The accelerator and the carpenter

May 29, 2009 | 5:46 pm

Part of the wooden sculpture named for the Large Hadron Collider.

Carpenters at DESY never expected to rebuild the Large Hadron Collider–but they did part of it, out of wood. Now, that 1/25th scale model of the LHC’s ATLAS detector, featured in this month’s symmetry, isn’t the only wooden interpretation of the experiment.

Russian artist Nikolay Polissky creates “land art,” which consists of large structures built from many smaller, individually shaped pieces of wood. His latest piece is called Large Hadron Collider, and is Polissky’s tribute to the massive experiment. Inspired by the deep connection LHC scientists have with the natural world, Polissky made drawings of metal machinery, wires, and cables that he and his team of carpenters carved out of wood. The entire piece consists of many separate structures, all resembling pieces of an odd wooden playground, with some of them towering over fifteen feet tall.

Now you can watch a video documenting the entire process of planning, carving, and building the installation.

Images of the piece can be found on Polissky’s website or in this press release from the Mudam Museum in Luxembourg, where the piece will be shown.

Calla Cofield

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Theorists reveal path to "true muonium"

May 29, 2009 | 10:00 am

In this artist's depiction of how experimentalists could create true muonium, an electron (blue) and a positron (red) collide, producing a virtual photon (green) and then a muonium atom, made of a muon (small yellow) and an anti-muon (small purple). The muonium atom then decays back into a virtual photon and then a positron and an electron. Overlaying this process is a figure indicating the structure of the muonium atom: one muon (large yellow) and one anti-muon (large purple). (Graphic: Terry Anderson, SLAC.)

In this artist's depiction of how experimentalists could create true muonium, an electron (blue) and a positron (red) collide, producing a virtual photon (green) and then a muonium atom, made of a muon (small yellow) and an anti-muon (small purple). The muonium atom then decays back into a virtual photon and then a positron and an electron. Overlaying this process is a figure indicating the structure of the muonium atom: one muon (large yellow) and one anti-muon (large purple). (Graphic: Terry Anderson, SLAC.)

True muonium, a long-theorized but never-seen atom, might be observed in future experiments, thanks to recent theoretical work by researchers at the Department of Energy’s SLAC National Accelerator Laboratory and Arizona State University. True muonium was first theorized more than 50 years ago, but until now no one had uncovered an unambiguous method by which it could be created and observed.

“We don’t usually work in this area, but one day we were idly talking about how experimentalists could create exotic states of matter,” said SLAC theorist Stanley Brodsky, who worked with Arizona State’s Richard Lebed on the result. “As our conversation progressed, we realized ‘Gee…we just figured out how to make true muonium.’”

True muonium is made of a muon and an anti-muon, and is distinguished from what’s also been called “muonium”-an atom made of an electron and an anti-muon. Both muons and anti-muons are created frequently in nature when energetic particles from space strike the earth’s atmosphere. Yet both have a fleeting existence, and their combination, true muonium, decays naturally into other particles in a few trillionths of a second. This makes observation of the exotic atom quite difficult.

In a paper published this week in Physical Review Letters, Brodsky and Lebed describe two methods by which electron-positron accelerators could detect the signature of true muonium’s formation and decay.

In the first method, an accelerator’s electron and positron beams are arranged to merge, crossing at a glancing angle. Such a collision would produce a single photon, which would then transform into a single true muonium atom that would be thrown clear of the other particle debris. Because the newly created true muonium atoms would be traveling so fast that the laws of relativity govern, they would decay much slower than they would otherwise, making detection easier.

In the second method, the electron and positron beams collide head-on. This would produce a true muonium atom and a photon, tangled up in a cloud of particle debris. Yet simply by recoiling against each other, the true muonium and the photon would push one another out of the debris cloud, creating a unique signature not previously searched for.

“It’s very likely that people have already created true muonium in this second way,” Brodsky said. “They just haven’t detected it.”

