Fermilab's luminosity celebration

April 18, 2008 | 4:09 am

Upgrades–we often think about them in the everyday stuff of the world. You can upgrade your car, your computer, your software, even the windows in your home.

What if you designed (or bought) an item and you were told, “We can upgrade that so it delivers 300 times its performance!” That would be like upgrading a Scion to a Lamborghini! Would you believe it?

After many years, many brilliant breakthroughs, and a lot of plain old hard work, the Fermilab Tevatron is in such a position, where it is now delivering as many collisions to the experimenters in a record-breaking week’s time as it did during its first experimental run, which lasted for years.

Expectations were high for the data delivery during Run II; with 100 times the data expected. The Fermilab Accelerator Division has delivered.

With the Tevatron running so well, the experimenters at CDF and DZero wanted to celebrate the successes with the Accelerator Division. A simple celebration of pizza, drinks, and fellowship was held at Kuhn Barn in early April, 2008.

The Tevatron’s performance has helped keep the collaborations intact, with great potential for discovery in the tremendous amount of data. There has been a groundswell of support for extending Run II to capitalize on the remarkable luminosity.

The following is a brief look inside the luminosity celebration.

By Jim Shultz, Fermilab

Guest author

2 Comments »

A first encounter with the LHC

April 18, 2008 | 2:32 am

Katrin Voss visits the LHCKatrin Voss is Germany’s new Large Hadron Collider communicator. She doesn’t come from a science background so was excited to see the accelerator and detectors up close. She shared her first experience of visiting CERN with the readers of ILC NewsLine.

I started the Open Day at the ATLAS experiment. Although I had seen quite a few photographs of ATLAS before coming to CERN, I was amazed at the sheer size of the experiment. The information that 4 000 kilometres of cable had been installed in it is almost inconceivable for someone who has never had to do with particle accelerators. Equally interesting were the visit at the ATLAS control centre and the short 3D film about the construction work at ATLAS.

David Harris

1 Comment »

Like droplets on a spiderweb

April 17, 2008 | 7:00 am

I just saw physicist Peter Steinberg’s blog on artwork with ties to science. The image that caught my eye shows an intricate web occupying an entire room, which he describes as “a room-size set of connecting elastic rope segments.”

I’m not always a fan of sculpture, but every once in a while you find examples that demand your attention. The artist, Tomas Saraceno, is known for combining elements of physics, engineering, and architecture into his works. This particular piece, from his latest exhibition “Galaxies Forming Along Filaments, Like Droplets Along the Strands of A Spider’s Web” is an interpretation of our early universe.

The gallery describes the work this way:

In this new installation Saraceno takes the spider’s web as a starting point. Investigating how the gossamer thin filaments of these intricate webs are able to suspend life by way of intricate geometry, Saraceno suggests at a conceptual architectural proposal that relies on this most delicate and prehistoric system of life to take us into our future. Of particular interest is the application of this phenomenon throughout the history of time. A keystone to Saraceno’s fascination with these web constructions was the recent discovery that suggests the early universe was a sponge-like form, with galaxies forming along filaments, like droplets on a spider’s web.

Steinberg writes:

I have to admit that it does a pretty good job evoking the images coming from dark matter simulations, where dark matter clumps up into filaments that sketch out a “spongy” structure.

By Matt Cunningham, symmetry intern

Guest author

No Comments »

Extreme particle acceleration with lasers (APS April 2008)

April 17, 2008 | 3:47 am

The APS April meeting is over but I still have a few more stories to post and I’ll get them up over the next week.

The leading edge of particle acceleration technology in use today is made of superconducting cavities that shape radiofrequency waves for particles to surf to higher energies. However, that technology is limited because the cavities themselves, made of superconducting niobium, have a maximum strength of rf waves that they can sustain.

Machines are now enormous as they strive for the energy frontier that physicists want to explore. There is, however, a limit to the size of big machines, particularly for financial and space reasons. That size limit is the motivation for exploring the alternative techniques being tested now. One of these is plasma wakefield acceleration. It’s a promising approach and each year there are great new advances, some of which were reported here today. A topic we haven’t really talked about in symmetry is an alternative wakefield approach using lasers.

Wim Leemans of Lawrence Berkeley National Laboratory talked about a project called BELLA that could potentially match the energy of the proposed 20 kilometer International Linear Collider in a few hundred meters instead. The technology is years away from working so that comparison is really just to give an idea of how much greater the acceleration is than conventional superconducting technology. However, if laser wakefield (or plasma wakefield) acceleration is successful, it would open the way to creating compact particle accelerators for medical applications and other uses.

