A milestone for ArgoNeuT

July 3, 2009 | 5:00 am


A screen capture of ArgoNeuT's first neutrino interaction event, as seen by induction and collection wire planes in the detector.

A screen capture of ArgoNeuT's first neutrino interaction event.

The Argon Neutrino Teststand, or ArgoNeuT, has seen its first neutrino–the first one observed by a liquid argon detector in the United States.

We at symmetry have closely followed the ArgoNeuT’s voyage.  For one thing, it’s named for the Argonauts, a brave band of mythical explorers led by Jason in search of the Golden Fleece; this makes for many fine nautical metaphors and puns. It has a time projection chamber–very cool, even though it has nothing whatsoever to do with time travel. Cooler still, this liquid argon technology may offer a cheaper, more efficient way to capture neutrinos, mysterious particles that may hold the key to why the universe is made of matter, and therefore to why we exist; for details, see this feature in the August 2008 issue of the magazine.

Subsequent updates reported ArgoNeuT’s first observations of cosmic rays–an important step in testing and calibrating the detector–and the lowering of the detector into a Fermilab tunnel 350 feet below ground, where it’s shielded from those same troublesome rays.

Now here’s the latest, from Wednesday’s Fermilab Today:

“Liquid-argon detectors can achieve high accuracy in determining the type of particle interaction. Because of this, they are very good at rejecting background events. These detectors can also get the same measurements as much larger detectors that use different technologies,” said Brian Page, a graduate student at Michigan State University who works on ArgoNeuT.

ArgoNeuT, a small, 175-liter, liquid-argon-filled detector, sits upstream of the MINOS detector in the neutrino beamline. Neutrinos from the NuMI beamline enter the ArgoNeuT detector chamber and interact with argon atoms. The interactions produce light and charged particles, which continue to travel through the argon and knock electrons loose. A wire plane attracts these electrons, which induce electrical signals. The data collected helps scientists reconstruct a 3-D image of the original interaction event.

Scientists lowered the experiment, commissioned in 2008, into a detector hall in January 2009. It was filled with liquid argon this May, and saw the first interactions on May 27.

“Seeing the neutrino interactions is another step towards showing us that we can build these detectors for the long baseline neutrino oscillation program at the proposed Deep Underground Science and Engineering Laboratory,” said Bonnie Fleming, ArgoNeuT spokesperson.

All we can say is: Smooth sailing!

Glennda Chui

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Data-taking dress rehearsal proves world’s largest computing grid is ready for LHC restart

July 1, 2009 | 2:38 pm

The Worldwide LHC ComputingGrid is gearing up to handle the massive amount of data expected shortly after the restart of the Large Hadron Collider.

Read how CERN is preparing to take record-setting amounts of data in this Interactions press release.

And read in the press release below how Brookhaven National Laboratory and Fermi National Accelerator Laboratory will lead the US portion of the data distribution.

Tape storage at Brookhaven National Laboratory's Tier-1 computing center. Image Credit BNL

Tape storage at Brookhaven National Laboratory's Tier-1 Computing Center. Photo Courtesy of BNL.

BATAVIA, IL and UPTON, NY–The world’s largest computing grid has passed its most comprehensive tests to date in anticipation of the restart of the world’s most powerful particle accelerator, the Large Hadron Collider (LHC). The successful dress rehearsal proves that the Worldwide LHC Computing Grid (WLCG) is ready to analyze and manage real data from the massive machine. The United States is a vital partner in the development and operation of the WLCG, with 15 universities and three US Department of Energy (DOE) national laboratories from 11 states contributing to the project.

The full-scale test, collectively called the Scale Test of the Experimental Program 2009 (STEP09), demonstrates the ability of the WLCG to efficiently navigate data collected from the LHC’s intense collisions at CERN, in Geneva, Switzerland, all the way through a multi-layered management process that culminates at laboratories and universities around the world. When the LHC resumes operations this fall, the WLCG will handle more than 15 million gigabytes of data every year.

Although there have been several large-scale WLCG data-processing tests in the past, STEP09, which was completed on June 15, was the first to simultaneously test all of the key elements of the process.

“Unlike previous challenges, which were dedicated testing periods, STEP09 was a production activity that closely matches the types of workload that we can expect during LHC data taking. It was a demonstration not only of the readiness of experiments, sites and services but also the operations and support procedures and infrastructures,” said CERN’s Ian Bird, leader of the WLCG project.

