The ILC in one minute flat

July 22, 2010 | 3:27 pm

The folks working on the proposed International Linear Collider have created a one-minute animation  that flies you through its 30-kilometer-long tunnel.  It has no sound, but the visuals speak for themselves:  Electrons and positrons are generated on opposite arms of the collider, circle in opposite directions in a damping ring, fly out to the ends of the machine and jet back into the middle, where they collide.  For more details about the humongous project – which is scheduled to present a progress report at the International Conference on High Energy Physics on Saturday –  go here.

Glennda Chui

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Cool summer job: Teens build a neutrino detector

July 15, 2010 | 5:35 pm

If  you’ve been reading symmetry for a while you may remember our reports on the Cyclotron Kids – Heidi Baumgartner, Peter Heuer, and German Diagama  — who came home from astronomy camp three years ago with the dream of building a cyclotron.  (They’re still at it; we’ll have an update on the Kids as well as other amateur cyclotron builders in the August issue of symmetry.)

So we were pleased to see this story from Minnesota Public Radio on students from the University of Minnesota with an unusual summer job: building parts for a neutrino detector.  It’s a smaller version of the giant detector, as tall as a six-story building, that will be installed deep in Soudan Mine in Minnesota as part of the Fermilab-based NOvA project.

In a 100,000-square-foot warehouse near campus, 19-year-old Dylan Skerbitz is cleaning the ends of a white PVC panel the size of a garage door. He’s using a corona arc discharge machine, which looks like a high-tech hair dryer spitting out a purple flame.

“It creates an electrical spark, and it burns off any excess dust or particles so glue will connect better with this,” he says.

Each one of these PVC panels — there will be about 500 stacked together in the finished detector — is made up of rows of tubes. Each of the tubes will be fitted with long strands of fiber optic thread. Those threads will pick up barely detectable flashes of light when neutrinos do a sub-atomic dance through the detector. A computer will record the findings.

Not exactly a do-it-yourself project, but still impressive, especially considering that the UM team includes both physics buffs and liberal-arts types.  The mini-detector will be used to test the technology of the maxi-experiment.  The MPR  website has photos.

Glennda Chui

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June 2010 issue of symmetry now online

July 14, 2010 | 12:26 pm

In this issue:

Science road trip,”  an epic tour of American Big Science.

The Muon Guys lead an experiment, called Mu2e, that will look for an event so rare that it was thought no one could build a machine sensitive enough to see it.

 In “The LHC decoded,” walk through three of the computer displays that highlight scientific and technical milestones from the Large Hadron Collider’s first few months of operation.

Plus:  A CERN chip inspires a teen space project and high-school research network;  an artist turns electronic junk into works inspired by particle physics; the fast-paced life of an accelerator scientist at the world’s brightest X-ray laser; sterilizing medical supplies with accelerators; CERN invents the touch screen; charged leptons explained;  and, as always, Signal to Background and highlights from our blog.

You can download a pdf version of the magazine here.

Glennda Chui

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People in physics: Listening to the universe with Amedeo Balbi

July 12, 2010 | 5:15 am

Photo_balbi_croppedAmedeo Balbi, researcher at the University of Rome “Tor Vergata”, is one of the rare scientists with a gift for explaining his research to a non-expert public. His main field of expertise is the study of the Cosmic Microwave Background, the fossil radiation from the big bang. More recently he became interested in dark energy and the interdisciplinary realm of astrobiology, the scientific study of life outside our planet Earth.

Balbi always had a knack for communicating science. An avid reader of popular science books, he found it quite natural to become a tour guide at Italy’s National Institute for Nuclear Physics in Frascati when he was a student. Off-duty, he never got tired of explaining what he was doing to his friends. He practiced the story of the birth and evolution of the Universe so often that he began to toy with the idea of writing a book about it, with a plot based on the captivating tale of scientists’ quest to map the early Universe using the Cosmic Microwave Background radiation.

“After all,” Balbi muses, “if the Universe had always been the same, cosmology would not be as fascinating as it is.”

Balbi started writing his book in the summer of 2004, while a visit to Fermilab in Illinois provided a break from Rome’s nightlife. But two years later he was still too absorbed by his research to finish. Then in 2006 the Nobel Prize was awarded to George Smoot for his work on the Cosmic Background Explorer Satellite. Balbi had  worked with Smoot on the MAXIMA experiment, and this gave him the push that he needed. Within a few months he had not only finished the book but had also started Keplero, now one of Italy’s top science blogs.

