OPERA catches its first tau neutrino

May 31, 2010 | 6:49 am

The OPERA detector underground at Italy's Gran Sasso National Laboratory. Image credit OPERA Collaboration.

The OPERA detector underground at Italy's Gran Sasso National Laboratory. Image credit OPERA Collaboration.

Scientists from the OPERA experiment at INFN’s Gran Sasso National Laboratory have announced the first direct observation of  a neutrino transforming from one type into another. When confirmed by a few more such events, this observation will provide further  evidence that neutrinos have mass, a phenomenon that remains unexplained by physicists’ recipe for understanding the universe, the Standard Model.

Neutrinos are very light, neutral particles that exist in three types: electron, muon and tau. Over the past 15 years, several experiments have shown that neutrinos can spontaneously change type, or oscillate, as they travel long distances. These experiments, however, all measured the disappearance of certain types of neutrinos, leaving open the question of whether oscillation is a one-way or a two-way process. OPERA is the first experiment to measure the appearance of a tau neutrino in a beam of muon neutrinos, thus confirming that neutrinos oscillate between different types.

The scientists of the OPERA experiment have spent the last three years searching for the appearance of a tau particle in their detector as a beam of muon neutrinos, created 732 kilometers away at CERN in Geneva, Switzerland, passed through their underground experiment. The appearance of a tau particle in their detector indicates that one of the billions upon billions of muon neutrinos transformed into a tau neutrino.

More details can be found in the INFN press release and CERN press release, or you can watch this video from CERN that describes neutrinos and the oscillation phenomenon, the OPERA detector and creation of the muon neutrino beam, and today’s announcement.

Katie Yurkewicz

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The ATLAS Experiment: Popping up next month across North America (and on Tuesday in NYC)

May 20, 2010 | 1:59 pm

The world’s first Large Hadron Collider pop-up book has gotten a makeover for North American readers. The silver edition of “Voyage to the Heart of Matter” features changes to text and design, as well as some enhanced pop-up action to better represent the Large Hadron Collider and ATLAS detector. The new edition of the eight-page book will be available from major bookstores and online retailers in the United States and Canada starting at the end of June.

LHC-philes (and pop-up aficionados) in the New York City area can get a sneak preview of the book and learn more about the world’s most powerful particle accelerator at a special event next Tuesday evening, May 25 at the New York Academy of Sciences. “Pop-Up Particle Physics from the Large Hadron Collider” will feature a panel discussion moderated by Alan Alda, book-signing and reception. Panelists will include Harvard theoretical physicist Lisa Randall, ATLAS physicist and Columbia University professor Michael Tuts, and book author Emma Sanders from CERN.

Katie Yurkewicz

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Fermilab scientists find evidence for significant matter-antimatter asymmetry

May 18, 2010 | 1:25 pm

The DZero collaboration has found evidence for a new way in which elementary particles break the matter-antimatter symmetry of nature. This new type of CP violation is in disagreement with the predictions of the theoretical framework known as the Standard Model of particles and their interactions. The effect ultimately may help to explain why the universe is filled with matter while antimatter disappeared shortly after the big bang. Credit: DZero collaboration

The DZero collaboration has found evidence for a new way in which elementary particles break the matter-antimatter symmetry of nature. This new type of CP violation is in disagreement with the predictions of the theoretical framework known as the Standard Model of particles and their interactions. The effect ultimately may help to explain why the universe is filled with matter while antimatter disappeared shortly after the big bang. Credit: DZero collaboration

Scientists of the DZero collaboration at the Department of Energy’s Fermi National Accelerator Laboratory announced Friday, May 14, that they have found evidence for significant violation of matter-antimatter symmetry in the behavior of particles containing bottom quarks beyond what is expected in the current theory, the Standard Model of particle physics. The new result, submitted for publication in Physical Review D by the DZero collaboration, an international team of 500 physicists, indicates a one percent difference between the production of pairs of muons and pairs of antimuons in the decay of B mesons produced in high-energy collisions at Fermilab’s Tevatron particle collider.

