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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.
S. Pahor
Nuclear Science and Engineering | Volume 26 | Number 2 | October 1966 | Pages 192-197
Technical Paper | doi.org/10.13182/NSE66-A28161
Articles are hosted by Taylor and Francis Online.
The solutions of various time-independent one-speed half-space transport problems, such as the generalized Milne and albedo problems, are derived with the help of the Chandrasekhar S-function and the Case eigenfunctions. First the S-function is expressed by Chandrasekhar's H-function and Busbridge's q-polynomials. These polynomials can be separately determined by solving systems of linear equations. Using the S-function, the emerging distribution is obtained by simple physical arguments. Then, the distribution inside the medium is found by applying full-range orthogonality relations between the Case eigenfunctions.