Cables at Fermilab's Grid Computing Center. Image Credit Fermilab

Cables at Fermilab's Grid Computing Center. Photo Courtesy Fermilab.

Once LHC data have been collected at CERN, dedicated optical fiber networks distribute the data to 11 major “Tier-1″ computer centers in Europe, North America and Asia, including those at DOE’s Brookhaven National Laboratory in New York and Fermi National Accelerator Laboratory in Illinois. From these, data are dispatched to more than 140 “Tier-2″ centers around the world, including 12 in the United States. It will be at the Tier-2 and Tier-3 centers that physicists will analyze data from the LHC experiments–ATLAS, CMS, ALICE, and LHCb–leading to new discoveries. Support for the Tier-2 and Tier-3 centers is provided by the DOE Office of Science and the National Science Foundation.

“In order to really prove our readiness at close-to-real-life circumstances, we have to carry out data replication, data reprocessing, data analysis, and event simulation all at the same time and all at the expected scale for data taking,” said Michael Ernst, director of Brookhaven National Laboratory’s Tier-1 Computing Center. “That’s what made STEP09 unique.”

The result was “wildly successful,” Ernst said, adding that the US distributed computing facility for the ATLAS experiment completed 150,000 analysis jobs at an efficiency of 94 percent.

A key goal of the test was gauging the analysis capabilities of the Tier 2 and Tier 3 computing centers. During STEP09’s 13-day run, seven US Tier 2 centers for the CMS experiment, and four US CMS Tier 3 centers, performed around 225,000 successful analysis jobs.

“We knew from past tests that we wanted to improve certain areas,” said Oliver Gutsche, the Fermilab physicist who led the effort for the CMS experiment. “This test was especially useful because we learned how the infrastructure behaves under heavy load from all four LHC experiments. We now know that we are ready for collisions.”

US contributions to the WLCG are coordinated through the Open Science Grid (OSG), a national computing infrastructure for science. OSG not only contributes computing power for LHC data needs, but also for projects in many other scientific fields including biology, nanotechnology, medicine and climate science.

“This is another significant step to demonstrating that shared infrastructures can be used by multiple high-throughput science communities simultaneously,” said Ruth Pordes, executive director of the Open Science Grid Consortium. “ATLAS and CMS are not only proving the usability of OSG, but contributing to maturing national distributed facilities in the US for other sciences.”

Physicists in the United States and around the world will sift through the LHC data in search of tiny signals that will lead to discoveries about the nature of the physical universe. Through their distributed computing infrastructures, these physicists also help other scientific researchers increase their use of computing and storage for broader discovery.

Read the full press release here.

Tona Kunz

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World Science Festival: Time Since Einstein

July 1, 2009 | 7:31 am

There was a strong science vibe in New York City as the World Science Festival rang in its third year. Founded by string theorist and author Brian Greene and  journalist Tracy Day, the festival hosted forty events over four days that sold out at various locations throughout the city.

“Time, I think, is a little bit like love,” began moderator John Hockenberry. “It’s accessible to all of us; it is intuitively experienced by all of us in the same way; yet it retains its mystery at whatever level you weigh in on it. It is a mysterious force that we all can experience and share.” And so Hockenberry opened the panel discussion at the World Science Festival titled “Time Since Einstein.” The award-winning journalist nearly slaps his audience awake with his booming voice and dramatic inflection, and by the end of the talk you just want to chat with him for hours.

The panel members were enough to make this science nerd drool: physicists George Ellis, Roger Penrose, Sean Carroll, and Fotini Markopoulou-Kalamara, who were joined by the two very physics-savvy philosophers David Albert and Michael Heller. The panel had its work cut out for it, given the task to cover everything we’ve learned and begun to question about time since the relativity revolution incited by Einstein. By the end, my friend and I wondered, “Would someone with no physics background think these people knew an incredible amount about time, or nothing at all?” And really, both are true. For as much as we’ve learned since Einstein, we’ve only found more to wonder about.

What is time? No, really, what is it? A dimension of space-time, says relativity, but is it physical? Or just mental? Why does it seem to move forward and not back? Does the universe acknowledge the arrow of time that we experience? How big is time? Does our notion of “now” have any validity? Is time quantized? And are the answers to these questions within the grasp of physics?