The dominance of matter that we observe in the universe is possible only if there are differences in the behavior of particles and antiparticles. Although physicists have observed such differences (called “CP violation”) in particle behavior for decades, these known differences are much too small to explain the observed dominance of matter over antimatter in the universe and are fully consistent with the Standard Model. If confirmed by further observations and analysis, the effect seen by DZero physicists could represent another step towards understanding the observed matter dominance by pointing to new physics phenomena beyond what we know today.

Using unique features of their precision detector and newly developed analysis methods, the DZero scientists have shown that the probability that this measurement is consistent with any known effect is below 0.1 percent (3.2 standard deviations).

“This exciting new result provides evidence of deviations from the present theory in the decays of B mesons, in agreement with earlier hints,” said Dmitri Denisov, co-spokesperson of the DZero experiment, one of two collider experiments at the Tevatron collider. Last year, physicists at both Tevatron experiments, DZero and CDF, observed such hints in studying particles made of a bottom quark and a strange quark.

When matter and anti-matter particles collide in high-energy collisions, they turn into energy and produce new particles and antiparticles. At the Fermilab proton-antiproton collider, scientists observe hundreds of millions every day. Similar processes occurring at the beginning of the universe should have left us with a universe with equal amounts of matter and anti-matter. But the world around is made of matter only and antiparticles can only be produced at colliders, in nuclear reactions or cosmic rays. “What happened to the antimatter?” is one of the central questions of 21st–century particle physics.

The DZero result is based on the comparison of the distributions of positively and negatively charged muons (μ+ and μ-) emerging from high-energy proton-antiproton collisions produced by the Tevatron particle collider. A strong magnetic field inside the DZero particle detector forces the muons that emerge from those collisions to travel along a curved path. Two muons with opposite charge follow paths that curve in opposite direction (see graphic). Scientists first compared the muon distributions when the the magnetic field inside the DZero detector pointed in one direction (configuration 1) and then compared their distributions when the magnetic field had been reversed (configuration 2). If the matter-antimatter symmetry were perfect, the comparison of the muon distributions in the two configurations would yield the same result. Instead, the DZero experiment observed a one-percent deviation, evidence for a matter-antimatter asymmetry. Credit: Fermilab

The DZero result is based on the comparison of the distributions of positively and negatively charged muons (μ+ and μ-) emerging from high-energy proton-antiproton collisions produced by the Tevatron particle collider. A strong magnetic field inside the DZero particle detector forces the muons that emerge from those collisions to travel along a curved path. Two muons with opposite charge follow paths that curve in opposite direction (see graphic). Scientists first compared the muon distributions when the the magnetic field inside the DZero detector pointed in one direction (configuration 1) and then compared their distributions when the magnetic field had been reversed (configuration 2). If the matter-antimatter symmetry were perfect, the comparison of the muon distributions in the two configurations would yield the same result. Instead, the DZero experiment observed a one-percent deviation, evidence for a matter-antimatter asymmetry. Credit: Fermilab

To obtain the new result, the DZero physicists performed the data analysis “blind,” to avoid any bias based on what they observe. Only after a long period of verification of the analysis tools, did the DZero physicists look at the full data set. Experimenters reversed the polarity of their detector’s magnetic field during data collection to cancel instrumental effects.

“Many of us felt goose bumps when we saw the result,” said Stefan Soldner-Rembold, co-spokesperson of DZero. “We knew we were seeing something beyond what we have seen before and beyond what current theories can explain.”

The precision of the DZero measurements is still limited by the number of collisions recorded so far by the experiment. Both CDF and DZero therefore continue to collect data and refine analyses to address this and many other fundamental questions.

“The Tevatron collider is operating extremely well, providing Fermilab scientists with unprecedented levels of data from high energy collisions to probe nature’s deepest secrets. This interesting result underlines the importance and scientific potential of the Tevatron program,” said Dennis Kovar, Associate Director for High Energy Physics in DOE’s Office of Science.