Balbi’s book “The Music of the Big Bang” – available in English – reads like a novel. It tells the story of the Universe we live in, as it has been decoded by cosmologists from the faint footprints left in the Cosmic Microwave Background: the acoustic waves in the CMB are like a music in which scientists have to try and identify the different instruments. The language is simple and direct, although he makes no concessions to inaccuracy in the scientific descriptions. As with all good science communicators and storytellers, Balbi refers the readers to familiar images to help them grasp mind-boggling thoughts. The book does not contain any personal recollections: Balbi’s true interest lies in the tale of science, and not in the anecdotes. Nevertheless, the book is also a great introduction to the job of cosmologists, who can be considered like archaeologists studying the most ancient signal of the big bang with the tools offered by physics and mathematics.

The same clarity of mind, coupled with a dose of humor and extensive pop culture references, is evident in his blog posts (unfortunately Italian-only). When blogging, Balbi first finds a good story to tell, and then finds a smart way to tell it, often with some hidden references to songs, movies, books, or anything that triggers his imagination. And so his readers may find themselves discussing whether “And I feel fine,” the title of a post about the possible dangers of mini-black holes created at the LHC, comes from a Beatles or R.E.M. song (the correct answer was R.E.M.).

Balbi is always looking for the next challenge. Even though his research is now entering an extremely exciting period, as he becomes deeply involved in the analysis of the data sent by the Planck space observatory, he could not resist joining the prestigious crew of bloggers for the online newspaper “Il Post”. Time to brush up on your Italian!

by Manuela Cirilli

Guest author

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Protons crack a Dead Sea Scroll secret

July 6, 2010 | 5:01 am

One of the Dead Sea Scrolls, 4Q Testimonia

One of the Dead Sea Scrolls, 4Q Testimonia

Researchers who probed tiny pieces of a Dead Sea Scroll with protons found that its chemistry matches the chemistry of the water  in the area where the ancient document was found – in Qumran, near the Dead Sea.  This supports the idea that it was made locally, according to the INFN, Italy’s National Institute for Nuclear Physics.

This particular scroll, one of 900 that were discovered half a century ago in caves near the Dead Sea, is known as the Temple Scroll.  Unlike other Dead Sea scrolls that constitute the earliest known biblical texts, dating from about 200 years before the birth of Christ to several decades after it, this one describes the construction and life of a temple and dictates how laws are to be communicated to the people.

The analysis was done at INFN’s National Laboratories of the South using protons from a particle accelerator and a new system, called XPIXE, that was invented there.  Details are in the INFN press release.

Press Release

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SLAC’s new X-ray laser peels and cores atoms

July 2, 2010 | 5:30 pm

 
The world's first hard X-ray free-electron laser started operation with a bang. First experiments at SLAC National Accelerator Laboratory's Linac Coherent Light Source stripped electrons one by one from neon atoms (illustrated above) and nitrogen molecules, in some cases removing only the innermost electrons to create "hollow atoms." Understanding how the machine's ultra-bright X-ray pulses interact with matter will be critical for making clear, atomic-scale images of biological molecules and movies of chemical processes. (Image: SLAC InfoMedia Solutions.)

The world's first hard X-ray free-electron laser started operation with a bang. First experiments at SLAC National Accelerator Laboratory's Linac Coherent Light Source stripped electrons one by one from neon atoms (illustrated above) and nitrogen molecules, in some cases removing only the innermost electrons to create "hollow atoms." Understanding how the machine's ultra-bright X-ray pulses interact with matter will be critical for making clear, atomic-scale images of biological molecules and movies of chemical processes. (Image: SLAC InfoMedia Solutions.)

 In the March/April 08 issue of symmetry we introduced SLAC’s Linac Coherent Light Source, a first-of-its-kind machine that would probe matter at the atomic scale with ultra-fast, ultra-bright pulses of X-ray laser light.  Now the first scientific results have been published, from early experiments aimed at understanding how these powerful pulses interact with matter in its simplest forms — individual atoms and molecules of nitrogen gas, which contain two atoms each.  Here’s the text of the SLAC press release, plus links to stories in Wired and Nature.   And yes, we’re stealing respectfully appropriating Nature’s headline, because it’s awesome.

Menlo Park, Calif.—The first published scientific results from the world’s most powerful hard X-ray laser, located at the Department of Energy’s SLAC National Accelerator Laboratory, show its unique ability to control the behaviors of individual electrons within simple atoms and molecules by stripping them away, one by one—in some cases creating hollow atoms.

