores of middle and high school students from across the metro area crowded through the solar houses as their teachers held up flags and otherwise tried to keep them in order. As two middle-school boys walked between the houses, one turned to the other and said, "Wouldn't it be so awesome if one of these had a solar powered hot tub."

But that idea has already come and gone.

A house entered in the 2007 competition by the University of Texas in Austin actually included a working solar-powered hot tub, but the designs featured in this year's competition were all evidently spa-free.



Based on material from Inside Science News Service.

Jim Dawson and Devin Powell

Edited by Paul Guinnessy


Nature News: A new generation of light sources—the newly completed Linac Coherent Light Source (LCLS) at the SLAC National Accelerator Laboratory in Menlo Park, California, one under construction in Japan and the European X-Ray Free-Electron Laser (XFEL) being built at at DESY in Germany—are getting set not only to put atoms and molecules under the spotlight, but also to illuminate their dynamics.

The devices, called X-ray free-electron lasers, produce flashes of X-ray light with angstrom-level wavelengths—small and coherent enough to image individual atoms. The flashes are also more intense than any created before—stuffed with enough photons to create and study extreme states of matter such as plasma.

But perhaps most importantly, the bursts of light are short—just hundreds of femtoseconds long, the time it takes for light to cross a human hair. Pulses as brief as this can record functions, not just forms: the folding of a protein, the action of a catalyst, the splitting of a chemical bond.

Science: The two great ice sheets—Greenland's and Antarctica's—are closely monitored for ice loss.

Surveys of ice-sheet volume made from planes and satellites have quantified these losses, but those assessments have been spotty in time, space, or both.

Now the latest analysis of the most comprehensive, essentially continuous monitoring of the ice sheets shows that the losses have not eased in the past few years. More ominously, losses from both Greenland and Antarctica appear to have accelerated during the past 7 years.

BBC News: Scientists in Italy think they may have come up with a new way to scan for cancer of the stomach or colon.

The 'spider pill,' which is fitted with a camera, is swallowed by the patient and once within the colon or intestine the legs are opened and the device crawls along the intestine tract, taking pictures as it goes.

ISNS: With the speed of computers so regularly seeing dramatic increases in their processing speed, it seems that it shouldn't be too long before the machines become infinitely fast—except they can't.

A pair of physicists has shown that computers have a speed limit as unbreakable as the speed of light. If processors continue to accelerate as they have in the past, we'll hit the wall of faster processing in less than a century.

Intel co-founder Gordon Moore predicted 40 years ago that manufacturers could double computing speed every two years or so by cramming ever-tinier transistors on a chip. His prediction became known as Moore's Law, and it has held true throughout the evolution of computers—the fastest processor today beats out a ten-year-old competitor by a factor of about 30.

If components are to continue shrinking, physicists must eventually code bits of information onto ever smaller particles. Smaller means faster in the microelectronic world, but physicists Lev Levitin and Tommaso Toffoli at Boston University in Massachusetts, have slapped a speed limit on computing, no matter how small the components get.

"If we believe in Moore's law ... then it would take about 75 to 80 years to achieve this quantum limit," Levitin said.

"No system can overcome that limit. It doesn't depend on the physical nature of the system or how it's implemented, what algorithm you use for computation ... any choice of hardware and software," Levitin said. "This bound poses an absolute law of nature, just like the speed of light."

Scott Aaronson, an assistant professor of electrical engineering and computer science at the Massachusetts Institute of Technology in Cambridge, thought Levitin's estimate of 75 years extremely optimistic.

Moore's Law, he said, probably won't hold for more than 20 years.

In the early 1980s, Levitin singled out a quantum elementary operation, the most basic task a quantum computer could carry out. In a paper published in Physical Review Letters, Levitin and Toffoli present an equation for the minimum sliver of time it takes for this elementary operation to occur. This establishes the speed limit for all possible computers.

Using their equation, Levitin and Toffoli calculated that, for every unit of energy, a perfect quantum computer spits out ten quadrillion more operations each second than today's fastest processors. 

"It's very important to try to establish a fundamental limit—how far we can go using these resources," Levitin explained.

The physicists pointed out that technological barriers might slow down Moore's law as we approach this limit. Quantum computers, unlike electrical ones, can't handle "noise"—a kink in a wire or a change in temperature can cause havoc. Overcoming this weakness to make quantum computing a reality will take time and more research.

As computer components are packed tighter and tighter together, companies are finding that the newer processors are getting hotter sooner than they are getting faster. Hence the recent trend in duo and quad-core processing; rather than build faster processors, manufacturers place them in tandem to keep the heat levels tolerable while computing speeds shoot up. Scientists who need to churn through vast numbers of calculations might one day turn to superconducting computers cooled to drastically frigid temperatures. But even with these clever tactics, Levitin and Toffoli said, there's no getting past the fundamental speed limit.

Aaronson called it beautiful that such a limit exists.

"From a theorist's perspective, it's good to know that fundamental limits are there, sort of an absolute ceiling," he said. "You may say it's disappointing that we can't build infinitely fast computers, but as a picture of the world, if you have a theory of physics allows for infinitely fast computation, there could be a problem with that theory."

Lauren Schenkman
First published at Inside Science News

NYTimes.com: Holger Bech Nielsen, of the Niels Bohr Institute in Copenhagen, and Masao Ninomiya of the Yukawa Institute for Theoretical Physics in Kyoto, Japan, have suggested that the hypothesized Higgs boson, which physicists hope to produce with CERN's Large Hadron Collider, might be so abhorrent to nature that its creation would ripple backward through time and stop the collider before it could make one, like a time traveler who goes back in time to kill his grandfather.