The idea is to create a narrow channel in sapphire with a low density gas inside. A laser is piped down the channel and pushes a bunch of electrons, getting them to high energies. So far, the technique has been demonstrated to work to do some acceleration but hasn’t achieved the really high energies needed to be competitive with energy frontier machines like the Tevatron (for now) and the LHC (later this year).

It’s exciting stuff and also necessary if particle accelerators are to increase the energy frontier much beyond the LHC and ILC targets.

See all posts from the American Physical Society April 2008 conference here.

David Harris

No Comments »

DAMA-LIBRA presents new dark matter claim

April 17, 2008 | 1:30 am

On Saturday, I mentioned that sources had told me the DAMA-LIBRA collaboration were about to claim that their new experimental run supported their 2000 result.

I was traveling when the results were released so I’ll leave you in the capable hands of Dennis Overbye at the New York Times and JR Minkel at Scientific American to give you more details.

However, the quick version is that the DAMA-LIBRA again claim to see evidence of dark matter, but the result is complicated and still contentious. Other sources tell me that even the scientists working on the experiment aren’t sure about how to best interpret their results.

More will come out over time but it doesn’t look like anybody is too convinced at this point that this will count as a discovery of dark matter particles. Tommaso Dorigo is skeptical.

You can judge some of this for yourself by looking at the slides presented at the meeting by Rita Bernabei.

David Harris

No Comments »

Science is cool???

April 16, 2008 | 7:48 am

High-energy particle physics uses mammoth, powerful metal-and-wire machines to search for the smallest constituents of life and matter by creating “explosions of energy” at nearly the speed of light. The process recreates at a tiny, tiny scale the primordial conditions of the universe just after the big bang.

I was sure I could excite a rough-and-tumble boy with this big, violent concept. Really, you can’t get much more monumental–or, in boy-speak, “cool”–than that, right? Yet, as I tried to explain what Fermilab does to my science-loving 8-year-old son on the way to a Wonders of Science show there, I was hard-pressed to convince him that high-energy physics was even a little bit cool.

“They shoot a big beam, like a laser, underground,” I said.

“Cool. Can you see it?”

“No.”

“Oh.”

“They smash tiny particles together that create the building blocks of life. Those particles fit together like your Legos.”

“Cool. You can see those?”

“No. Not without a really expensive particle detector that works like a super microscope.”

“Oh….That’s really boring.”

I had run out of explanations and lost the interest battle–but not the war, I was soon to find out.

At the 21st incarnation of the Wonders of Science show, my son’s interest was piqued. He sat upright. Then he teetered on the edge of his seat, raising his hand high in the air to volunteer. By the end of the two-hour show, he was chanting “I love science” and planning what to tell his class on Monday.

Clad in colorful goggles, three high school teachers put on the same show at the Batavia laboratory that has appeared, in part, on television programs including Late Night with David Letterman.

The science teachers hooked my son, just like they hooked Letterman, with bangs, flashes, and noxious odors. His stimulus-loving radar fully awakened, they proceeded to educate him on cryogenics, superconductivity, and plasma beams.

The show included the rerequisite demonstrations on the basics of gravity and electricity, and even some shooting of toilet paper into the crowd. But the teachers focused most of the show on making the concepts behind particle physics accessible to elementary school-aged children, not a simple feat.

The teachers used easy-to-do and visually appealing classroom experiments to explain the concepts behind the world’s most powerful high-energy particle accelerator at Fermilab. A short explanation before each experiment told the children how the science concept and experiment tied into Fermilab’s daily work.

Exploding frozen racquetballs and bubbles of gassy air demonstrated the cryogenics that cool the magnets that focus particle beams. A magnetic cube levitating above a cooled magnet showed how superconductivity reduces the resistance on the particles’ paths. Graphite and a toothpick in a microwave showed the crowd the concepts behind focusing a beam of plasma particles. The ensuing smell and glowing microwave interior had my son uttering “Cool.”

The rest of the day he proudly told everyone we met that he knew people who worked at Fermilab.