These early results—one published today, the other last week—describe in great detail how the Linac Coherent Light Source’s intense pulses of X-ray light change the very atoms and molecules they are designed to image. Controlling those changes will be critical to achieving the atomic-scale images of biological molecules and movies of chemical processes that the LCLS is designed to produce.

In a report published in the July 1 issue of Nature, a team led by Argonne National Laboratory physicist Linda Young describes how they were able to tune LCLS pulses to selectively strip electrons, one by one, from atoms of neon gas. By varying the photon energies of the pulses, they could do it from the outside in or—a more difficult task—from the inside out, creating so-called “hollow atoms.”

“Until very recently, few believed that a free-electron X-ray laser was even possible in principle, let alone capable of being used with this precision,” said William Brinkman, director of DOE’s Office of Science. “That’s what makes these results so exciting.”

Young, who led the first experiments in October with collaborators from SLAC and five other institutions, said, “No one has ever had access to X-rays of this intensity, so the way in which ultra-intense X-rays interact with matter was completely unknown. It was important to establish these basic interaction mechanisms.”

SLAC’s Joachim Stöhr, director of the LCLS, said, “When we thought of the first experiments with LCLS ten years ago, we envisioned that the LCLS beam may actually be powerful enough to create hollow atoms, but at that time it was only a dream. The dream has now become reality.”

In another report, published June 22 in Physical Review Letters, a team led by physicist Nora Berrah of Western Michigan University—the third group to conduct experiments at the LCLS—describes the first experiments on molecules. Her group also created hollow atoms, in this case within molecules of nitrogen gas, and found surprising differences in the way short and long laser pulses of exactly the same energies stripped and damaged the nitrogen molecules.

“We just introduced molecules into the chamber and looked at what was coming out there, and we found surprising new science,” said Matthias Hoener, a postdoctoral researcher in Berrah’s group at WMU and visiting scientist at Lawrence Berkeley National Laboratory who was first author of the paper. “Now we know that by reducing the pulse length, the interaction with the molecule becomes less violent. “

While the first experiments were designed to see what the LCLS can do and how its ultra-fast, ultra-bright pulses interact with atoms and molecules, they also pave the way for more complex experiments to come. Its unique capabilities make the LCLS a powerful tool for research in a wide range of fields, including physics, chemistry, biology, materials and energy sciences.

The LCLS forms images by scattering X-ray light off an atom, molecule or larger sample of material. Yet when the LCLS X-rays are tightly focused by mirrors, each powerful laser pulse destroys any sample it hits. Since certain types of damage, like the melting of a solid, are not instantaneous and only develop with time, the trick is to minimize the damage during the pulse itself and record the X-ray snapshot with a camera before the sample disintegrates.

Both teams found that the shorter the laser pulse, the fewer electrons are stripped away from the atom or molecule and the less damage is done. And both delved into the detailed mechanisms behind that damage.

Atoms are a little like miniature solar systems, with their electrons orbiting at various distances from the nucleus in a sort of quantum fuzz. To make things simpler, scientists describe the electrons as orbiting in “shells” at specific distances from the nucleus. The innermost shell contains up to two electrons, the next one up to eight, the third one up to 18, and so on.

Since they’re closest to the positively charged nucleus, the two innermost electrons are generally the hardest to wrest away. But they also most readily absorb photons of X-ray light, and so are the most vulnerable to getting stripped away by intense X-rays.

Although previous experiments with intense optical lasers had stripped neon atoms of most of their electrons, Young’s was the first to discover how ultra-intense X-ray lasers do this. At low photon energies, the outer electrons are removed, leaving the inner electrons untouched. However, at higher photon energies, the inner electrons are the first to be ejected; then the outer electrons cascade into the empty inner core, only to be kicked out by later parts of the same X-ray pulse. Even within the span of a single pulse there may be times when both inner electrons are missing, creating a hollow atom that is transparent to X-rays, Young said.

“This transparency associated with hollow atoms could be a useful property for future imaging experiments, because it decreases the fraction of photons doing damage and allows a higher percentage of photons to scatter off the atom and create the image,” Young said. She said application of this phenomenon will also allow researchers to control how deeply an intense X-ray pulse penetrates into a sample.

Berrah’s team bombarded puffs of nitrogen gas with laser pulses that ranged in duration from about four femtoseconds, or quadrillionths of a second, to 280 femtoseconds. No matter how short or long it was, though, each pulse contained the same amount of energy in the form of X-ray light; so you might expect that they would have roughly the same effects on the nitrogen molecules.

