LHC Update: July 31, 2009

July 31, 2009 | 9:54 am

This week’s issue of the CERN Bulletin reports on the suspected cause of two vacuum leaks discovered in mid-July that have pushed the LHC restart date until at least November. The likely culprit is a flexible hose in the liquid helium transport circuits. The same type of hose caused a vacuum leak in another LHC sector two years ago, which was fixed by replacing the flexible hose with a smaller, solid tube. If the flexible hose is confirmed as the cause of the new leaks, it will be repaired using the same technique.

In other LHC repair news, Science magazine reports today that more bad connections between superconducting magnets may reduce the maximum energy for the LHC’s first run, or further delay the restart.

Katie Yurkewicz

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In the works: a movie starring subatomic particles and two Star Trek captains

July 31, 2009 | 5:00 am

Dave the Photon Courtesy of Jupiter 9 Productions.

Dave the Photon (Image from the Jupiter 9 Productions Web site.)

TrekMovie.com has posted an interesting review of a new movie that highlights the study of space and touches on particle physics in a unique and fun way.

Quantum Quest: A Cassini Space Odyssey blends education and entertainment though the use of 3D computer-generated animation and footage from seven NASA space missions, including the Cassini Huygens mission to Saturn.

Audience members will get a tour of the outer planets and moons of our solar system while meeting the movie’s cast of characters, which includes a photon, neutrino, proton and an evil genius, The Void, who represents “nothingness” and seems to have traits similar to dark matter and dark energy.  A number of celebrities lend their voices to characters, including former Star Trek captain William Shatner as The Core, a figure that represents the sun and knowledge, and, arguably, all visible matter.

From a press release:

The full voice cast includes Chris Pine (Captain Kirk in J.J. Abrams’
upcoming “Star Trek XI” feature film), Samuel L. Jackson (”The Spirit,”
“Pulp Fiction,” “Star Wars”), Hayden Christensen (”Jumper,” “Star Wars”),
Amanda Peet (”X-Files Movie 2,” “The Whole Nine Yards”), Robert Picardo
(”Stargate Atlantis”), Jason Alexander (”Seinfeld”), Tom Kenny (voice of
“Sponge Bob Squarepants,” “Transformers”), Sandra Oh (”Sideways,” “Grey’s
Anatomy”), Brent Spiner (”Independence Day,” “Star Trek: Next
Generation”), James Earl Jones (”Star Wars”), William Shatner (”Boston
Legal,” “Star Trek”), Mark Hamill (”Star Wars”), Neil Armstrong, Doug
Jones (”Pan’s Labyrinth,” “Abe Sabien – Hell Boy”), Abigail Breslin
(”Little Miss Sunshine,” “Kit Kittredge: An American Girl”), Spencer
Breslin (”The Happening”), Gary Graham (”Alien Nation,” “Enterprise”),
and Janina Gavankar (”The L Word”).

The movie features the voices of two Captain Kirks (veteran William
Shatner and Chris Pine, star of JJ Abrams’ upcoming “Star Trek” movie)
and two Darth Vaders (James Earl Jones and Hayden Christensen) — a first
for Hollywood and a first for the galaxy.

The movie is expected to appear in theaters worldwide sometime in 2010 in IMAX and conventional 3D format. It is the brainchild of Jupiter 9 Productions producer Harry Kloor, who has Ph.D.s in physics and chemistry and has written for the Star Trek franchise.

The movie was initiated by NASA’s Jet Propulsion Laboratory as part of the outreach program for the Cassini Huygens space mission in 1996.  About once a week for the nine months leading up to the film’s release, its creators will post video clips and supplemental educational material on the film’s Web site.

The main Web site has limited movie clips available so far, but computer-generated images posted with the TrekMovie.com story look amazing. It doesn’t look anything like your typical education-based film, and the story definitely seems worth a read.

Tona Kunz

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Tiny droplets carry proteins, viruses into the paths of bright x-ray imagers

July 30, 2009 | 5:00 am

John Spence, a physicist at Arizona State University, is a longtime user of the Advanced Light Source at Lawrence Berkeley National Laboratory, where he has contributed to major advances in lensless imaging. It’s a particularly apt propensity for someone who works with x-rays, since they can’t be focused with ordinary lenses.