Photos by Cindy Arnold

Tona Kunz

No Comments »

The hunt for rare materials (APS April 2008)

April 15, 2008 | 9:38 am

Before you build an experiment to find a rare particle, you need to find the rare material to make the detectors! The hunt for these materials is getting more challenging every year as the needs of science experiments, high-tech industries, and other disciplines turn what used to be everyday stuff into prized commodities.

I have been coming across a lot of tales at the APS conference about the difficulty of procuring the right materials for science experiments and have asked around on some of the topics. The common aspect to most of the searches for materials is the desire to obtain stuff that isn’t contaminated by or with some form of radiation. Combine that with the increasing demand by industry for many elements that were previously used primarily by science, and the entire market is changing, and causing scientists to get more creative about finding new supplies.

Xenon in demand

Some of the promising dark matter searches and neutrino experiments use noble gases as the detection medium. Dark matter experiments have had great success with xenon, but it is quite expensive, and now xenon is in huge demand from other places so the price has risen rapidly. It turns out that some semiconductor manufacturers have discovered that creating their chips in an atmosphere of xenon can be quite beneficial. The semiconductor industry is so big that it can suck up the world’s production of xenon pretty quickly, thereby inflating the prices. When a particle physics experiment needs 10kg, 100kg, perhaps a tonne of xenon, it can quickly get beyond the budget of science experiments.

Radioactive argon

So why not turn to a cheaper noble gas like argon? Argon is incredibly cheap. But argon from the atmosphere (the most plentiful supply) has a lot of argon-39, which is radioactive, due to the effects of cosmic rays, a big problem for experiments that rely on cutting down background sources of radiation so that they know any signals they are seeing come from the things they are looking for, like dark matter particles or neutrinos. Purifying argon to remove the radioactive isotope is extremely difficult and so it is expensive. Why not look for argon somewhere the cosmic rays don’t reach, like natural gas from underground, where it is also plentiful? Well, you can get argon there but it has been contaminated by radioactive elements in the Earth. So either way, you lose out. Argon is cheap and plentiful but it becomes as expensive as xenon when you have to purify it.

Searching for sunken lead

Even if you have a material that has low radioactivity, you still want to shield it from other external sources of radiation like cosmic rays, radon underground, or even the natural radioactivity of humans nearby, which is some cases can be enough to cause a measurable effect. Lead is a great shield for some forms of radiation but the lead from mines is contaminated with uranium and thorium. The contamination takes the form of lead-210. It has a half-life of 22 years so the radioactive component will die away but it takes time. Centuries-old lead, however, is perfect. But where to find it?

Some of the preferred options for purely lack-of-radioactivity reasons: ancient Roman ruins, sunken ships, and the lead from old stained-glass windows in churches. The lead in all of these is perfect to use, but it obviously incurs a significant cultural cost. Fortunately, some of the sunken ships contain ingots of Roman lead, so using it doesn’t cause any harm to anybody and cultural authorities in the past have given permission to use those ingots. The supply of this lead is limited so we can expect to see a second-hand trade in lead among scientific experiments as the found supply dwindles.

Demand for helium rising

Back to noble gases, helium is also in short supply. Despite being the second-most abundant element in the universe, there is not enough to go around to let kids inflate as many balloons as they want. Prices for balloon gas have spiked and many stores no longer stock it. The world can probably live without helium balloons but will they be prepared to say no more MRIs? When it comes to healthcare, people definitely want to have testing equipment available. MRIs have superconducting magnets inside them and they need to be cooled with liquid helium. The number of MRI machines and demand for their use is increasing, partly due to some ill-advised promotions by companies for full-body scans. Some physicists are looking at ways of creating MRI machines that don’t use liquid helium as the coolant for the magnets, so there is a promising way out of that bind.

Helium is used in many other places also, especially in the electronics industry. It is used to make flat-panel TVs and computer monitors, and in the production of computer chips and optical fibers. In total, demand for helium is up 80% in the past 20 years. Prices for helium have gone up 15-30% each year in recent years.

The list of materials in demand goes on; it seems that the resource struggle the whole world is facing has an impact on basic science research. Fortunately, the ingenuity of scientists generally finds a way around the problem, but this is one more challenge in the conduct of an experiment.

See all posts from the American Physical Society April 2008 conference here.

David Harris

4 Comments »

The Fermilab underground

April 15, 2008 | 4:32 am

Sometimes to find the biggest and best things, you have to dig deep — 360 feet, to be precise.