Einstein revolutionized our notion of time, and experimental evidence has since shown that time is in fact relative; it depends on where you are and how you are moving. Time was once the stage on which events occurred, but after Einstein, it became a player on the stage, equally influenced by the other players. “Our notion of time is very physical,” says Markopoulou-Kalamara. She’s referring to the fact that our concept of time often relies on physical cues, such as something we heard or saw. So is time just a series of events or changes in spatial dimensions? Einstein linked space and time into the dimension of space-time, and now scientists wonder if they can ever untangle the two. The nature of time, like many of physics’ most confounding issues, is explored on both the largest and the smallest scales we know of.

The notion of time plays different roles in general relativity and quantum mechanics. Markopoulou-Kalamara is at the forefront of the pursuit to link the two. She has worked in the development of loop quantum gravity, an alternative to string theory, and she is also developing models of space-time that account for the flow of time. While quantum mechanics suggests that the future is not planned, we don’t know if it equals a spontaneous present where we can chose our actions. Following this thread, she had this back and forth with Hockenberry:

Hockenberry: Can there be a non-deterministic future that actually exists?
Markopoulou-Kalamara: This is the conflict between the two theories–general relativity and quantum theory. So in general relativity, yes, it is deterministic. You never have to choose anything, everything is chosen for you.
H: Which is depressing. (laughs from the audience)
M-K:…Or freeing. (more laughs and some applause.) But in quantum mechanics that’s not true.
H: Which is…liberating or depressing?
M-K: Depends.

Einstein, a member of the elite group that shaped quantum mechanics, took a deterministic view; maybe he thought an intrinsically probabilistic universe was too frightening. Quantum mechanics doesn’t guarantee free will, but does it prove that the future is distinct from the past? George Ellis says that it does.

“There are many theoretical physicists who think the flow of time is an illusion,” he says. “And I think that’s a great mistake…according to quantum physics you don’t know the outcome of events until they happen. We know what happened in the past, there’s a time called the present when things are happening, and there’s a time in the future which is not yet determined. That’s my view on it, which is not a very widely supported one.”

A professor emeritus of applied mathematics at the University of Capetown, Ellis is the co-author with Stephen Hawking of The Large Scale Structure of Space Time, and investigates the physical foundations of the flow of time. He notes that subatomic particles, in the form of cosmic rays, affected the formation of life on this planet beginning four billion years ago. Even if we knew everything there was to know about the Earth then, we couldn’t have predicted the way things would turn out. Doesn’t that imply a distinct future?

Time on the quantum scale also challenges our notion of the present. One audience member asked if “now” really exists; can we take a picture of this moment and make it distinct? To totally freeze this moment would mean to collapse the wave functions of many things which would otherwise have been left as probabilites. In some ways, “now” is not definite.

The notion that time moves forward is something we humans can’t escape. As Carroll pointed out, if you’re out in space you might get confused about up and down, but you wouldn’t get confused about the past and the present (unless  you got a severe case of space madness). But most of the laws of physics are untouched by that notion–they are time symmetric, meaning if you run them backwards they look the same as they do running forward. A few rare particle experiments, however, done at CERN and Fermilab, have demonstrated a time asymmetry. The second law of thermodynamics is another heavy hitter for the idea of an arrow of time. The second law states that in a closed system things get more random; one can scramble an egg but not unscramble it. Entropy will always increase, and moving backwards in time would violate that.

Carroll, a senior research associate at the California Institute of Technology, is the author of the upcoming From Eternity to Here, a book about cosmology and the arrow of time. Always good for an elegant and enlightening talk despite the great complexity of his own research, he discussed the question “How long does time go?”:

“Scientists have gotten used to the idea that when people ask us ‘What happened before the big bang?’ we give St. Augustine’s answer: we say there was no such thing as before the big bang. But in very recent times, beyond Einstein, we’re realizing that we have absolutely no justification for saying that that’s true. We have to move beyond Einstein to understand what happened at the big bang. And the answer might be that the universe came into existence at the big bang; there’s nothing before. Or it might not. There could be something before the big bang….Cosmologists, people who are working on quantum gravity, are very interested in what we’ve learned since Einstein to answer these questions and go back and answer St. Augustine’s question.”

Ellis adds that Einstein also hated the idea of a beginning of time. It does seem rather odd that something with a very distinct beginning would simply have no end, or to think that even 14 billion years after the big bang (if the universe is infinite) we are still infinitesimally close to the beginning.

