Twirl yourself dizzy in a virtual LHC

August 15, 2008 | 5:00 am

Image by Peter McCready

Image by Peter McCready

As excitement builds toward the Large Hadron Collider start-up, things are doubtlessly getting a bit feverish at CERN. But you can stumble around the LHC machinery in the calm of your own home thanks to photographer Peter McCready, who has created stunning 360-degree images of the ALICE, ATLAS, and CMS detectors and posted them to his Web site. (We couldn’t get to the images through the Web site late yesterday–too much traffic?–but found the ALICE image here.)

According to International Science Grid This Week, McCready took 102 individual photos and stitched them together into one seamless spherical image. The controls take a bit of getting used to, but by clicking on an image and dragging your cursor, you can “turn” the camera to look in any direction you like.  Just be careful not to make yourself sick with all the twisting!

Kelen Tuttle

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On course for a convincing supernova

August 14, 2008 | 7:40 am

A still from a conventional supernova simulation depicts the rebounding shockwave (visible as the front between inwards-falling outer gases and outwards-blowing stellar materials). Lighter colors indicate regions of greater density. (Image courtesy of Tony Li)

A still from a conventional supernova simulation depicts the rebounding shockwave (visible as the front between inwards-falling outer gases and outwards-blowing stellar materials). Lighter colors indicate regions of greater density. (Image courtesy of Tony Li)

A cataclysmic explosion that lights up an entire galaxy is hard enough to fit in your mind’s eye, much less a computer.

As a summer research student in the SULI program at Stanford Linear Accelerator Center, Tony Li has learned that, despite 40 years of development, simulations of stars which are nearing the requisite conditions for a supernova have failed to undergo the critical transformation. A supernova is the intensely brilliant explosion of a dying star’s matter bursting through its own shock front. Working with astrophysicist Shizuka Akiyama, Li hopes to make progress in this direction with a model that, unlike previous ones, operates three-dimensionally and grapples with the effects of a very strong magnetic field on core collapse.

Extremely massive stars at the end of their lifetime undergo gravitational implosion when they’ve run out of fuel to burn. Deprived of the outward pressure formerly supplied by the fusion process, the star’s iron core begins to disassociate into subatomic particles in an effort to compress as much as possible. At some point, the star succumbs to a gravitational free-fall that involves the entire star, converting virtually all of its potential energy to outrushing neutrinos. Collapsing outer materials and plasma collide with the star’s core, transferring much energy to reactions inside the core, and the rest to a rebounding shockwave that, though dampened, begins to push against the star’s gaseous envelope.

Recent consensus has emerged that this is the true precipice of a supernova. Thermal pressure produced by the neutrinos is supposed to cook the stellar bubble until it explodes. But in current simulations of large stars, no explosion occurs, and the shockwave merely sits inside the shell.

Because scientists can’t create their own experiments with stars in a laboratory, astrophysicists rely heavily on computer models to study the respective contributions of parameters in a given physical system.
Equations representing the collected body of physical and astronomical knowledge form a code that, when fed with initial conditions, runs the system and produces profiles for components like temperature, density, and velocity of outwards-blowing stellar matter.

The computer program has limits, however. As Li says, “The catch with our code is that we don’t have every single detail of physics in it.” Supernova science is highly complex, pooling cosmic-scale physics of gravity with the particle level and calling for equations of state that no one understands for the extreme density and temperature conditions involved.

Only recently has computing power advanced to include 3-dimensional grids, a capacity crucial for simulating the inherently multidimensional effects of magnetic fields. Previously, scientists used 2-D models and were obliged to make assumptions about the symmetry of the core’s rotation.

Now that computing power has reached this stage, attention in the field is expanding beyond the conventional theory of neutrino heating and looking to other sources that could provide the missing energy.

Akiyama believes that a magnetic field effect within the neutron star could be factor that revives the retarding shockwave. Magnetic tension caused by differential rotation causes magnetic fluid inside the iron core to fluctuate chaotically, creating flashes of spectacular field strength where field lines are briefly closer. The leap in magnetic force in these areas would produce an added kick to the rebounding stellar plasma, because plasma has a magnetic component. Because the instability serves to dramatically amplify existing magnetic field strength, its addition to the theory means that a huge amount of energy could be created from initially weak fields.

Currently writing and modifying code for a 3-D simulation, Li aims to fulfill one step in the larger picture of Akiyama’s research. A battery of tests will narrow the models down to those most susceptible to the magnetic field effect. The future will see extensions of this program, and a better understanding of how a very powerful magnetic field contributes to not just supernovae, but even more energetic products of core collapse, such as gamma ray bursts and magnetars.

Zoë Macintosh

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New issue of symmetry available

August 13, 2008 | 11:16 am

symmetry magazine, August 2008

symmetry magazine, August 2008

The August 2008 issue of symmetry has just been posted online and print subscribers will be receiving their copies soon.