In their paper, Lebed and Brodsky also describe a possible, but more difficult, means by which experimentalists could create true tauonium, a bound state of a tau lepton and its antiparticle. The tau was first created at SLAC’s SPEAR storage ring, a feat for which SLAC physicist Martin Perl received the 1995 Nobel Prize in physics.

Brodsky attributes the pair’s successful work to a confluence of events: various unrelated lectures, conversations and ideas over the years, pieces of which came together suddenly during his conversation with Lebed.

“Once you pull all of the ideas together, you say ‘Of course! Why not?’ Brodsky said. “That’s the process of science-you try to relate everything new to what you already know, creating logical connections.”

Now that those logical connections are firmly in place, Brodsky said he hopes that one of the world’s colliders will perform the experiments he and Lebed describe, asking, “Who doesn’t want to see a new form of matter that no one’s ever seen before?”

Kelen Tuttle

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Simulating a more efficient linear collider

May 28, 2009 | 10:32 am

An electromagnetic mode contributing to wakefield effects in a superconducting ILC cavity, as calculated by SLAC's Advanced Computations Department team. Reds, oranges, and yellows indicate strong fields, greens and blues weaker ones. (Image courtesy of Cho Ng.)

An electromagnetic mode contributing to wakefield effects in a superconducting ILC cavity, as calculated by SLAC's Advanced Computations Department team. Reds, oranges and yellows indicate strong fields, greens, and blues weaker ones. (Image courtesy of Cho Ng.)

Scientists around the world are working hard to hammer out a workable blueprint for the next big particle accelerator, the International Linear Collider, by 2012. A group at SLAC National Accelerator Laboratory is doing its part, running supercomputer simulations to maximize the accelerator’s performance and keep costs down on the proposed multi-billion-dollar collider.

The team, from SLAC’s Advanced Computations Department, or ACD, is researching how to minimize the effects of charge “wakes” in the ILC, which will smash electrons and positrons into each other. As bunches of these particles race down accelerator tracks, electromagnetic wakes rise behind them. These wakefields can make the going rough for bunches to come, causing some particles to stray off course. As a result, beam quality can suffer and heat can build up inside accelerator cavities, potentially degrading their performance.

The more powerful the accelerator beam, the greater the potential wakefield effects. And the ILC’s beam will be powerful, generating collision energies of about 500 billion electronvolts-ten times what SLAC’s linac is capable of producing.

“Wakefields are an important issue for the ILC,” said SLAC physicist Kwok Ko, head of ACD. “Controlling them is key.”

To supplement planned wakefield experiments run on scaled-down ILC models–which are in the works at Fermilab–the SLAC team is running computer simulations. Such research, a marriage of physics and computational science, is what ACD does so well, and what makes the group unique. Other institutions have physicists and computational scientists on staff, but ACD, which was created in 2001, brings five researchers from each field together under one roof.

“ACD is the first department in the Department of Energy accelerator complex that has put together a team like this–physicists and computational scientists working together to solve big problems,” Ko said.

Simulations of particle behavior in an accelerator, while much faster and cheaper than hardware experiments, are complicated endeavors. For one thing, they require specialized computer codes, which the SLAC group has been key in developing. From 2001 to 2005, Ko co-led a project, funded by the DOE’s Scientific Discovery through Advanced Computing program, to hash some out. Two of his colleagues in ACD, Lie-Quan Lee and Cho Ng, are working on a current SciDAC project to improve upon the original algorithms and thus better tackle the ILC wakefield problem.

SLAC's team is using the Jaguar supercomputer to model wakefield effects. (Image: National Center for Computational Sciences, Oak Ridge National Laboratory.)

SLAC's team is using the Jaguar supercomputer to model wakefield effects. (Image: National Center for Computational Sciences, Oak Ridge National Laboratory.)