But to the team’s surprise, that was not the case, Hoener said. The long pulses stripped every single electron from the nitrogen molecules, starting with the ones closest to the nucleus; the short ones stripped off only some of them.

Their report attributes this to the “frustrated absorption effect”: Since the molecule’s electrons are preferentially stripped from the innermost shells, there is simply not enough time during a short pulse for the molecule’s outermost electrons to refill the innermost shells and get kicked out in turn.

With all this activity going on inside the atom, scientists have a new way to explore atomic structure and dynamics. Further experiments have investigated nanoclusters of atoms, protein nanocrystals and even individual viruses, with results expected to be published in coming months.

Young’s research was primarily supported by the DOE Office of Science, with additional support from the Alexander von Humboldt Foundation. Berrah’s research was supported by the DOE Office of Science.

The LCLS is a DOE Office of Science-funded project led by SLAC National Accelerator Laboratory in partnership with Argonne National Laboratory and Lawrence Livermore National Laboratory. Pacific Northwest National Laboratory provided initial project management support. Lawrence Berkeley National Laboratory and Cornell University contributed key subsystems. University of California, Los Angeles provided theoretical physics support throughout the project; Brookhaven and Los Alamos national laboratories were active in the early stages of LCLS research and development.

SLAC National Accelerator Laboratory is a multi-program laboratory exploring frontier questions in photon science, astrophysics, particle physics and accelerator research. SLAC is located in Menlo Park, California, and is operated by Stanford University for the U.S. Department of Energy Office of Science.

Argonne National Laboratory seeks solutions to pressing national problems in science and technology. The nation’s first national laboratory, Argonne conducts leading-edge basic and applied scientific research in virtually every scientific discipline. Argonne researchers work closely with researchers from hundreds of companies, universities, and federal, state and municipal agencies to help them solve their specific problems, advance America’s scientific leadership and prepare the nation for a better future. With employees from more than 60 nations, Argonne is managed by UChicago Argonne, LLC, for the U.S. Department of Energy’s Office of Science.

Western Michigan University is a dynamic, student-centered research university with an enrollment of 25,000. WMU is focused on delivering high-quality undergraduate instruction, advancing its growing graduate division and fostering significant research activities.

Glennda Chui

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World Cup Fever at CERN

July 2, 2010 | 12:12 pm

Normally, the data points from the CERN cafeteria are extremely repeatable over the course of a week.  Monday through Friday the data points cluster briefly at the coffee machine at 9 am, and then around the pizza station at 12:30.  They shift from the patio region to the indoor region around October, and reverse their movement in April. The start up of the Large Hadron Collider saw an increase in data volume, but otherwise the points spread themselves out evenly over the expanse of the cafeteria, day in and day out.

World Cup fans cram into the CERN cafeteria, even sitting on the floor, to get a seat where they can see the game.

World Cup fans cram into the CERN cafeteria, even sitting on the floor, to get a seat where they can see the game.

Anyone watching the data from the past few weeks, however, will notice a bump that appears just to the right of the cash registers, near a satellite TV projector, between 4 and 5:30 pm. The bump appears again between 8:30 and 10 pm. The data points tend to remain rigid for most of the 90 minutes, with momentary displays of excited behavior.

CERN has always been a hub of international collaboration; a place where people from many nations come together for a single goal. It is said that in the CERN cafeteria, a visitor can hear ten languages being spoken over the course of one meal. During the past few weeks, national pride has hit a high, with the World Cup football (soccer) competition in full swing. Save for the Olympics, it is the only sporting event  where everyone at CERN has a home team to cheer for.

CMS physicist Dave Barney, who also handles outreach for the collaboration, confesses that people have had the games running on laptops during shifts in the control room. “Our philosophy is professionalism comes first and if there is any spare time to look at football then it is ok,” said Barney in an email. “And in general (what I have seen) the matches might be on in the background – no-one is *just* watching them!

“Lots of us are REALLY into the competition,” Barney continued. He wore his England jersey to work even after his home country’s elimination. “Working in an international environment makes it quite fun in a way – lots of teasing! But it also makes you feel like a school kid, waiting for the embarrassment of facing your friends after a disastrous performance from your own team against theirs.”

Another story from Burton DeWilde, a graduate student from Stony Brook University working on ATLAS, confirms Barney’s report:

All eyes on the game.

All eyes on the game.

