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Going Nuclear: Notes from the officially unofficial book tour
I work in the analytical labs at one of Europe’s oldest and largest nuclear sites: Sellafield, in northwestern England. I spend my days at the fume hood front, pipette in one hand and radiation probe in the other (and dosimeter pinned to my chest, of course). Outside the lab, I have a second job: I moonlight as a writer and public speaker. My new popular science book—Going Nuclear: How the Atom Will Save the World—came out last summer, and it feels like my life has been running at full power ever since.
David B. Reister
Nuclear Science and Engineering | Volume 46 | Number 2 | November 1971 | Pages 197-202
Technical Paper | doi.org/10.13182/NSE71-A22353
Articles are hosted by Taylor and Francis Online.
Optimum upper and lower flux bounds are sought for a general space-time reactor problem. The bounds are much narrower than previous bounds. Each bound is a sum of the products of known spatial modes and unknown time-dependent amplitude functions. To determine a bound, the amplitude functions must satisfy certain inequalities given by a comparison theorem of the Nagumo-Westphal type. An optimum bound is one that satisfies the inequalities and minimizes a “payoff function. In this paper, the payoff function is the weighted average of the magnitude of the bound at several points in the reactor. It is shown that an optimum bound can be determined by solving a linear programming problem at each time step. (Linear programming can be used even if there is feedback and the problem is nonlinear.) Using linear programming theory it is shown that an optimum bound always exists, although it may not be unique. Furthermore, an optimum bound satisfies the original space-time equation at each point in the reactor sampled by the payoff function. In an example, narrow bounds are determined for a difficult example in which the spatial shape of the flux changes radically with time.