Expert Voices

Powerful linear accelerator begins smashing atoms – 2 scientists on the team explain how it could reveal rare forms of matter

A new particle accelerator at Michigan State University is set to discover thousands of never-before-seen isotopes. (Image credit: Facility for Rare Isotope Beams, CC BY-ND)

This article was originally published at The Conversation (opens in new tab). The publication contributed the article to Space.com's Expert Voices: Op-Ed & Insights.

Sean Liddick (opens in new tab), Associate Professor of Chemistry, Michigan State University

Artemis Spyrou (opens in new tab), Professor of Nuclear Physics, Michigan State University

Just a few hundred feet from where we are sitting is a large metal chamber devoid of air and draped with the wires needed to control the instruments inside. A beam of particles passes through the interior of the chamber silently at around half the speed of light until it smashes into a solid piece of material, resulting in a burst of rare isotopes.

This is all taking place in the Facility for Rare Isotope Beams (opens in new tab), or FRIB, which is operated by Michigan State University for the U.S. Department of Energy Office of Science. Starting in May 2022, national and international teams of scientists converged at Michigan State University and began running scientific experiments at FRIB with the goal of creating, isolating and studying new isotopes. The experiments promised to provide new insights into the fundamental nature of the universe.

Related: Our expanding universe: Age, history & other facts

We are two professors in nuclear chemistry and nuclear physics who study rare isotopes. Isotopes are, in a sense, different flavors of an element with the same number of protons in their nucleus but different numbers of neutrons.

The accelerator at FRIB started working at low power, but when it finishes ramping up to full strength, it will be the most powerful heavy-ion accelerator on Earth. By accelerating heavy ions – electrically charged atoms of elements – FRIB will allow scientists like us to create and study thousands of never-before-seen isotopes. A community of roughly 1,600 nuclear scientists from all over the world (opens in new tab) has been waiting for a decade to begin doing science enabled by the new particle accelerator.

The first experiments at FRIB (opens in new tab) were completed over the summer of 2022. Even though the facility is currently running at only a fraction of its full power, multiple scientific collaborations working at FRIB have already produced and detected about 100 rare isotopes (opens in new tab). These early results are helping researchers learn about some of the rarest physics in the universe.

What is a rare isotope?

It takes incredibly high amounts of energy to produce most isotopes. In nature, heavy rare isotopes are produced during the cataclysmic deaths of massive stars called supernovas or during the merging of two neutron stars.

To the naked eye, two isotopes of any element look and behave the same way – all isotopes of the element mercury would look just like the liquid metal used in old thermometers. However, because the nuclei of isotopes of the same element have different numbers of neutrons, they differ in how long they live, what type of radioactivity they emit and in many other ways.

For example, some isotopes are stable and do not decay or emit radiation, so they are common in the universe. Other isotopes of the very same element can be radioactive so they inevitably decay away as they turn into other elements. Since radioactive isotopes disappear over time, they are relatively rarer.

Not all decay happens at the same rate though. Some radioactive elements – like potassium-40 – emit particles through decay at such a low rate that a small amount of the isotope can last for billions of years (opens in new tab). Other, more highly radioactive isotopes like magnesium-38 exist for only a fraction of a second before decaying away into other elements. Short-lived isotopes, by definition, do not survive long and are rare in the universe. So if you want to study them, you have to make them yourself.

The Facility for Rare Isotope Beams was designed to allow researchers to create rare isotopes and measure them before they decay. (Image credit: Facility for Rare Isotope Beams, CC BY-ND)

Creating isotopes in a lab

While only about 250 isotopes naturally occur on Earth (opens in new tab), theoretical models predict that about 7,000 isotopes should exist in nature (opens in new tab). Scientists have used particle accelerators to produce around 3,000 of these rare isotopes (opens in new tab).

The green-colored chambers use electromagnetic waves to accelerate charged ions to nearly half the speed of light. (Image credit: Facility for Rare Isotope Beams, CC BY-ND)

The FRIB accelerator is 1,600 feet long and made of three segments folded in roughly the shape of a paperclip. Within these segments are numerous, extremely cold vacuum chambers that alternatively pull and push the ions using powerful electromagnetic pulses. FRIB can accelerate any naturally occurring isotope – whether it is as light as oxygen or as heavy as uranium – to approximately half the speed of light (opens in new tab).

To create radioactive isotopes, you only need to smash this beam of ions into a solid target like a piece of beryllium metal or a rotating disk of carbon.

