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Conference Spotlight
2025 ANS Winter Conference & Expo
November 9–12, 2025
Washington, DC|Washington Hilton
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A webinar, and a new opportunity to take ANS’s CNP Exam
Applications are now open for the fall 2025 testing period for the American Nuclear Society’s Certified Nuclear Professional (CNP) exam. Applications are being accepted through October 14, and only three testing sessions are offered per year, so it is important to apply soon. The test will be administered from November 12 through December 16. To check eligibility and schedule your exam, click here.
In addition, taking place tomorrow (September 19) from 12:00 noon to 1:00 p.m. (CDT), ANS will host a new webinar, “How to Become a Certified Nuclear Professional.” More information is available below in this article.
Fred Cooper, John Dienes
Nuclear Science and Engineering | Volume 68 | Number 3 | December 1978 | Pages 308-321
Technical Paper | doi.org/10.13182/NSE78-A27308
Articles are hosted by Taylor and Francis Online.
We investigate the growth of Rayleigh-Taylor instabilities following the deceleration of fuel by a less dense coolant using the method of generalized coordinates, which allows us to study the nonlinear, late-time aspects of the problem as well as the possibility of fuel freezing at the interface. We consider liquid coolant in contact with three possible states of fuel—pure liquid, pure solid, and liquid fuel freezing at the interface—and treat several acceleration mechanisms. Assuming the instability starts at a planar interface as a velocity perturbation proportional to the interfacial velocity, we find that when the fuel is completely frozen or freezing at the interface, instabilities will not grow unless the initial interfacial relative velocity satisfies a relationship of the form where υ0 is the initial relative velocity, ρf the density of the fuel, Y0 the yield strength of the frozen fuel, λ the wavelength of the instability, and L a characteristic length. The specific form of C depends on the acceleration mechanism and when freezing begins. For the case of UO2 and sodium, we follow the growth of the fastest growing wavelength instability for different acceleration mechanisms and determine the impulse needed for instabilities to grow when freezing is occurring at the interface.