It seems the discussion of time swings quickly between the largest scale and the smallest scale. Discussion of the ultimate length of time begs the question, is time quantized? Can we break it up into packets like photons and quarks? Markopoulou-Kalamara says it depends on your notion of time. In terms of the geometric notion of time, as in the time dimension of a space-time, she says yes; she believes it has to break down. But if you’re referring to time as change, something that has happened, “I doubt it,” she says. Ellis adds that quantization of time may have to confront something like Zeno’s paradox of infinite halves:

“If you look between my fingers, the question is how many points are between there. And in some views of physics there’s not just an infinite number of points, there’s an uncountable infinity of points in between. I don’t believe it. I believe there’s got to be a discrete number of points. The same thing happens if I were to say one…two. How many points were between there and there? Was there an uncountable infinity of points? I don’t think so. I think there was a discrete number of time events between that point and that point.”

So, what is time?

“Change,” says Markopoulou-Kalamara.

“I would have to prepare a two-semester course,” says Heller.

Ellis:  ”It’s what clocks measure.”

Hockenberry closed with “The coming of wisdom with time,” by W.B. Yeats:

Though leaves are many, the root is one;
Through all the lying days of my youth
I swayed my leaves and flowers in the sun;
Now I may wither into the truth.

Calla Cofield

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Researchers find evidence for the origin of cosmic rays

June 30, 2009 | 7:00 am

Studies of supernova remnant RCW 86 have revealed the origin of cosmic rays. (Image courtesy of ESO/E. Helder and NASA/Chandra.)

Studies of supernova remnant RCW 86 have revealed the origin of cosmic rays. (Image courtesy of ESO/E. Helder and NASA/Chandra.)

An international team of researchers has discovered strong evidence that extremely energetic cosmic rays are born in supernova remnants.

“Cosmic rays constantly bombard the earth’s atmosphere but, until now, we didn’t have proof of where in our galaxy they originated,” said co-author Stefan Funk of the Kavli Institute for Particle Astrophysics and Cosmology at SLAC National Accelerator Laboratory. “That’s because cosmic rays are almost entirely made of protons, which as charged particles are bent by magnetic forces as they travel to Earth. So we can’t just trace a straight line back to know where they originated, like we can with light.”

Instead, the researchers traced the sources of cosmic rays by indirect means.

In a paper published last week in Science Express, the researchers describe measurements made with the European Southern Observatory’s Very Large Telescope and NASA’s Chandra X-ray Observatory. These measurements, of a star that exploded in the year A.D. 185, compare the temperature of the gas immediately behind the shockwave created by the stellar explosion with the speed of the shockwave itself. If the energy of the stellar explosion was converted solely into heat and motion, these two measurements should have been directly related by a very well-known and well-tested equation. Yet when the researchers plugged their measurements into the equation, it didn’t balance. Something else was being energized by the explosion.

“When a star explodes in what we call a supernova, a large part of the explosion energy is used for accelerating some particles up to extremely high energies,” said co-author Eveline Helder of the Astronomical Institute Utrecht in the Netherlands. “The energy that is used for particle acceleration is at the expense of heating the gas, which is therefore much colder than theory predicts.”

The researchers concluded that the missing energy goes into accelerating protons to nearly the speed of light-creating the cosmic rays that continually pummel our solar system, creating flashes of light behind the eyelids of astronauts and causing glitches in electronic components on Earth.

“Our observations reveal the smoking gun,” said Helder.

This story was first published in SLAC Today on June 30, 2009.

Kelen Tuttle

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Fermilab's CDF observes Omega-sub-b baryon

June 29, 2009 | 2:43 pm

This press release was issued by Fermilab today.

Once produced, the Omega-sub-b (Ωb) particle travels about a third of a millimeter before it disintegrates into two intermediate particles called J/Psi (J/ψ) and Omega-minus (Ω-). The J/Psi then promptly decays into a pair of muons. The Omega-minus baryon, on the other hand, can travel several centimeters and occasionally be measured in the CDF silicon vertex detector. The particle decays into an unstable particle called a Lambda (Λ) baryon along with a long-lived kaon particle (K). The Lambda baryon, which has no electric charge, also can travel several centimeters prior to decaying into a proton (p) and a pion (π). Credit: CDF collaboration.

Once produced, the Omega-sub-b (Ωb) particle travels about a third of a millimeter before it disintegrates into two intermediate particles called J/Psi (J/ψ) and Omega-minus (Ω-). The J/Psi then promptly decays into a pair of muons. The Omega-minus baryon, on the other hand, can travel several centimeters and occasionally be measured in the CDF silicon vertex detector. The particle decays into an unstable particle called a Lambda (Λ) baryon along with a long-lived kaon particle (K). The Lambda baryon, which has no electric charge, also can travel several centimeters prior to decaying into a proton (p) and a pion (π). Credit: CDF collaboration.

