Physics Grad Student Publishes Class Project in Top Journal
Dany Yaacoub, a second-year master’s student in the physics department, has had a paper accepted for publication in Physical Review Letters, the world’s premiere physics journal. Even more notably, this paper began as a class project in the spring 2024 semester.
The paper presents the results of complex plasma physics simulations and includes a new model for calculating the mobility of nuclei in plasmas.
“Plasmas are an ionized state of matter consisting of positively charged nuclei and free electrons, making them distinct from solids, liquids, and gases,” says Yaacoub. “In fact, most ordinary matter in the universe, by mass and by volume, is plasma.” The space between stars is filled with the sparse plasma of the interstellar medium, while stars themselves are giant plasma balls. “If anything, solids, liquids and gases are a rare exception,” Yaacoub says.
Yaacoub’s publication comes after taking PHY 462 Astrophysics last spring. When it came time to pick a final project for the semester, Yaacoub used the opportunity to develop his computational research for his master’s thesis in a new direction studying crystallized plasmas.
“Though most people think plasmas form at high heat, making them a bit like a gas, there are many kinds of plasmas,” Yaacoub explains. He adds, “Plasmas can freeze. Put anything under enough pressure and you can make a solid – so these specific plasmas crystallize, and can be found in dense dead stars, like white dwarfs and neutron stars.” Yaacoub further say that many properties of these plasmas, called ‘Coulomb crystals,’ are relatively poorly studied.
How exactly particles in these crystallized plasmas move, how they ‘diffuse,’ has been an open question for decades, but new supercomputing capabilities at ISU made the new work possible.
“These simulations have to run for days to generate enough data to build a theoretical model,” according to associate professor of physics Dr. Matt Caplan, who teaches Astrophysics and is also Yaacoub’s research advisor. Caplan goes onto explain that these simulations simply weren’t possible in the past when supercomputers were smaller and computer processors were slower.
“With modern supercomputers it’s fairly easy to get terabytes and terabytes of data,” Caplan said. “Chewing through that data to get new science out is now the hard part, that requires a talented scientist like Dany.”
Yaacoub’s research is supported by the Simons Collaboration on Extreme Electrodynamics of Compact Sources (SCEECS), a group of theoretical physicists funded by the Simons Foundation studying black holes and neutron stars, and his results will be used by scientists across the US, Canada, and Israel.
“The enormous pressure from a neutron star’s gravity compresses its plasma to densities trillions of times greater than any matter on earth. It forces the nuclei into a crystalline solid making it almost impossible for them to move past each other. [Yaacoub’s] shown that diffusion is in a sense ‘universal’ – the specific temperature, density, and composition of the plasma don’t matter,” said Caplan, a co-investigator in SCEECS. “These simulations and analysis tell us how fast this material can flow and how it responds to stresses, and that determines how it can break or shatter, for example in a starquake.”
Yaacoub was also the first MS student admitted to the physics department’s new master’s program, having graduated from ISU with a BS in physics in spring 2023. He remained at ISU as a non-degree seeking graduate student in the fall of 2023 to do research with Caplan. After the degree program was approved in March 2024, he enrolled officially as the first graduate student in physics.
“Starting a research project with Dr. Caplan before the master’s program existed was a calculated risk,” Yaacoub says, before adding with a smirk, “but we’re theoretical physicists. We’re really good at math.”
More Information: Caplan & Yaacoub, Universal Diffusion in Coulomb Crystals, Physical Review Letters (2024) [Preprint]
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