As new light sources evolve to produce brighter x-rays in faster pulses, lensless imaging becomes ever more critical for science. Among the promises of superbright, ultrafast x-ray pulses is the ability to solve the structure of the complicated molecules from which our bodies are made. All living things are made of proteins and nucleic acids, but relatively few of the atomic structures of the thousands, perhaps millions, of varieties of proteins are known.

The Linac Coherent Light Source (LCLS) will soon begin operation at the SLAC National Accelerator Laboratory in Menlo Park, California, using energetic electrons from a linear accelerator to produce coherent x-rays with an instrument called a free electron laser (FEL). The x-rays will be delivered 120 times a second in pulses only a tenth of a trillionth of a second long – about the time it takes light to travel the width of a human hair. These brief, bright pulses offer a novel approach to the problem of protein structure.

Unfolding the origami

Proteins begin as strings of amino acids that fold themselves into an amazing variety of origami-like structures, whose bumps and crannies and distribution of electrical charges determine how they act individually or fit together to form complex molecular machines. Simple organisms like viruses often consist of a few proteins fitted together to enclose a thread of DNA or RNA.

Proteins are usually large molecules containing many thousands of atoms. Drug molecules are much smaller, and do their work by attaching themselves to the larger protein molecules. A knowledge of the arrangement of a protein’s atoms is therefore a great help to drug designers, who like to understand how a drug molecule will dock with a protein to promote or inhibit its activity, or cripple the organism of which it is a part.

Until now, the best way to solve the structure of a protein or virus has been with x ray crystallography. The crystal consists of many copies of the protein or virus arranged in regular order. As the crystal rotates in the x-ray beam, x-rays scatter off the atoms and reveal – once these complex diffraction patterns have been converted into a 3-D image by computers – how the electrons, and thus the atoms, are arranged.

But many proteins can’t be crystallized at all, and others are so difficult to crystallize it’s virtually impossible to obtain crystals large enough to use in today’s light sources.

Ultrafast, ultrabright x-rays offer a way past this dilemma. The idea is that a quick pulse of tightly focused x-rays can be diffracted from a microcrystal or even a single protein or virus in solution. The pulse is so brief that it comes and goes before any of the atoms can move, freezing their orientation like a strobe light. Just as important, a sufficiently brief pulse may terminate before radiation damage effects can start. In this way it can outrun radiation damage, always one of the fundamental limitations to imaging in biology.

Another quick pulse could be diffracted from another copy of the protein in a different orientation. As the process is repeated, diffractions from different angles give the overlapping views needed for the computer to construct a 3-D image of the structure.

It’s a great idea, but as Spence notes, there are a few problems. “So as not to scatter, the x-ray beam has to be in a high vacuum, but a protein or virus in its natural state is usually wet. As in T. S. Eliot’s Wasteland, water is life. How do we maintain the protein or virus in an aqueous environment inside the vacuum?”

Shot from a microcannon

The answer was what Spence calls a “particle gun, like an ink-jet printer,” designed to inject a beam of water droplets across the tightly focused x-ray beam in single file, each droplet so small it contains only a single protein or virus. He and colleagues Bruce Doak and Uwe Weierstall of ASU designed a nozzle that can fire liquid droplets, each less than a millionth of a meter in diameter (one micrometer), faster than hundreds of thousands of times a second. The sample jet is designed to shoot droplets right through a pulsed beam of x-rays a billion times brighter than any ever created in a light source before.

It wasn’t easy. Nozzles made of solid material like glass invariably clog up, limiting droplets to at best 20 micrometers across. What Spence and his colleagues wanted was a jet of particles less than a micrometer in size. ASU postdoc Dan DePonte has done most of the recent hard work needed to make it all function.

The frequency at which droplets emerge is controlled by an acoustic trigger, which can be tuned so that each droplet containing a protein or virus meets an incoming pulse of x rays.

The frequency at which droplets emerge is controlled by an acoustic trigger, which can be tuned so that each droplet containing a protein or virus meets an incoming pulse of x-rays.