Nielsen and Ninomiya put this idea forward in a series of papers: "Test of Effect From Future in Large Hadron Collider: a Proposal" and "Search for Future Influence From LHC," posted on the physics Web site arXiv.org.

According to the so-called Standard Model that rules almost all physics, the Higgs is responsible for imbuing other elementary particles with mass.

"It is our prediction that all Higgs producing machines shall have bad luck," Nielsen told the New York Times in an email.

Nature: Since the Big Bang, the Universe's initial expansion has been gradually slowed by the gravitational pull from the mass it contains. Most of this mass is in the form of invisible and mysterious dark matter. Today, however, the Universe seems to be re-accelerating under the influence of even weirder stuff dubbed dark energy.

Almost nothing is understood about either dark matter or dark energy—but both are many times more common than visible matter.

Tracking the expansion of the Universe, from which the relative amounts of dark matter and dark energy can be inferred, requires measuring the distances to galaxies. Distances have always been the bane of astronomy: there are no simple red and green glasses to extrude our two-dimensional picture of the sky into an expanding movie.

Three rival techniques are currently trying to establish themselves as the best probe of cosmological expansion: observations of exploding stars called type Ia supernovae, the focal lengths of gravitational lenses, and baryon acoustic oscillations.

Astronomer Richard Massey from Edinburgh's Institute for Astronomy assess the advantages and disadvantages of the three techniques.

Related Link
Cosmology: Dark is the new black

Wall Street Journal: Hamid Biglari went from physics to finance. Now, he's helping lead efforts to revive Citigroup Inc. Born and raised in Tehran, Hamid Biglari came to the US in 1977 to study mathematics and physics at Cornell University.

Biglari planned to return in Tehran after getting his degree, but the 1979 Iranian Revolution derailed his plans. He realized that his career opportunities would be better in the US so filed for permanent residency.

After earning his PhD in astrophysics at Princeton in 1987 he became a theoretical physicist at the Princeton Plasma Physics Laboratory, writing one of the most cited papers in Tokamak fusion research.

But research budget cuts made Biglari consider a career in finance.

He had no business experience, but he cold-called management consultancy McKinsey & Co., and successfully persuaded them to hire him, based on his analytical and computational skills.

After moving to Citigroup in 2000, earlier this year Biglari became vice chairman in charge of strategy and resource allocation, a key post in reframing the company after last year's billion dollar loss.

Nature News: The High Frequency Active Auroral Research Program (HAARP), near Gakona, Alaska, has for twenty years used radio waves to probe Earth's magnetic field and ionosphere.

hpimage.jpgOne of the most visible results of the experiments—since the facility upgraded its transmission power output from 1 to 3.6 megawatts—is that they can create lights in the sky that are similar to auroras.

The technique works by using the high-frequency radio waves to accelerate electrons in the atmosphere, increasing the energy of their collisions and thereby creating a glow.

In February last year, HAARP unexpectedly managed to induce a strange bullseye pattern in the night sky. "This is the really exciting part—we've made a little artificial piece of ionosphere," said US Air Force Research Laboratory physicist Todd Pedersen to Nature's Naomi Lubick.

ScienceNow: Forgotten coin stashes suggest Roman population dropped as the republic became an empire, suggesting more than 100,000 people were killed in the Roman civil wars.

Science: Current computer-aided design tools are not making it easy for architects to design buildings for energy efficiency. New software is needed.

Related News Story
Training to climb an Everest of digital data New York Times

Physics Today: Adlène Hicheur, a 32-year-old postdoc at the Swiss Federal Institute of Technology in Lausanne working on the Large Hadron Collider (LHC)—who was arrested in Vienne, France, last week—was charged earlier today on the suspicion of terrorism, say French and Swiss newspapers.

Hicheur had told investigators over the weekend that he corresponded over the internet with a contact in north Africa's al-Qaida branch, said French officials to the Guardian.

The exchange vaguely discussed plans for terror attacks, but nothing concrete was planned, the French official said, speaking on condition that his name not be used because the investigation is ongoing.

French counterterrorism and intelligence agencies have been tracking Adlène Hicheur for 18 months by reading his e-mails, says the Independent. They concluded in recent days that he had reached the "intention or desire stage" of preparing to mount an attack and arranged for his arrest.

Hicheur had been working at CERN on data analysis for the LHC since 2003. CERN issued a statement saying the following:

[Hicheur] was not a CERN employee and performed his research under a contract with an outside institute. His work did not bring him into contact with anything that could be used for terrorism: CERN is a particle-physics research laboratory whose research addresses fundamental questions about the universe. None of our research has potential for military application, and all our results are published openly in the public domain. CERN is providing the support requested by the French police in this enquiry.

Hicheur had previously worked on the BaBar experiment in the US, and at the Rutherford Appleton Laboratory in Oxfordshire, UK.

Related News Story
Hadron Collider physicist Adlene Hicheur charged with terrorism London Times

Various: The experiment to smash part of a rocket upper stage into the Moon at high speed (as reported earlier this week) went without a hitch but did not produce a visible plume 10 kilometers high as expected.

moon.jpgVincent Eke, from the University of Durham, told the Independent that the lunar surface may not have reacted as expected and stressed it was still too early to know if the mission had been a success or failure.

