I worked on TRIUMF’s Five-Year Plan (2020-2025) last year, so Astroengine is featuring a few physicsy articles that were included in the document to tell the center’s story
Last year, I had the honor to help write TRIUMF’s Five-Year Plan for 2020-2025. TRIUMF is Canada’s particle accelerator center, located next to the University of British Columbia’s campus in Vancouver, and it tackles some of the biggest problems facing physics today.
Every five years, research facilities in Canada prepare comprehensive documents outlining their strategies for the next five. In this case, TRIUMF asked me to join their writer team and I was specifically tasked with collaborating with TRIUMF’s management to develop and write the Implementation Plan (PDF) — basically an expanded version of the Strategic Plan (PDF) — detailing the key initiatives the center will carry out between 2020 and 2025.
As the location of the world’s largest and oldest operational cyclotron, the center is a multi-faceted physics lab with hundreds of scientists and engineers working on everything from understanding the origins of matter to developing radiopharmaceuticals to treat late-stage cancers. I only had a vague understanding about the scope of TRIUMF’s work before last year, but, as the months progressed after visiting the center in April 2018, I was treated to an unparalleled learning experience that was as dizzying as it was rewarding.
As a science communicator, I wanted to understand what makes TRIUMF “tick,” so I decided to speak to as many TRIUMF scientists, engineers, collaborators, and managers as possible. During my interviews, I was excited and humbled to hear stories of science breakthroughs, personal achievements and mind-bending physics concepts, so I included a series of miniature articles to complement the Implementation Plan’s text. As the Five-Year Plan is a public document (you can download the whole Plan here, in English and French), I’ve been given permission by TRIUMF to re-publish these articles on Astroengine.
“Beyond Multimessenger Astronomy”
Background: To kick off the series, we’ll begin with nuclear science. Specifically, how astrophysical processes create heavy elements and how TRIUMF studies the formation of radioisotopes in the wake of neutron star collisions.
After the 2017 LIGO detection of gravitational waves caused by the collision of two neutron stars (get the details here), and the near-simultaneous detection of a gamma-ray burst from the same location, scientists heralded a new era for astronomy — nicknamed “multimessenger astronomy,” where gravitational wave and electromagnetic signals measured at the same time from the same event can create a new understanding of astrophysical processes. In this case, as it was confirmed to be a neutron star merger — an event that is theorized to generate r-process elements — spectroscopic analysis of the GRB’s afterglow confirmed that, yes, neutron star collisions do indeed create the neutron-rich breeding ground for heavy elements (like gold and platinum). Although multimessenger astronomy may be a new thing, TRIUMF has been testing these theories in the laboratory environment for years, using rare isotope beams colliding into targets that mimic the nuclear processes that produce the heavy elements in our universe. This process is known as nucleogenesis, and it’s how our cosmos forges the elements that underpin stardust, the stuff that makes the planets, stars, and the building blocks of life.
For this mini-article, I had a fascinating chat with Dr. Iris Dillmann, a nuclear physics research scientist at TRIUMF. I’ve lightly edited the text for context and clarity. The original article can be found on page 22 of the Implementation Plan (PDF).
The article: TRIUMF’s investigations into neutron-rich isotopes were well-established before the advent of multi-messenger astronomy. “It was a cherry on top of the cake to get this confirmation, but the experimental program was already going on,” said Dillmann.
“What we do is multi-messenger nuclear physics; we are not looking directly into stars. TRIUMF is doing experiments here on Earth.”
Whereas the combination of gravitational waves and electromagnetic radiation from astrophysical events gives rise to a new era of multi-messenger astronomy, TRIUMF’s Isotope Separator and Accelerator (ISAC) facilitates the investigation of heavy isotopes through an array of nuclear physics experiments all under one roof that can illuminate the characteristics of isotopes that have been identified in neutron star mergers.
“For example, astronomers can identify one interesting isotope and realize that they need more experimental information on that one isotope,” she said. “We then have the capability to go through the different setups and, say, measure the mass of the isotope with the TRIUMF Ion Trap for Atomic and Nuclear Science (TITAN) experiment’s Penning trap.”
From there, Dillmann added, the Gamma-Ray Infrastructure For Fundamental Investigations of Nuclei (GRIFFIN) experiment can use decay spectroscopy to investigate the half-lives of rare isotope beams and their underlying nuclear structure. Other nuclear properties such as moments and charge radii can be measured using laser spectroscopy. TRIUMF scientists can also directly measure the reaction cross-sections of explosive hydrogen and helium burning in star explosions with the Detector of Recoils And Gammas Of Nuclear reactions experiment (DRAGON) and the TRIUMF UK Detector Array (TUDA).
With ISAC, all these measurements are carried out in one place, where teams from each experiment work side by side to solve problems quickly and collaborate effectively. “We have the setups in the hall to investigate an isotope from different perspectives to try to get a complete picture just from one department — the nuclear physics department,” said Dillmann.
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