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Fusion Energy
This division promotes the development and timely introduction of fusion energy as a sustainable energy source with favorable economic, environmental, and safety attributes. The division cooperates with other organizations on common issues of multidisciplinary fusion science and technology, conducts professional meetings, and disseminates technical information in support of these goals. Members focus on the assessment and resolution of critical developmental issues for practical fusion energy applications.
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Conference on Nuclear Training and Education: A Biennial International Forum (CONTE 2025)
February 3–6, 2025
Amelia Island, FL|Omni Amelia Island Resort
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Wyoming OKs construction of TerraPower’s Natrium plant
Progress continues for TerraPower’s Natrium plant, with the latest win coming in the form of a state permit for construction of nonnuclear portions of the advanced reactor.
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.