There are many different instruments designed to measure specific attributes of the particles created during experiments at FRIB – like this instrument called FDSi, which is built to measure charged particles, neutrons and photons. (Image credit: Facility for Rare Isotope Beams, CC BY-ND)

The impact of the ion beam on the fragmentation target breaks the nucleus of the stable isotope apart (opens in new tab) and produces many hundreds of rare isotopes simultaneously. To isolate the interesting or new isotopes from the rest, a separator sits between the target and the sensors. Particles with the right momentum and electrical charge will be passed through the separator while the rest are absorbed. Only a subset of the desired isotopes will reach the many instruments (opens in new tab) built to observe the nature of the particles.

The probability of creating any specific isotope during a single collision can be very small. The odds of creating some of the rarer exotic isotopes can be on the order of 1 in a quadrillion (opens in new tab) – roughly the same odds as winning back-to-back Mega Millions jackpots. But the powerful beams of ions used by FRIB contain so many ions and produce so many collisions in a single experiment that the team can reasonably expect to find even the rarest of isotopes (opens in new tab). According to calculations, FRIB's accelerator should be able to produce approximately 80% of all theorized isotopes (opens in new tab).

The first two FRIB scientific experiments

A multi-institution team led by researchers at Lawrence Berkeley National Laboratory, Oak Ridge National Laboratory (ORNL), University of Tennessee, Knoxville (UTK), Mississippi State University and Florida State University, together with researchers at MSU, began running the first experiment at FRIB on May 9, 2022. The group directed a beam of calcium-48 – a calcium nucleus with 28 neutrons instead of the usual 20 – into a beryllium target at 1 kW of power. Even at one quarter of a percent of the facility’s 400-kW maximum power, approximately 40 different isotopes passed through the separator to the instruments (opens in new tab).

The FDSi device recorded the time each ion arrived, what isotope it was and when it decayed away. Using this information, the collaboration deduced the half-lives of the isotopes; the team has already reported on five previously unknown half-lives (opens in new tab).

The second FRIB experiment began on June 15, 2022, led by a collaboration of researchers from Lawrence Livermore National Laboratory, ORNL, UTK and MSU. The facility accelerated a beam of selenium-82 and used it to produce rare isotopes of the elements scandium, calcium and potassium. These isotopes are commonly found in neutron stars, and the goal of the experiment was to better understand what type of radioactivity these isotopes emit as they decay. Understanding this process could shed light on how neutron stars lose energy (opens in new tab).

The first two FRIB experiments were just the tip of the iceberg of this new facility’s capabilities. Over the coming years, FRIB is set to explore four big questions in nuclear physics: First, what are the properties of atomic nuclei with a large difference between the numbers of protons and neutrons? Second, how are elements formed in the cosmos? Third, do physicists understand the fundamental symmetries of the universe, like why there is more matter than antimatter in the universe? Finally, how can the information from rare isotopes be applied in medicine, industry and national security?

This story was updated to correctly represent the number of neutrons in the nucleus of calcium-48.

This article is republished from The Conversation (opens in new tab) under a Creative Commons license. Read the original article (opens in new tab).

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Sean Liddick
Associate Professor of Chemistry, Michigan State University

I am an experimental nuclear chemist interested in studying the basic properties of the atomic nucleus and the how elements are made in stellar explosions. I perform experiments at various facilities including the Facility for Rare Isotope Beams (FRIB) and focus on the study of the decay of short-lived rare isotopes. I am an Associate Professor of Chemistry and I also currently serve as the Associate Director of Experimental Science at FRIB.

  • allanrbrewer
    "scandium, calcium and potassium. These isotopes are commonly found in neutron stars..."
    Could you explain that quote a bit please - I thought that neutron stars were essentially one big nucleus?
    Reply
  • allanrbrewer
    "smash this beam of ions into a ...rotating disk of carbon."
    Why is the carbon rotating - what is the function of this?
    Reply
  • billslugg
    From Wiki:
    "Current models indicate that matter at the surface of a neutron star is composed of ordinary atomic nuclei crushed into a solid lattice with a sea of electrons flowing through the gaps between them."

    The target rotates so that no one spot gets all the energy. This would make it melt.
    Reply
  • allanrbrewer
    Thanks.
    re the targets - Carbon's melting point is higher than Beryllium so presumably the Be target would have to rotate also?
    Reply
  • billslugg
    allanrbrewer said:
    Thanks.
    re the targets - Carbon's melting point is higher than Beryllium so presumably the Be target would have to rotate also?
    Probably all linear collider targets rotate. Many X-ray tubes have rotating targets as well.
    Reply