First African School of Physics empowers students

August 30, 2010 | 5:25 pm

A small group of students from the first African School of Fundamental Physics and Applications enjoys a day of hands-on science at I-Themba Laboratory for Accelerator Based Science in South Africa.

A small group of students from the first African School of Fundamental Physics and Applications enjoys a day of hands-on science at I-Themba Laboratory for Accelerator Based Science in South Africa.

Students from 17 African countries came together for the rare opportunity to learn about particle physics this month.

Some African students have earned advanced science degrees but are looking for the specialized training in particle physics and its associated applications not usually offered on their own continent.

The first African School of Fundamental Physics and its Applications in Stellenbosch, South Africa, provided that training and financially supported some African students.

Sixty-five students from around the globe, including more than 50 from African countries, attended the three-week school for an overview of fundamental subatomic physics and its applications. They left with more information than they could process, new friends and connections, and ideas on how to pursue a particle-physics career.

“We really wanted to empower students,” said Fermilab scientist and school organizer Christine Darve. “We wanted them to have confidence in their skills and direction for their careers, but we also wanted them to become knowledge ambassadors – to take what they’ve learned back to their home countries.”

Between Aug. 1 and 21, students attended lectures from experts in the particle physics field and participated in small group discussions. They also learned about the benefits of particle physics to society from experts such as Jim Gates, a member of the President’s Council of Advisors on Science and Technology. On their last day, students attended a career workshop where they learned which particle physics institutions offer fellowships and what job opportunities exist.

“I think that most important were the opportunities to be a part of this and to receive guidance about how to grow academically and careerwise,” said Ekua Mensimah, a student from the University of Cape Coast, Ghana. “It was also reassuring to know that these opportunities don’t end on Aug. 21.”

While the students were learning about particle physics, the school organizers were learning more about the students’ countries.

“We want to document where these students were from and what science was offered in their home countries in order to better support this kind of education,” Darve said.

School organizers are still collecting feedback from the students, which they plan to use to inform the curriculum for the next school, which will take place in two years. The organizers will decide the next school’s location this fall.

Read the press release.

Rhianna Wisniewski

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Particle Accelerators for Dummies?

August 27, 2010 | 6:53 am

The Howard Hughes Medical Institute publishes a very nice in-house magazine called the HHMI Bulletin, with wonderful stories, illustrations, and photographs. In a fun Q&A piece, the Bulletin asked four HHMI researchers “What ‘For Dummies’ book are you most qualified to write?” One of the answers fits right in with what we think about at symmetry and the Bulletin gave us permission to republish it here.

Photo: John Eisele, CSU Photography

Photo courtesy of John Eisele, CSU Photography

“I would write a Synchrotron Survival Guide for Dummies for researchers tediously collecting data from these large particle accelerators. Practical tips would include: bring a toothbrush to combat the 3 a.m. fuzzy mouth feeling and warm sweaters for the midnight draft. Chocolate-covered coffee beans are a must. Another section would describe how to interact with synchrotron staff—make sure you have their cell phone numbers, and bring appeasement gifts if you have to call them at 2 a.m. (Swiss chocolate works best). Finally, bring your invisibility cloak in case you trip the entire beam and you need to escape the wrath of disgruntled researchers. If you don’t have one, bring more chocolate.”

Karolin Luger
HHMI Investigator
Colorado State University

David Harris

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LHC lawsuit dismissed by US court

August 26, 2010 | 12:54 pm

After a lengthy process examining a complaint by Walter Wagner about the risks of switching on the LHC, an appellate judge has dismissed the lawsuit, finding that Wagner had no standing before the court. According to the decision, Wagner failed to show a “credible threat of harm”, and the US government does not control the operation of the LHC and therefore is not the correct party to bring action against.

The decision itself is short and sweet. Read the entire text below or see the original (PDF).

Appeal from the United States District Court for the District of Hawaii
Helen Gillmor, Senior District Judge, Presiding

Argued and Submitted June 17, 2010
Honolulu, Hawaii

Before: B. FLETCHER, PREGERSON and CLIFTON, Circuit Judges.

