Particle 'mousetrap' could help answer gnawing cosmic questions

Apr 29, 2010
A reverse-cyclotron will help trap high-speed particles in a plasma soup. Credit: Michigan State University

Capturing fleeting bits of matter to reveal the nature of the universe is a little like trying to trap incredibly tiny, impossibly speedy mice alive.

A better mousetrap could be at hand, promising new insights that could bring researchers out of the woodwork to conduct cutting-edge experiments at Michigan State University's National Superconducting Cyclotron Laboratory.

Michigan State scientists landed a $3.28 million federal grant to develop an electromagnetic trap to snag and quickly extract rare isotope ricochets from high-speed they create.

"The products we make live for much less than one second before they decay into something else, so speed is very important," explained David Morrissey, a University Distinguished Professor of chemistry and the project's principal investigator.

Rare isotopes are the unstable versions of the found here on earth, but have too much or too little mass. Such atoms must be produced in nuclear reactions and are ionized, or electrically charged, losing some electrons that orbit the nucleus.

Stable atoms are flung together at about one-third of the by huge electromagnetic accelerators at MSU, creating rare isotopes that otherwise are only produced in stars. Based on a prototype and detailed calculations from Morrissey and his collaborators, a helium soup within a new cyclotron "decelerator" should be able to slow down and trap the speeding bits like marbles circling a bowl, slowing and separating them from the hot, gaseous whirlpool.

This is a diagram of the proposed particle stopper reverse-cyclotron. Credit: National Superconducting Cyclotron Laboratory, Michigan State University

"We're going to provide these small ions that have never been studied before to experimenters," he said. "It will be basic research, training students and developing new technology." It also will lay useful groundwork for the half-billion dollar Facility for Rare Isotope Beams, planned for construction at MSU in the next several years.

"A large fraction of the experimental program in the future will depend on our success," Morrissey added. "We have a number of scientists here and around the country and even the world who want to come here to use the new facility," thus helping secure the future of a physics program that already leads the world in analysis of such fast projectile fragments.

Much of the MSU program focuses on mimicking the violent stellar conditions following the Big Bang, which is thought to have kick-started the universe 14 billion years ago. The engine of our own solar system, the Sun, merely fuses hydrogen atoms together to produce helium and energy. So, scientists wonder, where did the rest of the stuff here come from - the copper, the carbon, the cheese nibbled by mice?

This is Michigan State University chemistry professor David Morrissey. Credit: G.L. Kohuth, Michigan State University

"There are chemical elements on earth that couldn't have been made in the Sun, so they had to be made somewhere else and yet end up here," Morrissey said. The best guess, he added, is that they were formed from different kinds of stars. But because many such elemental precursors lived for only an instant, scientists must muster huge physical forces to deconstruct today's elements to figure out how they were made.

Michigan State's funding agreement with the National Science Foundation, which made the three-year grant, calls for the university to contribute $1.4 million, primarily in the form of expert manpower. The NSF funds are part of the $15 billion scientific research component of the American Recovery and Reinvestment Act, known as the federal economic stimulus program. Compensation for participants - faculty, scientific staff and engineers, postdoctoral researchers, graduate and undergraduate students - will account for $1.38 million, and permanent equipment for $1.13 million of projected expenses.

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croghan27
not rated yet Apr 29, 2010
Is this not what CERN is doing, only more so?
KenK54
5 / 5 (1) Apr 30, 2010
No. Though both facilities are accelerators, they accelerate different particles to study different forces and structures.

CERN accelerates two beams of protons and smashes them together in order to study what they are made out of (quarks, gluons, etc.) and the forces holding them together.

NSCL/FRIB accelerates one beam of entire nuclei and collides them with a stationary target in order to study the structure and forces at work inside of a nucleus.

In short, one studies the guts of a nucleus and the other studies the guts of single particles.
croghan27
not rated yet Apr 30, 2010
Thanks Kenk ... I guess my mind is still locked in a 1950s 'atom smasher' mode. You explained what is going on there quite lucidly. (I understood you better than I understood the article)

My 'only more so' was that vague that I can see someone could be mislead.

Is there no other way to study the internals of these particles (be they protons like LHC or entire nuclei like NSCL/FRIB)?

It seems to me to be like studying the detritus of an explosion to see how a bomb works.

As well, I thought that it was agreed that the heavier elements had to be generated in the bowels of larger and hotter stars than our sun.
KenK54
5 / 5 (1) May 05, 2010
Actually, NSCL has been around since 1963 and accelerating nuclei since 1981, but you hear about the big 'atom smashers' more because its much 'sexier' science.

Anyways, no there is no other way to physically study the inside of an atom. Even the best electron microscopes don't actually 'see' atoms, and the nucleus of an atom is 10,000 times smaller than its electron shells. And how do mechanical engineers learn how a new product works or a 10-year-old boy learn how a toy train works? They take them apart and put them back together. Similarly, accelerators take atomic structures apart and scientists put them back together.

And yes, it is widely agreed that heavier elements are generated in stars in two ways; s-process and r-process, only the latter creates the heaviest elements; in supernovae and colliding neutron stars. And that's just a widely-accepted theory since they don't know how the process works and can't examine it directly, thus the experiments.

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