"If it turns out to be as dull as it looked, I'd imagine the soil just didn't respond as was hoped to being hit," said Dr Eke. "It might mean we don't get sufficient data, which would be a shame."

Researchers are now analyzing the data gathered from the event, NASA told NPR, and expect to know for certain if the impact dislodged any water in about two weeks.

Related Links
Targeting the Moon: Observatories gear up for Friday lunar crash Space.com
Moon 'bombing' makes an impact—really The Independent
Spacecraft crashes into Moon in search of water NPR

APS News: Restrictions imposed by the US Air Force on the use of lasers are significantly diminishing the utility of adaptive optics for studying the cosmos, according to a number of astronomers.

The Economist: Dialysis is an unpleasant process that involves being hooked up to a huge machine—often at a hospital—at least three times a week, in order to have your blood cleansed of waste that would normally be voided, via the kidneys, as urine.

1_kidney_gura_220.jpgVictor Gura, of the University of California, Los Angeles, hopes to make this process more pleasant with an invention that is now undergoing clinical trials. By going back to basics, he has come up with a completely new sort of dialyser—one you can wear.

At the heart of the machine is a lightweight pump. The pump drives blood from a patient through a hollow fiber filter as well as water containing some minerals. The water is constantly purified by circulating through chemicals that capture the blood's impurities. The blood is then pumped back to the patient. The filter needs to be replaced about once a week and the chemicals once a day.

In clinical trials reported in the December 15, 2007 issue of the medical journal Lancet, five men and three women with end-stage kidney failure successfully dialyzed themselves with Gura's prototype device for up to eight hours.

Related Links
A wearable artificial kidney for patients on the go UCLA news
Some related publications
A wearable haemodialysis device for patients with end-stage renal failure: a pilot study The Lancet

Hunting for lost art

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New York Times: Leonardo da Vinci probably would have loved the use of scientific gadgetry to locate his lost masterpiece.

The Guardian: An orchestra of ancient instruments, many of which exist only in paintings and yellowing manuscripts, will perform its first concert at the end of the year.

Many of the instruments have not been heard since the times of Socrates in the fifth century BC, though some of the instruments date back even further, to the bronze age a thousand years earlier.

Scientists are reconstructing the sounds of the instruments, including the earliest predecessors of the bass guitar, harp and oboe, by building mathematical models of them on computers, using descriptions in ancient texts and paintings on artifacts recovered from archaeological sites in Greece.

Inside Science: Early on Tuesday morning, 1977 Nobel Prize winning physicist Philip Anderson's home phone rang. When the Princeton University emeritus professor answered, it was William Brinkman, director of the Office of Science for the US Department of Energy.

"Score another one for Bell Labs," Brinkman said, referring to the just-announced winners of the 2009 Nobel Prize in Physics. Two of three winners of the 2009 prize did their research in 1969 at Bell Labs, the research arm of the then giant telephone monopoly AT&T. That brings to 13 the number of Bell Labs scientists who have won a share of the seven Nobel Prizes for work done at what was once considered the preeminent research lab in the world.

Bell Labs, in Murray Hill, NJ, still exists as part of the French-based Alcatel-Lucent telecommunications company, but it is no longer the hotbed of basic research in the physical sciences where researchers worked for decades on projects that often produced great science, but not necessarily products, for the parent company. "You're reaching pretty far back for those," Anderson said of the 2009 Nobel Prize winners.

Physics Today: The Royal Swedish Academy of Sciences has decided to award the Nobel Prize in Chemistry for 2009 jointly to

Venkatraman Ramakrishnan, MRC Laboratory of Molecular Biology, Cambridge,United Kingdom
Thomas A. Steitz, Yale University, New Haven, CT, USA
Ada E. Yonath, Weizmann Institute of Science, Rehovot, Israel

"for studies of the structure and function of the ribosome."

chemistrynobel.jpg

Inside every cell in all organisms, there are DNA molecules. They contain the blueprints for how a human being, a plant, or a bacterium looks and functions.

The DNA is transformed into living matter through the work of ribosomes. Based upon the information in DNA, ribosomes make the chemistry of life: proteins, such as oxygen-transporting hemoglobin, antibodies of the immune system, hormones such as insulin, the collagen of the skin, or enzymes that break down sugar.

There are tens of thousands of proteins in the body and they all have different forms and functions.

Ramakrishnan, Steitz, and Yonath discovered what the ribosome looks like and how it functions at the atomic level.

All three used X-ray crystallography to map the position for each and every one of the hundreds of thousands of atoms that make up the ribosome and created 3D models that show how different antibiotics bind to the ribosome. X-ray crystallography is a fundamental research tool in biophysics and chemistry, and has resulted in a number of Nobel Prizes.

"Today's award is one of the great stories in biophysics," says Jason Bardi, a spokesperson for the American Institute of Physics (which publishes Physics Today). "People worked for years to get these structures, and for a long time, many in the field doubted whether it could even be done."

The ribosome is a massive protein, weighing in at 2.5 million atomic mass units (amu) and has a complicated structure.

Ribosomes are so big that they can often be spotted under electron microscopes but attempts to look at their structures using diffracted light of much shorter X-wavelengths proved to be challenging.

When the hi-resolution images of ribosomes came out a decade ago by the three laureates, it was held as a significant breakthrough. "Frankly I was stunned," says Bardi. "The ribosomal structure most familiar to me previous to that was the one that adorned my "GENES IV" textbook in graduate school. It was a big purple blob—a molecular Barney. Now suddenly, I could see a thousand interwoven protein helices and finger-like sheets and an impossibly complicated tangle of RNA. It was a truly stunning image."