The wakefield work also demands a huge number-crunching capacity. In 2007, the DOE awarded the SLAC team an Innovative and Novel Computational Impact on Theory and Experiment grant. It was good for 4.5 million processor hours on Jaguar, a DOE supercomputer at Oak Ridge National Laboratory that can perform 1.64 quadrillion operations per second. This past December, the SLAC researchers got another INCITE grant, this one for eight million hours on Jaguar. They still have about 6.5 million hours left.

“We expect to use them all by the end of the year,” said Lee, computational mathematics group leader in ACD.

As currently planned, the ILC will consist of two 14-kilometer-long linear accelerators facing each other. The basic unit of each accelerator is a meter-long cavity. Nine cavities make up one super-cooled, superconducting cryomodule, of which the ILC will contain about 3000. The SLAC scientists are unbowed by this scale and complexity.

“If you can understand one cryomodule, you have a better understanding of how the whole machine will work,” said Ng, deputy department head of ACD.

And the researchers are well on their way to doing that. They have modeled wakefield effects throughout an entire cryomodule, finding that ILC designers can reduce wakefields considerably by providing enough damping. Absorbers between cryomodules–already part of ILC design–mean that wakefield effects across these accelerator components may not be a major factor.

Such findings could improve the collider’s efficiency and make it more affordable. Building accelerator cavities will make up about 30 percent of the ILC’s total price tag, according to the ILC’s Global Design Effort. So improving the cavities even slightly–damping wakefield effects and thus reducing heating loads, for example–could minimize maintenance costs, leading to big savings.

“That was the motivation behind this simulation work,” Lee said.

The team is confident that their simulations mirror reality. They benchmark all of their codes, comparing their results against experimental data and models employing other software packages. The researchers found their codes to be accurate within 0.01 percent. Further, their techniques are applicable to other particle accelerators, not just the ILC. Using the same codes, they recently performed a simulation for the Thomas Jefferson National Accelerator Facility in Virginia. The SLAC team’s work showed that one cavity in a prototype cryomodule was eight millimeters shorter than it should have been–a measurement engineers confirmed when they looked at the actual machine. This fabrication error was identified as the cause of beam breakup in the cryomodule.

“We really can use simulation to solve a real-world problem,” Ng said. “That’s very exciting.”

For more information about the SLAC team’s ILC simulation work, see “Watching Wakefields to Keep Particles on Track.”

by Michael Wall

This story first appeared in SLAC Today on May 28, 2009

Symmetry Intern

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May 2009 issue of symmetry now online

May 27, 2009 | 1:06 pm

Scientists can feel like they are swimming in a sea of names in modern collaborations of more than 1000 physicists, where youre just one on a very long A-to-Z list of authors on published results. So how can individuals be recognized for their efforts and distinguished from others when it comes to promotion and tenure decisions?

Scientists can feel like they are swimming in a sea of names in modern collaborations of more than 1000 physicists.

In the new issue of symmetry, read about how scientists find ways to stand out in collaborations with hundreds of thousands of members, the recently upgraded “charm factory” in Beijing, a profile of CERN Director-General Rolf-Dieter Heuer, a guide to the Standard Model of particle physics through Nobel Prizes, a gallery of Da Vinci-style drawings of the latest particle physics experiments, and the discovery of the Van Allen radiation belts.

See the full table of contents.

David Harris

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Peering at the people and process of particle physics

May 26, 2009 | 10:25 am

Colliding Particles – Episode 1: Codename Eurostar from Mike Paterson on Vimeo.

For years, Large Hadron Collider documentaries focused on the project’s engineering and construction challenges, scientific goals, or doomsday scenarios. The scientists who appeared in the films were usually there to explain the Higgs boson, or how thousand-ton detector pieces are lowered underground. But recently, some documentary producers have shifted their attention to the lives of the people who make the LHC and other particle physics experiments a reality.

The online documentary series Colliding Particles follows this trend, delving into the lives and work of one of the hundreds of research groups working on the LHC experiments, and documenting the process of scientific research. Each 7-10-minute-long episode focuses on a different aspect of the scientific process. In the four episodes available so far, viewers are introduced to the group members and the LHC, visit the ATLAS experiment on the day of LHC startup, tag along to a particle physics conference, and learn about how theoretical and experimental physicists work to resolve problems.

