Research from North Carolina State University shows that a type of modified titania, or titanium dioxide, holds promise as an electrical insulator¹ for superconducting magnets, allowing heat to dissipate while preserving the electrical paths along which current flows. Superconducting magnets are being investigated for use in next-generation power generating technologies and medical devices. Regular conductors conduct electricity, but a small fraction of that energy is lost during transmission. Superconductors can handle much higher currents per square centimeter and lose virtually no energy through transmission. However, superconductors only have these desirable properties at low temperatures.

 

"Superconducting magnets need electrical insulators² to ensure proper operation," says Dr. Sasha Ishmael, a postdoctoral researcher at NC State and lead author of a paper describing the work. "Changing the current inside the superconductor is important for many applications, but this change generates heat internally. The magnets will operate much more safely if the electrical insulators are able to shed any excess heat. Otherwise, the higher temperatures could destroy the superconductor.

 

"This titania-based material is up to 20 times better at conducting heat than comparable electrical insulators," Ishmael says. "It has characteristics that are very promising³ for use as electrical insulators for superconducting technologies."

 

The precise chemical composition of the modified titania is proprietary⁴ information. The material's development and characterization was a joint⁵ effort between NC State and nGimat LLC, based in Lexington, Kentucky.

 

"We're now looking at the effect of radiation on this material, to determine if it can be used for high energy physics applications, such as particle colliders," says Dr. Justin Schwartz, senior author of the paper and Kobe Steel Distinguished⁶ Professor and head of the Department of Materials Science and Engineering at NC State.

 

The research was supported by the Department of Energy under grant DE-SC0004657-001 and the National Science Foundation under grant CBET-1336464.

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