Paul Guinnessy

Related Physics Today Resources
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Science News: For all its tumult—erupting stars, colliding galaxies, collapsing black holes—the cosmos is a surprisingly orderly place. Theoretical calculations have long shown that the entropy of the universe—a measure of its disorder—is but a tiny fraction of the maximum allowable amount.

But an analysis by Chas Egan of the Australian National University in Canberra and Charles Lineweaver of the University of New South Wales in Sydney indicates that the collective entropy of all the supermassive black holes at the centers of galaxies is about 100 times higher than previously calculated. Because supermassive black holes are the largest contributor to cosmic entropy, the finding suggests that the entropy of the universe is also about 100 times larger than previous estimates.

Wired.com: The Superconducting Super Collider has been a stain on US scientific history ever since the project was canceled in 1993 says Paul Berger in Wired magazine. Photo Credit: SSC Scientific and Technical Electronic RepositoryIt was hoped the collider would reveal new forms of matter and energy, like the elusive Higgs boson, by firing proton beams in opposite directions and smashing atoms into each other inside a 54-mile circular tunnel buried 250 feet underground (see photo of tunnel construction left). US physicists had to give up its project in Texas after Congress yanked funding—though not before the Department of Energy had built infrastructure, warehouses and almost 15 miles of underground tunnels at a $2 billion cost to the US taxpayer. The land and facilities are now up for sale, and yours for only $20 million. From the Physics Today archive SSC cost and size perplex Congress, Irwin Goodwin, May 1984 SSC design goes to DOE: ICFA discusses CERN hadron collider, Gloria B. Lubkin, June 1984 R & D funding for the Super Collider, Gloria B. Lubkin, October 1984 The SSC: A machine for the nineties, Sheldon L. Glashow and Leon M. Lederman, March 1985 Reagan endorses the SSC, a colossus among colliders, Irwin Goodwin, March 1987 The SSC vs Murphy's Law, Robert J. Yaes, Edwin L. Goldwasser, July 1987 Will High-Tc superconductivity affect the SSC's design? Irwin Goodwin, August 1987 Alternatives to the Superconducting Super Collider, Freeman Dyson, February 1988 Amazing race: The SSC contest generates disorder and discord, Irwin Goodwin, May 1988 SSC alternatives: Critics collide with Dyson, Edwin L. Goldwasser, Robert Siemann, Martin Einhorn and Gordon Kane, A. Abashian, and Freeman Dyson May 1988 SSC: Essential science or unnecessary expense? Robert E. Marshak, Lels L. Larson, Michael J. Glaubman, Daniel M. Smith, Steven Weinberg, John F. Waymouth, October 1988 Four reasons for forsaking the SSC, Truman Hunter, May 1990 A proposed detector for the SSC is approved, Bertram Schwarzschild March 1991 As SSC project accelerates, its cost exceeds $8.2 Billion, Irwin Goodwin, March 1991 What's gone wrong with the SSC? It's political, not technological, Irwin Goodwin, August 1992 Tunnel boring begins at Superconducting Super Collider, Bertram Schwarzschild, March 1993 Some thoughts on the SSC and the management of science, Sidney D. Drell, July 1993 Congress cancels SSC and allocates high budgets for technology in 1994, Irwin Goodwin, November 1993 An open letter to colleagues who publicly opposed the SSC, Leon M. Lederman, March 1994 The SSC's end: What happened? And what now?, Wolfgang K. H. Panofsky, Doug Pewitt, David R. Nygren, Pierre Ramond, Robert J. Reiland, Christopher Carone, Rustum Roy, March 1994 Reassigning blame for the SSC's demise, Timothy E. Toohig and Lawrence Cranberg, October 1994 Four years after SSC's demise, US Reaches agreement on `unprecedented' collaboration in CERN's LHC, Irwin Goodwin, January 1998

Physics Today: [First published 6:10am EST 10/6/09, last updated 11:33am EST] The Royal Swedish Academy of Sciences has decided to award the Nobel Prize in Physics for 2009 with one half of the $1.4 million to

Charles K. Kao
Standard Telecommunication Laboratories, Harlow, UK, and Chinese University of Hong Kong

"for groundbreaking achievements concerning the transmission of light in fibers for optical communication"

and the other half jointly to

Willard S. Boyle and George E. Smith
Bell Laboratories, Murray Hill, NJ, USA

"for the invention of an imaging semiconductor circuit – the CCD sensor."

boyle_smith_charge-coupled_photo.jpg
Bell Labs researchers Willard Boyle (left) and George Smith (right) with the charge-coupled device. Photo taken in 1974. Photo credit: Alcatel-Lucent/Bell Labs.


"The [transfer of] information in society today is completely based on [this research]," said Joseph Nordgren, the chair of the Nobel Prize committee in a press conference announcing the prize. "The practical implications for this research were enormous...It is something that has changed our life, not just in science but in society as whole."

Fred Dylla, CEO of the American Institute of Physics, which publishes Physics Today, concurs. "When combined with the laser and the transistor, the invention of an efficient, low-loss optical fiber has made nearly instantaneous communication possible across the entire globe. This mode of communication is essential for high-speed internet and forms the optical backbone of 21st century commerce. The CCD sensor has revolutionized technical, professional, and consumer photography in the last few decades. Taken together these inventions may have had a greater impact on humanity than any others in the last half century."