Walter L. Wagner (“Wagner”) appeals the district court’s dismissal of his claim against the United States Department of Energy, the National Science Foundation (collectively, “the U.S. government”), and others. The parties are familiar with the facts of this case, which we repeat here only to the extent necessary to explain our decision. We have jurisdiction under 28 U.S.C. § 1291, and we affirm.

This court can affirm on any ground supported by the record. Cook v. AVI Casino Enters., Inc., 548 F.3d 718, 722 (9th Cir. 2008). We review questions of standing de novo, Mayfield v. United States, 599 F.3d 964, 970 (9th Cir. 2010), and factual findings for clear error. Robinson v. United States, 586 F.3d 683, 685 (9th Cir. 2009). To establish standing, Wagner must demonstrate (1) an “injury in fact,” (2) “a causal connection between the injury and the conduct complained of” that is not attributable to “the independent action of some third party not before the court,” and (3) a likelihood that a favorable decision will redress the injury. Lujan v. Defenders of Wildlife, 504 U.S. 555, 560-61 (1992).

Wagner cannot demonstrate that he has standing. A plaintiff alleging a procedural injury, such as Wagner, must still establish injury in fact. See Laub v. U.S. Dep’t. of Interior, 342 F.3d 1080, 1086 (9th Cir. 2003). Injury in fact requires some “credible threat of harm.” Cent. Delta Water Agency v. United States, 306 F.3d 938, 950 (9th Cir. 2002). At most, Wagner has alleged that experiments at the Large Hadron Collider (the “Collider”) have “potential adverse consequences.” Speculative fear of future harm does not constitute an injury in fact sufficient to confer standing. Mayfield, 599 F.3d at 970.

Even if Wagner has demonstrated injury in fact, he nevertheless fails to satisfy the causality or redressability prongs set out in Lujan. The European Center for Nuclear Research (“CERN”) proposed and constructed the Collider, albeit with some U.S. government support. The U.S. government enjoys only observer status on the CERN council, and has no control over CERN or its operations. Accordingly, the alleged injury, destruction of the earth, is in no way attributable to the U.S. government’s failure to draft an environmental impact statement.

CERN maintains total ownership, management, and operational control of the Collider. CERN has never been properly served, and is not a party to this case. Even if this court were to render a decision in Wagner’s favor, such a decision would have no impact on CERN or Collider operations, and would not afford Wagner the relief he seeks. [[Because our determination of standing is not dependent on the identity of the Appellant, we need not address whether Luis Sancho is a party to this appeal.]]

AFFIRMED.

Thanks to R. Penner for the tip that the decision had been reached.

David Harris

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The Particle Physics Song

August 26, 2010 | 9:41 am

“I’m watching something very strange right now,” a colleague texted from the CERN Control Center on Feb. 3.

Members of the CERN choir, all in black, had gathered there to perform their rendition of a song that a non-physicist had submitted to CERN’s monthly publication.

Danuta Orlowska, a clinical psychologist with Guy’s and St. Thomas’ NHS Foundation Trust in London, wrote “The Particle Physics Song,” an ode to the Higgs boson to be sung to the tune of “The Hippopotamus Song” by British comedians Michael Flanders and Donald Swann.

Though singing at a particle physics laboratory might seem strange, the sight should come as little surprise to CERN afficianados familiar with this video or this one.

This week CERN posted a video of the choir’s performance of “The Particle Physics Song” to the CERNTV YouTube site. Enjoy!