“I did manage to catch America’s third game, against Algeria. I was in a bar surrounded by Brits watching their game (against Slovenia) on a television, while a handful of Americans huddled around a laptop screen in 90 minutes of tense anticipation. The Brits had already won, but we were still tied 0-0. In the last couple minutes, though, America finally scored a goal. We went CRAZY, and you could see the Brits look over with something between disappointment and amusement. At any rate, everybody in the bar was thrilled that their team was progressing — except one person, who was from Slovenia. America’s victory had kicked his team out of the competition; you could actually hear his heart break. He finished his beer and snuck quietly away. Better luck next World Cup…”

As the World Cup enters the third round, and home countries are defeated, many people say they continue to cheer for other countries – perhaps those they once visited or lived in, or countries where colleagues are from. Some CERN members also admit that their World Cup loyalties come down to cheering against the team that eliminated their home country (though always with a wink and a smile, and never so seriously as to offend colleagues from those countries).

Matches today and tomorrow, July 2nd and 3rd, determine which teams will move onto the semi-finals. Still in the competition are CERN member states Spain, Germany, and the Netherlands — which knocked Brazil out of the competition early today — plus Argentina, Uruguay, Paraguay, and Ghana.

Calla Cofield

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New Yorker cartoonist Roz Chast on the LHC

July 1, 2010 | 5:14 am

cover_big

One of our favorite symmetry covers is the one drawn by New Yorker cartoonist Roz Chast for our May 07 issue – “a family album of teensy-weentsy particles (some slightly less than real),” as she put it.  I’m especially fond of the slepton and the poserino.  She also illustrated our story on the search for dark energy. Well, she’s at it again with a brochure of FAQs on the Large Hadron Collider.  It ‘s reprinted in today’s iSGTW newsletter:

Q.  What would happen if I went inside it?

A.  Just. Don’t.

Glennda Chui

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CERN opens dazzling new public exhibition

June 30, 2010 | 1:58 pm

Inside Universe of Particles (image courtesy of CERN).

Inside Universe of Particles (image courtesy of CERN).

It’s like stepping into a science fiction film: Eerie blue and green lighting; spherical white chairs with black cushions; touch-operated computer information stations; a full-wall projection of stars and galaxies; and a calming voice coming over a loudspeaker and asking, “Why are we here?”

If the architectural firm behind the new exhibition, Atelier Bruckner, wanted to get their audience excited about science, they have certainly succeeded. The new CERN public exhibition Universe of Particles will make a fantastic starting point for lab visitors. In dramatic fashion, it presents them with the big, exciting questions that CERN scientists would like to answer, like “What is dark energy?” and “What will be the fate of our universe?”  These questions alone will inspire excitement in many people, but the design group has used a dramatic setting to ramp up visitors’ excitement. Like a good sci-fi flick, it ignites the feeling of excitement that comes with the start of a great adventure.

The Interactive Globe features information about facilities working with CERN world wide.

The Interactive Globe features information about facilities working with CERN world wide.

From the entrance of the room, visitors notice what appears to be a large globe, standing over four feet high. But an up-close view shows that the massive ball is blank, until a projection from above turns it into a globe of the Earth. As visitors spin the globe (technically referred to as the Interactive Ball), the light projection keeps up and reveals a complete map of our planet, but with the addition of circular markers that open up to reveal information about each country’s participation at CERN. Hit a button to change the rolling display to a timeline of CERN’s history. A few other display screens use the same projection-based, touch sensitive technology that makes you feel like you’re playing with a giant iPhone.

To get away from the crowd for a moment, visitors can sink into chairs cut from white spheres, creating a small cave-like setting. Select a language, and a speaker begins to explain the search for the cause of the matter/antimatter asymmetry or the basis for string theory. Display cases, also cut out of futuristic white spheres, feature a few artifacts of physics like the first World Wide Web server and parts from old detectors.

The Globe (image courtesy of CERN).

The Globe (image courtesy of CERN).

About every half hour, the lights dim even more, and a soothing voice from above begins to narrate a visual presentation about the great universal questions that CERN science seeks to answer. The projection plays on one segment of the curved wall, and on a large angled surface in the middle of the room. When the show ends, a projection on the slanted surfaces plays recreations of particle collisions.