"Optics technologies are exceptionally significant for scientific developments in today’s world," said Elizabeth Rogan, CEO, of the Optical Society of America. "We congratulate Kao, Boyle and Smith on this much-deserved recognition."

Kao

In 1966, Charles K. Kao made a discovery that led to a breakthrough in fiber optics. He carefully calculated how to transmit light over long distances via optical glass fibers. With a fiber of purest glass it would be possible to transmit light signals over 100 kilometers, compared to only 20 meters for the fibers available in the 1960s. "It was the impurities, and other limiting factors such as scattering, atomic motion, that limited glass fibers in the 1960s," said Nordgren.

Kao presented his research at the 1966 London meeting of the Institution of Electrical Engineers. The first ultrapure fiber was successfully fabricated just four years later, in 1970 by the Corning company.

"The Nobel Prize isn't awarded for lifetime achievement, it is given for diverse research, clearly Kao's work achieved a breakthrough that led to a whole new research and technology field," said Nordgren.

Boyle and Smith

In 1969 Willard S. Boyle and George E. Smith invented the first successful imaging technology using a digital sensor, a CCD (charge-coupled device).

The two researchers came up with the idea in just an hour of brainstorming, according to Boyle who spoke during a press conference today. "It is amazing that a [the CCD device] was created so quickly," said Nordgren. "There are so many breakthroughs that came out of research at Bell labs...it's unfortunate that during the 80s, US companies abandoned the idea of having a scientific environment such as Bell labs," said Nordgren.

Boyle said that to him, the biggest achievement of his work was seeing images transmitted back from Mars. "It wouldn't have been possible without our invention," he said.

The CCD technology makes use of the photoelectric effect, as theorized by Albert Einstein and for which he was awarded the 1921 Nobel Prize. By this effect, light is transformed into electric signals. The challenge, when designing an image sensor, was to gather and read out the signals in a large number of image points, pixels, in a short time.

The CCD is the digital camera's electronic eye. It revolutionized how images were collected from spacecraft, by telescopes, and in medical imaging, and has eventually replaced the film camera in every aspect of photography.

Related Physics Today articles on fiber optics
Maurer and Kao win Ericsson Prize, May 1979
An Overview of Lightguide communication, Solomon J. Buchsbaum, May 1976
The fiber lightguide, Alan G. Chynoweth, May 1976
Fiber optics, Alastair M. Glass, October 1993
The golden age of optical fiber amplifiers, Emmanuel Desurvire, January 1994


Related Physics Today articles on CCDs
Charge-coupled devices would be cheap, compact Gloria B. Lubkin, October 1970
From photons to bits, Rajinder P. Khosla, December 1992

Other Related Physics Today Resources
Industrial R&D in transition, R. Joseph Anderson and Orville R. Butler, July 2009
The bell tolls for Bell Labs Toni Feder, October 2008
Industry R&D forecast is bullish despite concerns over talent dearth, Jermey N. A. Matthews, April 2008
Bell Labs fissions, yielding AT&T Bell Labs and Bellcore, Gloria B. Lubkin, May 1984

Related Resources
2009 Physics Nobel Prize Resources American Institute of Physics
A 2004 oral history interview with Charles K. Kao IEEE History Center
A 2001 oral history interview with George E. Smith IEEE History Center

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Science: In the coming weeks, on the plains of Inner Mongolia, China plans to launch its first large-scale effort to capture and store carbon emissions.

A new coal-to-liquid plant in Erdos will burn coal to make, at the outset, a little over 1 million metric tons per year of diesel and other petrochemicals. Operated by China's biggest coal producer, Shenhua Group, the plant will generate as a byproduct about 3.6 million tons of carbon dioxide (CO2) a year. In an effort to make carbon capture pay, much of the gas will be sequestered in nearby oil reservoirs, where pressure from the CO2 will force hard-to-get oil to the surface.

Shenhua's plant is one of two pivotal carbon capture and storage efforts in China. The other is GreenGen, an integrated gasification combined cycle (IGCC) plant that the Chinese government approved last June for construction in Tianjin.

Instead of pulverizing coal as a conventional power plant does, IGCC plants turn it into gas, which allows for easy separation of CO2 from combustible gases--and far easier CO2 capture. If successful, GreenGen could redefine how power is generated from coal in China, says Richard Morse of the Program on Energy and Sustainable Development at Stanford University in Palo Alto, California. "You could make a very strong case that it's the leading carbon-capture project for coal-fired power in the world," he says.

London Times Online: The Lunar Crater Observation and Sensing Satellite (LCROSS) will blast two huge chunks out of the lunar surface on Friday in order to have a closer look at what the Moon is made of.

The plume will be created by dropping the Centaur upper stage of the rocket that fired LCROSS to lunar orbit onto the surface near one of the lunar poles.

When the 2.4-tonne Centaur hits the ground, it will be traveling at 2.5km per second, and throw up a plume of debris 10km high that can be analyzed by instruments on the LCROSS spacecraft.

Physics Today: An article in the London Times that suggesting the UK was considering pulling out of the CERN has caused consternation in the physics community, and denials from the Science and Technology Facilities Council (STFC), but a review of the UK's science expenditure is ongoing.

The Science and Technology Facilities Council (STFC) has suffered from a financial crisis caused by over-spending on some high-profile projects such as the Diamond synchrotron light source. In response, STFC has cut back some grants and support for some facilities, and is conducting a major science review through its advisory panels, and with input from the science community and STFC's international partners. The report is due in December. The STFC has "to live within constrained budgets if need be, and to diversify our funding base," says STFC's Keith Mason.