Kathryn Grim

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The Fermilab Jargon-Free Plain-English Tour Guide Competition

August 24, 2010 | 5:32 pm

Doug Glenzinski, right, with Fermilab Director Pier Oddone -- and a very special vintage

Doug Glenzinski, right, with Fermilab Director Pier Oddone -- and a very special vintage

Anyone who read about Fermilab’s Mu2e experiment in our June issue knows the complexity of the science behind it. It’s one thing to explain the project in a 3000-word feature article — but in a five-minute talk?  That’s how long physicist Doug Glinzinski was given to explain the project to Senate staffer Leland Cogliani during a lab tour last week. He did such a good job that he won the Fermilab Jargon-Free Plain-English Tour Guide Competition, and a special prize from lab Director Pier Oddone: a bottle of 2003 Dry Creek Valley Zinfandel from the Oddone Vineyard in California.

It was the first time Fermilab put on such a contest, and it worked so well, lab insiders say, that it may not be the last.

Onward to a Jargon-Free Tomorrow!

Glennda Chui

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The strange case of solar flares and radioactive elements

August 23, 2010 | 11:50 am

Peter Sturrock, Stanford professor emeritus of applied physics. Photo by L.A. Cicero

Peter Sturrock, Stanford professor emeritus of applied physics. Photo by L.A. Cicero

This story is from the Aug. 23, 2010 issue of Stanford Report.

When researchers found an unusual linkage between solar flares and the inner life of radioactive elements on Earth, it touched off a scientific detective investigation that could end up protecting the lives of space-walking astronauts and maybe rewriting some of the assumptions of physics.

It’s a mystery that presented itself unexpectedly: The radioactive decay of some elements sitting quietly in laboratories on Earth seemed to be influenced by activities inside the sun, 93 million miles away.

Is this possible?

Researchers from Stanford and Purdue universities believe it is. But their explanation of how it happens opens the door to yet another mystery.

There is even an outside chance that this unexpected effect is brought about by a previously unknown particle emitted by the sun. “That would be truly remarkable,” said Peter Sturrock, Stanford professor emeritus of applied physics and an expert on the inner workings of the sun.

The story begins, in a sense, in classrooms around the world, where students are taught that the rate of decay of a specific radioactive material is a constant. This concept is relied upon, for example, when anthropologists use carbon-14 to date ancient artifacts and when doctors determine the proper dose of radioactivity to treat a cancer patient.

Random numbers

But that assumption was challenged in an unexpected way by a group of researchers from Purdue University who at the time were more interested in random numbers than nuclear decay. (Scientists use long strings of random numbers for a variety of calculations, but they are difficult to produce, since the process used to produce the numbers has an influence on the outcome.)

Ephraim Fischbach, a physics professor at Purdue, was looking into the rate of radioactive decay of several isotopes as a possible source of random numbers generated without any human input. (A lump of radioactive cesium-137, for example, may decay at a steady rate overall, but individual atoms within the lump will decay in an unpredictable, random pattern. Thus the timing of the random ticks of a Geiger counter placed near the cesium might be used to generate random numbers.)

As the researchers pored through published data on specific isotopes, they found disagreement in the measured decay rates – odd for supposed physical constants.

Checking data collected at Brookhaven National Laboratory on Long Island and the Federal Physical and Technical Institute in Germany, they came across something even more surprising: long-term observation of the decay rate of silicon-32 and radium-226 seemed to show a small seasonal variation. The decay rate was ever so slightly faster in winter than in summer.

Was this fluctuation real, or was it merely a glitch in the equipment used to measure the decay, induced by the change of seasons, with the accompanying changes in temperature and humidity?

“Everyone thought it must be due to experimental mistakes, because we’re all brought up to believe that decay rates are constant,” Sturrock said.

The sun speaks

On Dec 13, 2006, the sun itself provided a crucial clue, when a solar flare sent a stream of particles and radiation toward Earth. Purdue nuclear engineer Jere Jenkins, while measuring the decay rate of manganese-54, a short-lived isotope used in medical diagnostics, noticed that the rate dropped slightly during the flare, a decrease that started about a day and a half before the flare.

If this apparent relationship between flares and decay rates proves true, it could lead to a method of predicting solar flares prior to their occurrence, which could help prevent damage to satellites and electric grids, as well as save the lives of astronauts in space.