The DZero result is based on data collected over the last eight years by the DZero experiment: over 6 inverse femtobarns in total integrated luminosity, corresponding to hundreds of trillions of collisions between protons and antiprotons in the Tevatron collider.

“Tevatron collider experiments study high energy collisions in every detail, from searches for the Higgs boson, to precision measurement of particle properties, to searches for new and yet unknown laws of nature. I am delighted to see yet another exciting result from the Tevatron,” said Fermilab Director Pier Oddone.

DZero is an international experiment of about 500 physicists from 86 institutions in 19 countries. It is supported by the U.S. Department of Energy, the National Science Foundation and a number of international funding agencies.

Fermilab is a national laboratory funded by the Office of Science of the U.S. Department of Energy, operated under contract by Fermi Research Alliance, LLC.

Press Release

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Neutrinos: a fishy explanation

May 18, 2010 | 1:13 pm

Collaboration members for the NOvA neutrino experiment held public tours of the future site of the NOvA detector facility the weekend of Minnesota’s annual Governor’s Fishing Opener. Aside from proximity of the site to the opener, held on Lake Kabetogama, does the experiment have anything to do with fishing? Maybe. Fishing guide Frank House and physicist Mark Messier explain.

Kathryn Grim

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Minnesota governor visits NOvA site

May 17, 2010 | 8:29 pm

Saturday, May 15, marked a state holiday in Minnesota. Enthusiasts headed north to the annual Governor’s Fishing Opener, the first day of the fishing season, in search of Minnesota’s state fish, the walleye.

On Friday, Minnesota Gov. Tim Pawlenty stopped to visit Minnesota residents and visitors interested in a different type of catch: neutrinos.

Pawlenty took a quick tour of the future site of the NOvA neutrino detector facility in Ash River, Minn. The facility is not far from where Minnesotans cast their lines during this year’s opener, Lake Kabetogama. Scientists and those managing construction held public tours on Friday before welcoming the governor.

Pawlenty expressed his support for conducting the research in Minnesota. But he didn’t stay long; the afternoon clouds had begun to clear just in time for the Fishing Opener community picnic.

Kathryn Grim

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Looking at the Galaxy Zoo with (gravitational) lenses

May 14, 2010 | 1:00 pm

An example gravitational lens from the SDSS data set.

An example gravitational lens from the SDSS data set. This image is known as the 8 o'clock arc.

Can you tell a gravitational lens from a distant spiral galaxy? With an expansion of the Galaxy Zoo citizen science project, you can try your eye at lens identification, thanks in part to the efforts of Phil Marshall at SLAC and Stanford’s Kavli Institute for Particle Astrophyics and Cosmology.

Galaxy Zoo, which has been running for three years, is now turning to the Hubble Space Telescope for data, coinciding with HST’s 20th anniversary. The original Galaxy Zoo project allowed people to comb through mountains of image data from the Sloan Digital Sky Survey, a ground-based telescope system in New Mexico. The “Zooites,” as these 21st century amateur astronomers are known, are able to classify galaxies accurately and efficiently, thus taking part in a massive scientific project and unloading a lot of work from professional astrophysicists. From the very beginning, the Zooites started spotting new and unusual objects–including gravitational lens candidates, on a discussion forum thread started by the Zoo’s instigator, Kevin Schawinski.

The website leads visitors through a questionnaire that helps them learn to properly identify galaxy types, such as elliptical or spiral. Marshall, who studies strong gravitational lenses, and Chris Lintott, Galaxy Zoo principal investigator, realized they could help the Zooites spot lenses more efficiently by adding an additional question to the procedure. This resulted in users identifying several thousand Galaxy Zoo galaxies that show potential lensing-like features. From this large list, Aprajita Verma, who is leading the follow-up investigation from Oxford, selected 20-30 good gravitational lens candidates for further observation.