Back in 1878 Lord Rayleigh, a professor of experimental physics at Cambridge University, discovered that a smooth, cylindrical jet of liquid emerging from an orifice spontaneously breaks up to form a train of spherical droplets. In the late 1990s, physicist Alfonso Gañán-Calvo of the University of Seville found a way to surround the streaming liquid with pressurized gas to make a co-flowing liquid sheath. By adjusting gas and liquid pressure and other parameters, he was able to create a “virtual nozzle” that could shrink the diameter of the liquid jet to a thread so small it would not clog the physical aperture of the tube. In effect, the gas sheath acts to focus the liquid stream.

Spence and his colleagues needed a true microthread of liquid, however, one that produced droplets sized a millionth of a meter or less. In their nozzle, liquid flows through a narrow capillary inside the tube through which the gas flows; the liquid issues from the capillary some distance from the opening in the outer tube, so the gas surrounds it, then increases speed and pressure as it approaches the opening, squeezing and accelerating the thin stream of liquid until it is so small that the proteins or viruses dissolved in the liquid can only fit into the droplets one at a time.

And the nozzle won’t clog, because even a particle bigger than the sample protein or virus – bigger than the stream of liquid itself – can still fly through the glass nozzle without hitting the walls and getting stuck.

The frequency at which the droplets emerge can be controlled by an oscillator the researchers call an “acoustic trigger.” Tuning the acoustic trigger adjusts the frequency so that each droplet containing a protein or virus meets an incoming pulse of x-rays.

The entire device – which the researchers call a gas dynamic virtual nozzle (GDVN) – is only about a millimeter in diameter (not counting feed lines and cables) and fits to the side of the beamline’s vacuum chamber. After passing through the beam, the liquid droplets and the gas (typically carbon dioxide) freeze in a trap opposite the injection point, without significantly reducing the vacuum.

The liquid flows through a narrow capillary, issuing some distance from the opening in the outer tube through which the gas flows. Approaching the narrow opening, gas pressure and speed increase, focusing the thin stream of liquid until it is so small only a single protein or virus can fit into each droplet.

The liquid flows through a capillary, issuing some distance from the opening in the outer tube through which the gas flows. Approaching the narrow opening, gas pressure and speed increase, focusing the thin stream of liquid until it is so small only a single protein or virus can fit into each droplet.

In 2008 Spence and his colleagues, including Berkeley Lab’s David Shapiro, successfully tested the GDVN on the Advanced Light Source beamline 9.0.1, managed by Berkeley Lab’s Stefano Marchesini. The test was done with protein microcrystals extracted from the fluid in which researchers were attempting to grow larger crystals. These are the smallest protein nanocrystals from which diffraction patterns have ever been obtained, and the first from membrane protein nanocrystals – among the most resistant to crystallization.

Although the microcrystals weren’t individual protein specimens, and while the 9.0.1’s x-ray beams aren’t as bright or as rapidly pulsed as SLAC’s LCLS will be, the experiment demonstrated the jet technique’s high potential for speeds and exposures that won’t subject the samples to radiation damage. Some of the patterns the researchers obtained come from nanocrystals just a few molecules on a side, with a width of about 100 billionths of a meter (100 nanometers). At SLAC, the researchers plan to steadily reduce the nanocrystal size down to single molecules.

The corresponding reduction in scattered intensity will hasten and improve lensless imaging. The first step in lensless imaging is scattering the beam from the sample; the second step is constructing the image by interpreting and combining the data from the diffracted x-rays.

In order to merge the different views (projections) of an object, which is subsequently vaporized in this “diffract-and-destroy” mode, it is important that they all be identical. In biology, that leaves only molecules like proteins and viruses. DNA or RNA inside a virus is often packed differently in each virus, and cells are not identical at the molecular level, so cannot be studied in 3-D by this method.

Besides identical particles, successful data-merging also depends partly on knowing how the sample was oriented in the beam – easy to do with a large crystal, not so easy to do with a sample inside a drop of liquid whizzing across the beam. It may be possible to orient flying droplets by optical methods such as polarized laser beams or with specially shaped nozzles.

