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Conference Spotlight
Nuclear Energy Conference & Expo (NECX)
September 8–11, 2025
Atlanta, GA|Atlanta Marriott Marquis
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The Standards Committee is responsible for the development and maintenance of voluntary consensus standards that address the design, analysis, and operation of components, systems, and facilities related to the application of nuclear science and technology. Find out What’s New, check out the Standards Store, or Get Involved today!
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Deep Space: The new frontier of radiation controls
In commercial nuclear power, there has always been a deliberate tension between the regulator and the utility owner. The regulator fundamentally exists to protect the worker, and the utility, to make a profit. It is a win-win balance.
From the U.S. nuclear industry has emerged a brilliantly successful occupational nuclear safety record—largely the result of an ALARA (as low as reasonably achievable) process that has driven exposure rates down to what only a decade ago would have been considered unthinkable. In the U.S. nuclear industry, the system has accomplished an excellent, nearly seamless process that succeeds to the benefit of both employee and utility owner.
W. R. Rhyne, A. C. Lapsley
Nuclear Science and Engineering | Volume 40 | Number 1 | April 1970 | Pages 91-100
Technical Paper | doi.org/10.13182/NSE70-A18881
Articles are hosted by Taylor and Francis Online.
A numerical method for the solution of the time- and space-dependent multigroup diffusion equations is presented. The method permits a significant reduction in the computer time required to solve these equations by substantially increasing the allowable time step size. In the point reactor case, a form of the method considerably simplifies the calculation by removing the explicit dependence on the generation time and the delayed-neutron terms. The space-time equations are transformed into the Laplace domain and after multiplication by a weighting function they are transformed back into the time domain. By appropriate choice of the weighting function the equations appear either as coupled convolution integrals, where numerically difficult (e.g., generation time and delayed neutron) terms have been canceled, or as coupled integral equations in the weighted residual form, which permits very large time steps to be taken.