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Conference Spotlight
Nuclear Energy Conference & Expo (NECX)
September 8–11, 2025
Atlanta, GA|Atlanta Marriott Marquis
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DOE fast tracks test reactor projects: What to know
The Department of Energy today unveiled 10 companies racing to bring test reactors online by next year to meet Trump's deadline of next Independance Day, leveraging a new DOE pathway that allows reactor authorization outside national labs. As first outlined in one of the four executive orders on nuclear energy released by President Trump on May 23 and in the request for applications for the Reactor Pilot Program released June 18, the companies must use their own money and sites—and DOE authorization—to get reactors operating. What they won’t need is a Nuclear Regulatory Commission license.
R. P. Gardner, K. Verghese, J. I. Cehn
Nuclear Technology | Volume 16 | Number 2 | November 1972 | Pages 418-429
Technical Paper | Radioisotope | doi.org/10.13182/NT72-A31207
Articles are hosted by Taylor and Francis Online.
A mathematical model is developed for predicting the spectra of alpha particles of distributed energy emitted at a point, transmitted through gas mixtures, and detected by a circular detector. Circular sources located coaxially with the detector are also treated. Experimental results verify the accuracy of the model. Possible applications of the model include the calibration and optimum design of all transmission-type alpha-particle gauges for specific measurements such as atmospheric densitometers. A new gauging principle based on the alpha particle stopping power is also identified and preliminary experiments indicate its feasibility. This principle consists of using a nonlinear search on the amounts of gaseous components present to obtain the best fit between experimental and calculated alpha-particle spectra. If the stopping powers at the different alpha-particle energies are different for all components, then, in principle, one can analyze for the amounts of each component. Potential application of this principle to measurements of density (free of composition interferences) and gas composition of planetary atmospheres is discussed.