Article features FRIB, North Carolina State University research collaboration

27 November 2023

North Carolina State University (NC State) published an article (“Understanding Charged Particles Helps Physicists Simulate Element Creation in Stars”) that discusses a new Physical Review Letters publication (“Charged-particle bound states in periodic boxes”). Hang Yu, graduate student at NC State; Sebastian König, assistant professor of physics at NC State and FRIB Theory Alliance bridge faculty member; and Dean Lee, professor of physics at FRIB and in Michigan State University’s Department of Physics and Astronomy and head of the Theoretical Nuclear Science department at FRIB, are the authors of the publication.

There are several useful applications of this work to the FRIB science program, explained Lee. Nuclear binding energies can now be more accurately predicted from ab initio lattice simulations using high-fidelity nuclear interactions. These calculations use finite volume boxes and must be extrapolated to infinite box size. This work derives the expected volume dependence. How the binding energy changes with box size also gives important information about the “tail” of the nuclear state when the constituent parts are well separated. The tail of the nuclear state plays an important role in low-energy astrophysical reactions such as the capture of protons and alpha particles. It is also probed in reactions involving nuclei that are weakly bound and in peripheral nuclear collisions where most of the nucleus is left intact.

The full article is reprinted below.

Understanding Charged Particles Helps Physicists Simulate Element Creation in Stars

By Tracey Peake, North Carolina State University

New research from North Carolina State University and Michigan State University opens a new avenue for modeling low-energy nuclear reactions, which are key to the formation of elements within stars. The research lays the groundwork for calculating how nucleons interact when the particles are electrically charged.

Predicting the ways that atomic nuclei – clusters of protons and neutrons, together referred to as nucleons – combine to form larger compound nuclei is an important step toward understanding how elements are formed within stars.

Since the relevant nuclear interactions are very difficult to measure experimentally, physicists use numerical lattices to simulate these systems. The finite lattice used in such numerical simulations essentially acts as an imaginary box around a group of nucleons that enables physicists to calculate the properties of a nucleus formed out of these particles.

But such simulations have so far lacked a way to predict properties that govern low-energy reactions involving charged clusters arising from multiple protons. This is important because these low-energy reactions are vital to element formation in stars, among other things.

“While the ‘strong nuclear force’ binds protons and neutrons together in atomic nuclei, the electromagnetic repulsion between protons plays an important role in the nucleus’ overall structure and dynamics,” says Sebastian König, assistant professor of physics at NC State and corresponding author of the research.

“This force is particularly strong at the lowest energies, where many important processes take place that synthesize the elements that make up the world we know,” König says. But it is challenging for theory to predict these interactions.”

So König and colleagues decided to work backward. Their approach looks at the end result of the reactions within a lattice – the compound nuclei – and then backtracks to discover the properties and energies involved in the reaction.

“We aren’t calculating the reactions themselves; rather, we’re looking at the structure of the end product,” König says. “As we change the size of the ‘box,’ the simulations and results will also change. From this information we can actually extract parameters that determine what happens when these charged particles interact.”

“The derivation of the formula was unexpectedly challenging,” adds Hang Yu, graduate student at NC State and first author of the work, “but the final result is quite beautiful and has important applications.”

From this information the team developed a formula and tested it against benchmark calculations, which are evaluations done via traditional methods, to ensure the results were accurate and ready to be used in future applications.

“This is the background work that tells us how to analyze a simulation in order to extract the data we need to improve predictions for nuclear reactions,” König says. “The cosmos is enormous, but to understand it you have to look at its tiniest components. That’s what we’re doing here – focusing on the small details to better inform our analysis of the bigger picture.”

The work appears in Physical Review Letters and was supported by the National Science Foundation and by the U.S. Department of Energy. NC State graduate student Hang Yu is first author. Dean Lee, professor of physics and theoretical nuclear science department head at the Facility for Rare Isotope Beams at Michigan State University, co-authored the work. Lee was formerly at NC State and remains an adjunct professor of physics at NC State.

Read the original article from NC State.

Michigan State University (MSU) operates the Facility for Rare Isotope Beams (FRIB) as a user facility for the U.S. Department of Energy Office of Science (DOE-SC), supporting the mission of the DOE-SC Office of Nuclear Physics. User facility operation is supported by the DOE-SC Office of Nuclear Physics as one of 28 DOE-SC user facilities.

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