A misquoted article

The Times article misquoted the STFC's chief operating officer Richard Wade, says Mason and took other comments out of context.

The UK's agreement with CERN is governed by an international treaty, and could only be changed with UK Government approval and with consultation with the other CERN partners, it cannot be made unilaterally by the STFC alone. It was the strength of this international agreement that during the 1980s, protected the UK's particle physics community's membership of CERN but also allowed the UK to negotiate a reduction in its membership fees.

CERN membership did however, have a knock on effect of leading to cuts in other areas of UK particle physics.

A vision for today

"The STFC's position in relation to the LHC is made clear in our July vision document," says Mason, "which states that 'our highest priority in particle physics is to exploit the Large Hadron Collider at CERN'."

The vision document also says that the UK's highest priorities in ground-based astronomy is to exploit membership of the European Southern Observatory, which gives access to the Very Large Telescope and to the ALMA millimeter astronomy array, and to carry out R&D towards the next generation European Extremely Large Telescope. The UK is also heavily involved in the proposed Square Kilometer Array radio telescope.

A bleak UK budget

However, the public sector, which funds the majority of research in the UK, is expected to suffer significant cuts next year because of the recession. The ongoing science review will "ensure STFC is prudently prepared for the tougher budget environment," says Mason, and "ask tough questions about the future direction of our science and technology program, including the balance between [science] disciplines."

The consultation encompasses all of STFC's programs, and includes an examination of the cost-effectiveness of international subscriptions, including CERN, the European Southern Observatory, the ILL neutron source and others.

"All UK publicly-funded bodies have a responsibility to ensure value-for-money," says Mason, "and STFC has discussed with our international partners the need to restrain costs and, if possible, reduce expenditure."

The next few months will be challenging says Mason, "but an exciting opportunity [for STFC] to set the course for the future."

Paul Guinnessy

Nature: Two experiments that produce laser light by exploiting the collective wave-like motion of free electrons on a metal surface bring the science and technology of lasers into the realm of the nano-scale.

New Scientist: The first of the asteroid-hunting Pan-STARRS telescopes will be taken apart today in an effort to solve problems with image quality.

The 1.8-metre PS1 telescope is the first of a suite of instruments—the Panoramic Survey Telescope and Rapid Response System - designed to find asteroids and comets with orbits that could bring them close to Earth. Sited atop a volcano on the Hawaiian island of Maui, PS1 is the prototype for a planned four telescopes that will image the whole sky visible from Hawaii three times each month.

To scan so much sky, PS1 boasts a 1.4-billion-pixel digital camera and specially designed software to process the terabytes of data collected by the telescope each night.

But since the camera was installed in 2007, the telescope team has been struggling to get PS1's image quality to its targeted level. "There have been problems that we just didn't anticipate," says Pan-STARRS principal investigator Nick Kaiser of the University of Hawaii at Manoa.

Physics Today: Images from the Herschel observatory, obtained during the performance verification phase, reveal previously unseen detail in a region of the Milky Way near the Galactic Plane.
Herschel_image.jpg
Copyright: ESA and the SPIRE & PACS consortia.
This composite image above has been constructed from a series of images taken by two instruments: SPIRE (SPIRE is a three band imaging photometer and an imaging fourier transform spectrometer) and PACS (an imaging photometer and integral field line spectrometer for wavelengths between 60 and 210 µm.) The image uses color coding the different observed wavelengths: the blue denotes 70 µm, green is 160 µm emission, while red is the combination of the emission from all three SPIRE bands at 250/350/500 µm. The color-coding differentiates material that is extremely cold (red) from that which is slightly warmer. The image contains an incredible network of filamentary structures with surprising features indicative of a chain of near-simultaneous star-formation events, glittering rather like beads of water on a string in the sunlight. The images are of a 2x2 degree field in an area near the Galactic Plane, 60 degrees from the Galactic Centre, in the constellation of the Southern Cross. This area of the night sky is considered to be a good test case for the telescope as the area is crowded with many molecular clouds along the line-of-sight, which should show whether the telescope can resolve fine detail easily. The images shown here were obtained on 3 September 2009 and are based on just over 6 hours of observations. Since stars form in cold, dense environments, the composite image easily locates the star-forming filaments that would be very difficult to isolate from a map made at a single far-infrared or submillimeter wavelength.

NPR: In a new biography called The Strangest Man: The Hidden Life of Paul Dirac, Mystic of the Atom, author Graham Farmelo digs deep into the archives and personal papers of a Nobel-winning physicist.

0FB96ED0-7099-4E16-9ED8-835B800EE2A5.jpgYou can also read an interview of Paul Dirac through the American Institute of Physics's history center.

Oral History Transcript—Paul Adrien Maurice Dirac

NYTimes.com: The world leaders who met at the United Nations to discuss climate change this week are faced with an intricate challenge: building momentum for an international climate treaty at a time when global temperatures have been relatively stable for a decade and may even drop in the next few years.

The plateau in temperatures has been seized upon by skeptics as evidence that the threat of global warming is overblown. And some climate experts worry that it could hamper treaty negotiations and slow the progress of legislation to curb carbon dioxide emissions in the United States.

Scientists say the pattern of the last decade—after a precipitous rise in average global temperatures in the 1990s—is a result of cyclical variations in ocean conditions and has no bearing on the long-term warming effects of greenhouse gases building up in the atmosphere.

But trying to communicate such scientific nuances to the public—and to policy makers—can be frustrating, they say.