In this issue, read about the three-pronged approach to particle physics discoveries recently announced in a strategic planning document; ArgoNeuT, a liquid-argon-based detector looking for neutrinos; and the symmetry collection of physics-based license plates.

Look inside the newest generation of bubble chambers, and see the logbook page from the first discovery of the Z boson, 25 years ago.

David Harris

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LHC test successful

August 11, 2008 | 12:26 pm

A schematic showing the beam in the first two sectors of the LHC.

A schematic showing the beam in the first two sectors of the LHC.

CERN just released an update announcing that they successfully completed the first beam injection test. Read the update here.

Elizabeth Clements

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First protons injected into the LHC

August 8, 2008 | 4:52 pm

First protons in the Large Hadron Collider.

The Large Hadron Collider saw its first protons today, around 6:30 p.m. at CERN (12:30 p.m. US EDT), as scientists conducted the first beam injection test in one section of the collider. The protons traveled just a few meters into the LHC in a clockwise direction. The tests will continue through the weekend to transfer the beam from one section of the accelerator complex to another. A second beam injection test is scheduled for later in August. Protons will circulate around the entire collider for the first time on September 10.

Elizabeth Clements

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Most everything you wanted to know about, well, everything….

August 8, 2008 | 6:16 am

If you always wanted to know more about science but don’t have time to go back to school or visit your neighborhood laboratory, Fermilab has an online library made just for you.

Since 2000, the high-energy particle physics laboratory in Batavia, Illinois, has recorded lectures for public consumption. The lectures all touch on science in some way be it recent research results, commentary from experts and academics in scientific or technology-related fields, or tales from those who cover science for the media.

Many topics involve particle physics, but many also cover weather phenomena, medical research, information technology advances, cosmology, and climatology. Just about every topic that incorporates research has been touched on in the 301 recorded talks, which each last about an hour.

“The Mechanisms of Nicotine Addiction” and “The Global Coral Reef Crisis” show up among lists of physics talks about the Large Hadron Collider, the Tevatron, and Gamma Rays.

So sit down, grab a cup of coffee and expand your mind.

Watch the talks here

Tona Kunz

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CERN first beam due September 10, 2008

August 7, 2008 | 10:07 am

CERN officially announced today that the first attempt to circulate a beam through the Large Hadron Collider will be made on September 10, 2008.

Read the press release.

David Harris

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Amateur finds new cosmic object

August 7, 2008 | 6:06 am

Hanny's Object

Hanny's Object

A Dutch schoolteacher with no previous interest in science has identified a new type of cosmic object, reports the BBC. The object is a green blob of gas that was once powered by a quasar now gone dim. Professional astronomers confirm that object is one of a kind.

In the last issue of symmetry, the cover story talked about contributions amateurs could make to science. Astronomical discoveries rate as one of the most common types of outsider contributions and this definitely fits the pattern.

The teacher, Hanny Van Arkel, said she had no previous interest in astronomy so the path she followed to get involved in this project is an interesting and instructive one. Van Arkel had an interest in music and, so, when Queen guitarist Brian May co-authored a popular astronomy book Bang! The Complete History of the Universe, she read it and her curiosity grew. That led to her joining the Galaxy Zoo project, through which she identified the mysterious green object which is being referred to as “Hanny’s Voorwerp.” (Voorwerp means object in Dutch.)

Interest in science can come through many paths, and a growing number of people in science outreach now recognize that they can have a lot of influence on people’s engagement in science through seemingly tangential means. The great part of this story is how that serendipitous interest in astronomy for one person led to a significant contribution to science.

David Harris

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Particle physics is a dirty, dirty job

August 6, 2008 | 6:19 am

Inside the Super-K detector

A new genre of television extols the virtues of those willing to get dirty and sweaty for a living.  Dirty Jobs, Ice-Road Truckers and Ax Men highlight workers who face danger, rather than paperwork deadlines, to get a pay check.

These shows tout the working class as tougher than its white-collar counterpart.

Maybe those producers haven’t met experimental physicists yet. Especially Mark Vagins.

As a US lead scientist working on Super-K, or Super Kamiokande, a neutrino observatory in Japan, Vagins works in conditions that at times can rival any reality TV obstacle.

His underground laboratory, sits 3300 feet underground within an old zinc mine housed in a mountain 200 km from Tokyo. Traffic jams give way to rocky terrain and freezing winds for the morning commute. While angry fellow motorists are absent, bears and snow monkeys whose eyes follow their every move confront the scientists on their way into the mountain.

“They just stare,” Vagins says. “It is really creepy.”

Bells tied to clothing to deter predators became the norm after a black bear chased Vagins’ coworker, who was walking from the main above-ground laboratory to the cave entrance. The bear encounters have stopped, for now.