Perhaps simpler is to use the ever-increasing power of the computer – which for a lensless imaging system is where most of the functions of a lens reside. Computer systems have been developed that infer the orientation of the sample from the diffraction pattern itself, even when as few as four percent of the pixels in the detector light up. It does take a lot of diffraction patterns to derive an image this way – as many as 10 million – which will take the LCLS a few hours until better ways of orienting the droplets can be devised.

Nevertheless, Spence’s group recently obtained excellent diffraction patterns of MS2 virus capsids at the ALS by subtracting the diffraction “noise” of the liquid jet itself. These capsids, made in Mat Francis’s lab at the University of California at Berkeley, are the shells of the virus lacking its RNA genome and have the regular shape of buckyballs. Eventually the LCLS will be able to get a good diffraction pattern from a target like this with a single ultrabright pulse. In this case, however, computer processing was able to derive an excellent pattern by averaging diffraction from a series of samples.

DePonte will soon install Spence and Doak’s ultrafine, ultrafast “inkjet printer,” tested at the ALS, on the powerful new SLAC machine. It will be the first step into a bold new future for investigating the biological universe, one big molecule at a time.

Additional information

X-ray imaging beyond the limits,” by Henry N. Chapman, appeared in Nature Materials, April, 2009.

Powder diffraction from a continuous microjet of submicrometer protein crystals,” by D. A. Shapiro, H. N. Chapman, D. DePonte, R. B. Doak, P. Fromme, G. Hembree, M. Hunter, S. Marchesini, K. Schmidt, J. Spence, D. Starodub, and U. Weierstall, appeared in the Journal of Synchrotron Radiation, November, 2008.

Gas dynamic virtual nozzle for generation of microscopic droplet streams,” by D. P. DePonte, U. Weierstall, K. Schmidt, J. Warner, D. Starodub, J. C. H. Spence, and R. B. Doak, appeared in the Journal of Physics D: Applied Physics, 19 September, 2008.

By Paul Preuss

This article first appeared on July 28, 2009 on the Berkeley Lab News Center.

Guest author

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The CERN Courier's 50th anniversary issue

July 29, 2009 | 5:00 am

Issue one of the Cern Courier

Issue one of the CERN Courier

For those who enjoy a nostalgic look back, the CERN Courier has posted a treat:  The very first issue of the Courier, which started as an in-house newsletter and now reaches 25,000 subscribers around the world.

Writing in the July/August issue, CERN Director-General Rolf Heuer notes that both the European lab and the Courier have changed beyond recognition since the first issue came out 50 years ago:

One thing that has stayed the same, however, is the magazine’s openness to the world. Issue number 1 reported not only on progress towards starting up the PS [Proton Synchrotron], but also carried news of the City of Hamburg’s purchase of a 40 MeV linac for a new lab known as the Deutsches Elektronen Synchrotron. Back then, the Courier felt the need to spell out the DESY acronym. There was also news from the US, including bold ambitions for linear accelerator developments at Stanford University. CERN’s mission of bringing nations together for peaceful collaboration is witnessed by a report from a trip to the USSR, precursor to a long and fruitful collaboration with the Joint Institute for Nuclear Research at Dubna.

The anniversary issue highlights five decades of science from the Courier archives, from the 1959 announcement of the first beam in the Proton Synchrotron (news so fresh that the issue had to be made over at the last minute to fit it in) to accelerator milestones, particle discoveries, Nobel Prizes, the invention of the World Wide Web and the startup of the Large Hadron Collider. 

As someone who loves browsing through old postcards and magazines — and who owns a 55-year-old issue of Life magazine from the month I was born — I have to say I love this stuff:  The typefaces, then so modern and now so charmingly retro; the pastel pages; the thought of how much harder it was back then to put out a publication like this one; and the language of a dynamic, yet more genteel time, as in this request for suggestions from page 8 of issue one:

You don’t have to sign them. If you believe you might blush in seeing your name in print in our next issue, or if modesty prevents you from being further associated with your idea, then just drop us a note “incognito.”  You may be sure your appeal will always receive due consideration, even if it is not so tender to us.  Editors are — and should be — rugged people…

That, at least, has not changed!