The decay-rate aberrations that Jenkins noticed occurred during the middle of the night in Indiana – meaning that something produced by the sun had traveled all the way through the Earth to reach Jenkins’ detectors. What could the flare send forth that could have such an effect?

Jenkins and Fischbach guessed that the culprits in this bit of decay-rate mischief were probably solar neutrinos, the almost massless particles famous for flying at nearly the speed of light through the physical world – humans, rocks, oceans or planets – with virtually no interaction with anything.

Then, in a series of papers published in Astroparticle Physics, Nuclear Instruments and Methods in Physics Research and Space Science Reviews, Jenkins, Fischbach and their colleagues showed that the observed variations in decay rates were highly unlikely to have come from environmental influences on the detection systems.

Reason for suspicion

Their findings strengthened the argument that the strange swings in decay rates were caused by neutrinos from the sun. The swings seemed to be in synch with the Earth’s elliptical orbit, with the decay rates oscillating as the Earth came closer to the sun (where it would be exposed to more neutrinos) and then moving away.

So there was good reason to suspect the sun, but could it be proved?

Enter Peter Sturrock, Stanford professor emeritus of applied physics and an expert on the inner workings of the sun. While on a visit to the National Solar Observatory in Arizona, Sturrock was handed copies of the scientific journal articles written by the Purdue researchers.

Sturrock knew from long experience that the intensity of the barrage of neutrinos the sun continuously sends racing toward Earth varies on a regular basis as the sun itself revolves and shows a different face, like a slower version of the revolving light on a police car. His advice to Purdue: Look for evidence that the changes in radioactive decay on Earth vary with the rotation of the sun. “That’s what I suggested. And that’s what we have done.”

A surprise

Going back to take another look at the decay data from the Brookhaven lab, the researchers found a recurring pattern of 33 days. It was a bit of a surprise, given that most solar observations show a pattern of about 28 days – the rotation rate of the surface of the sun.

The explanation? The core of the sun – where nuclear reactions produce neutrinos – apparently spins more slowly than the surface we see. “It may seem counter-intuitive, but it looks as if the core rotates more slowly than the rest of the sun,” Sturrock said.

All of the evidence points toward a conclusion that the sun is “communicating” with radioactive isotopes on Earth, said Fischbach.

But there’s one rather large question left unanswered. No one knows how neutrinos could interact with radioactive materials to change their rate of decay.

“It doesn’t make sense according to conventional ideas,” Fischbach said. Jenkins whimsically added, “What we’re suggesting is that something that doesn’t really interact with anything is changing something that can’t be changed.”

“It’s an effect that no one yet understands,” agreed Sturrock. “Theorists are starting to say, ‘What’s going on?’ But that’s what the evidence points to. It’s a challenge for the physicists and a challenge for the solar people too.”

If the mystery particle is not a neutrino, “It would have to be something we don’t know about, an unknown particle that is also emitted by the sun and has this effect, and that would be even more remarkable,” Sturrock said.

– by Dan Stober with contributions from Chantal Jolagh, a science-writing intern at the Stanford News Service.

Press Release

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Math’s highest honor given for work in mathematical physics

August 20, 2010 | 4:18 pm

It was a good week for mathematical physics. Three of the four winners of the 2010 Fields Medal, considered the Nobel Prize for mathematics, were honored for studies in the field.

The Fields Medal is not entirely analogous to the Nobel: The award is given once every four years; its recipients must be younger than 40; and Fields medalists win about $14,000, compared to about $1.4 million that come with a Nobel.

(The fact is, there is no Nobel Prize in mathematics and never has been, and so the Fields Medal is the highest honor a mathematician can receive. Maybe mathematicians are just above all that.)

At the award ceremony on Aug. 19 in Hyderabad, India, the International Mathematical Union honored mathematicians Cedric Villani, Stanislav Smirnov and Elon Lindenstrauss, as well as mathematician Ngo Bau Chau.