“We know that lenses are very rare,” Marshall says. Now, Galaxy Zoo is providing a number of tools to allow the zooites to whittle down their list of lens candidates themselves. “We hope that ‘crowd-sourcing’ this problem will provide a more complete sample of gravitational lenses than could be generated blindly by computer.”

With the addition of the Hubble data, scientists have a plethora of new galaxies to sort – galaxies that are much younger and further away because of Hubble’s increased scope. Considering there are nearly 250,000 users of Galaxy Zoo, they have plenty of help!

by Julie Karceski

You can see more about gravitational lenses in this short film explaining how to make your own.

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National Lab Day brings Fermilab physics to students

May 12, 2010 | 12:06 pm

Fermilab scientist Al Sondgeroth demonstrates force and motion to students from Annunciation BVM School in Aurora.

Fermilab scientist Al Sondgeroth demonstrates force and motion to students from Annunciation BVM School in Aurora.

“I want to try, too!” This was the chorus that rang out across Jennifer Wardynski’s sixth grade class last Tuesday, when Fermilab’s Al Sondgeroth got students involved in a demonstration of angular momentum at Annunciation BVM elementary school in Aurora.

Sondgeroth was one of 20 Fermilab volunteers who gave hands-on presentations in area elementary and high schools last week to celebrate National Lab Day. His presentation gave students an opportunity to experience Issac Newton’s laws in action.

“It helped bridge the gap between the abstract concepts of physics and real-world applications that are all around us,” Wardynski said.

In addition to Sondgeroth’s presentation on force and motion, volunteers talked about topics such as electricity and magnetism, light and color and the physics of sports.

On Thursday, Fermilab Deputy Director Young-Kee Kim spoke to the young women in teacher Falguni Soni’s chemistry classes at Rosary High School. Her visit to Rosary was prompted in part by the interest of sophomore Emily Launer, who wrote a prize-winning research piece on the history of Fermilab.

Kim discussed the field of particle physics and some of the scientific mysteries that Fermilab pursues. She also encouraged the girls who have an interest in science and advised them not to be daunted by a field historically dominated by men.

Many of the students said the presentation helped them relate the science that they are learning about in the classroom to the physics at Fermilab.

“It was all really interesting,” said junior Mary LeDoux. “I had heard some of the information about science done at Fermilab before but it really helps to hear it all again because these are very deep concepts.”

National Lab Day is a response to President Obama’s call to encourage students across the country to learn about math, science, technology and engineering. Over the course of the week, Fermilab presentations reached about 2500 elementary and high school students.

by Daisy Yuhas

This story first appeared in Fermilab Today on May 12, 2010.

Symmetry Intern

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As you can see, there is nothing to see!

May 7, 2010 | 6:16 am

The Axion-Like Particle Search experiment at DESY in Hamburg, Germany published its results showing no signs of exotic particles passing, like magic, through a wall, but it does place the tightest constraints yet on a type of particle predicted by various theories.

The Axion-Like Particle Search experiment at DESY in Hamburg, Germany, published its results showing no signs of exotic particles passing, like magic, through a wall, but it does place the tightest constraints yet on a type of particle predicted by various theories.

The Axion-Like Particle Search, or ALPS, came, saw nothing and conquered anyway. The “light through the wall” experiment, looking for very light particles in so far unenlightened realms of our world has now published its results. So did they find axions or similar light particles? Unfortunately not.

“But we have the most sensitive experiment in this field and we were able to considerably extend the exclusion limits for such particles,” explains ALPS spokesman Axel Lindner. He is particularly pleased that after a development period of two years the experiment was able to make measurements with much higher precision than expected. The group, made up of scientists from Deutsches Elektronen-Synchrotron, the Albert Einstein Institute and the Laser Zentrum in Hanover, and the Hamburger Sternwarte, wanted to find photons that transform into hidden light particles in the magnetic field of a superconducting magnet from DESY’s past HERA facility.