We wish the Courier  a very happy anniversary and many exciting reports ahead.

Glennda Chui

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Bowling for neutrinos

July 28, 2009 | 5:00 am

Bonnie Fleming is bowling for neutrinos

Bonnie Fleming is bowling for neutrinos.

What do you get when you bring together a neutrino physicist and the son of a bowling champion who made his name as a host for an MTV dating show?

You get a very entertaining and accessible video with an explanation of research into neutrinos, one of the most elusive building blocks of matter.

WIRED Science host Chris Hardwick joined Fermilab physicist and Yale University professor Bonnie Fleming at a Chicago bowling alley to discuss her career and his hobby. They look at the similarities between neutrinos and bowling and learn that smashing atoms apart for a living doesn’t necessarily translate into being good at sending pins flying.

The brief video is part of the Careers in Science feature of WIRED Science, a weekly TV series arising from a partnership with Wired Magazine and PBS. Wired explains the show’s goal on its Web site as:

Each week, WIRED Science correspondents take viewers to the frontiers of discovery across the country and around the world, spotlighting the cutting-edge innovations and research that are defining 21st-century culture, and introducing the high-tech mavericks who are making it happen.

That description fits Fleming, who has worked on several of the leading neutrino projects of the decade, including MiniBooNE, the experiment that searched for a fourth neutrino; ArgoNeuT, the first U.S.-based liquid-argon neutrino detector test, which just recorded its first neutrino; and a proposal to create the world’s longest-baseline neutrino experiment by using a neutrino beam from Fermilab, Illinois, to a site in South Dakota.

Tona Kunz

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Q&As on Higgs search article in Parade magazine

July 27, 2009 | 7:47 am

This Sunday, Parade – the 16-page magazine inserted into more than 30 million copies of Sunday newspapers – featured an article on the search for the elusive Higgs boson at the Fermi National Accelerator Laboratory in Illinois. This blog provides links to some background information and a list of Q&As related to the Parade article.

The article’s author, Stephen Fried, an adjunct professor at Columbia University Graduate School of Journalism and a writer for national magazines, visited Fermilab in April to interview scientists and take a tour of the laboratory. A few weeks before his visit, Fermilab had announced in a press release its most stringent constraints on the mass of the Higgs particle. Scientists expect that either the Tevatron particle collider at Fermilab or the Large Hadron Collider at the European laboratory CERN will produce a signal for the Higgs particle in the next couple of years.

Fried had the chance to see the LHC Remote Operations Center at Fermilab, where more than 300 people gathered for a pajama party the night of September 9-10 to celebrate and watch via video conference the startup of the LHC accelerator in Europe. He toured the CDF and DZero collider experiments at Fermilab and interviewed Fermilab Director Pier Oddone. He saw the laboratory’s Main Control Room and learned about the applications of particle physics technology in medicine and industry.

His article “The Race for the Secret of the Universe” is a superb example of how one can tell an exciting particle physics story in less than 1300 words without skimping on the details.

In response to the Parade article, people have submitted questions to Fermilab. Here are the answers. I’ll post more as they come in.

Q: Why is the Higgs boson called “the God particle”? 
A: In the early 1990s, Nobel laureate Leon Lederman wrote a book on particle physics and the search for the Higgs boson. According to Lederman, his publisher came up with the title “The God Particle” for the book, hoping it would attract more attention than a conventional particle physics title. Well, it worked. But among scientists, the nickname is frowned upon.

Q: How does a Higgs boson make matter?
A: In addition to a Higgs boson, there is a Higgs field. The field permeates the entire universe. In physics, that concept is nothing unusual. Physicists also know of gravitational fields, electromagnetic fields, etc. The Higgs field gives mass to elementary particles such as electrons and quarks. I like to think of the Higgs field as an invisible fog that fills the universe, and the Higgs bosons are tiny droplets – condensation – in the fog. Elementary particles such as electrons interact with the Higgs field by just being surrounded by it. Different particles interact with the Higgs field with different strength. That’s why an electron is much lighter than a top quark.