IMU granted the award to Villani, of the Henri Poincare Institute in Paris, for his achievements in understanding Boltzmann’s kinetic theory of gases. This theory explains entropy, but instead of  “tracking the individual motion of billions of individual atoms, it studies the evolution of the probability that a particle occupies a certain position and has a certain velocity,” according to the International Congress of Mathematicians website. Villani’s work also dealt with plasma physics.

Smirnov, of the University of Geneva, investigated what happens to probability in lattice models — grids used in statistical physics — when the blocks in the grid become infinitely small. “The proof is elegant, and it is based on extremely insightful combinatorial arguments,” the website said. “Smirnov’s work gave the solid foundation for important methods in statistical physics like Cardy’s Formula, and provided an all-important missing step in the theory of Schramm-Loewner Evolution in the scaling limit of various processes.”

IMU awarded the Fields Medal to Lindenstrauss, of the Hebrew University of Jerusalem, for studies of ergodic theory, which had implications for other theories, including quantum theory.

According to his profile, Lindenstrauss and his collaborators “have found many other unexpected applications of these ergodic theoretic techniques in problems in classical number theory. His work is exceptionally deep.”

Kathryn Grim

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Neutrinos and the evolution of young scientists

August 19, 2010 | 5:44 am

A slice of the action during the 2010 SSI versus SLAC soccer game. SSI outscored SLAC by one goal.
A slice of the action during the 2010 SSI versus SLAC soccer game. SSI outscored SLAC by one goal.

This story first appeared in the Aug. 19 issue of SLAC Today.

Last Friday marked the end of the 38th annual SLAC Summer Institute, during which more than 150 graduate students, postdocs and researchers attended two weeks of lectures, topical mini-conferences, and opportunities for in-depth discussions with visiting experts, all in an effort to get to know “Neutrinos: Nature’s Mysterious Messengers.”

“Of all the known particles, neutrinos are the most mysterious,” explained JoAnne Hewett, one of SSI’s four program directors, “yet they’re all around us. They played an essential role in the evolution of the universe.”

SSI’s particular focus, though, was the role of neutrinos in the evolution of young scientists. Along with the lectures, discussions and mini-conferences, SSI 2010 offered a variety of social events such as dinners, SLAC tours, an opportunity to present posters on current research and the traditional SLAC versus SSI soccer game. On the weekend the students organized their own trip to the Santa Cruz boardwalk, and several missed the start of the final sessions because of a late night Perseid meteor-watching session.

“The kids seemed to have a great time,” Hewett said with a laugh. “We got them started” with group dinners, she said, “and they took over.” Hewett warned not to downplay the social aspects of SSI. “These students will be colleagues throughout their careers, and the bonds that are formed now at places such as SSI stay throughout their life.”

The students said they appreciated the social activities but reserved their highest praise for the quality of the speakers and course content. Katie Richardson, a graduate student at the University of New Mexico, said she liked the discussion sessions, which she termed “quality time with the experts.”

“Most of the speakers have been fantastic,” said Geoffrey Ryan, a graduate student at the University of Alberta. “It’s motivating me to be a better speaker and teacher.”

“SSI is an institution recognized by the worldwide particle physics community and some professors send their students here every year,” said Hewett, now in her eighth year as an SSI program director. “There are lab directors from around the world who have attended SSI. It’s a real training ground for graduate students.”

As Geoffrey Ryan, the graduate student from the University of Alberta, said at the soccer game: “There are young people in physics I can actually talk to.” He lifted his can of soda to his new friends. “You guys are awesome.”

Trillions of neutrinos whizzed past the discussion, but were unavailable for comment.

—Lori Ann White

Symmetry Intern

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Nicola Cabibbo: 1935–2010

August 18, 2010 | 12:55 pm

Nicola_Cabibbo

From the Aug. 17 Physics World:

The Italian physicist Nicola Cabibbo, who many said should have shared the Nobel Prize for Physics in 2008 for his contribution to understanding the mechanism of quark mixing, died yesterday [Aug. 16] at the age of 75.