Nature: In 1992, three years after the fall of the Berlin Wall, a spy walked into the US embassy in Warsaw and offered to sell the CIA the real and code names of all intelligence agents from the HVA (Hauptverwaltung Aufklärung)—the foreign department of the Stasi, the East German Ministry for State Security. The CIA bought the highly sensitive information for a mere US$75,000.

The spoils—released to the Berlin Stasi archive and made available to history professor Kristie Macrakis at the Georgia Institute of Technology in Atlanta in 2005—have the potential to alter popular perceptions of the activities of the East German intelligence agency and secret police.

Macrakis's analysis of the CIA material reveals that about 40% of all HVA sources planted in West German companies, research institutions, and universities were stealing scientific and technical secrets.

Physics Today: Earlier this week Alan Taub became the new vice president of Research and Development for General Motors. Despite going into and out of bankruptcy, GM is still one of the largest companies in the US that conducts industrial R&D.

taub.jpgTaub (see left image) has run GM's eight science labs for the last nine years and was a key player in building GM's newest R&D lab in Shanghai that officially opened last month.

In his new role, Taub will still coordinate all the advanced technical work within GM, but will be more closely involved in managing GM's collaborative R&D ventures with academia, the Department of Energy, and other strategic partners.

Physics Today Online was lucky enough to ask some questions in a public webcast held on Tuesday. An edited transcript is below.

[Question]: What is the future of fuel cells within the new GM, do we have enough funds to run them?

Taub: Fuel cells are still an important activity for General Motors. And part of the solution to diversifying the energy source for vehicles. We remain committed to developing the technology but as we approach early commercialization, the costs of development are increasing.

[Question]: How do you envision the global R&D organizations work together? How will "who does what" be determined?

Taub: Working with my leadership team, we select the competencies to be developed at each of the eight R&D labs'. Multidisciplinary teams then integrate the labs programs globally to gain the most effective results. The competency selection for each site is based on availability of talent.

[Question]: Why do you believe globalization of GM's R&D activities is necessary?

Taub: Innovation and breakthrough research are enabled by diversity—diversity of education, the working environment and the local marketplace. We have been successful at having researchers located in different sites globally and bringing their ideas together so the team has more perspectives for new ideas.

[Question]: The easiest way to improve fuel efficiency is to cut down on weight. The New York Times had an article on how 60% of the weight of a car is due to steel, and how new types of steel are going into cars to provide safety and lightness. What is GM doing in this area, do you do the basic R&D yourself or do you rely on your partners?

Taub: In the past 15 years, we have dramatically changed the [steel] material mix on vehicles. For example, GM is increasing it's usage of high-strength steels to the point that in the next 10 years we will see very little low-carbon steel in the structural bodies of GM vehicles.

As well as changing the steel mix, GM is also increasing usage of aluminum and magnesium. This is accomplished by collaborations of GM and supplier engineers as well as precompetitive research with Ford and Chrysler in US.

[Question]: Battery technology seems to have significant limitations. Is GM looking at ultra-capacitors as well?

Taub: Yes, we are looking at batteries, fuel cells and ultracapacitors as energy storage devices. We see a role for each.

saturn-vue-two-mode-full2.jpg[Question]
Will you use the plugin technology from the canceled Saturn Vue "two-mode" hybrid in any other small SUVs in the future?

Taub: All we said so far is that the technology will go into another GM product. Stay tuned.

[Question]: To succeed, GM needs world class scientists. After bankruptcy, how does it propose to attract and retain them?

Taub: We have been successful at attracting the best and the brightest from around the world to the various GM global laboratories. People are intrigued by the combination of deep technical assignments on products that make a difference to consumers everywhere.

[Question]: We've seen impressive demos on Vehicle to Vehicle communications technology from GM. What are the remaining obstacles to introducing this technology into the marketplace?

Taub: We are continuing "harden" the technology in order to enable commercialization. Because this is a safety-related technology, it must be robust. It also requires standards for all of GM's suppliers since the vehicle parts needs to interact. There is progress being made on all fronts.

[Question]: What do you see as the biggest challenge in transitioning to wide-spread electric vehicle use?

Taub: Two things. Getting the cost down and the supply base ready.

[Question]: What is your personal favorite research topic at the moment?

Taub: Clearly, it is the electrification of the vehicle. Batteries, motors, hydrogen fuel cells are dominating the research portfolio. At the same time, the connected vehicle (e.g. navigation, OnStar, infotainment) is probably the most fun because we get to implement it at consumer electronics speed.

[Question]: Do you envision GM R&D researchers doing fundamental researchers? Or do you see the researchers act as project managers, and the universities act as the actual researchers?

Taub: The answer is both. Inside GM, we have the world's best individual contributors performing leading edge research on critical automotive applications. They do their work inside our walls while collaborating with the best professors and engineers in universities and national labs.

[Question]: Can you speak to GM's R&D center in Honeoye Falls, New York, the role its played so far, and the type of role it might play moving forward?

Taub: Honeoye Falls is the site of one of our eight global laboratories. It is our main site for fuel cell stack research and more recently battery system research. It will continue to be an important element of our research infrastructure.

[Question]: How's that shape-changing NiTinol material coming along. Any production plans on the horizon?

Taub: Our first application is being deployed as we speak. I just can't tell you at this time what that vehicle is.

[Question]: I wonder what makes fuel cells expensive? It seems very affordable for a new technology. If a fuel cell car has 100 grams of platinum, which is about $3000-4000, the rest of the materials involved is not that much expensive.