Q: What is a Higgs boson made of?
A: A Higgs boson does not contain smaller particles, according to our current understanding. Instead, the Higgs boson is the localization of a tiny amount of energy in space. Scientists also call it a resonance. It is a resonance of the Higgs field and it requires a specific amount of energy to be produced. (That’s why it is called a resonance.) Albert Einstein discovered that energy and mass are equivalent: E=mc2. Hence energy can produce particles (resonances), and particles can convert back into energy. When a particle collision sets free the right amount of energy, it can produce a Higgs boson. The energy is transformed into the mass of the Higgs boson. But low-energy collisions such as the collisions of molecules in a gas don’t have enough energy to produce the Higgs boson. They won’t do the trick. Scientists must use high-energy particle accelerators to produce high-energy particle collisions. Scientists think that particle accelerators such as Fermilab’s Tevatron and CERN’s Large Hadron Collider can produce particle collisions that have enough energy to produce a Higgs particle. Once a Higgs boson is produced, it decays quickly into lighter particles, converting some of its mass back into the mass and kinetic energy of lighter particles.

Q: How small is a Higgs boson?
A: The theoretical framework that accurately describes the behavior of all particles, known as the Standard Model of particles and their interactions, requires elementary particles such as quarks, leptons and bosons to be point-like particles. They have zero diameter. This might seem weird, but after all, these elementary particles do not contain any smaller building blocks. In contrast, composite particles – such as the proton – have a finite, non-zero diameter. In the case of the proton it is 10-15 meters. That is tiny, but it provides plenty of space for the (zero-diameter) quarks inside a proton.

Q: What are leptons and quarks?
A: Scientists know of six quarks and six leptons. They are elementary particles (that means they contain no smaller particles as far as we know). They are the most fundamental building blocks of all matter on Earth. Their names are:
up quark, down quark, strange quark, charm quark, bottom quark, top quark;
electron, electron neutrino, muon, muon neutrino, tau, tau neutrino.
The Standard Model of particles and interactions describes how quarks and leptons interact with each other through the exchange of bosons. For more information, check out the Particle Adventure.

Q: Are quarks and leptons part of an atom?
A: Yes. An atom is made of electrons (which are a type of lepton) and an atomic nucleus made of protons and neutrons. Those protons and neutrons are made of quarks. Hence an atom contains both quarks and leptons. An atom is larger than a proton, and a proton is larger than a quark.

Q: What is the Big Bang theory?
A: Based on the measurements of the motion of stars and galaxies, scientists know that the universe is expanding. Examining the history of the universe and – like an archeologist – discovering older and older galaxies and other cosmic objects and phenomena, scientists found that all matter in the universe came from a single outburst of energy larger than anyone can imagine - the Big Bang. Here is a NASA Web site that explains in more detail what the Big Bang theory is and it lists in great detail all the experimental observations that again and again have confirmed the Big Bang theory. Today’s telescopes and measurements are so precise that scientists have determined that the Big Bang occurred 13.7 billion years ago. But what triggered the Big Bang and what was before the Big Bang are unknown.

Q: How is the Higgs boson related to the Big Bang theory?
A: The Big Bang was an enormous outburst of particles and radiation (energy). The Higgs field endowed elementary particles such as quarks and leptons with mass. As the universe expanded and cooled, particles started to clump together, eventually forming simple atoms such as hydrogen and helium. If there were no Higgs field (or something else that gives elementary particles mass), the electron would have no mass and atoms would not form. There would be no chemical bonding, no stable structures, no Earth and no physicists.

Q: Does the Higgs make atoms?
A: No, other forces are responsible for making atoms. But without the Higgs, the electron would have no mass and atoms could not form. Since electrons do have mass, they are slow enough to be captured by atomic nuclei via the electromagnetic force and form atoms.  