Cabibbo held many high-profile positions throughout his career including president of the Italian National Institute of Nuclear Physics (INFN). At the time of his death he was working at the University of Rome “La Sapienza”, and was president of the Pontifical Academy of Sciences and chair of the scientific council at the Abdus Salam International Centre for Theoretical Physics (ICTP).

Only last week Cabibbo, together with Ennackal Chandy George Sudarshan of the University of Texas at Austin, were awarded the ICTP’s 2010 Dirac medal for their “fundamental contributions to the understanding of weak interactions and other aspects of theoretical physics.” A friend or colleague of Cabibbo will now be invited to accept the award on his behalf when it is presented in November by Irina Bokova, the director general of the United Nations Educational, Scientific and Cultural Organization.

The article goes on to explain Cabibbo’s contributions to the understanding of the weak interaction in quarks, the mixing between different “flavors” of quarks and the development of the Cabibbo-Kobayashi-Maskawa matrix, which among other things predicted the existence of the top, bottom, and charm quarks.  Many physicists feel he should have shared the 2008 Nobel Prize in physics with Makoto Kobayashi and Toshihide Maskawa; instead they shared the prize with theorist Yoichiro Nambu. Several US national laboratories — SLAC, Fermilab, and Brookhaven – also had connections to this Nobel Prize-winning work.

Glennda Chui

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Dark energy studies top astronomy and astrophysics priorities

August 13, 2010 | 10:01 am

High-energy physics interests are ranked highly in the decadal study of astronomy and astrophysics priorities released by a National Research Council committee today. The top-ranked projects in “New Worlds, New Horizons in Astronomy and Astrophysics“  include studies of dark energy and dark matter although a strong emphasis on extra-solar planet astronomy pushed some high-energy physics further down the list.

Topping the list for large-scale ground-based projects is LSST, the Large Synoptic Survey Telescope, which would image over half the sky every three nights. Its 8.4-meter telescope in Chile will create a 3D map of the universe, locating dark matter and characterizing the properties of dark energy. You can read more about LSST in stories about the search for dark energy (a symmetry feature illustrated by Roz Chast); the largest digital camera ever created; and the work needed to store all the data the telescope will collect.

The large-scale space-based list is led by a newly named project WFIRST, the Wide-Field Infrared Survey Telescope. It will use three different techniques to explore dark energy from space with the big advantage that it can see deep into the infrared spectrum. That is important for observing the most distant supernovae, a key component in understanding dark energy. The design of WFIRST is based on one of the proposed designs for the Joint Dark Energy Mission between NASA and the US Department of Energy, but those proposals had been put on ice until this report came out. WFIRST adds some extra capabilities to the JDEM “Omega” proposal, including a search for extra-solar planets.

Second on the space-based list is a collection of projects in the NASA Explorer range. A previous Explorer project was the Wilkinson Microwave Anisotropy Probe, or WMAP, which has provided stunning data about the cosmic microwave background. The specific projects in this category are not determined yet but will come from proposal competitions recommended to occur annually. Although the high-energy physics component of these proposals is unclear, past missions have added significant value to the high-energy physics mission.

Back on the ground, participation in the Atmospheric Cerenkov Telescope Array, or ACTA, ranked lower. However, the committee says this area is important due to the recent demonstrated progress and that prospects are good for building a much more capable facility not too far into the future

Looking at DOE budget scenarios, the committee recommends that if the budget doubling path continues, enough funding would be available to participate strongly in LSST, WFIRST, and ACTA plus some additional smaller projects recommended by PASAG, the Particle Astrophysics Scientific Advisory Group. If the budget stays closer to flat over the next decade then DOE involvement will need to be more selective. As DOE is a smaller player than others in the large-scale projects, DOE should prioritize LSST over the others because it has a larger fractional participation.

Astronomers and astrophysicists will be chewing over the details in the 224-page document for some time but NASA, DOE, and NSF will all be getting together in the next few weeks to look at their existing plans in light of the report.

David Harris

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