While the episodes make great viewing on their own (and include some cool chalk-drawing style animations), educators can go even further. The Colliding Particles team has put together a set of teaching resources that includes powerpoint presentations, student activities and ‘classroom edits’ of each episode in various formats. Created with the support of the United Kingdom’s Science and Technology Facilities Council Science and Society Programme, the teacher resources are designed specifically for the ‘How Science Works’ element of the UK curriculum, but, like the scientific process itself, could transcend national borders.

Katie Yurkewicz

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The LHC quench protection system

May 22, 2009 | 1:46 pm

The new quench protection system (QPS) has the crucial roles of providing an early warning for any part of the superconducting coils and busbars that develop high resistance, as well as triggering the switch-off of the machine. Over 2000 new detectors will be installed around the LHC to make sure every busbar segment between magnets is monitored and protected.

One of the major consolidation activities for the LHC is the addition of two new detectors to the quench protection system. A magnet quench occurs when part of the superconducting cable becomes normally-conducting. When the protection system detects an increased resistance the huge amount of energy stored in the magnet chains is safely extracted and ‘dumped’ into specially designed resistors. In the case of the main dipole chain, the stored energy in a single LHC sector is roughly the same as the kinetic energy of a passenger jet at cruising speed.

The first new detector is designed to monitor the superconducting busbars, including the joints between segments–the part that caused the incident in Sector 3-4 last September. The new system can measure the busbar resistance to about 1 nano-ohm (one billionth of an ohm) and will provide an early warning for any joint that develops high resistance.

“With this detector in place, we would have caught the ‘bad joint’ in Sector 3-4 two days earlier–safely in time to prevent any damage”, explains Knud Dahlerup-Petersen from the Quench Protection team. In total, 2132 of these detectors will be installed around the machine, so that every busbar segment between the magnets will be monitored.

The second new detector protects against ‘symmetric quenches’. It was originally planned to add this second phase of the protection system during the first winter shutdown period. In February this year, however, it was decided that the system should be in place before the LHC restart. “So it has been a real effort to catch up, but our group (TE/MPE) had a lot of help from other groups, mainly TE/EPC and other departments, in particular PH and EN, and we’re now fairly confident that the whole system will be ready in time”, says Petersen.

Symmetric quenches were only discovered in June last year during the campaign of training quenches in sector 5-6. When a magnet quenches, a symmetric quench can occasionally occur in the neighbouring magnets. It is caused by the heat transfer between the magnets, but it is particularly difficult to detect as the quench develops identically in both parts of the magnet coils which are used for the quench signal. The existing detection system compares the voltage signals from the two coils to detect a resistive build-up in either one. However if the quench develops in both at the same time, the two voltage signals remain the same, and the quench goes unnoticed.

The new protection system monitors the voltage across 4 adjacent dipoles (or 2 adjacent quadrupoles), allowing a symmetric quench to be detected and also provides a back-up detection method for ‘normal’ (asymmetric) quenches. However, the 4-magnet measuring system is based on digital quench detector technology, as opposed to analogue electronics used in the present QPS system. “It is notoriously difficult to find digital electronics that will not degrade in the high-radiation environment, so we had to choose the components carefully.” Says Petersen. “We have now fully radiation-tested the first prototype, and we are basically ready to start mass production of the so-called SymQ detector board.”

The thousands of new detector boards will be housed in 436 crates around the LHC. As the complex design lead to a relatively long R&D period there’s now not enough time to tender production out to an external company. Therefore, a production line for assembling of the complete protection units has been set up in a CERN workshop.