Using the Earth as a filter

The Super-K tank half-filled with water

Vagins, a University of California -Irvine, scientist with a joint appointment at the University of Tokyo, and about 120 other researchers from several countries run the gauntlet to the underground laboratory because it’s one of the few ways to study the mysterious, subatomic particle, the neutrino. These elusive particles are produced in nuclear reactions occurring in the sun, supernovae, and cosmic rays that shower the Earth.

Neutrinos could hold the key to explaining why particles cling together to form matter, including planets and people, rather than remain as they were just after the Big Bang 13.7 billion years ago–clouds of free-floating energy and light.

Neutrinos move at nearly the speed of light, passing through most matter unnoticed. Trillions pass through your body each second. Because they are essentially invisible and rarely interact with matter, scientists must build giant detectors to increase the probability of seeing a signal of a neutrino. Rock and dirt layers covering the detectors ease this task by absorbing the particles that are not neutrinos but that create a static-like signal in the underground detector. By using the earth to filter out these “background” particles, scientists can get a clearer signal of the neutrino’s passage through the detector to study.

To get to the Super-K detector, Vagins rides 16,404 feet in a mine car to a lift reminiscent of a window washer cart that drops him another 128 feet.

And he’s inside.

“I like to think of it as a big cathedral,” Vagins says. “The inside is like a giant silent chamber. When you stand at the bottom and you look up, you have to shout at the absolute top of your voice to be heard at the top of the tank. The space inside the detector tends to swallow up all the sound.”

A 14-story tall tank holding 50,000 tons of ultra-pure water is covered on the inside with 11,146 television-sized photomultiplier tubes that record flashes of light given off when a neutrino passes through the water exciting other particles with its wake. The other particles give off light. These flashes are collected by detectors, which translate the light into computer data to paint a picture of the energy, direction, and type of neutrino incident.

“Every so often we have to go in there and replace the photomultiplier tubes that have failed,” Vagins says.

That’s when the job gets even tougher.

Getting wet for science

Mark Vagins performs maintenance by boat in the Super-K tank

Since the detector started taking data in 1996, scientists have had to drain it three times for maintenance. More maintenance could occur as soon as summer 2009, though likely a couple years later. Typical cleaning takes two months. An infamous malfunction that shattered 7000 tubes and left 250,000 pounds of glass in the water took close to a year to repair.

Jumping in row boats, scientists hand clean each tube as the water rises. They try not to contaminate the water by touching it, but mishaps do occur.

“Once when we bought some cheaper boats in town, it got half way around the detector before it began to sink,” Vagins says. “Also, one of our Japanese colleagues fell into the water after losing his balance while working on and jumping among large floating pieces of foam.”

Dropped equipment such as flashlights require scuba divers to swim the 120 feet to the bottom of the detector where they risk decompression sickness.

Cleaning the photomultiplier tubes in the Super-K tank

While the cleaning can get monotonous, the view makes it worthwhile.

“Just being in the tank is kind of a kick,” Vagins says. “When you are in the center of the detector in the boat or hanging in the air in the gondola lift, all of these hand-blown glass tubes kind of twinkle in the half light in a different way.”

by Jennifer L. Johnson

Photos courtesy of Mark Vargins and the Super-K collaboration.

Guest author

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Preparing the next generation of neutrino physicists

August 5, 2008 | 6:42 am

Georgia Karagiorgi and Matt Toups want to build a giant, super-intense laser with a 100-kilometer beamline to detect “relic neutrinos” from 14 billion years ago. This cosmic neutrino spectrometer could some day explain how the universe evolved two or thee seconds after the big bang.

Such big ideas are exactly they type of innovative, enthusiastic thinking Fermilab scientists want to stir in upcoming researchers.

The pair of Columbia University students received a first place award at the User’s Meeting in June for their unique proposal in a neutrino experimental challenge held at Fermilab last year during a 10-day Neutrino Physics Summer School.

“It was so much fun,” Karagiorgi says. “And, it was just in the spirit of the school. Matt and I took what we learned in the lectures and applied it to our projects.”

The contest was one of the many activities designed to get students thinking about future experiments for neutrinos, a growing focus of research, particularly in the United States. Students were discouraged from letting today’s resource constraints limit their ideas.

“We have so many questions. What caused matter to dominate antimatter? Neutrinos are fundamental constituents of the universe. They pass through our bodies at the rate of trillions per second. We should probably know a little more about them,” says Gina Ramieka, the school’s co-director and head of Fermilab’s neutrino department.

The biannual school, one of few in existence, offers college students the opportunity to discuss and hear lectures from leading neutrino physicists. Fermilab’s school incorporates neutrino research conducted in the sky, underground, in reactors, and with accelerators.

“There is a danger in getting too narrow in this subject, so we wanted to keep everything very broad,” Ramieka says. “You can’t do all of particle physics in a single experiment. There are many tools you have to use to get to the fundamentals.”

By Jennifer L. Johnson

Guest author

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