Q: Could there be more to an atom than many scientists think, or have all possibilities been explored?
A: Science is about making measurements and observations, finding explanations, predicting the outcome of new experiments based on those explanations, and carrying out experiments to test the predictions and, if necessary, make changes to the explanations. Scientists are always looking for new ways to test the makeup and behavior of atoms. So far, experiments again and again have confirmed our current understanding of what an atom is and what it is made. But some day an experiment could, for example, show that electrons – one of the building blocks of all atoms - are made of even smaller building blocks themselves. Then scientists would need to refine the current theory and develop an explanation that explains everything that is already known and the new observation. Developing better experimental tools and designing clever experiments is the only way to find out whether our current explanations are not yet complete.

Kurt Riesselmann

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Fermi telescope captures a solar eclipse

July 24, 2009 | 3:31 pm

Voltage data from the solar-charged battery onboard the Fermi Gamma-ray Space Telescope for the days prior to and including the July 22 solar eclipse. (Image: Fermi Gamma-ray Space Telescope Collaboration.)

Voltage data from the solar-charged battery onboard the Fermi Gamma-ray Space Telescope for the days prior to and including the July 22 solar eclipse. (Image: Fermi Gamma-ray Space Telescope Collaboration.)

The Fermi Gamma-ray Space Telescope was launched to study gamma rays, not sunshine.  Yet that’s what it has done, most recently last week, when one of its instruments registered signals from a solar eclipse.

Shawne Workman writes in today’s edition of SLAC Today :

During Wednesday’s total solar eclipse, the moon blacked out the sun from vantage points in India, Asia and the Pacific Ocean for as long as 6 minutes, 39 seconds. Of course, it also shadowed the intervening space, between the moon and Earth—including, by chance, a swath of the Fermi Gamma-ray Space Telescope’s orbit.

The telescope passed through the eclipse at roughly 3:30 Universal Time (3:30 a.m. at zero longitude, or 8:30 p.m. PDT). The main power voltage to the Large Area Telescope took a dip as the sun’s power-charging rays hid behind the moon. The eclipse created a downward spike in the LAT’s regular cycle of increasing voltage as the battery charges in the sun, followed by a drop as the battery discharges during the telescope’s brief night.

It turns out that the sun itself is a source of gamma rays, although very faint ones.  They’re created when high-energy cosmic rays hit the sun’s atmosphere.  So the LAT can watch the sun moving across its field of view in a matter of hours against a background of stars, and is monitoring those emissions around the clock and in high quality for the first time, according to principal investigator Peter Michelson. Read more here from the Feb. 19, 2009 issue of SLAC Today.  Here’s a scientific poster  about that work, as well as coverage of Michelson’s talk in science journalist Ivan Semeniuk’s Embedded Universe blog.

Glennda Chui

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Fermilab stars in new documentary

July 24, 2009 | 5:00 am

Fermi National Accelerator Laboratory has become quite the movie star, with connections to three films released in the last twelve months.

The latest is The Matter of Everything, a documentary produced by Canadian filmmakers. It takes a look at quantum physics through the work done at Fermilab. Here’s a trailer. The film has several showings in Canada this summer. For those south of the border, a DVD is available on the filmmakers’ Web site.

The Web site states:

The Matter of Everything is a feature documentary that explores quantum reality and the interconnectedness of nature from the quantum to the universe. Challenging us to see beyond our everyday sense of experience, the film reveals what we are, a billionth of a billionth of the human scale. At that level, physicists at Fermilab, one of the world’s largest particle accelerators, describe a world more unified than ever imagined.

Through her interviews, Olga Antzoulatos, a non-science educator, soon finds that “the human scale is not preferred for understanding nature – even on the human scale” as physicist Chris Quigg notes.

The scientists involved in the film are: Janet Conrad, Enrico Lunghi, Arlene Lennox, Chris Quigg, Rocky Kolb, Peter Skands, Paul Delaney, Paul Nienaber Sr., and Scott Menary.

Courtesy of 137 Films

Poster for The Atom Smashers. Courtesy of 137 Films

Fermilab also was featured in the Chicago-based documentary The Atom Smashers, which was released last fall. It aired on PBS’s Independent Lens and was showcased at science and film festivals in several countries. PBS Channel WYCC will broadcast the film on August 20. The documentary highlights the race between Fermilab’s Tevatron experiments and CERN’s Large Hadron Collider experiments to find the Higgs boson, the particle that explains why elementary particles have mass.