At a recent physics seminar at the Department of Energy’s Fermi National Accelerator Laboratory, Fermilab physicist Pat Lukens of the CDF experiment announced the observation of a new particle, the Omega-sub-b (Ωb). The particle contains three quarks, two strange quarks and a bottom quark (s-s-b). It is an exotic relative of the much more common proton and has about six times the proton’s mass.

The discovery of this “doubly strange” particle, predicted by the Standard Model, is significant because it strengthens physicists’ confidence in their understanding of how quarks form matter–and because it conflicts with a 2008 result announced by CDF’s sister experiment, DZero.

The Omega-sub-b is the latest entry in the “periodic table of baryons.” Baryons are particles formed of three quarks, the most common examples being the proton and neutron. The Tevatron particle accelerator at Fermilab is unique in its ability to produce baryons containing the b quark, and the large data samples now available after many years of successful running enable experimenters to find and study these rare particles.  The observation opens a new window for scientists to investigate its properties and better understand this rare object.

Combing through almost half a quadrillion (1000 billion) proton-antiproton collisions produced by Fermilab’s Tevatron particle collider, the CDF collaboration isolated 16 examples in which the particles emerging from a collision revealed the distinctive signature of the Omega-sub-b. Once produced, the Omega-sub-b travels a few millimeters before it decays into lighter particles. This decay, mediated by the weak force, occurs in about a trillionth of a second.

Late in 2008, DZero, the sister experiment to CDF, announced its own observation of the Omega-sub-b based on a smaller sample of Tevatron data.  Interestingly, the new CDF observation announced here is in direct conflict with the earlier DZero result.  The CDF physicists measured the Omega-sub-b mass to be 6054.4±6.8(stat.) ±0.9(syst.) GeV/c2 , compared to DZero’s 6.165 ± 0.016 GeV/c2. These two experimental results are statistically inconsistent with each other leaving scientists from both experiments wondering whether they are measuring the same particle.  Furthermore, the experiments observed different rates of production of this particle. Perhaps most interesting is that neither experiment sees a hint of evidence for the particle at the other’s measured value.

Although the latest result announced by CDF agrees with theoretical expectation for the Omega-sub-b both in the measured production rate and in the mass value, further investigation is needed to solve the puzzle of these conflicting results.

The Omega-sub-b discovery follows the observation of the Cascade-b-minus baryon (Ξb), first observed at the Tevatron in 2007, and two types of Sigma-sub-b baryons (Σb), discovered at the Tevatron in 2006.

The CDF collaboration submitted a paper that summarizes the details of its discovery to the journal Physical Review D.

Kurt Riesselmann

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Steven Chu's energy challenge

June 26, 2009 | 5:44 pm

Secretary of Energy Steven Chu speaking at SLAC on Friday morning. Photo: Brad Plummer.

Secretary of Energy Steven Chu speaking at SLAC on Friday morning. Photo: Brad Plummer, SLAC.

Update: A video of Chu’s nearly two-hour talk is now available on SLAC Today.  Here are links to coverage of the talk in the Contra Costa Times and Palo Alto Online.

Speaking to a crowd of more than 800 this morning at SLAC National Accelerator Laboratory, Secretary of Energy Steven Chu urged researchers to confront what he called “the energy challenge.”

“For the first time in history, science has shown humans altering the destiny of our planet in a meaningful way,” he said. “We have to try to enlist some of the very best intellectual horsepower to deal with this.”

In a wide-ranging speech that touched on worldwide emissions, climbing global temperatures, changing precipitation patterns, increasing atmospheric carbon dioxide concentrations, and the rising sea level, Chu demonstrated how the energy challenge cuts across many areas and is intensely tied to our economic prosperity.

“But there’s reason for hope,” he said. “Scientists by their very nature have to be very optimistic… We can fix this.”

Pointing to historical examples of research easing global problems-including the invention of artificial fertilizer, which helped set off the so-called “green revolution”-Chu expressed his belief that science research would again come to the world’s aid.

“It was scientific discoveries that enabled the world to feed itself,” Chu said. Now, he continued, scientific discoveries can increase energy efficiency and develop improved means of generating clean energy.

“There are lots of really exciting things that people at SLAC can think about,” he said. “Research can spur incredible intellectual achievement. And in the field of energy, I think we can do some really great science. A physicist or applied mathematician can really start to drool at these problems.”