A television crew for The History Channel wanted to learn about modern-day atom smashing underground, so they traveled to Fermilab to see the world’s most intense neutrino accelerator beam. It takes a tunnel wider and taller, in some places, than a two-story home to house the beam, which helps physicists look for some of the smallest pieces of matter: neutrinos.

The television crew spent nearly two full days at Fermilab, which sits in the middle of a historic prairie in Illinois.

The resulting video clip, part of the Chicago episode of “Cities of the Underworld,” is about five minutes long.  It takes viewers into Fermilab’s NuMI tunnel, where a beam of neutrinos is aimed at a detector in the adjacent tunnel as part of the MINOS experiment. A second MINOS detector sits 450 miles away in a mine in Soudan, Minnesota. The show offers vivid graphics describing how neutrinos and other particles interact along the underground journey.

The journey begins underground at Fermilab, where an intense beam of protons hits a target and produces a mix of other particles. By the time these particles reach the Fermilab MINOS detector, a quarter mile or so away, only muons–heavy cousins of the electron–and muon neutrinos remain. The muons get absorbed by the rock on the way to the second detector in Soudan mine, leaving only muon neutrinos for it to catch.  

The underground game of catch helps physicists learn about the personality disorder of neutrinos: As they travel, neutrinos switch identities. On their journey from Fermilab to the Soudan mine, about a quarter of the muon neutrinos change into tau neutrinos, electron neutrinos, or perhaps an unknown type of particle that the MINOS detector doesn’t register. Examining this transformation could help explain one of the mysteries of the early universe — why matter came to dominate antimatter, allowing for the formation of planets, stars, and people.

The show schedule and information on purchasing individual episodes are here.

Tona Kunz

No Comments »

What can we expect from the LHC? (APS April 2008)

April 14, 2008 | 1:37 pm

In a press conference this morning, Abe Seiden of the University of California, Santa Cruz, showed a great timeline that plots the amount of data to be collected at the Large Hadron Collider against time, and then pointed out where physicists expect to make certain discoveries if nature has those discoveries waiting to be made. See the graphic below.

In summary, here are the potential milestones with my comments on each:

2009: Supersymmetry–if the appropriate energy scale is 1TeV

2009/2010: Higgs particle–if it is around 200 GeV in mass.

2010/2011: Higgs particle–if it is around 120 GeV in mass. (The lower energy is harder to see because at that energy, it would decay with the key signature involving photons. However, other decays also have similar photons so you need better statistics to tell the difference. A Higgs at higher energy would probably decay primarily into W bosons, with very obvious characteristic jets of particles coming out of the collision.)

2012: Extra dimensions of space–if the energy scale is 9 TeV

2012: Compositeness–if quarks are actually composite particles instead of being fundamental and that composite nature reveals itself on an energy scale of 40 TeV.

2017: Supersymmetry–if the appropriate energy scale is 3 TeV.

2019: Z‘–if there is a new type of force that comes into play around the 6 TeV energy scale. If it does, the particle that communicates the force is represented by the temporary name Z‘ in analogy with the Z that transmits the weak force.

This timeline is of course dependent on the LHC starting up according to the current plan. The director-general of CERN recently made a statement that said CERN plans to have the LHC cooled down by mid-June with first beam injection two months later. The world is waiting excitedly!

Timeline for possible LHC discoveries

See all posts from the American Physical Society April 2008 conference here.

David Harris

2 Comments »

The dime of a lifetime

April 14, 2008 | 4:23 am

A couple of weeks ago Jim Shultz of Fermilab’s Visual Media Services was following his usual routine. As Jim puts it, “It was a normal day like any other” including a stop at the cafeteria for his morning coffee.

“I was in line to pay and there was some small talk at the cashier’s station and as I was walking away, I glanced at the change before I put it in my pocket. One coin looked slightly dark. My initial thought was that I had gotten a Canadian coin in my change. Upon closer inspection, I recognized that the coin was a dime, and somewhat aged. But when I really looked at it, I realized that I had gotten a dime from 1892!”

“When I was younger, I used to collect coins, so I was vaguely familiar with the terms of numismatics and the condition of coins. For its age, this coin was in relatively good shape.”

Later that day Jim examined it a little closer. A quick Web search revealed that this was in fact an 1892 Barber Dime, minted in Philadelphia. It was the first year of issue for this particular design, so 12 million of them were minted. Consequently, many of them were saved, which is why this coin might have been available in circulation 116 years later. Read the rest of this entry »

Fred Ullrich

1 Comment »