Antimatter canister from "Angels & Demons". Courtesy of Sony Pictures

Hollywood invention: antimatter canister from "Angels & Demons." Courtesy of Sony Pictures

This spring, particle accelerators and antimatter were featured in the Hollywood movie Angels & Demons, starring Tom Hanks. The movie featured footage shot at the European laboratory CERN, and particle physicsists around the world used the opportunity for a lecture series on the science behind Angels & Demons.

Since 1985, Fermilab has produced more than nine nanograms (billionth of a gram) of antiprotons, more than any other laboratory. But even this amount is about 100 million times less than the amount that thieves steal from CERN in the Angels & Demons movie.

 Learn more about how and why Fermilab produces and captures antimatter in this 8-minute podcast by Keith Gollwitzer, head of Fermilab’s antiproton source.

Tona Kunz

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Antimatter from bananas

July 23, 2009 | 8:56 am

U.S.-based scientists and students working on research and experiments with the Large Hadron Collider contribute to a blog supported by the National Science Foundation and the Department of Energy that offers articles about particle physics and insight into the life as a physicist. This week, Flip Tanedo, a graduate student at Cornell University, posted an interesting entry on bananas and antimatter.

Positrons from bananas

July 21, 2009

I was recently preparing a “Physics of Angels & Demons” talk for a group of high school physics teachers who were visiting Cornell for a “Contemporary Physics for Teachers” workshop. While researching natural sources of antimatter, I discovered a curious article about a naturally occurring potassium isotope that, some fraction of the time, decays via positron emission. The conclusion was that:

“The average banana (rich in potassium) produces a positron roughly once every 75 minutes.”

Now any time you find something like this you have to remember that not everything on the Internet is true – not even Wikipedia, but I checked it out (e.g. the LBNL/Lunds table of isotopes) and indeed this seems to be correct!

Potassium-40 is a naturally occurring isotope that is unstable and decays, but it has a huge half life, about a billion years. These days only a small fraction (100 parts per million) of potassium atoms are actually Potassium-40, but objects that are dense in potassium – such as bananas – are likely to have tens of micrograms of the stuff. If one crunches the numbers (as they do in the original article), it turns out that bananas pop out a positron every 75 minutes or so.

These positrons quickly annihilate with ambient electrons, perhaps undergoing some other interactions and releasing some photons beforehand. I’m sure the bloggers here who work on LHC calorimetry would have a better description of what happens to it! Advanced readers can read the “Passage of particles through matter” section of the PDG.

Potassium plays a necessary role in our biology, so yes, even you produce positrons every once in a while.

by Flip Tanedo

Find Tanedo’s original blog and other LHC-related blogs at the US LHC Blog Web site.

Note: Discover magazine had an interesting article on radiation exposure a couple of years ago. That article stated:

Eating 600 bananas is about the equivalent of having one chest X-ray.

The article also lists other sources of radiation – radon, medical, cosmic rays. According to the article, the average American gets a dose of radiation roughly the equivalent of 36 X-rays per year.

Guest author

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Photo contest turns lens on research at DESY

July 22, 2009 | 9:36 am

Courtesy DESY

Photographers search DESY for interesting images during the first Science Photo Walk. Photo: DESY

This spring, two German research centers, the Deutsches Elektronen-Synchtrotron and the GKSS Research Centre, invited 100 amateur photographers to aim their cameras at research. The first Science Photo Walk gave researchers and the public alike a new perspective on the ways people view science.

The visitors captured more than 2500 images. A selection of 150 photos from the event is available online, allowing an inside glimpse at cutting-edge facilities and providing insight into the researchers’ world.

The images captured everything, including camp beds set up for a night shift, technical details in the cryogenic hall, and researchers carefully handling research samples.

The public and a laboratory-organized committee each voted to pick the top three winners of the photo contest. Interestingly, the two groups chose entirely different images. The 50 best images went on display at an exhibit in the Levantehaus mall in Hamburg in May.

Tona Kunz

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