Chu, who received the 1997 Nobel Prize in Physics for his work in cooling and trapping atoms with laser light, is a former chair of the Stanford University physics department. Prior to becoming Secretary of Energy, he was a professor of physics and molecular and cellular biology at the University of California, Berkeley, and the director of the Lawrence Berkeley National Laboratory.

Kelen Tuttle

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Crews dig in at NOvA site

June 26, 2009 | 10:30 am

The crew will blast through 50 feet of rock at the NOvA site to accommodate the detector facility.

The crew will blast through 50 feet of rock at the NOvA site to accommodate the detector facility.

Construction crews began digging at the future site of the NOvA detector facility in Ash River, Minn., on June 1.

The American Reinvestment and Recovery Act provided funds for the civil construction project.

Fifteen workers from Hoover Construction, a subcontractor of Adolfson & Peterson Construction, have been clearing the top layer of dirt and developing the roads at the site.

“It’s pretty much earth work now,” said Davin “Buddy” Juusola, senior project manager for Adolfson & Peterson. But once the dirt is cleared, the construction crew will face the Canadian Shield, a mass of 2.7 billion-year-old Precambrian rock that stretches 3 million square miles across Canada and dips into a small northern edge of the U.S.

Crews from Adolfson & Peterson often work with rock, but blasting at the NOvA site will present a unique challenge, said Juusola, who has worked with the construction company for nine years.

The crew will blast down 50 feet to accommodate the NuMI Off-Axis Electron Neutrino Appearance, NOvA, detector facility. The laboratory will house a 15,000-ton particle detector that physicists will use to study a beam of neutrinos originating at Fermilab.

Members of the crew have talked to local residents about the project, Juusola said. “They seem very excited. They’re very receptive to it.”

The appeal goes beyond an interest in the science. Local supplier Seppi Brothers Concrete Products, based in Virginia, Minn., will provide concrete for the site, and other businesses will likely become involved.

Juusola said this will be his first experience building a laboratory.

“There are not too many neutrino labs built,” he said. “It’s very unique, which makes it exciting. It’s a nice project to have on your resume.”

This story first appeared in Fermilab Today on June 26, 2009.

Kathryn Grim

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A Higgs boson without the mess

June 26, 2009 | 6:08 am

If CERN's Large Hadron Collider (LHC) can create Higgs bosons, a handful may appear in rare "exclusive" reactions that don't destroy the colliding protons--similar to a reaction now observed at Fermilab. CERN's ATLAS and CMS teams are considering adding equipment to their detectors (CMS shown here) to look for such events. Photo: CERN

If CERN's Large Hadron Collider (LHC) can create Higgs bosons, a handful may appear in rare "exclusive" reactions that don't destroy the colliding protons--similar to a reaction now observed at Fermilab. CERN's ATLAS and CMS teams are considering adding equipment to their detectors (CMS shown here) to look for such events. Photo: CERN

Particle physicists at CERN’s Large Hadron Collider (LHC) hope to discover the Higgs boson amid the froth of particles born from proton-proton collisions. Results in the 19 June Physical Review Letters show that there may be a way to cut through some of that froth. An experiment at Fermilab’s proton-antiproton collider in Illinois has identified a rare process that produces matter from the intense field of the strong nuclear force but leaves the proton and antiproton intact. There’s a chance the same basic interaction could give LHC physicists a cleaner look at the Higgs.

A proton is always surrounded by a swarm of ghostly virtual photons and gluons associated with the fields of the electromagnetic and strong nuclear forces. Researchers have predicted that when two protons (or a proton and an antiproton) fly past one another at close range, within about a proton’s diameter, these virtual particle clouds may occasionally interact to create new, real (not virtual) particles. The original protons would merely lose some momentum and separate from the beam. Such an “exclusive” reaction–where the original particles don’t break apart–gives unusually clean data because there are so few particles to detect.

In the new experiment, researchers were looking for signs that the interaction of virtual gluons had generated short-lived particles including the Χc (”Chi-c”) and J/ψ mesons, which are charm-anticharm quark pairs that decay into muons and antimuons. The Χc reaction would be especially rare because it requires protons to donate two gluons each, a requirement that also makes detailed predictions challenging, says Fermilab’s Mike Albrow, a member of the Collider Detector at Fermilab (CDF) collaboration.