Another important measure taken is the consolidation of the network of Uninterruptable Power Supplies (UPS), designed and operated by EN/EL. The UPS provide power to all the essential parts of the machine, including the quench protection system, even if there is a problem with the mains grid. However, the UPS was not completely fail-safe as certain parts were not fully redundant. During the energy extraction, which takes up to 6 minutes in the dipole circuits, the magnet system remained unprotected in the event of a UPS failure. New cables have been laid and modifications applied to the UPS to make sure that the part of the UPS which powers the QPS systems is completely backed-up.

This story first appeared in the CERN Bulletin today.

Guest author

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LHC update: May 22, 2009

May 22, 2009 | 1:42 pm

From the CERN Bulletin today:

New test diagnostics are being developed to measure the electrical resistance of the copper component of the superconducting busbars, specifically within the interconnections that join the busbars together (see previous update). The first test is very precise but requires local access to the interconnection, which therefore needs to be open. A second test has been developed that can be performed externally using voltage tap connections. This allows the resistance of a 30-40m segment to be measured without opening interconnections. The two methods have been checked to give consistent results and can be used to identify the interconnections with the highest resistances, which are subsequently repaired. In parallel simulations and laboratory tests are also being carried out. All dipole interconnections in the four sectors have been measured at room temperature. Work is ongoing to measure the quadrupole lines, which have much longer busbar segments. A further test is currently being developed to be performed at cryogenic, but non-superconducting temperatures, to allow the rest of the machine to be checked.

The installation work on the pressure release ports of the inner triplets magnets has now been completed.

Guest author

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A side of cloud with your grid, ma'am?

May 21, 2009 | 10:34 am

Belle II co-spokesman Masanori Yamauchi (left) with 2008 Nobel prize winner in physics Makoto Kobayashi. Image courtesy of Belle II.

Belle II co-spokesman Masanori Yamauchi (left) with 2008 Nobel prize winner in physics Makoto Kobayashi. Image courtesy of Belle II.

As the cloud becomes a more popular computing solution in the commercial world, it is starting to pique the interest of the academic research community. Collaborators of the experiment at the High Energy Accelerator Research Organization, known as KEK, in Japan are considering supplementing their computing with Amazon’s Elastic Compute Cloud (EC2), which provides on-demand, virtual computing resources over the Internet.

The KEKB particle accelerator produces a more densely-packed, intense beam than any currently operating collider, and an upgrade to the machine in 2013 is expected to increase the intensity by a factor of 50. The new Belle II detector will come online at the same time equipped to handle the estimated hundred-fold increase in data—expected to total 40 petabytes per year. This load will require more than 100,000 CPU cores, leading the collaboration to consider new computing options, said Martin Sevior, a KEK collaborator based at the University of Melbourne in Australia.

Sevior and his colleagues ran the complete Belle simulated data analysis chain on EC2 to test it, and found it easy to deploy jobs. They created an Amazon Machine Image (AMI), a computing environment customized to contain both the Scientific Linux operating system and applications for the Belle analysis system. Each AMI contains eight CPU cores—imagine eight PCs—and can be duplicated 20 times, creating a virtual 160-core cluster. To lower costs, the team set up an automation system that duplicates the AMI on demand and shuts down instances of it as need drops.

Martin Sevior. Image courtesy of M. Sevior.

Martin Sevior. Image courtesy of M. Sevior.

CPU usage is not consistent in high-energy physics experiments, so building a data center to satisfy peak demand would result in significant periods of underutilization. Since EC2 allows flexibility in scaling, Sevior said, a possible solution might be a hybrid system where the cloud provides for peak demand and the grid supplies base-load resources.

Sevior is concerned about remaining challenges, however. Although EC2 works nicely at the scales tested so far, it may not be feasible at the scales needed by Belle II in 2013. Pricing may need to come down before then, too, if it is to be a competitive option. Finally, he suspects that Belle II’s requirements for data production may exceed Amazon’s capacity to transfer the data back to the Belle II grid.