The new exhibit rests inside the most recognizable building at CERN, The Globe (although it is technically not on the CERN campus, but directly across the street from the main entrance). The Globe of Science and Innovation is a 130-foot-wide, 88-foot-tall sphere made of five types of timber, making it a natural carbon sink. It was built for an exhibition in Hanover, Switzerland, as a symbol of sustainable building. Two walking ramps spiral up the outside of The Globe from the ground floor (where the exhibition is located), and another walking ramp connects the two floors from the inside.  The second floor is a high-ceilinged room with exposed wood walls. CERN uses the space for some press conferences and public events. The bottom half is now dedicated to the exhibit center, along with the hallway winding down on the inside, which features posters explaining the big bang.

During the audio visual presentation inside Universe of Particles (image courtesy of CERN).

During the audio visual presentation inside Universe of Particles (image courtesy of CERN).

Rolex sponsored the entirety of the exhibition hall, and Jacques Baur, Associate Director and Head of Research for the company, spoke at a press event for the new exhibition last week. Baur emphasized just how impressed he was with the detectors he saw at CERN and the work going on there. He discussed how the exhibit falls under Rolex’s philosophy of philanthropy, particularly toward science.

Universe of Particles is open to the public starting July 1, 2010.

Calla Cofield

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CMS Exotica hotline leads hunt for exotic particles

June 24, 2010 | 1:59 pm

Strangers in the dark: they meet, make contact, and break away with force, careless of what they leave behind. At midnight each night, snapshots of these frenzied chance encounters are collected for curious eyes. In the morning, those onlookers reconstruct the story that each image tells, tracing the mysterious paths born from a fateful meeting.

This is the CMS exotica hotline, and no, it’s not a 900 number.

Those snapshots are event displays, pictorial descriptions of proton collisions in the CMS detector, selected from the previous 24 hours. Every morning, 10 CMS collaborators volunteer to review between 20 and 100 hotline displays to get a sneak-peek at the latest data. By picking out the most unusual events first, CMS physicists hope to learn more about how the detector is functioning and spot exotic physics.

Exotic physics is the physics that breaks rules and defies expectations. This is the realm beyond the Standard Model and even beyond supersymmetry —the domain of the unstable and excited, the string balls, black holes, and extra dimensions. The CMS group devoted to seeking out these events is called the exotica group, and the hotline supports their search.

Every morning, CMS collaborator Tulika Bose of Boston University, a lead developer of the hotline, scans event displays to parse potential physics from peculiar equipment signals. She explains that the hotline offers an open-minded way of developing new search criteria for exotic events.

“New physics at the LHC may have none of the characteristics that our search groups are looking for, so this helps cover the area of the unknown,” Bose says.

The concept is not without controversy. Event displays are traditionally created only after extensive analyses suggest an event deserves a closer look. The exotica hotline, in a sense, works backwards, using a graphic display before numerical analysis.

“The hotline is not to replace the analysis,” says Massimiliano Chiorboli, a CMS collaborator who co-designed the software for the exotica hotline. “CMS is a very big community and a lot of people are working on analysis. We want to provide more information to those analysts and show the community when we recognize something special.”

The inspiration for the project comes from a previous CERN experiment on the Super Proton Synchrotron. In the ’80s, the UA1 experiment’s control room kept a bell that collaborators would ring at the first hint of a special event. A similar early warning system was later used by experiments at DESY’s HERA and Fermilab’s Tevatron collider. This inspired Chiorboli, of the University of Catania and INFN, and CERN’s Maurizio Pierini to develop a similar system to alert their collaborators.

At midnight each night, Chiorboli and Pierini’s program collects express-stream events from the previous day. The express-stream data is a subset of the total collected CMS data, assembled and reconstructed into recognizable physics events for those who need to quickly check the detector’s condition. Displays for the hotline are filtered to include only the most convincing and interesting events.

Around 9 a.m., the hotline software sends an automated e-mail summarizing select displays. The 10 volunteers who receive this e-mail come from all areas of the collaboration. They critically examine the hotline to decipher what they see. Volunteers are also on the lookout for strange events that could be misleading or distracting in later analysis.

Thus far, the hotline has called attention to unusual detector signals and rare but familiar physics, such as Z and W bosons. That makes this an ideal time to fine-tune the hotline’s filters, a task that Alexey Ferapontov of Brown University, who looks for exotic multi-jet events, assists.

“The exotica hotline cannot be treated as an analysis, but it gives us valuable experience,” Ferapontov says. “The whole CMS collaboration can profit from this and there is always the possibility that we find something really new and unseen before. This makes participation very fun!”

The exotica hotline offers new thrills to CMS collaborators in their physics searches—and what’s more, they won’t get in trouble for watching at work.

by Daisy Yuhas

Symmetry Intern

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