In 2007, CDF researchers observed hints of exclusive, virtual gluon reactions in the form of high-energy photons radiating from colliding protons and antiprotons. Now the team has sifted through nearly 500 muon-antimuon pairs, identifying 65 that must have come from the decay of the Χc–very close to the rate predicted in 2005 by a team at Durham University in England. Because the Χc has similar particle properties to the much heavier Higgs boson, the same basic reaction should produce the Higgs at the higher collision energies provided by the LHC, says Albrow. “It’s the strongest evidence that the Higgs boson must be produced this way, if it does exist.”

Based on the rate of Χc production, Albrow estimates LHC collisions could produce 100 to 1000 Higgs bosons per year in each of the accelerator’s two largest particle detectors, ATLAS and CMS. “Even a few dozen events per year would enable you to measure the [Higgs's] mass, spin, and other properties,” he says. That’s why ATLAS and CMS teams are reviewing proposals to add detectors to look for exclusive Higgs events.

But not everyone is so optimistic that these events would be detectable in significant numbers. “It looks hard, but one should never say never,” says Joseph Incandela of the University of California, Santa Barbara, deputy physics coordinator for CMS. Incandela points out that once the LHC is operating at full capacity, every crossing of its twin proton beams is expected to yield about 20 collisions, throwing up other particles that may obscure exclusive reactions. But he says there are scenarios such as supersymmetry, a proposed extension to the standard model (the textbook theory of particle physics) in which there could be multiple Higgs bosons. In those situations, Albrow adds, exclusive reactions might be the only ones clean enough to distinguish the different Higgs particles.

by JR Minkel

JR Minkel is a freelance science writer in Nashville, Tennessee. His first book, Instant Egghead Guide: The Universe, comes out in July.

This story was first published in Physical Review Focus and is copyright American Physical Society. Reprinted with permission.

For more information on exclusive events, see the CERN Courier.

Guest author

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Dancing with science, or, a little light music

June 25, 2009 | 8:00 am

In honor of the start of construction for NSLS-II, members of the Center for Dance, Movement and Somatic Learning at Stony Brook University performed a special interpretive dance titled Time and Space for Celebration. Photo: Brookhaven National Laboratory

In honor of the start of construction for NSLS-II, members of the Center for Dance, Movement and Somatic Learning at Stony Brook University performed a special interpretive dance titled Time and Space for Celebration. Photo: Brookhaven National Laboratory

While writers have produced volumes of words on the beauty of scientific discovery, science and the performing arts have traditionally had a much lower rate of interaction.

However, such happy anomalies do sometimes occur.

Before the official speeches began at the National Synchrotron Light Source II start-of-construction celebration on June 15, 2009, employees, users, and guests of Brookhaven National Laboratory were reminded of the more poetic side of science by a distinctly non-verbal type of communication.

Slowly creeping in from stage-right, a lone dancer dressed in fluorescent green quickly commanded the attention of the audience with tribal stomps and dramatic leaps, performing a contemporary dance piece titled, Time and Space for Celebration.

Michelle Mitchell, a dance student majoring in engineering at Stony Brook University, seemed to question and explore her environment through movement, dancing to music that was both primal and futuristic. Her only companion on the stage was a giant three-dimensional geometric figure–an icosahedron–constructed of white PVC pipe.

A sense of curiosity, according to Amy Yopp Sullivan, choreographer and director of the Center for Dance, Movement and Somatic Learning at Stony Brook, was the main inspiration for the piece.

“We [the creative team] played with the idea of a primal, organic creature interacting with a mathematical structure,” she recalled. “We explored the mystery of discovery.”

To convey the scientific aspect of the theme, Yopp chose a life-sized icosahedrons–the 20-sided Platonic solid–to be the focal point of the piece. Mitchell interacted with the figure throughout the dance, approaching it with hesitation at first, but eventually dancing with and even inside of the structure. But the icosahedron was no arbitrary prop.

In addition to being visually striking, this figure also has strong ties to the “spatial harmony” ideas of the dance theorist Rudolf Laban. Working in the early decades of the 20th Century, Laban is most famous for his development of a highly influential system of movement notation, much akin to the dots and shapes used by composers to represent sound. His further contributions included introducing concepts typically associated with music, such as scale, resonance, and harmony, to the world of dance. Like a symphony from the few notes of a theme, Laban’s theory facilitated the construction of large-scale choreography from the rudimentary materials of movement.