“EC2 is competitive for jobs that need a lot of resources for a short time, but we have not yet demonstrated it will be useful for the very large-scale needs of Belle II,” Sevior said. “What is clear is that we will need a distributed computing solution very much like a conventional grid and are currently planning to employ gLite for the bulk of our computing. Our investigations are to see to what extent cloud computing can or should supplement this.”

by Amelia Williamson

This story first appeared in International Science Grid This Week on May 20, 2009.

Guest author

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The mural a half-mile underground

May 20, 2009 | 10:44 am

Minnesota artist Joseph Giannetti painted this mural on the rock wall near the MINOS detector.

Minnesota artist Joseph Giannetti painted this mural on the rock wall near the MINOS detector.

It seems unnecessary to put windows in an office located half a mile underground. But even if the employees of the Soudan Underground Laboratory cannot watch the clouds roll by as they sit at their desks, many of them gaze through the blinds at a color-soaked 25-by-60-foot mural painted on the rock wall.

An old ore mine in northern Minnesota houses the laboratory, home to the detector for the Main Injector Neutrino Oscillation Search experiment. Minnesota artist Joseph Giannetti created the mural, which represents the laboratory’s work. He stood on a window-washer’s platform and painted while others pieced together the detector below, said Soudan Mine Assistant Lab Manager Jerry Meier.

“In order to make everything look right because the rock is so rough, he had to use a projector to project his image on the rock,” Meier said. “Then he would paint on it and move the projector over and paint another part.”

The MINOS experiment is a long-baseline neutrino experiment that searches for neutrino oscillation — neutrinos changing from one type to another. To do this, physicists fire a beam of neutrinos straight through the earth from Fermilab in Illinois to the Soudan Mine in Minnesota. It takes the subatomic particles a fraction of a second to complete the 450-mile trip.

Physicists study the make-up of the beam using two detectors, one at the source of the neutrinos at Fermilab and the other in the Soudan Mine. Because neutrinos travel at the speed of light, physicists need to place their detectors far away to give the neutrinos time to oscillate. The MINOS collaboration members are studying neutrino oscillation to see whether it can answer questions about the abundance of matter in the universe.

The mural by the MINOS detector is full of representative images, such as the faces of famous physicists and a picture of the iconic Wilson Hall at Fermilab, the laboratory which creates the beam of neutrinos the MINOS detector studies.

Some of the mural’s images are more apparent than others, Meier said. Faces hide in the shadows of bat wings. The word “change,” written in different languages, is tucked throughout the mural.

“It’s like a treasure hunt,” Meier said. “You have to find every little bit.”

Listen to an interview with Meier about the mural.

To see a key that labels several of the images in the mural, check out this symmetry deconstruction piece.

Kathryn Grim

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Mystery of the cosmos hidden in a coffee cup?

May 19, 2009 | 6:37 am

You will never look at your coffee the same way again.

Your coffee cup, it seems, can do much more than contain the jolt of energy you need to start your day. It may hold the key to understanding the mysterious 25 percent of the universe that acts as an invisible source of gravity holding galaxies together and influencing the motion of stars.

According to a Duke University study funded by the National Science Foundation,  “A Duke University professor and his graduate student have discovered a universal principle that unites the curious interplay of light and shadow on the surface of your morning coffee with the way gravity magnifies and distorts light from distant galaxies.

Seeing a gravitational lens in a wine glass

“They think scientists will be able to use violations of this principle to map unseen clumps of dark matter in the universe. “

Back in 2005 in the second issue of symmetry, we ran an “Explain it in 60 seconds” about gravitational lensing in which postdoc Phil Marshall described his very geeky party trick of using a wine glass to help explain gravitational lensing, the topic of this new Duke work. That gravitational lensing in a wine glass experiment also shows the light curves known as caustics along with the multiple images caused by gravitational lenses.

Perhaps all the secrets to the universe can be found in the crockery and glassware of the dinner table!

Update: Thanks to @kristazala for a great alternative title for this story in a tweet: “Coffee chiaroscuro explains dark matter in a light roast”

Tona Kunz

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