For this purpose, they sent green laser light back and forth in a so-called optical cavity in the front part of the magnet. Had any hidden particles emerged they would have traversed the wall in the middle of the magnet and would have transformed back into light in the second half of the magnet. However, there was only darkness during the complete 36 hours of data taking.

Nevertheless, Lindner remains confident and plans the continuation of ALPS. “There are many hints for axion-like particles in many sectors of physics,” he explains. “We only have to measure with more precision.” According to theorists’ calculations, it is necessary to look about 10,000 times more precisely to detect these particles. In order to do that the complete experiment has to be refurbished and equipped with a stronger laser, more magnets, and a more sensitive detector.

The follow-up experiment ALPS II will be equipped with an infrared laser beam instead of a green one, with at least 150 times more power, and with the advantage that the optical cavity will be built with custom-tested components. A second cavity in the rear part will enhance the probability of a conversion of the hidden particles back to light. Two LHC dipoles or four HERA proton magnets, for example, could be used as magnets for ALPS II. In comparison to the single magnets currently in use, there is the advantage of building part of the cavities’ mirror system between the magnets, which makes them more accessible and adjustable.

For measuring the light at the end of the magnet a superconducting detector could be installed which would also improve the measuring sensitivity by a factor of 100. A possible site is also available for the installation of the experiment: the X-ray Free Electron Laser, or XFEL, mock-up tunnel, which will be become available in 2013 at the latest.

In about one year, the ALPS collaboration will have completed the Technical Design Report for ALPS II. And when Lindner is talking of “his” experiment, you won’t doubt for a second that this is going to happen.

ALPS and the light particles

The “light-through-the-wall” experiment is seeking for very light or low-energy particles (<1eV). According to a string-theory-inspired extension of the Standard Model, a large variety of these particles may exist. These WISPs (weakly interacting sub-eV particles) only have an extremely low interaction with normal matter. They are not visible in high-energy collisions as in the LHC, but they might emerge from light and be detected in highly sensitive experiments such as ALPS. These particles might help to explain various physics effects: For example, dark matter might consist of these particles.

by Thomas Zoufal

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LHC: the catalog shot

May 6, 2010 | 5:59 am

The Jameco Electronics May 2010 catalog cover featuring the LHC's ATLAS experiment.

The Jameco Electronics May 2010 catalog cover featuring the LHC's ATLAS experiment.

In case you hadn’t noticed, I’m a geek. I haven’t done research physics since I became a journalist but the geekiness remains, often in the form of building electronic stuff. I like to make embedded microprocessor objects that react to the environments and behaviors around them, and so I need to get my hands on all kinds of electronic bits and pieces.

My geek confession for today: I love the day the Jameco Electronics catalog arrives in the mail. But to make it even geekier, I was excited to see that the latest cover features a photograph of the construction of the ATLAS detector at the Large Hadron Collider. It’s a photo many symmetry readers will have seen before.

What I really like about the LHC pic on the catalog cover is that it reminds us that behind those many kilometers of accelerator, behind the many floors of detector, are electronic components that might be smaller than you can easily handle or larger than you. And behind those electronic components are the research discoveries that allowed electronics to be invented. And behind those research discoveries are the fundamental laws of electromagnetism, a unification of the previously separate observations of electricity and of magnetism, and the discovery of how the photon is part of that world.

So we go full circle: from the unification of laws based on observation, we create technology. Some of this technology revolutionized society, while other parts fed back into the research enterprise. As that research enterprise has evolved, we now stand at a point where we are attempting to understand an even larger-scale unification of the laws of the universe, through the discoveries anticipated at the LHC.

With that path of progress, what can we say about the next round? Maxwell couldn’t have anticipated the world of electronic gadgetry, and physicists now can’t predict what will come from the discoveries at the LHC. We can, however, be confident that there will be world-changing developments somewhere down the road.