Another key element of Laban’s work was his intense fascination with the Platonic solids–a family of three-dimensional geometric figures which includes the tetrahedron, cube, and icosahedron–and with what he saw to be the movements suggested by their division of space. Sullivan found this idea to be particularly relevant to Celebration, relying heavily on Laban’s work in constructing her choreography.

“Through Laban’s theory, we can understand how movement is organized by space,” Sullivan explained. “The shape of the space suggests certain pulls and following those pulls yields organization in the body.”

Mitchell added that it was “a lot of fun” to experiment with how her body could relate to the shape.

While the inherent structure of the icosahedron influenced much of Mitchell’s movements in Celebration, the accompanying musical score was equally important. Written by professional composer and SBU graduate student Max Giteck Duykers, the 10 minutes of music comprised a wide palate of electronic and acoustic sounds layered over driving rhythms.

According to Duykers, scientific concepts of light–appropriate for a new light source–figured heavily in his compositional process.

“I was thinking a lot about light frequencies and particles moving, slowing down, and speeding up,” he said regarding the origins of the music. “You can hear that in the way that the tempo changes.”

Another notable aspect of the score was a repeated fluttering figure, a gesture that Mitchell seemed to imitate in her physical motions at times by quickly tapping her chest and stamping her feet. Remarking that, as a choreographer, she “is always inspired by Max’s music,” Sullivan explained that this correlation has to do with the heart being the organic “core” of the body.

“The heart feeds the whole body. The fluttering in Max’s music seems to echo that enlivening process,” she said. Reflecting on the gesture, Sullivan and Mitchell agreed that the tapping motion may have been the actual seed of the choreography. “The rest probably grew organically from there,” Mitchell concluded.

Indeed, “organic” was the main word the artists used to describe the creation of the piece. A main question for both choreographer and composer, Sullivan said, was, “How do we remain connected to an organic existence in an increasingly artificial world?” In discussing the development of the work, the team stressed the importance of a “collaborative, creative process” in which the movements and music changed and grew toward the final product in tandem.

Considering the result of their efforts, each artist hoped that the audience would leave the performance with a new perspective on the connectedness of art and science, as well as an invigorated passion for discovery.

“I hope people see that they can reach past their current circumstances,” Mitchell said with a smile. “We shouldn’t be stagnant. We can go after our dreams.”

With a projected commissioning date in 2015, the scientists and engineers currently constructing NSLS-II are doing just that.

By J. Bryan Lowder

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Profile: Cervando Castro - steady hands and sharp eyes

June 24, 2009 | 3:58 pm

Cervando Castro (left) watches the monitors and operates the remote crane control with technicians John Featherstone and Keith Anderson (center) for the NuMI experiment.

Cervando Castro (left) watches the monitors and operates the remote crane control with technicians John Featherstone and Keith Anderson (center) for the NuMI experiment.

In a few weeks, Cervando Castro will use a remote control crane to change a key piece of equipment in Fermilab’s neutrino program. He will be located behind several feet of concrete shielding at distances of up to 100 feet from the component. It’s a job where steady hands and sharp eyes are essential.

“Cervando’s very focused and very calm in high-pressure situations,” said Kris Anderson, lead engineer for NuMI target hall operations. “We rely on him a lot.”

As part of regular maintenance, Cervando will swap out the NuMI target, the piece of the experiment that helps to create neutrinos from protons. But, because the target sits directly in the beam path and becomes radioactive, Castro will use several video monitors and a remote crane control from behind shielding to do the job.

“Cervando has a lot of experience in the lab, he’s our main crane guy,” said Mike Andrews, NuMI shutdown coordinator.

Castro, who has a background in welding and auto mechanics, is the senior technician for the NuMI target hall. He assembles, installs and maintains equipment and parts for the experiment, a job he previously did in the mechanical support department for the Tevatron.

While assembly and maintenance are relativelyf commonplace for the 25-year laboratory veteran, Castro was thrilled about his new challenges and his vertical commute when he started at NuMI.

“The first couple of times I was pretty excited to go down 150 feet into the NuMI target hall,” Castro said.

Then, the diversity of tasks Castro’s job includes–from assembling very delicate pieces of equipments to moving large chunks of concrete–keep him challenged. The largest piece of equipment he has had to move with the crane weighed 50,000 pounds. His schedule keeps him busy too. As a NuMI technician, Castro has to make himself available day or night as his job requires.

“I’m willing to do that because I want help make this place run smoothly,” Castro said.

by Tia Jones

This story first appeared in Fermilab Today on June 22, 2009.

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