Taub: There are many elements that contribute to the cost of vehicle components. Raw material is only one aspect. On the fuel cell stack, our next-generation technology dramatically reduces the platinum loading, making it competitive with that on after-treatment for internal combustion engines.

[Question]: What is the research focus of the science lab in China?

Taub: Glad you asked. I am just back from Shanghai and the jet lag is almost gone. The initial areas of attention are improving the efficiency of internal combustion engines, lightweight materials and the joining technology for those materials, emerging market safety, consumer research methodologies and batteries.

[Question]: How far into the future do think it will be before we see automated cars driving on the expressway?

Taub: I'm on the record for promising limited autonomy driving on highways by 2015. This is enabled by a combination of lane keeping and stop-and-go adaptive cruise control.

[Question]: How does GM R&D foster a culture of innovation and creativity while simultaneously having researchers be accountable for their work and in tune with the overall cost of their projects?

Taub: Welcome to the challenge of leading an industrial research laboratory. We pull on our researchers to solve the tough problems facing the industry while adding to the world's scientific knowledge base. We lead the industry in patents—we filed more than 600 within R&D alone last year—and lead in technology implementation in the product.

[Question]: In your introduction you talked about "mainstreaming R&D." What does this mean and is GM allowing other employees to contribute ideas?

Taub: R&D is now fully integrated into Product Development at GM. That is allowing us to get more streamlined in our technology development and implementation activities. We are always looking for good ideas from both inside and outside the company. Feel free to contact any of our group managers, lab directors or me if you don't know who else to email.

[Question]: The development of the next generation of fuel-efficient vehicles requires advancements and a deep understanding across a wide range of materials (electrode materials for batteries, catalysts for fuel cells). How do you draw the line between what GM can develop and what must be developed by others to make a particular technology successful? Basically how deep into basic research does GM want to go?

Taub: The make-buy decision is different for every technology. For example, stamping of metals for the key components of the vehicle is a core technology within GM. The plastic parts are generally purchased from suppliers. The recent decision to vertically integrated into battery pack manufacturing does not mean we would be manufacturing our own battery cells. However, we are working internally on next-generation cell technology in collaboration with various suppliers.

Various: Two earthquakes caused devastation across the Pacific earlier this week. One, based off the coast of Samoa caused a tsunami; the other, near Sumatra, was so deep that no tsunami occurred, but the loss of life on the surrounding area may be greater.

"The chances of there being a connection between these two earthquakes is extremely slim," said University of Ulster geophysicist John McCloskey, told the London Times. The 10,000 km distance between the quakes and the orientation of the tectonic plates made a causal link physically implausible, he said.

"The real danger in the coming days is that a second larger quake with a magnitude of around 8.5 could occur just off the coast of Padang," Professor McCloskey said. That could result in a huge tsunami submerging the town and surrounding coastline, which has a population of about 1.5 million.

A magnitude 6.6 event off the coast of Sumatra happened earlier today.

The tsunami earthquake

The tsunami that devastated the islands of Samoa, American Samoa, and Tonga was the result of a shallow rupture in the earth's crust on one of the most geologically active areas of the world—where the Pacific plate is plunging westward under the Australia plate at a rate of 86 mm a year.

The earthquake, which was measured as high as 8.3 on the Richter scale, occurred 190 kilometers southwest of American Samoa. The event caused one side of the fault line to push up several meters higher than the other side, according to initial estimates.

Gary Gibson, a senior seismologist at Environmental Systems and Services in Melbourne, told Australia's ABC network that the energy released in the earthquake was approximately one-thirtieth the size of the Boxing Day 2004 earthquake near the island of Sumatra, Indonesia.

Gibson also mentioned to the Sydney Morning Herald that this earthquake was unusual in that it was due to a north-east to south-west tension in the crust. "The earth [was] being stretched rather than compressed," he said.

After the earthquake, the Pacific Tsunami Warning Centre issued a tsunami warning for South Pacific nations, including New Zealand, which experienced a rise in sea level of 40 cm, but Samoa, American Samoa and Tonga were too close to the initial event to get enough warning.

"People who live in areas where tsunamis can occur are generally educated about them," said John Bellini, a geophysicist with the National Earthquake Information Center in Denver, Colorado. "If you feel an earthquake, get to high ground as fast as you can." In this case, he adds, "Five minutes was not enough time for emergency services to move into action."

Analysis of the data indicated that Hawaii was too far away for any major tide rise to occur.


Related Links
Map of the two earthquakes
Sumatra and Samoa earthquakes were inside the 'Ring of Fire' fault lines London Times
Samoan tsunami caused by 'shallow quake'
When two plates collide: rupture set off wave Sydney Morning Herald
Tsunami forecasts quicker, more accurate Honolulu Advertiser
Tsunami warning system unable to help Samoans Inside Science

Science: After spending nearly 2 decades developing China's first space-based observatory, Li Tipei now fears that the project may never get off the ground.

china_x_ray_satellite.jpgThe Hard X-ray Modulation Telescope (HXMT) mission is scheduled for launch next year, but with the clock running down, Science has learned that no government agency has stepped forward to pay the estimated US$146 million to build the satellite—putting the mission in jeopardy.

li_tipei.jpg"It would be a shame for the Chinese scientific community if the project dies prematurely," says Li, an astrophysicist and chief mission scientist at the Chinese Academy of Sciences Institute of High Energy Physics (IHEP) and Tsinghua University.