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Discovery
Nuclear Scientists Explore the Core of Existence

A journalist at the National Superconducting Cyclotron Laboratory describes physicists' experiments to understand the neutron dripline and some surprising results

Photo of Matt Johnson, NSCL staff engineer, inspecting a 45-degree dipole magnet

Staff engineer Matt Johnson inspects a 45-degree dipole magnet.
Credit and Larger Version

March 24, 2008

The strong nuclear force is the strongest of the four fundamental forces of nature, binding protons and neutrons in the cores of atoms. Yet, the same force prevents those fundamental particles from combining in certain combinations.

When I first learned that, my entire view of the physical world was shaken. It was like learning that only certain mixes of peanut butter and jelly could be put into a sandwich.

As a journalist at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University, one of the nation's top nuclear science laboratories, the strangeness of this truth provided my first glimpse into the peculiar nature of matter at the subatomic level.

Full of Uncertainties

Scientists' knowledge of the strong nuclear force is full of uncertainties. To learn more, physicists are going to the extremes of nuclear existence in pursuit of understanding the "neutron dripline." The term refers to a boundary on a graph plotting the number of neutrons in a nucleus against the number of protons. In other words, it reflects the limit for how many neutrons can be piled into a single nucleus before the particles begin to bounce off. The neutron dripline has preoccupied nuclear physicists for the past half century, and for many of them, the issue is about more than understanding the nuclear force.

"We want to explore things as far away from what we know as possible," said Alex Brown, a professor of physics at NSCL. "This is testing new aspects of our models that we are not able to see in any other way. What are the constituents of our world? How many nuclei exist? And how are they formed in the process of the evolution of the universe? All of that depends on where the dripline is."

Brown and his colleagues discovered three nuclei near the dripline that had never been observed before: magnesium-40 with 12 protons and 28 neutrons; aluminum-42 with 13 protons and 29 neutrons; and aluminum-43 with 13 protons and 30 neutrons.

Magnesium-40 was the goal of the experiment, and the elusive isotope was a hot find--scientists had pursued it for more than 20 years without success. But most surprising were the two other nuclei--aluminum-42 and aluminum-43--that physicists thought should not have existed at all.

"The implication is that our models still have a long way to go," said Brad Sherrill, university distinguished professor of physics at Michigan State University. "Surprises eventually lead to a deeper understanding of the science," Sherrill said. "But at the moment, it's just a surprise."

The research team's findings were published in the Oct. 25, 2007, issue of the journal Nature.

One-hundred eighteen elements have been observed in the universe, but the neutron dripline has been found for only the first eight.

"You would think, 'if it's so interesting to explore the dripline, why hasn't it been done yet?'" asked Thomas Baumann, a beam physicist at NSCL and lead researcher on the magnesium and aluminum study.

So Baumann and his colleagues started a search at NSCL.

Half of Light-speed

In an experiment that ran in 2007, the cyclotron accelerated a beam of calcium nuclei to nearly half the speed of light--fast enough to circle the Earth three times in one second. The nuclei collide into a tungsten target, producing a thick smattering of various nuclei and other particles. Only one out of billions--sometimes trillions or quadrillions--of the resultant nuclei is the one that researchers seek. Producing the desired nucleus by knocking out an exact number of protons, and while leaving the neutrons untouched, is akin to throwing a chocolate chip cookie at the wall and knocking out only chocolate chips.

A complex system of magnets downstream filters out the desired particles, and over 11 days, three particles of magnesium-40 were detected, a proportion comparable to finding three particles of sand in all the beaches of western North America.

"Everything has to work perfectly," said Kirby Kemper, a collaborator from Florida State University. "It's the golden amount, when everything you've worked for comes together and works--that's what you live for as a scientist."

The findings showed physicists that the neutron dripline is not as well understood as they thought, and to better define it, they must venture into rarer nuclei.

For every nucleus closer to the dripline, Sherrill estimates that experimentally producing it would be 100 to 1,000 times harder, requiring more powerful equipment or taking much more time.

"We made magnesium-40 in 11 days. Making magnesium-42 (with current technology) would take 1,100 days. That's three years of running. It's kind of impossible," Sherrill said. As a more realistic alternative, physicists stress the need to continue to develop new technology. "One hundred years from now, when people are a lot smarter, this will all be really easy," Sherill added. And so the pursuit proceeds.

A video featuring the researchers talking about the recent discovery is available here.

-- Annie Jia, National Superconducting Cyclotron Laboratory, Michigan State University nscl.anniejia@gmail.com

This Behind the Scenes article was provided to LiveScience in partnership with the National Science Foundation.

Investigators
Thomas Baumann
Alex Brown
Kirby Kemper
Brad Sherrill

Related Institutions/Organizations
Michigan State University

Locations
Michigan

Related Awards
#0606007 Operation of the National Superconducting Cyclotron Laboratory at Michigan State University as a National User Facility & Support for its Research Program

Total Grants
$28,250,006

Related Websites
LiveScience.com: Behind the Scenes: Nuclear Scientists Explore the Core of Existence: /news/longurl.cfm?id=72
The Greatest Mysteries in Science: /news/longurl.cfm?id=38
Greatest Mysteries: How Did the Universe Begin?: /news/longurl.cfm?id=39

Picture from the NSCL experimenters' logbook used to create three super-heavy isotopes.
A picture from the logbook used by the NSCL experimenters who created three super-heavy isotopes.
Credit and Larger Version

Photo showing a closeup of the exposed guts of the NSCL K500 cyclotron
Closeup of the exposed guts of the NSCL K500 cyclotron.
Credit and Larger Version



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