David Harris

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Frontier guides computing through the collision landscape

May 5, 2010 | 10:31 am

Just like you might have trouble navigating using this antique map, detector experiments can’t make sense of their data using an out-of-date map of their detector. Image courtesy Boston Public Library’s Norman B. Leventhal Map Center under Creative Commons license

Just like you might have trouble navigating using this antique map, detector experiments can’t make sense of their data using an out-of-date map of their detector. Image courtesy Boston Public Library’s Norman B. Leventhal Map Center under Creative Commons license

From today’s issue of iSGTW.

The colossal particle detectors that monitor collisions at the Tevatron in Illinois and the Large Hadron Collider in Switzerland are unique beasts.

Scientists design most of the parts inside them to meet an individual set of specifications. But every once in a while, they find something the detectors can share.

Scientists at the CMS and ATLAS experiments at CERN are using a software system that Fermilab’s Computing Division originally designed for the CDF experiment at the Tevatron. The system, called Frontier, helps scientists distribute at lightning speed information needed to interpret collision data. The system is based upon the widely used Squid web cache technology.

“Since data is often shared between sites or pulled from a remote site, the speed of data return is critical,” said John DeStefano, an engineer at the RHIC and ATLAS Computing Facility at Brookhaven National Laboratory. “Not even the fastest database servers can bridge the physical gap between geographically disparate sites. People noticed how efficiently Frontier worked for CMS, and so far there has been a notable benefit for ATLAS as well.”

Frontier caught on thanks to the interconnectedness of the particle physics community, said Fermilab engineer Liz Sexton-Kennedy. Many scientists now working on experiments at the LHC also worked on experiments at the Tevatron.

Fermilab computer scientists Jim Kowalkowski and Marc Paterno came up with the original idea for Frontier. A group of computer scientists at Fermilab who had previously gained experience with a similar system designed for the DZero experiment worked to implement the ideas at CDF. Another group from Johns Hopkins University contributed by testing the system.

Adjusting for a changing frontier

Particle detectors like CDF, CMS and ATLAS are large, complex machines whose many parts move in amounts imperceptible to the eye but are critical to a scientist making precise measurements of particle tracks.

A diagram of the Frontier architecture within CMS; to enlarge, please click on the image. Image courtesy Dave Dykstra, Fermilab

A diagram of the Frontier architecture within CMS. Image courtesy Dave Dykstra, Fermilab

This makes reading data from inside a particle detector a bit like driving in a dream landscape whose features frequently shift. To navigate such an unpredictable setting, drivers continually need to swap out their maps for new, updated ones. In order to properly read data that detectors collect about an event, physicists need to know the lay of the land inside the detector at the time of collision.

What’s more, hundreds of thousands of computers around the world all need to pair that updated information with collision data as they analyze it, said Dave Dykstra, a Fermilab engineer who now heads the Frontier project.

“All of them need to load the data all at once,” he said. “It’s a big challenge.”

Scientists do not monitor the conditions of the detectors during each individual collision. In the CDF detector, beams of protons and antiprotons cross paths about 1.7 million times each second, each pass representing an opportunity for collisions. Scientists plan to cross beams of even more protons 3.1 million times per second in the CMS and ATLAS detectors once the LHC is up to full power.

Rather than try to keep up, scientists take new readings at frequent, regular intervals. A Frontier server takes information about the changing landscape of the detector from a database and sends it to other servers around the world, which then cache the information and share it with other, nearby computers. Only the Frontier server needs to request updated maps from the database.

The Frontier system uses HTTP, the same language Web sites use to communicate with Web browsers, to send database requests out to servers. HTTP is nimble enough to deliver information over long distances in multiple short bursts, and designed to handle huge numbers of users. Without Frontier, experiments would communicate through database queries better suited to a smaller number of local users.

Thanks to a recent upgrade by Dykstra, the system now saves even more time and computing power by skipping the step of reloading information if the detector maps have not changed. Frontier has earned its popularity, but like the computers it keeps supplied with new data, it must keep adapting to keep up with the changing landscape.

Kathryn Grim

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