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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.
M. Caner, M. Segev, S. Yiftah
Nuclear Science and Engineering | Volume 59 | Number 4 | April 1976 | Pages 395-405
Technical Paper | doi.org/10.13182/NSE76-A26840
Articles are hosted by Taylor and Francis Online.
A consistent compound nucleus theory of (n, 2n) and (n, 3n) neutron emission was applied to 238U to obtain the energy spectra of the second and third secondary neutrons. The evaluation was based on inelastic level excitation and evaporation data for 238U, 237U, and 236U. The 238U and 236U data were retrieved from ENDF/B-IV files; the 237U data were evaluated in the Soreq Nuclear Research Center using experimental information and statistical reaction theory codes. At reaction energies E0 just above the (n, 2n) threshold energy B2, the energy E of the second inelastic neutron has a spectrum of (E0 - B2 - E); above the (n, 3n) threshold, B3, the third neutron energy has a spectrum of (E0 - B2 - E)3. At energies E0, high above the thresholds, the second and third neutron spectra approach the evaporation form. A secondary neutron spectrum for any given reaction energy E0 is approximated by a composite form where i = 2, 3 for the second and third neutrons, respectively. The temperatures Ti and blending coefficients βi were evaluated for several energies in the range from threshold up to 15 MeV.